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PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field * * Partly based on observations taken with the MMT, a joint facility operated by the University of Arizona and the Smithsonian Institution.

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

PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field * * Partly based on observations taken with the MMT, a joint facility operated by the University of Arizona and the Smithsonian Institution. Thumbnail


Authors

Christopher N. A. Willmer

Chun Ly

Satoshi Kikuta

S. A. Kattner

Rolf A. Jansen

Seth H. Cohen

Rogier A. Windhorst

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



Abstract

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 arcmin2 in Y, H, and K, and 313 arcmin2 in J. Using Monte Carlo simulations, we estimate a 1σ 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.

Citation

Willmer, C. N. A., Ly, C., Kikuta, S., Kattner, S. A., Jansen, R. A., Cohen, S. H., …Grogin, N. A. (2023). PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field * * Partly based on observations taken with the MMT, a joint facility operated by the University of Arizona and the Smithsonian Institution. Astrophysical Journal Supplement, 269(1), Article 21. https://doi.org/10.3847/1538-4365/acf57d

Journal Article Type Article
Acceptance Date Aug 28, 2023
Online Publication Date Nov 1, 2023
Publication Date 2023-11
Deposit Date Nov 10, 2023
Publicly Available Date Nov 10, 2023
Journal The Astrophysical Journal Supplement Series
Print ISSN 0067-0049
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 269
Issue 1
Article Number 21
DOI https://doi.org/10.3847/1538-4365/acf57d
Keywords Galaxy evolution, Galaxy photometry, Catalogs, Galaxy counts, Surveys
Public URL https://durham-repository.worktribe.com/output/1884004

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