Iptf13dcc

Author: zjff

August undefined, 2024

WebThe hydrogen-poor superluminous supernova iPTF13ajg and its host galaxy in absorption and emission WebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe), iPTF15esb and iPTF13dcc, whose light curves (LCs) show significant deviation from the …

Roni WALDMAN Hebrew University of Jerusalem, Jerusalem

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. how to see committed changes in git

13858 - The environment of the rarest and most energetic …

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. WebFig. 3.— Same as in Figure 1 but for iPTF13dcc. Data are obtained from Vreeswijk et al. (2024). The fitting parameters are shown in the text and Table 1. - "A Multiple Ejecta-Circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc" 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. … how to see community posts on youtube pc

The Energy Sources of Double-peaked Superluminous …

ORCID

WebTD-050FFEC01-A-ZVG/US. Hygienic design for the requirements of the food and beverage industry. Fast response dynamics and very short power-on delay time. Clearly visible … WebiPTF13dcc LS014bdq DES14X3taz 5dtg SN2024cad SN2024dge SN2024ehk SN2024bvc - SN2024faa 10 days since exo 100 losion . Created Date: 9/20/2024 8:24:00 AM ... how to see committed files in gitWebof 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 ... how to see commit message in git bash

"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 … " - Iptf13dcc

Iptf13dcc

A Multiple Ejecta-circumstellar Medium Interaction Model …

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.

Did you know?

http://export.arxiv.org/abs/1609.08145v1 WebThe 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...

WebMar 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 WebSep 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.

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... 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...

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

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 … how to see complete dataframe in pythonWebFeb 23, 2024 · The early-time LC of iPTF13dcc shows a long duration bump followed by the second peak. Here we propose an ejecta-circumstellar medium (CSM) interaction model involving multiple shells/winds and use it to explain the LCs of iPTF15esb and iPTF13dcc. We find that the theoretical LCs reproduced by this model can well match the … how to see compiler errors in unityWebIn this paper, we investigate two hydrogen-poor superluminous supernovae (SLSNe) iPTF15esb and iPTF13dcc whose light curves (LCs) show significant deviation from the … how to see competitors display adsWebA Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc The Astrophysical Journal 2024-03-26 Journal article how to see companies facebook adsWebSomehow 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. how to see competitors google adsWebSep 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 … how to see competitor ads on facebookWebWe 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 ... how to see competitors twitter ads