Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

Adame, A. G.; Aguilar, J.; Ahlen, S.; Alam, S.; Aldering, G.; Alexander, D. M.; Alfarsy, R.; Allende Prieto, C.; Alvarez, M.; Alves, O.; Anand, A.; Andrade-Oliveira, F.; Armengaud, E.; Asorey, J.; Avila, S.; Aviles, A.; Bailey, S.; Balaguera-Antolínez, A.; Ballester, O.; Baltay, C.; Bault, A.; Bautista, J.; Behera, J.; Beltran, S. F.; BenZvi, S.; Beraldo e Silva, L.; Bermejo-Climent, J. R.; Berti, A.; Besuner, R.; Beutler, F.; Bianchi, D.; Blake, C.; Blum, R.; Bolton, A. S.; Brieden, S.; Brodzeller, A.; Brooks, D.; Brown, Z.; Buckley-Geer, E.; Burtin, E.; Cabayol-Garcia, L.; Cai, Z.; Canning, R.; Cardiel-Sas, L.; Carnero Rosell, A.; Castander, F. J.; Cervantes-Cota, J. L.; Chabanier, S.; Chaussidon, E.; Chaves-Montero, J.; Chen, S.; Chen, X.; Chuang, C.; Claybaugh, T.; Cole, S.; Cooper, A. P.; Cuceu, A.; Davis, T. M.; Dawson, K.; de Belsunce, R.; de la Cruz, R.; de la Macorra, A.; de Mattia, A.; Demina, R.; Demirbozan, U.; DeRose, J.; Dey, A.; Dey, B.; Dhungana, G.; Ding, J.; Ding, Z.; Doel, P.; Doshi, R.; Douglass, K.; Edge, A.; Eftekharzadeh, S.; Eisenstein, D. J.; Elliott, A.; Escoffier, S.; Fagrelius, P.; Fan, X.; Fanning, K.; Fawcett, V. A.; Ferraro, S.; Ereza, J.; Flaugher, B.; Font-Ribera, A.; Forero-Sánchez, D.; Forero-Romero, J. E.; Frenk, C. S.; Gänsicke, B. T.; García, L. Á.; García-Bellido, J.; Garcia-Quintero, C.; Garrison, L. H.; Gil-Marín, H.; Golden-Marx, J.; A Gontcho, S. Gontcho; Gonzalez-Morales, A. X.; Gonzalez-Perez, V.; Gordon, C.; Graur, O.; Green, D.; Gruen, D.; Guy, J.; Hadzhiyska, B.; Hahn, C.; Han, J. J.; Hanif, M. S.; Herrera-Alcantar, H. K.; Honscheid, K.; Hou, J.; Howlett, C.; Huterer, D.; Iršič, V.; Ishak, M.; Jana, A.; Jiang, L.; Jimenez, J.; Jing, Y. P.; Joudaki, S.; Jullo, E.; Joyce, R.; Juneau, S.; Kizhuprakkat, N.; Karaçaylı, N. G.; Karim, T.; Kehoe, R.; Kent, S.; Khederlarian, A.; Kim, S.; Kirkby, D.; Kisner, T.; Kitaura, F.; Kneib, J.; Koposov, S. E.; Kovács, A.; Kremin, A.; Krolewski, A.; L’Huillier, B.; Lahav, O.; Lambert, A.; Lamman, C.; Lan, T. -W.; Landriau, M.; Lang, D.; Lange, J. U.; Lasker, J.; Le Guillou, L.; Leauthaud, A.; Levi, M. E.; Li, T. S.; Linder, E.; Lyons, A.; Magneville, C.; Manera, M.; Manser, C. J.; Margala, D.; Martini, P.; McDonald, P.; Medina, G. E.; Medina-Varela, L.; Meisner, A.; Mena-Fernández, J.; Meneses-Rizo, J.; Mezcua, M.; Miquel, R.; Montero-Camacho, P.; Moon, J.; Moore, S.; Moustakas, J.; Mueller, E.; Mundet, J.; Muñoz-Gutiérrez, A.; Myers, A. D.; Nadathur, S.; Napolitano, L.; Neveux, R.; Newman, J. A.; Nie, J.; Niz, G.; Norberg, P.; Noriega, H. E.; Paillas, E.; Palanque-Delabrouille, N.; Palmese, A.; Zhiwei, P.; Parkinson, D.; Penmetsa, S.; Percival, W. J.; Pérez-Fernández, A.; Pérez-Ràfols, I.; Pieri, M.; Poppett, C.; Porredon, A.; Prada, F.; Pucha, R.; Raichoor, A.; Ramírez-Pérez, C.; Ramirez-Solano, S.; Rashkovetskyi, M.; Ravoux, C.; Rocher, A.; Rockosi, C.; Ross, A. J.; Rossi, G.; Ruggeri, R.; Ruhlmann-Kleider, V.; Sabiu, C. G.; Said, K.; Saintonge, A.; Samushia, L.; Sanchez, E.; Saulder, C.; Schaan, E.; Schlafly, E. F.; Schlegel, D.; Scholte, D.; Schubnell, M.; Seo, H.; Shafieloo, A.; Sharples, R.; Sheu, W.; Silber, J.; Sinigaglia, F.; Siudek, M.; Slepian, Z.; Smith, A.; Sprayberry, D.; Stephey, L.; Suárez-Pérez, J.; Sun, Z.; Tan, T.; Tarlé, G.; Tojeiro, R.; Ureña-López, L. A.; Vaisakh, R.; Valcin, D.; Valdes, F.; Valluri, M.; Vargas-Magaña, M.; Variu, A.; Verde, L.; Walther, M.; Wang, B.; Wang, M. S.; Weaver, B. A.; Weaverdyck, N.; Wechsler, R. H.; White, M.; Xie, Y.; Yang, J.; Yèche, C.; Yu, J.; Yuan, S.; Zhang, H.; Zhang, Z.; Zhao, C.; Zheng, Z.; Zhou, R.; Zhou, Z.; Zou, H.; Zou, S.; Zu, Y.

