<?xml version='1.0' ?>
<!DOCTYPE datasets SYSTEM "http://www.cs.washington.edu/research/projects/xmltk/xmldata/data/nasa/dataset_053.dtd">
<datasets>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Proper Motions of Stars in the Zone Catalogue -40 to -52 degrees
of 20843 Stars for 1900</title>
  <altname type="ADC">1005</altname>
  <altname type="CDS">I/5</altname>
  <altname type="brief">Proper Motions in Cape Zone Catalogue -40/-52</altname>
  <reference>
   <source>
    <other>
     <title>Proper Motions of Stars in the Zone Catalogue -40 to -52 degrees
of 20843 Stars for 1900</title>
     <author>
      <initial>J</initial>
      <initial>H</initial>
      <lastName>Spencer</lastName>
     </author>
     <author>
      <initial>J</initial>
      <lastName>Jackson</lastName>
     </author>
     <name>His Majesty's Stationery Office, London</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1936</year>
     </date>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
   <keyword xlink:href="Proper_motions.html">Proper motions</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>This catalog, listing the proper motions of 20,843 stars
    from the Cape Astrographic Zones, was compiled from three series of
    photographic plates. The plates were taken at the Royal Observatory,
    Cape of Good Hope, in the following years: 1892-1896, 1897-1910,
    1923-1928. Data given include centennial proper motion, photographic
    and visual magnitude, Harvard spectral type, Cape Photographic
    Durchmusterung (CPD) identification, epoch, right ascension and
    declination for 1900.</para>
   </description>
   <details/>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="czc.dat">
     <title>The catalogue</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>---</name>
     <definition>Number 5</definition>
     <units>---</units>
    </field>
    <field>
     <name>CZC</name>
     <definition>Catalogue Identification Number</definition>
     <units>---</units>
    </field>
    <field>
     <name>Vmag</name>
     <definition>Visual Magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right Ascension for 1900 hours</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right Ascension for 1900 minutes</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAcs</name>
     <definition>Right Ascension seconds in 0.01sec 1900</definition>
     <units>0.01s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Declination Sign</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination for 1900 degrees</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination for 1900 arcminutes</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEds</name>
     <definition>Declination for 1900 arcseconds</definition>
     <units>0.1arcsec</units>
    </field>
    <field>
     <name>Ep-1900</name>
     <definition>Epoch -1900</definition>
     <units>cyr</units>
    </field>
    <field>
     <name>CPDZone</name>
     <definition>Cape Photographic
                                        Durchmusterung Zone</definition>
     <units>---</units>
    </field>
    <field>
     <name>CPDNo</name>
     <definition>Cape Photographic Durchmusterung Number</definition>
     <units>---</units>
    </field>
    <field>
     <name>Pmag</name>
     <definition>Photographic Magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>Sp</name>
     <definition>HD Spectral Type</definition>
     <units>---</units>
    </field>
    <field>
     <name>pmRAs</name>
     <definition>Proper Motion in RA
      <footnote>
       <para>the relation is   pmRA = 15 * pmRAs * cos(DE)
    if pmRAs is expressed in s/yr and pmRA in arcsec/yr</para>
      </footnote>
     </definition>
     <units>0.1ms/yr</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Proper Motion in RA</definition>
     <units>mas/yr</units>
    </field>
    <field>
     <name>pmDE</name>
     <definition>Proper Motion in Dec</definition>
     <units>mas/yr</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Julie Anne Watko</lastName>
     <affiliation>SSDOO/ADC</affiliation>
    </creator>
    <date>
     <year>1995</year>
     <month>Nov</month>
     <day>03</day>
    </date>
   </ingest>
  </history>
  <identifier>I_5.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Catalogue of 20554 Faint Stars in the Cape Astrographic Zone -40 to -52 Degrees
for the Equinox of 1900.0</title>
  <altname type="ADC">1006</altname>
  <altname type="CDS">I/6</altname>
  <altname type="brief">Cape 20554 Faint Stars, -40 to -52, 1900.0</altname>
  <reference>
   <source>
    <other>
     <title>Catalogue of 20554 Faint Stars in the Cape Astrographic Zone -40 to -52 Degrees
for the Equinox of 1900.0</title>
     <author>
      <initial>J</initial>
      <initial>H</initial>
      <lastName>Spencer</lastName>
     </author>
     <author>
      <initial>J</initial>
      <lastName>Jackson</lastName>
     </author>
     <name>His Majesty's Stationery Office, London</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1939</year>
     </date>
     <bibcode>1939HMSO..C......0S</bibcode>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
   <keyword xlink:href="Proper_motions.html">Proper motions</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>This catalog contains positions, precessions, proper motions, and
  photographic magnitudes for 20,554 stars.  These were derived from
  photographs taken at the Royal Observatory, Cape of Good Hope between 1923
  and 1928.  It covers the astrographic zones -40 degrees to -52 degrees of
  declination.  The positions are given for epoch 1900 (1900.0).  It includes
  spectral types for many of the stars listed.  It extends the earlier
  catalogs derived from the same plates to fainter magnitudes.  The
  computer-readable version consists of a single data table.</para>
    <para>The stated probable error for the star positions is 0.024 seconds of time
  (R.A.) and 0.25 seconds of arc (dec.) for stars with one determination,
  0.017 seconds of time, and 0.18 seconds of arc for two determinations, and
  0.014 / 0.15 for stars with three determinations.</para>
    <para>The precession and secular variations were derived from Newcomb's constants.</para>
    <para>The authors quote probable errors of the proper motions in both coordinates
  of 0.008 seconds of arc for stars with one determination, 0.0055 seconds for
  stars with two determinations, and 0.0044 for stars with three.</para>
    <para>The photographic magnitudes were derived from the measured diameters on the
  photographic plates and from the magnitudes given in the Cape Photographic
  Durchmusterung.</para>
    <para>The spectral classification of the cataloged stars was done with the
  assistance of Annie Jump Cannon of the Harvard College Observatory.</para>
    <para>The user should consult the source reference for more details of the
  measurements and reductions.  See also the notes in this document for
  additional information on the interpretation of the entries.</para>
   </description>
   <details/>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="faint.dat">
     <title>Data</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ID</name>
     <definition>Cape Number</definition>
     <units>---</units>
    </field>
    <field>
     <name>rem</name>
     <definition>Remark
      <footnote>
       <para>A = Astrographic Star
   F = Faint Proper Motion Star
   N = Other Note</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>CPDZone</name>
     <definition>Cape Phot. Durchmusterung (CPD) Zone
      <footnote>
       <para>All CPD Zones are negative. - signs are not included in data.
        "0" in column 8 signifies Astrographic Plate instead of CPD.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>CPD</name>
     <definition>CPD Number or Astrographic Plate
      <footnote>
       <para>See also note on CPDZone.
        Astrographic plate listed "is the more southerly on which the
        star occurs." Thus, y-coordinate is positive wherever possible.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>n_CPD</name>
     <definition>[1234] Remarks
      <footnote>
       <para>A number from 1-4 appears in this byte for double stars where
    the same CPD number applies to more than one star.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>mpg</name>
     <definition>Photographic Magnitude
      <footnote>
       <para>The Photographic Magnitude is "determined from the CPD Magnitude
        and the diameter on the Cape Astrographic Plates by means of the
        data given in the volume on the Magnitudes of Stars in the Cape
        Zone Catalogue."
