Iptf13dcc
WebFeb 23, 2024 · In this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation … WebThe two fainter galaxies (iPTF13dcc with V~23.6 and iPTF13ehe with 21) still host the ongoing supernova (equal in brightness or fainter than the galaxy) and we will observe them with ACS with one filter (F625W). We intend to divide each orbit in a few sub-exposures and dither them to correct for cosmic rays and bad pixels.
Iptf13dcc
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WebThe spectra of iPTF16asu and iPTF13dcc (fig. 5 in Vreeswijk et al. 2024) near peak are pretty featureless, consistent with CSM–ejecta SNe. However, the spectra of iPTF15esb (fig. 1 in Yan et al. 2024) near peak light show prominent absorption at rest frame ∼ 4100 ˚A. WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the …
Webtask dataset model metric name metric value global rank remove WebSep 26, 2016 · A model combining a shock breakout in an extended envelope with late-time magnetar energy injection provides a reasonable fit to the iPTF13dcc observations. …
WebSomehow this event is getting removed before the import completes. It appears that the data is being imported when its task is run (the ascii task), but it is not surviving cleanup. WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe), iPTF15esb and iPTF13dcc, whose light curves (LCs) show significant deviation from the …
WebIn contrast, the long-duration (>30days) early excess emission in iPTF13dcc, whose brightness competes with that of the main peak, appears to be of a different nature. We construct bolometric light curves for both targets, and fit a variety of light-curve models to both the early bump and main peak in an attempt to understand the nature of
WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe), iPTF15esb and iPTF13dcc, whose light curves (LCs) show significant deviation from the … chiseled cheeks makeupWebWell sampled light curves of SN2015bn and iPTF13dcc have also resulted in discov- eries of LC undulations of SLSNe-I, suggesting possible ejecta interaction with H-poor CSM (Nicholl et al. 2016; Vreeswijk et al. 2024). In this paper, we report two new SLSNe-I events, iPTF15esb and iPTF16bad, showing late-time H emis- sion, similar to iPTF13ehe. chiseled carpet tileWebA Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc The Astrophysical Journal 2024-03-26 Journal article chiseled college wrestlerWebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar … graphite hoover washing machineWebIn 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 … chiseled constructWebSep 26, 2016 · We gratefully acknowledge support from the Simons Foundation and member institutions. > astro-ph > arXiv:1609.08145v1 chiseled constructionWebMar 26, 2024 · This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our chiseled columbia