doi:10.3847/1538-3881/ad0b08

Title: Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

Journal Article · Mon Jan 15 00:00:00 EST 2024 · The Astronomical Journal

DOI:https://doi.org/10.3847/1538-3881/ad0b08· OSTI ID:2281914

Adame, A. G.; Aguilar, J.;

;

; Aldering, G.;

; Alfarsy, R.; Allende Prieto, C.; Alvarez, M.; Alves, O.;

;

; Baltay, C. more »

The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg² over 5 yr to constrain the cosmic expansion history through precise measurements of baryon acoustic oscillations (BAO). The scientific program for DESI was evaluated during a 5 month survey validation (SV) campaign before beginning full operations. This program produced deep spectra of tens of thousands of objects from each of the stellar Milky Way Survey (MWS), Bright Galaxy Survey (BGS), luminous red galaxy (LRG), emission line galaxy (ELG), and quasar target classes. These SV spectra were used to optimize redshift distributions, characterize exposure times, determine calibration procedures, and assess observational overheads for the 5 yr program. In this paper, we present the final target selection algorithms, redshift distributions, and projected cosmology constraints resulting from those studies. We also present a One-Percent Survey conducted at the conclusion of SV covering 140 deg² using the final target selection algorithms with exposures of a depth typical of the main survey. The SV indicates that DESI will be able to complete the full 14,000 deg² program with spectroscopically confirmed targets from the MWS, BGS, LRG, ELG, and quasar programs with total sample sizes of 7.2, 13.8, 7.46, 15.7, and 2.87 million, respectively. These samples will allow exploration of the Milky Way halo, clustering on all scales, and BAO measurements with a statistical precision of 0.28% over the redshift interval z < 1.1, 0.39% over the redshift interval 1.1 < z < 1.9, and 0.46% over the redshift interval 1.9 < z < 3.5.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); USDOE Office of Science (SC), Basic Energy Sciences (BES). Scientific User Facilities (SUF)

Contributing Organization:: DESI Collaboration

Grant/Contract Number:: SC0009959; AC02-05CH11231; AC02-07CH11359

OSTI ID:: 2281914

Alternate ID(s):: OSTI ID: 1988475

Report Number(s):: FERMILAB-PUB-23-317-PPD; arXiv:2306.06307

Journal Information:: The Astronomical Journal, Vol. 167, Issue 2; ISSN 0004-6256

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples Betoule, M.; Kessler, R.; Guy, J. Astronomy & Astrophysics, Vol. 568 https://doi.org/10.1051/0004-6361/201423413	journal	August 2014
Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies Eisenstein, Daniel J.; Zehavi, Idit; Hogg, David W. The Astrophysical Journal, Vol. 633, Issue 2 https://doi.org/10.1086/466512	journal	November 2005

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