<?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 deep X-ray radio blazar survey. I. Methods and first results.</title>
	<altname type="ADC">J/AJ/115/1253</altname>
		<altname type="CDS">J/AJ/115/1253</altname>
		<altname type="brief">Deep X-Ray Radio Blazar Survey</altname>
	<reference>
		<source>
<journal>
	<title>The deep X-ray radio blazar survey. I. Methods and first results.</title>
	<author>
			<initial>E</initial>
			<initial>S</initial>
			<lastName>Perlman</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Padovani</lastName></author>
	<author>
			<initial>P</initial>
			<lastName>Giommi</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Sambruna</lastName></author>
	<author>
			<initial>L</initial>
			<initial>R</initial>
			<lastName>Jones</lastName></author>
	<author>
			<initial>A</initial>
			<lastName>Tzioumis</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Reynolds</lastName></author>
	<name>Astron. J.</name>
	<volume>115</volume>
	<pageno>1253</pageno>
		<date>
			<year>1998</year></date>
	<bibcode>1998AJ....115.1253P</bibcode></journal></source>
	<related>
			<holding role="similar">IX/12 : The WGACAT version of ROSAT sources (White+ 1995)<xlink:simple href="IX/12"/></holding>
			<holding role="similar">VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)<xlink:simple href="VIII/38"/></holding>
			<holding role="similar">VIII/40 : GB6 catalog of radio sources at 4.85GHz (Gregory+ 1996)<xlink:simple href="VIII/40"/></holding>
			<holding role="similar">VIII/15 : Parkes Radio Sources Catalogue (PKSCAT90) (Wright+ 1990)<xlink:simple href="VIII/15"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="BL_Lac_objects.html">BL Lac objects</keyword>
			<keyword xlink:href="QSOs.html">QSOs</keyword>
			<keyword xlink:href="Radio_sources.html">Radio sources</keyword>
			<keyword xlink:href="Surveys.html">Surveys</keyword>
			<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="BL_Lacertae_objects_general.html">BL Lacertae objects: general</keyword>
			<keyword xlink:href="quasars_general.html">quasars: general</keyword>
			<keyword xlink:href="radio_continuum.html">radio continuum</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We have undertaken a survey, the Deep X-Ray Radio Blazar Survey
    (DXRBS), of archived, pointed ROSAT Position Sensitive Proportional
    Counter data for blazars by correlating the ROSAT WGACAT database with
    several publicly available radio catalogs, restricting our candidate
    list to serendipitous flat radio spectrum sources ({alpha}_r_&lt;=0.70,
    where S_{nu}_{prop}{nu}^-{alpha}_r_^). We discuss our survey methods,
    identification procedure, and first results. Our survey is found to be
    95% efficient at finding flat-spectrum radio-loud quasars (FSRQs; 59
    of our first 85 identifications) and BL Lacertae objects (22 of our
    first 85 identifications), a figure that is comparable to or greater
    than that achieved by other radio and X-ray survey techniques. The
    identifications presented here show that all previous samples of
    blazars (even when taken together) did not representatively survey the
    blazar population, missing critical regions of (LX, LR) parameter
    space within which large fractions of the blazar population lie.
    Particularly important is the identification of a large population of
    FSRQs (>=25% of DXRBS FSRQs) with ratios of X-ray to radio luminosity
    >=10^-6^({alpha}_rx_&lt;=0.78). In addition, as a result of our greater
    sensitivity, the DXRBS has already more than doubled the number of
    FSRQs in complete samples with 5GHz (radio) luminosities between
    10^31.5^ and 10^33.5^ergs/s/Hz, and fills in the region of parameter space
    between X-ray-selected and radio-selected samples of BL Lac objects.
    The DXRBS is the very first sample to contain statistically
    significant numbers of blazars at low luminosities, approaching what
    should be the lower end of the FSRQ luminosity function.</para></abstract>
                        <details><para><observatory base="space"> ROSAT</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3.dat">
	<title>Positional information</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>1WGA</name>
			<definition>WGACAT name</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>WGACAT right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>WGACAT right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>WGACAT right ascension (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>WGACAT declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>WGACAT declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>WGACAT declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>WGACAT declination (J2000)</definition>
			<units>arcsec</units></field>
		<field>
			<name>oWGA</name>
			<definition>Offset from field center in X-ray</definition>
			<units>arcsec</units></field>
		<field>
			<name>eWGA</name>
			<definition>WGACAT error
	<footnote footnoteId="???"><para>number=1</para>
			<para>WGACAT positional error circles. This was done as follows:
    WGACAT was cross-correlated with the Hipparcos Input Catalogue (Cat.
