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
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
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
The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
The Environment of the Binary Neutron Star Merger GW170817
The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
Instrument
WFC3/IR
Temporal Coverage
2017-08-22T07:34:17Z/2017-08-26T23:30:32Z
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.
European Space Agency, Levan comma Andrew James, 2018, 'Rapid ToO observations of the first gravitational wave counterparts', 1.0, European Space Agency, https://doi.org/10.5270/esa-ec0mzvr