J/A+A/319/413       ROSAT detected quasars. I. (Brinkmann+ 1997)

Broad-band energy distribution of ROSAT detected quasars. I. Radio-loud objects. Brinkmann W., Yuan W., and Siebert J. <Astron. Astrophys. 319, 413 (1997)> =1997A&A...319..413B 1997A&A...319..413B (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; X-ray sources Mission_Name: ROSAT Keywords: galaxies: active - quasars: general - radio sources: galaxies - X-rays: galaxies Abstract: We have compiled a sample of all quasars with measured radio emission from the Veron-Cetty - Veron catalogue (1993, VV93 VII/166) detected by ROSAT in the ALL-SKY SURVEY (RASS, Voges 1992), as targets of pointed observations, or as serendipitous sources from pointed observations as publicly available from the ROSAT point source catalogue (ROSAT-SRC, Voges et al. 1995). The total number of ROSAT detected radio quasars from the above three sources is 654 objects. 69 of the objects are classified as radio-quiet using the defining line at a radio-loudness of 1.0, and 10 objects have no classification. The 5GHz data are from the 87GB radio survey, the NED database, or from the Veron-Cetty - Veron catalogue. The power law indices and their errors are estimated from the two hardness ratios given by the SASS assuming Galactic absorption. The X-ray flux densities in the ROSAT band (0.1-2.4keV) are calculated from the count rates using the energy to counts conversion factor for power law spectra and Galactic absorption. For the photon index we use the value obtained for a individual source if the estimated 1 sigma error is smaller than 0.5, otherwise we use the mean value 2.14. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1 109 654 654 ROSAT detected radio quasars -------------------------------------------------------------------------------- See also: VII/188 : Quasars and Active Galactic Nuclei (7th Ed.) (Veron+ 1996) IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1996) IX/11 : ROSAT Source Catalog (Voges+ 1994) J/A+A/330/108 : ROSAT detected quasars. II. (Yuan+ 1998) Byte-by-Byte Description of file: table1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- IAU IAU name of the object 11 A1 --- n_IAU [ *?!] A flag for classification 12- 29 A18 --- Name *Alternative name from VV93 VII/166 31- 32 I2 h RAh Right ascension J2000 (hours) 34- 35 I2 min RAm Right ascension J2000 (minutes) 37- 40 F4.1 s RAs Right ascension J2000 (seconds) 42 A1 --- DE- Declination sign 43- 44 I2 deg DEd Declination J2000 (degrees) 46- 47 I2 arcmin DEm Declination J2000 (') 49- 50 I2 arcsec DEs Declination J2000 (") 52- 56 F5.3 --- z *[]? Redshift 58- 62 F5.2 mag Vmag *[]? Magnitude from VV93 VII/166 64- 69 F6.3 Jy F6cm []? 6cm radio flux density 71- 75 F5.2 --- alpha_r []? Radio spectral index 77- 82 F6.2 10-12mW/m2 Fx [] Unabsorbed X-ray flux density 84- 88 F5.2 10-12mW/m2 e_Fx *[] Error of X-ray flux density 90- 93 F4.2 --- Gamma *[]? X-ray spectral photon index 95- 98 F4.2 --- E_Gamma *[]? Positive error of photon index 100-103 F4.2 --- e_Gamma *[]? Negative error of photon index 105-106 A2 --- Com *[SP ] Notes on the X-ray detection 108-109 A2 --- Ref *? Reference for the quoted spectral index -------------------------------------------------------------------------------- Note on Name: A '*' denotes a radio-quiet object; a '?' mark indicates that no 5GHz flux is available; and a '!' means that the X-ray flux is probably corrupted by another source. Note on z: A '0' as the 3rd decimal is mostly an artifact of the machine readable form of the catalogue. See the printed version of VV93 VII/166 for the appropriate values. Note on Vmag and e_Fx: One sigma statistical errors from count rates only Note on Gamma: Spectral photon index in the ROSAT energy band for a power law fit (S=C*E**(-Gamma)) with Galactic absorption Note on E_Gamma and e_Gamma: One sigma errors. If no error is given, the value of the error is unphysically large. Note on Com: S: detected in RASS; P: detected in Pointed observations Note on Ref: BP: Buehler P., et al. (1995A&A...295..309B 1995A&A...295..309B) BH: Brunner H., et al. (1994A&A...287..436B 1994A&A...287..436B) BW: Brinkmann W. & Siebert J. (1995A&A...300L..33B 1995A&A...300L..33B) EM: Elvis M., et al. (1994ApJ...422...60E 1994ApJ...422...60E) LA: Laor A., et al. (1994ApJ...435..611L 1994ApJ...435..611L) NM: Neumann M., et al. J/A+AS/106/303 SN: Schartel N., et al. (1996A&A...307...33) SJ: Siebert J., et al., (1996A&A...307....8S 1996A&A...307....8S) ZY: Zhang Y.F. & Marscher A.P., 1994 AIP Conf. Proc. 313, p.406 -------------------------------------------------------------------------------- Acknowledgements: Weimin Yuan References: Brinkmann W, Siebert J., 1995, A&A, 300, L33 =1995A&A...300L..33B 1995A&A...300L..33B Brunner H. et al., 1994, A&A 287, 436 =1994A&A...287..436B 1994A&A...287..436B Buehler P. et al., 1995, A&A 295, 309 =1995A&A...295..309B 1995A&A...295..309B Elvis M. et al., 1994, ApJ 422, 60 =1994ApJ...422...60E 1994ApJ...422...60E Laor A. et al., 1994, ApJ 435, 611 =1994ApJ...435..611L 1994ApJ...435..611L Neumann M. et al., 1994, A&AS 106, 303 =Cat. J/A+AS/106/303 Schartel N. et al., 1996, A&A 307, 33 =1996A&A...307...33 Siebert J. et al., 1996, A&A 307, 8 =1996A&A...307....8S 1996A&A...307....8S Veron-Cetty, M.-P. & Veron, P., 1993 (VV93) =Catalogue VII/166 Voges W., 1992, In: Proc. of the ISY Conference ''Space Science'', ESA ISY-3, ESA Publications, p.9 (See catalogue IX/10) Voges W., et al., 1995, ROSAT NEWS No. 32 =Catalogue IX/11 Zhang Y. F., Marscher A. P., 1994, AIP Conf. Proc. 313, p.406
(End) Patricia Bauer [CDS] 27-Sep-1996
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