SN 2017dio: A Type-Ic Supernova Exploding in a Hydrogen-rich Circumstellar Medium∗ ∗ Based on observations made with the NOT, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofisica de Canarias. This work is based (in part) on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere, Chile as part of PESSTO, (the Public ESO Spectroscopic Survey for Transient Objects Survey) ESO program 188.D-3003, 191.D-0935, 197.D-1075. Based on observations made with the Liverpool Telescope operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council.
The Astrophysical Journal Letters American Astronomical Society 854:1 (2018) l14
Publisher Correction: Hydrogen-rich supernovae beyond the neutrino-driven core-collapse paradigm
Nature Astronomy Springer Nature 2:2 (2018) 173-173
The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am∗ ∗ This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.
The Astrophysical Journal American Astronomical Society 853:1 (2018) 62
Hydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey
The Astrophysical Journal American Astronomical Society 852:2 (2018) 81