Dark Energy Spectroscopic Instrument

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Dark Energy Spectroscopic Instrument
DESI crossfade 4 (sunset-Workup-04-CC).tiff
DESI installed on the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory
Alternative namesDESI OOjs UI icon edit-ltr-progressive.svg
Part of Kitt Peak National Observatory
Nicholas U. Mayall Telescope   OOjs UI icon edit-ltr-progressive.svg
Location(s) Kitt Peak, Arizona
Coordinates 31°57′51″N111°36′00″W / 31.96406°N 111.6°W / 31.96406; -111.6 OOjs UI icon edit-ltr-progressive.svg
Organization Lawrence Berkeley National Laboratory   OOjs UI icon edit-ltr-progressive.svg
Altitude2,100 m (6,900 ft) OOjs UI icon edit-ltr-progressive.svg
Wavelength 360 nm (830 THz)–980 nm (310 THz)
Built2015– (2015–) OOjs UI icon edit-ltr-progressive.svg
First light 2019  OOjs UI icon edit-ltr-progressive.svg
Telescope style scientific instrument
spectrometer   OOjs UI icon edit-ltr-progressive.svg
Website desi.lbl.gov OOjs UI icon edit-ltr-progressive.svg
Usa edcp relief location map.png
Red pog.svg
Location of Dark Energy Spectroscopic Instrument
  Commons-logo.svg Related media on Commons
[ edit on Wikidata]

The Dark Energy Spectroscopic Instrument (DESI) is a scientific research instrument for conducting spectrographic astronomical surveys of distant galaxies. Its main components are a focal plane containing 5,000 fiber-positioning robots, and a bank of spectrographs which are fed by the fibers. The instrument enables an experiment to probe the expansion history of the universe and the mysterious physics of dark energy. [1] [2] The main DESI survey started in May 2021. DESI sits at an elevation of 6,880 feet (2,100 m), where it has been retrofitted onto the Mayall Telescope on top of Kitt Peak in the Sonoran Desert, which is located 55 miles (89 km) from Tucson, Arizona, US.

Contents

The instrument is operated by the Lawrence Berkeley National Laboratory under funding from the US Department of Energy's Office of Science. Construction of the instrument was principally funded by the US Department of Energy's Office of Science, and by other numerous sources including the US National Science Foundation, the UK Science and Technology Facilities Council, France's Alternative Energies and Atomic Energy Commission, Mexico's National Council of Science and Technology, Spain's Ministry of Science and Innovation, by the Gordon and Betty Moore Foundation, by the Heising-Simons Foundation, and by collaborating institutions worldwide. [3] [4]

Science goals

An artistic celebration of the Dark Energy Spectroscopic Instrument (DESI) year-one data, showing a slice of the larger 3D map that DESI is constructing during its five-year survey. Artistic Composition of DESI Year-One Data Slice Above the Nicholas U Mayall 4-meter Telescope (noirlab2408a).jpg
An artistic celebration of the Dark Energy Spectroscopic Instrument (DESI) year-one data, showing a slice of the larger 3D map that DESI is constructing during its five-year survey.

The expansion history and large-scale structure of the universe is a key prediction of cosmological models, and DESI observations will permit scientists to probe diverse aspects of cosmology, from dark energy to alternatives to General Relativity to neutrino masses to the early universe. The data from DESI will be used to create three-dimensional maps of the distribution of matter covering an unprecedented volume of the universe with unparalleled detail. This will provide insight into the nature of dark energy and establish whether cosmic acceleration is due to a cosmic-scale modification of General Relativity. DESI will be transformative in the understanding of dark energy and the expansion rate of the universe at early times, one of the greatest mysteries in the understanding of the physical laws.

