An HST study of the supernovae accompanying GRB 040924 and GRB 041006

A. M. Soderberg; S. R. Kulkarni; P. A. Price; D. B. Fox; E. Berger; D. S. Moon; S. B. Cenko; A. Gal-Yam; D. A. Frail; R. A. Chevalier; L. Cowie; G. S. Da Costa; A. MacFadyen; P. J. Mccarthy; N. Noel; H. S. Park; B. A. Peterson; M. M. Phillips; M. Rauch; A. Rest; J. Rich; K. Roth; M. Roth; B. P. Schmidt; R. C. Smith; P. R. Wood

doi:10.1086/498009

An HST study of the supernovae accompanying GRB 040924 and GRB 041006

A. M. Soderberg, S. R. Kulkarni, P. A. Price, D. B. Fox, E. Berger, D. S. Moon, S. B. Cenko, A. Gal-Yam, D. A. Frail, R. A. Chevalier, L. Cowie, G. S. Da Costa, A. MacFadyen, P. J. Mccarthy, N. Noel, H. S. Park, B. A. Peterson, M. M. Phillips, M. Rauch, A. RestJ. Rich, K. Roth, M. Roth, B. P. Schmidt, R. C. Smith, P. R. Wood

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Abstract

We present the results from a Hubble Space Telescope ACS study of the supernovae (SNe) associated with gamma-ray bursts (GRBs) 040924 (z = 0.86) and 041006 (z = 0.71). We find evidence that both GRBs were associated with an SN 1998bw-like supernova dimmed by ∼ 1.5 and ∼0.3 mag, respectively, making GRB 040924 the faintest GRB-associated SN ever detected. We study the luminosity dispersion in GRB/XRF-associated SNe and compare to local Type Ibc SNe from the literature. We find significant overlap between the two samples, suggesting that GRB/XRF-associated SNe are not necessarily more luminous and do not necessarily produce more ⁵⁶Ni than local SNe. Based on the current (limited) data sets, we find that the two samples may share a similar ⁵⁶Ni production mechanism.

Original language	English (US)
Pages (from-to)	391-399
Number of pages	9
Journal	Astrophysical Journal
Volume	636
Issue number	1 I
DOIs	https://doi.org/10.1086/498009
State	Published - Jan 1 2006

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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Soderberg, A. M., Kulkarni, S. R., Price, P. A., Fox, D. B., Berger, E., Moon, D. S., Cenko, S. B., Gal-Yam, A., Frail, D. A., Chevalier, R. A., Cowie, L., Da Costa, G. S., MacFadyen, A., Mccarthy, P. J., Noel, N., Park, H. S., Peterson, B. A., Phillips, M. M., Rauch, M., ... Wood, P. R. (2006). An HST study of the supernovae accompanying GRB 040924 and GRB 041006. Astrophysical Journal, 636(1 I), 391-399. https://doi.org/10.1086/498009

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title = "An HST study of the supernovae accompanying GRB 040924 and GRB 041006",

abstract = "We present the results from a Hubble Space Telescope ACS study of the supernovae (SNe) associated with gamma-ray bursts (GRBs) 040924 (z = 0.86) and 041006 (z = 0.71). We find evidence that both GRBs were associated with an SN 1998bw-like supernova dimmed by ∼ 1.5 and ∼0.3 mag, respectively, making GRB 040924 the faintest GRB-associated SN ever detected. We study the luminosity dispersion in GRB/XRF-associated SNe and compare to local Type Ibc SNe from the literature. We find significant overlap between the two samples, suggesting that GRB/XRF-associated SNe are not necessarily more luminous and do not necessarily produce more 56Ni than local SNe. Based on the current (limited) data sets, we find that the two samples may share a similar 56Ni production mechanism.",

