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Identifying Active Galactic Nuclei at z ∼ 3 from the HETDEX Survey Using Machine Learning

Tardugno Poleo, Valentina; Finkelstein, Steven L.; Leung, Gene; Mentuch Cooper, Erin; Gebhardt, Karl; Farrow, Daniel J.; Gawiser, Eric; Zeimann, Greg; Schneider, Donald P.; Morabito, Leah; Mock, Daniel; Liu, Chenxu

Authors

Valentina Tardugno Poleo

Steven L. Finkelstein

Gene Leung

Erin Mentuch Cooper

Karl Gebhardt

Eric Gawiser

Greg Zeimann

Donald P. Schneider

Leah Morabito

Daniel Mock

Chenxu Liu



Abstract

We used data from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) to study the incidence of AGN in continuum-selected galaxies at z ∼ 3. From optical and infrared imaging in the 24 deg2 Spitzer HETDEX Exploratory Large Area survey, we constructed a sample of photometric-redshift selected z ∼ 3 galaxies. We extracted HETDEX spectra at the position of 716 of these sources and used machine-learning methods to identify those which exhibited AGN-like features. The dimensionality of the spectra was reduced using an autoencoder, and the latent space was visualized through t-distributed stochastic neighbor embedding. Gaussian mixture models were employed to cluster the encoded data and a labeled data set was used to label each cluster as either AGN, stars, high-redshift galaxies, or low-redshift galaxies. Our photometric redshift (photoz) sample was labeled with an estimated 92% overall accuracy, an AGN accuracy of 83%, and an AGN contamination of 5%. The number of identified AGN was used to measure an AGN fraction for different magnitude bins. The ultraviolet (UV) absolute magnitude where the AGN fraction reaches 50% is M UV = −23.8. When combined with results in the literature, our measurements of AGN fraction imply that the bright end of the galaxy luminosity function exhibits a power law rather than exponential decline, with a relatively shallow faint-end slope for the z ∼ 3 AGN luminosity function.

Citation

Tardugno Poleo, V., Finkelstein, S. L., Leung, G., Mentuch Cooper, E., Gebhardt, K., Farrow, D. J., …Liu, C. (2023). Identifying Active Galactic Nuclei at z ∼ 3 from the HETDEX Survey Using Machine Learning. Astronomical Journal, 165(4), Article 153. https://doi.org/10.3847/1538-3881/acba92

Journal Article Type Article
Acceptance Date Feb 7, 2023
Online Publication Date Mar 10, 2023
Publication Date Apr 1, 2023
Deposit Date Apr 17, 2024
Publicly Available Date Apr 23, 2024
Journal Astronomical Journal
Print ISSN 0004-6256
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 165
Issue 4
Article Number 153
DOI https://doi.org/10.3847/1538-3881/acba92
Public URL https://hull-repository.worktribe.com/output/4626508

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0

Copyright Statement
© 2023. The Author(s). Published by the American Astronomical Society.
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.




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