<?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>408-MHz observations of two fields in the region 10h30m, +46deg.
I. The surveys</title>
	<altname type="ADC">J/MNRAS/274/324</altname>
		<altname type="CDS">J/MNRAS/274/324</altname>
		<altname type="brief">408MHz Penticton observations of 51P &amp; 52P</altname>
	<reference>
		<source>
<journal>
	<title>408-MHz observations of two fields in the region 10h30m, +46deg.
I. The surveys</title>
	<author>
			<initial>D</initial>
			<initial>A</initial>
			<lastName>Green</lastName></author>
	<author>
			<initial>J</initial>
			<initial>M</initial>
			<lastName>Riley</lastName></author>
	<name>Mon. Not. R. Astron. Soc.</name>
	<volume>274</volume>
	<pageno>324</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995MNRAS.274..324G</bibcode></journal></source>
	<related>
			<holding role="similar">J/MNRAS/246/169 :  14P and 15P sources<xlink:simple href="J/MNRAS/246/169"/></holding>
			<holding role="similar">J/A+A/241/551 :  18P and 19P sources<xlink:simple href="J/A+A/241/551"/></holding>
			<holding role="similar">J/A+AS/77/31 :  20P and 21P sources<xlink:simple href="J/A+AS/77/31"/></holding>
			<holding role="similar">J/A+AS/115/345 :  32P and 33P sources<xlink:simple href="J/A+AS/115/345"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Radio_sources.html">Radio sources</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="catalogs.html">catalogs</keyword>
			<keyword xlink:href="radio_continuum_general.html">radio continuum: general</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We present  results from  radio continuum  observations of  two fields
    made at 408 and 1420MHz with the DRAO Synthesis Telescope. Two sets of
    data, one year apart, were obtained of each field, and here we present
    source   lists  from  the   average  408-MHz  images,   and  from  the
    second-epoch 1420-MHz images. Variability studies at 408MHz from these
    observations will be presented in a forthcoming paper.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="tables">
	<title>1008+46 and 1046+46 fields at 408 and 1240MHz</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Name
	<footnote footnoteId="???"><para>number=1</para>
			<para>51P sources are in 1008+46 field, 52P sources are in 1046+46 field.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Peak right ascension B1950</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Peak right ascension B1950</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Peak right ascension B1950</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Peak declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Peak declination B1950</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Peak declination B1950</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Peak declination B1950</definition>
			<units>arcsec</units></field>
		<field>
			<name>S408pk</name>
			<definition>Peak flux density at 408MHz</definition>
			<units>mJy</units></field>
		<field>
			<name>S408int</name>
			<definition>Integrated peak density at 408MHz</definition>
			<units>mJy</units></field>
		<field>
			<name>n_S408int</name>
			<definition>See note
	<footnote footnoteId="???"><para>number=2</para>
			<para>In some cases the integration area for one peak may contain other
     local maxima from the list; where this has occured the integrated flux
     density will be the same for two or more peaks (indicated by an
     asterisk)
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>S1420pk</name>
			<definition>Peak flux density at 1420MHz</definition>
			<units>mJy</units></field>
		<field>
			<name>S1420int</name>
			<definition>Integrated peak density at 1420MHz</definition>
			<units>mJy</units></field>
		<field>
			<name>n_S1420int</name>
			<definition>See note
	<footnote footnoteId="???"><para>number=2</para>
			<para>In some cases the integration area for one peak may contain other
     local maxima from the list; where this has occured the integrated flux
     density will be the same for two or more peaks (indicated by an
     asterisk)
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Pbm</name>
			<definition>Telescope primary beam response value</definition>
			<units>---</units></field>
		<field>
			<name>S/N</name>
			<definition>Estimate signal-to-noise ratio of the source</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>May</month><day>02</day></date><acknowledgement>The catalogue was provided by Heinz Andernach (R180 in his list)
    &lt;hja@vilspa.esa.es>

    Dave Green   &lt;dag@mrao.cam.ac.uk></acknowledgement></ingest>
		</history>
	<identifier>J_MNRAS_274_324.xml</identifier></dataset>
