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RATAN-600 NCP bright radio sources

RATAN-600 NCP bright radio sources

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2001A&A...370...78Mingaliev+
J/A+A/370/78        RATAN-600 NCP bright radio sources       (Mingaliev+, 2001)
================================================================================
Observations of the bright radio sources in the North Celestial Pole region
at the RATAN-600 radio telescope.
    Mingaliev M.G., Stolyarov V.A., Davies R.D., Melhuish S.J., Bursov N.A.,
    Zhekanis G.V.
   
   =2001A&A...370...78M
================================================================================
ADC_Keywords: Galaxies, radio ; Radio sources

Keywords: radio astronomy - radio continuum - galaxies


Abstract:
    A survey of the North Celestial Pole region using the RATAN-600 radio
    telescope at five frequencies in the range 2.3 to 21.7 GHz is
    described. Sources were chosen from the NVSS catalogue. The flux
    densities of 171 sources in the Declination range +75deg +88deg
    are presented; typical flux density errors are 5-10 percent including
    calibration errors. About 20 percent of the sources have flat spectra
    or a flat component.

File Summary:

       FileName      Lrecl  Records   Explanations

? ReadMe            80        .   This file
? table3.dat        29       17   Complex sources list
? table4.dat       106      171   Fluxes of the sources in the NCP region


See also:
     VIII/33     : Spectral characteristics of RATAN (RC) Catalog (Bursov+ 1989)
 J/A+AS/87/1     : RATAN-600 7.6 cm catalog of radio sources (Parijskij+ 1991)
 J/AZh/74/42     : RATAN-600 radio sources spectra (Bursov 1997)
  : RATAN-600 radio sources spectra (Bursov 1996)
    : RATAN-600 RC radio sources (Parijskij+ 1996)


Byte-by-byte Description of file:  table3.dat

   Bytes Format Units   Label     Explanations

   1- 14  A14   ---     NVSS      Name in NVSS
  16- 29  A14   ---     Source    Name in the Table 4


Byte-by-byte Description of file:  table4.dat

   Bytes Format Units   Label     Explanations

   1- 14  A14   ---     Source    Source name  (NVSS notation), corresponding to
				   epoch J2000 coordinates (1)
  16- 21  F6.3  Jy     S0.325GHz  ? Flux density at 0.325GHz (WENSS catalog,
				     Rengelink et al., 1997, Cat. VIII/62)
  23- 27  F5.3  Jy   e_S0.325GHz  ? rms uncertainty on S0.325GHz
  29- 34  F6.3  Jy      S1.4GHz   NVSS Flux density at 1.4GHz (NVSS catalogue,
				   Condon et al., 1998, Cat. VIII/65)
  36- 40  F5.3  Jy     e_S1.4GHz  rms uncertainty on S1.4GHz
  42- 46  F5.3  Jy      S2.3GHz   ? Flux density at 2.3GHz
  48- 52  F5.3  Jy     e_S2.3GHz  ? rms uncertainty on S2.3GHz
  54- 58  F5.3  Jy      S3.9GHz   ? Flux density at 3.9GHz
  60- 64  F5.3  Jy     e_S3.9GHz  ? rms uncertainty on S3.9GHz
  66- 70  F5.3  Jy      S7.7GHz   ? Flux density at 7.7GHz
  72- 76  F5.3  Jy     e_S7.7GHz  ? rms uncertainty on S7.7GHz
  78- 82  F5.3  Jy      S11.2GHz  ? Flux density at 11.2GHz
  84- 88  F5.3  Jy    e_S11.2GHz  ? rms uncertainty on 11.2GHz
  90- 94  F5.3  Jy      S21.7GHz  ? Flux density at 21.7GHz
  96-100  F5.3  Jy    e_S21.7GHz  ? rms uncertainty 21.7GHz
 102-106  F5.2  ---     Sp-Index  Spectral index 0.325 to 11.2 (2)

Note (1): 7 complex sources, J0222XX+861XXX, J074XXX+802XXX, J101XXX+855XXX,
	   J184XXX+794XXX, J2042XX+750XXX, J2118XX+751XXX and J2355XX+795XXX
	   were not fully resolved in the RATAN-600 observations.
	   The list of the closely adjacent sources in the NVSS are in table 3.
Note (2): Spectral index ?=-log(S?1/S({nu2})/log(?1/{nu2}),
	   computed between fluxes at 0.325 and 11.2 GHz (or the nearest
	   available frequencies).


History:
    From electronic version of the journal
================================================================================
(End)                         James Marcout, Patricia Bauer [CDS]    10-Jul-2001


---------
| Table |
---------
name        WENSS_data       NVSS_data                 RATAN-600 data
	    (0.325 GHz)      (1.4 GHz)           (2.3  GHz)        (3.9  GHz)       (7.7  GHz)        (11.2  GHz)      (21.7  GHz)

	    Flux  eFlux     Flux  eFlux          Flux  eFlux      Flux  eFlux       Flux  eFlux       Flux   eFlux     Flux   eFlux
	     Jy     Jy       Jy    Jy             Jy     Jy        Jy    Jy          Jy     Jy          Jy    Jy        Jy    Jy