Characterizing the Ordinary Broad-line Type Ic SN 2023pel from the Energetic GRB 230812B

Srinivasaragavan, Gokul P. and Swain, Vishwajeet and O’Connor, Brendan and Anand, Shreya and Ahumada, Tomás and Perley, Daniel and Stein, Robert and Sollerman, Jesper and Fremling, Christoffer and Cenko, S. Bradley and Antier, S. and Guessoum, Nidhal and Hussenot-Desenonges, Thomas and Hello, Patrice and Lesage, Stephen and Hammerstein, Erica and Miller, M. Coleman and Andreoni, Igor and Bhalerao, Varun and Bloom, Joshua S. and Dutta, Anirban and Gal-Yam, Avishay and Hinds, K. -Ryan and Jaodand, Amruta and Kasliwal, Mansi and Kumar, Harsh and Kutyrev, Alexander S. and Ragosta, Fabio and Ravi, Vikram and Sharma, Kritti and Teja, Rishabh Singh and Yang, Sheng and Anupama, G. C. and Bellm, Eric C. and Coughlin, Michael W. and Mahabal, Ashish A. and Masci, Frank J. and Pathak, Utkarsh and Purdum, Josiah and Roberts, Oliver J. and Smith, Roger and Wold, Avery

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