Published in The Astrophysical Journal, 2022
This paper presents radiative transfer models of the SN Ic-bl 2014ad along with UV and NIR spectra.
Recommended citation: Kwok, Lindsey A., Williamson, Marc et al. "Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad." arXiv preprint arXiv:2204.03716 (2022). https://ui.adsabs.harvard.edu/abs/2022arXiv220403716K/abstract
Published in The Astrophysical Journal, 2021
This paper places an upper limit of 0.05 solar masses on the Helium content in the ejecta of stripped supernova 1994I using radiative transfer modeling.
Recommended citation: Williamson, Marc, Wolfgang Kerzendorf, and Maryam Modjaz. "Modeling Type Ic Supernovae with tardis: Hidden Helium in SN 1994I?." The Astrophysical Journal 908.2 (2021): 150. https://ui.adsabs.harvard.edu/abs/2021ApJ...908..150W/abstract
Published in The Astrophysical Journal, 2019
This paper presents the SESNPCA code, a public spectral classifier for stripped supernovae.
Recommended citation: Williamson, Marc, Maryam Modjaz, and Federica B. Bianco. "Optimal classification and outlier detection for stripped-envelope core-collapse supernovae." The Astrophysical Journal Letters 880.2 (2019): L22. https://ui.adsabs.harvard.edu/abs/2019ApJ...880L..22W/abstract
Published in Astronomy & Astrophysics, 2022
This paper presents the first large-scale code comparison between many of the most commonly used supernova radiative transfer codes.
Recommended citation: Blondin, Stephane; et al. (2022). https://ui.adsabs.harvard.edu/abs/2022arXiv220911671B/abstract
Published in The Astrophysical Journal, 2022
This paper presents early time ultraviolet and optical spectra of the nearby SN IIP 2021yja. We the radiative transfer code TARDIS to model the spectra and constrain the ejecta velocity structure, extinction, and metallicity.
Recommended citation: Vasylyev, Sergiy; et al. (2022). https://ui.adsabs.harvard.edu/abs/2022ApJ...934..134V/abstract
Published in The Astrophysical Journal, 2022
We present a sample of SN Icn supernova spectra. SN Icn are a newly discovered supernova class showing evidence of interaction with H and He poor CSM. This sample highlights the range of spectral behaviors observed.
Recommended citation: Pellegrino, Craig; et al. (2022). https://ui.adsabs.harvard.edu/abs/2022arXiv220507894P/abstract
Published in MNRAS, 2021
We present UV spectroscopy and corresponding radiative transfer models using TARDIS of the normal SN Ia ASASSN-14lp which exhibits suppressed UV flux in its spectra. Models suggest that this UV suppression may be due to high levels of Ni56 mixing in the ejecta.
Recommended citation: Barnabas, Barna; et al. (2022). https://ui.adsabs.harvard.edu/abs/2021MNRAS.506..415B/abstract
Published in The Astrophysical Journal Letters, 2021
We present the first application of the DALEK emulator-assisted TARDIS modeling framework to fit models to the SN Ia 2002bo. Posterior distributions over model parameters like elemental abundances are produced and comparisons are made to hydrodynamical models of different types of SN Ia explosion mechanisms.
Recommended citation: OBrien, John; et al. (2021). https://ui.adsabs.harvard.edu/abs/2021ApJ...916L..14O/abstract
Published in The Astrophysical Journal, 2021
We present optical and UV data on SN2018gep, a supernova that exhibited a fast rise with blue, featureless spectra until after peak light, when the spectra developed broad features typically seen in SNe Ic-bl. Significant blue excess flux is observed compared to other stripped SNe.
Recommended citation: Pritchard, Tyler; et al. (2021). https://ui.adsabs.harvard.edu/abs/2021ApJ...915..121P/abstract
Published in The Astrophysical Journal Letters, 2021
We present DALEK, a neural network based emulator for the TARDIS radiative transfer code. DALEK can predict the output of TARDIS (synthetic spectra) to extremely high accuracy. A single DALEK evalution takes only milliseconds compared to thousands of seconds for a full TARDIS simulation, thus unlocking the ability to evaluate millions of TARDIS in mere hours.
Recommended citation: Kerzendorf, Wolfgang; et al. (2021). https://ui.adsabs.harvard.edu/abs/2021ApJ...910L..23K/abstract
Published in The Astrophysical Journal, 2021
We present NIR and optical spectroscopy of SN Ic 2020oi and SN Ic-bl 2020bvc. The NIR spectrum of SN2020oi shows clear CO emission and is the first such dust detection for an SN Ic. SN2020bvc exhibits extremely high ejecta velocities consistent with SN-GRBs despite the lack of observed GRB.
Recommended citation: Rho, Jeonghee; et al. (2021). https://ui.adsabs.harvard.edu/abs/2021ApJ...908..232R/abstract