The Astrophysical Journal (Jan 2024)

PEARLS: Discovery of Point-source Features within Galaxies in the North Ecliptic Pole Time Domain Field

  • Rafael Ortiz III,
  • Rogier A. Windhorst,
  • Seth H. Cohen,
  • Steven P. Willner,
  • Rolf A. Jansen,
  • Timothy Carleton,
  • Patrick S. Kamieneski,
  • Michael J. Rutkowski,
  • Brent M. Smith,
  • Jake Summers,
  • Cheng Cheng,
  • Dan Coe,
  • Christopher J. Conselice,
  • Jose M. Diego,
  • Simon P. Driver,
  • Jordan C. J. D’Silva,
  • Brenda L. Frye,
  • Hansung B. Gim,
  • Norman A. Grogin,
  • Heidi B. Hammel,
  • Nimish P. Hathi,
  • Benne W. Holwerda,
  • Minhee Hyun,
  • Myungshin Im,
  • William C. Keel,
  • Anton M. Koekemoer,
  • Juno Li,
  • Madeline A. Marshall,
  • Tyler J. McCabe,
  • Noah J. McLeod,
  • Stefanie N. Milam,
  • Rosalia O’Brien,
  • Nor Pirzkal,
  • Aaron S. G. Robotham,
  • Russell E. Ryan Jr.,
  • Christopher N. A. Willmer,
  • Haojing Yan,
  • Min S. Yun,
  • Adi Zitrin

DOI
https://doi.org/10.3847/1538-4357/ad6d5e
Journal volume & issue
Vol. 974, no. 2
p. 258

Abstract

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The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as seen in the longer-wavelength filters. We visually identified a sample of 66 galaxies (∼1 galaxy arcmin ^–2 ) with pointlike cores and have modeled their two-dimensional light profiles with GalFit , identifying 16 galactic nuclei with measurable point-source components. GalFit suggests that the visual sample is a mix of both compact stellar bulge and point-source galaxy cores. This core classification is complemented by spectral energy distribution modeling to infer the sample’s active galactic nucleus (AGN) and host-galaxy parameters. For galaxies with measurable point-source components, the median fractional AGN contribution to their 0.1–30.0 μ m flux is 0.44, and 14/16 are color-classified AGN. We conclude that near-infrared point-source galaxy cores are signatures of AGN. In addition, we define an automated sample-selection criterion to identify these point-source features. This criterion can be used in other extant and future NIRCam images to streamline the search for galaxies with unresolved IR-luminous AGN. The James Webb Space Telescope’s superb angular resolution and sensitivity at infrared wavelengths are resurrecting the morphological identification of AGN.

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