Posted in astro-ph.HE · 2026-01-01 · Aravind P. Ravi, Sahana Kumar, Raphael Baer-Way, Stefano Valenti, Maryam Modjaz, Bart F. A. van Baal, Anders Jerkstrand, Yize Dong, Lindsey A. Kwok, Jeniveve Pearson, David J. Sand, Daichi Hiramatsu, Alexei V. Filippenko, Jennifer Andrews, Moira Andrews, Prasiddha Arunachalam, K. Azalee Bostroem, Thomas G. Brink, Collin Christy, Liyang Chen, Kyle W. Davis, Ali Esamdin, Joseph Farah, Ryan J. Foley, Emily Hoang, Griffin Hosseinzadeh, D. Andrew Howell, Brian Hsu, Ruifeng Huang, Abdusamatjan Iskander, Daryl Janzen, Saurabh W. Jha, Ravjit Kaur, Michael J. Lundquist, Curtis McCully, Darshana Mehta, Yuan Qi Ni, Nicolas Meza Retamal, Kishore C. Patra, Conor Ransome, Manisha Shrestha, Nathan Smith, Bhagya Subrayan, Kirsty Taggart, Xiaofeng Wang, Kathryn Wynn, Yi Yang, Shengyu Yan, Weikang Zheng, Dan Coe
Supernova (SN) 2025coe at a distance of $\sim$25 Mpc is the second-closest calcium-strong (CaST) transient. It was discovered at a large projected offset of $\sim$34 kpc from its potential host galaxy NGC 3277. Multiband photometry of SN 2025coe indicates the presence of two peaks at day $\sim$2 and day $\sim$11 after explosion....