Iptf13dcc

Author: lnpk

August undefined, 2024

WebSep 27, 2016 · http://arxiv.org/abs/1609.08145 We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the … WebSep 27, 2016 · We 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 …

[1609.08145v3] On the early-time excess emission in …

WebThe hydrogen-poor superluminous supernova iPTF13ajg and its host galaxy in absorption and emission WebA Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc The Astrophysical Journal 2024-03-26 Journal article inanno borth

ON the EARLY-TIME EXCESS EMISSION in HYDROGEN-POOR …

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. Web4 www.irf.com Fig 11. Maximum Effective Transient Thermal Impedance, Junction-to-Ambient Fig 9. Maximum Drain Current vs. Case Temperature Fig 10. Threshold Voltage … 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. incha organics sacha inchi oil

13858 - The environment of the rarest and most energetic …

On the early-time excess emission in hydrogen-poor …

WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the … 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. inanna\\u0027s temple of uruk inanny essity

"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. " - Iptf13dcc

Iptf13dcc

A Multiple Ejecta-Circumstellar Medium Interaction Model and Its ...

WebWell 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. 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 ...

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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 … WebUsing 1D, non-local thermodynamic equilibrium and time-dependent radiative transfer simulations, we study the ejecta properties required to match the early- and late-time photometric and...

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WebMar 26, 2024 · The theoretical LC of iPTF13dcc is shown in Figure 3. The best-fitting parameters and the corresponding confidence contour corners of iPTF13dcc are shown … WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the …

WebFeb 20, 2024 · In this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation …

Webof PTF12dam and iPTF13dcc; Liu et al. (2024) develop a multiple CSI model involving the collisions between the ejecta and the CSM shells or winds locating at different sites and use these models to ﬁt the LCs of iPTF15esb and iPTF13dcc. In this paper, we study two hydrogen-poor SNe, PS1-12cil and SN 2012aa. PS1-12cil is an SLSN I discovered ... inchad diniWebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar … inanothercountry中文版WebiPTF13dcc LS014bdq DES14X3taz 5dtg SN2024cad SN2024dge SN2024ehk SN2024bvc - SN2024faa 10 days since exo 100 losion . Created Date: 9/20/2024 8:24:00 AM ... inchackWebThe explosion mechanism of broad-lined type Ic supernovae (SNe Ic-BL) is not very well understood despite their discovery more than two decades ago. Recently a serious confrontation of SNe Ic-BL... inchae cvWebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the … inanna\\u0027s festival norwichWebSep 26, 2024 · The Intermediate Palomar Transient Factory reported the discovery of an unusual type II-P supernova iPTF14hls. Instead of an ∼100 day plateau as observed for ordinary type II-P supernovae, the light curve of iPTF14hls has at least five distinct peaks, followed by a steep decline at ∼1000 days since discovery. inanna\u0027s 8 pointed star imagesWebJan 20, 2024 · We present the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transien... inchae hissab