<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>Catalogue of 20457 Star Positions Obtained by Photography in the Declination
Zone -48 to -54 Degrees (1950)</title>
	<altname type="ADC">1073B</altname>
		<altname type="CDS">I/73B</altname>
		<altname type="brief">Sydney Photographic Cat 20457 Stars, -48 to -54</altname>
	<reference>
		<source>
<journal>
	<title>Catalogue of 20457 Star Positions Obtained by Photography in the Declination
Zone -48 to -54 Degrees (1950)</title>
	<author>
			<initial>H</initial>
			<lastName>Eichhorn</lastName></author>
	<author>
			<initial>W</initial>
			<initial>D</initial>
			<lastName>Googe</lastName></author>
	<author>
			<initial>C</initial>
			<initial>F</initial>
			<lastName>Lukac</lastName></author>
	<author>
			<initial>J</initial>
			<initial>K</initial>
			<lastName>Murphy</lastName></author>
	<name>AJ</name>
	<volume>88</volume>
	<pageno>546</pageno>
		<date>
			<year>1983</year></date>
	<bibcode>1983AJ.....88..546E</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>
			<keyword xlink:href="Photographic_catalog.html">Photographic catalog</keyword></keywords>
	<descriptions>
				<description>
				<para>
   This catalog is also known as the Sydney Photographic Catalogue -48 to -54
   Degrees or SPC and gives positions determined by the plate
   overlap method from plates taken at the Sydney Observatory in 1964.  The
   catalog was originally planned to fill part of the gap left by the Yale
   Zone and Cape Photographic Catalogues, although the gap has in the meantime
   been closed by catalogs prepared at Sydney Observatory (Nicholson 1979,
   King and Lomb 1983).  Data in the catalog include star number (CPD;
   identifications not complete), source catalog identification (AC zones) and
   related information, right ascension/declination on the FK4 system (equinox
   and equator B1950, average epoch 1964.475), photovisual magnitude, and
   numbers of images and pairs of diffraction spectra used in computing
   position.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>Catalog Data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>CPDnum</name>
			<definition>Number in Cape Photographic Durchmusterung
	<footnote>
			<para>
    From Gill and Kapteyn (1897, 1900).   The zone sign (always -) is in byte 1,
    the zone in bytes 2-3, byte 4 is blank, and the number is in bytes 5-9.
    The identifications are not complete, i.e., existing CPD numbers are not
    always present.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Source</name>
			<definition>Source catalog identification
	<footnote>
			<para>
    A       Gill and Hough (1923)
    B       Jackson and Stoy (1955)
    1-120   Plates in Cape AC zone -49 deg
    121-240 Plates in Cape AC zone -51 deg (Cape 1913-1926)
    241-360 Plates in Sydney AC zone -53 deg (Sydney Obs. 1923-1933; see Wood
             1971)
    where each AC zone is covered by 120 plates and 120 or 240 is subtracted
    to obtain plate numbers in the -51 deg and -53 deg zones, respectively.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>number</name>
			<definition>Star or plate number in the source catalog</definition>
			<units>---</units></field>
		<field>
			<name>refstar</name>
			<definition>Asterisk (*) means the star served as a
                                   reference star.</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension hours (1950)
	<footnote>
			<para>
    Given for the mean coordinate system 1950, ostensibly on the system
    of the FK4, at the average epoch 1964.475 of all plates which provided
    data.  (If higher accuracy epochs are required, Table I of Eichhorn et al.
    1983 should be consulted.)</para></footnote></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>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>Ptm</name>
			<definition>Photovisual magnitude, taken from existing
                                   sources.
	<footnote>
			<para>
    For AC stars, the magnitudes were computed from data given in the AC and
    are photographic.  Magnitudes are neither precise nor accurate and are
    given for reference purposes only.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>o_image</name>
			<definition>Number of measured central images used to
                                   calculate the published position.</definition>
			<units>---</units></field>
		<field>
			<name>o_spect</name>
			<definition>Number of pairs of diffraction spectra used
                                   to calculate the published position.
	<footnote>
			<para>
    The number of individual images measured for computing a published
    position is the number in byte 51 plus twice the number in byte 53
    (see Eichhorn et al. 1983).
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="adc.doc"><name>adc.doc</name><description><para>ADC Documentation</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>James E. Gass</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1997</year><month>Jul</month><day>31</day></date><acknowledgement>Appreciation is expressed to Dr. H. Eichhorn for providing the SPC
    on tape and for reviewing and commenting on the original ADC document.</acknowledgement></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>   The machine-readable version of the SPC was received on magnetic tape from
   records with bytes 1-25 blank and many other blanks throughout the records.
   The records on this tape had been designed specifically for printing the
   catalog and microfiching rather than for efficient storage and computing.
   To increase storage efficiency the following modifications were made after
   checking with the first author to be certain that the changes would be
   acceptable.

   1. Superfluous blanks were removed from throughout the data records,
      except for a single separator blank between each of the data fields
      decreasing the logical record length from 104 to 53 bytes.

   2. Leading zeros were added to all right ascension and declination fields.</para></revision></revisions></history>
	<identifier>I_73B.xml</identifier></dataset>
