<?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>Optical identification of EUV sources from the ROSAT Wide Field
Camera all-sky survey.</title>
	<altname type="ADC">J/MNRAS/274/1194</altname>
		<altname type="CDS">J/MNRAS/274/1194</altname>
		<altname type="brief">Optical Identifications of ROSAT EUV Sources</altname>
	<reference>
		<source>
<journal>
	<title>Optical identification of EUV sources from the ROSAT Wide Field
Camera all-sky survey.</title>
	<author>
			<initial>K</initial>
			<initial>O</initial>
			<lastName>Mason</lastName></author>
	<author>
			<initial>B</initial>
			<initial>J</initial>
			<initial>M</initial>
			<lastName>Hassall</lastName></author>
	<author>
			<initial>G</initial>
			<initial>E</initial>
			<lastName>Bromage</lastName></author>
	<author>
			<initial>D</initial>
			<initial>A</initial>
			<initial>H</initial>
			<lastName>Buckley</lastName></author>
	<author>
			<initial>T</initial>
			<lastName>Naylor</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>O'Donoghue</lastName></author>
	<author>
			<initial>M</initial>
			<initial>G</initial>
			<lastName>Watson</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>Bertram</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Branduardi-Raymont</lastName></author>
	<author>
			<initial>P</initial>
			<initial>A</initial>
			<lastName>Charles</lastName></author>
	<author>
			<initial>B</initial>
			<lastName>Cooke</lastName></author>
	<author>
			<initial>K</initial>
			<initial>H</initial>
			<lastName>Elliott</lastName></author>
	<author>
			<initial>M</initial>
			<initial>R</initial>
			<initial>S</initial>
			<lastName>Hawkins</lastName></author>
	<author>
			<initial>S</initial>
			<initial>T</initial>
			<lastName>Hodgkin</lastName></author>
	<author>
			<initial>S</initial>
			<initial>J</initial>
			<lastName>Jewell</lastName></author>
	<author>
			<initial>C</initial>
			<initial>M</initial>
			<lastName>Jomaron</lastName></author>
	<author>
			<initial>K</initial>
			<lastName>Sekiguchi</lastName></author>
	<author>
			<initial>B</initial>
			<initial>J</initial>
			<lastName>Kellett</lastName></author>
	<author>
			<initial>A</initial>
			<lastName>Lawrence</lastName></author>
	<author>
			<initial>I</initial>
			<lastName>McHardy</lastName></author>
	<author>
			<initial>J</initial>
			<initial>P</initial>
			<initial>D</initial>
			<lastName>Mittaz</lastName></author>
	<author>
			<initial>C</initial>
			<initial>D</initial>
			<lastName>Pike</lastName></author>
	<author>
			<initial>T</initial>
			<initial>J</initial>
			<lastName>Ponman</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Schmitt</lastName></author>
	<author>
			<initial>W</initial>
			<lastName>Voges</lastName></author>
	<author>
			<initial>W</initial>
			<lastName>Wargau</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>Wonnacott</lastName></author>
	<name>Mon. Not. R. Astron. Soc.</name>
	<volume>274</volume>
	<pageno>1194</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995MNRAS.274.1194M</bibcode></journal></source>
	<related>
			<holding role="similar">J/MNRAS/260/77 :  ROSAT Wide Field Camera EUV Bright Sources (Pounds+ 1993)<xlink:simple href="J/MNRAS/260/77"/></holding>
			<holding role="similar">J/MNRAS/274/1165 :  The 2RE Source Catalogue (Pye+ 1995)<xlink:simple href="J/MNRAS/274/1165"/></holding>
			   Pye J.P. et al.,     =1995MNRAS.274.1165P
   Schwartz R.D. et al. =1995PASP..107..667S</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>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="binaries_general.html">binaries: general</keyword>
			<keyword xlink:href="catalogs.html">catalogs</keyword>
			<keyword xlink:href="galaxies_active.html">galaxies: active</keyword>
			<keyword xlink:href="novae_cataclysmic_variables.html">novae, cataclysmic variables</keyword>
			<keyword xlink:href="stars_activity.html">stars: activity</keyword>
			<keyword xlink:href="white_dwarfs.html">white dwarfs</keyword></keywords>
	<descriptions>
				<description>
				<para>
    Optical identifications for 195 EUV sources located in the ROSAT Wide
    Field Camera all-Sky survey are presented. We list 69 previous unknown
    EUV-emitting white dwarfs, 114 active stars, 7 new magnetic
    cataclysmic variables and 5 active galaxies. Several of the white
    dwarfs have resolved M-type companions, while five are unresolved
    white dwarf/M-star pairs. Finding charts are given for the optical
    counterparts.</para></description>
                        <details><para><observatory base="space"> ROSAT</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>WFC optical identification programme ID summary</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>l_S1</name>
			<definition>Limit flag on S1</definition>
			<units>---</units></field>
		<field>
			<name>S1</name>
			<definition>WFC survey filter S1 (60-140A) counts</definition>
			<units>10-3ct/s</units></field>
		<field>
			<name>l_S2</name>
			<definition>Limit flag on S2</definition>
			<units>---</units></field>
		<field>
			<name>S2</name>
			<definition>WFC survey filter S2 (110-200A) counts</definition>
			<units>10-3ct/s</units></field>
		<field>
			<name>NH</name>
			<definition>Hydrogen column density</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension J2000</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension J2000</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension J2000</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination J2000</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination J2000</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination J2000</definition>
