A year in the life of GW 170817: the rise and fall of a structured jet from a binary neutron star merger
Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
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
Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
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 outflow structure of GW170817 from late-time broad-band observations
The X-ray counterpart to the gravitational-wave event GW170817
Instrument
WFC3/UVIS
Temporal Coverage
2017-08-25T13:48:51Z/2017-08-28T21:07:19Z
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, Troja comma Eleonora, 2017, 'Identify the signature of neutron star mergers through rapid Chandra/Hubble observations of a short GRB', 1.0, European Space Agency, https://doi.org/10.5270/esa-cogdqoi