We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supernova (SLSN) spectroscopically confirmed to date. The light curves and Gemini spectroscopy of DES15E2mlf indicate that it is a Type I superluminous supernova (SLSN-I) at z = 1.861 (a lookback time of similar to 10 Gyr) and peaking at M-AB = -22.3 +/- 0.1 mag. Given the high redshift, our data probe the rest-frame ultraviolet (1400-3500 angstrom) properties of the SN, finding velocity of the C III feature changes by similar to 5600 km s(-1) over 14 d around maximum light. We find the host galaxy of DES15E2mlf has a stellar mass of 3.5(-2.4)(+3.6) x 10(9) M-circle dot, which is more massive than the typical SLSN-I host galaxy.NSF AST-1518052...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superlumin...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...
We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supe...
We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supe...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superlumin...
We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the...
We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the...
Artículo de publicación ISIWe present DES14X3taz, a new hydrogen-poor superluminous supernova (SLSN-...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superlumin...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...
We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supe...
We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supe...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superlumin...
We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the...
We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the...
Artículo de publicación ISIWe present DES14X3taz, a new hydrogen-poor superluminous supernova (SLSN-...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of SN 2015bn (=PS15ae = CSS141223-113342+004332 = MLS150211-113342+004333), ...
We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superlumin...
Context. Super-luminous supernovae (SLSNe) are rare events defined as being significantly more lumin...