On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box

J.M.C. Ceron; J. Gorosabel; A.J. Castro-Tirado; V.V. Sokolov; V.L. Afanasiev; T.A. Fatkhullin; S.N. Dodonov; V.N. Komarova; A.M. Cherepashchuk; K.A. Postnov; U. Lisenfeld; J. Greiner; S. Klose; J. Hjorth; J.P.U. Fynbo; Henrik Pedersen; E. Rol; J. Fliri; M. Feldt; G. Feulner; M.I. Andersen; B.L. Jensen; M.D.P. Ramirez; F.J. Vrba; A.A. Henden; G. Israelian; N.R. Tanvir

doi:10.1051/0004-6361:20035921

On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box

J.M.C. Ceron, J. Gorosabel, A.J. Castro-Tirado, V.V. Sokolov, V.L. Afanasiev, T.A. Fatkhullin, S.N. Dodonov, V.N. Komarova, A.M. Cherepashchuk, K.A. Postnov, U. Lisenfeld, J. Greiner, S. Klose, J. Hjorth, J.P.U. Fynbo, Henrik Pedersen, E. Rol, J. Fliri, M. Feldt, G. FeulnerM.I. Andersen, B.L. Jensen, M.D.P. Ramirez, F.J. Vrba, A.A. Henden, G. Israelian, N.R. Tanvir

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Abstract

We present optical and NIR (near infrared) follow up observations of the GRB 001109 from 1 to 300 days after the burst. No transient emission was found at these wavelengths within this GRB's (Gamma Ray Burst) 50" radius BeppoSAX error box. Strong limits (3sigma) are set with: Rgreater than or similar to21, 10.2 h after the GRB; Igreater than or similar to23, 11.4 h after the GRB; Hgreater than or similar to20.7, 9.9 h after the GRB; and K(S)greater than or similar to20, 9.6 h after the GRB. We discuss whether the radio source found in the GRB's error box (Taylor et al. 2000) might be related to the afterglow. We also present a multiwavelength study of a reddened starburst galaxy, found coincident with the potential radio and the X-ray afterglow. We show that our strong I band upper limit makes of the GRB 001109 the darkest one localised by the BeppoSAX's NFI (Narrow Field Instrument), and it is one of the most constraining upper limits on GRB afterglows to date. Further to it, the implications of these observations in the context of dark GRBs are considered.

Original language	English
Journal	Astronomy and Astrophysics
Volume	424
Issue number	3
Pages (from-to)	833-839
ISSN	0004-6361
DOIs	https://doi.org/10.1051/0004-6361:20035921
Publication status	Published - 2004

Keywords

Galaxy : fundamental parameters
gamma rays : bursts
techniques : photometric

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10.1051/0004-6361:20035921

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Ceron, J. M. C., Gorosabel, J., Castro-Tirado, A. J., Sokolov, V. V., Afanasiev, V. L., Fatkhullin, T. A., Dodonov, S. N., Komarova, V. N., Cherepashchuk, A. M., Postnov, K. A., Lisenfeld, U., Greiner, J., Klose, S., Hjorth, J., Fynbo, J. P. U., Pedersen, H., Rol, E., Fliri, J., Feldt, M., ... Tanvir, N. R. (2004). On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box. Astronomy and Astrophysics, 424(3), 833-839. https://doi.org/10.1051/0004-6361:20035921

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title = "On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box",

abstract = "We present optical and NIR (near infrared) follow up observations of the GRB 001109 from 1 to 300 days after the burst. No transient emission was found at these wavelengths within this GRB's (Gamma Ray Burst) 50{"} radius BeppoSAX error box. Strong limits (3sigma) are set with: Rgreater than or similar to21, 10.2 h after the GRB; Igreater than or similar to23, 11.4 h after the GRB; Hgreater than or similar to20.7, 9.9 h after the GRB; and K(S)greater than or similar to20, 9.6 h after the GRB. We discuss whether the radio source found in the GRB's error box (Taylor et al. 2000) might be related to the afterglow. We also present a multiwavelength study of a reddened starburst galaxy, found coincident with the potential radio and the X-ray afterglow. We show that our strong I band upper limit makes of the GRB 001109 the darkest one localised by the BeppoSAX's NFI (Narrow Field Instrument), and it is one of the most constraining upper limits on GRB afterglows to date. Further to it, the implications of these observations in the context of dark GRBs are considered.",

keywords = "Galaxy : fundamental parameters, gamma rays : bursts, techniques : photometric",

