WebNov 16, 2024 · The exception to this is iPTF13dcc (Vreeswijk et al. 2024 ), which showed either a plateau or an unusually bright bump around the light-curve peak. The data around this phase are noisy and highly oversampled, so we rebin to a daily cadence before fitting. WebSep 26, 2016 · We gratefully acknowledge support from the Simons Foundation and member institutions. > astro-ph > arXiv:1609.08145v1
The Magnetar Model for Type I Superluminous Supernovae. I.
WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the smooth rise and fall. The LC of iPTF15esb exhibits two peaks and a post-peak plateau, and furthermore the late-time spectrum of iPTF15esb shows a strong, broad H α emission … WebWe present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient Factory. Both show excess emission at ... simple hash table c
A Multiple Ejecta-circumstellar Medium Interaction Model and Its ...
WebWe present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient... WebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transien... Webtask dataset model metric name metric value global rank remove simplehat clicker