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Principal Component Analysis of Gamma-Ray Bursts' Spectra
Stockholm University, Faculty of Science, Department of Astronomy.
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2005 (English)In: Nuovo Cimento C, Vol. 28, no 3, 295-298 p.Article in journal (Refereed) Published
Abstract [en]

The origin of dark bursts--i.e. that have no observed afterglows in X-ray, optical/NIR and radio ranges--is unclear yet. Different possibilities--instrumental biases, very high redshifts, extinction in the host galaxies--are discussed and shown to be important. On the other hand, the dark bursts should not form a new subgroup of long gamma-ray bursts themselves.

Place, publisher, year, edition, pages
2005. Vol. 28, no 3, 295-298 p.
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Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:su:diva-11321DOI: doi:10.1393/ncc/i2005-10045-1OAI: oai:DiVA.org:su-11321DiVA: diva2:177840
Available from: 2008-01-10 Created: 2008-01-10 Last updated: 2011-01-12Bibliographically approved

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