A UV census of the environments of stripped-envelope supernovae
New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra
Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions
The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge
The changing-type SN 2014C may come from an 11-M star stripped by binary interaction and violent eruption
The interacting nature of dwarf galaxies hosting superluminous supernovae
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2016-11-13T21:06:42Z/2018-05-03T01:02:15Z
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, Maund et al., 2018, 'A UV census of the sites of core-collapse supernovae', 1.0, European Space Agency, https://doi.org/10.5270/esa-g7dbf5n