Photometric Redshifts for Next-Generation Surveys

Newman, Jeffrey A.; Gruen, Daniel

doi:10.1146/annurev-astro-032122-014611

Photometric Redshifts for Next-Generation Surveys

Journal Article · 18 August 2022 · Annual Review of Astronomy and Astrophysics

DOI:https://doi.org/10.1146/annurev-astro-032122-014611· OSTI ID:1980841

Newman, Jeffrey A. ^[1]; Gruen, Daniel ^[2]

Department of Physics and Astronomy and Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh, Pittsburgh, Pennsylvania, USA,
University Observatory, Faculty of Physics, Ludwig-Maximilians-Universität, Munich, Germany

Photometric redshifts are essential in studies of both galaxy evolution and cosmology, as they enable analyses of objects too numerous or faint for spectroscopy. The Rubin Observatory, Euclid, and Roman Space Telescope will soon provide a new generation of imaging surveys with unprecedented area coverage, wavelength range, and depth. To take full advantage of these data sets, further progress in photometric redshift methods is needed. In this review, we focus on the greatest common challenges and prospects for improvement in applications of photometric redshifts to the next generation of surveys: ∙ Gains in performance (i.e., the precision of redshift estimates for individual galaxies) could greatly enhance studies of galaxy evolution and some probes of cosmology. ∙ Improvements in characterization (i.e., the accurate recovery of redshift distributions of galaxies in the presence of uncertainty on individual redshifts) are urgently needed for cosmological measurements with next-generation surveys. To achieve both of these goals, improvements in the scope and treatment of the samples of spectroscopic redshifts that make high-fidelity photometric redshifts possible will also be needed. For the full potential of the next generation of surveys to be reached, the characterization of redshift distributions must improve by roughly an order of magnitude compared with the current state of the art, requiring progress on a wide variety of fronts. We conclude by presenting a speculative evaluation of how photometric redshift methods and the collection of the necessary spectroscopic samples may improve by the time near-future surveys are completed.

Research Organization:: Univ. of Pittsburgh, PA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

DOE Contract Number:: SC0007914; SC0020256

OSTI ID:: 1980841

Journal Information:: Annual Review of Astronomy and Astrophysics, Vol. 60, Issue 1; ISSN 0066-4146

Publisher:: Annual Reviews

Country of Publication:: United States

Language:: English

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