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JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results

  • Authors: Rogier A. Windhorst, Seth H. Cohen, Rolf A. Jansen, Jake Summers, Scott Tompkins, Christopher J. Conselice, Simon P. Driver, Haojing Yan, Dan Coe, Brenda Frye, Norman Grogin, Anton Koekemoer, Madeline A. Marshall, Rosalia O'Brien, Nor Pirzkal, Aaron Robotham, Russell E. Ryan, Christopher N. A. Willmer, Timothy Carleton, Jose M. Diego, William C. Keel, Paolo Porto, Caleb Redshaw, Sydney Scheller, Stephen M. Wilkins, S. P. Willner, Adi Zitrin, Nathan J. Adams, Duncan Austin, Richard G. Arendt, John F. Beacom, Rachana A. Bhatawdekar, Larry D. Bradley, Tom Broadhurst, Cheng Cheng, Francesca Civano, Liang Dai, Hervé Dole, Jordan C. J. D'Silva, Kenneth J. Duncan, Giovanni G. Fazio, Giovanni Ferrami, Leonardo Ferreira, Steven L. Finkelstein, Lukas J. Furtak, Hansung B. Gim, Alex Griffiths, Heidi B. Hammel, Kevin C. Harrington, Nimish P. Hathi, Benne W. Holwerda, Rachel Honor, Jia-Sheng Huang, Minhee Hyun, Myungshin Im, Bhavin A. Joshi, Patrick S. Kamieneski, Patrick Kelly, Rebecca L. Larson, Juno Li, Jeremy Lim, Zhiyuan Ma, Peter Maksym, Giorgio Manzoni, Ashish Kumar Meena, Stefanie N. Milam, Mario Nonino, Massimo Pascale, Andreea Petric, Justin D. R. Pierel, Maria del Carmen Polletta, Huub J. A. Röttgering, Michael J. Rutkowski, Ian Smail, Amber N. Straughn, Louis-Gregory Strolger, Andi Swirbul, James A. A. Trussler, Lifan Wang, Brian Welch, J. Stuart B. Wyithe, Min Yun, Erik Zackrisson, Jiashuo Zhang, Xiurui Zhao

Rogier A. Windhorst et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 6.

Object detection, classification, and counts in the El Gordo noncluster module in the F090W, F115W, F150W, and F200W filters. (a) (Left): SourceExtractor AB-magnitude error bars vs. MAG_AUTO AB-mag resulting from the adopted SourceExtractor-parameters (Section 3.1). Horizontal dashed lines show the adopted 5σ point-source detection limits (Table 1). (b) (Middle): star–galaxy classification diagram based on SourceExtractor MAG_AUTO AB-magnitudes vs. image FWHM. Left solid vertical lines indicate the NIRCam diffraction limit for each image with its current sampling. Blue points represent galaxies. The box to the right of the vertical line identifies objects classified as stars (red points). Objects with FWHM < FWHM(PSF) have been flagged and removed from this plot as spurious detections or border imperfections. The green dashed lines indicate for each image the effective point-source (horizontal) and SB (slanted) detection limits. (c) (Right): resulting star counts (red) and galaxy counts (blue). The vertical dashed line is the limit to which stellar objects are defined.

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