2010MNRAS.404..963K


C.D.S. - SIMBAD4 rel 1.7 - 2020.10.21CEST14:28:21

2010MNRAS.404..963K - Mon. Not. R. Astron. Soc., 404, 963-974 (2010/May-2)

Limits on radioactive powered emission associated with a short-hard GRB 070724A in a star-forming galaxy.

KOCEVSKI D., THONE C.C., RAMIREZ-RUIZ E., BLOOM J.S., GRANOT J., BUTLER N.R., PERLEY D.A., MODJAZ M., LEE W.H., COBB B.E., LEVAN A.J., TANVIR N. and COVINO S.

Abstract (from CDS):

We present results of an extensive observing campaign of the short-duration, hard spectrum gamma-ray burst (GRB) 070724A, aimed at detecting the radioactively powered emission that might follow from a binary merger or collapse involving compact objects. Our multiband observations span the range in time over which this so-called Li-Paczy{nacute}ski mini-supernova (mini-SN) could be active, beginning within 3 h of the GRB trigger and represent some of the deepest and most comprehensive searches for such emission. We find no evidence for such activity and place limits on the abundances and the lifetimes of the possible radioactive nuclides that could form in the rapid decompression of nuclear density matter. Furthermore, our limits are significantly fainter than the peak magnitude of any previously detected broad-lined Type Ic SN associated with other GRBs, effectively ruling out a long GRB-like SN for this event. Given the unambiguous redshift of the host galaxy (z = 0.456), GRB 070724A represents one of a small, but growing, number of short-hard GRBs for which firm physical/rest-frame quantities currently exist. The host of GRB 070724A is a moderately star-forming galaxy with an older stellar population component and a relatively high metallicity of 12 + log(O/H)KD02 = 9.1. We find no significant evidence for large amounts of extinction along the line of sight that could mask the presence of an SN explosion and estimate a small probability for chance alignment with the putative host. We discuss how our derived constraints fit into the evolving picture of short-hard GRBs, their potential progenitors and the host environments in which they are thought to be produced.

Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS

Journal keyword(s): gamma-rays: bursts

Nomenclature: Fig. 4: [KTR2010] GRB 070724A Host G N=1, [KTR2010] GN (Nos G2-G5).

Simbad objects: 30

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Number of rows : 30

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 495 1
2 GRB 070724A gB 01 51 14.08 -18 35 38.8           ~ 148 0
3 [KTR2010] GRB 070724A Host G G 01 51 14.08 -18 35 38.8           ~ 1 0
4 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 834 1
5 GRB 070714B gB 03 51 22.30 +28 17 51.3           ~ 170 1
6 GRB 071227 gB 03 52 31.09 -55 59 03.3           ~ 146 0
7 GRB 060313 gB 04 26 28.180 -10 50 37.95 20.55 21.03 19.66     ~ 131 0
8 GRB 061006 gB 07 24 07.660 -79 11 55.10           ~ 163 1
9 GRB 060121 gB 09 09 51.930 +45 39 45.41           ~ 112 1
10 GRB 061210 gB 09 38 05.270 +15 37 17.30           ~ 114 0
11 GRB 061217 gB 10 41 39.320 -21 07 22.11           ~ 107 0
12 GRB 050509B gB 12 36 18.000 +29 01 24.00           ~ 278 1
13 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 568 1
14 GRB 070809 gB 13 35 04.2 -22 07 07           ~ 113 0
15 GRB 060801 gB 14 12 01.290 +16 58 54.00           ~ 137 0
16 GRB 050813 gB 16 07 57.190 +11 14 57.80           ~ 122 1
17 GRB 050724 gB 16 24 44.400 -27 32 27.90     19.70     ~ 386 1
18 GRB 070707 gB 17 50 58.49 -68 55 27.0           ~ 52 1
19 GRB 060502B gB 18 35 46.060 +52 37 51.45           ~ 121 1
20 GRB 080503 gB 19 06 28.74 +68 47 35.8           ~ 127 0
21 GRB 080905A gB 19 10 39.10 -18 51 55.4           ~ 138 0
22 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1658 2
23 GRB 070429B gB 21 52 03.820 -38 49 42.20           ~ 95 0
24 GRB 051221 gB 21 54 48.626 +16 53 27.16 19.49         ~ 309 1
25 GRB 061201 gB 22 08 32.060 -74 34 47.90           ~ 156 0
26 BD+17 4708 SB* 22 11 31.3751899315 +18 05 34.158392398 9.73 9.91 9.46 9.03 8.70 sdF8 538 0
27 GRB 090510 gB 22 14 12.60 -26 35 51.1           ~ 412 1
28 LP 877-23 PM* 22 52 41.0353308036 -20 35 32.995847106   13.02 11.90     ~ 104 0
29 GRB 050709 gB 23 01 26.960 -38 58 39.50           ~ 260 1
30 Feige 110 HS* 23 19 58.3995050606 -05 09 56.170282845 10.360 11.45 11.50 11.970 12.145 sdO8VIIIHe5 559 1

    Equat.    Gal    SGal    Ecl

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2020.10.21-14:28:21

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