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/journal_tables/AJ/99/1071/

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J/AJ/99/1071        1.4 GHz source survey            (Condon+ 1990)
================================================================================
A 1.4 GHz source survey in an area without nearby rich galaxy clusters
       Condon J.J., Dickey J.M., Salpeter E.E.
      <Astron. J. 99, 1071 (1990)>
      =1990AJ.....99.1071C      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Radio sources ; Galaxies, radio

Abstract:
    We report on 1.4GHz continuum observations for 56 contiguous VLA
    fields, using the D configuration, in a region devoid of nearby, rich
    galaxy clusters (at z<0.4). 354 continuum sources are tabulated, with
    fluxes down to about 1.5mJy, in an area of about 12degres^+2^. Only
    about seven of the 354 radio sources are associated with known rich
    galaxy clusters at z>0.4 (tabulated by Gunn, Hoessel, and Oke,
    1986ApJ...306...30G). We compare source positions with those from an
    optical catalog (generated from a POSS plate with the use of the
    Minnesota Automated Plate Scanner) and find mild correlations on
    angular scales of order 1arcmin. This suggests some association of
    radio sources with galaxy groups (sizes of order 200 kpc) at redshifts
    of order z~0.1, even though there are no rich galaxy clusters in this
    redshift range.

File Summary:
--------------------------------------------------------------------------------
  FileName        Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table1.dat         35       56   Center of fields and sensitivity of VLA fields
table2.dat         57      354   Radio sources detected by the VLA.
table3.dat         48      130   Large optical galaxies from POSS plates
table4.dat         64       58   Optical objects coincident with radio sources
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table1.dat
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  Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---     Field    Field number
   6-  7  I2    h       RAh      Right Ascension B1950 of field center (hours)
   8-  9  I2    min     RAm      Right Ascension B1950 of field center (minutes)
  10- 11  I2    s       RAs      [0,60] Right Ascension B1950          (seconds)
      12  A1    ---     DE-      Declination B1950 of field center (sign)
  13- 14  I2    deg     DEd      Declination B1950 of field center (degrees)
  15- 16  I2    arcmin  DEm      Declination B1950 of field center (minutes)
  20- 23  F4.2  mJy     Srms     RMS noise flux density
  26- 29  F4.2  mJy     Sneg     ? Flux level for "negative" detections
  32- 35  F4.2  mJy     Smin     Minimum flux level adopted for detection
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  4  A4    ---     Source    Source name
       5  A1    ---   n_Source    ['?] Note on Source (1)
   7-  9  I3    ---     Field     Field whose center is closest to the source
      10  A1    ---   n_Field     [*] Note on Field (2)
      12  I1    h       RAh       Right ascension (1950)
  14- 15  I2    min     RAm       Right ascension (1950)
  17- 20  F4.1  s       RAs       Right ascension (1950)
      21  A1    ---     DE-       Declination sign
  22- 23  I2    deg     DEd       Declination (1950)
  25- 26  I2    arcmin  DEm       Declination (1950)
  28- 29  I2    arcsec  DEs       [0,60] Declination (1950)
  31- 35  F5.1  mJy     Smax      Peak flux at 1.4GHz
  37- 41  F5.1  mJy     Sint      Area integrated flux at 1.4GHz
  43- 46  F4.2  ---     PBC       Primary-beam correction factor (3)
--------------------------------------------------------------------------------
Note (1): ? : slightly suspect detections
          ' : Smax < 2(PBC)Smin
Note (2): * : the source is fairly close to the center of a second field
Note (3): PBC(t)=exp[10.7t^2^ + 25.3t^4^] where t is the distance from the
           source to the field center in degrees.
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---     Gno       Galaxy source Number
   6-  7  I2    h       RAh       Right Ascension B1950 (hours)
   8-  9  I2    min     RAm       Right Ascension B1950 (minutes)
  10- 13  F4.1  s       RAs       Right Ascension B1950 (seconds)
      14  A1    ---     DE-       Declination B1950 (sign)
  15- 16  I2    deg     DEd       Declination B1950 (degrees)
  17- 18  I2    arcmin  DEm       Declination B1950 (minutes)
  19- 20  I2    arcsec  DEs       [0,60] Declination B1950 (seconds)
  24- 26  I3    um      R65%diam  Diameter on red plate at level 65%  (1)
  29- 31  I3    um      R30%diam  Diameter on red plate at level 30%  (1)
  35- 37  I3    um      B65%diam  Diameter on blue plate at level 65% (1)
  40- 42  I3    um      B30%diam  Diameter on blue plate at level 30% (1)
  45- 48  F4.1  mag     mZw       ? Zwicky magnitude of galaxy
--------------------------------------------------------------------------------
Note (1): the levels are defined from the transmission density.
     Diameters are in microns (1um = 0.067") from the POSS plates 1st epoch
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table4.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  4  A4    ---     Source    Source name, as in table2
       5  A1    ---   u_Source    [?] Uncertainty flag
       7  A1    ---     Otype     [Gf] optical Galaxy or faint object  (1)
  10- 14  F5.2  mJy     Smax      Peak flux at 1.4GHz
  16- 17  I2    h       RAh       Right Ascension B1950 (hours)
  18- 19  I2    min     RAm       Right Ascension B1950 (minutes)
  20- 23  F4.1  s       RAs       Right Ascension B1950 (seconds)
      24  A1    ---     DE-       Declination B1950 (sign)
  25- 26  I2    deg     DEd       Declination B1950 (degrees)
  27- 28  I2    arcmin  DEm       Declination B1950 (minutes)
  29- 30  I2    arcsec  DEs       [0,60] Declination B1950 (seconds)
  34- 36  I3    um      R65%diam  Diameter on red plate at level 65%  (2)
  39- 41  I3    um      R30%diam  Diameter on red plate at level 30%  (2)
  46- 48  I3    um      B65%diam  Diameter on blue plate at level 65% (2)
  51- 53  I3    um      B30%diam  Diameter on blue plate at level 30% (2)
  57- 58  I2    arcsec  Sep       Separation between optical and radio sources
  62- 64  I3    ---     Gno       ? Number in table3 (1)
--------------------------------------------------------------------------------
Note (1):
    'G' indicates a coincidence with a galaxy; when this galaxy was
        optically identified in table3, its number is listed in the
        last column. These coincidences are listed in table4a of the
        publication.
    'g' indicates a coincidence with an optical faint or unresolved
        objet, originally listed in table4b of the publication.
Note (2): the levels are defined from the transmission density.
     Diameters are in microns (1um = 0.067") from the POSS plates 1st epoch
--------------------------------------------------------------------------------

Acknowledgements:
     We thank Heinz Andernach for supplying the tables 1, 3 and 4.

History:
  * 14-Nov-1997: table2 prepared via OCR at CDS.
  * 14-Dec-1997: an error in R120 declination was detected by
         H. Andernach <heinz@polaris.astro.ugto.mx> and corrected.
  * 28-Oct-1998: tables 1,3,4 prepared by H. Andernach (catalogue
         numbered R187 in his list) were added.
  * 03-Nov-1998: an error in table3 (Gno 115 was labelled Gno 117) was
        detected by Fabienne Woelfel and corrected
================================================================================
(End)  Marie-Jose Wagner, Patricia Bauer, Francois Ochsenbein [CDS]  28-Oct-1998

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