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UV star-formation rates of GRB host galaxies

Open access
Christensen, L., Hjorth, J., Gorosabel, J.·2004·Astronomy & Astrophysics

Abstract

We study a magnitude-limited sample of 10 gamma-ray burst (GRB) host galaxies with known spectroscopic redshifts (). From an analysis of the spectral energy distributions (SEDs), based on published broad-band optical and near-infrared photometry, we derive photometric redshifts, galaxy types, ages of the dominant stellar populations, internal extinctions, and ultraviolet (UV) star-formation rates (SFRs) of the host galaxies. The photometric redshifts are quite accurate despite the heterogeneous nature of the sample: the rms errors are and with no significant systematic offsets. All the host galaxies have SEDs similar to young starburst galaxies with moderate to low extinction. A comparison of specific SFRs with those of high-redshift galaxies in the Hubble Deep Fields shows that GRB hosts are most likely similar to the field galaxies with the largest specific SFRs. On the other hand, GRB hosts are not significantly younger than starburst field galaxies at similar redshifts, but are found to be younger than a sample of all types of field galaxies.

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Metadata

Authors
Christensen, L., Hjorth, J., & Gorosabel, J.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2004-09-28
Volume
425
Issue
3
Pages
913-926
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
OpenAlex
W2103734507
Cited by
290
References
1
FWCI
17.33
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: UV star-formation rates of GRB host galaxies. https://app.cochat.ai/papers/10.1051/0004-6361:20040361
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Christensen, L., Hjorth, J., & Gorosabel, J. (2004). UV star-formation rates of GRB host galaxies. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20040361

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