Abstract

ASASSN-14ae is a candidate tidal disruption event (TDE) found at the center of SDSS J110840.11+340552.2 (d≃200d\simeq200~Mpc) by the All-Sky Automated Survey for Supernovae (ASAS-SN). We present ground-based and Swift follow-up photometric and spectroscopic observations of the source, finding that the transient had a peak luminosity of L≃8×1043L\simeq8\times10^{43}~erg~s−1^{-1} and a total integrated energy of E≃1.7×1050E\simeq1.7\times10^{50} ergs radiated over the ∼5\sim5 months of observations presented. The blackbody temperature of the transient remains roughly constant at T∼20,000T\sim20,000~K while the luminosity declines by nearly 1.5 orders of magnitude during this time, a drop that is most consistent with an exponential, L∝e−t/t0L\propto e^{-t/t_0} with t0≃39t_0\simeq39~days. The source has broad Balmer lines in emission at all epochs as well as a broad He II feature emerging in later epochs. We compare the color and spectral evolution to both supernovae and normal AGN to show that {\name} does not resemble either type of object and conclude that a TDE is the most likely explanation for our observations. At z=0.0436z=0.0436, ASASSN-14ae is the lowest-redshift TDE candidate discovered at optical/UV wavelengths to date, and we estimate that ASAS-SN may discover 0.1−30.1 - 3 of these events every year in the future.

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