A late-time view of the progenitors of five Type IIP supernovae
Constraints for the Progenitor Masses of 17 Historic Core-collapse Supernovae
Late-time Light Curves of Type II Supernovae: Physical Properties of Supernovae and Their Environment
Late-time Optical Emission from Core-collapse Supernovae
Late-time spectroscopy of SN 2002hh: a continued visible light echo with no shock interaction yet
Luminous blue variable eruptions and related transients: diversity of progenitors and outburst properties
On the nature of the progenitors of three Type II-P supernovae: 2004et, 2006my and 2006ov
Optical and Infrared Analysis of Type II SN 2006bc
Optical and near-infrared coverage of SN 2004et: physical parameters and comparison with other Type IIP supernovae
The effects of dust on the optical and infrared evolution of SN 2004et
The initial masses of the red supergiant progenitors to Type II supernovae
The search for failed supernovae with the Large Binocular Telescope: first candidates
Thirty Years of SN 1980K: Evidence for Light Echoes
Unmasking the Supernova Impostors
Instrument
NICMOS, NICMOS/NIC2, WFPC2, WFPC2/PC
Temporal Coverage
2007-07-08T05:50:16Z/2008-04-27T20:55:02Z
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, Meixner comma Margaret, 2009, 'SEEDS: The Search for Evolution of Emission from Dust in Supernovae with HST and Spitzer', 1.0, European Space Agency, https://doi.org/10.5270/esa-wa4ktig