<?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>Compendium of Radio Spectra and Luminosities for three complete samples of
Radio Sources</title>
	<altname type="ADC">J/ApJS/81/83</altname>
		<altname type="CDS">J/ApJS/81/83</altname>
		<altname type="brief">Compendium of Radio Spectra and Luminosities</altname>
	<reference>
		<source>
<journal>
	<title>Compendium of Radio Spectra and Luminosities for three complete samples of
Radio Sources</title>
	<author>
			<initial>T</initial>
			<lastName>Herbig</lastName></author>
	<author>
			<initial>A</initial>
			<initial>C</initial>
			<initial>S</initial>
			<lastName>Readhead</lastName></author>
	<name>Astrophys. J. Suppl.</name>
	<volume>81</volume>
	<pageno>83</pageno>
		<date>
			<year>1992</year></date>
	<bibcode>1992ApJS...81...83H</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 is a complete sample of 256 powerful extragalactic radio
  sources. The catalog includes source idenfification, redshift, luminosities
  and spectral indices at standard rest frequencies as well as bolometric
  luminosities between emitted frequencies of 10 MHz and 100 GHz. The paper
  also includes fits to the measured radio spectra which have not been
  included in this catalog.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1.dat">
	<title>Table 1 of Herbig &amp; Readhead 1992, ApJS 81, 83</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>IAUname</name>
			<definition>IAU name of the object.</definition>
			<units>---</units></field>
		<field>
			<name>name</name>
			<definition>Other common name.</definition>
			<units>---</units></field>
		<field>
			<name>z</name>
			<definition>Redshift of the object.</definition>
			<units>---</units></field>
		<field>
			<name>n_z</name>
			<definition>[* ] * means Estimated redshifts
	<footnote>
			<para>
  For 18 of the sources no redshifts were available. For Sources with
  optical identifications but no reliable published redshifts, these were
  estimated from their apparent optical magnitudes. In the case of five
  sources not identified optically, a redshift of 1 was assumed. The
  redshift of these sources has been flagged with a * in this field.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>P_150</name>
			<definition>Emitted Luminosity at 150 MHz
	<footnote>
			<para>
  Emitted specific luminosities at the emitted frequencies shown for a
  value of the Hubble constant of Ho = 100 h km/s/Mpc. The values scale
  with (H/Ho)^-2. To estimate the fluxdensities measured data points
  were interpolated with a cubic spline fit to the observed flux densities.
  Most fits were made in the log S(nu) - log (nu) plane. Closeness of the
  spline fit was adjusted by eye with the parameter phi. Specific
  luminosities were evaluated at the satndard frequencies for a universe
  with qo=0.5 and Lambda=0. The bolometric luminosities were calculated
  from the spline fits. To extrapolate to the limits of the band the spectra
  were extended as power laws from the endpoints of the spline fits.</para></footnote></definition>
			<units>W/Hz</units></field>
		<field>
			<name>P_2500</name>
			<definition>Emitted Luminosity at 2.5 GHz</definition>
			<units>W/Hz</units></field>
		<field>
			<name>P_4000</name>
			<definition>Emitted Luminosity at 40 GHz</definition>
			<units>W/Hz</units></field>
		<field>
			<name>Pbol</name>
			<definition>Emitted bolometric luminosities</definition>
			<units>W</units></field>
		<field>
			<name>alph150</name>
			<definition>Spectral index (S ~ nu^alpha at 150MHz)</definition>
			<units>---</units></field>
		<field>
			<name>alph2500</name>
			<definition>Spectral index at 2.5 GHz</definition>
			<units>---</units></field>
		<field>
			<name>alph4000</name>
			<definition>Spectral index at 40 GHz</definition>
			<units>---</units></field>
		<field>
			<name>phi</name>
			<definition>Spline fitting parameter</definition>
			<units>---</units></field>
		<field>
			<name>mem</name>
			<definition>[ABC ] Sample membership
	<footnote>
			<para>
   (A) revised 3CR survey of Laing et al. 1983 (LRL)
   (B) survey of Peacock and Wall 1981 (PW)
   (C) VLBI sample of Pearson and Readhead 1988 (PR).</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>r_z</name>
			<definition>References to redshifts
	<footnote>
			<para>
   (1) Laing et al. 1983
   (2) Pearson and Readhead 1988
   (3) Peacock and Wall 1981
   (4) Riley, priv. comm.
   (5) Lawrence, priv. comm.
   (6) Xu, priv. comm.
   (7) Murphy 1988
   (8) Veron and Veron 1981
   (9) Spencer et al. 1989
   (10) Hewitt and Burbidge 1987.
   A blank in this column indicates that no reliable redshift is
   available.
   The sources designated as "U" are not identified optically.
</para></footnote></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>
		</history>
	<identifier>J_ApJS_81_83.xml</identifier></dataset>
