SPECTROSCOPIC IDENTIFICATIONS OFSPITZERSOURCES IN THE SWIRE/XMM-NEWTON/ELAIS-S1 FIELD: A LARGE FRACTION OF ACTIVE GALACTIC NUCLEI WITH HIGHF(24 μm)/F(R) RATIO-Reference-Cited by-同舟云学术

SPECTROSCOPIC IDENTIFICATIONS OFSPITZERSOURCES IN THE SWIRE/XMM-NEWTON/ELAIS-S1 FIELD: A LARGE FRACTION OF ACTIVE GALACTIC NUCLEI WITH HIGHF(24 μm)/F(R) RATIO

Published:2009-09-15 Issue:2 Volume:703 Page:1778-1790
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Sacchi N.,La Franca F.,Feruglio C.,Fiore F.,Puccetti S.,Cocchia F.,Berta S.,Brusa M.,Cimatti A.,Comastri A.,Franceschini A.,Gruppioni C.,Maiolino R.,Matute I.,Polletta M.,Pozzetti L.,Pozzi F.,Vignali C.,Zamorani G.,Oliver S.,Rowan-Robinson M.,Smith G.,Lonsdale C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference79 articles.

1. The European Large‐AreaInfrared Space ObservatorySurvey V: ABeppoSAXHard X‐Ray Survey of the S1 Region

2. Reliable Identification of Compton‐thick Quasars atz≈ 2:SpitzerMid‐Infrared Spectroscopy of HDF‐oMD49

3. Infrared Power‐Law Galaxies in the Chandra Deep Field–South: Active Galactic Nuclei and Ultraluminous Infrared Galaxies

4. Does the AGN Unified Model Evolve with Redshift? Using the X‐Ray Background to Predict the Mid‐Infrared Emission of AGNs

5. The ESO-Spitzer Imaging extragalactic Survey (ESIS)

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