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J/AJ/115/1253       Deep X-Ray Radio Blazar Survey (DXRBS). I. (Perlman+ 1998)
================================================================================
The deep X-ray radio blazar survey. I. Methods and first results.
       Perlman E.S., Padovani P., Giommi P., Sambruna R., Jones L.R.,
       Tzioumis A., Reynolds J.
      <Astron. J. 115, 1253 (1998)>
      =1998AJ....115.1253P      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: QSOs ; BL Lac objects ; Surveys ; X-ray sources ; Radio sources
Mission_Name: ROSAT
Keywords: BL Lacertae objects: general - quasars: general - radio continuum -
          surveys

Abstract:
    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_<=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_<=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.

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table3.dat        116      102   Positional information
table4.dat         90      102   Newly identified objects
table6.dat         76       97   Previously identified blazars
notes.dat          80      182   Individual notes
--------------------------------------------------------------------------------

See also:
   IX/12 : The WGACAT version of ROSAT sources (White+ 1995)
 VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)
 VIII/40 : GB6 catalog of radio sources at 4.85GHz (Gregory+ 1996)
 VIII/15 : Parkes Radio Sources Catalogue (PKSCAT90) (Wright+ 1990)

Byte-by-byte Description of file: table3.dat
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   Bytes Format Units      Label    Explanations
--------------------------------------------------------------------------------
   1- 16  A16   ---        1WGA      WGACAT name
  18- 19  I2    h          RAh       WGACAT right ascension (J2000)
  21- 22  I2    min        RAm       WGACAT right ascension (J2000)
  24- 27  F4.1  s          RAs       WGACAT right ascension (J2000)
      29  A1    ---        DE-       WGACAT declination sign
  30- 31  I2    deg        DEd       WGACAT declination (J2000)
  33- 34  I2    arcmin     DEm       WGACAT declination (J2000)
  36- 37  I2    arcsec     DEs       WGACAT declination (J2000)
  39- 42  F4.1  arcsec    oWGA       Offset from field center in X-ray
  44- 45  I2    arcsec    eWGA       WGACAT error (1)
  47- 48  I2    h          RA1h      PMN or GB6 right ascension (J2000)
  50- 51  I2    min        RA1m      PMN or GB6 right ascension (J2000)
  53- 56  F4.1  s          RA1s      PMN or GB6 right ascension (J2000)
      58  A1    ---        DE1-      PMN or GB6 declination sign
  59- 60  I2    deg        DE1d      PMN or GB6 declination (J2000)
  62- 63  I2    arcmin     DE1m      PMN or GB6 declination (J2000)
  65- 66  I2    arcsec     DE1s      PMN or GB6 declination (J2000)
  68- 69  I2    h          RA2h      Optical Counterpart right ascension (J2000)
  71- 72  I2    min        RA2m      Optical Counterpart right ascension (J2000)
  74- 77  F4.1  s          RA2s      Optical Counterpart right ascension (J2000)
      79  A1    ---        DE2-      Optical Counterpart declination sign
  80- 81  I2    deg        DE2d      Optical Counterpart declination (J2000)
  83- 84  I2    arcmin     DE2m      Optical Counterpart declination (J2000)
  86- 87  I2    arcsec     DE2s      Optical Counterpart declination (J2000)
  89- 96  A8    ---        Source    Source (2)
  98-102  F5.2  arcsec     Offset    Absolute offset (X-O) value
 104-105  I2    arcsec    eCount     Counterpart error
 107-111  F5.2  arcsec     Error     Cumulative error
 113-116  F4.2  ---     Offset/Error Ratio of Offset to Error
--------------------------------------------------------------------------------
Note (1): WGACAT positional error circles. This was done as follows:
    WGACAT was cross-correlated with the Hipparcos Input Catalogue (Cat.
    <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).

Note (2): Source codes are:
     APM: APM survey
     GB6: Green Bank 6cm catalog, Cat. <VIII/40>
     PMN: Parkes-MIT-NRAO catalog, Cat. <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 <VIII/51>)
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table4.dat
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   Bytes Format Units   Label       Explanations
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   1- 16  A16   ---     1WGA        WGACAT name
  18- 22  F5.3  ct/s    Crate       ROSAT count rate
  24- 31  E8.2  mW/m2   F(0.1-2.0)  0.1-2.0keV flux
  33- 37  F5.3  uJy     F1keV       Flux density at 1keV
  39- 44  F6.2  ---     log(FX/FR)  ? X-flux to radio-flux ratio
  46- 49  I4    mJy     F6cm        ? Flux density at 6cm
  51- 55  F5.2  ---     SI          ? Radio spectral index
      57  A1    ---   l_Bmag        Limit flag on Bmag
  58- 61  F4.1  mag     Bmag        ? B magnitude
      63  A1    ---   l_Rmag        Limit flag on Rmag
  64- 67  F4.1  mag     Rmag        ? R magnitude
  69- 75  A7    ---     Class       Classification (1)
  77- 81  F5.3  ---     z           ? Redsifht
      82  A1    ---   u_z           [?] Uncertainty flag on z
  84- 86  A3    ---     Cat         Other catalogs (2)
--------------------------------------------------------------------------------
Note (1):  Classification is:
      RG: radio galaxy
    FSRQ: flat-spectrum radio-loud quasar
    SSRQ: steep-spectrum radio-loud quasar
  BL Lac: BL Lac object
Note (2): Other catalogs are numbered:
       1: RASS Bright Source Catalog, Cat. <IX/10>
       2: HBQS, Homogeneous Bright QSO Survey, Cat. <J/A+AS/112/347>
       3: V Zwicky Catalog of Galaxies, Cat. <VII/190>
       4: 4C, Fourth Cambridge Survey, Cat. <VIII/4>
       5: Einstein Slew Survey, Elvis et al., 1992ApJS...80..257E
       6: FIRST Bright Quasar Survey, See Cat. <VIII/51>
       7: B3, Third Bologna Survey, Cat. <VIII/37>
       8: Las Campanas Redshift Survey, Cat. <VII/203>
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Byte-by-byte Description of file: table6.dat
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   Bytes Format Units   Label       Explanations
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   1- 15  A15   ---     Name        Source name
  17- 21  F5.3  ct/s    Crate       ROSAT count rate
  23- 30  E8.2  mW/m2   F(0.1-2.0)  0.1-2.0keV flux
  32- 37  F6.3  uJy     F1keV       Flux density at 1keV
  39- 44  F6.2  ---     log(FX/FR)  X-flux to radio-flux ratio
  46- 50  I5    mJy     F6cm        Flux density at 6cm
  52- 56  F5.2  ---     SI          Radio spectral index
  58- 61  F4.1  mag     Vmag        ? V magnitude
  63- 68  A6    ---     Class       Classification (1)
      70  A1    ---   l_z           Limit flag on z
  71- 75  F5.3  ---     z           ? Redsifht
      76  A1    ---   u_z           [?] Uncertainty flag on z
--------------------------------------------------------------------------------
Note (1): Classification is:
      RG: radio galaxy
    FSRQ: flat-spectrum radio-loud quasar
  BL Lac: BL Lac object
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Byte-by-byte Description of file: notes.dat
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   Bytes Format Units   Label     Explanations
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   1- 16  A16   ---     1WGA      WGACAT name (repeated of more than 1 line)
  18- 80  A63   ---     Note      Text of the note
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History: From AJ electronic version
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(End)                                          Patricia Bauer [CDS]  11-Aug-1998

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