<?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>The 5C13 deep radio survey (16h, +42)</title>
	<altname type="ADC">J/MNRAS/272/699</altname>
		<altname type="CDS">J/MNRAS/272/699</altname>
		<altname type="brief">The 5C13 deep radio survey</altname>
	<reference>
		<source>
<journal>
	<title>The 5C13 deep radio survey (16h, +42)</title>
	<author>
			<initial>C</initial>
			<initial>R</initial>
			<lastName>Benn</lastName></author>
	<name>Mon. Not. R. Astron. Soc.</name>
	<volume>272</volume>
	<pageno>699</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995MNRAS.272..699B</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="radio_continuum_general.html">radio continuum: general</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<description>
				<para>
    A deep 0.4-GHz survey of a 4deg-diameter region in Hercules is
    reported. 232 sources brighter than 9.5 mJy were detected. In a
    simultaneous 1.4-GHz survey of the concentric area 1deg in diameter,
    45 sources brighter than 1.7 mJy were detected. The differential
    0.4-GHz radio source count is presented; it is in good agreement with
    that from other 5C surveys. This survey brings to 3220 the number of
    0.4-GHz sources catalogued by the published 5C surveys.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>The 5C13 catalogue</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>5C13</name>
			<definition>5C13 serial number</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (1950)
	<footnote footnoteId="???"><para>number=1</para>
			<para>measured at 0.4 GHz or, if detected at higher frequency, at 1.4 GHz</para></footnote></definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (1950)
	<footnote footnoteId="???"><para>number=1</para>
			<para>measured at 0.4 GHz or, if detected at higher frequency, at 1.4 GHz</para></footnote></definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (1950)
	<footnote footnoteId="???"><para>number=1</para>
			<para>measured at 0.4 GHz or, if detected at higher frequency, at 1.4 GHz</para></footnote></definition>
			<units>s</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>e_RA</name>
			<definition>rms uncertainty in measured right ascension</definition>
			<units>arcsec</units></field>
		<field>
			<name>S0.4</name>
			<definition>Peak 0.4-GHz flux density</definition>
			<units>mJy</units></field>
		<field>
			<name>e_S0.4</name>
			<definition>rms uncertainty on flux density</definition>
			<units>mJy</units></field>
		<field>
			<name>P0.4</name>
			<definition>Envelope attenuation at 0.4-GHz
	<footnote footnoteId="???"><para>number=2</para>
			<para>S0.4 must be multiplied by this factor to recover the apparent
          flux density S'0.4 with which the source appears on the synthesized
          map, and hence the signal-to-noise ratio
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>S1.4</name>
			<definition>Peak 1.4-GHz flux density</definition>
			<units>mJy</units></field>
		<field>
			<name>e_S1.4</name>
			<definition>rms uncertainty on flux density</definition>
			<units>mJy</units></field>
		<field>
			<name>P1.4</name>
			<definition>Envelope attenuation at 1.4-GHz
	<footnote footnoteId="???"><para>number=2</para>
			<para>S0.4 must be multiplied by this factor to recover the apparent
          flux density S'0.4 with which the source appears on the synthesized
          map, and hence the signal-to-noise ratio
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Alpha</name>
			<definition>Radio spectral index {alpha}
                                   (0.4, 1.4 GHz)</definition>
			<units>---</units></field>
		<field>
			<name>Notes</name>
			<definition>Notes</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>5C13 0.4-GHz source counts</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>S0.4(1)</name>
			<definition>Peak 0.4-GHz lower limit for the
                                        flux density range</definition>
			<units>mJy</units></field>
		<field>
			<name>S0.4(2)</name>
			<definition>Peak 0.4-GHz upper limit for the
                                        flux density range</definition>
			<units>mJy</units></field>
		<field>
			<name>m1</name>
			<definition>Number of sources detected in the
                                        given flux density range before
                                        polar-diagram correction</definition>
			<units>---</units></field>
		<field>
			<name>m2</name>
			<definition>Number of sources detected in the
                                        given flux density range after
                                        polar-diagram correction</definition>
			<units>---</units></field>
		<field>
			<name>DelN</name>
			<definition>Source density</definition>
			<units>10+5sr-1</units></field>
		<field>
			<name>5C13DelN/No</name>
			<definition>5C13 Source density
	<footnote footnoteId="???"><para>number=3</para>
			<para>Normalized to Euclidean integral count 750(S/Jy)^-1.5^/sr
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_5C13DelN/No</name>
			<definition>Error on source density</definition>
			<units>---</units></field>
		<field>
			<name>5CDelN/No</name>
			<definition>Mean source density (3) for the
                                        published 5C surveys
	<footnote footnoteId="???"><para>number=1</para>
			<para>Benn and Wall 1995</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_5CDelN/No</name>
			<definition>Error on source density</definition>
			<units>---</units></field>
		<field>
			<name>B3DelN/No</name>
			<definition>Mean source density (3)
                                        for the B3 survey
	<footnote footnoteId="???"><para>number=2</para>
			<para>Grueff 1988</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_B3DelN/No</name>
			<definition>Error on source density</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout, Simona Mei</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Aug</month><day>16</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> 
    #A022 in H. Andernach's list; Completed at CDS</para></revision></revisions></history>
	<identifier>J_MNRAS_272_699.xml</identifier></dataset>
