A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae
An Extensive Hubble Space Telescope Study of the Offset and Host Light Distributions of Type I Superluminous Supernovae
A population of luminous accreting black holes with hidden mergers
A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies
Host-galaxy Properties of 32 Low-redshift Superluminous Supernovae from the Palomar Transient Factory
Obscured Star Formation in the Host Galaxies of Superluminous Supernovae
The impact of satellite trails on Hubble Space Telescope observations
The interacting nature of dwarf galaxies hosting superluminous supernovae
What powers the 3000-day light curve of SN 2006gy?
Zooming In on the Progenitors of Superluminous Supernovae With the HST
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-11-07T17:25:38Z/2013-12-02T03:41:31Z
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 et al., 2014, 'Unveiling the progenitors of the most luminous supernovae', 1.0, European Space Agency, https://doi.org/10.5270/esa-0g7g4mp