    A null value (99.9) signifies a variable star.</para>
      </footnote>
     </definition>
     <units>mag</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Mean Right Ascension hours 1900</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Mean Right Ascension minutes 1900</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Mean Right Ascension seconds 1900</definition>
     <units>s</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Mean Declination degrees 1900</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Mean Declination arcminutes 1900</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Mean Declination arcseconds 1900</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>N</name>
     <definition>Number of Observations</definition>
     <units>---</units>
    </field>
    <field>
     <name>Epoch</name>
     <definition>Epoch +1900</definition>
     <units>yr</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Proper Motion in RA seconds of time</definition>
     <units>s/a</units>
    </field>
    <field>
     <name>pmRAas</name>
     <definition>Proper Motion in RA arcseconds</definition>
     <units>arcsec/a</units>
    </field>
    <field>
     <name>pmDE</name>
     <definition>Proper Motion in Dec arcseconds</definition>
     <units>arcsec/a</units>
    </field>
    <field>
     <name>Sp</name>
     <definition>HD Spectral Type</definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Julie Anne Watko</lastName>
     <affiliation>SSDOO/ADC</affiliation>
    </creator>
    <date>
     <year>1996</year>
     <month>Mar</month>
     <day>26</day>
    </date>
   </ingest>
  </history>
  <identifier>I_6.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Proper Motions of 1160 Late-Type Stars</title>
  <altname type="ADC">1014</altname>
  <altname type="CDS">I/14</altname>
  <altname type="brief">Proper Motions of 1160 Late-Type Stars</altname>
  <reference>
   <source>
    <journal>
     <title>Proper Motions of 1160 Late-Type Stars</title>
     <author>
      <initial>H</initial>
      <initial>J</initial>
      <lastName>Fogh Olsen</lastName>
     </author>
     <name>Astron. Astrophys. Suppl. Ser.</name>
     <volume>2</volume>
     <pageno>69</pageno>
     <date>
      <year>1970</year>
     </date>
     <bibcode>1970A&amp;AS....2...69O</bibcode>
    </journal>
   </source>
   <related>
    <holding role="similar">II/38 : Stars observed photoelectrically by Dickow et al.
     <xlink:simple href="II/38"/>
    </holding>Fogh Olsen H.J. 1970, Astron. Astrophys. Suppl. Ser., 2, 69.
   Fogh Olsen H.J. 1970, Astron. Astrophys., Suppl. Ser., 1, 189.</related>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Proper_motions.html">Proper motions</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>Improved proper motions for the 1160 stars contained in the photometric
   catalog by Dickow et al. (1970) are presented. Most of the proper motions
   are from the GC, transferred to the system of FK4. For stars not included
   in the GC, preliminary AGK or SAO proper motions are given. Fogh Olsen
   (Astron. Astrophys. Suppl. Ser., 1, 189, 1970) describes the method of
   improvement. The mean errors of the centennial proper motions increase with
   increasing magnitude. In Right Ascension, these range from 0.0043/cos(dec)
   for very bright stars to 0.096/cos(dec) for the faintest stars. In Dec-
   lination, the range is from 0.065 to 1.14.</para>
   </description>
   <details/>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="pmlate.dat">
     <title>Proper motion data</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>No</name>
     <definition>Number
      <footnote>
       <para>Henry Draper or Bonner Durchmusterung number</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Centennial Proper Motion RA</definition>
     <units>s/ca</units>
    </field>
    <field>
     <name>pmDE</name>
     <definition>Centennial Proper Motion Dec</definition>
     <units>arcsec/ca</units>
    </field>
    <field>
     <name>RV</name>
     <definition>Radial Velocity</definition>
     <units>km/s</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Julie Anne Watko</lastName>
     <affiliation>ADC</affiliation>
    </creator>
    <date>
     <year>1996</year>
     <month>Jun</month>
     <day>03</day>
    </date>
   </ingest>
  </history>
  <identifier>I_14.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Katalog von 3356 Schwachen Sternen fuer das Aequinoktium 1950
+89 degrees</title>
  <altname type="ADC">1016</altname>
  <altname type="CDS">I/16</altname>
  <altname type="brief">Catalog of 3356 Faint Stars, 1950</altname>
  <reference>
   <source>
    <other>
     <title>Katalog von 3356 Schwachen Sternen fuer das Aequinoktium 1950
+89 degrees</title>
     <author>
      <initial>J</initial>
      <lastName>Larink</lastName>
     </author>
     <author>
      <initial>A</initial>
      <lastName>Bohrmann</lastName>
     </author>
     <author>
      <initial>H</initial>
      <lastName>Kox</lastName>
     </author>
     <author>
      <initial>J</initial>
      <lastName>Groeneveld</lastName>
     </author>
     <author>
      <initial>H</initial>
      <lastName>Klauder</lastName>
     </author>
     <name>Verlag der Sternwarte, Hamburg-Bergedorf</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1955</year>
     </date>
     <bibcode>1955</bibcode>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Fundamental_catalog.html">Fundamental catalog</keyword>
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
   <keyword xlink:href="Proper_motions.html">Proper motions</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>This catalog of 3356 faint stars was derived from meridian circle
   observations at the Bergedorf and Heidelberg Observatories. The
   positions are given for the equinox 1950 on the FK3 system. The stars
   are mainly between 8.0 and 10.0 visual magnitude. A few are brighter
   than 8.0 mag. The lower limit in brightness resulted from the visibility
   of the stars.</para>
   </description>
   <details>
    <para>All stars were observed at both the Heidelberg and Bergedorf
   Observatories. Normally, at each observatory, two observations were
   obtained with the clamp east and two with the clamp west. The mean
   errors are comparable for the two observatories with no significant
   systematic difference in the positions between them. The mean errors of
   the resulting positions should be approximated 0.011s/cos(dec) in right
   ascension and ).023" in declination.</para>
    <para>The proper motions were derived from a comparison with the catalog
   positions with the positions in the AGK2 and AGK2A with a 19 year
   baseline and from a comparison of new positions with those in Kuestner
   1900 with about a fifty year baseline.</para>
    <para>The magnitudes were taken from the AGK2. Most spectral types were
   determined by A. N. Vyssotsky. A few are from the Bergedorfer
   Spektraldurchmusterung.</para>
   </details>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="catalog.dat">
     <title>The catalog</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ID</name>
     <definition>Catalog number</definition>
     <units>---</units>
    </field>
    <field>
     <name>DMz</name>
     <definition>BD zone</definition>
     <units>---</units>
    </field>
    <field>
     <name>DMn</name>
     <definition>BD number</definition>
     <units>---</units>
    </field>
    <field>
     <name>mag</name>
     <definition>Photographic magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>Sp</name>
     <definition>Spectral class</definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right Ascension hours (1950)</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right Ascension minutes (1950)</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Right Ascension seconds (1950)</definition>
     <units>s</units>
    </field>
    <field>
     <name>Pr-RA1</name>
     <definition>First order precession in RA per century</definition>
     <units>0.01s/a</units>
    </field>
    <field>
     <name>Pr-RA2</name>
     <definition>Second order precession in RA per century</definition>
     <units>0.0001s2/a2</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Proper motion in RA from AGK2 positions</definition>
     <units>0.01s/a</units>
    </field>
    <field>
     <name>pmRA2</name>
     <definition>Proper motion in RA from Kuestner positions</definition>
     <units>0.01s/a</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Sign of declination (1950)</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination degrees (1950)</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination minutes (1950)</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Declination seconds (1950)</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>Pr-de1</name>
     <definition>First order precession in dec per century</definition>
     <units>arcsec/ha</units>
    </field>
    <field>
     <name>Pr-de2</name>
     <definition>Second order precession in dec per century</definition>
     <units>arcsec2/ha2</units>
    </field>
    <field>
     <name>pmdec</name>
     <definition>Proper motion in DE from AGK2 positions</definition>
     <units>arcsec/ha</units>
    </field>
    <field>
     <name>pmdec2</name>
     <definition>Proper motion in DE from Kuestner positions</definition>
     <units>arcsec/ha</units>
    </field>
    <field>
     <name>epoch</name>
     <definition>Epoch of observation - 1900.0</definition>
     <units>yr</units>
    </field>
    <field>
     <name>rem</name>
     <definition>Note for star in printed catalog
      <footnote>
       <para>1 = ma (blend?)
