2019MNRAS.485.5294P

Query : 2019MNRAS.485.5294P

2019MNRAS.485.5294P - Mon. Not. R. Astron. Soc., 485, 5294-5318 (2019/June-1)

A multiwavelength analysis of a collection of short-duration GRBs observed between 2012 and 2015.

PANDEY S.B., HU Y., CASTRO-TIRADO A.J., POZANENKO A.S., SANCHEZ-RAMIREZ R., GOROSABEL J., GUZIY S., JELINEK M., TELLO J.C., JEONG S., OATES S.R., ZHANG B.-B., MAZAEVA E.D., VOLNOVA A.A., MINAEV P.Y., VAN EERTEN H.J., CABALLERO-GARCIA M.D., PEREZ-RAMIREZ D., BREMER M., WINTERS J.-M., PARK I.H., NICUESA GUELBENZU A., KLOSE S., MOSKVITIN A., SOKOLOV V.V., SONBAS E., AYALA A., CEPA J., BUTLER N., TROJA E., CHERNENKO A.M., MOLKOV S.V., VOLVACH A.E., INASARIDZE R.Y., EGAMBERDIYEV S.A., BURKHONOV O., REVA I.V., POLYAKOV K.A., MATKIN A.A., IVANOV A.L., MOLOTOV I., GUVER T., WATSON A.M., KUTYREV A., LEE W.H., FOX O., LITTLEJOHNS O., CUCCHIARA A., GONZALEZ J., RICHER M.G., ROMAN-ZUNIGA C.G., TANVIR N.R., BLOOM J.S., PROCHASKA J.X., GEHRELS N., MOSELEY H., DE DIEGO J.A., RAMIREZ-RUIZ E., KLUNKO E.V., FAN Y., ZHAO X., BAI J., WANG C., XIN Y., CUI C., TUNGALAG N., PENG Z.-K., KUMAR A., GUPTA R., ARYAN A., KUMAR B., VOLVACH L.N., LAMB G.P. and VALEEV A.F.

Abstract (from CDS):

We investigate the prompt emission and the afterglow properties of short-duration gamma-ray burst (sGRB) 130603B and another eight sGRB events during 2012-2015, observed by several multiwavelength facilities including the Gran Canarias Telescope 10.4 m telescope. Prompt emission high energy data of the events were obtained by INTEGRAL-SPI-ACS, Swift-BAT, and Fermi-GBM satellites. The prompt emission data by INTEGRAL in the energy range of 0.1-10 MeV for sGRB 130603B, sGRB 140606A, sGRB 140930B, sGRB 141212A, and sGRB 151228A do not show any signature of the extended emission or precursor activity and their spectral and temporal properties are similar to those seen in case of other short bursts. For sGRB 130603B, our new afterglow photometric data constrain the pre-jet-break temporal decay due to denser temporal coverage. For sGRB 130603B, the afterglow light curve, containing both our new and previously published photometric data is broadly consistent with the ISM afterglow model. Modeling of the host galaxies of sGRB 130603B and sGRB 141212A using the LePHARE software supports a scenario in which the environment of the burst is undergoing moderate star formation activity. From the inclusion of our late-time data for eight other sGRBs we are able to: place tight constraints on the non-detection of the afterglow, host galaxy, or any underlying 'kilonova' emission. Our late-time afterglow observations of the sGRB 170817A/GW170817 are also discussed and compared with the sub-set of sGRBs.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): gamma-rays: general - X-ray: bursts - techniques: photometric - radiation mechanims : non-thermalonova

Simbad objects: 31

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Number of rows : 31
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 140930B gB 00 25 23.40 +24 17 41.7           ~ 52 0
2 SDSS J002523.61+241727.0 * 00 25 23.6284037832 +24 17 27.126418560           ~ 1 0
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
4 GRB 080426 gB 01 45 59.79 +69 28 06.0           ~ 50 0
5 GRB 141212A G 02 36 29.9570 +18 08 47.228           ~ 70 0
6 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
7 GRB 121226A G 11 14 34.1210 -30 24 22.840           ~ 44 0
8 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0
9 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
10 Ton 599 Bla 11 59 31.83391383 +29 14 43.8268224   14.80 14.41 17.652 13.39 ~ 989 1
11 GALEX J123205.0-105600 Bz? 12 32 04.9717245480 -10 56 00.722548932         16.421 ~ 186 0
12 SDSS J123612.87+285858.8 BiC 12 36 12.8803407000 +28 58 58.780075656           ~ 328 1
13 NGC 4993 Sy2 13 09 47.6908761600 -23 23 02.314044636   13.34   11.92   ~ 397 0
14 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
15 USNO-B1.0 1275-00258743 G 13 27 01.07 +37 35 32.1           ~ 1 0
16 GRB 140606A gB 13 27 11.70 +37 35 56.5           ~ 25 0
17 USNO-B1.0 1275-00258796 G 13 27 18.97272 +37 34 06.1824           ~ 1 0
18 GRB 060801 G 14 12 01.2620 +16 58 55.970           ~ 172 0
19 GRB 151228A gB 14 16 -17.7           ~ 27 0
20 GRB 020531 gB 15 14 55.8 -19 24 54           ~ 60 0
21 NSC J155202+273349 ClG 15 52 02.14 +27 33 48.7           ~ 3 0
22 HD 142178 SB* 15 52 02.5995325392 +27 36 11.140224372       8.9   K0 12 0
23 GRB 140903A G 15 52 03.2650 +27 36 10.710           ~ 138 0
24 GRB 051105A gB 17 41 10.010 +34 55 45.16 21.26 21.20 20.33     ~ 53 0
25 Fermi bn160821937 gB 18 39 54.550 +62 23 30.35           ~ 190 0
26 GRB 080503 gB 19 06 28.74 +68 47 35.8           ~ 172 0
27 GRB 131224A gB 19 47 20.1 +31 40 04           ~ 12 0
28 EM* MWC 349 ** 20 32 45.499080 +40 39 36.74124   15.88 13.15 12.13   Bep 837 0
29 GRB 140622A gB 21 08 41.56 -14 25 09.5           ~ 61 0
30 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
31 NVSS J230126-385839 rG 23 01 26.7650 -38 58 40.422   22.22 21.22 21   ~ 325 1

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