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JWST advanced deep extragalactic survey: NIRCam imaging to z > 10

Published online by Cambridge University Press:  04 June 2020

Marcia Rieke Open the ORCID record for Marcia Rieke [Opens in a new window]
Marcia Rieke*
Affiliation:
Steward Observatory, University of Arizona, 933 N. Cherry, Tucson, AZ85721USA email: [email protected]
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Abstract

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The JWST Advanced Deep Extragalactic Survey (JADES) is a joint program of the JWST NIRCam and NIRSpec Guaranteed Time Observation (GTO) teams involving over 800 hours of observation. This paper describes the imaging portion of the program which covers nearly 200 square arc minutes divided between two well-studied fields with excellent supporting data (e.g. from Chandra, ALMA, and HST-CANDELS): GOODS North and South, including the Ultra Deep Field. NIRCam imaging will enable the study of galaxy evolution to z ∼ 10 and higher using multi-color imaging with 9 filters covering 0.9 to 5 microns. Such data will provide photometric redshifts and a wealth of data for constructing luminosity and mass functions. A key component of the program is rapid turn around of imaging into NIRSpec target lists. Preparing for this program has benefited from the development of a mock catalog and simulated imaging to test these processes.

Keywords

galaxies: evolutiongalaxies: high-redshiftsurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S352: Uncovering Early Galaxy Evolution in the ALMA and JWST Era , June 2019 , pp. 337 - 341
Copyright
© International Astronomical Union 2020

References

Cowley, W., Baugh, C. M.Cole, S., Frenk, C. S., & Lacey, C. G. 2018, MNRAS, 474, 235210.1093/mnras/stx2897CrossRefGoogle Scholar
Dressler, A. 1996, HST and Beyond (Washington: Association of Universities for Research in Astronomy)Google Scholar
Grogin, N. A, Kocevski, D. D., Faber, S. M., Ferguson, H. C., Koekemoer, A. M., et al. 2011, ApJS, 207, 24Google Scholar
Rasappu, N., Smit, R., Labbe, I., Stark, D. P.Ellis, R. S., & Oesch, P. A. 2016, MNRAS, 461, 388610.1093/mnras/stw1484CrossRefGoogle Scholar
Williams, C. C., Curtis-Lake, E., Hainline, K. N., Chevallard, J., Robertson, B. E., Charlot, S., Endsley, R., Stark, D. P., Willmer, C. N. A., Alberts, S., Amorin, R., Arribas, S., Baum, S., Bunker, A., Carniani, S., Crandall, S., Egami, E., Eisenstein, D. J., Ferruit, P., Husemann, B., Maseda, M., Maiolino, R., Rawle, T. D., Rieke, M., Smit, R., Tacchella, S., & Willott, C. J. 2018, ApJS, 236, 3310.3847/1538-4365/aabcbbCrossRefGoogle Scholar