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A Large-scale Search for Photometrically Variable Active Galactic Nuclei in Dwarf Galaxies Using the Young Supernova Experiment

Title: A Large-scale Search for Photometrically Variable Active Galactic Nuclei in Dwarf Galaxies Using the Young Supernova Experiment
Authors: Messick, A; Baldassare, V; Jones, DO; French, KD; Raimundo, SI; Earl, N; Auchettl, K; Coulter, DA; Huber, ME; Verrico, ME; de Boer, T; Chambers, KC; Gao, H; Lin, CC; Wainscoat, RJ
Publisher Information: American Astronomical Society
Publication Year: 2025
Collection: The University of Melbourne: Digital Repository
Description: We conduct an analysis of over 60,000 dwarf galaxies ( 7 ≲ log M * / M ⊙ ≲ 10 ) in search of photometric variability indicative of active galactic nuclei (AGNs). Using data from the Young Supernova Experiment, a time domain survey on the Pan-STARRS telescopes, we construct light curves for each galaxy in up to four bands (griz) where available. We select objects with AGN-like variability by fitting each light curve with a damped random walk (DRW) model. After quality cuts and removing transient contaminants, we identify 1100 variability-selected AGN candidates (representing 2.4% of the available sample). We analyze their spectra to measure various emission lines and calculate black hole (BH) masses, finding general agreement with previously found mass scaling relations and nine potential intermediate-mass BH candidates. Furthermore, we reanalyze the light curves of our candidates to calculate the dampening timescale τ DRW associated with the DRW and see a similar correlation between this value and the BH mass. Finally, we estimate the active fraction as a function of stellar mass and see evidence that the active fraction increases with host mass.
Document Type: article in journal/newspaper
Language: unknown
ISSN: 0004-637X
Relation: https://hdl.handle.net/11343/365987
Availability: https://hdl.handle.net/11343/365987
Rights: https://creativecommons.org/licenses/by/4.0/ ; CC-BY
Accession Number: edsbas.44CEF55A
Database: BASE