<?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>A Catalogue of Homogeneous Photometry of Bright Stars on the DDO System</title>
	<altname type="ADC">2080</altname>
		<altname type="CDS">II/80</altname>
		<altname type="brief">Homogeneous Photometry Bright Stars on DDO System</altname>
	<reference>
		<source>
<journal>
	<title>A Catalogue of Homogeneous Photometry of Bright Stars on the DDO System</title>
	<author>
			<initial>R</initial>
			<initial>D</initial>
			<lastName>McClure</lastName></author>
	<author>
			<initial>W</initial>
			<initial>T</initial>
			<lastName>Forrester</lastName></author>
	<name>Publ. Dominion Astrophys. Obs.</name>
	<volume>15</volume>
	<pageno>439</pageno>
		<date>
			<year>1981</year></date>
	<bibcode>1981PDAO...15...14M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_DDO.html">Photometry, DDO</keyword>
			<keyword xlink:href="Stars_bright.html">Stars, bright</keyword></keywords>
	<descriptions>
				<description>
				<para>
  The catalogue of homogeneous photometry of bright stars on the DDO
  (System McClure and Forrester 1981) is a compilation of DDO
  photometry of 2196 bright G and K stars prepared from observations
  made at Kitt Peak National and Cerro Tololo Inter-American
  Observatories over the last several years using filter sets well
  matched to the standard system.  The catalogue includes a large
  number of DDO stars whose data have been taken directly from the
  standard-star paper of McClure (1976), plus a representative sample
  of stars selected from the Catalogue of Bright Stars (Hoffleit 1964)
  and the Catalogue of High-Velocity Stars (Eggen 1964) to have good
  velocities, spectral types and freedom from companion contamination.
  The catalogue contains HD Catalogue numbers, DM identifications; and
  the standard photometric indices of the DDO system:  magnitude at
  4800 angstroms, and the color indices c(45-48), c(42-45), c(41-42),
  c(38-41), and c(35-38).  The number of observations from which each
  index was determined is also given, along with standard errors.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>Catalog data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>cat</name>
			<definition>Henry Draper (HD) Catalogue number (blank
                                   for five stars not in the HD)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>flag1</name>
			<definition>HD Code (1 = A component; 9 if HD and HD+1
                                  included in observation, e.g. 179957/8; 0
                                  otherwise)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>DM</name>
			<definition>Durchmusterung catalog (DM) identification
	<footnote>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>sign</name>
			<definition>Sign of DM zone
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>DMzon</name>
			<definition>DM zone
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>DMnum</name>
			<definition>DM number
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>m48</name>
			<definition>48 filter magnitude m48
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_m48</name>
			<definition>Standard error sigma/sqrt(N) of m48
	<footnote>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>f_m48</name>
			<definition>Asterisk if error in m48 > 0.099 magnitude
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>C(45-48)</name>
			<definition>Color-index C(45-48)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_C(45-48)</name>
			<definition>Standard error of C(45-48)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mmag</units></field>
		<field>
			<name>C(42-45)</name>
			<definition>Color index C(42-45)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_C(42-45)</name>
			<definition>Standard error of C(42-45). See bytes 34-35.
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>C(41-42)</name>
			<definition>Color index C(41-42)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_C(41-42)</name>
			<definition>Standard error of C(41-42). See bytes 34-35.
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>C(38-41)</name>
			<definition>Color index C(38-41)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_C(38-41)</name>
			<definition>Standard error of C(38-41). See bytes 25-26.
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>f_C(38-41)</name>
			<definition>Asterisk if error in C(38-41) > 0.099
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>C(35-38)</name>
			<definition>Color index C(35-38)
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_C(35-38)</name>
			<definition>Standard error of C(35-38). See bytes 25-26.
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>f_C(35-38)</name>
			<definition>Asterisk if error in C(35-38) > 0.099
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Nobs</name>
			<definition>Number of observations
	<footnote>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>f_Nobs</name>
			<definition>Note on Nobs
	<footnote>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  BD = Bonner Durchmusterung
  CD = Cordoba Durchmusterung
  CP = Cape Photographic Duchmusterung</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  blank = no mean error given because of only a single observation, standard
          star, or error > 0.099</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Array of 6 digits giving numbers of observations, Nobs, contributing to the
  magnitude and colors, respectively. Fields are all blanks for standard stars
  where data are taken directly from McClure (1976), and in cases where all
  Nobs > 9 (see byte 79).</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  * = Nobs is blank because number of observations is > 9
  S = Standard star
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>M.C. Larkin</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
			<creator>
				<lastName>C.-H. Joseph Lyu</lastName>
				<affiliation>Hughes STX/NASA</affiliation></creator>
	<date>
		<year>1995</year><month>May</month><day>10</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  The catalogue was received on magnetic tape from Dr. Robert D. McClure of
  the Dominion Astrophysical Observatory on 5 January 1982.  The following
  modifications to the original format were made in order to make the data
  easier to process by the general user while still retaining all
  information and coding in the original data set:
  1.  All records were condensed by eliminating unused bytes between the data
      fields in order to make room for the addition of Durchmusterung (DM)
      numbers for the HD stars.
  2.  DM numbers were inserted into the records by retrieving them from an
      updated and corrected version of the SAO-HD-DM-GC Cross Index
      (Warren and Roman 1981) which had been sorted by HD number.  Eleven
      stars not in the cross index (non-SAO stars) were looked up manually
      using the HD catalogue and inserted.
  3.  Multiple HD numbers, e.g. HD 110379/80 were replaced by the lower
      number alone followed by a 9 to indicate that the data are for HD and
      HD + 1, i.e. the standard codes adopted by the Centre de Donnees
      Stellaires, Strasbourg, were added to all HD numbers (see description
      for byte 7).
  4.  Asterisks in the standard error fields of m48, C(38-41) and C(35-38),
      used to indicate errors > 0.099 mag, were moved to the flag bytes
      27, 63 and 72 and those standard error fields were blanked out to
      allow the fields to be read with real format specifications.
  5.  Asterisks in the numbers of observations (Nobs) fields were converted to
      blanks and a single asterisk moved to byte 79 for the same reason as
      above.  Also, the abbreviation "STD" in the Nobs fields was changed to
      blanks and the character "S" placed into byte 79 to flag standard stars.
  6.  Plus signs were added to all positive color-index data, always in the
      byte immediately preceding each datum.</para></revision></revisions></history>
	<identifier>II_80.xml</identifier></dataset>