AT 2022fpx , the SIMBAD biblio

AT 2022fpx , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:08:07


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Title First 3 Authors
2024MNRAS.532..112K 3163 T   A S   X C F     67 10 ~ The extreme coronal line emitter
AT 2022fpx: varying optical polarization properties and late-time X-ray flare.
KOLJONEN K.I.I., LIODAKIS I., LINDFORS E., et al.
2024MNRAS.535.1095C 90           X         2 41 ~ The rate of extreme coronal line emitting galaxies in the Sloan Digital Sky Survey and their relation to tidal disruption events. CALLOW J., GRAUR O., CLARK P., et al.
2024ApJ...974..172A 18       D               1 61 ~ Anomaly Detection and Approximate Similarity Searches of Transients in Real-time Data Streams. ALEO P.D., ENGEL A.W., NARAYAN G., et al.
2024ApJ...977..258N 108       D       C       2 29 ~ Mapping the Inner 0.1 pc of a Supermassive Black Hole Environment with the Tidal Disruption Event and Extreme Coronal-line Emitter AT 2022upj. NEWSOME M., ARCAVI I., HOWELL D.A., et al.
2025MNRAS.537.2024W 1698       D     X C F     35 37 ~ A systematically selected sample of luminous, long-duration, ambiguous nuclear transients. WISEMAN P., WILLIAMS R.D., ARCAVI I., et al.
2025ApJ...983L..39C 47           X         1 17 ~ Discovery of Quasiperiodic Eruptions in the Tidal Disruption Event and Extreme Coronal Line Emitter AT2022upj: Implications for the QPE/TDE Fraction and a Connection to ECLEs. CHAKRABORTY J., KARA E., ARCODIA R., et al.
2025MNRAS.539..231C 140           X         3 33 ~ The rate of extreme coronal line emitters in the Baryon Oscillation Spectroscopic Survey LOWZ sample. CALLOW J., GRAUR O., CLARK P., et al.
2025MNRAS.540..871C 439       D     X   F     9 49 ~ AT 2018dyk: tidal disruption event or active galactic nucleus? Follow-up observations of an extreme coronal line emitter with the Dark Energy Spectroscopic Instrument. CLARK P., CALLOW J., GRAUR O., et al.
2025ApJ...990...22L 2454 T   A     X C       51 25 ~ Insights from the “Red Devil”
AT 2022fpx: A Dust-reddened Family of Tidal Disruption Events Excluded by Their Apparent Red Color?
LIN Z., JIANG N., WANG Y., et al.
2025MNRAS.542.2238K 47           X         1 5 ~ Optical polarization properties of the closest tidal disruption event AT 2023clx indicate origin from tidal stream shocks. KOLJONEN K.I.I., NILSSON K., LIODAKIS I., et al.
2025A&A...701A.224B 373           X C       7 31 ~ A new Bowen fluorescence flare and extreme coronal line emitter discovered by SRG/eROSITA. BALDINI P., RAU A., ARCODIA R., et al.
2025ApJS..281....7Y 112       D     X         3 171 ~ Distinguishing Tidal Disruption Events and Changing-look Active Galactic Nuclei via Variation in Mid-infrared Color. YAO Y., YE J., SUN L., et al.
2025A&A...703A..81F 485       D     X         11 29 ~ Polarimetric diversity in tidal disruption events: Comparative study of low-polarised sources with AT2020mot. FLORIS A., LIODAKIS I., KOLJONEN K.I.I., et al.
2025A&A...704A.250J 373           X C F     6 21 ~ Optical polarisation of stellar-fed active and quiescent supermassive black holes. JORDANA-MITJANS N., FRANCKOWIAK A., RAMIREZ-RUIZ E., et al.
2026A&A...705A.250W 50           X         1 28 ~ Revisiting the unification of tidal disruption events with polarimetry. WICHERN H.C.I., LELOUDAS G., PURSIAINEN M., et al.
2026A&A...706A.324V viz 150           X C       2 41 ~ Back from the dead: AT2019aalc as a candidate repeating tidal disruption event in an active galactic nucleus. VERES P.M., FRANCKOWIAK A., VAN VELZEN S., et al.
2026ApJ...999..181Z 70       D     X         2 54 ~ TTC: Transformer-based TDE Classifier for the Wide Field Survey Telescope (WFST). ZHENG R., LIN Z., KONG X., et al.
2026A&A...707A.171L viz 350           X C       6 68 ~ Repeating flares, X-ray outbursts and delayed infrared emission: A comprehensive compilation of optical tidal disruption events TDECat. LANGIS D.A., LIODAKIS I., KOLJONEN K.I.I., et al.
2026A&A...707L..19V 170       D     X C       3 25 ~ Precursors in tidal disruption events: Repeating, fast, and active galactic nucleus-hosted TDEs. VERES P.M.

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