Detection of a supernova signature associated with GRB 011121

J. S. Bloom; S. R. Kulkarni; P. A. Price; D. Reichart; T. J. Galama; B. P. Schmidt; D. A. Frail; E. Berger; P. J. McCarthy; R. A. Chevalier; J. C. Wheeler; J. P. Halpern; D. W. Fox; S. G. Djorgovski; F. A. Harrison; R. Sari; T. S. Axelrod; R. A. Kimble; J. Holtzman; K. Hurley; F. Frontera; L. Piro; E. Costa

doi:10.1086/341551

Detection of a supernova signature associated with GRB 011121

J. S. Bloom
, S. R. Kulkarni
, P. A. Price
, D. Reichart
, T. J. Galama
, B. P. Schmidt
, D. A. Frail
, E. Berger
, P. J. McCarthy
, R. A. Chevalier
, J. C. Wheeler
, J. P. Halpern
, D. W. Fox
, S. G. Djorgovski
, F. A. Harrison
, R. Sari
, T. S. Axelrod
, R. A. Kimble
, J. Holtzman
, K. Hurley

F. Frontera, L. Piro, E. Costa

Research output: Contribution to journal › Article › peer-review

128 Scopus citations

Abstract

Using observations from an extensive monitoring campaign with the Hubble Space Telescope, we present the detection of an intermediate-time flux excess that is redder in color relative to the afterglow of GRB 011121, currently distinguished as the gamma-ray burst with the lowest known redshift. The red "bump," which exhibits a spectral rollover at ∼7200 A, is well described by a redshifted Type le supernova that occurred approximately at the same time as the gamma-ray burst event. The inferred luminosity is about half that of the bright supernova SN 1998bw. These results serve as compelling evidence for a massive star origin of long-duration gamma-ray bursts. Models that posit a supernova explosion weeks to months preceding the gamma-ray burst event are excluded by these observations. Finally, we discuss the relationship between spherical core-collapse supernovae and gamma-ray bursts.

Original language	English (US)
Pages (from-to)	L45-L49
Journal	Astrophysical Journal
Volume	572
Issue number	1 II
DOIs	https://doi.org/10.1086/341551
State	Published - Jun 10 2002

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1086/341551

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Bloom, J. S., Kulkarni, S. R., Price, P. A., Reichart, D., Galama, T. J., Schmidt, B. P., Frail, D. A., Berger, E., McCarthy, P. J., Chevalier, R. A., Wheeler, J. C., Halpern, J. P., Fox, D. W., Djorgovski, S. G., Harrison, F. A., Sari, R., Axelrod, T. S., Kimble, R. A., Holtzman, J., ... Costa, E. (2002). Detection of a supernova signature associated with GRB 011121. Astrophysical Journal, 572(1 II), L45-L49. https://doi.org/10.1086/341551

@article{5bef052f44c34aaeb613d08ca9dc0408,

title = "Detection of a supernova signature associated with GRB 011121",

abstract = "Using observations from an extensive monitoring campaign with the Hubble Space Telescope, we present the detection of an intermediate-time flux excess that is redder in color relative to the afterglow of GRB 011121, currently distinguished as the gamma-ray burst with the lowest known redshift. The red {"}bump,{"} which exhibits a spectral rollover at ∼7200 A, is well described by a redshifted Type le supernova that occurred approximately at the same time as the gamma-ray burst event. The inferred luminosity is about half that of the bright supernova SN 1998bw. These results serve as compelling evidence for a massive star origin of long-duration gamma-ray bursts. Models that posit a supernova explosion weeks to months preceding the gamma-ray burst event are excluded by these observations. Finally, we discuss the relationship between spherical core-collapse supernovae and gamma-ray bursts.",

author = "Bloom, \{J. S.\} and Kulkarni, \{S. R.\} and Price, \{P. A.\} and D. Reichart and Galama, \{T. J.\} and Schmidt, \{B. P.\} and Frail, \{D. A.\} and E. Berger and McCarthy, \{P. J.\} and Chevalier, \{R. A.\} and Wheeler, \{J. C.\} and Halpern, \{J. P.\} and Fox, \{D. W.\} and Djorgovski, \{S. G.\} and Harrison, \{F. A.\} and R. Sari and Axelrod, \{T. S.\} and Kimble, \{R. A.\} and J. Holtzman and K. Hurley and F. Frontera and L. Piro and E. Costa",

