Tripling the Census of Dwarf AGN Candidates Using DESI Early Data

  • Ragadeepika Pucha
  • , S. Juneau
  • , Arjun Dey
  • , M. Siudek
  • , M. Mezcua
  • , J. Moustakas
  • , S. BenZvi
  • , K. Hainline
  • , R. Hviding
  • , Yao Yuan Mao
  • , D. M. Alexander
  • , R. Alfarsy
  • , C. Circosta
  • , Wei Jian Guo
  • , V. Manwadkar
  • , P. Martini
  • , B. A. Weaver
  • , J. Aguilar
  • , S. Ahlen
  • , D. Bianchi
  • D. Brooks, R. Canning, T. Claybaugh, K. Dawson, A. de la Macorra, Biprateep Dey, P. Doel, A. Font-Ribera, J. E. Forero-Romero, E. Gaztañaga, S. Gontcho A Gontcho, G. Gutierrez, K. Honscheid, R. Kehoe, S. E. Koposov, A. Lambert, M. Landriau, L. Le Guillou, A. Meisner, R. Miquel, F. Prada, G. Rossi, E. Sanchez, D. Schlegel, M. Schubnell, H. Seo, D. Sprayberry, G. Tarlé, H. Zou

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

Using early data from the Dark Energy Spectroscopic Instrument (DESI) survey, we search for active galactic nuclei (AGN) signatures in 410,757 line-emitting galaxies. By employing the BPT emission-line ratio diagnostic diagram, we identify AGNs in 75,928/296,261 (≈25.6%) high-mass ( log ( M ⋆ / M ⊙ ) > 9.5) and 2444/114,496 (≈2.1%) dwarf ( log ( M ⋆ / M ⊙ ) ≤ 9.5) galaxies. Of these AGN candidates, 4181 sources exhibit a broad Hα component, allowing us to estimate their BH masses via virial techniques. This study more than triples the census of dwarf AGNs and doubles the number of intermediate-mass black hole (MBH ≤ 106M) candidates, spanning a broad discovery space in stellar mass (7 < log ( M ⋆ / M ⊙ ) < 12) and redshift (0.001 <z < 0.45). The observed AGN fraction in dwarf galaxies (≈2.1%) is nearly four times higher than prior estimates, primarily due to DESI’s smaller fiber size, which enables the detection of lower-luminosity dwarf AGN candidates. We also extend the MBH-M scaling relation down to log ( M ⋆ / M ⊙ ) ≈ 8.5 and log ( M BH / M ⊙ ) ≈ 4.4, with our results aligning well with previous low-redshift studies. The large statistical sample of dwarf AGN candidates from current and future DESI releases will be invaluable for enhancing our understanding of galaxy evolution at the low-mass end of the galaxy mass function.

Original languageEnglish (US)
Article number10
JournalAstrophysical Journal
Volume982
Issue number1
DOIs
StatePublished - Mar 20 2025

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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