Survey Operations for the Dark Energy Spectroscopic Instrument

The Dark Energy Spectroscopic Instrument (DESI) survey is a spectroscopic survey of tens of millions of galaxies at 0 < z < 3.5 covering 14,000 sq. deg. of the sky. In its first 1.1 yr of survey operations, it has observed more than 14 million galaxies and 4 million stars. We describe the proc...

Full description

Bibliographic Details
Main Authors: Edward F. Schlafly, David Kirkby, David J. Schlegel, Adam D. Myers, Anand Raichoor, Kyle Dawson, Jessica Aguilar, Carlos Allende Prieto, Stephen Bailey, Segev BenZvi, Jose Bermejo-Climent, David Brooks, Axel de la Macorra, Arjun Dey, Peter Doel, Kevin Fanning, Andreu Font-Ribera, Jaime E. Forero-Romero, Juan García-Bellido, Satya Gontcho A Gontcho, Julien Guy, ChangHoon Hahn, Klaus Honscheid, Mustapha Ishak, Stéphanie Juneau, Robert Kehoe, Theodore Kisner, Anthony Kremin, Martin Landriau, Dustin A. Lang, James Lasker, Michael E. Levi, Christophe Magneville, Christopher J. Manser, Paul Martini, Aaron M. Meisner, Ramon Miquel, John Moustakas, Jeffrey A. Newman, Jundan Nie, Nathalie. Palanque-Delabrouille, Will J. Percival, Claire Poppett, Constance Rockosi, Ashley J. Ross, Graziano Rossi, Gregory Tarlé, Benjamin A. Weaver, Christophe Yèche, Rongpu Zhou, DESI Collaboration
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/ad0832
_version_ 1797517058114584576
author Edward F. Schlafly
David Kirkby
David J. Schlegel
Adam D. Myers
Anand Raichoor
Kyle Dawson
Jessica Aguilar
Carlos Allende Prieto
Stephen Bailey
Segev BenZvi
Jose Bermejo-Climent
David Brooks
Axel de la Macorra
Arjun Dey
Peter Doel
Kevin Fanning
Andreu Font-Ribera
Jaime E. Forero-Romero
Juan García-Bellido
Satya Gontcho A Gontcho
Julien Guy
ChangHoon Hahn
Klaus Honscheid
Mustapha Ishak
Stéphanie Juneau
Robert Kehoe
Theodore Kisner
Anthony Kremin
Martin Landriau
Dustin A. Lang
James Lasker
Michael E. Levi
Christophe Magneville
Christopher J. Manser
Paul Martini
Aaron M. Meisner
Ramon Miquel
John Moustakas
Jeffrey A. Newman
Jundan Nie
Nathalie. Palanque-Delabrouille
Will J. Percival
Claire Poppett
Constance Rockosi
Ashley J. Ross
Graziano Rossi
Gregory Tarlé
Benjamin A. Weaver
Christophe Yèche
Rongpu Zhou
DESI Collaboration
author_facet Edward F. Schlafly
David Kirkby
David J. Schlegel
Adam D. Myers
Anand Raichoor
Kyle Dawson
Jessica Aguilar
Carlos Allende Prieto
Stephen Bailey
Segev BenZvi
Jose Bermejo-Climent
David Brooks
Axel de la Macorra
Arjun Dey
Peter Doel
Kevin Fanning
Andreu Font-Ribera
Jaime E. Forero-Romero
Juan García-Bellido
Satya Gontcho A Gontcho
Julien Guy
ChangHoon Hahn
Klaus Honscheid
Mustapha Ishak
Stéphanie Juneau
Robert Kehoe
Theodore Kisner
Anthony Kremin
Martin Landriau
Dustin A. Lang
James Lasker
Michael E. Levi
Christophe Magneville
Christopher J. Manser
Paul Martini
Aaron M. Meisner
Ramon Miquel
John Moustakas
Jeffrey A. Newman
Jundan Nie
Nathalie. Palanque-Delabrouille
Will J. Percival
Claire Poppett
Constance Rockosi
Ashley J. Ross
Graziano Rossi
Gregory Tarlé
Benjamin A. Weaver
Christophe Yèche
Rongpu Zhou
DESI Collaboration
author_sort Edward F. Schlafly
collection DOAJ
description The Dark Energy Spectroscopic Instrument (DESI) survey is a spectroscopic survey of tens of millions of galaxies at 0 < z < 3.5 covering 14,000 sq. deg. of the sky. In its first 1.1 yr of survey operations, it has observed more than 14 million galaxies and 4 million stars. We describe the processes that govern DESI’s observations of the 15,000 fields composing the survey. This includes the planning of each night’s observations in the afternoon; automatic selection of fields to observe during the night; real-time assessment of field completeness on the basis of observing conditions during each exposure; reduction, redshifting, and quality assurance of each field of targets in the morning following observation; and updates to the list of future targets to observe on the basis of these results. We also compare the performance of the survey with historical expectations and find good agreement. Simulations of the weather and of DESI observations using the real field-selection algorithm show good agreement with the actual observations. After accounting for major unplanned shutdowns, the dark time survey is progressing about 7% faster than forecast, which is good agreement given approximations made in the simulations.