note = "Funding Information: sights toward the improvement of this work. A. MacFadyen and E. Ramirez-Ruiz are acknowledged for their constructive comments on the Letter. J. S. B. is a Fannie and John Hertz Foundation Fellow. F. A. H. acknowledges support from a Presidential Early Career award. S. R. K. and S. G. D. thank the NSF for support. R. S. is grateful for support from a NASA ATP grant. R. S. and T. J. G. acknowledge support from the Sherman Fairchild Foundation. J. C. W. acknowledges support from NASA grant NAG59302. K. H. is grateful for Ulysses support under JPL contract 958056 and for IPN support under NASA grants FDNAG 5-11451 and NAG 5-17100. Support for Proposal HST-GO-09180.01-A was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.",

year = "2002",

month = jun,

day = "10",

doi = "10.1086/341551",

language = "English (US)",

volume = "572",

pages = "L45--L49",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1 II",

}

Bloom, JS, Kulkarni, SR, Price, PA, Reichart, D, Galama, TJ, Schmidt, BP, Frail, DA, Berger, E, McCarthy, PJ, Chevalier, RA, Wheeler, JC, Halpern, JP, Fox, DW, Djorgovski, SG, Harrison, FA, Sari, R, Axelrod, TS, Kimble, RA, Holtzman, J, Hurley, K, Frontera, F, Piro, L & Costa, E 2002, 'Detection of a supernova signature associated with GRB 011121', Astrophysical Journal, vol. 572, no. 1 II, pp. L45-L49. https://doi.org/10.1086/341551

TY - JOUR

T1 - Detection of a supernova signature associated with GRB 011121

AU - Bloom, J. S.

AU - Kulkarni, S. R.

AU - Price, P. A.

AU - Reichart, D.

AU - Galama, T. J.

AU - Schmidt, B. P.

AU - Frail, D. A.

AU - Berger, E.

AU - McCarthy, P. J.

AU - Chevalier, R. A.

AU - Wheeler, J. C.

AU - Halpern, J. P.

AU - Fox, D. W.

AU - Djorgovski, S. G.

AU - Harrison, F. A.

AU - Sari, R.

AU - Axelrod, T. S.

AU - Kimble, R. A.

AU - Holtzman, J.

AU - Hurley, K.

AU - Frontera, F.

AU - Piro, L.

AU - Costa, E.

N1 - Funding Information: sights toward the improvement of this work. A. MacFadyen and E. Ramirez-Ruiz are acknowledged for their constructive comments on the Letter. J. S. B. is a Fannie and John Hertz Foundation Fellow. F. A. H. acknowledges support from a Presidential Early Career award. S. R. K. and S. G. D. thank the NSF for support. R. S. is grateful for support from a NASA ATP grant. R. S. and T. J. G. acknowledge support from the Sherman Fairchild Foundation. J. C. W. acknowledges support from NASA grant NAG59302. K. H. is grateful for Ulysses support under JPL contract 958056 and for IPN support under NASA grants FDNAG 5-11451 and NAG 5-17100. Support for Proposal HST-GO-09180.01-A was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.

PY - 2002/6/10

Y1 - 2002/6/10

N2 - Using observations from an extensive monitoring campaign with the Hubble Space Telescope, we present the detection of an intermediate-time flux excess that is redder in color relative to the afterglow of GRB 011121, currently distinguished as the gamma-ray burst with the lowest known redshift. The red "bump," which exhibits a spectral rollover at ∼7200 A, is well described by a redshifted Type le supernova that occurred approximately at the same time as the gamma-ray burst event. The inferred luminosity is about half that of the bright supernova SN 1998bw. These results serve as compelling evidence for a massive star origin of long-duration gamma-ray bursts. Models that posit a supernova explosion weeks to months preceding the gamma-ray burst event are excluded by these observations. Finally, we discuss the relationship between spherical core-collapse supernovae and gamma-ray bursts.

AB - Using observations from an extensive monitoring campaign with the Hubble Space Telescope, we present the detection of an intermediate-time flux excess that is redder in color relative to the afterglow of GRB 011121, currently distinguished as the gamma-ray burst with the lowest known redshift. The red "bump," which exhibits a spectral rollover at ∼7200 A, is well described by a redshifted Type le supernova that occurred approximately at the same time as the gamma-ray burst event. The inferred luminosity is about half that of the bright supernova SN 1998bw. These results serve as compelling evidence for a massive star origin of long-duration gamma-ray bursts. Models that posit a supernova explosion weeks to months preceding the gamma-ray burst event are excluded by these observations. Finally, we discuss the relationship between spherical core-collapse supernovae and gamma-ray bursts.

UR - https://www.scopus.com/pages/publications/18344412795

UR - https://www.scopus.com/pages/publications/18344412795#tab=citedBy

U2 - 10.1086/341551

DO - 10.1086/341551

M3 - Article

AN - SCOPUS:18344412795

SN - 0004-637X

VL - 572

SP - L45-L49

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 II

ER -

Detection of a supernova signature associated with GRB 011121

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