author = "J.M.C. Ceron and J. Gorosabel and A.J. Castro-Tirado and V.V. Sokolov and V.L. Afanasiev and T.A. Fatkhullin and S.N. Dodonov and V.N. Komarova and A.M. Cherepashchuk and K.A. Postnov and U. Lisenfeld and J. Greiner and S. Klose and J. Hjorth and J.P.U. Fynbo and Henrik Pedersen and E. Rol and J. Fliri and M. Feldt and G. Feulner and M.I. Andersen and B.L. Jensen and M.D.P. Ramirez and F.J. Vrba and A.A. Henden and G. Israelian and N.R. Tanvir",

year = "2004",

doi = "10.1051/0004-6361:20035921",

language = "English",

volume = "424",

pages = "833--839",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "3",

}

Ceron, JMC, Gorosabel, J, Castro-Tirado, AJ, Sokolov, VV, Afanasiev, VL, Fatkhullin, TA, Dodonov, SN, Komarova, VN, Cherepashchuk, AM, Postnov, KA, Lisenfeld, U, Greiner, J, Klose, S, Hjorth, J, Fynbo, JPU, Pedersen, H, Rol, E, Fliri, J, Feldt, M, Feulner, G, Andersen, MI, Jensen, BL, Ramirez, MDP, Vrba, FJ, Henden, AA, Israelian, G & Tanvir, NR 2004, 'On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box', Astronomy and Astrophysics, vol. 424, no. 3, pp. 833-839. https://doi.org/10.1051/0004-6361:20035921

TY - JOUR

T1 - On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box

AU - Ceron, J.M.C.

AU - Gorosabel, J.

AU - Castro-Tirado, A.J.

AU - Sokolov, V.V.

AU - Afanasiev, V.L.

AU - Fatkhullin, T.A.

AU - Dodonov, S.N.

AU - Komarova, V.N.

AU - Cherepashchuk, A.M.

AU - Postnov, K.A.

AU - Lisenfeld, U.

AU - Greiner, J.

AU - Klose, S.

AU - Hjorth, J.

AU - Fynbo, J.P.U.

AU - Pedersen, Henrik

AU - Rol, E.

AU - Fliri, J.

AU - Feldt, M.

AU - Feulner, G.

AU - Andersen, M.I.

AU - Jensen, B.L.

AU - Ramirez, M.D.P.

AU - Vrba, F.J.

AU - Henden, A.A.

AU - Israelian, G.

AU - Tanvir, N.R.

PY - 2004

Y1 - 2004

N2 - We present optical and NIR (near infrared) follow up observations of the GRB 001109 from 1 to 300 days after the burst. No transient emission was found at these wavelengths within this GRB's (Gamma Ray Burst) 50" radius BeppoSAX error box. Strong limits (3sigma) are set with: Rgreater than or similar to21, 10.2 h after the GRB; Igreater than or similar to23, 11.4 h after the GRB; Hgreater than or similar to20.7, 9.9 h after the GRB; and K(S)greater than or similar to20, 9.6 h after the GRB. We discuss whether the radio source found in the GRB's error box (Taylor et al. 2000) might be related to the afterglow. We also present a multiwavelength study of a reddened starburst galaxy, found coincident with the potential radio and the X-ray afterglow. We show that our strong I band upper limit makes of the GRB 001109 the darkest one localised by the BeppoSAX's NFI (Narrow Field Instrument), and it is one of the most constraining upper limits on GRB afterglows to date. Further to it, the implications of these observations in the context of dark GRBs are considered.

AB - We present optical and NIR (near infrared) follow up observations of the GRB 001109 from 1 to 300 days after the burst. No transient emission was found at these wavelengths within this GRB's (Gamma Ray Burst) 50" radius BeppoSAX error box. Strong limits (3sigma) are set with: Rgreater than or similar to21, 10.2 h after the GRB; Igreater than or similar to23, 11.4 h after the GRB; Hgreater than or similar to20.7, 9.9 h after the GRB; and K(S)greater than or similar to20, 9.6 h after the GRB. We discuss whether the radio source found in the GRB's error box (Taylor et al. 2000) might be related to the afterglow. We also present a multiwavelength study of a reddened starburst galaxy, found coincident with the potential radio and the X-ray afterglow. We show that our strong I band upper limit makes of the GRB 001109 the darkest one localised by the BeppoSAX's NFI (Narrow Field Instrument), and it is one of the most constraining upper limits on GRB afterglows to date. Further to it, the implications of these observations in the context of dark GRBs are considered.

KW - Galaxy : fundamental parameters

KW - gamma rays : bursts

KW - techniques : photometric

U2 - 10.1051/0004-6361:20035921

DO - 10.1051/0004-6361:20035921

M3 - Journal article

VL - 424

SP - 833

EP - 839

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

IS - 3

ER -

On the constraining observations of the dark GRB 001109 and the properties of a z=0.398 radio selected starburst galaxy contained in its error box

Abstract

Keywords

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