DESI will measure the expansion history of the universe using the baryon acoustic oscillations (BAO) imprinted in the clustering of galaxies, quasars, and the intergalactic medium. [5] The BAO technique is a robust way to extract cosmological distance information from the clustering of matter and galaxies. It relies only on very large-scale structure and it does so in a manner that enables scientists to separate the acoustic peak of the BAO signature from uncertainties in most systematic errors in the data. BAO was identified in the 2006 Dark Energy Task Force report as one of the key methods for studying dark energy. [6] In May 2014, the High-Energy Physics Advisory Panel, a federal advisory committee, commissioned by the US Department of Energy (DOE) and the National Science Foundation (NSF) endorsed DESI. [7]

3D map of the universe

Comparison of the Sloan survey at left consisting of around 4 million galaxies and quasars taken from 2000 to 2020 and the DESI survey at right consisting of around 7.5 million during its 7 first months starting in 2021 and expected to be completed by 2026 with 35 million. Sloan2020vsDESI2022.jpg
Comparison of the Sloan survey at left consisting of around 4 million galaxies and quasars taken from 2000 to 2020 and the DESI survey at right consisting of around 7.5 million during its 7 first months starting in 2021 and expected to be completed by 2026 with 35 million.

The baryon acoustic oscillations method requires a three-dimensional map of distant galaxies and quasars created from the angular and redshift information of a large statistical sample of cosmologically distant objects. By obtaining spectra of distant galaxies it is possible to determine their distance, via the measurement of their spectroscopic redshift, and thus create a 3-D map of the universe. [10] The 3-D map of the large-scale structure of the universe also contains more information about dark energy than just the BAO and is sensitive to the mass of the neutrino and parameters that governed the primordial universe. During its five-year survey, which began on May 15, 2021, the DESI experiment is expected to observe 40 million galaxies and quasars. [11]

Development

The DESI instrument implements a new highly multiplexed optical spectrograph on the Mayall Telescope. [12] The new optical corrector design creates a very large, 8.0 square degree field of view on the sky, which combined with the new focal plane instrumentation weighs approximately 10 tonnes. The focal plane accommodates 5,000 small computer controlled fiber positioners on a 10.4 millimeter pitch. The entire focal plane can be reconfigured for the next exposure in less than two minutes while the telescope slews to the next field. The DESI instrument is capable of taking 5,000 simultaneous spectra over a wavelength range from 360 nm to 980 nm. The DESI project scope included construction, installation, and commissioning of the new wide-field corrector and corrector support structure for the telescope, the focal plane assembly with 5,000 robotic fiber positioners and ten guide/focus/alignment sensors, a 40-meter optical fiber cabling system that brings light from the focal plane to the spectrographs, ten 3-arm spectrographs, an instrument control system, and a data analysis pipeline.

The instrument fabrication was managed by the Lawrence Berkeley National Laboratory and oversees operation of the experiment including a 600-person international scientific collaboration. Cost of construction was $56M from the US Department of Energy's Office of Science plus an additional $19M from other non-federal sources including contributions in-kind. The leadership of DESI currently consists of the director, Dr. Michael E. Levi, collaboration co-spokespersons Prof. Kyle Dawson and Dr. Nathalie Palanque-Delabrouille, project scientists Dr. David J. Schlegel and Dr. Julien Guy, project manager Dr. Patrick Jelinsky, instrument scientists Prof. Klaus Honscheid and Prof. Constance Rockosi. Past collaboration spokespersons have been Prof. Daniel Eisenstein and Prof. Risa Wechsler.

DOE approved CD-0 (Mission Need) on September 18, 2012, approved CD-1 (Alternative Selection and Cost Range) on March 19, 2015, and CD-2 (Performance Baseline) on September 17, 2015. Congressional approval for the start of DESI as a new Major Item of Equipment was provided in the FY15 Energy & Water appropriations legislation. Construction on the new instrument started June 22, 2016 with CD-3 (Start Construction) approval and was largely assembled by 2019 with commissioning finishing in March 21, 2020 in advance of the pandemic and marking the formal end of the project (CD-4). [13] DESI was completed under budget by $1.9M and 17 months ahead of schedule. As a consequence, the project received the DOE Project Management Excellence Award for 2020. [14] After a pause for the pandemic and a transition to remote operations, DESI returned to survey operations in December, 2020 with a final checkout and validation phase prior to starting its planned five-year survey. The five-year survey began on May 14, 2021. [15] DESI was shut down for three months in the summer of 2022 due to the Contreras fire which engulfed Kitt Peak. DESI was undamaged and is acquiring scientific data. [16]

DESI Legacy Imaging Surveys

To provide targets for the DESI survey three telescopes surveyed the northern and part of the southern sky in the g, r and z-band. Those surveys were the Beijing-Arizona Sky Survey (BASS), using the Bok 2.3-m telescope, the Dark Energy Camera Legacy Survey (DECaLS), using the Blanco 4m telescope and the Mayall z-band Legacy Survey (MzLS), using the 4-meter Mayall telescope. The area of the surveys is 14,000 square degrees (about one third of the sky) and avoids the Milky Way. These surveys were combined into the DESI Legacy Imaging Surveys, or Legacy Surveys. [17] [18] Colored images of the survey can be viewed in the Legacy Survey Sky Browser. [19] The legacy survey covers 16,000 square degrees of the night sky containing 1.6 billion objects including galaxies and quasars out to 11 billion years ago.

