Optical Emission from Luminous and Very Soft X-Ray Sources in Nearby Galaxies: Testing the Scenario of Edge-on Supercritical Accretion Systems
SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova
SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS
The impact of satellite trails on Hubble Space Telescope observations
The progenitor star of SN 2023ixf: a massive red supergiant with enhanced, episodic pre-supernova mass loss
The SN 2023ixf Progenitor in M101. II. Properties
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2014-01-09T18:39:06Z/2014-10-18T18:34:13Z
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, Blair et al., 2015, 'Discovering and Characterizing the Young Supernova Remnant Population in M101', 1.0, European Space Agency, https://doi.org/10.5270/esa-gbox66p
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.