<?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>3CR Source Identifications, Update 1990</title>
	<altname type="ADC">J/PASP/97/932</altname>
		<altname type="CDS">J/PASP/97/932</altname>
		<altname type="brief">3CR Source Identifications</altname>
	<reference>
		<source>
<journal>
	<title>3CR Source Identifications, Update 1990</title>
	<author>
			<initial>H</initial>
			<lastName>Spinrad</lastName></author>
	<author>
			<initial>S</initial>
			<lastName>Djorgovski</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Marr</lastName></author>
	<author>
			<initial>L</initial>
			<lastName>Aguilar</lastName></author>
	<name>Publ. Astron. Soc. Pac.</name>
	<volume>97</volume>
	<pageno>932</pageno>
		<date>
			<year>1985</year></date>
	<bibcode>1985PASP...97..932S</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Radio_sources.html">Radio sources</keyword>
			<keyword xlink:href="Redshifts.html">Redshifts</keyword></keywords>
	<descriptions>
				<description>
				<para>
   This catalog contains the third major update of new optical and radio data
   for the strong sources in the Revised Third Cambridge Catalogue (3CR).
   Positions, redshifts, magnitudes, and identifications are included,
   as well as some radio data for 298 3CR sources.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="3CR.dat">
	<title>catalog</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>3CR</name>
			<definition>3CR catalog number
	<footnote>
			<para>
  This columns gives the catalog number in the Revised 3CR Catalog of Radio
  Sources.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 1950 - hours</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension  - minutes</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension  - seconds</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 - degrees</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination - arc minutes</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination - arc seconds</definition>
			<units>arcsec</units></field>
		<field>
			<name>V</name>
			<definition>V visual magnitude
	<footnote>
			<para>
  These columns contain information about the visual magnitude of the source.
  The mv column lists the visual magnitude of the object.  If the mv is given
  in an even 0.5-magnitude interval, it has normally been estimated from the
  Palomar Sky Survey or direct photographic plates and therefore carries
  substantial errors (+/- 0.5-1.0 magnitude).  An asterisk in the mvar_flg
  column indicates variability in mv with amplitude greater than 0.1 magnitude.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>Vflag</name>
			<definition>[* ] variable magnitude flag</definition>
			<units>---</units></field>
		<field>
			<name>z</name>
			<definition>redshift</definition>
			<units>---</units></field>
		<field>
			<name>S(178)</name>
			<definition>flux density at 178 MHz from Kellerman et al</definition>
			<units>Jy</units></field>
		<field>
			<name>Alph</name>
			<definition>spectral index
	<footnote>
			<para>
  These columns give information on the spectral index of the source.
  The spectral index given typically between 38 MHz and 750 MHz (see flags
  listed below) and is taken from Kellermann et al. (1969).  The spectral
  index is defined as S prop. nu^(-alpha).</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>b</name>
			<definition>galactic lattitude</definition>
			<units>---</units></field>
		<field>
			<name>r_ID</name>
			<definition>reference for optical position
	<footnote>
			<para>
  The values refer to these references by number, and
  concern the origin of the optical identification, redshift, and
  radio map.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>r_z</name>
			<definition>reference for redshift</definition>
			<units>---</units></field>
		<field>
			<name>r_Radio</name>
			<definition>reference for radio position</definition>
			<units>---</units></field>
		<field>
			<name>notes</name>
			<definition>Remarks on source
	<footnote>
			<para>
  This column gives additional information about the optical identification.
  For the optical identification we have generally listed the first published
  ID with a good finding chart.  In cases where a previous paper without a
  good finding chart published the same ID or where the ID was confirmed by a
  subsequent, more detailed study, these references are listed under this
  column.   In addition to listing additional information and redshift
  references, the remarks column gives other names (such as NGC number) and
  the character of the optical spectrum of radio galaxies using the following
  abbreviations:

   SE   strong emission lines
   E    emission lines present but not necessarily strong
   WE   weak emission lines
   ABS  only stellar absorption features are seen

  ABS remarks for QSOs indicates the presence of absorption features at one
  or more redshifts.  Abbreviations used here include:

   CL   cluster
   EF   empty field
   FC   finding chart
   G    galaxy
   ID   identification
   N    NGC
   Q    QSO
   SP   spectrophotometry
   X    indicates that the reference number preceding gives an incorrect
   *    probable or possible identification or redshift</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>ID</name>
			<definition>IDentification of source
	<footnote>
			<para>
  These columns give information about the optical identification.
  The following abbreviations are used in the id column:

   B:   BL Lac Object
   G:   Galaxy
   N:   N Galaxy
   Q:   QSO</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="ref.dat">
	<title>list of references</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>RefID</name>
			<definition>Reference identification number</definition>
			<units>---</units></field>
		<field>
			<name>RefText</name>
			<definition>Reference text</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>N.P.M. Kuin</lastName>
				<affiliation>ADC/SSDOO/NASA</affiliation></creator>
	<date>
		<year>1995</year><month>Feb</month><day>14</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>   The data were provided to the ADC on  1993-07-20 by Mark Dickinson for Hy i
   Spinrad.  The documentation was updated with documentation written by D.E.
   Harris of SAO for the ADS version of this catalog. The ADS version includes
   extra fields: a Red Magnitude flag, a spectral index flag,  and an
   identification flag. This catalog is also in the Andernach radio catalog
   archive as A035.</para></revision></revisions></history>
	<identifier>J_PASP_97_932.xml</identifier></dataset>
