J/AZh/72/12 Spectroscopy of Sources from 87GB Catalog (Mingaliev+, 1995)
Spectroscopic Study of a Sample of Radio Sources from the 87GB Catalog
Mingaliev M., Khabrakhmanov A.
<Astron. Zh. 72, 12 (1995)>
=1995AZh....72...12M 1995AZh....72...12M
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 VIII/14 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 --- leFlux2.7 ? 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 --- leFlux31 ? 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