ELG spectroscopic systematics analysis of the DESI Data Release 1
J. Yu et al. -- Dark Energy Spectroscopic Instrument (DESI) survey Year 1 results. -- ArXiv ePrint: 2405.16657
| Autores: | , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/385425 |
| Acesso em linha: | http://hdl.handle.net/10261/385425 |
| Access Level: | acceso abierto |
| Palavra-chave: | Cosmological parameters from LSS Galaxy clustering Galaxy surveys Redshift surveys |
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| dc.title.none.fl_str_mv |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| title |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| spellingShingle |
ELG spectroscopic systematics analysis of the DESI Data Release 1 Yu, Jiaxi Cosmological parameters from LSS Galaxy clustering Galaxy surveys Redshift surveys |
| title_short |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| title_full |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| title_fullStr |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| title_full_unstemmed |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| title_sort |
ELG spectroscopic systematics analysis of the DESI Data Release 1 |
| dc.creator.none.fl_str_mv |
Yu, Jiaxi Gaztañaga, Enrique Prada, Francisco |
| author |
Yu, Jiaxi |
| author_facet |
Yu, Jiaxi Gaztañaga, Enrique Prada, Francisco |
| author_role |
author |
| author2 |
Gaztañaga, Enrique Prada, Francisco |
| author2_role |
author author |
| dc.contributor.none.fl_str_mv |
National Science Foundation (US) Department of Energy (US) Science and Technology Facilities Council (UK) Gordon and Betty Moore Foundation Heising Simons Foundation Commissariat à l'Ènergie Atomique et aux Ènergies Alternatives (France) Consejo Nacional de Humanidades, Ciencias y Tecnologías (México) Ministerio de Ciencia e Innovación (España) Yu, Jiaxi [0009-0001-7217-8006] Gaztañaga, Enrique [0000-0001-9632-0815] Prada, Francisco [0000-0001-7145-8674] Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Cosmological parameters from LSS Galaxy clustering Galaxy surveys Redshift surveys |
| topic |
Cosmological parameters from LSS Galaxy clustering Galaxy surveys Redshift surveys |
| description |
J. Yu et al. -- Dark Energy Spectroscopic Instrument (DESI) survey Year 1 results. -- ArXiv ePrint: 2405.16657 |
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2025 |
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2025 2025 2025 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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publishedVersion |
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http://hdl.handle.net/10261/385425 |
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http://hdl.handle.net/10261/385425 |
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Inglés |
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Inglés |
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The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1088/1475-7516/2025/01/126 https://doi.org/10.1088/1475-7516/2025/01/126 Sí |
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openAccess |
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application/pdf |
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IOP Publishing |
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IOP Publishing |
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reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
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Consejo Superior de Investigaciones Científicas (CSIC) |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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1869422505918201857 |
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ELG spectroscopic systematics analysis of the DESI Data Release 1Yu, JiaxiGaztañaga, EnriquePrada, FranciscoCosmological parameters from LSSGalaxy clusteringGalaxy surveysRedshift surveysJ. Yu et al. -- Dark Energy Spectroscopic Instrument (DESI) survey Year 1 results. -- ArXiv ePrint: 2405.16657Dark Energy Spectroscopic Instrument (DESI) uses more than 2.4 million Emission Line Galaxies (ELGs) for 3D large-scale structure (LSS) analyses in its Data Release 1 (DR1). Such large statistics enable thorough research on systematic uncertainties. In this study, we focus on spectroscopic systematics of ELGs. The redshift success rate (fgoodz) is the relative fraction of secure redshifts among all measurements. It depends on observing conditions, thus introduces non-cosmological variations to the LSS. We, therefore, develop the redshift failure weight (wzfail) and a per-fibre correction (ηzfail) to mitigate these dependences. They have minor influences on the galaxy clustering. For ELGs with a secure redshift, there are two subtypes of systematics: 1) catastrophics (large) that only occur in a few samples; 2) redshift uncertainty (small) that exists for all samples. The catastrophics represent 0.26% of the total DR1 ELGs, composed of the confusion between [O ii] and sky residuals, double objects, total catastrophics and others. We simulate the realistic 0.26% catastrophics of DR1 ELGs, the hypothetical 1% catastrophics, and the truncation of the contaminated 1.31 < z < 1.33 in the AbacusSummit ELG mocks. Their Pℓ show non-negligible bias from the uncontaminated mocks. But their influences on the redshift space distortions (RSD) parameters are smaller than 0.2σ. The redshift uncertainty of DR1 ELGs is 8.5km s-1 with a Lorentzian profile. The code for implementing the catastrophics and redshift uncertainty on mocks can be found in https://github.com/Jiaxi-Yu/modelling_spectro_sys.JY, DFS, and JPK acknowledge the support from the SNF 200020_175751 and 200020_207379 “Cosmology with 3D Maps of the Universe” research grant. We would like to thank Anand Raichoor, Allyson Brodzeller, Ruiyang Zhao and Julien Guy for their helpful discussions. We also would like to thank Andrei Variu for his support in visualising DESI spectra. This material is based upon work supported by the U.S. Department of Energy (DOE), Office of Science, Office of High-Energy Physics, under Contract No. DE-AC02-05CH11231, and by the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility under the same contract. Additional support for DESI was provided by the U.S. National Science Foundation (NSF), Division of Astronomical Sciences under Contract No. AST-0950945 to the NSF’s National Optical-Infrared Astronomy Research Laboratory; the Science and Technology Facilities Council of the United Kingdom; the Gordon and Betty Moore Foundation; the Heising-Simons Foundation; the French Alternative Energies and Atomic Energy Commission (CEA); the National Council of Humanities, Science and Technology of Mexico (CONAHCYT); the Ministry of Science and Innovation of Spain (MICINN), and by the DESI Member Institutions: https://www.desi.lbl.gov/collaborating-institutions. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the U.S. National Science Foundation, the U.S. Department of Energy, or any of the listed funding agencies. The authors are honored to be permitted to conduct scientific research on Iolkam Du’ag (Kitt Peak), a mountain with particular significance to the Tohono O’odham Nation.Peer reviewedIOP PublishingNational Science Foundation (US)Department of Energy (US)Science and Technology Facilities Council (UK)Gordon and Betty Moore FoundationHeising Simons FoundationCommissariat à l'Ènergie Atomique et aux Ènergies Alternatives (France)Consejo Nacional de Humanidades, Ciencias y Tecnologías (México)Ministerio de Ciencia e Innovación (España)Yu, Jiaxi [0009-0001-7217-8006]Gaztañaga, Enrique [0000-0001-9632-0815]Prada, Francisco [0000-0001-7145-8674]Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252025info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/385425reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)InglésThe underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1088/1475-7516/2025/01/126https://doi.org/10.1088/1475-7516/2025/01/126Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3854252026-05-22T06:33:51Z |
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