GCN Circular 289
Subject
GRB 970228: Redshift and properties of the host galaxy
Date
1999-05-03T18:05:33Z (26 years ago)
From
George Djorgovski at Caltech/Palomar <george@oracle.caltech.edu>
GRB 970228: Redshift and properties of the host galaxy
S. G. Djorgovski, S. R. Kulkarni, J. S. Bloom (Caltech), and D. A. Frail
(NRAO) report on behalf of the Caltech-CARA-NRAO GRB Collaboration:
Spectra of the host galaxy of GRB 970228 were obtained in the course of
several runs at the Keck-II 10-m telescope. A prominent emission line at
6319 A was observed in at least 3 independent data sets, along with a very
blue continuum, showing no apparent breaks between about 4000 and 8900 A.
We interpret this emission line as [O II] 3727 at z = 0.695 +- 0.002.
Moreover, possible emission lines are detected corresponding to [Ne III]
3869 and [O III] 5007 at the same redshift. We thus consider this redshift
to be practically secure.
Assuming a cosmology with H_0 = 65 km/s/Mpc, Omega_0 = 0.2, and Lambda_0 = 0,
we derive the luminosity distance of 1.28 e28 cm. The measured fluence from
Ulysses (cf. Hurley et al. 1997, ApJ, 485, L1) of 4.3 e-6 erg/cm2 then implies
E(gamma,isotropic) = 5.2 e51 erg.
We detect continuum flux in the V band of about 0.12 uJy, uncertain by at
least 20%. This is in an excellent agreement with the published ground-based
and HST photometry, corresponding to V ~ 26 mag.
The [O II] line has the equivalent width 75 +- 15 A (observed), or 44 +- 9 A
(restframe), typical for star-forming galaxies at comparable redshifts. The
very blue continuum suggests little restframe extinction in this galaxy.
In the following estimates, we assume a Galactic extinction correction A(V) =
0.75 mag. From the [O II] line flux, we estimate SFR = 0.47 Msun/yr, and from
the continuum power at 2800 A (rest), SFR = 0.35 Msun/yr. Both of these are
uncertain by at least 30%. The absolute restframe B band luminosity of the
galaxy corresponds to about 0.05 to 0.1 L_* today. Thus, neither the SFR
nor the SFR per unit mass are especially high.
This note can be cited.
[GCN OPERATOR'S NOTE (04 May 99): This archived copy was corrected
for the mistaken citation that BATSE yielded the fluence. The true
source of the fluence for the burst came from Ulysses.]