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=0.01107 and a peak UV/optical luminosity of (5.4Β±0.4)Γ1042
erg sβ1, ASASSN-23bd is the lowest-redshift and least-luminous TDE
discovered to date. Spectroscopically, ASASSN-23bd shows HΞ± 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 59988β1+1β, βΌ9 days before discovery, with a nearly
linear rise in flux, peaking in the g band on MJD 60000β3+3β. Scaling
relations and TDE light curve modelling find a black hole mass of βΌ106Mββ, which is on the lower end of supermassive black hole masses.
ASASSN-23bd is a dim X-ray source, with an upper limit of
L0.3β10keVβ<1.0Γ1040 erg sβ1 from stacking all
\emph{Swift} observations prior to MJD 60061, but with soft (βΌ0.1 keV)
thermal emission with a luminosity of L0.3β2keVββΌ4Γ1039 erg sβ1 in \emph{XMM-Newton}
observations on MJD 60095. The rapid (t<15 days) light curve rise, low
UV/optical luminosity, and a luminosity decline over 40 days of ΞL40βββ0.7 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