Constraints on the Binary Companion to the SN Ic 1994I Progenitor
Discovery of an Intermediate-luminosity Red Transient in M51 and Its Likely Dust-obscured, Infrared-variable Progenitor
The impact of satellite trails on Hubble Space Telescope observations
The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data
The transient ultraluminous X-ray source, ULX-4, in M51
The young star cluster population of M51 with LEGUS - I. A comprehensive study of cluster formation and evolution
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2014-09-11T01:54:59Z/2014-09-11T07:29:08Z
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, Van Dyk et al., 2015, 'Detecting a Hot Companion to the Progenitor of the Type Ic Supernova 1994I in M51', 1.0, European Space Agency, https://doi.org/10.5270/esa-0n5og58