Christopher N. A. Willmer
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.
Authors
Chun Ly
Satoshi Kikuta
S. A. Kattner
Rolf A. Jansen
Seth H. Cohen
Rogier A. Windhorst
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
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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Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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