A multi-frequency study of the deep Pavo field

A multi-frequency study of the deep Pavo field

We test the prediction of Hamilton and Helfand (1993) that faint radio selected galaxies are a new class contributing to the diffuse X-ray background (XRB) radiation. The test is based on the correlation of X-ray optical and radio positions for sources detected in ROSAT (S0.08−2.4 keV> 6 x 10−15...

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Bibliographic Details
Main Authors: Filipović M.D., Anderson M., Ekers R.D., Danziger I.J., Zimmermann H.U., White G.L., Jones P.A., Borun B.C.P., Payne J.L., Dionne M., Ganis M., Ognjanović M.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2003-01-01
Series:Serbian Astronomical Journal
Subjects:
cosmology: diffuse radiation
galaxies: active $ galaxies: Seyfert
radio continuum: galaxies
X-rays: galaxies
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2003/1450-698X0366013F.pdf

Internet

http://www.doiserbia.nb.rs/img/doi/1450-698X/2003/1450-698X0366013F.pdf

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