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  A method for quantifying the gamma-ray burst bias. Application in the redshift range of 0–1.1

Boissier, S., Salvaterra, R., Le Floc’h, E., Basa, S., Buat, V., Prantzos, N., et al. (2013). A method for quantifying the gamma-ray burst bias. Application in the redshift range of 0–1.1. Astronomy & Astrophysics, 557: A34, pp. 1-8. doi:10.1051/0004-6361/201321666.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0015-83BC-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-5078-1
Genre: Journal Article

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 Creators:
Boissier, S., Author
Salvaterra, R., Author
Le Floc’h, E., Author
Basa, S., Author
Buat, V., Author
Prantzos, N., Author
Vergani, S. D., Author
Savaglio, S.1, Author              
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2013-09
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201321666
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Title: Astronomy & Astrophysics
  Abbreviation : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 557 Sequence Number: A34 Start / End Page: 1 - 8 Identifier: ISSN: 0004-6361