J/other/AstBu/70.264    Sample of 877 blazars                (Mingaliev+, 2015)

A study of the synchrotron component in the blazar spectral energy distributions. Mingaliev M.G., Sotnikova Yu.V., Mufakharov T.V., Erkenov A.K., Udovitskiy R.Yu. <Astrophys. Bull., 70, 264 (2015)> =2015AstBu..70..264M 2015AstBu..70..264M
ADC_Keywords: Active gal. nuclei ; Galaxies, radio ; Radio continuum Keywords: galaxies: general - galaxies: active - radio continuum: galaxies Description: We study the synchrotron component of the spectral energy distribution on the sample of 877 blazars using ASDC SED Builder Tool with available broadband data from the literature. Our sample includes 423 flat-spectrum radio sources (FSRQs), 361 BL Lac objects and candidates, and 93 blazars of uncertain type. We have made an estimation of the synchrotron peak frequency for the 875 objects and further classified them as high, intermediate and low synchrotron peaked sources (HSPs/ISPs/LSPs). For each source NVSS name (RA (HHMMSS) and DEC (DDMMSS) for the J2000.0 epoch), alias, redshift, R band magnitude, synchrotron peak frequency, correlation coefficient, flux density at 4.8GHz, SED class, blazar type and selection method are presented. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table.dat 107 877 Data for 877 objects -------------------------------------------------------------------------------- See also: VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998) J/A+A/495/691 : Multifrequency catalogue of blazars, Roma-BZCAT (Massaro+ 2009) Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- NVSS NVSS Name (HHMMSS+DDMMSS, J2000) 16- 38 A23 --- OName Alias name 41- 45 F5.3 --- z [0/4.3] Redshift (from NED) 48- 51 F4.1 mag Rmag ? R band magnitude (2) 55- 59 F5.2 [Hz] lognup [11.8/18.9]? Logarithm of the synchrotron peak frequency logνp 62- 65 F4.2 --- k [0/1]? Correlation coefficient (1) 67- 72 F6.3 Jy S4.8 ? Radio flux density at 4.8GHz 74- 78 F5.3 Jy e_S4.8 ? Error of the flux density at 4.8GHz 82- 84 A3 --- Class Classification by SED type (4) 87-100 A14 --- Type Blazar type (2) 105-107 A3 --- Meth Classification by selection method (3) -------------------------------------------------------------------------------- Note (1): Correlation strength between observational data points in SED and polynomial approximation (from ASDC SED Builder Tool) Note (2): R band magnitude and blazar type according to the Roma-BZCAT catalogue 3d edition (2009A&A...495..691M 2009A&A...495..691M, Cat. J/A+A/495/691) Note (3): Blazar type as follows: RBL = radio-selected BL Lac XBL = X-ray-selected BL Lac OBL = optically-selected BL Lac Note (4): Classification as follows: HSP = high synchrotron peaked ISP = intermediate synchrotron peaked LSP = low synchrotron peaked ----------------------------------------------------------------------------- Acknowledgements: Yu. Sotnikova, sjv(at)sao.ru
(End) Yu. Sotnikova [SAO, Russia], Patricia Vannier [CDS] 30-Jul-2015
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