first_indexed 2024-03-10T07:09:32Z
format Article
id doaj.art-51d2c8e17068455287e0a7467c36376b
institution Directory Open Access Journal
issn 1538-3881
language English
last_indexed 2024-03-10T07:09:32Z
publishDate 2023-01-01
publisher IOP Publishing
record_format Article
series The Astronomical Journal
spelling doaj.art-51d2c8e17068455287e0a7467c36376b2023-11-22T15:30:16ZengIOP PublishingThe Astronomical Journal1538-38812023-01-01166625910.3847/1538-3881/ad0832Survey Operations for the Dark Energy Spectroscopic InstrumentEdward F. Schlafly0https://orcid.org/0000-0002-3569-7421David Kirkby1https://orcid.org/0000-0002-8828-5463David J. Schlegel2https://orcid.org/0000-0002-5042-5088Adam D. Myers3Anand Raichoor4https://orcid.org/0000-0001-5999-7923Kyle Dawson5https://orcid.org/0000-0002-0553-3805Jessica Aguilar6Carlos Allende Prieto7https://orcid.org/0000-0002-0084-572XStephen Bailey8https://orcid.org/0000-0003-4162-6619Segev BenZvi9https://orcid.org/0000-0001-5537-4710Jose Bermejo-Climent10David Brooks11https://orcid.org/0000-0002-8458-5047Axel de la Macorra12Arjun Dey13https://orcid.org/0000-0002-4928-4003Peter Doel14Kevin Fanning15https://orcid.org/0000-0003-2371-3356Andreu Font-Ribera16https://orcid.org/0000-0002-3033-7312Jaime E. Forero-Romero17https://orcid.org/0000-0002-2890-3725Juan García-Bellido18https://orcid.org/0000-0002-9370-8360Satya Gontcho A Gontcho19https://orcid.org/0000-0003-3142-233XJulien Guy20https://orcid.org/0000-0001-9822-6793ChangHoon Hahn21https://orcid.org/0000-0003-1197-0902Klaus Honscheid22Mustapha Ishak23https://orcid.org/0000-0002-6024-466XStéphanie Juneau24https://orcid.org/0000-0002-0000-2394Robert Kehoe25https://orcid.org/0000-0002-7101-697XTheodore Kisner26https://orcid.org/0000-0003-3510-7134Anthony Kremin27https://orcid.org/0000-0001-6356-7424Martin Landriau28https://orcid.org/0000-0003-1838-8528Dustin A. Lang29https://orcid.org/0000-0002-1172-0754James Lasker30https://orcid.org/0000-0003-2999-4873Michael E. Levi31https://orcid.org/0000-0003-1887-1018Christophe Magneville32Christopher J. Manser33https://orcid.org/0000-0003-1543-5405Paul Martini34https://orcid.org/0000-0002-0194-4017Aaron M. Meisner35https://orcid.org/0000-0002-1125-7384Ramon Miquel36https://orcid.org/0000-0002-6610-4836John Moustakas37https://orcid.org/0000-0002-2733-4559Jeffrey A. Newman38https://orcid.org/0000-0001-8684-2222Jundan Nie39https://orcid.org/0000-0001-6590-8122Nathalie. Palanque-Delabrouille40https://orcid.org/0000-0003-3188-784XWill J. Percival41https://orcid.org/0000-0002-0644-5727Claire Poppett42Constance Rockosi43https://orcid.org/0000-0002-6667-7028Ashley J. Ross44https://orcid.org/0000-0002-7522-9083Graziano Rossi45Gregory Tarlé46https://orcid.org/0000-0003-1704-0781Benjamin A. Weaver47Christophe Yèche48https://orcid.org/0000-0001-5146-8533Rongpu Zhou49https://orcid.org/0000-0001-5381-4372DESI CollaborationSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USADepartment of Physics and Astronomy, University of California , Frederick Reines Hall, Irvine, CA 92697, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Physics and Astronomy, University of Wyoming , Laramie, WY 82071, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Physics and Astronomy, The University of Utah , 115 South 1400 East, Salt Lake City, UT 84112, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USAInstituto de Astrofísica de Canarias , C/Vía Láctea, s/n, E-38205 La Laguna, Tenerife, Spain; Universidad de La Laguna , Dept. de Astrofísica, E-38206 La Laguna, Tenerife, SpainLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Physics & Astronomy, University