   3 = pr (preceding)
   4 = seq (following)
   5 = bor (northern)
   6 = au (southern)
   * = other note in printed volume (All notes in the printed volume have not
       been indicated in this version.)
   the printed volume sometimes has additional information on the systems with
   numerical remarks.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Nancy Grace Roman</lastName>
     <affiliation>ADC/SSDOO</affiliation>
    </creator>
    <date>
     <year>1996</year>
     <month>Feb</month>
     <day>01</day>
    </date>
   </ingest>
  </history>
  <identifier>I_16.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Astrographic Catalogue</title>
  <altname type="ADC">1021A</altname>
  <altname type="CDS">I/21A</altname>
  <altname type="brief">AC Toulouse, Bordeaux, Paris &amp; Oxford</altname>
  <reference>
   <source>
    <other>
     <title>Astrographic Catalogue</title>
     <author>
      <initial>P</initial>
      <lastName>Lacroute</lastName>
     </author>
     <author>
      <initial>A</initial>
      <lastName>Valbousquet</lastName>
     </author>
     <name>CDS Bull. No. 6, p. 38</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1974</year>
     </date>
     <bibcode>1974BICDS...6...38L</bibcode>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Astrographic_zones.html">Astrographic zones</keyword>
   <keyword xlink:href="Magnitudes_photographic.html">Magnitudes, photographic</keyword>
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>The "Carte de Ciel" (or "Astrographic Catalogue") is a catalogue of star
   positions and magnitudes, determined on the photographic plates taken
   by the normal astrographs which are installed in observatories of various
   latitudes, as a world-wide astronomical project (see Eichhorn, 1974, p279).
   The catalogue is divided into 22 declination zones, each of which is
   assigned to each observatory, e.g., a zone from +18 to +24 degrees is to
   Paris observatory.
   Each observatory has taken photographs of 2 deg x 2 deg area in and covering
   each zone, measured the X,Y coordinates of star images on the photographic
   plates, and published the results as the printed catalogues.
   The present catalogue is the results of reduction of these X,Y coordinates
   into right ascension and declination values, for declination zones of +05
   to +31, by using AGK2/3 catalogue as the reference.</para>
   </description>
   <details/>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="f1">
     <title>Toulouse zone (+05 to +10 and +11 degree)</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ZONE</name>
     <definition>plate identifier
      <footnote>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>PLATE</name>
     <definition>plate identifier
      <footnote>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>HYPH</name>
     <definition>hyphen
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>STAR</name>
     <definition>running number of star on the plate
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>right ascension (hours)   [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>right ascension (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>ascension (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>declination sign
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>declination (degrees)     [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>declination (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>declination (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>EPOCH</name>
     <definition>plate epoch
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>a</units>
    </field>
    <field>
     <name>mB</name>
     <definition>photographic magnitude
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>mag</units>
    </field>
    <field>
     <name>AGKNO</name>
     <definition>AGK2 number
      <footnote>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>SUFFIX</name>
     <definition>suffix to the AGK2 number
      <footnote>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="f2">
     <title>Bordeaux zone (+11 to +17 degree)</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ZONE</name>
     <definition>plate identifier
      <footnote>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>PLATE</name>
     <definition>plate identifier
      <footnote>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>HYPH</name>
     <definition>hyphen
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>STAR</name>
     <definition>running number of star on the plate
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>right ascension (hours)   [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>right ascension (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>ascension (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>declination sign
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>declination (degrees)     [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>declination (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>declination (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>EPOCH</name>
     <definition>plate epoch
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>a</units>
    </field>
    <field>
     <name>mB</name>
     <definition>photographic magnitude
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>mag</units>
    </field>
    <field>
     <name>AGKNO</name>
     <definition>AGK2 number
      <footnote>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>SUFFIX</name>
     <definition>suffix to the AGK2 number
      <footnote>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="f3">
     <title>Paris zone (+18 to +24 degree)</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ZONE</name>
     <definition>plate identifier
      <footnote>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>PLATE</name>
     <definition>plate identifier
      <footnote>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>HYPH</name>
     <definition>hyphen
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>STAR</name>
     <definition>running number of star on the plate
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>right ascension (hours)   [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>right ascension (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>ascension (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>declination sign
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>declination (degrees)     [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>declination (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>declination (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>EPOCH</name>
     <definition>plate epoch
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>a</units>
    </field>
    <field>
     <name>mB</name>
     <definition>photographic magnitude
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>mag</units>
    </field>
    <field>
     <name>AGKNO</name>
     <definition>AGK2 number
      <footnote>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>SUFFIX</name>
     <definition>suffix to the AGK2 number
      <footnote>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="f4">
     <title>Oxford I zone (+25 to +31 degree)</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ZONE</name>
     <definition>plate identifier
      <footnote>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>PLATE</name>
     <definition>plate identifier
      <footnote>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>HYPH</name>
     <definition>hyphen
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>STAR</name>
     <definition>running number of star on plate
      <footnote>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>right ascension (hours)   [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>right ascension (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>right ascension (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>declination sign
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>declination (degrees)     [B1950]
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>declination (minutes)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>declination (seconds)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>EPOCH</name>
     <definition>plate epoch
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>a</units>
    </field>
    <field>
     <name>mB</name>
     <definition>photographic magnitude
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>mag</units>
    </field>
    <field>
     <name>AGKNO</name>
     <definition>AGK2 number, if AGK2/3 star was
      <footnote>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>SUFFIX</name>
     <definition>suffix to the AGK2 number
      <footnote>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that zones lower from 27 deg have generally 180 plates,
        and those higher from 28 deg have 160 plates.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>Note that this number in the Oxford I zone is so determined to be
        unique in a whole zone (e.g., in the zone +25 deg.).</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>AGK2 number, if AGK2/3 star was identified, otherwise CR/LF.
