2006ApJ...636..391S

Query : 2006ApJ...636..391S

2006ApJ...636..391S - Astrophys. J., 636, 391-399 (2006/January-1)

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

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., REST A., RICH J., ROTH K., ROTH M., SCHMIDT B.P., SMITH R.C. and WOOD P.R.

Abstract (from CDS):

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.

Abstract Copyright: ∼

Journal keyword(s): Gamma Rays: Bursts - Radiation Mechanisms: Nonthermal - Stars: Supernovae: General

Nomenclature: Text:[SKP2006] GRB 041006 Host G.

Simbad objects: 33

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Number of rows : 33
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 021004 gB 00 26 54.68 +18 55 41.6           ~ 560 0
2 [SKP2006] GRB 041006 Host G G 00 54 50.17 +01 14 07.0           ~ 5 0
3 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 202 2
4 OT 20041006 ? 00 54 50.17 +01 14 07.0           ~ 2 0
5 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 587 1
6 GRB 040924 gB 02 06 22.52 +16 08 48.8           ~ 169 1
7 GRB 000911 gB 02 18 42 +07 48.0           ~ 163 0
8 SN 1984L SN* 02 35 30.54 -07 09 30.3   14.0       SNIb 197 1
9 SN 1983V SN* 03 33 31.63 -36 08 55.0   14.67       SNIc 102 1
10 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 650 1
11 SN 1997ef SN* 07 57 02.87 +49 33 41.3     16.5     SNIc-BL 281 1
12 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 576 0
13 SN 2002lt SN* 08 08 59.858 +06 43 37.52           SNIc: 363 1
14 SN 1987M SN* 09 08 06 +78 05.4   15.3       SNIc 131 1
15 SN 1999as SN* 09 16 30.86 +13 39 02.2     18.3     SNIcpec 55 1
16 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
17 SN 2003L SN* 11 03 12.33 +11 04 38.3     16.9     SNIc 77 1
18 GRB 011121 gB 11 34 26.67 -76 01 41.6       23.0   ~ 286 1
19 SN 1990B SN* 12 36 33.86 +11 14 29.9     15.75     SNIc 131 1
20 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 645 1
21 SN 1983N SN* 13 36 51.23 -29 54 01.7   11.7       SNIb 278 1
22 SN 1991D SN* 13 41 13.58 -14 38 47.6     16.4     SNIb 35 1
23 GRB 020405 gB 13 58 03.12 -31 22 22.2   21.9 21.5     ~ 259 1
24 GRB 991208 gB 16 33 53.51 +46 27 21.5           ~ 269 1
25 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
26 GRB 040701 G 20 47 46.3 -40 14 13           ~ 45 1
27 SN 1999ex SN* 22 16 07.27 -36 50 53.7   17.35       SNIb 149 2
28 GRB 990712 gB 22 31 53.061 -73 24 28.58           ~ 268 1
29 GRB 020903 gB 22 48 42.34 -20 46 09.3           ~ 248 1
30 GRB 010921 gB 22 55 59.90 +40 55 52.9           ~ 173 1
31 GRB 040916 gB 23 00 55.1 -05 38 43           ~ 35 0
32 SN 1992ar SN* 23 17 28.40 -44 38 53.8   20.70       SNIc 30 1
33 GRB 980703 gB 23 59 06.7 +08 35 07           ~ 453 1

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