of Rochester , Bausch and Lomb Hall, Rochester, NY 14627-0171, USADepartment of Physics & Astronomy, University of Rochester , Bausch and Lomb Hall, Rochester, NY 14627-0171, USADepartment of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UKInstituto de Física, Universidad Nacional Autónoma de México , Cd. de México C.P. 04510, MéxicoNSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USADepartment of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UKThe Ohio State University , Columbus, OH 43210, USAInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, E-08193 Bellaterra Barcelona, SpainDepartamento de Física, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio Ip, CP 111711, Bogotá, ColombiaInstituto de Física Teórica (IFT) UAM/CSIC, Universidad Autónoma de Madrid , Cantoblanco, E-28049, Madrid, SpainLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Astrophysical Sciences, Princeton University , Princeton, NJ 08544, USAThe Ohio State University , Columbus, OH 43210, USA; Center for Cosmology and AstroParticle Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA; Department of Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USAUniversity of Texas , Dallas, 800 W Campbell Road, Richardson, TX 75080, USANSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USADepartment of Physics, Southern Methodist University , 3215 Daniel Avenue, Dallas, TX 75275, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USAPerimeter Institute for Theoretical Physics , 31 Caroline Street North, Waterloo, ON N2L 2Y5, Canada; Department of Physics and Astronomy, University of Waterloo , 200 University Avenue W, Waterloo, ON N2L 3G1, CanadaDepartment of Physics, Southern Methodist University , 3215 Daniel Avenue, Dallas, TX 75275, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USAIRFU, CEA, Université Paris-Saclay , F-91191 Gif-sur-Yvette, FranceAstrophysics Group, Department of Physics, Imperial College London , Prince Consort Road, London, SW7 2AZ, UK; Department of Physics, University of Warwick , Coventry, CV4 7AL, UKCenter for Cosmology and AstroParticle Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA; Department of Astronomy, The Ohio State University , 4055 McPherson Laboratory, 140 W 18th Avenue, Columbus, OH 43210, USANSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USAInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, E-08193 Bellaterra Barcelona, Spain; Institució Catalana de Recerca i Estudis Avançats , Passeig de Lluís Companys, 23, E-08010 Barcelona, SpainDepartment of Physics and Astronomy, Siena College , 515 Loudon Road, Loudonville, NY 12211, USADepartment of Physics & Astronomy and Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh , 3941 O’Hara Street, Pittsburgh, PA 15260, USANational Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Rd., Chaoyang District, Beijing, 100012, People's Republic of ChinaLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; IRFU, CEA, Université Paris-Saclay , F-91191 Gif-sur-Yvette, FrancePerimeter Institute for Theoretical Physics , 31 Caroline Street North, Waterloo, ON N2L 2Y5, Canada; Department of Physics and Astronomy, University of Waterloo , 200 University Avenue W, Waterloo, ON N2L 3G1, Canada; Waterloo Centre for Astrophysics, University of Waterloo , 200 University Avenue W, Waterloo, ON N2L 3G1, CanadaLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; Space Sciences Laboratory, University of California , Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA; University of California , Berkeley, 110 Sproul Hall #5800 Berkeley, CA 94720, USADepartment