        Note that this is incomplete.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>suffix to the AGK2 number, if needed, otherwise CR/LF.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>J.A. Watko</lastName>
     <affiliation>SSDOO/ADC</affiliation>
    </creator>
    <date>
     <year>1995    Koichi Nakajima [CDS]   24-Sep-1993</year>
     <month>Nov</month>
     <day>16</day>
    </date>
   </ingest>
  </history>
  <identifier>I_21A.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Astrographic Catalogue</title>
  <altname type="ADC">1022A</altname>
  <altname type="CDS">I/22A</altname>
  <altname type="brief">Astrographic Catalogue Algier, -02 to +04</altname>
  <reference>
   <source>
    <other>
     <title>Astrographic Catalogue</title>
     <author>
      <initial>P</initial>
      <lastName>Lacroute</lastName>
     </author>
     <author>
      <initial>A</initial>
      <lastName>Valbousquet</lastName>
     </author>
     <name>CDS Bull. No. 6, p. 38</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1974</year>
     </date>
     <bibcode>1974BICDS...6...38L</bibcode>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
   <keyword xlink:href="Astrographic_zones.html">Astrographic zones</keyword>
   <keyword xlink:href="Magnitudes_photographic.html">Magnitudes, photographic</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>The "Carte de Ciel" (or "Astrographic Catalogue") is a catalogue of star
   positions and magnitudes, determined on the photographic plates taken
   by the normal astrographs which are installed in observatories of various
   latitudes, as a world-wide astronomical project (see Eichhorn, 1974, p279).
   The catalogue is divided into 22 declination zones, each of which is
   assigned to each observatory, e.g., a zone from +18 to +24 degrees is to
   Paris observatory.
   Each observatory has taken photographs of 2 deg x 2 deg area in and covering
   each zone, measured the X,Y coordinates of star images on the photographic
   plates, and published the results as the printed catalogues.
   The present catalogue is the results of reduction of these X,Y coordinates
   into right ascension and declination values, for declination zones of +05
   to +31, by using AGK2/3 catalogue as the reference.</para>
   </description>
   <details/>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="catalog">
     <title>catalog</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ZONE</name>
     <definition>plate identifier
      <footnote>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>PLATE</name>
     <definition>plate identifier
      <footnote>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>STAR</name>
     <definition>running number of star on the plate
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAmas</name>
     <definition>right ascension  (B1950)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>mas</units>
    </field>
    <field>
     <name>DEmas</name>
     <definition>declination  (B1950)
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>mas</units>
    </field>
    <field>
     <name>EPOCH</name>
     <definition>plate epoch from 180000
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>ca</units>
    </field>
    <field>
     <name>mB</name>
     <definition>photographic magnitude
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>dmag</units>
    </field>
    <field>
     <name>X</name>
     <definition>X coordinate on the plate
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>0.1um</units>
    </field>
    <field>
     <name>Y</name>
     <definition>Y coordinate on the plate
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>0.1um</units>
    </field>
    <field>
     <name>AGK3Z</name>
     <definition>AGK3 number : zone number
      <footnote>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>deg</units>
    </field>
    <field>
     <name>AGK3N</name>
     <definition>AGK3 number : star number
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>ZERO</name>
     <definition>zero
      <footnote footnoteId="???">
       <para>number=</para>
       <para>declination zone, or the declination of the center of each
        astrographic plate</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>running number of plate in the zone
        Note that this number is negative when the zone is negative.</para>
      </footnote>
      <footnote footnoteId="???">
       <para>number=</para>
       <para>No signs on any AGK3 zones.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Koichi Nakajima</lastName>
     <affiliation>CDS</affiliation>
    </creator>
    <date>
     <year>1993    J.A. Watko [SSDOO/ADC]  21-Feb-1996</year>
     <month>Sep</month>
     <day>24</day>
    </date>
   </ingest>
  </history>
  <identifier>I_22A.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Results of observations with the nine-inch transit circle 1913-1926.
Catalogue of 9989 standard and intermediary stars, Miscellaneous stars.</title>
  <altname type="ADC">1040</altname>
  <altname type="CDS">I/40</altname>
  <altname type="brief">WASHINGTON 20 Catalog</altname>
  <reference>
   <source>
    <other>
     <title>Results of observations with the nine-inch transit circle 1913-1926.
Catalogue of 9989 standard and intermediary stars, Miscellaneous stars.</title>
     <author>
      <initial>H</initial>
      <initial>R</initial>
      <lastName>Morgan</lastName>
     </author>
     <name>Publ. USNO, 2nd series, vol. XIII, Washington</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1933</year>
     </date>
     <bibcode>1983</bibcode>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Meridian_observations.html">Meridian observations</keyword>
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
   <keyword xlink:href="Historical_catalog.html">Historical catalog</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>This catalogue contains the two parts: the 9989 first stars are the
    standard and intermediary stars, +90 to -36 degrees of declination,
    observed in the years 1913 to 1926, and reduced without proper motion
    to the equinox 1920.0 ; the second part (stars numbered 9990 to 10571)
    are 582 miscellaneous stars.</para>
   </description>
   <details/>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="catalog.dat">
     <title>The catalog of (9989 + 582) stars.</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>Seq</name>
     <definition>Running number</definition>
     <units>---</units>
    </field>
    <field>
     <name>DM</name>
     <definition>Durchmusterung (BD or CD) identification</definition>
     <units>---</units>
    </field>
    <field>
     <name>Sp</name>
     <definition>Spectral type, from HD</definition>
     <units>---</units>
    </field>
    <field>
     <name>NumSp</name>
     <definition>Coded spectral type
      <footnote footnoteId="???">
       <para>number=1</para>
       <para>the numeric spectral type exists only for stars 1-10400;
     it is coded on 3 bytes as follows:
       -------------------------------
       Byte#16     Byte#17    Byte#18
       -------------------------------
          R=0    a or 0=0
        Oe5=1    b or 1=1
          O=2    c or 2=2
          B=2    d or 3=3        *=3
          A=4    e or 4=4
          F=5         5=5        e=5
          G=6         6=6
          K=7         7=7
          M=8         8=8
          N=9         9=9
          S=-                    p=-
       -------------------------------
       Special cases:
          Mb=83  Mc=88, Md=8 5, Me=8-5,
          Np=9</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>Vmag</name>
     <definition>Magnitudes (from Harvard Revised Photometry
                                    or corrected BD)</definition>
     <units>mag</units>
    </field>
    <field>
     <name>n_Vmag</name>
     <definition>for variable star</definition>
     <units>---</units>
    </field>
    <field>
     <name>ObsMag</name>
     <definition>Observed magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right Ascension B1920 (hours), at Epoch</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right Ascension B1920 (minutes), at Epoch</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Right Ascension B1920 (seconds), at Epoch</definition>
     <units>s</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Annual proper motion in RA (in Boss system)</definition>