History

DESI received a go-ahead to start R&D for the project in December 2012 with the assignment of the Lawrence Berkeley National Laboratory as the managing laboratory. Dr. Michael Levi, a senior scientist at the Lawrence Berkeley National Laboratory was appointed by the laboratory to be DESI's project director who served in that role starting in 2012 and throughout construction. Henry Heetderks was project manager from 2013 until 2016, Robert Besuner was project manager from 2016 until 2020. Congressional authorization was provided in 2015, and the US Department of Energy's Office of Science approved the start of physical construction in June 2016. First light of the new corrector system was obtained on the night of April 1, 2019, and first-light of the entire instrument was achieved on the night of October 22, 2019. Commissioning ensued after first light and was completed in March, 2020, then paused during the pandemic in 2020. [20] DESI started its 5-year main scientific survey on May 14, 2021. DESI is currently operating normally after surviving the Contreras fire in 2022. [21]

Data Releases

Example spectrum taken by DESI for the Early Data Release. The image shows the spectrum of the galaxy LEDA 1787534. DESI EDR example galaxy LEDA 1787534.png
Example spectrum taken by DESI for the Early Data Release. The image shows the spectrum of the galaxy LEDA 1787534.

All of the publicly available data including redshift catalogs, added-value catalogs, and documentation, can be accessed through DESI sata portal. Individuals with accounts at the National Energy Research Scientific Computing Center (NERSC) can access the entire public portion of the DESI data. DESI catalogs also exist in a database format. For convenience, a copy of the public databases is also hosted by the NOIRLab Astro Data Lab science platform, and by using the SPectral Analysis and Retrievable Catalog Lab (SPARCL). [22] One easy way to access DESI spectra online is to use the legacy viewer at the DESI Legacy Imaging Surveys. [23] Users have to check the box for DESI spectra and click on an encircled galaxy or star for a link to the DESI Spectral Viewer to show up. [24] The spectrum can be explored in the DESI Spectral Viewer. [25] (Please see External Links under Index| Legacy Surveys)

Early Data Release

On 13 June 2023 the DESI Early Data Release (EDR) was announced. [26] The EDR contains spectra of nearly two million galaxies, quasars and stars. [22] One early result of the EDR was announced in February 2023 and described a mass migration of stars into the Andromeda Galaxy. [27] The EDR also revealed very distant quasars and very metal-poor stars. [22] [28]

Possibly evolving dark energy levels

From the level of detail able to be observed, the largest 3-D map of the universe at this point has been created (2024). [29] From this precise data, DESI Director Michael Levi stated:

We’re also seeing some potentially interesting differences that could indicate that dark energy is evolving over time. Those may or may not go away with more data, so we’re excited to start analyzing our three-year dataset soon. [30]

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<span class="mw-page-title-main">Kitt Peak National Observatory</span> United States astronomical observatory

The Kitt Peak National Observatory (KPNO) is a United States astronomical observatory located on Kitt Peak of the Quinlan Mountains in the Arizona-Sonoran Desert on the Tohono Oʼodham Nation, 88 kilometers (55 mi) west-southwest of Tucson, Arizona. With more than twenty optical and two radio telescopes, it is one of the largest gatherings of astronomical instruments in the Earth's northern hemisphere.

<span class="mw-page-title-main">Quasar</span> Active galactic nucleus containing a supermassive black hole

A quasar is an extremely luminous active galactic nucleus (AGN). It is sometimes known as a quasi-stellar object, abbreviated QSO. The emission from an AGN is powered by a supermassive black hole with a mass ranging from millions to tens of billions of solar masses, surrounded by a gaseous accretion disc. Gas in the disc falling towards the black hole heats up and releases energy in the form of electromagnetic radiation. The radiant energy of quasars is enormous; the most powerful quasars have luminosities thousands of times greater than that of a galaxy such as the Milky Way. Quasars are usually categorized as a subclass of the more general category of AGN. The redshifts of quasars are of cosmological origin.

