Abstract

We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong AGN activity over the past decade. With a redshift of z=0.01107z = 0.01107 and a peak UV/optical luminosity of (5.4Β±0.4)Γ—1042(5.4\pm0.4)\times10^{42} erg sβˆ’1^{-1}, ASASSN-23bd is the lowest-redshift and least-luminous TDE discovered to date. Spectroscopically, ASASSN-23bd shows HΞ±\alpha and He I emission throughout its spectral time series, and the UV spectrum shows nitrogen lines without the strong carbon and magnesium lines typically seen for AGN. Fits to the rising ASAS-SN light curve show that ASASSN-23bd started to brighten on MJD 59988βˆ’1+1^{+1}_{-1}, ∼\sim9 days before discovery, with a nearly linear rise in flux, peaking in the gg band on MJD 60000βˆ’3+360000^{+3}_{-3}. Scaling relations and TDE light curve modelling find a black hole mass of ∼\sim106^6 MβŠ™M_\odot, which is on the lower end of supermassive black hole masses. ASASSN-23bd is a dim X-ray source, with an upper limit of L0.3βˆ’10 keV<1.0Γ—1040L_{0.3-10\,\mathrm{keV}} < 1.0\times10^{40} erg sβˆ’1^{-1} from stacking all \emph{Swift} observations prior to MJD 60061, but with soft (∼0.1\sim 0.1 keV) thermal emission with a luminosity of L0.3βˆ’2 keV∼4Γ—1039L_{0.3-2 \,\mathrm{keV}}\sim4\times10^{39} erg sβˆ’1^{-1} in \emph{XMM-Newton} observations on MJD 60095. The rapid (t<15(t < 15 days) light curve rise, low UV/optical luminosity, and a luminosity decline over 40 days of Ξ”L40β‰ˆβˆ’0.7\Delta L_{40}\approx-0.7 make ASASSN-23bd one of the dimmest TDEs to date and a member of the growing ``Low Luminosity and Fast'' class of TDEs.Comment: 17 pages, 13 figures, submitted to MNRA

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