Cited by 98Galaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysical ResearchStellar, planetary, and galactic studies

Spectroscopic needs for imaging dark energy experiments

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Newman, Jeffrey A., Abate, Alexandra, Abdalla, Filipe B., Allam, Sahar, Allen, Steven W., Ansari, Réza, Bailey, Stephen, Barkhouse, Wayne A. +55 more·2015·Astroparticle Physics

Integrity signals

Registry

Crossref · 10.1016/j.astropartphys.2014.06.007

Cites

97 of 97 references verified0 citation errors · 0 not checkable

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  • Requiring more training data than currently exists to define the template set degrades the expected σ/(1+z) to about 0.05, which is still within the expected range for a Stage IV dark energy experiment.

    “The degradation in photometric redshift quality associated with requiring more training data than currently exists to de fi ne the template set increases the expected σ / ( 1 + z ) to ∼ 0.05 ( e.g., Newman et al. 2015; Graham et al. 2018 ) , which is still well within the expected range for a Stage IV dark energy experiment.”

    From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Newman et al. 2015

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Authors
Newman, J. A., Abate, A., Abdalla, F. B., Allam, S., Allen, S. W., Ansari, R., Bailey, S., Barkhouse, W. A., Beers, T. C., Blanton, M. R., Brodwin, M., Brownstein, J. R., Brunner, R. J., Carrasco Kind, M., Cervantes-Cota, J. L., Cheu, E., Chisari, N. E., Colless, M., Comparat, J., Coupon, J., Cunha, C. E., de la Macorra, A., Dell’Antonio, I. P., Frye, B. L., Gawiser, E. J., Gehrels, N., Grady, K., Hagen, A., Hall, P. B., Hearin, A. P., Hildebrandt, H., Hirata, C. M., Ho, S., Honscheid, K., Huterer, D., Ivezić, Ž., Kneib, J.-P., Kruk, J. W., Lahav, O., Mandelbaum, R., Marshall, J. L., Matthews, D. J., Ménard, B., Miquel, R., Moniez, M., Moos, H. W., Moustakas, J., Myers, A. D., Papovich, C., Peacock, J. A., Park, C., Rahman, M., Rhodes, J., Ricol, J.-S., Sadeh, I., Slozar, A., Schmidt, S. J., Stern, D. K., Anthony Tyson, J., von der Linden, A., Wechsler, R. H., Wood-Vasey, W. M., & Zentner, A. R.
Affiliations
  • University of Pittsburgh (US)
  • University of Arizona (US)
  • University College London (GB)
  • Fermi National Accelerator Laboratory (US)
  • Université Paris-Sud (FR)
  • Lawrence Berkeley National Laboratory (US)
  • University of North Dakota (US)
  • New York University (US)
  • University of Missouri–Kansas City (US)
  • University of Utah (US)
  • University of Illinois Urbana-Champaign (US)
  • Princeton University (US)
  • Australian National University (AU)
  • Consejo Superior de Investigaciones Científicas (ES)
  • University of Geneva (CH)
  • Stanford University (US)
  • Brown University (US)
  • Rutgers, The State University of New Jersey (US)
  • Goddard Space Flight Center (US)
  • Pennsylvania State University (US)
  • York University (CA)
  • Yale University (US)
  • The Ohio State University (US)
  • Carnegie Mellon University (US)
  • University of Washington (US)
  • Aix-Marseille Université (FR)
  • Texas A&M University (US)
  • Johns Hopkins University (US)
  • Universitat Autònoma de Barcelona (ES)
  • Université Paris-Saclay (FR)
  • University of Wyoming (US)
  • University of Edinburgh (GB)
  • Korea Institute for Advanced Study (KR)
  • California Institute of Technology (US)
  • Université Grenoble Alpes (FR)
  • University of California, Davis (US)
Corresponding author
Newman, Jeffrey A.
Venue
Astroparticle Physics
Publisher
Elsevier BV
Published
2015-03
Volume
63
Pages
81-100
ISSN
0927-6505 (ISSN-L)
OpenAlex
W1516039273
Cited by
98
References
104
Citations by year
2026: 7 · 2025: 9 · 2024: 4 · 2023: 4 · 2022: 12 · 2021: 5 · 2020: 8 · 2019: 8 · 2018: 7 · 2017: 12 · 2016: 15 · 2015: 3 · 2014: 3
FWCI
5.93
Type
journal article
Language
en
Update notices
erratum (2015-05-01)
Open access
Locations
  • Astroparticle Physics (acceptedVersion)
  • HAL (submittedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • ANU Open Research (Australian National University) (submittedVersion)
  • OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
  • UND Scholarly Commons (University of North Dakota) (submittedVersion, cc-by-nc-nd)
  • UCL Discovery (University College London) (submittedVersion)
  • Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion)
  • Infoscience (Ecole Polytechnique Fédérale de Lausanne) (submittedVersion, cc-by-nc-nd)
Funders
  • US Department of Energy
  • ERC
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
spectroscopic redshifts, photometric redshifts, dark energy, galaxy spectroscopy, Giant Magellan Telescope, Extremely Large Telescope, systematic and random errors

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.

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