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“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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Metadata
- 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
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