of Astronomy and Astrophysics, University of California , Santa Cruz, 1156 High Street, Santa Cruz, CA 95065, USA; University of California Observatories , 1156 High Street, Sana Cruz, CA 95065, USACenter for Cosmology and AstroParticle Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USADepartment of Physics and Astronomy, Sejong University , Seoul, 143-747, Republic of KoreaUniversity of Michigan , Ann Arbor, MI 48109, USANSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USAIRFU, CEA, Université Paris-Saclay , F-91191 Gif-sur-Yvette, FranceLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USAThe Dark Energy Spectroscopic Instrument (DESI) survey is a spectroscopic survey of tens of millions of galaxies at 0 < z < 3.5 covering 14,000 sq. deg. of the sky. In its first 1.1 yr of survey operations, it has observed more than 14 million galaxies and 4 million stars. We describe the processes that govern DESI’s observations of the 15,000 fields composing the survey. This includes the planning of each night’s observations in the afternoon; automatic selection of fields to observe during the night; real-time assessment of field completeness on the basis of observing conditions during each exposure; reduction, redshifting, and quality assurance of each field of targets in the morning following observation; and updates to the list of future targets to observe on the basis of these results. We also compare the performance of the survey with historical expectations and find good agreement. Simulations of the weather and of DESI observations using the real field-selection algorithm show good agreement with the actual observations. After accounting for major unplanned shutdowns, the dark time survey is progressing about 7% faster than forecast, which is good agreement given approximations made in the simulations.https://doi.org/10.3847/1538-3881/ad0832Redshift surveysSpectroscopyObservatories
spellingShingle Edward F. Schlafly
David Kirkby
David J. Schlegel
Adam D. Myers
Anand Raichoor
Kyle Dawson
Jessica Aguilar
Carlos Allende Prieto
Stephen Bailey
Segev BenZvi
Jose Bermejo-Climent
David Brooks
Axel de la Macorra
Arjun Dey
Peter Doel
Kevin Fanning
Andreu Font-Ribera
Jaime E. Forero-Romero
Juan García-Bellido
Satya Gontcho A Gontcho
Julien Guy
ChangHoon Hahn
Klaus Honscheid
Mustapha Ishak
Stéphanie Juneau
Robert Kehoe
Theodore Kisner
Anthony Kremin
Martin Landriau
Dustin A. Lang
James Lasker
Michael E. Levi
Christophe Magneville
Christopher J. Manser
Paul Martini
Aaron M. Meisner
Ramon Miquel
John Moustakas
Jeffrey A. Newman
Jundan Nie
Nathalie. Palanque-Delabrouille
Will J. Percival
Claire Poppett
Constance Rockosi
Ashley J. Ross
Graziano Rossi
Gregory Tarlé
Benjamin A. Weaver
Christophe Yèche
Rongpu Zhou
DESI Collaboration
Survey Operations for the Dark Energy Spectroscopic Instrument
The Astronomical Journal
Redshift surveys
Spectroscopy
Observatories
title Survey Operations for the Dark Energy Spectroscopic Instrument
title_full Survey Operations for the Dark Energy Spectroscopic Instrument
title_fullStr Survey Operations for the Dark Energy Spectroscopic Instrument
title_full_unstemmed Survey Operations for the Dark Energy Spectroscopic Instrument
title_short Survey Operations for the Dark Energy Spectroscopic Instrument
title_sort survey operations for the dark energy spectroscopic instrument
topic Redshift surveys
Spectroscopy
Observatories
url https://doi.org/10.3847/1538-3881/ad0832
work_keys_str_mv AT edwardfschlafly surveyoperationsforthedarkenergyspectroscopicinstrument
AT davidkirkby surveyoperationsforthedarkenergyspectroscopicinstrument
