A multiwavelength view of the nearby Calcium-Strong Transient SN 2025coe in the X-Ray, Near-Infrared, and Radio Wavebands. Kumar, S., Baer-Way, R., Ravi, A. P., Modjaz, M., Chandra, P., Valenti, S., Kwok, L. A., Tinyanont, S., Foley, R. J., Howell, D. A., Hiramatsu, D., Andrews, J. E., Bostroem, K. A., Christy, C., Franz, N., Hsu, B., Pearson, J., Sand, D. J., Shrestha, M., Smith, N., & Subrayan, B. January, 2026. arXiv:2601.19018 [astro-ph]
A multiwavelength view of the nearby Calcium-Strong Transient SN 2025coe in the X-Ray, Near-Infrared, and Radio Wavebands [link]Paper  doi  abstract   bibtex   
Calcium-strong transients (CaSTs) are a subclass of faint and rapidly evolving supernovae (SNe) that exhibit strong calcium features and notably weak oxygen features. The small but growing population of CaSTs exhibits some aspects similar to thermonuclear supernovae and others that are similar to massive star core-collapse events, leading to intriguing questions on the physical origins of CaSTs. SN 2025coe is one of the most nearby CaSTs discovered to date, and our coordinated multi-wavelength observations obtained days to weeks post-explosion reveal new insights on these enigmatic transients. With the most robust NIR spectroscopic time-series of a CaST collected to date, SN 2025coe shows spectral signatures characteristic of Type Ib SNe (SNe Ib, i.e. He-rich stripped-envelope SNe). SN 2025coe is the third X-ray detected CaST and our analysis of the Swift X-ray data suggest interaction with 0.12 ± 0.11 M⊙ of circumstellar material (CSM) extending to at least 2 × 1015cm (∼ 30, 000 R⊙), while our analysis of the 1-240 GHz radio non-detections gives an outer radius of that CSM of at most ∼ 4 × 1015 cm. This inferred nearby high-density CSM extending out to 3 ± 1 × 1015 cm is similar to that seen in the other two X-ray detected CaSTs, and its presence suggests that either intensive mass-loss or some polluting mechanism may be a common feature of this subclass. Our work also expands upon recent studies on the optical properties of SN 2025coe and explores our current understanding of different progenitor systems that could possibly produce CaSTs.
@misc{kumar_multiwavelength_2026,
	title = {A multiwavelength view of the nearby {Calcium}-{Strong} {Transient} {SN} 2025coe in the {X}-{Ray}, {Near}-{Infrared}, and {Radio} {Wavebands}},
	url = {http://arxiv.org/abs/2601.19018},
	doi = {10.48550/arXiv.2601.19018},
	abstract = {Calcium-strong transients (CaSTs) are a subclass of faint and rapidly evolving supernovae (SNe) that exhibit strong calcium features and notably weak oxygen features. The small but growing population of CaSTs exhibits some aspects similar to thermonuclear supernovae and others that are similar to massive star core-collapse events, leading to intriguing questions on the physical origins of CaSTs. SN 2025coe is one of the most nearby CaSTs discovered to date, and our coordinated multi-wavelength observations obtained days to weeks post-explosion reveal new insights on these enigmatic transients. With the most robust NIR spectroscopic time-series of a CaST collected to date, SN 2025coe shows spectral signatures characteristic of Type Ib SNe (SNe Ib, i.e. He-rich stripped-envelope SNe). SN 2025coe is the third X-ray detected CaST and our analysis of the Swift X-ray data suggest interaction with 0.12 ± 0.11 M⊙ of circumstellar material (CSM) extending to at least 2 × 1015cm (∼ 30, 000 R⊙), while our analysis of the 1-240 GHz radio non-detections gives an outer radius of that CSM of at most ∼ 4 × 1015 cm. This inferred nearby high-density CSM extending out to 3 ± 1 × 1015 cm is similar to that seen in the other two X-ray detected CaSTs, and its presence suggests that either intensive mass-loss or some polluting mechanism may be a common feature of this subclass. Our work also expands upon recent studies on the optical properties of SN 2025coe and explores our current understanding of different progenitor systems that could possibly produce CaSTs.},
	language = {en},
	urldate = {2026-02-06},
	publisher = {arXiv},
	author = {Kumar, Sahana and Baer-Way, Raphael and Ravi, Aravind P. and Modjaz, Maryam and Chandra, Poonam and Valenti, Stefano and Kwok, Lindsey A. and Tinyanont, Samaporn and Foley, Ryan J. and Howell, D. Andrew and Hiramatsu, Daichi and Andrews, Jennifer E. and Bostroem, K. Azalee and Christy, Collin and Franz, Noah and Hsu, Brian and Pearson, Jeniveve and Sand, David J. and Shrestha, Manisha and Smith, Nathan and Subrayan, Bhagya},
	month = jan,
	year = {2026},
	note = {arXiv:2601.19018 [astro-ph]},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena},
}
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