2005ApJ...627..877S


Query : 2005ApJ...627..877S

2005ApJ...627..877S - Astrophys. J., 627, 877-887 (2005/July-2)

An HST search for supernovae accompanying X-ray flashes.

SODERBERG A.M., KULKARNI S.R., FOX D.B., BERGER E., PRICE P.A., CENKO S.B., HOWELL D.A., GAL-YAM A., LEONARD D.C., FRAIL D.A., MOON D., CHEVALIER R.A., HAMUY M., HURLEY K.C., KELSON D., KOVIAK K., KRZEMINSKI W., KUMAR P., MacFADYEN A., McCARTHY P.J., PARK H.S., PETERSON B.A., PHILLIPS M.M., RAUCH M., ROTH M., SCHMIDT B.P. and SHECTMAN S.

Abstract (from CDS):

We present the results from a Hubble Space Telescope ACS search for supernovae associated with X-ray flashes 020903, 040701, 040812, and 040916. We find strong evidence that XRF 020903 (z=0.25) was associated with a SN 1998bw-like supernova and confirm this using optical spectroscopy at t∼25 days. We find no evidence, however, for SN 1998bw-like supernovae associated with the other three events. In the case of XRF 040701 (z=0.21), we rule out even a faint supernova similar to SN 2002ap, using template light curves for several local Type Ic supernovae. For the two cases in which the redshift is not known, XRFs 040812 and 040916, we derive robust redshift limits, assuming that they were accompanied by supernovae similar to SN 1998bw, and compare these limits with photometric redshift constraints provided by their host galaxies. We supplement this analysis with results for three additional events (XRFs 011030, 020427, and 030723) and discuss the observed diversity of supernovae associated with X-ray flashes and gamma-ray bursts. We conclude that XRF-SNe exist but can be significantly fainter than SN 1998bw, possibly consistent with the observed spread in local Type Ibc supernovae.

Abstract Copyright:

Journal keyword(s): Gamma Rays: Bursts - Radiation Mechanisms: Nonthermal - X-Rays: Bursts

Simbad objects: 32

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Number of rows : 32
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 197 2
2 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 563 1
3 GRB 000911 gB 02 18 42 +07 48.0           ~ 156 0
4 SN 1984L SN* 02 35 30.54 -07 09 30.3   14.0       SNIb 194 1
5 SN 1983V SN* 03 33 31.63 -36 08 55.0   14.67       SNIc 97 1
6 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 638 1
7 SN 1997ef SN* 07 57 02.87 +49 33 41.3     16.5     SNIc-BL 270 1
8 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 548 0
9 SN 2002lt SN* 08 08 59.858 +06 43 37.52           SNIc: 352 1
10 SN 1987M SN* 09 08 06 +78 05.4   15.3       SNIc 126 1
11 SN 1999as SN* 09 16 30.86 +13 39 02.2     18.3     SNIcpec 52 1
12 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1208 1
13 SN 2003L SN* 11 03 12.33 +11 04 38.3     16.9     SNIc 72 1
14 GRB 011121 gB 11 34 26.67 -76 01 41.6       23.0   ~ 275 1
15 SN 1990B SN* 12 36 33.86 +11 14 29.9     15.75     SNIc 127 1
16 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 625 1
17 SN 1983N SN* 13 36 51.23 -29 54 01.7   11.7       SNIb 273 1
18 SN 1991D SN* 13 41 13.58 -14 38 47.6     16.4     SNIb 32 1
19 GRB 020405 gB 13 58 03.12 -31 22 22.2   21.9 21.5     ~ 249 1
20 GRB 040812 gB 16 26 08.5 -44 41 04           ~ 29 0
21 GRB 991208 gB 16 33 53.51 +46 27 21.5           ~ 260 1
22 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1821 2
23 ESO 184-82 AG? 19 35 04.416 -52 50 38.04   15.17   14.26   ~ 108 2
24 GRB 011030 gB 20 43 35.4 +77 17 20           ~ 75 0
25 GRB 040701 G 20 47 46.3 -40 14 13           ~ 44 1
26 GRB 020427 gB 22 09 28.3 -65 19 32           ~ 49 0
27 SN 1999ex SN* 22 16 07.27 -36 50 53.7   17.35       SNIb 141 2
28 GRB 990712 gB 22 31 53.061 -73 24 28.58           ~ 262 1
29 GRB 020903 gB 22 48 42.34 -20 46 09.3           ~ 234 1
30 GRB 040916 gB 23 00 55.1 -05 38 43           ~ 35 0
31 SN 1992ar SN* 23 17 28.40 -44 38 53.8   20.70       SNIc 30 1
32 GRB 980703 gB 23 59 06.7 +08 35 07           ~ 445 1

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