Statistics and characteristics of MgII absorbers along GRB lines of sight observed with VLT-UVES

S. D. Vergani; P. Petitjean; C. Ledoux; P. Vreeswijk; A. Smette; E. J. A. Meurs

doi:10.1051/0004-6361/200911747

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Volume 503 / No 3 (September I 2009)

A&A, 503 3 (2009) 771-781

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Table 1:

GRB sample and log of UVES observations.
GRB	UT^a	$\delta t$ ^b	$t_{\rm total}$ ^c	ESO Program	PI
(yymmdd)	Swift	(hh:mm)	(h)	ID
021004	12:06:13	13:31	2.0	070.A-0599^d	Fiore
050730	19:58:23	04:09	1.7	075.A-0603	Fiore
050820A	06:34:53	00:33	1.7	075.A-0385	Vreeswijk
050922C	19:55:50	03:33	1.7	075.A-0603	Fiore
060418	03:06:08	00:10	2.6	077.D-0661	Vreeswijk
060607A	05:12:13	00:08	3.3	077.D-0661	Vreeswijk
071031	01:06:36	00:09	2.6	080.D-0526	Vreeswijk
080310	08:37:58	00:13	1.3	080.D-0526	Vreeswijk
080319B	06:12:49	00:09	2.1	080.D-0526^e	Vreeswijk
080413A	02:54:19	03:42	2.3	081.A-0856	Vreeswijk

^a UT of trigger by the BAT instrument on-board Swift. Exception:
GRB 021004, detected by WXM on-board HETE-2. ^b Time delay between the satellite trigger and the start of the first UVES exposure. ^c Total UVES exposure time including all instrument setups. ^d Also 070.D-0523 (PI: van den Heuvel). ^e Also 080.A-0398 (PI: Fiore).

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