GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8

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GRB 051008 : a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8. / Volnova, A. A.; Pozanenko, A. S.; Gorosabel, J.; Perley, D. A.; Frederiks, D. D.; Kann, D. A.; Rumyantsev, V. V.; Biryukov, V. V.; Biryukov, V. V.; Castro-Tirado, A. J.; Ferrero, P.; Golenetskii, S. V.; Klose, S.; Loznikov, V. M.; Minaev, P. Yu.; Stecklum, B.; Svinkin, D. S.; Tsvetkova, A. E.; Ugarte Postigo, Antonio de; Ulanov, M. V.

I: Royal Astronomical Society. Monthly Notices, Bind 442, Nr. 3, 11.08.2014, s. 2586-2599.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Volnova, AA, Pozanenko, AS, Gorosabel, J, Perley, DA, Frederiks, DD, Kann, DA, Rumyantsev, VV, Biryukov, VV, Biryukov, VV, Castro-Tirado, AJ, Ferrero, P, Golenetskii, SV, Klose, S, Loznikov, VM, Minaev, PY, Stecklum, B, Svinkin, DS, Tsvetkova, AE, Ugarte Postigo, AD & Ulanov, MV 2014, 'GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8', Royal Astronomical Society. Monthly Notices, bind 442, nr. 3, s. 2586-2599. https://doi.org/10.1093/mnras/stu999

APA

Volnova, A. A., Pozanenko, A. S., Gorosabel, J., Perley, D. A., Frederiks, D. D., Kann, D. A., Rumyantsev, V. V., Biryukov, V. V., Biryukov, V. V., Castro-Tirado, A. J., Ferrero, P., Golenetskii, S. V., Klose, S., Loznikov, V. M., Minaev, P. Y., Stecklum, B., Svinkin, D. S., Tsvetkova, A. E., Ugarte Postigo, A. D., & Ulanov, M. V. (2014). GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8. Royal Astronomical Society. Monthly Notices, 442(3), 2586-2599. https://doi.org/10.1093/mnras/stu999

Vancouver

Volnova AA, Pozanenko AS, Gorosabel J, Perley DA, Frederiks DD, Kann DA o.a. GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8. Royal Astronomical Society. Monthly Notices. 2014 aug. 11;442(3):2586-2599. https://doi.org/10.1093/mnras/stu999

Author

Volnova, A. A. ; Pozanenko, A. S. ; Gorosabel, J. ; Perley, D. A. ; Frederiks, D. D. ; Kann, D. A. ; Rumyantsev, V. V. ; Biryukov, V. V. ; Biryukov, V. V. ; Castro-Tirado, A. J. ; Ferrero, P. ; Golenetskii, S. V. ; Klose, S. ; Loznikov, V. M. ; Minaev, P. Yu. ; Stecklum, B. ; Svinkin, D. S. ; Tsvetkova, A. E. ; Ugarte Postigo, Antonio de ; Ulanov, M. V. / GRB 051008 : a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8. I: Royal Astronomical Society. Monthly Notices. 2014 ; Bind 442, Nr. 3. s. 2586-2599.

Bibtex

@article{a3ac4bfb054b468198f17441b61d31a1,
title = "GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8",
abstract = "We present observations of the dark gamma-ray burst GRB 051008 provided by Swift/BAT, Swift/XRT, Konus-WIND, INTEGRAL/SPI-ACS in the high-energy domain and the Shajn, Swift/UVOT, Tautenburg, NOT, Gemini and Keck I telescopes in the optical and near-infrared bands. The burst was detected only in gamma- and X-rays and neither a prompt optical nor a radio afterglow was detected down to deep limits. We identified the host galaxy of the burst, which is a typical Lyman-break galaxy (LBG) with R-magnitude of 24.06 ± 0.10 mag. A redshift of the galaxy of z=2.77+0.15−0.20 is measured photometrically due to the presence of a clear, strong Lyman-break feature. The host galaxy is a small starburst galaxy with moderate intrinsic extinction (AV = 0.3) and has a star formation rate of ∼60 M⊙ yr−1 typical for LBGs. It is one of the few cases where a GRB host has been found to be a classical LBG. Using the redshift we estimate the isotropic-equivalent radiated energy of the burst to be Eiso = (1.15 ± 0.20) × 1054 erg. We also provide evidence in favour of the hypothesis that the darkness of GRB 051008 is due to local absorption resulting from a dense circumburst medium. ",
author = "Volnova, {A. A.} and Pozanenko, {A. S.} and J. Gorosabel and Perley, {D. A.} and Frederiks, {D. D.} and Kann, {D. A.} and Rumyantsev, {V. V.} and Biryukov, {V. V.} and Biryukov, {V. V.} and Castro-Tirado, {A. J.} and P. Ferrero and Golenetskii, {S. V.} and S. Klose and Loznikov, {V. M.} and Minaev, {P. Yu.} and B. Stecklum and Svinkin, {D. S.} and Tsvetkova, {A. E.} and {Ugarte Postigo}, {Antonio de} and Ulanov, {M. V.}",
year = "2014",
month = aug,
day = "11",
doi = "10.1093/mnras/stu999",
language = "English",
volume = "442",
pages = "2586--2599",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "3",

