An Extensive Hubble Space Telescope Study of the Offset and Host Light Distributions of Type I Superluminous Supernovae
A VLA Survey of Late-time Radio Emission from Superluminous Supernovae and the Host Galaxies
Detection of Broad Ha Emission Lines in the Late-time Spectra of a Hydrogen-poor Superluminous Supernova
Host-galaxy Properties of 32 Low-redshift Superluminous Supernovae from the Palomar Transient Factory
Light Curves of Hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory
Obscured Star Formation in the Host Galaxies of Superluminous Supernovae
On the Early-time Excess Emission in Hydrogen-poor Superluminous Supernovae
Spatially resolved analysis of superluminous supernovae PTF 11hrq and PTF 12dam host galaxies
The impact of satellite trails on Hubble Space Telescope observations
The interacting nature of dwarf galaxies hosting superluminous supernovae
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2014-10-16T17:59:45Z/2015-02-17T22:25:22Z
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, De Cia comma Annalisa, 2016, 'The environment of the rarest and most energetic supernovae: do pair-instability explosions exist in the nearby Universe?', 1.0, European Space Agency, https://doi.org/10.5270/esa-ue4a3di