The many flavours of photometric redshifts
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Photometric redshift estimation is a task of great importance to sky surveys.
“Thus, a task of great importance to sky surveys is photometric redshift (photoz ) estimation (for a recent review, see Salvato et al. 2019).”
From Self-supervised Representation Learning for Astronomical Images (2021) · cites this paper as Salvato et al. 2019
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MAGPHYS+photo-z: Constraining the Physical Properties of Galaxies with Unknown Redshifts
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Foreword to the Focus Issue on Machine Intelligence in Astronomy and Astrophysics
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A comparison of photometric redshift techniques for large radio surveys
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A Comparison of Photometric Redshift Techniques for Large Radio Surveys
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Self-citationPhotometric redshifts for the Pan-STARRS1 survey
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Exploring galactic properties with machine learning
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Stellar Mass Calibrations for Local Low-mass Galaxies
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Identifying AGN Host Galaxies by Machine Learning with HSC+WISE
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Simulation-based inference of deep fields: galaxy population model and redshift distributions
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Estimating Galaxy Parameters with Self-organizing Maps and the Effect of Missing Data
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Photometric classification of Hyper Suprime-Cam transients using machine learning
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Surveys of the Cosmic X-Ray Background
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A Photometric Redshift Catalogue of Galaxies from the DESI Legacy Imaging Surveys DR10
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Photometric redshifts for the Pan-STARRS1 survey
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Li, S., Kuijken, K. H., Hoekstra, H., Hildebrandt, H., Joachimi, B., & Kannawadi, A. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202039254 · Cited by 12 · see citing works
- Authors
- Salvato, M., Ilbert, O., & Hoyle, B.
- Affiliations
- Max Planck Institute for Extraterrestrial Physics (DE)
- Laboratoire d’Astrophysique de Marseille (FR)
- Corresponding author
- Salvato, Mara
- Ilbert, Olivier
- Hoyle, Ben
- Venue
- Nature Astronomy
- Published
- 2018-06-04
- Volume
- 3
- Issue
- 3
- Pages
- 212-222
- ISSN
- 2397-3366 (ISSN-L)
- OpenAlex
- W2963284157
- Cited by
- 234
- References
- 156
- Citations by year
- 2026: 23 · 2025: 31 · 2024: 36 · 2023: 25 · 2022: 35 · 2021: 35 · 2020: 22 · 2019: 25 · 2018: 2
- FWCI
- 11.30
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- Locations
- Nature Astronomy (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion, other-oa)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- photometric redshifts, cosmological distances, template fitting, machine learning, redshift accuracy, survey strategy, wide-field survey, dark energy, stellar mass assembly, galaxy evolution
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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