<?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>Cape Photographic Catalogue 2</title>
	<altname type="ADC">1085</altname>
		<altname type="CDS">I/85</altname>
		<altname type="brief">Cape Photographic Catalogue 2</altname>
	<reference>
		<source>
<journal>
	<title>Cape Photographic Catalogue 2</title>
	<author>
			<initial>W</initial>
			<lastName>Nicholson</lastName></author>
	<author>
			<initial>M</initial>
			<initial>J</initial>
			<lastName>Penston</lastName></author>
	<author>
			<initial>C</initial>
			<initial>A</initial>
			<lastName>Murray</lastName></author>
	<author>
			<initial>C</initial>
			<lastName>de Vegt</lastName></author>
	<name>Mon. Not. Roy. Astron. Soc.</name>
	<volume>208</volume>
	<pageno>911</pageno>
		<date>
			<year>1984</year></date>
	<bibcode>1984MNRAS.208..911N</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="Proper_motions.html">Proper motions</keyword>
			<keyword xlink:href="Photographic_catalog.html">Photographic catalog</keyword></keywords>
	<descriptions>
				<description>
				<para>
   This catalog contains the provisional positions for 51018 stars in the
   Cape zone -40 deg. to -52 deg., on the FK4 system for the equinox
   1950.0. The internal mean error of a single coordinate obtained from the
   mean of r=four plates is estimated to be less than +/- 0.1" at the mean
   epoch of observation, about 1962. The systematic deviation from the FK4
   system in a small area is probably also about +/-0.1". New proper
   motions have been determined for 22731 stars which are also in the
   Smithsonian Astrophysical Observatory (SAO) catalogue; the formal mean
   error of an annual proper motion in each coordinate is about
   +/-0.004"/a.</para></description>
			<details>
			<para>
   The usable width of each plate is 4.1 deg. Stars were selected from the
   SRS and SAO catalogs, with the SRS providing the reference frame. All
   SAO stars were included except in crowded fields near the galactic
   plane, in which many SAO stars were omitted. Stars were then added by
   visual inspection to bring the number up to about 250, with as uniform a
   distribution as possible over the plate. The number of stars measured
   per plate varied from 70 to more than 700.</para><para>   The numbering system adopted is based on the South Polar Distance of a
   band of declination 1 deg. wide with the stars within each band being
   numbered sequentially in the order of right ascension.</para><para>   Approximate visual magnitudes have been determined from the image
   diameters calibrated by the V values from the published literature. Only
   three plates have fewer than 10 such standards; 75% of the plates have
   between 15 and 30. Generally, the available stars are brighter than
   V-9.5 mag.</para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="cpc2.dat">
	<title>The catalog</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>CPC2P number</definition>
			<units>---</units></field>
		<field>
			<name>SAO</name>
			<definition>SAO number</definition>
			<units>---</units></field>
		<field>
			<name>SRS</name>
			<definition>SRS number</definition>
			<units>---</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension seconds (1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign of declination</definition>
			<units>---</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination seconds (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>mag</name>
			<definition>Magnitude</definition>
			<units>cmag</units></field>
		<field>
			<name>ep</name>
			<definition>Epoch of observation - 1900</definition>
			<units>a</units></field>
		<field>
			<name>e_RAs</name>
			<definition>Internal mean error in RAs</definition>
			<units>arcsec</units></field>
		<field>
			<name>e_DEs</name>
			<definition>Internal mean error in DEs</definition>
			<units>arcsec</units></field>
		<field>
			<name>n_mag</name>
			<definition>Magnitude status
	<footnote>
			<para>
   0 = not available
   1 = normal
   2 = variable
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>o_pos</name>
			<definition>Number of plates used for position</definition>
			<units>---</units></field>
		<field>
			<name>o_mag</name>
			<definition>Number of plates used for magnitude</definition>
			<units>---</units></field>
		<field>
			<name>del_SS</name>
			<definition>Separation of SRS and CPC2 positions</definition>
			<units>arcsec</units></field>
		<field>
			<name>pmRA</name>
			<definition>Annual proper motion in RA</definition>
			<units>s-4/a</units></field>
		<field>
			<name>pmDE</name>
			<definition>Annual proper motion in declination</definition>
			<units>marcsec/a</units></field>
		<field>
			<name>e_pmRA</name>
			<definition>Mean error of proper motion in RA</definition>
			<units>s-4/a</units></field>
		<field>
			<name>e_pmDE</name>
			<definition>Mean error of pm in declination</definition>
			<units>marcsec/a</units></field>
		<field>
			<name>del_pm</name>
			<definition>Larger pm diff. |CPC2-SAO| in RA or DE</definition>
			<units>marcsec/a</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>N. G. Roman</lastName>
				<affiliation>ADC/SSDOO</affiliation></creator>
	<date>
		<year>1997</year><month>Jul</month><day>25</day></date></ingest>
		</history>
	<identifier>I_85.xml</identifier></dataset>
