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1995AZh....72...12M
1995ARep...39....9M
J/AZh/72/12    Spectroscopy of Sources from 87GB Catalog    (Mingaliev+, 1995)
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Spectra Study of a Sample of Radio Sources from the 87GB Catalog
     Mingaliev M., Khabrakhmanov A.
    
    =1995AZh....72...12M
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ADC_Keywords: Radio sources

Description:

A sample of 112 sources with flux densities higher than 200mJy at the 4.85GHz and with the range of declinations from +3 till +5 degrees from the Green Bank survey catalog 87GB was observed at three frequencies: 0.96, 3.95, and 11.1GHz. The observations were performed in January and February 1992, in the Northern sector of the RATAN-600 radio telescope. The accuracy of the source right ascensions was improved by a factor of 5-10 (for 70% of the sources the accuracy of the right ascension is 0.1arcsec). About 80% of the objects studied were identified with sources from the Texas survey.
File Summary:
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  FileName      Lrecl  Records   Explanations
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ReadMe             80        .   This file
table             114      112   Radio spectra of a sample of 112 sources
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See also:
    VIII/14 : 87GB Catalog of radio sources (Gregory et al., 1991)
    VIII/42 : Texas Survey of radio sources at 365MHz (Douglas+ 1996)

Byte-by-byte Description of file: table
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   Bytes Format  Units   Label    Explanations
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   1-  2  I2     h       RAh      Right ascension (1950) from 87GB
   4-  5  I2     min     RAm      Right ascension (1950) from 87GB
   7- 10  F4.1   s       RAs      Right ascension (1950) from 87GB
      13  A1     ---     DE-      Declination sign
      14  I1     deg     DEd      Declination (1950) from 87GB
  16- 17  I2     arcmin  DEm      Declination (1950) from 87GB
  19- 20  I2     arcsec  DEs      Declination (1950) from 87GB
  23- 24  I2     h       RARh     ? Right ascension (1950) (RATAN-600)
  26- 27  I2     min     RARm     ? Right ascension (1950) (RATAN-600)
  29- 33  F5.2   s       RARs     ? Right ascension (1950) (RATAN-600)
  36- 39  F4.2   s       e_RARs   ? Uncertainty in Right ascension (1950)
  41- 44  I4     Jy      Flux2.7  ? Flux density in the 2.7cm (11.1GHz)
      46  A1     --- l_e_Flux2.7  ? Limit symbol on relative uncertainty of
                                    flux densities in the 2.7cm
  47- 49  I3     Jy    e_Flux2.7  Relative uncertainty of flux densities
                                  in the 2.7cm
      51  A1     ---   l_Flux6.2  ? Limit symbol on flux density in the 6.2cm
  52- 55  I4     Jy      Flux6.2  Flux density in the 6.2cm (4,8GHz)
  58- 60  I3     Jy    e_Flux6.2  Relative uncertainty of flux densities
                                  in the 6.2cm
  63- 66  I4     Jy      Flux7.6  ? Flux density in the 7.6cm (3.9GHz)
  69- 70  I2     Jy    e_Flux7.6  ? Relative uncertainty of flux densities
                                    in the 7.6cm
  73- 76  I4     Jy      Flux31   ? Flux density in the 31cm (970MHz)
      79  A1     --- l_e_Flux31   ? Limit symbol on relative uncertainty of
                                     flux densities in the 31cm
  80- 82  I3     Jy    e_Flux31   ? Relative uncertainty of flux densities
                                     in the 31cm
  84- 88  I5     Jy      Flux82   ? Flux density in the 82cm (370MHz)
  90- 92  I3     Jy    e_Flux82   ? Relative uncertainty of flux densities
                                     in the 82cm
  94- 98  F5.2   ---     alpha1   ? Spectral index from 14P and 15P
 101-105  F5.2   ---     alpha2   ? Spectral index from 14P and 15P
 107-109  A3     ---     Rem      * Remarks
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Note on Rem:
    # = The spectral indices were determined from flux densities at 7.6 and 31cm
         (in the absence of identification with the Texas survey)
    * = the source is from the Sternberg Astronomical Institute survey list
   ** = the source is identified with the adjacent lobe
  *** = the source signal was not distinguished because of interference from a
         nearby background source. The flux densities at 6.2 and 82cm from
         the Green Bank and Texas surveys.
  ref = a reference object
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(End)                           Veta Avedisova [INASAN]              10-May-1997