Peter Lundqvist

TL;DR: Observations of supernova 1987A reveal the presence of a population of cold dust grains radiating with a temperature of about 17 to 23 kelvin at a rate of about 220 times the luminosity of the Sun, implying that supernovae can produce the large dust masses detected in young galaxies at very high redshifts.

TL;DR: The first data release (SSDR1) contains flux calibrated spectra from the first year (April 2012-2013), and a total of 221 confirmed supernovae were classified, and they released calibrated optical spectra and classifications publicly within 24 h of the data being taken as mentioned in this paper.

TL;DR: The radio and X-ray observations of SN 1993J during the first year can be consistently explained as a result of interaction of the expanding ejecta with a circumstellar medium as discussed by the authors.

TL;DR: In this paper, the optical/UV light curves of SN 1987A were analyzed with the multi-energy group radiation hydrodynamics code STELLA and the authors derived the most likely range of E/M (explosion energy over ejecta mass) and R0 (radius of the progenitor).

TL;DR: In this article, the authors describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1 (SSDR1).