A dataset provided by the European Space Agency

Name 14353
Title The Astrophysics of the Most Energetic Gamma-Ray Bursts
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14353;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-9378amm
Author Fruchter, Andrew S.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14353&mission=hst
Publication
  • A Radio-selected Population of Dark, Long Gamma-Ray Bursts: Comparison to the Long Gamma-Ray Burst Population and Implications for Host Dust Distributions
  • The impact of satellite trails on Hubble Space Telescope observations
  • The Late-time Afterglow Evolution of Long Gamma-Ray Bursts GRB 160625B and GRB 160509A
  • The Late-time Radio Behavior of Gamma-ray Burst Afterglows: Testing the Standard Model
Instrument WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage 2016-06-13T17:02:08Z/2017-11-11T13:21:09Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2018-11-12T09:57:04Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Fruchter et al., 2018, 'The Astrophysics of the Most Energetic Gamma-Ray Bursts', 1.0, European Space Agency, https://doi.org/10.5270/esa-9378amm