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Apparently fainter gamma-ray bursts at smaller redshifts: An absurdity or a reality?
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0002-9769-8016
2012 (English)In: Memorie della Societa Astronomica Italiana, Supplementi - Journal of the Italian Astronomical Society, Supplement, ISSN 1824-0178, Vol. 21, p. 198-201Article in journal (Refereed) Published
Abstract [en]

Naturally, it is expected that the apparently fainter objects should, on average, lie at larger redshifts. It is shown - by theoretical and observational studies of different satellite data samples - that this need not be the case for the long gamma-ray bursts (GRBs). Therefore, bursts at redshifts larger than 5 should be really rare due to this inverse behaviour. The apparently fainter objects can, on average, be at smaller redshifts indeed.

Place, publisher, year, edition, pages
2012. Vol. 21, p. 198-201
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-168816Scopus ID: 2-s2.0-84922277911OAI: oai:DiVA.org:kth-168816DiVA, id: diva2:819087
Conference
GRBs as Probes: From the Progenitors Environment to the High; Como; Italy
Note

QC 20150610

Available from: 2015-06-10 Created: 2015-06-09 Last updated: 2015-06-10Bibliographically approved

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Ryde, Felix

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