SIMBAD references

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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