THE IMPACT OF JWST BROADBAND FILTER CHOICE ON PHOTOMETRIC REDSHIFT ESTIMATION

The determination of galaxy redshifts in the James Webb Space Telescope's (JWST) blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST's Near-Infrared Camera (NIRCam) at 0.6-5.0 mu m and Mid Infrared Instrument (MIRI) at lambda > 5.0 mm. In th...

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Bibliographic Details
Main Authors:	Bisigello, L., Caputi, K. I., Colina, L., Fèvre, O. Le, Nørgaard-Nielsen, H. U., Pérez-González, P. G., Pye, J., Werf, P. van der, Ilbert, O., Grogin, N., Koekemoer, A.
Other Authors:	Univ Arizona, Steward Observ
Language:	en
Published:	IOP PUBLISHING LTD 2016
Subjects:	galaxies: distances and redshifts galaxies: high-redshift galaxies: photometry
Online Access:	http://hdl.handle.net/10150/622361 http://arizona.openrepository.com/arizona/handle/10150/622361

Internet

http://hdl.handle.net/10150/622361
http://arizona.openrepository.com/arizona/handle/10150/622361

THE IMPACT OF JWST BROADBAND FILTER CHOICE ON PHOTOMETRIC REDSHIFT ESTIMATION

Internet

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