     <units>s/a</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Declination B1920 (sign)</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination B1920 (degrees)</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination B1920 (minutes)</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Declination B1920 (0.01arcsec)</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>pmDE</name>
     <definition>Annual proper motion in Dec (in Boss system)</definition>
     <units>arcsec/a</units>
    </field>
    <field>
     <name>o_RAs</name>
     <definition>Number of observations in RA</definition>
     <units>---</units>
    </field>
    <field>
     <name>o_DEs</name>
     <definition>Number of observations in Dec
      <footnote footnoteId="???">
       <para>number=2</para>
       <para>the value is not specified when it is identical to the
     corresponding number for RA.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>EpRA-1900</name>
     <definition>Mean Epoch of Right Ascension</definition>
     <units>0.01a</units>
    </field>
    <field>
     <name>EpDE-1900</name>
     <definition>Mean Epoch of Declination
      <footnote footnoteId="???">
       <para>number=2</para>
       <para>the value is not specified when it is identical to the
     corresponding number for RA.</para>
      </footnote>
     </definition>
     <units>0.01a</units>
    </field>
    <field>
     <name>Note</name>
     <definition>indicates a note in the catalog</definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Francois Ochsenbein, James Marcout</lastName>
     <affiliation>CDS</affiliation>
    </creator>
    <date>
     <year>1998</year>
     <month>Jun</month>
     <day>10</day>
    </date>
   </ingest>
   <revisions>
    <revision>
     <creator>
      <lastName>UNKNOWN</lastName>
     </creator>
     <date>
      <year>UNKNOWN</year>
     </date>
     <para>The catalogue was originally keypunched at the Astronomisches
    Rechen-Institut, Heidelberg, Germany, in the 70's. It contained 10400
    stars, i.e. 171 stars were missing (note from Richard Swifte, Royal
    Greenwich Observatory, October 1981). The missing stars were added in
    June 1998, with the help of an Optical Character Recognition system.</para>
    </revision>
   </revisions>
  </history>
  <identifier>I_40.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Catalogue of Coordinates of Reference Faint,  Bright and Double Stars South of
-47 Degree and Corrections to FK4 Positions as Observed by Pulkovo
Astronomers with the Meridian Circle at the Cerro-Kalan Observatory
(Chile) in 1963-1968</title>
  <altname type="ADC">1044</altname>
  <altname type="CDS">I/44</altname>
  <altname type="brief">Second Cat of Fundamental Stars</altname>
  <reference>
   <source>
    <journal>
     <title>Catalogue of Coordinates of Reference Faint,  Bright and Double Stars South of
-47 Degree and Corrections to FK4 Positions as Observed by Pulkovo
Astronomers with the Meridian Circle at the Cerro-Kalan Observatory
(Chile) in 1963-1968</title>
     <author>
      <initial>G</initial>
      <initial>D</initial>
      <lastName>Baturina</lastName>
     </author>
     <author>
      <initial>V</initial>
      <initial>S</initial>
      <lastName>Bedin</lastName>
     </author>
     <author>
      <initial>K</initial>
      <initial>G</initial>
      <lastName>Gnevysheva</lastName>
     </author>
     <author>
      <initial>M</initial>
      <initial>S</initial>
      <lastName>Zverev</lastName>
     </author>
     <author>
      <initial>A</initial>
      <initial>A</initial>
      <lastName>Naumova</lastName>
     </author>
     <author>
      <initial>A</initial>
      <initial>I</initial>
      <lastName>Plugina</lastName>
     </author>
     <author>
      <initial>D</initial>
      <initial>D</initial>
      <lastName>Polozhentsev</lastName>
     </author>
     <author>
      <initial>T</initial>
      <initial>A</initial>
      <lastName>Polozhentseva</lastName>
     </author>
     <author>
      <initial>E</initial>
      <initial>A</initial>
      <lastName>Stepanova</lastName>
     </author>
     <name>Tr. Glav. Astron. Obs. Pulkovo, ser.</name>
     <volume>2 86</volume>
     <pageno>4-158</pageno>
     <date>
      <year>1986</year>
     </date>
     <bibcode>1986TrPul..86....4B</bibcode>
    </journal>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>The Catalogue  SPF2  was obtained from  observations of the
   fundamental FK4 stars as a reference stars for SRS,  BS and DS star.
   Observations were made by Pulkovo observers  in  the declination zone
   -42 to -90 and +16 to -16 degrees using Repsold Meridian Circle of
   the Cerro Calan  Observatory (Santiago, Chile) from 1963 to 1968.</para>
   </description>
   <details>
    <para>They worked in closed cooperations with their Chilean colleagues
   who  observed  other declination zones. In total 15160 observations
   were made of FK4 stars. The reductions of observations were
   made by the quasi-absolute method proposed  by M.S.Zverev (1969).
   Investigations were carried out of the systematic differences of
   type "E-W" as well as of the personal  equations. Also differences of
   type "Upper - Lower culmination" were investigated. All these
   corrections were applied to the  observations. The  mean  error of
   the single observations reduced to the equator is +/- 14.0 millisecond
   of time.  The mean error  of the position of a single star reduced
   to the equator is +/- 2.8 millisec of time (each position in the
   middle are consists from 25 observations). The main results of the
   systematic errors were published by Zverev and Naumova.</para>
   </details>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="spf2.dat">
     <title>+16 to -16 deg - RA corrections</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>03</name>
     <definition>"03"</definition>
     <units>---</units>
    </field>
    <field>
     <name>ID</name>
     <definition>FK4 number</definition>
     <units>---</units>
    </field>
    <field>
     <name>mag</name>
     <definition>Magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right Ascension (B1950.0) hours</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right Ascension (B1950.0) minutes</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Right Ascension (B1950.0) seconds</definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Declination (B1950.0) sign</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination (B1950.0) degrees</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination (B1950.0) arcminutes</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Declination (B1950.0) arcsec</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>del_RA</name>
     <definition>RA-RA(FK4)</definition>
     <units>s</units>
    </field>
    <field>
     <name>Ep</name>
     <definition>Epoch of mean observation - 1900 years</definition>
     <units>a</units>
    </field>
    <field>
     <name>e</name>
     <definition>Error
      <footnote>
       <para>E*cos(DE)    where E = error of observations</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>N</name>
     <definition>Number of observations</definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="spf2a.dat">
     <title>-40 to -90 deg - RA and Dec. for 280 stars</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>rem</name>
     <definition>Remark
      <footnote>
       <para>"-3"    data of spf2b.dat exist
        "03"    data of spf2b.dat do not exist</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>ID</name>
     <definition>FK4 number</definition>
     <units>---</units>
    </field>
    <field>
     <name>mag</name>
     <definition>Magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right Ascension (B1950.0) hours</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right Ascension (B1950.0) minutes</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Right Ascension (B1950.0) seconds</definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Declination (B1950.0) sign</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination (B1950.0) degrees</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination (B1950.0) arcminutes</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Declination (B1950.0) arcsec</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>del_RA</name>
     <definition>RA-RA(FK4)</definition>
     <units>s</units>
    </field>
    <field>
     <name>Ep</name>
     <definition>Epoch of mean observation - 1900 years</definition>
