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J/A+A/285/812   Spectral properties of X-ray extragal. sources (Brinkmann+ 1994)

Spectral properties of X-ray loud extragalactic radio sources BRINKMANN W., SIEBERT J. <Astron. Astrophys. 285, 812 (1994)> =1994A&A...285..812B
ADC_Keywords: Galaxies, UV-excess; Radio sources; X-ray sources Keywords: galaxies: active - quasars - BL Lac objects: X-rays - galaxies - radio continuum: galaxies File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 144 68 Spectral properties of X-ray loud extragalactic radio sources
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
2- 15 A14 --- ROSAT ROSAT name (position J2000.0) 17- 32 A16 --- Name Other name of the source 34- 36 A3 --- Type Optical identification given in the NED 39- 42 F4.2 --- Gamma X-ray spectral index 44- 47 F4.2 --- e_Gamma rms uncertainty on X-ray spectral index 51- 54 F4.2 10+21cm-2 N(H) Absorbing neutral hydrogen column density (best fit) 56- 59 F4.2 10+21cm-2 e_N(H) rms uncertainty on N(H) 62- 65 F4.2 --- chi2 Reduced chi2 for the fit (Errors are 1 sigma) 67- 68 I2 --- nu []? Degrees of freedom for chi2 71- 74 F4.2 --- GammaN(H)g X-ray spectral index for fixed galactic N(H) 76- 79 F4.2 --- e_GammaN(H)g rms uncertainty on GammaN(H)g 82- 85 F4.2 10+21cm-2 N(H)g Absorbing neutral hydrogen column density for fixed galactic N(H) 88- 91 F4.2 --- chi2(g) Reduced chi2 for the fit for fixed galactic N(H) (Errors are 1 sigma) 93- 94 I2 --- nu(g) []? Degrees of freedom for chi2(g) 97-102 F6.2 10-11mW/m2 fX Unabsorbed X-ray flux in the total ROSAT energy band, computed by using the best fit values for Gamma and N(H) 104-109 F6.2 Jy frad Radio flux at 5 GHz (Green Bank sources) or 408 MHz (Molonglo sources) 112 A1 --- n_frad note (1) 115-144 A30 --- ref References
Note (1): c refer to the Gregory & Condon catalog m refer to the Molonglo catalog b denotes fluxes from a catalog created at MPIfR using the Green Bank data.

(End) Patricia Bauer [CDS] 23-Feb-1994
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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