The Astrophysical Journal Supplement Series (Jan 2023)

PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field

  • Christopher N. A. Willmer,
  • Chun Ly,
  • Satoshi Kikuta,
  • S. A. Kattner,
  • Rolf A. Jansen,
  • Seth H. Cohen,
  • Rogier A. Windhorst,
  • Ian Smail,
  • Scott Tompkins,
  • John F. Beacom,
  • Cheng Cheng,
  • Christopher J. Conselice,
  • Brenda L. Frye,
  • Anton M. Koekemoer,
  • Nimish Hathi,
  • Minhee Hyun,
  • Myungshin Im,
  • S. P. Willner,
  • X. Zhao,
  • Walter A. Brisken,
  • F. Civano,
  • William Cotton,
  • Günther Hasinger,
  • W. Peter Maksym,
  • Marcia J. Rieke,
  • Norman A. Grogin

DOI
https://doi.org/10.3847/1538-4365/acf57d
Journal volume & issue
Vol. 269, no. 1
p. 21

Abstract

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We present near-infrared (NIR) ground-based Y , J , H , and K imaging obtained in the James Webb Space Telescope (JWST) North Ecliptic Pole Time Domain Field (NEP TDF) using the MMT-Magellan Infrared Imager and Spectrometer on the MMT. These new observations cover a field of approximately 230 arcmin ^2 in Y , H , and K, and 313 arcmin ^2 in J . Using Monte Carlo simulations, we estimate a 1 σ depth relative to the background sky of ( Y, J, H, K ) = (23.80, 23.53, 23.13, 23.28) in AB magnitudes for point sources at a 95% completeness level. These observations are part of the ground-based effort to characterize this region of the sky, supplementing space-based data obtained with Chandra, NuSTAR, XMM, AstroSat, Hubble Space Telescope, and JWST. This paper describes the observations and reduction of the NIR imaging and combines these NIR data with archival imaging in the visible, obtained with the Subaru Hyper-Suprime-Cam, to produce a merged catalog of 57,501 sources. The new observations reported here, plus the corresponding multiwavelength catalog, will provide a baseline for time-domain studies of bright sources in the NEP TDF.

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