ATLAS OF QUASAR ENERGY-DISTRIBUTIONS

被引:1598
作者
ELVIS, M
WILKES, BJ
MCDOWELL, JC
GREEN, RF
BECHTOLD, J
WILLNER, SP
OEY, MS
POLOMSKI, E
CUTRI, R
机构
[1] KITT PEAK NATL OBSERV,NATL OPT ASTRON OBSERV,TUCSON,AZ 85726
[2] UNIV ARIZONA,STEWARD OBSERV,TUCSON,AZ 85721
[3] CTR EXTREME ULTRAVIOLET ASTROPHYS,BERKELEY,CA
关键词
ATLASES; GALAXIES; PHOTOMETRY; QUASARS; GENERAL;
D O I
10.1086/192093
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an atlas of the spectral energy distributions (SEDs) of normal, nonblazar, quasars over the whole available range ( radio to 10 keV X-rays) of the electromagnetic spectrum. The primary (UVSX) sample includes 47 quasars for which the spectral energy distributions include X-ray spectral indices and UV data. Of these, 29 are radio quiet, and 18 are radio loud. The SEDs are presented both in figures and in tabular form, with additional tabular material published on CD-ROM. Previously unpublished observational data for a second set of quasars excluded from the primary sample are also tabulated. The effects of host galaxy starlight contamination and foreground extinction on the UVSX sample are considered and the sample is used to investigate the range of SED properties. Of course, the properties we derive are influenced strongly by the selection effects induced by quasar discovery techniques. We derive the mean energy distribution (MED) for radio-loud and radio-quiet objects and present the bolometric corrections derived from it. We note, however, that the dispersion about this mean is large (similar to one decade for both the infrared and ultraviolet components when the MED is normalized at the near-infrared inflection). At least part of the dispersion in the ultraviolet may be due to time variability, but this is unlikely to be important in the infrared. The existence of such a large dispersion indicates that the MED reflects only some of the properties of quasars and so should be used only with caution.
引用
收藏
页码:1 / 68
页数:68
相关论文
共 145 条
[1]  
Adam G., 1978, Astronomy and Astrophysics Supplement Series, V31, P151
[2]  
Adam G., 1985, Astronomy & Astrophysics Supplement Series, V61, P225
[3]  
[Anonymous], 1985, IAU S
[4]  
Antonucci R., 1990, Astrophysical Journal, V353, P416, DOI 10.1086/168628
[5]   THE CORES OF LOBE-DOMINANT QUASARS [J].
ANTONUCCI, RRJ ;
BARVAINIS, R .
ASTROPHYSICAL JOURNAL, 1988, 325 (02) :L21-L23
[6]   EXOSAT OBSERVATIONS OF A STRONG SOFT-X-RAY EXCESS IN MKN-841 [J].
ARNAUD, KA ;
BRANDUARDIRAYMONT, G ;
CULHANE, JL ;
FABIAN, AC ;
HAZARD, C ;
MCGLYNN, TA ;
SHAFER, RA ;
TENNANT, AF ;
WARD, MJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1985, 217 (01) :105-+
[7]  
Azusenis A., 1969, Astronomicheskii Zhurnal, V46, P402
[8]   MILLIMETER, CENTIMETER, AND CARBON-MONOXIDE OBSERVATIONS OF RADIO-QUIET QUASARS AND LUMINOUS SEYFERT-1 GALAXIES DETECTED BY IRAS [J].
BARVAINIS, R ;
ANTONUCCI, R .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1989, 70 (02) :257-270
[9]  
BEZLER M, 1984, ASTRON ASTROPHYS, V136, P351
[10]   STUDIES OF THE VIRGO CLUSTER .1. PHOTOMETRY OF 109 GALAXIES NEAR THE CLUSTER CENTER TO SERVE AS STANDARDS [J].
BINGGELI, B ;
SANDAGE, A ;
TARENGHI, M .
ASTRONOMICAL JOURNAL, 1984, 89 (01) :64-&