     <units>a</units>
    </field>
    <field>
     <name>e</name>
     <definition>Error
      <footnote>
       <para>E*cos(DE)    where E = error of observations</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>N</name>
     <definition>Number of observations</definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="spf2b.dat">
     <title>-40 to -90 deg - RA with upper and lower
                                 culmination separate</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>3</name>
     <definition>"3"</definition>
     <units>---</units>
    </field>
    <field>
     <name>ID</name>
     <definition>FK4 number</definition>
     <units>---</units>
    </field>
    <field>
     <name>mag</name>
     <definition>Magnitude</definition>
     <units>mag</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right Ascension (B1950.0) hours</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right Ascension (B1950.0) minutes</definition>
     <units>min</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Declination (B1950.0) sign</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination (B1950.0) degrees</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination (B1950.0) arcminutes</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>uRA</name>
     <definition>RA-RA(FK4) (upper culmination)</definition>
     <units>s</units>
    </field>
    <field>
     <name>uEp</name>
     <definition>Epoch of mean obs (upper culmination) - 1900</definition>
     <units>a</units>
    </field>
    <field>
     <name>ue</name>
     <definition>Error (upper culmination)</definition>
     <units>s</units>
    </field>
    <field>
     <name>uN</name>
     <definition>Number of observations (upper culmination)</definition>
     <units>---</units>
    </field>
    <field>
     <name>lRA</name>
     <definition>RA-RA(FK4) (lower culmination)</definition>
     <units>s</units>
    </field>
    <field>
     <name>lEp</name>
     <definition>Epoch of mean obs (lower culmination) - 1900</definition>
     <units>a</units>
    </field>
    <field>
     <name>le</name>
     <definition>Error (lower culmination)</definition>
     <units>s</units>
    </field>
    <field>
     <name>lN</name>
     <definition>Number of observations</definition>
     <units>---</units>
    </field>
   </fields>
  </tableHead>
  <history>
   <ingest>
    <creator>
     <lastName>Nancy Grace Roman and Julie Anne Watko</lastName>
     <affiliation>SSDOO/ADC</affiliation>
    </creator>
    <date>
     <year>1996</year>
     <month>Feb</month>
     <day>29</day>
    </date>
    <acknowledgement>We appreciate the extensive information provided by D. Polojentsev.</acknowledgement>
   </ingest>
  </history>
  <identifier>I_44.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>AGK3 Catalogue</title>
  <altname type="ADC">1061B</altname>
  <altname type="CDS">I/61B</altname>
  <altname type="brief">AGK3 Catalogue</altname>
  <reference>
   <source>
    <other>
     <title>AGK3 Catalogue</title>
     <author>
      <initial>W</initial>
      <lastName>Dieckvoss</lastName>
     </author>
     <author>
      <initial>O</initial>
      <lastName>Heckmann</lastName>
     </author>
     <name>Hamburg-Bergedorf</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1975</year>
     </date>
     <bibcode>1975QB6.A15.......D</bibcode>
    </other>
   </source>
   <related>
    <holding role="similar">I/176 : AGK3U: an updated version of the AGK3 (Bucciarelli+ 1992)
     <xlink:simple href="I/176"/>
    </holding>
    <holding role="similar">I/69 : AGK3 Catalogue by Right Ascension (Dieckvoss, Heckmann 1975)
     <xlink:simple href="I/69"/>
    </holding>
    <holding role="similar">I/161 : AGK3R (Smith  1990)
     <xlink:simple href="I/161"/>
    </holding>Cannon, A. J. (1925-1936), The Henry Draper Extension, Ann. Astron. Obs.
      Harvard College 100.
   Cannon, A. J. and Pickering, E. C. (1918-1924), The Henry Draper Catalogue,
      Ann. Astron. Obs. Harvard College 91-99.
   Dieckvoss, W. (in collaboration with H. Kox, A. Gunther and E. Brosterhus)
      (1975), AGK3 Star Catalogue of Positions and Proper Motions North of
      -2.5 Degrees Declination, Hamburg-Bergedorf.
   Nagy, T. A. 1979, Documentation for the Machine-Readable Version of the AGK3
      Catalogue of Positions and Proper Motions North of -2.5 Degrees
      Declination, Systems and Applied Sciences Corporation R-SAW-7/79-35.
   Warren, W. H. Jr. and Kress, K. 1980, Astron. Data Center Bull. 1, 19.
   Willstrop, R. V. 1983, Bull. Inf. Cent. Donnees Stellaires No. 24, 65.</related>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Positional_data.html">Positional data</keyword>
   <keyword xlink:href="Proper_motions.html">Proper motions</keyword>
   <keyword xlink:href="Magnitudes_photographic.html">Magnitudes, photographic</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>The AGK3 provides positions and proper motions for stars north of -2.5
    degrees. For  the most part, it contains the  stars in the AGK2 but is
    based on newly remeasured reference stars whose positions were reduced
    to the FK4 system.  A list of  446 AGK2 stars  not in the  AGK3 and of
    three new stars  is provided. All  plates were taken  at the Bergedorf
    Observatory. In addition to the  positions  and  proper  motions,  the
    catalog contains magnitudes and  spectral  types,  the  epoch  of  the
    observations,  the epoch difference between the AGK2 and AGK3, and the
    BD numbers.</para>
   </description>
   <details>
    <para>The  AGK3 Star Catalogue of Positions and Proper Motions North of -2.5
    Degrees Declination  (hereinafter  AGK3)  was  conceived  and  planned
    during discussions between O.  Heckmann  and  D.  Brouwer  at  Hamburg
    Observatory  following the 1952 International Astronomical Union (IAU)
    General  Assembly in Rome. It was concluded that an adequate number of
    reference stars (AGK3R) should be observed by as many meridian circles
    of as many observatories  as possible,  the revision  of FK3,  then in
    progress (FK4), should  define  the  reference  frame,  and  the  same
    instruments as  used for AGK2 should be  used for the observations for
    AGK3.</para>
    <para>A  formal recommendation was adopted through  Commission 8 at the 1955
    IAU  General Assembly in Dublin, with the observatories at Babelsberg,
    Bergedorf,  Bordeaux, Greenwich, Heidelberg, Nikolajew, Ottawa, Paris,
    Pulkovo,  Strasbourg and Washington (USNO) to collaborate in the work,
    and with  F.  P.  Scott  (USNO)  to  coordinate  the  meridian  circle
    observations of  AGK3R  stars.  The  completion  of  the  photographic
    observations was to be the  responsibility  of  the  observatories  at
    Bergedorf and  Bonn, with  all plate  measurements to  be done  at the
    former. (However, it was finally decided that all plates, even for the
    AGK2 Bonn zones, would  be taken  at Bergedorf.)  The plates  for AGK3
    were  secured at  Bergedorf between  August 1956  and June  1964, with
    special  precautions (exposures  on both  sides of  the pier)  made to
    compensate for possible changes in the camera objective.</para>
    <para>The two  sets  of  plates  were  measured  at  Bergedorf  in  opposite
    directions  and averaged to obtain final x,y coordinates. The detailed
    procedures  for the correction of magnitude-color errors, reduction of
    the measures using  the AGK3R  stars, re-reduction  of AGK2  using its
    reference catalog AGK2A transformed  to  the  FK4  system,  and  final
    reduction  of the AGK3 positions and  proper motions, are discussed by
    W.  Dieckvoss in his  technical introduction to  the source reference.
    Although  a more detailed discussion of  errors is given by Dieckvoss,
    the  standard error for one coordinate on one plate as determined from
    a limited  sample of 110 pairs  of plates is +/- 0.025" for AGK3.</para>
   </details>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="agk3.dat">
     <title>Catalog Data</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>AGsign</name>
     <definition>Sign of AGK3 number.</definition>
     <units>---</units>
    </field>
    <field>
     <name>AGzone</name>
     <definition>AGK3 zone.</definition>
     <units>---</units>
    </field>
    <field>
     <name>AGnum</name>
     <definition>AGK3 number
      <footnote>
       <para>AGK3 number in increasing order within each declination zone.
