A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

Journal: The Astrophysical Journal Letters

Published: 2018-02-23

DOI: 10.3847/2041-8213/aaad64

Affiliations: 21

Authors: 28

Go to article
Institutions FC
Harvard-Smithsonian Center for Astrophysics (CfA), United States of America (USA) 0.29
INAF - Astronomical Observatory of Teramo (OACTe), Italy 0.07
Warwick Department of Physics, United Kingdom (UK) 0.07
Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), NU, United States of America (USA) 0.07
INAF - Astronomical Observatory of Brera (OAB) - Merate, Italy 0.07
Astrophysical Institute, Ohio, United States of America (USA) 0.04
Dark Cosmology Centre (DARK), NBI UCPH, Denmark 0.04
INAF - Astronomical Observatory of Capodimonte, Italy 0.04
Space Telescope Science Institute (STScI), United States of America (USA) 0.04
Institute of Astrophysics of Andalusia (IAA), CSIC, Spain 0.04
Utah Valley University (UVU), United States of America (USA) 0.04
INAF - Astronomical Observatory of Rome (OAR), Italy 0.04
Department of Physics and Astronomy, University of Leicester, United Kingdom (UK) 0.04
Institute of Gravitational Wave Astronomy, UB, United Kingdom (UK) 0.04
Enrico Fermi Institute (EFI), UChicago, United States of America (USA) 0.02
INFN Gran Sasso National Laboratory (LNGS), Italy 0.02
Gran Sasso Science Institute (GSSI), Italy 0.02
Gemini Observatory Southern Operations Center, Chile 0.02
NRC Herzberg Astronomy and Astrophysics Research Centre (NRC Herzberg), Canada 0.02
Department of Physics, UChicago, United States of America (USA) 0.01

Return