We report the discovery of a progenitor candidate for the Type~IIb SN2024abfo using multi-epoch pre-explosion images from the Hubble Space Telescope and the Dark Energy Camera Legacy Survey. The progenitor exhibited a ~0.7 mag decline in F814W from 2001 to 2013, followed by significant brightening and color fluctuations in the g, r and z bands. This is the first time that substantial photometric variability has been found for the progenitor of a SN IIb. We suggest that the variability is caused by intrinsic changes in the progenitor star instead of varying obscuration by circumstellar dust. Our results show that the progenitor of SN2024abfo was likely a yellow supergiant star with an initial mass of 12--18 Msun for circumstellar reddening of E(B-V)_CSM < 0.2 mag. Our study underscores the critical role of multi-epoch imaging surveys in revealing the final stages of core-collapse supernovae progenitors.
@article{arxiv.2504.20407,
title = {Discovery of a variable yellow supergiant progenitor for the Type IIb SN 2024abfo},
author = {Zexi Niu and Ning-Chen Sun and Justyn R. Maund and Zhen Guo and Wenxiong Li and Meng Sun and Jifeng Liu},
journal= {arXiv preprint arXiv:2504.20407},
year = {2025}
}