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

被引:2
|
作者
Willmer, Christopher N. A. [1 ]
Ly, Chun [1 ]
Kikuta, Satoshi [2 ]
Kattner, S. A. [3 ]
Jansen, Rolf A. [4 ]
Cohen, Seth H. [4 ]
Windhorst, Rogier A. [4 ]
Smail, Ian [5 ]
Tompkins, Scott [4 ]
Beacom, John F. [6 ,7 ,8 ]
Cheng, Cheng [9 ]
Conselice, Christopher J. [10 ]
Frye, Brenda L. [1 ]
Koekemoer, Anton M. [11 ]
Hathi, Nimish [11 ]
Hyun, Minhee [12 ]
Im, Myungshin [13 ]
Willner, S. P. [14 ]
Zhao, X. [14 ]
Brisken, Walter A. [15 ]
Civano, F. [16 ]
Cotton, William [17 ]
Hasinger, Guenther [18 ]
Maksym, W. Peter [14 ]
Rieke, Marcia J. [1 ]
Grogin, Norman A. [11 ]
机构
[1] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA
[2] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[3] Univ Arizona, MMT Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA
[4] Arizona State Univ, Sch Earth & Space Explorat, 550 E Tyler Mall, Tempe, AZ 85287 USA
[5] Univ Durham, Ctr Extragalact Astron, Dept Phys, South Rd, Durham DH1 3LE, England
[6] Ctr Cosmol & AstroParticle Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA
[7] Ohio State Univ, Dept Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA
[8] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
[9] Chinese Acad Sci, South Amer Ctr Astron, Natl Astron Observ, Beijing 100101, Peoples R China
[10] Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, England
[11] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[12] Korea Astron & Space Sci Inst, 776 Daedeok Daero, Daejeon 34055, South Korea
[13] Seoul Natl Univ, Astron Res Ctr, Dept Phys & Astron, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea
[14] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[15] Long Baseline Observ, 1003 Lopezville Rd, Socorro, NM 87801 USA
[16] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[17] Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA
[18] European Space Astron Ctr ESAC, ESA, Camino Bajo CastilloS-N, E-28692 Madrid, Spain
来源
基金
新加坡国家研究基金会;
关键词
GALAXY NUMBER COUNTS; DATA RELEASE; DEEP; FAINT; EVOLUTION; MAGNITUDE; REDUCTION; SOFTWARE; CATALOG; STARS;
D O I
10.3847/1538-4365/acf57d
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 sigma 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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页数:17
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