   The field is filled with preceding zeros.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>m_AGnum</name>
     <definition>Component for duplicates
      <footnote>
       <para>Component identification where duplicates AGK3 numbers occur.
   The lower case letters "a" and "b" may be present.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>Pmag</name>
     <definition>Photographic magnitude from AGK2</definition>
     <units>mag</units>
    </field>
    <field>
     <name>Sp</name>
     <definition>Spectral type
      <footnote>
       <para>Spectral Type from Henry Draper Catalogue (Cannon and Pickering,
   1918-1924), its Extension (Cannon, 1925-1936), Schildt (Yale
   Transactions) or determined by A. N. Vyssotsky and collaborators at
   the Leander-McCormick Obs.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right ascension hours (1950.0)</definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right ascension minutes (1950.0)</definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Right ascension seconds</definition>
     <units>s</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Sign of declination (1950.0)</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination degrees (1950.0)</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination minutes</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Declination seconds</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>nobs</name>
     <definition>Number of photographic observations
      <footnote>
       <para>Number of photographic observations used to determine the position.
   Single-digit numbers are preceded by a zero.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>Ep-1900</name>
     <definition>Epoch of AGK3 position minus 1900</definition>
     <units>yr</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Annual proper motion in right ascension
      <footnote>
       <para>Annual proper motion in right ascension multiplied by cos(delta),
   determined by differencing the AGK3 and AGK2 positions and dividing
   by the epoch difference. Proper motions are missing for stars new
   in AGK3 (see Table 6).  If a calculated value of the proper motion
   exceeded the field capacity a value of "9999" is given with a "+"
   in byte 38.  The suggested format reads the datum in the correct
   units.</para>
      </footnote>
     </definition>
     <units>mas/yr</units>
    </field>
    <field>
     <name>pmDE</name>
     <definition>Annual proper motion in declination</definition>
     <units>mas/yr</units>
    </field>
    <field>
     <name>dEpoch</name>
     <definition>Epoch difference AGK3-AGK2</definition>
     <units>yr</units>
    </field>
    <field>
     <name>BD</name>
     <definition>Full BD catalog designation
      <footnote>
       <para>The full BD identification (see cat. &lt;I/122>) contains:
    bytes 59-60: "BD" or blank
    byte     61:  Sign of BD zone number
    bytes 62-63:  BD zone number
    bytes 64-68:  BD number within zone</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>m_BD</name>
     <definition>Component of multiple system
      <footnote>
       <para>Numerical code for identification of a component of a multiple
   system: (1 = primary [P]; 2 = secondary [S]; 3 = A; 4 = B; 5 = S1;
   6 = S2; 7 = P1; 8 = P2; 9 = C).  BD supplemental stars (lower case
   letters) are assigned codes but are indistinguishable from A and B
   designations because the codes are the same. Since the file format
   only allows one byte for the duplicity code, and nine codes are
   already used, the distinction cannot be drawn.  If it is necessary
   to distinguish or identify supplemental stars, the Catalog of BD
   Supplemental Stars (Warren and Kress 1980) should be used.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>Sum</name>
     <definition>Sum of discrepancy codes
      <footnote>
       <para>Sum of discrepancy codes, calculated as the sum of 2**v (2 to the
   power of v), where v = 0 (BD number), 1 (mpg and/or spectral type),
   2 (AGK2 right ascension), 3 (AGK2 declination), 4 (AGK3 right
   ascension), 5 (AGK3 declination).</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>pmsec</name>
     <definition>Annual proper motion in seconds of RA,
                                  computed by dividing by 15cos(delta)</definition>
     <units>s/yr</units>
    </field>
    <field>
     <name>dRA</name>
     <definition>The difference in right ascension in the
                                  sense AGK3 - AGK2modified
      <footnote>
       <para>The residual quantity of the difference in right ascension
   (multiplied by cos(delta)) in the sense AGK3 - (AGK2modified), where
   the last quantity denotes data from the re-reduced AGK2.</para>
      </footnote>
     </definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>dDE</name>
     <definition>The difference in declination in the sense
                                  AGK3 - AGK2modified</definition>
     <units>arcsec</units>
    </field>
   </fields>
  </tableHead>
  <textFile xlink:href="agk3.doc">
   <name>agk3.doc</name>
   <description>
    <para>Documentation</para>
   </description>
  </textFile>
  <history>
   <ingest>
    <creator>
     <lastName>James E. Gass and Gail L. Schneider</lastName>
     <affiliation>SSDOO/ADC</affiliation>
    </creator>
    <date>
     <year>1997</year>
     <month>Jul</month>
     <day>01</day>
    </date>
   </ingest>
   <revisions>
    <revision>
     <creator>
      <lastName>UNKNOWN</lastName>
     </creator>
     <date>
      <year>UNKNOWN</year>
     </date>
     <para>The machine version of the AGK3 was received on magnetic tape from
   the Centre de Donnees Stellaires, Strasbourg in 1978.  The version
   received had been obtained originally from the Astronomisches
   Rechen- Institut in Heidelberg.  A preliminary document for a
   modified and corrected version of the catalog was produced by Nagy
   (1979).  The following changes were made to the Heidelberg file in
   order to correct some minor errors and to produce a file conforming
   more closely to the published version:

     1.  AGK3 component identifications for stars where more than one
         AGK3 star has the same number were changed from upper case
         characters (A, B) to lower case (a, b) as in the printed edition.

     2.  Nine stars in AGK3 zone -00, but in BD zone +00 were found to
         have a BD zone of +90.  The BD zone for these stars was changed
         to +00.  These stars are: AGK3 -00 1467, 1510, 1530, 1531, 1532,
         1602, 1693, 1774, and 2120.

    1-Jul-1997: Explicit decimal points added to floating point fields in
       computer-readable version.  Document brought up to standard.
