Photometric Redshift Estimation

Photometric Redshift Estimation is a method in observational astronomy that determines the redshift of celestial objects by comparing their observed fluxes across multiple broad- or intermediate-band filters in a photometric system to template spectral energy distributions, distinguishing it from spectroscopic techniques by relying on broadband photometry rather than high-resolution spectral features.

775

Publications

62.9K

Citations

3.5K

Authors

741

Institutions

Publications per year

2017–2026

233

Variants

Photo-z Estimation

Authors

3.5K

  1. ES
    E. Sánchez

    University of Michigan, United States

    37 publications · 4.7K citations

    31

    h-index

  2. EG
    E. Gaztañaga

    Institute of Space Sciences, Spain

    33 publications · 4.1K citations

    31

    h-index

  3. FJ
    F. J. Castander

    Institute of Space Sciences, Spain

    38 publications · 4.5K citations

    29

    h-index

  4. IS
    I. Sevilla-Noarbe

    Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Spain

    33 publications · 4.3K citations

    28

    h-index

  5. OL
    O. Lahav

    University College London, United Kingdom

    27 publications · 4.4K citations

    27

    h-index

1–5 of 3.5K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    232 publications · 17.1K citations

    71

    h-index

  2. The Astrophysical Journal

    ApJ · 164 publications · 17.3K citations

    68

    h-index

  3. Astronomy and Astrophysics

    99 publications · 8.8K citations

    45

    h-index

  4. The Astronomical Journal

    AJ · 48 publications · 4K citations

    33

    h-index

  5. The Astrophysical Journal Supplement Series

    28 publications · 3.3K citations

    23

    h-index

1–5