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Fundamental Properties of GRB-Selected Galaxies: A Swift/VLT Legacy Survey Palli Jakobsson Centre for Astrophysics Research (University of Hertfordshire)
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Main Collaborators Jens Hjorth (DARK, NBI) [PI] Johan Fynbo (DARK, NBI) Javier Gorosabel (IAA-CSIC, Granada) Nial Tanvir (CAR, Herts) Andrew Levan (CAR, Herts) Paul Vreeswijk (ESO) Rhaana Starling (Amsterdam) Gulli Björnsson (Science Institute, Reykjavík) Cedric Ledoux (ESO) Evert Rol (Leicester) Andreas Jaunsen (Oslo)
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Concrete Goals (LP: 272 hours) Identify the GRB hosts: R = 27 and K = 21.5 [17]. Measure redshifts for GRBs without absorption redshifts [4]. Search for the Ly α line when possible [7]. Determine the dust reddening within hosts. Detailed studies (spectroscopy) of particularly interesting targets: short GRB hosts [3] and bright hosts [1]. Determine the luminosity function.
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Redshift Distribution of Swift GRBs Jakobsson et al. (2006)
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Sample Definition GRBs detected by Swift after 1 March 2005, when it was fully operational and automatically slewing. An X-ray position is available obtained by the Swift XRT detector. The Galactic extinction is less than A V < 0.5. Declination favorable for VLT (< +25º).
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LF: GRB Hosts vs. LBGs (z ~ 3) Blue: GRB hosts Black: LBGs R* LBGs: 24.54 -1.57 Hosts: 24.60 -1.55 Jakobsson et al. (2005) ULIRGs ??? < 30% ???
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LF: GRB Hosts vs. LBGs (z ~ 3) 36 detections (24 < R < 28) 10 upper limits (R > 28) 8 detections 7 upper limits
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GRB 050315 R = 24.6
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GRB 050318
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GRB 030429 A galaxy only 1.2” away from the OA initially considered to be a probable host galaxy. VLT spectroscopy soon showed: z GRB = 2.66 z galaxy = 0.84
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GRB 050318
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GRB 050401 R = 25.7
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GRB 050406
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GRB 050412 R ~ 27 (β OX < 0.05)
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GRB 050416A R = 23.1 XRF Short? Cluster
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GRB 050502B
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GRB 050603 R = 26.1
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GRB 050714B X-ray lines: z ~ 2.5 ??
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GRB 050726 R = 25.3
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GRB 050730 R = 26.9
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GRB 050801 R = 26.3
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GRB 050820A R = 24.7
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GRB 050822 R = 24.1 X-ray lines: z ~ 2.5 ??
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GRB 050915A R = 24.5
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GRB 050922C
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GRB 051006
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GRB 051016B R = 22.6
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GRB 051117B R = 24.1
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LF: GRB Hosts vs. LBGs (z ~ 3)
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Mosaic
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