2005MNRAS.362..245J


Query : 2005MNRAS.362..245J

2005MNRAS.362..245J - Mon. Not. R. Astron. Soc., 362, 245-251 (2005/September-1)

Ly+ and ultraviolet emission from high-redshift gamma-ray burst hosts: to what extent do gamma-ray bursts trace star formation ?

JAKOBSSON P., BJORNSSON G., FYNBO J.P.U., JOHANNESSON G., HJORTH J., THOMSEN B., MOLLER P., WATSON D., JENSEN B.L., OSTLIN G., GOROSABEL J. and GUDMUNDSSON E.H.

Abstract (from CDS):

We report the result of a search for Lyα emission from the host galaxies of the gamma-ray bursts (GRBs) 030226 (z= 1.986), 021004 (z= 2.335) and 020124 (z= 3.198). We find that the host galaxy of GRB 021004 is an extended (around 8 kpc) strong Lyα emitter with a rest-frame equivalent width (EW) of 68+12–11Å, and a star formation rate of 10.6 ±2.0 M☉/yr. We do not detect the hosts of GRB 030226 and GRB 020124, but the upper limits on their Lyα fluxes do not rule out large rest-frame EWs. In the fields of GRB 021004 and GRB 030226 we find seven and five other galaxies, respectively, with excess emission in the narrow-band filter. These galaxies are candidate Lyα-emitting galaxies in the environment of the host galaxies. We have also compiled a list of all z≳ 2 GRB hosts, and demonstrate that a scenario where they trace star formation in an unbiased way is compatible with current observational constraints. Fitting the z= 3 luminosity function (LF) under this assumption results in a characteristic luminosity of R*= 24.6 and a faint-end slope of α=-1.55, consistent with the LF measured for Lyman-break galaxies.

Abstract Copyright: 2005 RAS

Journal keyword(s): dust, extinction - galaxies: evolution - galaxies: formation - galaxies: high-redshift - gamma-rays: bursts

Nomenclature: Fig.2, Table 2: [JBF2005] S1004-N (Nos 1 to 7). Fig.2, Table 3: [JBF2005] S0226-N (Nos 1 to 5).

CDS comments: Standard star BD +28 not identified, incomplete format.

Simbad objects: 18

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Number of rows : 18
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 GD 71 WD* 05 52 27.6198591816 +15 53 13.228887444 11.675 12.783 13.032 13.169 13.337 DA1.5 407 0
3 GRB 000131 gB 06 13 31.08 -51 56 41.7     24.7     ~ 172 1
4 GRB 050505 gB 09 27 03.300 +30 16 23.70     20.74     ~ 206 0
5 GRB 020124 gB 09 32 50.8 -11 31 11           ~ 155 0
6 GRB 050319 gB 10 16 47.900 +43 32 53.80   18.02 17.01     ~ 274 0
7 GRB 030323 gB 11 06 09.4 -21 46 13           ~ 138 1
8 GRB 011211 gB 11 15 16 -21 56.0           ~ 305 0
9 GRB 030226 gB 11 33 04.9 +25 53 56           ~ 212 0
10 PKS J1140-2628 rG 11 40 48.35884 -26 29 08.6316     22.00     ~ 325 1
11 GRB 971214 gB 11 56 26.4 +65 12 01           ~ 445 1
12 GRB 030429 gB 12 13 07.495 -20 54 49.54     23.70     ~ 132 0
13 HZ 44 HS* 13 23 35.2629445608 +36 07 59.544140304 10.186 11.42 11.65 12.00 11.995 sdBN0VIIHe28 439 0
14 GRB 050502A gB 13 29 46.250 +42 40 27.50           ~ 65 0
15 GRB 000301C gB 16 20 18.5 +29 26 35           ~ 361 0
16 GRB 050401 gB 16 31 28.84 +02 11 14.5           ~ 348 0
17 GRB 000926 gB 17 04 15 +51 46.0           ~ 373 0
18 GRB 050315 gB 20 25 54.100 -42 36 02.19           ~ 225 0

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