}

RIS

TY - JOUR

T1 - GRB 051008

T2 - a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z = 2.8

AU - Volnova, A. A.

AU - Pozanenko, A. S.

AU - Gorosabel, J.

AU - Perley, D. A.

AU - Frederiks, D. D.

AU - Kann, D. A.

AU - Rumyantsev, V. V.

AU - Biryukov, V. V.

AU - Biryukov, V. V.

AU - Castro-Tirado, A. J.

AU - Ferrero, P.

AU - Golenetskii, S. V.

AU - Klose, S.

AU - Loznikov, V. M.

AU - Minaev, P. Yu.

AU - Stecklum, B.

AU - Svinkin, D. S.

AU - Tsvetkova, A. E.

AU - Ugarte Postigo, Antonio de

AU - Ulanov, M. V.

PY - 2014/8/11

Y1 - 2014/8/11

N2 - We present observations of the dark gamma-ray burst GRB 051008 provided by Swift/BAT, Swift/XRT, Konus-WIND, INTEGRAL/SPI-ACS in the high-energy domain and the Shajn, Swift/UVOT, Tautenburg, NOT, Gemini and Keck I telescopes in the optical and near-infrared bands. The burst was detected only in gamma- and X-rays and neither a prompt optical nor a radio afterglow was detected down to deep limits. We identified the host galaxy of the burst, which is a typical Lyman-break galaxy (LBG) with R-magnitude of 24.06 ± 0.10 mag. A redshift of the galaxy of z=2.77+0.15−0.20 is measured photometrically due to the presence of a clear, strong Lyman-break feature. The host galaxy is a small starburst galaxy with moderate intrinsic extinction (AV = 0.3) and has a star formation rate of ∼60 M⊙ yr−1 typical for LBGs. It is one of the few cases where a GRB host has been found to be a classical LBG. Using the redshift we estimate the isotropic-equivalent radiated energy of the burst to be Eiso = (1.15 ± 0.20) × 1054 erg. We also provide evidence in favour of the hypothesis that the darkness of GRB 051008 is due to local absorption resulting from a dense circumburst medium.

AB - We present observations of the dark gamma-ray burst GRB 051008 provided by Swift/BAT, Swift/XRT, Konus-WIND, INTEGRAL/SPI-ACS in the high-energy domain and the Shajn, Swift/UVOT, Tautenburg, NOT, Gemini and Keck I telescopes in the optical and near-infrared bands. The burst was detected only in gamma- and X-rays and neither a prompt optical nor a radio afterglow was detected down to deep limits. We identified the host galaxy of the burst, which is a typical Lyman-break galaxy (LBG) with R-magnitude of 24.06 ± 0.10 mag. A redshift of the galaxy of z=2.77+0.15−0.20 is measured photometrically due to the presence of a clear, strong Lyman-break feature. The host galaxy is a small starburst galaxy with moderate intrinsic extinction (AV = 0.3) and has a star formation rate of ∼60 M⊙ yr−1 typical for LBGs. It is one of the few cases where a GRB host has been found to be a classical LBG. Using the redshift we estimate the isotropic-equivalent radiated energy of the burst to be Eiso = (1.15 ± 0.20) × 1054 erg. We also provide evidence in favour of the hypothesis that the darkness of GRB 051008 is due to local absorption resulting from a dense circumburst medium.

U2 - 10.1093/mnras/stu999

DO - 10.1093/mnras/stu999

M3 - Journal article

VL - 442

SP - 2586

EP - 2599

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 3

ER -

ID: 139977144