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  X-ray observations of highly obscured τ9.7 μm > 1 sources: an efficient method for selecting Compton-thick AGN?

Georgantopoulos, I., Dasyra, K. M., Rovilos, E., Pope, A., Wu, Y., Dickinson, M., et al. (2011). X-ray observations of highly obscured τ9.7 μm > 1 sources: an efficient method for selecting Compton-thick AGN? Astronomy & Astrophysics, 531: A116, pp. 1-11. doi:10.1051/0004-6361/201016338.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-2828-6 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-2829-4
Genre: Journal Article

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 Creators:
Georgantopoulos, I., Author
Dasyra, K. M., Author
Rovilos, E.1, Author              
Pope, A., Author
Wu, Y., Author
Dickinson, M., Author
Comastri, A., Author
Gilli, R., Author
Elbaz, D., Author
Armus, L., Author
Akylas, A., Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2011-07
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201016338
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Title: Astronomy & Astrophysics
  Abbreviation : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 531 Sequence Number: A116 Start / End Page: 1 - 11 Identifier: ISSN: 0004-6361