<span class="mw-page-title-main">Redshift</span> Change of wavelength in photons during travel

In physics, a redshift is an increase in the wavelength, and corresponding decrease in the frequency and photon energy, of electromagnetic radiation. The opposite change, a decrease in wavelength and increase in frequency and energy, is known as a blueshift, or negative redshift. The terms derive from the colours red and blue which form the extremes of the visible light spectrum. The main causes of electromagnetic redshift in astronomy and cosmology are the relative motions of radiation sources, which give rise to the relativistic Doppler effect, and gravitational potentials, which gravitationally redshift escaping radiation. All sufficiently distant light sources show cosmological redshift corresponding to recession speeds proportional to their distances from Earth, a fact known as Hubble's law that implies the universe is expanding.

<span class="mw-page-title-main">Reionization</span> Process that caused matter to reionize early in the history of the Universe

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<span class="mw-page-title-main">Australian Astronomical Observatory</span> Observatory

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<span class="mw-page-title-main">Sloan Digital Sky Survey</span> Multi-spectral imaging and spectroscopic redshift survey

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<span class="mw-page-title-main">Redshift survey</span>

In astronomy, a redshift survey is a survey of a section of the sky to measure the redshift of astronomical objects: usually galaxies, but sometimes other objects such as galaxy clusters or quasars. Using Hubble's law, the redshift can be used to estimate the distance of an object from Earth. By combining redshift with angular position data, a redshift survey maps the 3D distribution of matter within a field of the sky. These observations are used to measure detailed statistical properties of the large-scale structure of the universe. In conjunction with observations of early structure in the cosmic microwave background, these results can place strong constraints on cosmological parameters such as the average matter density and the Hubble constant.

