<?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 Einstein Two-Sigma Catalog</title>
	<altname type="ADC">J/ApJ/461/127</altname>
		<altname type="CDS">J/ApJ/461/127</altname>
		<altname type="brief">The Einstein Two-Sigma Catalog</altname>
	<reference>
		<source>
<journal>
	<title>The Einstein Two-Sigma Catalog</title>
	<author>
			<initial>E</initial>
			<initial>C</initial>
			<lastName>Moran</lastName></author>
	<author>
			<initial>D</initial>
			<initial>J</initial>
			<lastName>Helfand</lastName></author>
	<author>
			<initial>R</initial>
			<initial>H</initial>
			<lastName>Becker</lastName></author>
	<author>
			<initial>R</initial>
			<initial>L</initial>
			<lastName>White</lastName></author>
	<name>Astrophys. J.</name>
	<volume>461</volume>
	<pageno>127</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996ApJ...461..127M</bibcode></journal></source>
	<related>
			<holding role="similar">VII/152 : Einstein Medium Sensitivity Survey Catalog<xlink:simple href="VII/152"/></holding>
			   Moran, E.C., Helfand, D.J., Becker, R.H., White, R.L. 1996: ApJ. 461, 127. </related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="X-ray_sources.html">X-ray sources</keyword></keywords>
	<descriptions>
				<description>
				<para>
  The X-ray sources from the observations with the Einstein Observatory 
  (HEAO-2) with intensities of 2-sigma above the background are compiled
  in this catalog. This catalog covers more sky at fainter flux levels
  than the Einstein Medium Sensitivity Survey. Fields with diffuse 
  emission sources were excluded. Thus data within 10 degrees of the 
  galactic plane as well as fields within the boundaries of the 
  Magellanic Clouds were excluded. The catalog covers 1850 sq. degrees 
  of the sky.  </para><para>  The generation of the Einstein Two-Sigma Catalog was described in 
  detail by Moran et al. (1996).  Read this article carefully to ensure 
  responsible use of the Catalog.  Address any questions to Ed Moran 
  (edhed@igpp.llnl.gov). In particular it should be noted that only 28%,
  or about 13,000 sources in the 2-sigma catalog are real sources.
  The authors show that cross-correlations with other catalogs is an
  effective way to select sources in this catalog that are probably real.</para></description>
                        <details><para><observatory base="space"> HEAO-2</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="twosigma.dat">
	<title>The 2-sigma catalog</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>RAh</name>
			<definition>RA (1950) of the source</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>RA (1950) of the source</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>RA (1950) of the source</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign Declination (1950)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Dec (1950) of the source</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Dec (1950) of the source</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Dec (1950) of the source</definition>
			<units>arcsec</units></field>
		<field>
			<name>S/N</name>
			<definition>Signal-to-noise ratio of the source 
	<footnote>
			<para> 
  Signal-to-noise ratio of the source, based on the counts collected 
  within a 1.25 arcmin radius circular aperture.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>IPCSEQ</name>
			<definition>IPC Sequence number containing the source</definition>
			<units>---</units></field>
		<field>
			<name>cnts125</name>
			<definition>Number of background-subtracted counts 
                                 collected within a 1.25 arcmin radius 
                                 circular aperture
	<footnote>
			<para>
  The number of background-subtracted counts contained in the source,
  collected within circular apertures of radii 1.25 and 2.0 arcmin.</para></footnote></definition>
			<units>arcmin-2</units></field>
		<field>
			<name>cnts20</name>
			<definition>Number of background-subtracted counts
                                 collected within a 2.0 arcmin radius 
                                 circular aperture</definition>
			<units>arcmin-2</units></field>
		<field>
			<name>exp125</name>
			<definition>flatfield-weighted exposure time for the 
                                 source in the 1.25 arcmin radius aperture
	<footnote>
			<para> 
  The flatfield-weighted exposure time (sec) for the source in the 
  1.25 and 2.0 arcmin radius apertures.</para></footnote></definition>
			<units>s</units></field>
		<field>
			<name>exp20</name>
			<definition>flatfield-weighted exposure time for the  
                                 source in the 2.0 arcmin radius aperture</definition>
			<units>s</units></field>
		<field>
			<name>N125</name>
			<definition>Number of "good" pixels used for count in 
                                 the 1.25 arcmin radius aperture
	<footnote>
			<para>
  The number of ``good'' pixels used to accumulate counts for the
  source in the 1.25 arcmin and 2.0 arcmin radius apertures and
  for the background in the concentric 3-6 arcmin radius annulus.
  The edges of the IPC, its window support ribs, or pixel deletions
  resulting from the detection of brighter nearby sources can
  cause these numbers to be less than their maximum values of
  21, 45, and 304.  At least 15 of the 21 pixels in the 1.25 arcmin
  aperture had to be unshadowed and undeleted for a source to
  to be included in the Catalog.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>N20</name>
			<definition>Number of "good" pixels used for count in
                                 the 2.0 arcmin radius aperture</definition>
			<units>---</units></field>
		<field>
			<name>Nbg</name>
			<definition>Number of "good" pixels used for the background
                                 count in the concentric 3-6 arcmin radius 
                                 annulus</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Paul Kuin</lastName>
				<affiliation>NASA/ADC</affiliation></creator>
	<date>
		<year>1997</year><month>Mar</month><day>12</day></date></ingest>
		</history>
	<identifier>J_ApJ_461_127.xml</identifier></dataset>