    &lt;I/196>), and the offsets between the two databases were obtained for
    six bins of the distance from the WGACAT field center (0'-10',
    10'-20', etc.). These values range from 13" (for the inner 10' of the
    PSPC field) to 53" (for the 50'-60' ring).</para></footnote></definition>
			<units>arcsec</units></field>
		<field>
			<name>RA1h</name>
			<definition>PMN or GB6 right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RA1m</name>
			<definition>PMN or GB6 right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RA1s</name>
			<definition>PMN or GB6 right ascension (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DE1-</name>
			<definition>PMN or GB6 declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DE1d</name>
			<definition>PMN or GB6 declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DE1m</name>
			<definition>PMN or GB6 declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DE1s</name>
			<definition>PMN or GB6 declination (J2000)</definition>
			<units>arcsec</units></field>
		<field>
			<name>RA2h</name>
			<definition>Optical Counterpart right ascension (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RA2m</name>
			<definition>Optical Counterpart right ascension (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RA2s</name>
			<definition>Optical Counterpart right ascension (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DE2-</name>
			<definition>Optical Counterpart declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DE2d</name>
			<definition>Optical Counterpart declination (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DE2m</name>
			<definition>Optical Counterpart declination (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DE2s</name>
			<definition>Optical Counterpart declination (J2000)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Source</name>
			<definition>Source
	<footnote footnoteId="???"><para>number=2</para>
			<para>Source codes are:
     APM: APM survey
     GB6: Green Bank 6cm catalog, Cat. &lt;VIII/40>
     PMN: Parkes-MIT-NRAO catalog, Cat. &lt;VIII/27>
    ATCA: Austalian Telescope Compact Array, this paper
    NVSS: NRAO VLA Sky Survey, Condon et al., 1998AJ....115.1693C
   FIRST: FIRST project, Gregg et al., 1996AJ....112..407G;
          Laurent-Muehleisen et al., 1998, in prep. (see &lt;VIII/51>)
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Offset</name>
			<definition>Absolute offset (X-O) value</definition>
			<units>arcsec</units></field>
		<field>
			<name>eCount</name>
			<definition>Counterpart error</definition>
			<units>arcsec</units></field>
		<field>
			<name>Error</name>
			<definition>Cumulative error</definition>
			<units>arcsec</units></field>
		<field>
			<name>Offset/Error</name>
			<definition>Ratio of Offset to Error</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4.dat">
	<title>Newly identified objects</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>1WGA</name>
			<definition>WGACAT name</definition>
			<units>---</units></field>
		<field>
			<name>Crate</name>
			<definition>ROSAT count rate</definition>
			<units>ct/s</units></field>
		<field>
			<name>F(0.1-2.0)</name>
			<definition>0.1-2.0keV flux</definition>
			<units>mW/m2</units></field>
		<field>
			<name>F1keV</name>
			<definition>Flux density at 1keV</definition>
			<units>uJy</units></field>
		<field>
			<name>log(FX/FR)</name>
			<definition>X-flux to radio-flux ratio</definition>
			<units>---</units></field>
		<field>
			<name>F6cm</name>
			<definition>Flux density at 6cm</definition>
			<units>mJy</units></field>
		<field>
			<name>SI</name>
			<definition>Radio spectral index</definition>
			<units>---</units></field>
		<field>
			<name>l_Bmag</name>
			<definition>Limit flag on Bmag</definition>
			<units>---</units></field>
		<field>
			<name>Bmag</name>
			<definition>B magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>l_Rmag</name>
			<definition>Limit flag on Rmag</definition>
			<units>---</units></field>
		<field>
			<name>Rmag</name>
			<definition>R magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Class</name>
			<definition>Classification
	<footnote footnoteId="???"><para>number=1</para>
			<para>Classification is:
      RG: radio galaxy
    FSRQ: flat-spectrum radio-loud quasar
    SSRQ: steep-spectrum radio-loud quasar
  BL Lac: BL Lac object</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>z</name>
			<definition>Redsifht</definition>
			<units>---</units></field>
		<field>
			<name>u_z</name>
			<definition>Uncertainty flag on z</definition>
			<units>---</units></field>
		<field>
			<name>Cat</name>
			<definition>Other catalogs
	<footnote footnoteId="???"><para>number=2</para>
			<para>Other catalogs are numbered:
       1: RASS Bright Source Catalog, Cat. &lt;IX/10>
       2: HBQS, Homogeneous Bright QSO Survey, Cat. &lt;J/A+AS/112/347>
       3: V Zwicky Catalog of Galaxies, Cat. &lt;VII/190>
       4: 4C, Fourth Cambridge Survey, Cat. &lt;VIII/4>
       5: Einstein Slew Survey, Elvis et al., 1992ApJS...80..257E
       6: FIRST Bright Quasar Survey, See Cat. &lt;VIII/51>
       7: B3, Third Bologna Survey, Cat. &lt;VIII/37>
       8: Las Campanas Redshift Survey, Cat. &lt;VII/203>
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table6.dat">
	<title>Previously identified blazars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>Crate</name>
			<definition>ROSAT count rate</definition>
			<units>ct/s</units></field>
		<field>
			<name>F(0.1-2.0)</name>
			<definition>0.1-2.0keV flux</definition>
			<units>mW/m2</units></field>
		<field>
			<name>F1keV</name>
			<definition>Flux density at 1keV</definition>
			<units>uJy</units></field>
		<field>
			<name>log(FX/FR)</name>
			<definition>X-flux to radio-flux ratio</definition>
			<units>---</units></field>
		<field>
			<name>F6cm</name>
			<definition>Flux density at 6cm</definition>
			<units>mJy</units></field>
		<field>
			<name>SI</name>
			<definition>Radio spectral index</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Class</name>
			<definition>Classification
	<footnote footnoteId="???"><para>number=1</para>
			<para>Classification is:
      RG: radio galaxy
    FSRQ: flat-spectrum radio-loud quasar
  BL Lac: BL Lac object
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_z</name>
			<definition>Limit flag on z</definition>
			<units>---</units></field>
		<field>
			<name>z</name>
			<definition>Redsifht</definition>
			<units>---</units></field>
		<field>
			<name>u_z</name>
			<definition>Uncertainty flag on z</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="notes.dat">
	<title>Individual notes</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>1WGA</name>
			<definition>WGACAT name (repeated of more than 1 line)</definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>Text of the note</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1998</year><month>Aug</month><day>11</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> From AJ electronic version</para></revision></revisions></history>
	<identifier>J_AJ_115_1253.xml</identifier></dataset>