<span class="mw-page-title-main">2dF Galaxy Redshift Survey</span>

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References

  1. ↑ Bebek, C.J., ed. (2015-06-15). "DESI Design Report". Archived from the original on 2019-03-31. Retrieved 2016-02-12.
  2. ↑ Pultarova, Tereza (February 16, 2018). "How 5,000 Pencil-Size Robots May Solve the Mysteries of the universe". Live Science.
  3. ↑ Roberts, Jr., Glen (2019-10-28). "DESI Opens Its 5,000 Eyes to Capture the Colors of the Cosmos". Lawrence Berkeley National Laboratory . Retrieved 2020-02-03.
  4. ↑ Telescope tracks 35 million galaxies in Dark Energy hunt, BBC Science report, 28 October 2019
  5. ↑ Seo, Hee-Jong; Eisenstein, Daniel J. (2003). "Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys". The Astrophysical Journal . 598 (2): 720–740. arXiv: astro-ph/0307460 . Bibcode:2003ApJ...598..720S. doi:10.1086/379122. S2CID   13849508.
  6. ↑ Albrecht, Andreas; et al. (2006). "Report of the Dark Energy Task Force". arXiv: astro-ph/0609591 .
  7. ↑ "Building for Discovery: Strategic Plan for U.S. Particle Physics in the Global Context" (PDF). May 2014.
  8. ↑ "DESI at Kitt Peak Has Mapped More Galaxies Than All Previous 3D Surveys Combined - DOE Dark Energy Spectroscopic Instrument passes 7.5 million measured galaxy redshifts". www.noirlab.edu. Retrieved 2022-01-19.
  9. ↑ "Comparison of complete Sloan Digital Sky Survey and first DESI data". www.noirlab.edu. Retrieved 2022-01-19.
  10. ↑ Eisenstein, Daniel; et al. (2005). "Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies". The Astrophysical Journal. 633 (2): 560–574. arXiv: astro-ph/0501171 . Bibcode:2005ApJ...633..560E. doi:10.1086/466512. S2CID   4834543.
  11. ↑ "3-D Galaxy-mapping Project Enters Construction Phase". 2016-08-09.
  12. ↑ Levi, Michael; et al. (4 August 2013). "The DESI Experiment". arXiv: 1308.0847 [astro-ph.CO].
  13. ↑ Preuss, Paul (2015-09-21). "DESI, an Ambitious Probe of Dark Energy, Achieves its Next Major Milestone".
  14. ↑ "Office of Science Awards Successful Project Management Teams". Energy.gov. Retrieved 2022-10-26.
  15. ↑ Schulz, Bill (2021-05-17). "Successful Start of Dark Energy Spectroscopic Instrument (DESI) Follows Record-Setting Trial Run - Berkeley Lab". News Center. Retrieved 2022-10-26.
  16. ↑ Biron, Lauren (2022-10-07). "After Fire and Monsoons, DESI Resumes Cataloguing the Cosmos". News Center. Retrieved 2022-10-26.
  17. ↑ Dey, Arjun; Schlegel, David J.; Lang, Dustin; Blum, Robert; Burleigh, Kaylan; Fan, Xiaohui; Findlay, Joseph R.; Finkbeiner, Doug; Herrera, David; Juneau, Stéphanie; Landriau, Martin (May 2019). "Overview of the DESI Legacy Imaging Surveys". The Astronomical Journal. 157 (5): 168. arXiv: 1804.08657 . Bibcode:2019AJ....157..168D. doi: 10.3847/1538-3881/ab089d . hdl: 10150/633730 . ISSN   0004-6256. S2CID   56335994.
  18. ↑ "Index". Legacy Survey. 2012-11-08. Retrieved 2020-02-04.
  19. ↑ "Legacy Survey Sky Browser". legacysurvey.org. Retrieved 2020-02-04.
  20. ↑ Lincoln, Don. "Super New Telescope Opens Its Eyes For The First Time". Forbes. Retrieved 2019-11-09.
  21. ↑ Hill, Samantha (October 26, 2022). "Kitt Peak National Observatory mostly operational after fire". Astronomy.com. Retrieved 2022-10-26.
  22. 1 2 3 "Nearly Two Million Galaxies, Quasars, and Stars Contained in DESI Early Data Release - First small fraction of gigantic cosmic survey released and now available via DOE's Berkeley Laboratory with a portion hosted by NOIRLab's Astro Data Lab". noirlab.edu. Retrieved 2023-06-13.
  23. ↑ Survey, Legacy (2022-09-02). "Index". Legacy Survey. Retrieved 2024-04-13.
  24. ↑ "Legacy Survey Sky Browser with DESI Early Data Release enabled (centered around the galaxy IC 753)". www.legacysurvey.org. Retrieved 2023-06-13.
  25. ↑ "DESI spectral viewer (Spectrum of the galaxy IC 753)". www.legacysurvey.org. Retrieved 2023-06-13.
  26. ↑ Biron, Lauren (13 June 2023). "DESI Early Data Release Holds Nearly Two Million Objects". Lawrence Berkeley National Lab. Retrieved 16 June 2023.
  27. ↑ "Footprints of Galactic Immigration Uncovered in Andromeda Galaxy - The Dark Energy Spectroscopic Instrument reveals compelling evidence of a mass migration of stars into a galaxy other than the Milky Way". noirlab.edu. Retrieved 2023-06-13.
  28. ↑ Allende Prieto, Carlos; Aguado, David S.; González Hernández, Jonay I.; Rebolo, Rafael; Najita, Joan; Manser, Christopher J.; Rockosi, Constance; Slepian, Zachary; Mezcua, Mar; Valluri, Monica; Ezzeddine, Rana; Koposov, Sergey E.; Cooper, Andrew P.; Dey, Arjun; Gänsicke, Boris T. (2023-06-01). "GTC Follow-up Observations of Very Metal-Poor Star Candidates from DESI". The Astrophysical Journal. 957 (2): 76. arXiv: 2306.06321 . Bibcode:2023ApJ...957...76A. doi: 10.3847/1538-4357/acfa96 .
  29. ↑ Clowe, Douglas; Simard, Luc (2002), First Results from the ESO Distant Cluster Survey, Eso Astrophysics Symposia, Berlin/Heidelberg: Springer-Verlag, pp. 69–74, doi:10.1007/10856495_8, ISBN   3-540-43769-X , retrieved 2024-04-13
  30. ↑ Biron, Lauren (April 4, 2024). "First Results from DESI Make the Most Precise Measurement of Our Expanding Universe". Lawrence Berkeley National Laboratory. Retrieved April 15, 2024.
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