Predictions for high-frequency radio surveys of extragalactic sources

被引:217
|
作者
De Zotti, G
Ricci, R
Mesa, D
Silva, L
Mazzotta, P
Toffolatti, L
González-Nuevo, J
机构
[1] INAF, Osservatorio Astron Padova, I-35122 Padua, Italy
[2] Scuola Int Super Studi Avanzati, SISSA, I-34014 Trieste, Italy
[3] INAF, Osservatorio Astron Trieste, I-34131 Trieste, Italy
[4] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy
[5] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain
关键词
galaxies : active; galaxies : quasars : general; galaxies : BL Lacertae objects : general; radio continuum : general;
D O I
10.1051/0004-6361:20042108
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present detailed predictions of the contributions of the various source populations to the counts at frequencies of tens of GHz. New evolutionary models are worked out for flat-spectrum radio quasars, BL Lac objects, and steep-spectrum sources. Source populations characterized by spectra peaking at high radio frequencies, such as extreme GPS sources, ADAF/ADIOS sources and early phases of gamma-ray burst afterglows are also dealt with. The counts of different populations of star-forming galaxies ( normal spirals, starbursts, high-z galaxies detected by SCUBA and MAMBO surveys, interpreted as proto-spheroidal galaxies) are estimated taking into account both synchrotron and free-free emission, and dust re-radiation. Our analysis is completed by updated counts of Sunyaev-Zeldovich effects in clusters of galaxies and by a preliminary estimate of galactic-scale Sunyaev-Zeldovich signals associated to proto-galactic plasma.
引用
收藏
页码:893 / 903
页数:11
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