The Astrophysical Journal (Jan 2025)

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

DOI
https://doi.org/10.3847/1538-4357/adb1dd
Journal volume & issue
Vol. 982, no. 1
p. 10

Abstract

Read online

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 ( $\mathrm{log}({M}_{\star }/{M}_{\odot })\,\gt $ 9.5) and 2444/114,496 (≈2.1%) dwarf ( $\mathrm{log}({M}_{\star }/{M}_{\odot })\,\leqslant $ 9.5) galaxies. Of these AGN candidates, 4181 sources exhibit a broad H α 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 ( M _BH ≤ 10 ^6 M _⊙ ) candidates, spanning a broad discovery space in stellar mass (7 $\lt \mathrm{log}({M}_{\star }/{M}_{\odot })\,\lt $ 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 M _BH – M _⋆ scaling relation down to ${\rm{log}}({M}_{\star }/{M}_{\odot })\,\approx $ 8.5 and $\mathrm{log}({M}_{\mathrm{BH}}/{M}_{\odot })\,\approx $ 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.

Keywords