A Globular Cluster Luminosity Function Distance to NGC 4993 Hosting a Binary Neutron Star Merger GW170817/GRB 170817A
A kilonova as the electromagnetic counterpart to a gravitational-wave source
Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
Distance and Properties of NGC 4993 as the Host Galaxy of the Gravitational-wave Source GW170817
Electromagnetic evidence that SSS17a is the result of a binary neutron star merger
Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993
Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
Illuminating gravitational waves: A concordant picture of photons from a neutron star merger
Investigating the Observational Properties of Type Ib Supernova SN 2017iro
NGC 4993, the shell galaxy host of GW170817: constraints on the recent galactic merger
Spatially Resolved Properties of the GW170817 Host Galaxy
Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
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 Environment of the Binary Neutron Star Merger GW170817
The impact of satellite trails on Hubble Space Telescope observations
The Old Host-galaxy Environment of SSS17a, the First Electromagnetic Counterpart to a Gravitational-wave Source
Instrument
ACS, ACS/WFC
Temporal Coverage
2016-10-05T04:37:18Z/2018-03-25T23:18:31Z
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.
