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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, 198-201 p.Article 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, 198-201 p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-168816Scopus ID: 2-s2.0-84922277911OAI: oai:DiVA.org:kth-168816DiVA: 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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