J/MNRAS/298/637     7C: 151MHz survey of 3 regions           (Pooley+, 1998)
The 7C survey of radio sources at 151 MHz: three regions centred at
RA=10h05min, DE=53deg54', RA=10h42min, DE=57deg36' and RA=13h32min, DE=38deg10'
       Pooley D.M., Waldram E.M., Riley J.M.
      <Mon. Not. R. Astron. Soc. 298, 637 (1998)>
      =1998MNRAS.298..637P 1998MNRAS.298..637P
ADC_Keywords: Radio sources ; Surveys
Keywords: catalogues -  surveys - radio continuum: general
Abstract:
    The Cambridge Low Frequency Synthesis Telescope has been used at
    151MHz to survey three regions centred at RA=10h05min, DE=53°54',
    RA=10h42min, DE=57°36' and RA=13h32min, DE=38°10', each of
    area 7.3x7.3cosec(DE)deg2. The resolution is
    70x70cosec(DE)arcsec2, and the rms noise on the maps is typically
    15mJy/beam. We present positions and flux densities for 2381 sources
    which have signal-to-noise ratios >5.5.
File Summary:
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 FileName  Lrecl  Records     Explanations
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ReadMe        80        .     This file
100553.dat    74      743     7C sourcelist of 743 sources
104257.dat    74      757     7C sourcelist of 757 sources
133238.dat    74      881     7C sourcelist of 881 sources
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See also:
   VIII/84 : A final non-redundant catalogue for 7C 151-MHz survey (Hales+ 2007)
   J/A+AS/110/419 : 7C 151MHz survey of region RA=17h, DE=+65deg (Visser+, 1995)
  J/MNRAS/282/779 : 7C 151MHz survey of region 9-16h 20-35deg (Waldram+ 1996)
  J/MNRAS/294/607 : 7C(G) 151MHz survey of the Galactic plane (Vessey+ 1998)
Table 1: The RAxDec coverage, average rms noise, flux density of the faintest
          source listed and completeness limit for each region catalogued are
          given in the table below. All coordinates are equinox B1950.
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   Region    Coverage RA x DE  (see notes*)    av.rms noise  Sfaint    Scomp
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   1005+53   09h40m-10h30m;49deg05'-58deg20'   15mJy         50mJy     170mJy
   1042+57   10h10m-11h10m;53deg00'-61deg45'   13mJy         50mJy     150mJy
   1332+38   13h15m-13h50m;31deg40'-43deg45'   14mJy         50mJy     200mJy
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 *Note: RA coverage is indicated by approx RA range at DE of field centre
 *Note: DE coverage is indicated by approx DE range at RA of field centre
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Byte-by-byte Description of file: *.dat
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   Bytes   Format Units   Label  Explanations
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   1-  2   I2     h      RAh    Beam-fitted position right ascension (B1950) (1)
   4-  5   I2     min    RAm    Beam-fitted position right ascension (B1950)
   7- 10   F4.1   s      RAs    Beam-fitted position right ascension (B1950)
      12   A1     ---    DE-    Beam-fitted position declination sign (B1950)
  13- 14   I2     deg    DEd    Beam-fitted position declination (B1950)
  16- 17   I2     arcmin DEm    Beam-fitted position declination (B1950)
  19- 20   I2     arcsec DEs    Beam-fitted position declination (B1950)
  24- 25   I2     h      RACh   Centroid position right ascension (B1950)
  27- 28   I2     min    RACm   Centroid position right ascension (B1950)
  30- 33   F4.1   s      RACs   Centroid position right ascension (B1950)
      35   A1     ---    DEC-   Centroid position declination sign (B1950)
  36- 37   I2     deg    DECd   Centroid position declination (B1950)
  39- 40   I2     arcmin DECm   Centroid position declination (B1950)
  42- 43   I2     arcsec DECs   Centroid position declination (B1950)
  47- 52   F6.3   Jy     S      Beam-fitted 151MHz flux density (in Jy/beam) (2)
  54- 59   F6.3   Jy     Sint   Integrated 151MHz flux density (2)
  61- 65   F5.1   ---    SNR    Signal-to-noise ratio
  67- 70   F4.1   ---    Extent Extent of the source in units of local beam
                                   area
      74   I1     ---    Nmax   Number of local maxima within the integrated
                                   region
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Note (1): 1-sigma errors on the listed source positions may be approximated by:
             Right Ascension error(arcsec) = SQRT(1.0**2 + (32/SNR)**2)
             Declination error(arcsec) = 1.3cosec(DE) x (RA error)
Note (2): 1-sigma errors on the listed flux densities may be approximated by:
             Error on S beam-fitted(Jy)  =  SQRT(0.03**2 + SNR**-2) x S(Jy)
             Error on Sint(Jy) = 1.5 x SQRT(0.03**2 + SNR**-2) x Sint(Jy)
          For multi-component sources the SNR for the brightest component is
           used to estimate the Sint error.
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Acknowledgements: Sally Hales 
(End)                      Sally Hales [MRAO], Patricia Bauer [CDS]  13-Nov-1998