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.; Vergani, S. D.; Savaglio, S.

doi:10.1051/0004-6361/201321666

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

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Savaglio, S.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-83BC-9

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