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NOAO > Observing Info > Approved Programs > 2012A-0198 |
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PI: Bethany Cobb, The George Washington University, bcobb@gwu.edu
Address: Department of Physics, The George Washington University, Corcoran 105, 725 21st St, NW, Washington, DC 20052, USA, USA
CoI: Antonino Cucchiara, UCO/Lick Observatory
CoI: Nial Tanvir, University of Leicester, Department of Physics and Astronomy, University Road, Leicester LE1 7RH, United Kingdom
CoI: Derek Fox, Pennsylvania State University
CoI: Edo Berger, Harvard-Smithsonian Center for Astrophysics
CoI: Joshua Bloom, UC Berkeley (Astronomy)
CoI: Brad Cenko, UC Berkeley (Astronomy)
CoI: Daniel Perley, Caltech
CoI: Andrew Fruchter, Space Telescope Science Institute
CoI: Andrew Levan, University of Warwick
CoI: David Bersier, Liverpool John Moores University
CoI: Brian Schmidt, Australian National University
CoI: Andrew Bunker, Oxford
CoI: Hsiao-Wen Chen, University of Chicago
CoI: Wen-Fai Fong, Harvard-Smithsonian Center for Astrophysics
CoI: Ryan Chornock, Harvard-Smithsonian Center for Astrophysics
CoI: Kathy Roth, Gemini Observatory
CoI: Jochen Greiner, Max-Planck-Institute for Extraterrestrial Physics
CoI: Laskar Tanmoy, Harvard-Smithsonian Center for Astrophysics
CoI: Nat Butler, UC Berkeley (Astronomy)
CoI: Adam Morgan, UC Berkeley (Astronomy)
CoI: Paul O'Brien, University of Leicester
CoI: Sebastian Lopez, Universidad de Chile
CoI: Max Pettini, Institute of Astronomy, University of Cambridge
CoI: Jason X Prochaska, UC Santa Cruz
CoI: Enrico Ramirez-Ruiz, UC Santa Cruz
CoI: Rhaana Starling, University of Leicester,
CoI: Klaas Wiersema, University of Leicester
CoI: Bryan Penprase, Pomona College
CoI: Thomas de Jaeger, Universidad de Chile
CoI: Maria Jose Maureira, Yale University
CoI: Nicholas Tejos, Durham University
CoI: Arne Rau, Max-Planck-Institute for Extraterrestrial Physics
CoI: John Graham, Space Telescope Science Institute
CoI: Jens Hjorth, NBI: DARK, Copenhagen
CoI: Palle Jakobsson, University of Iceland
CoI: Karl Glazebrook, Swinburne University of Technology
CoI: Sharon Rapoport, Australian National University
Title: Late-time Observations of Exceptional Swift and Fermi GRBs: Gemini South Standard Targets of Opportunity
Abstract:
We propose to make late-time observations of gamma-ray burst (GRB) afterglows
initially observed under our companion "Rapid TOO" Gemini program. Science
goals for "Standard TOO" observations include: (1) low-redshift GRBs, to
exploring the diversity of GRB-SNe; (2) high-redshift GRBs, which are
providing a unique perspective on z>5 star formation and reionization; (3)
short-duration bursts, which are likely connected to compact object mergers;
and (4) Fermi-LAT bursts, which include the most luminous and relativistic
GRBs. Late-time observations are required to fully characterize these bursts,
for example, by constraining burst explosion geometry and total energy
through the detection of jet breaks. Even as a mature mission, Swift
continues to supply unexpected discoveries, as does the younger Fermi
mission. Gemini forms the cornerstone of our follow-up effort; its
capabilities are essential for capitalizing on the remaining years of the
Swift mission. Our merged global collaboration aims to secure Swift's legacy
by focusing on the extreme and rare GRBs that hold the greatest potential as
unique probes of the early universe and stellar death. We emphasise that our
long-running campaign at Gemini has been very successful, allowing us to
respond flexibly to rare GRB events: late-time observations have been a
critical component of this.
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360
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NOAO > Observing Info > Approved Programs > 2012A-0198 |
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