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An HST Study of the Supernovae Accompanying GRB 040924 and GRB 041006

, , , , , , , , , , , , , , , , , , , , , , , , , and

© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
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Author affiliations

1 Division of Physics, Mathematics, and Astronomy, 105-24, California Institute of Technology, Pasadena, CA 91125

2 University of Hawaii, Institute of Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822-1897

3 Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101

4 Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544

5 Hubble Fellow

6 Space Radiation Laboratory 220-47, California Institute of Technology, Pasadena, CA 91125

7 Robert A. Millikan Fellow

8 National Radio Astronomy Observatory, Socorro, NM 87801

9 Department of Astronomy, University of Virginia, P.O. Box 3818, Charlottesville, VA 22903-0818

10 Research School of Astronomy and Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia

11 Instituto de Astrofisica de Canarias, C/Via Lactea s/n, E-38200, La Laguna, Tenerife, Spain

12 Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, CA 94550

13 Cerro Tololo Inter-American Observatory, Casilla 603, La Serena, Chile

14 Gemini Observatory, 670 North A'ohoku Place, Hilo, HI 96720

Dates

Received 2005 April 18
Accepted 2005 September 12

Citation

A. M. Soderberg et al 2006 ApJ 636 391

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DOI

https://doi.org/10.1086/498009

Keywords

gamma rays: bursts; radiation mechanisms: non-thermal; supernovae: general

Journal RSS feed

0004-637X/636/1/391

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.

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