Are the hosts of gamma-ray bursts sub-luminous and blue galaxies?

E. Le Floc'h, P. A. Duc, I. F. Mirabel, D. B. Sanders, G. Bosch, R. J. Diaz, C. J. Donzelli, I. Rodrigues, T. J.L. Courvoisier, J. Greiner, S. Mereghetti, J. Melnick, J. Maza, D. Minniti

Resultado de la investigación: Article

217 Citas (Scopus)

Resumen

K-band imaging observations of ten gamma-ray burst (GRB) host galaxies were discussed. Optical and radio afterglow associated with the GRB event were also studied. Results showed that GRB host galaxies are lying at 0.5 ≲z≲1.5, infrared, mid-infrared and submillimeter deep surveys.

Idioma originalEnglish
Páginas (desde-hasta)499-510
Número de páginas12
PublicaciónAstronomy and Astrophysics
Volumen400
N.º2
DOI
EstadoPublished - 1 ene 2003

Huella dactilar

gamma ray bursts
radio
galaxies
extremely high frequencies
afterglows

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Citar esto

Le Floc'h, E., Duc, P. A., Mirabel, I. F., Sanders, D. B., Bosch, G., Diaz, R. J., ... Minniti, D. (2003). Are the hosts of gamma-ray bursts sub-luminous and blue galaxies? Astronomy and Astrophysics, 400(2), 499-510. https://doi.org/10.1051/0004-6361:20030001
Le Floc'h, E. ; Duc, P. A. ; Mirabel, I. F. ; Sanders, D. B. ; Bosch, G. ; Diaz, R. J. ; Donzelli, C. J. ; Rodrigues, I. ; Courvoisier, T. J.L. ; Greiner, J. ; Mereghetti, S. ; Melnick, J. ; Maza, J. ; Minniti, D. / Are the hosts of gamma-ray bursts sub-luminous and blue galaxies?. En: Astronomy and Astrophysics. 2003 ; Vol. 400, N.º 2. pp. 499-510.
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abstract = "K-band imaging observations of ten gamma-ray burst (GRB) host galaxies were discussed. Optical and radio afterglow associated with the GRB event were also studied. Results showed that GRB host galaxies are lying at 0.5 ≲z≲1.5, infrared, mid-infrared and submillimeter deep surveys.",
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Le Floc'h, E, Duc, PA, Mirabel, IF, Sanders, DB, Bosch, G, Diaz, RJ, Donzelli, CJ, Rodrigues, I, Courvoisier, TJL, Greiner, J, Mereghetti, S, Melnick, J, Maza, J & Minniti, D 2003, 'Are the hosts of gamma-ray bursts sub-luminous and blue galaxies?', Astronomy and Astrophysics, vol. 400, n.º 2, pp. 499-510. https://doi.org/10.1051/0004-6361:20030001

Are the hosts of gamma-ray bursts sub-luminous and blue galaxies? / Le Floc'h, E.; Duc, P. A.; Mirabel, I. F.; Sanders, D. B.; Bosch, G.; Diaz, R. J.; Donzelli, C. J.; Rodrigues, I.; Courvoisier, T. J.L.; Greiner, J.; Mereghetti, S.; Melnick, J.; Maza, J.; Minniti, D.

En: Astronomy and Astrophysics, Vol. 400, N.º 2, 01.01.2003, p. 499-510.

Resultado de la investigación: Article

TY - JOUR

T1 - Are the hosts of gamma-ray bursts sub-luminous and blue galaxies?

AU - Le Floc'h, E.

AU - Duc, P. A.

AU - Mirabel, I. F.

AU - Sanders, D. B.

AU - Bosch, G.

AU - Diaz, R. J.

AU - Donzelli, C. J.

AU - Rodrigues, I.

AU - Courvoisier, T. J.L.

AU - Greiner, J.

AU - Mereghetti, S.

AU - Melnick, J.

AU - Maza, J.

AU - Minniti, D.

PY - 2003/1/1

Y1 - 2003/1/1

N2 - K-band imaging observations of ten gamma-ray burst (GRB) host galaxies were discussed. Optical and radio afterglow associated with the GRB event were also studied. Results showed that GRB host galaxies are lying at 0.5 ≲z≲1.5, infrared, mid-infrared and submillimeter deep surveys.

AB - K-band imaging observations of ten gamma-ray burst (GRB) host galaxies were discussed. Optical and radio afterglow associated with the GRB event were also studied. Results showed that GRB host galaxies are lying at 0.5 ≲z≲1.5, infrared, mid-infrared and submillimeter deep surveys.

KW - Cosmology: observations

KW - Galaxies: evolution

KW - Galaxies: starburst

KW - Gamma rays: bursts

UR - http://www.scopus.com/inward/record.url?scp=0037339299&partnerID=8YFLogxK

U2 - 10.1051/0004-6361:20030001

DO - 10.1051/0004-6361:20030001

M3 - Article

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VL - 400

SP - 499

EP - 510

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

IS - 2

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Le Floc'h E, Duc PA, Mirabel IF, Sanders DB, Bosch G, Diaz RJ y otros. Are the hosts of gamma-ray bursts sub-luminous and blue galaxies? Astronomy and Astrophysics. 2003 ene 1;400(2):499-510. https://doi.org/10.1051/0004-6361:20030001