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JWST Observations of SN 2024abup: First Detection of CO in a Broad-lined Type Ic Supernova and Constraints on r-process Nucleosynthesis

  • Authors: Manisha Shrestha, Lindsey A. Kwok, David J. Sand, Stan Barmentloo, Collin Christy, Anders Jerkstrand, K. Azalee Bostroem, Jennifer E. Andrews, Kate D. Alexander, Yize Dong, 一泽 董, C. E. Fields, Emily Hoang, Griffin Hosseinzadeh, Brian Hsu, Daryl Janzen, Saurabh W. Jha, Joel Johansson, Jeniveve Pearson, M. J. Lundquist, Darshana Mehta, Aidan Martas, Maryam Modjaz, Bernhard Müller, Conor L. Ransome, Aravind P. Ravi, Mathieu Renzo, Nicolás Meza Retamal, Bhagya Subrayan, Nathan Smith, Stefano Valenti, Sergiy Vasylyev, Giacomo Ricigliano, Peter J. Brown, Moira Andrews, Joseph Farah, D. Andrew Howell, Curtis McCully, Megan Newsome, Kathryn Wynn, Ryan Chornock, Natalie LeBaron, Raffaella Margutti, Melissa Shahbandeh, Chris Ashall, Peter Hoeflich

Manisha Shrestha et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 5.

Comparison of extinction corrected absolute V-band magnitudes for a few different SN Ic-bl with (SN 1998bw) and without an associated GRB. The phases are given with respect to the date of ﹩{V}_{{\rm{\max }}}﹩. SN 2024abup (black circle) falls within a reasonable range with SN 1998bw, which is associated with a low-luminosity GRB, being the brightest.

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