Jaladh Singhal
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View article: OpenUniverse2024: a shared, simulated view of the sky for the next generation of cosmological surveys
OpenUniverse2024: a shared, simulated view of the sky for the next generation of cosmological surveys Open
The OpenUniverse2024 simulation suite is a cross-collaboration effort to produce matched simulated imaging for multiple surveys as they would observe a common simulated sky. Both the simulated data and associated tools used to produce it a…
View article: Introducing STARDIS: An Open and Modular Stellar Spectral Synthesis Code
Introducing STARDIS: An Open and Modular Stellar Spectral Synthesis Code Open
We introduce a new 1D stellar spectral synthesis Python code called stardis . stardis is a modular, open-source radiative transfer code that is capable of spectral synthesis from near-UV to IR for FGK stars. We describe the structure, inpu…
View article: 1991T-Like Type Ia Supernovae as an Extension of the Normal Population
1991T-Like Type Ia Supernovae as an Extension of the Normal Population Open
Type Ia supernovae (SNe) remain poorly understood despite decades of investigation. Massive computationally intensive hydrodynamic simulations have been developed and run to model an ever-growing number of proposed progenitor channels. Fur…
View article: Over 500 Days in the Life of the Photosphere of the Type Iax Supernova SN 2014dt
Over 500 Days in the Life of the Photosphere of the Type Iax Supernova SN 2014dt Open
Type Iax supernovae (SNe Iax) are the largest known class of peculiar white dwarf SNe, distinct from normal Type Ia supernovae (SNe Ia). The unique properties of SNe Iax, especially their strong photospheric lines out to extremely late tim…
View article: 1991T-Like Type Ia Supernovae as an Extension of the Normal Population
1991T-Like Type Ia Supernovae as an Extension of the Normal Population Open
Type Ia supernovae remain poorly understood despite decades of investigation. Massive computationally intensive hydrodynamic simulations have been developed and run to model an ever-growing number of proposed progenitor channels. Further c…
View article: TARDIS configuration and emulator weights and training data for "1991T-Like Type Ia Supernovae as an Extension of the Normal Population"
TARDIS configuration and emulator weights and training data for "1991T-Like Type Ia Supernovae as an Extension of the Normal Population" Open
This dataset contains two archives of data related to the paper "1991T-Like Type Ia Supernovae as an Extension of the Normal Population" The first dataset, TARDIS_Emulator_Config.tar.gz , contains the atomic data used to run TARDIS and a …
View article: TARDIS configuration and emulator weights and training data for "1991T-Like Type Ia Supernovae as an Extension of the Normal Population"
TARDIS configuration and emulator weights and training data for "1991T-Like Type Ia Supernovae as an Extension of the Normal Population" Open
This dataset contains two archives of data related to the paper "1991T-Like Type Ia Supernovae as an Extension of the Normal Population" The first dataset, TARDIS_Emulator_Config.tar.gz , contains the atomic data used to run TARDIS and a …
View article: Over 500 Days in the Life of the Photosphere of the Type Iax Supernova SN 2014dt
Over 500 Days in the Life of the Photosphere of the Type Iax Supernova SN 2014dt Open
Type Iax supernovae (SN Iax) are the largest known class of peculiar white dwarf supernovae, distinct from normal Type Ia supernovae (SN Ia). The unique properties of SN Iax, especially their strong photospheric lines out to extremely late…
View article: SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra
SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra Open
With the advent of high-cadence, all-sky automated surveys, supernovae (SNe) are now discovered closer than ever to their dates of explosion. However, young premaximum light follow-up spectra of Type Ic SNe (SNe Ic), probably arising from …
View article: SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra
SN 2019ewu: A Peculiar Supernova with Early Strong Carbon and Weak Oxygen Features from a New Sample of Young SN Ic Spectra Open
With the advent of high cadence, all-sky automated surveys, supernovae (SNe) are now discovered closer than ever to their dates of explosion. However, young pre-maximum light follow-up spectra of Type Ic supernovae (SNe Ic), probably arisi…
View article: StaNdaRT: a repository of standardised test models and outputs for supernova radiative transfer
StaNdaRT: a repository of standardised test models and outputs for supernova radiative transfer Open
We present the first results of a comprehensive supernova (SN) radiative-transfer (RT) code-comparison initiative (StaNdaRT), where the emission from the same set of standardised test models is simulated by currently used RT codes. We ran …
View article: StaNdaRT: A repository of standardized test models and outputs for supernova radiative transfer
StaNdaRT: A repository of standardized test models and outputs for supernova radiative transfer Open
We present the first results of a comprehensive supernova (SN) radiative-transfer (RT) code-comparison initiative (StaNdaRT), where the emission from the same set of standardized test models is simulated by currently-used RT codes. A total…
View article: StaNdaRT: A repository of standardized test models and outputs for supernova radiative transfer
StaNdaRT: A repository of standardized test models and outputs for supernova radiative transfer Open
We present the first results of a comprehensive supernova (SN) radiative-transfer (RT) code-comparison initiative (StaNdaRT), where the emission from the same set of standardized test models is simulated by currently-used RT codes. A total…
View article: Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type Ic Supernova 2014ad
Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type Ic Supernova 2014ad Open
Few published ultraviolet (UV) spectra exist for stripped-envelope supernovae and none to date for broad-lined Type Ic supernovae (SNe Ic-bl). These objects have extremely high ejecta velocities and are the only supernova type directly lin…
View article: Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad
Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad Open
Few published ultraviolet (UV) spectra exist for stripped-envelope supernovae, and none to date for broad-lined Type Ic supernovae (SN Ic-bl). These objects have extremely high ejecta velocities and are the only supernova type directly lin…
View article: tardis-sn/tardis: TARDIS v2021.11.14
tardis-sn/tardis: TARDIS v2021.11.14 Open
TARDIS - Temperature And Radiative Diffusion In Supernovae