			<units>arcsec</units></field>
		<field>
			<name>n_DE</name>
			<definition>A 'g' indicates that the data are from
                                   the Hubble Space Telescope Guide Star Catalog</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude of the optical counterpart</definition>
			<units>mag</units></field>
		<field>
			<name>n_Vmag2</name>
			<definition>'-' when interval</definition>
			<units>---</units></field>
		<field>
			<name>Vmag2</name>
			<definition>Upper limit of Vmag when n_Vmag2='-'</definition>
			<units>mag</units></field>
		<field>
			<name>u_Vmag</name>
			<definition>Uncertainty flag on Vmag</definition>
			<units>---</units></field>
		<field>
			<name>n_Vmag</name>
			<definition>Note on Vmag
	<footnote footnoteId="???"><para>number=1</para>
			<para>P: CCD or photoelectric photometry (Buckley, private communication;
              Schwartz et al. 1995)
          G: The HST Guide Star Catalog (v.1.1)
          cat: catalogued magnitudes (see Pye et al., 1995)
          E: POSS E digitized plate material
          J: SERC J digitized plate material
          S: uncorrected slit magnitudes taken from calibrated spectra
          A 'c' appended to the J and E codes indicates that accurate external
             zero-points were not been obtained by comparing the magnitudes of
             stars within 3arcmin of the EUV source that appear in the HST Guide
             Star Catalog (v.1.1) with the uncorrected values measured for those
             stars from the Schmidt-telescope Sky Survey Plates. If there is
             more than one counterpart, there are separate entries for each
             star when these are available.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V color index of the optical counterpart</definition>
			<units>mag</units></field>
		<field>
			<name>SpType</name>
			<definition>Spectral type of the optical counterpart</definition>
			<units>---</units></field>
		<field>
			<name>l_alpha</name>
			<definition>Limit flag on alpha</definition>
			<units>---</units></field>
		<field>
			<name>alpha</name>
			<definition>Source apparent EUV to optical flux ratio</definition>
			<units>---</units></field>
		<field>
			<name>Class</name>
			<definition>Identification class
	<footnote footnoteId="???"><para>number=2</para>
			<para>Star: all active stars
          WD: white dwarf
          CV: cataclysmic variable
          AGN: active galaxy</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>EWCa</name>
			<definition>Equivalent width of the Ca H 3933A
                                    chromospheric emission line (for stars only)</definition>
			<units>0.1nm</units></field>
		<field>
			<name>n_EWCa</name>
			<definition>Note on EWCa
	<footnote footnoteId="???"><para>number=3</para>
			<para>u: the line was covered but no measurable emission component was
              detected. Significant chromospheric emission may still be present,
              particularly when this refers to Halpha (e.g. the Halpha
              photospheric absorption line may be 'filled-in' by emission)
          -: the line was not covered in the spectra
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>---</name>
			<definition>Separator</definition>
			<units>---</units></field>
		<field>
			<name>EWHa</name>
			<definition>Equivalent width of the Halpha line
                                    (for stars only)</definition>
			<units>0.1nm</units></field>
		<field>
			<name>n_EWHa</name>
			<definition>Note on EWHa
	<footnote footnoteId="???"><para>number=3</para>
			<para>u: the line was covered but no measurable emission component was
              detected. Significant chromospheric emission may still be present,
              particularly when this refers to Halpha (e.g. the Halpha
              photospheric absorption line may be 'filled-in' by emission)
          -: the line was not covered in the spectra
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>FWHb</name>
			<definition>Full width at half maximum of the Hbeta line</definition>
			<units>10+3km/s</units></field>
		<field>
			<name>---</name>
			<definition>Separator</definition>
			<units>---</units></field>
		<field>
			<name>EWHb</name>
			<definition>Equivalent width of the Hbeta line</definition>
			<units>0.1nm</units></field>
		<field>
			<name>u_EWHb</name>
			<definition>Uncertainty flag on EWHb</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>y: there is an X-ray telescope position
                                    available for the source</definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>+: additional information in appena file</definition>
			<units>---</units></field>
		<field>
			<name>Com</name>
			<definition>Comments</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="table1.tex"><name>table1.tex</name><description><para>TeX version of table1</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Aug</month><day>23</day></date><acknowledgement>K.O. Mason &lt;kom@mssl.ucl.ac.uk></acknowledgement></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> In table1, 2RE J033711+255926 was identified to HD 224030
     instead of HD 22403. Correction made on 13-Feb-1998.</para></revision></revisions></history>
	<identifier>J_MNRAS_274_1194.xml</identifier></dataset>
