Ultraviolet to Infrared Spectroscopy of the Type Ibn SN 2023tsz Suggests a Lower-mass Progenitor
Sergiy S. Vasylyev, Griffin Hosseinzadeh, Luc Dessart, Ori Fox, David J. Sand, Alexei V. Filippenko, Qinan Wang, D. Andrew Howell, Jennifer E. Andrews, Moira Andrews, Pallas Beddow, K. Azalee Bostroem, Thomas G. Brink, Peter J. Brown, Asia deGraw, Yize Dong, Joseph Farah, Thomas R. Geballe, Sebastian Gomez, Emily T. Hoang, Brian Hsu, Saurabh W. Jha, Patrick Kelly, Curtis McCully, Darshana Mehta, Megan Newsome, Yuan Q. Ni, Seong Hyun Park, Jeniveve Pearson, Neil Pichay, Justin Pierel, Aravind P. Ravi, Nicolas E. Meza Retamal, Melissa Shahbandeh, Manisha Shrestha, Nathan Smith, Bhagya M. Subrayan, Tamás Szalai, Stefano Valenti, Schuyler D. Van Dyk, Jeonghee Rho, Kathryn Wynn, Yi Yang, Yossef Zenati, WeiKang Zheng
astro-ph.HE
Submitted: 2026-07-16
Comments: Submitted to ApJ
Code: https://github.com/svalenti/FLOYDS
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Pan-STARRS1 Surveys
- Spectral Diversity in Type Ibn Supernovae and the Large Host Offset of SN2024acyl
- SN 2021csp -- the explosion of a stripped envelope star within a H and He-poor circumstellar medium
- ASAS-SN Sky Patrol V2.0
- Early-Time Ultraviolet Spectroscopy and Optical Follow-up Observations of the Type IIP Supernova 2021yja
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