<?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>X-ray sources &lt;1 degree from Seyfert galaxies.</title>
	<altname type="ADC">J/A+A/319/18</altname>
		<altname type="CDS">J/A+A/319/18</altname>
		<altname type="brief">X-ray sources &lt;1 degree from Seyfert galaxies</altname>
	<reference>
		<source>
<journal>
	<title>X-ray sources &lt;1 degree from Seyfert galaxies.</title>
	<author>
			<initial>H</initial>
			<initial>-D</initial>
			<lastName>Radecke</lastName></author>
	<name>Astron. Astrophys.</name>
	<volume>319</volume>
	<pageno>18</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;A...319...18R</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Galaxies_Seyfert.html">Galaxies, Seyfert</keyword>
			<keyword xlink:href="X-ray_source.html">X-ray source</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_Seyfert.html">galaxies: Seyfert</keyword>
			<keyword xlink:href="galaxies_spiral.html">galaxies: spiral</keyword>
			<keyword xlink:href="X-rays_galaxies.html">X-rays: galaxies</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    Archived PSPC observations of 26 Seyfert galaxies have been analyzed
    for bright X-ray sources out to the full extent of the field
    (&lt; about 50'). Of all Seyferts known this represents a sample 88%
    complete to B_T_=10mag, 74% complete to 11mag and 50% complete to
    12mag. Using the same reduction algorithm, 14 fields centered on stars
    at high galactic latitudes have been used as control fields. Excluding
    the two brightest Seyferts, a subset of 24 Seyferts with corrected
    apparent magnitude between 8.04&lt;B^o,i^_T_&lt;12.90mag show a minimum
    excess of 46 bright X-ray sources generally distributed between 10 and
    25' from the target galaxy. The significances of association of these
    sources with the Seyferts in the median brightness range are as high
    as 7.4-sigma.</para></abstract>
                        <details><para><observatory base="space"> ROSAT</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Fields analyzed</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Object</name>
			<definition>Object name (Seyfert galaxies and reference
                                 stars) used in the analysis</definition>
			<units>---</units></field>
		<field>
			<name>Exp</name>
			<definition>ROSAT PSPC exposure time</definition>
			<units>ks</units></field>
		<field>
			<name>GLAT</name>
			<definition>Galactic latitude of the target object</definition>
			<units>deg</units></field>
		<field>
			<name>Bmag</name>
			<definition>Brightness of the target object (Apparent
                                   blue magnitude, corrected for galactic and
                                   internal absorption)</definition>
			<units>mag</units></field>
		<field>
			<name>1/2D25</name>
			<definition>Semi-apparent major isophotal diameter at
                                   surface brightness level 25.0 B-mag/arcsec^2^</definition>
			<units>arcmin</units></field>
		<field>
			<name>Class</name>
			<definition>Seyfert classification</definition>
			<units>---</units></field>
		<field>
			<name>MType</name>
			<definition>Seyfert type</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="appena">
	<title>Detected Sources with counts rate
                                  above 5.0*10^-3^cts/s</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Field</name>
			<definition>Field centered on the object mentioned</definition>
			<units>---</units></field>
		<field>
			<name>Object</name>
			<definition>Object number</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (2000) of the sources detected</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (2000) of the sources detected</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (2000) of the sources detected</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (2000) of the sources detected</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (2000) of the sources detected</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (2000) of the sources detected</definition>
			<units>arcsec</units></field>
		<field>
			<name>PosOff</name>
			<definition>Offaxis position of the detected sources</definition>
			<units>arcmin</units></field>
		<field>
			<name>Counts</name>
			<definition>Rate Counts rate of the detected sources</definition>
			<units>10-3ct/s</units></field>
		<field>
			<name>CF</name>
			<definition>CF for control field</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>May</month><day>06</day></date><acknowledgement>Hans Dieter Radecke &lt;hdr@mpe-garching.mpg.de></acknowledgement></ingest>
		</history>
	<identifier>J_A+A_319_18.xml</identifier></dataset>
