[vsnet-grb-info 1860] GRB 050724: Secure Host Redshift from Keck
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Sat Jul 30 03:16:03 JST 2005
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 3700
SUBJECT: GRB 050724: Secure Host Redshift from Keck
DATE: 05/07/29 18:13:53 GMT
FROM: Jason Prochaska at UCO/Lick Obs <xavier at ucolick.org>
J. X. Prochaska (UCO/Lick), J. S. Bloom (UCB), H.-W. Chen (MIT),
B. Hansen (UCLA), J. Kalirai (UCSC), M. Rich (UCLA) and H. Richer (UBC)
report on behalf of the GRAASP collaboration:
"We have obtained LRISb spectroscopy (900s; 2005-07-29 06:31 UT)
of the putative host galaxy of GRB 050724 (Object D in GCN #3672).
We confirm our previously reported redshift (GCN #3679)
based on the identification of Ca H+K, G-band absorption features,
and the 4000Ang break. We report a redshift z=0.258 +/- 0.002.
The velocity dispersion based on CaK appears to exceed 200km/s.
The galaxy shows no [OII] emission in our spectrum suggesting minimal
current star formation.
PAIRITEL imaging of the galaxy from July 29 UT yields a K-band magnitude
of 15.3 +/- 0.2 in a 3" radius aperture. At this redshift,
and including the effects of Galactic extinction, the galaxy
is 1.7 L* based off the 2MASS luminosity function.
The properties of this galaxy -- a massive early-type at
moderate redshift -- are strikingly similar to the probable host
galaxy of GRB 050509b (GCN #3399).
Based on this redshift and the reported fluence in GCN #3667,
the isotropic -equivalent energy release is
E_gamma(iso) = 9.9e49 erg [19-440 keV, comoving], more than 1
order of magnitude brighter than 050509b
(Bloom et al. astro-ph/0505480)."
Figures and imaging can be found at this following site:
http://www.graasp.org/Data/050724
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