<?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>A statistical analysis of the broadband 0.1 to 3.5keV spectral properties of
X-ray-selected active galactic nuclei.</title>
	<altname type="ADC">J/ApJ/434/54</altname>
		<altname type="CDS">J/ApJ/434/54</altname>
		<altname type="brief">Spectral properties of X-ray-selected AGNs</altname>
	<reference>
		<source>
<journal>
	<title>A statistical analysis of the broadband 0.1 to 3.5keV spectral properties of
X-ray-selected active galactic nuclei.</title>
	<author>
			<initial>R</initial>
			<initial>J</initial>
			<lastName>Thompson</lastName></author>
	<author>
			<initial>F</initial>
			<initial>A</initial>
			<lastName>Cordova</lastName></author>
	<name>Astrophys. J.</name>
	<volume>434</volume>
	<pageno>54</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994ApJ...434...54T</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Active_gal._nuclei.html">Active gal. nuclei</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="galaxies_active.html">galaxies: active</keyword>
			<keyword xlink:href="X-rays_galaxies.html">X-rays: galaxies</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We survey the broadband spectral properties of ~500 X-ray-selected
    active galactic nuclei (AGNs) observed with the Einstein Observatory.
    Included in this survey are the ~450 AGNs in the Extended Medium
    Sensitivity Survey of Gioia et al. (1990ApJS...72..567G) and the ~50
    AGNs in the Ultrasoft Survey of Cordova et al. (1992ApJS...81..661C).
    We present a revised version of the latter sample, based on the post
    publication discovery of a software error in the Einstein Rev-1b
    processing. We find that the mean spectral index of the AGNs between
    0.1 and 0.6keV is softer, and the distribution of indices wider, than
    previous estimates based on analyses of the X-ray spectra of optically
    selected AGNs. A subset of these AGNs exhibit flux variability, some
    on timescales as short as 0.05-days. A correlation between radio and
    hard X-ray luminosity is confirmed, but the data do not support a
    correlation between the radio and soft X-ray luminosities, or between
    radio loudness and soft X-ray spectral slope. Evidence for physically
    distinct soft and hard X-ray components is found, along with the
    possibility of a bias in previous optically selected samples toward
    selection of AGNs with flatter X-ray spectra.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1a">
	<title>Revised Ultrasoft Survey (RUSS) Sources</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name</definition>
			<units>---</units></field>
		<field>
			<name>n_Seq</name>
			<definition>Note
	<footnote footnoteId="???"><para>number=1</para>
			<para>*: source that satisfy our criteria for being "truly" soft, i.e.
              being free from shadowing by the detector support ribs and having
              good counting statistics (R1 +1{sigma}&lt;0.6)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Seq</name>
			<definition>IPC sequence</definition>
			<units>---</units></field>
		<field>
			<name>SRC</name>
			<definition>Source number</definition>
			<units>---</units></field>
		<field>
			<name>RAXh</name>
			<definition>X-ray right ascension (1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAXm</name>
			<definition>X-ray right ascension (1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAXs</name>
			<definition>X-ray right ascension (1950)</definition>
			<units>s</units></field>
		<field>
			<name>DEX-</name>
			<definition>X-ray declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEXd</name>
			<definition>X-ray declination (1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEXm</name>
			<definition>X-ray declination (1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEXs</name>
			<definition>X-ray declination (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>RAh</name>
			<definition>Optical right ascension (1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Optical right ascension (1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Optical right ascension (1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Optical declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Optical declination (1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Optical declination (1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Optical declination (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>z</name>
			<definition>Redshift</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>NH</name>
			<definition>Hydrogen column density</definition>
			<units>10+20cm-2</units></field>
		<field>
			<name>RECO</name>
			<definition>IPC RECO value
	<footnote footnoteId="???"><para>number=2</para>
			<para>Measure of the amount of shadowing by the detector support ribs,
           Harnden et al., 1984, Smithsonian Astrophys. Obs. Spec. Rep. No. 393
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Dits</name>
			<definition>Off-axis distance</definition>
			<units>arcmin</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1b">
	<title>RUSS X-Ray data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name, as in table1a</definition>
			<units>---</units></field>
		<field>
			<name>R1</name>
			<definition>Counts in colour ratio R1</definition>
			<units>---</units></field>
		<field>
			<name>e_R1</name>
			<definition>rms uncertainty on R1</definition>
			<units>---</units></field>
		<field>
			<name>R2</name>
			<definition>Counts in colour ratio R2 (C3/C2)</definition>
			<units>---</units></field>
		<field>
			<name>e_R2</name>
			<definition>rms uncertainty on R2</definition>
			<units>---</units></field>
		<field>
			<name>C1</name>
			<definition>Counts ratio at the energy band C1=0.16-0.56keV</definition>
			<units>---</units></field>
		<field>
			<name>e_C1</name>
			<definition>rms uncertainty on C1</definition>
			<units>---</units></field>
		<field>
			<name>C2</name>
			<definition>Counts ratio at the energy band C2=0.56-1.08keV</definition>
			<units>---</units></field>
		<field>
			<name>e_C2</name>
			<definition>rms uncertainty on C2</definition>
			<units>---</units></field>
		<field>
			<name>C3</name>
			<definition>Counts ratio at the energy band C3=1.08-3.5keV</definition>
			<units>---</units></field>
		<field>
			<name>e_C3</name>
			<definition>rms uncertainty on C3</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1c">
	<title>RUSS X-ray luminosities</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name, as in table1a</definition>
			<units>---</units></field>
		<field>
			<name>IPC</name>
			<definition>IPC counts</definition>
			<units>ct/s</units></field>
		<field>
			<name>e_IPC</name>
			<definition>rms uncertainty on IPC</definition>
			<units>ct/s</units></field>
		<field>
			<name>L1s</name>
			<definition>Soft-component luminosity for the 10eV
                                     rest-frame model</definition>
			<units>solLum</units></field>
		<field>
			<name>L2s</name>
			<definition>Soft-component luminosity for the 7.85eV
                                     observed-frame model</definition>
			<units>solLum</units></field>
		<field>
			<name>l_Lh</name>
			<definition>Limit flag on Lh</definition>
			<units>---</units></field>
		<field>
			<name>Lh</name>
			<definition>Hard-component luminosity from the
                                     observer-frame model</definition>
			<units>solLum</units></field>
		<field>
			<name>L0.2keV</name>
			<definition>Monochromatic 0.2keV luminosity</definition>
			<units>solLum</units></field>
		<field>
			<name>l_L2.0keV</name>
			<definition>Limit flag on L2.0keV</definition>
			<units>---</units></field>
		<field>
			<name>L2.0keV</name>
			<definition>Monochromatic 2.0keV luminosity</definition>
			<units>solLum</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout,   Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>Jun</month><day>06</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Prepared via OCR at CDS.</para></revision></revisions></history>
	<identifier>J_ApJ_434_54.xml</identifier></dataset>
