Ultraviolet to Infrared Spectroscopy of the Type Ibn SN 2023tsz Suggests a Lower-mass Progenitor

arXiv:2607.15342 · astro-ph.HE · Submitted 2026-07-16 · Read on arXiv

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/

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