       [J. Gass, ADC]

    1-Sep-1998: filled blanks between sign and value with zeroes in
       columns pmRA, pmDE, pmsec, dRA, dDE to allow correct interpretations
       [F. Ochsenbien, CDS]</para>
    </revision>
   </revisions>
  </history>
  <identifier>I_61B.xml</identifier>
 </dataset>
 <dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
  <title>Perth 70: A Catalogue of Positions of 24900 Stars Part B, Mean Values of the
Observations</title>
  <altname type="ADC">1062C</altname>
  <altname type="CDS">I/62C</altname>
  <altname type="brief">Perth 70 B: Positions 24900 Stars</altname>
  <reference>
   <source>
    <other>
     <title>Perth 70: A Catalogue of Positions of 24900 Stars Part B, Mean Values of the
Observations</title>
     <author>
      <initial>E</initial>
      <lastName>Hog</lastName>
     </author>
     <author>
      <initial>J</initial>
      <lastName>von der Heide</lastName>
     </author>
     <name>Abh. der Hamberger Sternwarte, Band IX.</name>
     <publisher>???</publisher>
     <city>???</city>
     <date>
      <year>1976</year>
     </date>
     <bibcode>1976AAHam...9....1H</bibcode>
    </other>
   </source>
  </reference>
  <keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
   <keyword xlink:href="Astrometric_data.html">Astrometric data</keyword>
   <keyword xlink:href="Photometry.html">Photometry</keyword>
  </keywords>
  <descriptions>
   <description>
    <para>This Perth 70: A Catalogue of Positions of 24900 Stars contains accurate
   positions and magnitudes of 24,871 reference stars, mostly in the
   southern hemisphere, plus other useful data such as approximate proper
   motions, radial velocities, and parallaxes. The Perth 70 is a result of
   meridian circle observations made by the Hamburg Observatory expedition
   to Perth as part of the international effort on Southern Reference Stars
   (SRS). The catalog described here provides the mean values for each
   star, including the position, magnitude, and mean epoch of observation;
   the proper motions, however, were neither observed nor recomputed from
   comparing the Perth positions to older material.</para>
   </description>
   <details>
    <para>This catalog is the September 1992 version of the results of meridian
   circle carried out at Perth in the late 1960's and early 1970's.</para>
    <para>Some 107 circumpolar stars occupy two records each, one for observations
   at upper culmination and one for observations at lower culmination, so
   the number of records is greater than the number of stars.</para>
    <para>This file contains the mean values of the meridian circle observations
   (position and magnitude) made at Perth, plus auxiliary quantities
   usually taken from the preliminary version of the Southern Reference
   Stars (SRS) catalog (Corwin, 1992). The first part of each record
   presents the same information that is contained in the printed catalog;
   the remaining information was not printed.</para>
    <para>Missing data are denoted by blank-filled fields except for the standard
   errors of one observation in R.A. * cos(dec) and in declination. In
   those fields, missing data are indicated by "0". Stars with numbers in
   the 30000's are in the FK4 catalog, with the last four digits being the
   FK4 number. Stars with numbers in the 40000's are in the Bright Star
   Catalog in the same format. Stars with other numbers are program stars.</para>
   </details>
  </descriptions>
  <tableHead>
   <tableLinks>
    <tableLink xlink:href="newperth.dat">
     <title>The catalog</title>
    </tableLink>
   </tableLinks>
   <fields>
    <field>
     <name>ID</name>
     <definition>Perth 70 catalog number</definition>
     <units>---</units>
    </field>
    <field>
     <name>n_ID</name>
     <definition>S means star is in the FK4 suppl.</definition>
     <units>---</units>
    </field>
    <field>
     <name>V</name>
     <definition>V magnitude
      <footnote>
       <para>If the hundredths place (byte 12) is blank, the number was copied from
   the preliminary SRS; otherwise, the magnitude was observed at Perth.</para>
      </footnote>
     </definition>
     <units>mag</units>
    </field>
    <field>
     <name>Sp</name>
     <definition>Spectral type; from SRS
      <footnote>
       <para>The spectral types are always those of the printed catalog. Two stars
   must be mentioned specifically: fl2 Velorum (SRS #30309) and O Cygni
   (SRS #44262). The first, a Wolf-Rayet star (type WC), is listed in the
   FK5 as "Oap" (the HD designation) and appears here as "O0." The second,
   a Mira Ceti-type pulsating variable, spectral type "S7ev," appears here
   as "M7."</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAh</name>
     <definition>Right ascension hours (B1950)
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
     </definition>
     <units>h</units>
    </field>
    <field>
     <name>RAm</name>
     <definition>Right ascension minutes (B1950)
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
     </definition>
     <units>min</units>
    </field>
    <field>
     <name>RAs</name>
     <definition>Right ascension minutes (B1950)
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
     </definition>
     <units>s</units>
    </field>
    <field>
     <name>cul</name>
     <definition>Culmination flag
      <footnote>
       <para>This is blank except for circumpolar stars, which have 2 records, one
   marked `U' for upper culmination observations, and one marked `L' for
   lower culmination observations.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>DE-</name>
     <definition>Sign of declination</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEd</name>
     <definition>Declination degrees (B1950)</definition>
     <units>deg</units>
    </field>
    <field>
     <name>DEm</name>
     <definition>Declination minutes (B1950)</definition>
     <units>arcmin</units>
    </field>
    <field>
     <name>DEs</name>
     <definition>Declination seconds (B1950)</definition>
     <units>arcsec</units>
    </field>
    <field>
     <name>epRA</name>
     <definition>Mean epoch of observation in RA -1900000
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
     </definition>
     <units>ma</units>
    </field>
    <field>
     <name>epDE</name>
     <definition>Mean epoch of observation in dec -1900000</definition>
     <units>ma</units>
    </field>
    <field>
     <name>o_RA</name>
     <definition>Number of observations in RA
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>RAdel</name>
     <definition>Indicates >=1 obser. in RA deleted
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>o_DE</name>
     <definition>Number of observations in declination</definition>
     <units>---</units>
    </field>
    <field>
     <name>DEdel</name>
     <definition>Indicates >=1 obser. in dec deleted</definition>
     <units>---</units>
    </field>
    <field>
     <name>q_RAs</name>
     <definition>Residual in right ascension
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
      <footnote>
       <para>These are the Perth position minus the position in the preliminary SRS,
   corrected for proper motion to the mean epoch of observation. The signs
   of the residuals are changed for circumpolar stars observed at lower
   culmination.</para>
      </footnote>
     </definition>
     <units>carcsec</units>
    </field>
    <field>
     <name>q_DEs</name>
     <definition>Residual in declination</definition>
     <units>carcsec</units>
    </field>
    <field>
     <name>pmRA</name>
     <definition>Proper motion in right ascension
      <footnote>
       <para>Positions are referred to the system of the FK4 (equinox B1950.0) at the
   mean epoch of observation for each coordinate for each star.</para>
      </footnote>
      <footnote>
       <para>These are copied from the preliminary SRS; the Perth 70 positions were
   not used to compute them. For centennial proper motions, use formats
   F7.3 and F7.2 for proper motion in RA and proper motion in declination,
   respectively.</para>
      </footnote>
     </definition>
     <units>s-5/a</units>
    </field>
    <field>
     <name>pmDE</name>
     <definition>Proper motion in declination
      <footnote>
       <para>These are copied from the preliminary SRS; the Perth 70 positions were
   not used to compute them. For centennial proper motions, use formats
   F7.3 and F7.2 for proper motion in RA and proper motion in declination,
   respectively.</para>
      </footnote>
     </definition>
     <units>arcsec-4/a</units>
    </field>
    <field>
     <name>DMcat</name>
     <definition>Durchmusterung catalog
      <footnote>
       <para>The catalog identifier (bytes 84-85) is either `BD' for Bonner
   Durchmusterung, `CD' for Cordoba Durchmusterung, or `CP' for Cape
   Photographic Durchmusterung. The zone is contained in bytes 87-89 (with
   the sign in byte 87), and the serial number, in bytes 90-94.</para>
      </footnote>
     </definition>
     <units>---</units>
    </field>
    <field>
     <name>DMzone</name>
     <definition>Durchmusterung zone</definition>
     <units>---</units>
    </field>
    <field>
     <name>DMnum</name>
     <definition>Durchmusterung number</definit