A dataset provided by the European Space Agency

Name 14771
Title r-process kilonovae, short-duration GRBs, and EM counterparts to gravitational wave sources
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=14771;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-vcgdwhp
Author Tanvir, Nial Rahil
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=14771&mission=hst
Publication
  • 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 year in the life of GW 170817: the rise and fall of a structured jet from a binary neutron star merger
  • Constraints on the ejecta of the GW170817 neutron star merger from its electromagnetic emission
  • Constraints on the presence of platinum and gold in the spectra of the kilonova AT2017gfo
  • Gamma-Ray Burst Afterglows in the Multimessenger Era: Numerical Models and Closure Relations
  • 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
  • Late-time Kilonova Light Curves and Implications to GW170817
  • Modelling the spectra of the kilonova AT2017gfo - II: Beyond the photospheric epochs
  • 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
  • Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
  • Properties of jet and surrounding material of GW/GRB 170817A
  • Spatially Resolved Properties of the GW170817 Host Galaxy
  • The Diversity of Kilonova Emission in Short Gamma-Ray Bursts
  • The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
  • The Environment of the Binary Neutron Star Merger GW170817
  • 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 Optical Afterglow of GW170817 at One Year Post-merger
  • The outflow structure of GW170817 from late-time broad-band observations
  • The X-ray counterpart to the gravitational-wave event GW170817
  • Transition Probabilities of Near-infrared Ce III Lines from Stellar Spectra: Applications to Kilonovae
Instrument WFC3/IR, WFC3/UVIS
Temporal Coverage 2017-08-28T01:50:09Z/2018-08-08T12:16:12Z
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 2018-11-08T20:47:17Z
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, Tanvir et al., 2018, 'r-process kilonovae, short-duration GRBs, and EM counterparts to gravitational wave sources', 1.0, European Space Agency, https://doi.org/10.5270/esa-vcgdwhp