author = "Soderberg, {A. M.} and Kulkarni, {S. R.} and Price, {P. A.} and Fox, {D. B.} and E. Berger and Moon, {D. S.} and Cenko, {S. B.} and A. Gal-Yam and Frail, {D. A.} and Chevalier, {R. A.} and L. Cowie and {Da Costa}, {G. S.} and A. MacFadyen and Mccarthy, {P. J.} and N. Noel and Park, {H. S.} and Peterson, {B. A.} and Phillips, {M. M.} and M. Rauch and A. Rest and J. Rich and K. Roth and M. Roth and Schmidt, {B. P.} and Smith, {R. C.} and Wood, {P. R.}",

year = "2006",

month = jan,

day = "1",

doi = "10.1086/498009",

language = "English (US)",

volume = "636",

pages = "391--399",

journal = "Astrophysical Journal",

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Soderberg, AM, Kulkarni, SR, Price, PA, Fox, DB, Berger, E, Moon, DS, Cenko, SB, Gal-Yam, A, Frail, DA, Chevalier, RA, Cowie, L, Da Costa, GS, MacFadyen, A, Mccarthy, PJ, Noel, N, Park, HS, Peterson, BA, Phillips, MM, Rauch, M, Rest, A, Rich, J, Roth, K, Roth, M, Schmidt, BP, Smith, RC & Wood, PR 2006, 'An HST study of the supernovae accompanying GRB 040924 and GRB 041006', Astrophysical Journal, vol. 636, no. 1 I, pp. 391-399. https://doi.org/10.1086/498009

TY - JOUR

T1 - An HST study of the supernovae accompanying GRB 040924 and GRB 041006

AU - Soderberg, A. M.

AU - Kulkarni, S. R.

AU - Price, P. A.

AU - Fox, D. B.

AU - Berger, E.

AU - Moon, D. S.

AU - Cenko, S. B.

AU - Gal-Yam, A.

AU - Frail, D. A.

AU - Chevalier, R. A.

AU - Cowie, L.

AU - Da Costa, G. S.

AU - MacFadyen, A.

AU - Mccarthy, P. J.

AU - Noel, N.

AU - Park, H. S.

AU - Peterson, B. A.

AU - Phillips, M. M.

AU - Rauch, M.

AU - Rest, A.

AU - Rich, J.

AU - Roth, K.

AU - Roth, M.

AU - Schmidt, B. P.

AU - Smith, R. C.

AU - Wood, P. R.

PY - 2006/1/1

Y1 - 2006/1/1

N2 - We present the results from a Hubble Space Telescope ACS study of the supernovae (SNe) associated with gamma-ray bursts (GRBs) 040924 (z = 0.86) and 041006 (z = 0.71). We find evidence that both GRBs were associated with an SN 1998bw-like supernova dimmed by ∼ 1.5 and ∼0.3 mag, respectively, making GRB 040924 the faintest GRB-associated SN ever detected. We study the luminosity dispersion in GRB/XRF-associated SNe and compare to local Type Ibc SNe from the literature. We find significant overlap between the two samples, suggesting that GRB/XRF-associated SNe are not necessarily more luminous and do not necessarily produce more 56Ni than local SNe. Based on the current (limited) data sets, we find that the two samples may share a similar 56Ni production mechanism.

AB - We present the results from a Hubble Space Telescope ACS study of the supernovae (SNe) associated with gamma-ray bursts (GRBs) 040924 (z = 0.86) and 041006 (z = 0.71). We find evidence that both GRBs were associated with an SN 1998bw-like supernova dimmed by ∼ 1.5 and ∼0.3 mag, respectively, making GRB 040924 the faintest GRB-associated SN ever detected. We study the luminosity dispersion in GRB/XRF-associated SNe and compare to local Type Ibc SNe from the literature. We find significant overlap between the two samples, suggesting that GRB/XRF-associated SNe are not necessarily more luminous and do not necessarily produce more 56Ni than local SNe. Based on the current (limited) data sets, we find that the two samples may share a similar 56Ni production mechanism.

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U2 - 10.1086/498009

DO - 10.1086/498009

M3 - Article

AN - SCOPUS:33644509604

SN - 0004-637X

VL - 636

SP - 391

EP - 399

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1 I

ER -

An HST study of the supernovae accompanying GRB 040924 and GRB 041006

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