AT davidjschlegel surveyoperationsforthedarkenergyspectroscopicinstrument
AT adamdmyers surveyoperationsforthedarkenergyspectroscopicinstrument
AT anandraichoor surveyoperationsforthedarkenergyspectroscopicinstrument
AT kyledawson surveyoperationsforthedarkenergyspectroscopicinstrument
AT jessicaaguilar surveyoperationsforthedarkenergyspectroscopicinstrument
AT carlosallendeprieto surveyoperationsforthedarkenergyspectroscopicinstrument
AT stephenbailey surveyoperationsforthedarkenergyspectroscopicinstrument
AT segevbenzvi surveyoperationsforthedarkenergyspectroscopicinstrument
AT josebermejocliment surveyoperationsforthedarkenergyspectroscopicinstrument
AT davidbrooks surveyoperationsforthedarkenergyspectroscopicinstrument
AT axeldelamacorra surveyoperationsforthedarkenergyspectroscopicinstrument
AT arjundey surveyoperationsforthedarkenergyspectroscopicinstrument
AT peterdoel surveyoperationsforthedarkenergyspectroscopicinstrument
AT kevinfanning surveyoperationsforthedarkenergyspectroscopicinstrument
AT andreufontribera surveyoperationsforthedarkenergyspectroscopicinstrument
AT jaimeeforeroromero surveyoperationsforthedarkenergyspectroscopicinstrument
AT juangarciabellido surveyoperationsforthedarkenergyspectroscopicinstrument
AT satyagontchoagontcho surveyoperationsforthedarkenergyspectroscopicinstrument
AT julienguy surveyoperationsforthedarkenergyspectroscopicinstrument
AT changhoonhahn surveyoperationsforthedarkenergyspectroscopicinstrument
AT klaushonscheid surveyoperationsforthedarkenergyspectroscopicinstrument
AT mustaphaishak surveyoperationsforthedarkenergyspectroscopicinstrument
AT stephaniejuneau surveyoperationsforthedarkenergyspectroscopicinstrument
AT robertkehoe surveyoperationsforthedarkenergyspectroscopicinstrument
AT theodorekisner surveyoperationsforthedarkenergyspectroscopicinstrument
AT anthonykremin surveyoperationsforthedarkenergyspectroscopicinstrument
AT martinlandriau surveyoperationsforthedarkenergyspectroscopicinstrument
AT dustinalang surveyoperationsforthedarkenergyspectroscopicinstrument
AT jameslasker surveyoperationsforthedarkenergyspectroscopicinstrument
AT michaelelevi surveyoperationsforthedarkenergyspectroscopicinstrument
AT christophemagneville surveyoperationsforthedarkenergyspectroscopicinstrument
AT christopherjmanser surveyoperationsforthedarkenergyspectroscopicinstrument
AT paulmartini surveyoperationsforthedarkenergyspectroscopicinstrument
AT aaronmmeisner surveyoperationsforthedarkenergyspectroscopicinstrument
AT ramonmiquel surveyoperationsforthedarkenergyspectroscopicinstrument
AT johnmoustakas surveyoperationsforthedarkenergyspectroscopicinstrument
AT jeffreyanewman surveyoperationsforthedarkenergyspectroscopicinstrument
AT jundannie surveyoperationsforthedarkenergyspectroscopicinstrument
AT nathaliepalanquedelabrouille surveyoperationsforthedarkenergyspectroscopicinstrument
AT willjpercival surveyoperationsforthedarkenergyspectroscopicinstrument
AT clairepoppett surveyoperationsforthedarkenergyspectroscopicinstrument
AT constancerockosi surveyoperationsforthedarkenergyspectroscopicinstrument
AT ashleyjross surveyoperationsforthedarkenergyspectroscopicinstrument
AT grazianorossi surveyoperationsforthedarkenergyspectroscopicinstrument
AT gregorytarle surveyoperationsforthedarkenergyspectroscopicinstrument
AT benjaminaweaver surveyoperationsforthedarkenergyspectroscopicinstrument
AT christopheyeche surveyoperationsforthedarkenergyspectroscopicinstrument
AT rongpuzhou surveyoperationsforthedarkenergyspectroscopicinstrument
AT desicollaboration surveyoperationsforthedarkenergyspectroscopicinstrument