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JWST Observations of SN 2023ixf II: The Panchromatic Evolution Between 250 and 720 Days After the Explosion

Fuente: arXiv

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Bibliographic Details
Main Authors:	Medler, K., Ashall, C., Hoeflich, P., Baron, E., DerKacy, J. M., Shahbandeh, M., Mera, T., Pfeffer, C. M., Hoogendam, W. B., Jones, D. O., Shiber, S., Fereidouni, E., Fox, O. D., Jencson, J., Galbany, L., Hinkle, J. T., Tucker, M. A., Shappee, B. J., Huber, M. E., Auchettl, K., Angus, C. R., Desai, D. D., Do, A., Payne, A. V., Shi, J., Kong, M. Y., Romagnoli, S., Syncatto, A., Clayton, G., Dulude, M., Engesser, M., Filippenko, A. V., Gomez, S., Hsiao, E. Y., de Jaeger, T., Johansson, J., Krisciunas, K., Kumar, S., Lu, J., Matsuura, M., Mazzali, P. A., Milisavljevic, D., Morrell, N., O'Steen, R., Park, S., Phillips, M. M., Ravi, A. P., Rest, A., Rho, J., Suntzeff, N. B., Sarangi, A., Smith, N., Stritzinger, M. D., Strolger, L., Szalai, T., Temim, T., Tinyanont, S., Van Dyk, S. D., Wang, L., Wang, Q., Wesson, R., Yang, Y., Zsiros, S.
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2507.19727