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J/A+A/330/108       ROSAT detected quasars. II. (Yuan+ 1998)
================================================================================
Broad band energy distribution of ROSAT detected quasars.
II. Radio-quiet objects
       Yuan W., Brinkmann W., Siebert J., Voges W.
      <Astron. Astrophys. 330, 108 (1998)>
      =1998A&A...330..108Y      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: QSOs ; X-ray sources
Keywords: galaxies: active - quasars - X-rays: galaxies
Mission_Name: ROSAT

Description:
    We have compiled a sample of all radio-quiet quasars or quasars
    without radio detection from the Veron-Cetty - Veron catalogue (1993,
    VV93, Cat. <VII/166>) detected by ROSAT in the ALL-SKY SURVEY (RASS,
    Voges 1992, in Proc. of the ISY Conference `Space Science', ESA ISY-3,
    ESA Publications, p.9, See Cat. <IX/10>), as targets of pointed
    observations, or as serendipitous sources from pointed observations
    publicly available from the ROSAT point source catalogue (ROSAT-SRC,
    Voges et al. 1995, Cat. <IX/11>). For all sources we used the results
    of the Standard Analysis Software System (SASS, Voges et al. 1992, in
    Proc. of the ISY Conference `Space Science', ESA ISY-3, ESA
    Publications, p.223), employing the most recent processing for the
    Survey data (RASS-II, Voges et al. 1996, Cat. <IX/10>). The total
    number of quasars is 846. 69 of the radio-quiet objects with radio
    detections have already been presented in a previous paper (Brinkmann,
    Yuan, & Siebert 1997, Cat. <J/A+A/319/413>) using the RASS-I results.
    17 objects were found to be radio-loud from recent radio surveys and
    were marked in the table. When available, the power law photon indices
    and the corresponding absorption column densities (NH) were estimated
    from the two hardness ratios given by the SASS, both with free fitted
    NH and for Galactic absorption. The unabsorbed X-ray flux densities in
    the ROSAT band (0.1-2.4keV) were calculated from the count rates using
    the energy to counts conversion factor for power law spectra and
    Galactic absorption. As the photon index we used the value obtained
    for the individual source if the estimated 1-{sigma} error is smaller
    than 0.5, otherwise we used the redshift-dependent mean value (see the
    paper for details).

File Summary:
--------------------------------------------------------------------------------
 FileName       Lrecl      Records      Explanations
--------------------------------------------------------------------------------
ReadMe          80            .         This file
table1         133          846         ROSAT detected radio-quiet quasars
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See also:
       VII/188 : Quasars and Active Galactic Nuclei (7th Ed.)  (Veron+ 1996)
         IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1996)
         IX/11 : ROSAT Source Catalog (Voges+ 1994)
 J/A+A/319/413 : ROSAT detected quasars. I. (Brinkmann+ 1997)

Byte-by-Byte Description of file: table1
--------------------------------------------------------------------------------
 Bytes  Format  Units       Label  Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---         IAU    IAU name of the object
      11  A1    ---       n_IAU   *[ *%?!] A flag for classification
  12- 29  A18   ---         VV93   Alternative name from VV93 (Cat. <VII/166>)
  31- 32  I2    h           RAh    Right Ascension J2000 (hours)
  34- 35  I2    min         RAm    Right Ascension J2000 (minutes)
  37- 40  F4.1  s           RAs    Right Ascension J2000 (seconds)
      42  A1    ---         DE-    Declination J2000 (Sign or blank)
  43- 44  I2    deg         DEd    Declination J2000 (degrees)
  46- 47  I2    arcmin      DEm    Declination J2000 (')
  49- 50  I2    arcsec      DEs    Declination J2000 (")
  52- 56  F5.3  ---         z     *? Redshift
  58- 62  F5.2  mag         Vmag  *? Magnitude from VV93 (Cat. <VII/166>)
  64- 69  F6.2 10-12mW/m2   FX     Unabsorbed X-ray flux density (0.1-2.4keV)
  71- 75  F5.2 10-12mW/m2 e_FX    *Error of X-ray flux density
  77- 80  F4.2  ---         Gfree *? X-ray photon index (free fitted NH)
  82- 85  F4.2  ---       E_Gfree *? Positive error of photon index Gfree
  87- 90  F4.2  ---       e_Gfree *? Negative error of photon index Gfree
  92- 96  F5.1  10+20cm-2   NH     ? X-ray absorbing column density
  98-101  F4.1  10+20cm-2 E_NH    *? Positive error of column density
 103-106  F4.1  10+20cm-2 e_NH    *? Negative error of column density
 108-111  F4.2  ---         Ggal  *? X-ray photon index (Galactic absorption)
 113-116  F4.2  ---       E_Ggal  *? Positive error of photon index Ggal
 118-121  F4.2  ---       e_Ggal  *? Negative error of photon index Ggal
 123-127  F5.2  10+20cm-2   NHgal *? Galactic column density
 129-130  A2    ---         Com   *[S P] Notes on the X-ray detection
 132-133  A2    ---         Ref   *? Reference for the quoted spectral index
--------------------------------------------------------------------------------
Note on n_IAU:
    *: object selected in other wave bands (X-ray, etc.) than in optical
    %: object found to be radio-loud in recent radio surveys (PMN, NVSS)
    ?: identification of the X-ray source is uncertain (see text)
    !: the X-ray flux might be contaminated by a nearby source
Note on z:
    A '0' as the 3rd decimal is mostly an artifact of the machine
    readable form of the catalogue. See the printed version of
    VV93 (Cat. VII/166>) for the appropriate values.
Note on Vmag:
    See the printed version of VV93 (Cat. VII/166>) for the appropriate values.
Note on e_FX::
    One {sigma} statistical errors from count rates only
Note on Gfree:
    Spectral photon index in the ROSAT energy band for a power law
    fit (S=C*E**(-Gamma)) with free fitted absorption
Note on E_Gfree, e_Gfree, E_NH, e_NH, E_Ggal and e_Ggal:
    One {sigma} errors. If no error is given, the value of the error
    is unphysically large.
Note on Ggal:
    Spectral photon index in the ROSAT energy band for a power law
    fit (S=C*E**(-Gamma)) with fixed Galactic absorption
Note on NHgal:
    Galactic column density from Dickey & Lockman (1990ARA&A..28..215D),
     see the paper.
Note on Com:
    S: detected in RASS; P: detected in pointed observations
Note on Ref:
    BJ: Bechtold J. et al., 1994AJ....108..374B
    LA: Laor A. et al., 1997ApJ...477...93L
    RD: Reimers D. et al., 1995A&A...296L..49R
    SN: Schartel N. et al., 1996, Cat. <J/A+A/307/33>
    UM: Ulrich M. et al., 1996ApJ...457...77U
    VC: Vignali C. et al., 1997MmSAI..68..141V
    WT: Wang T. et al., 1996, Cat. <J/A+A/309/81>
--------------------------------------------------------------------------------

Acknowledgements: Weimin Yuan <wey@rzg.mpg.de>
================================================================================
(End)                                          Patricia Bauer [CDS]  16-Dec-1997

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