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Gendreau, Lixin Dai, Matthew J. Graham, Muryel Guolo, Natalie LeBaron, Raffaella Margutti, Roger Smith, Ruancun Li, Russ R. Laher, Ryan Chornock, S. Bradley Cenko, S. R. Kulkarni, Suvi Gezari, Thomas Wevers, Tom M. Kwan, Vikram Ravi, Wenbin Lu, Yashvi Sharma, Yuhan Yao, Yukta Ajay","submitted_at":"2024-05-18T17:27:34Z","abstract_excerpt":"We present the tidal disruption event (TDE) AT2022lri, hosted in a nearby ($\\approx\\!144$ Mpc) quiescent galaxy with a low-mass massive black hole ($10^4\\,M_\\odot < M_{\\rm BH} < 10^6\\,M_\\odot$). AT2022lri belongs to the TDE-H+He subtype. More than 1 Ms of X-ray data were collected with NICER, Swift, and XMM-Newton from 187 d to 672 d after peak. The X-ray luminosity gradually declined from $1.5\\times 10^{44}\\,{\\rm erg\\,s^{-1}}$ to $1.5\\times 10^{43}\\,{\\rm erg\\,s^{-1}}$ and remains much above the UV and optical luminosity, consistent with a super-Eddington accretion flow viewed face-on. 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