We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2018bsz. The photometric evolution of SN 2018bsz has several surprising features, including an unusual pre-peak plateau and evidence for rapid formation of dust ≳200 d post-peak. We show here that the spectroscopic and polarimetric properties of SN 2018bsz are also unique. While its spectroscopic evolution closely resembles SLSNe-I, with early O I
International audienceSupernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically confirmed T...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present DES14X3taz, a new hydrogen-poor superluminous supernova (SLSN-I) discovered by the Dark E...
We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2...
We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2...
We present a spectroscopic analysis of Type I superluminous supernova (SLSN-I), SN 2018bsz. While it...
We present a spectroscopic analysis of Type I superluminous supernova (SLSN-I), SN 2018bsz. While it...
We present and discuss the optical spectrophotometric observations of the nearby (z = 0.087) Type I ...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...
SN 2018hti was a very nearby (z = 0.0614) superluminous supernova with an exceedingly bright absolut...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
Publisher Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal As...
We present the analysis of SN 2020wnt, an unusual hydrogen-poor super-luminous supernova (SLSN-I), a...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
International audienceSupernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically confirmed T...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present DES14X3taz, a new hydrogen-poor superluminous supernova (SLSN-I) discovered by the Dark E...
We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2...
We present a spectroscopic analysis of the most nearby Type I superluminous supernova (SLSN-I), SN 2...
We present a spectroscopic analysis of Type I superluminous supernova (SLSN-I), SN 2018bsz. While it...
We present a spectroscopic analysis of Type I superluminous supernova (SLSN-I), SN 2018bsz. While it...
We present and discuss the optical spectrophotometric observations of the nearby (z = 0.087) Type I ...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...
SN 2018hti was a very nearby (z = 0.0614) superluminous supernova with an exceedingly bright absolut...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
Publisher Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal As...
We present the analysis of SN 2020wnt, an unusual hydrogen-poor super-luminous supernova (SLSN-I), a...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
International audienceSupernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically confirmed T...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present DES14X3taz, a new hydrogen-poor superluminous supernova (SLSN-I) discovered by the Dark E...