A dataset provided by the European Space Agency

Name 15329
Title Fine-Tuned Search for Kilonova Emission in a Short Gamma-Ray Burst: Implications for the Progenitors, Advanced LIGO, and r-Process Nucleosynthesis
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=15329;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-x3vu505
Author Berger, Edo
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15329&mission=hst
Publication
  • A Decline in the X-Ray through Radio Emission from GW170817 Continues to Support an Off-axis Structured Jet
  • Analytic model for off-axis GRB afterglow images - geometry measurement and implications for measuring H0
  • A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
  • A Pulsar Wind Nebula Embedded in the Kilonova AT 2017gfo Associated with GW170817/GRB 170817A
  • First Multimessenger Observations of a Neutron Star Merger
  • Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
  • Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
  • Modelling the spectra of the kilonova AT2017gfo - II. Beyond the photospheric epochs
  • Multi-messenger Observations of a Binary Neutron Star Merger
  • Optical superluminal motion measurement in the neutron-star merger GW170817
  • Spatially Resolved Properties of the GW170817 Host Galaxy
  • Target-of-Opportunity Observation Detectability of Kilonovae with WFST
  • The Binary Neutron Star Event LIGO/Virgo GW170817 160 Days after Merger: Synchrotron Emission across the Electromagnetic Spectrum
  • The Broadband Counterpart of the Short GRB 200522A at z = 0.5536: A Luminous Kilonova or a Collimated Outflow with a Reverse Shock?
  • The Combined Ultraviolet, Optical, and Near-infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale
  • The evolution of the X-ray afterglow emission of GW 170817/ GRB 170817A in XMM-Newton observations
  • The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
  • The impact of satellite trails on Hubble Space Telescope observations
  • The X-ray counterpart to the gravitational-wave event GW170817
Instrument ACS/WFC, WFC3/IR, WFC3/UVIS
Temporal Coverage 2017-08-27T06:45:57Z/2018-07-20T08:56:06Z
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 2019-01-21T04:22:22Z
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, Berger et al., 2019, 'Fine-Tuned Search for Kilonova Emission in a Short Gamma-Ray Burst: Implications for the Progenitors, Advanced LIGO, and r-Process Nucleosynthesis', 1.0, European Space Agency, https://doi.org/10.5270/esa-x3vu505