• Skip to main content
  • Skip to primary sidebar
  • Skip to footer

Dark Energy Spectroscopic Instrument (DESI)

  • / science /
    • science overview
    • cosmology and dark energy
    • redshifts and distance
    • mapping the universe
    • the DESI science mission
    • the DESI survey
    • imaging surveys
  • / instrument /
    • instrument overview
    • telescope
      • tohono o’odham
    • corrector
    • focal plane system
    • fiber system
    • spectrograph
    • instrument control system
    • data systems
    • bringing DESI to life
      • commissioning Instrument
      • protoDESI
  • / collaboration /
    • DESI team
    • DESI builders
    • collaborating institutions
    • sponsors
    • code of conduct
    • vendors
    • collaboration policies
  • / press /
    • announcements
    • in the news
    • press releases
    • tweets by desisurvey
    • blog
    • acknowledgments
  • / galleries /
    • videos
    • image gallery
  • / for scientists /
    • data releases
    • instrument design
    • imaging data
    • target selection and survey validation
    • theory and simulations
    • other DESI science
    • key publications
    • all DESI papers
    • team login
    • request a DESI speaker
    • internal
  • / education & outreach /
    • meet a DESI member
    • blog
    • planetarium show
    • DESI high
    • interactive visualizations
    • DESI Merch

DESI imaging leaves a legacy at infrared wavelengths

November 17, 2020 by

Aaron Meisner, NOIRLab
November 17, 2020

It’s remarkable to think that our DESI Legacy Surveys team completed on order a thousand nights of ground-based observing from Kitt Peak and Cerro Tololo. All the while in low-Earth orbit, NASA’s WISE satellite has been steadily and reliably amassing nearly a decade of full-sky data at infrared wavelengths of 3-5 microns. WISE continuously obtains a new pair of degree-sized images every ~10 seconds, observing around the clock.

Selection of DESI’s luminous red galaxy and quasar targets requires not only optical data from telescopes like the Mayall and Blanco, but also infrared fluxes from WISE. It’s therefore crucial that DESI target selection make full use of the entire WISE data set. Once each year, we download millions of recently acquired raw WISE images to NERSC and use these to update DESI’s custom, coadded WISE maps. As of DR9, the raw WISE data set assembled at NERSC has grown to a quarter petabyte in size! Each year, upon completion of our latest WISE map-making efforts, we can once again declare that DESI has created the deepest ever full-sky maps and catalogs at mid-infrared wavelengths. DR9 incorporates seven years of WISE observations, versus five years for DR8 and just one year for DR1.

WISE has scanned the entire sky more than a dozen times, lending a strong time-domain component to the Legacy Surveys data products. Our Legacy Surveys WISE light curves for ~2 billion sources represent a totally unprecedented and as-yet little explored data set. Mining DR9’s infrared data products, especially in combination with optical Legacy Surveys photometry and DESI spectroscopy, will provide a diverse array of scientific opportunities throughout the coming years.

Light echoes from a Milky Way supernova, as seen in the time-domain ‘unWISE’ coadds of Legacy Surveys DR9. These custom WISE coadds also enable DESI’s selection of faint variable quasar candidates.

Filed Under: blog

Primary Sidebar

  • DESI High, the School of the Dark Universe, is Back!
  • DESI’s Evolving Dark Energy Lights up the News
  • At the Big Reveal: DESI’s December 2024 Unblinding Results
  • DESI DR2 Results: March 19 Guide
  • Closing Our Eyes to Truly See — “Blinding” in DESI’s Analysis of Its Cosmological Measurements
  • Charting the Dark Cosmic Web: Where DESI and Imaging Surveys Intersect
  • BaoBan Greets Spectators at 2025 Tohono O’odham Rodeo Parade
  • DESI Finds Black Holes are Common in Small Galaxies Too
  • Brushing Away the Dust to Uncover Cosmology: Examining the Sigma-8 Tension with DESI Galaxies
  • DESI’s 50M Milestone and a “Biggest Breakthrough” Honor
  • DESI 2024 Results: November 19 Guide
  • All is Not Lost: Tiny Groups of Galaxies Remember Their Origins
  • “5000 Eyes” Premieres in Mexico City
  • DESI 2024 Supporting Papers: June 11 Guide
  • DESI Joins in Hosting Kitt Peak Open Night for Tohono O’odham Nation; BaoBan Makes Guest Appearances
  • DESI 2024 in the News: Science Communicators Discuss the Cosmology Results from DESI’s Inaugural Year
  • DESI 2024 in the News: Is Dark Energy Weakening? New Uncertainty Invites Optimism About the Fate of the Universe
  • DESI 2024 Supporting Papers: April 11 Guide
  • DESI 2024 Results: April 4 Guide
  • A Record-Breaking Night
  • BaoBan Spotted at the Tohono O’odham Rodeo
  • A very nearby Type II Supernova in the Galaxy Messier 101
  • The DESI Early Data Release is now available
  • The new DESI ambassador: BaoBan
  • 5000 Eyes: creating the DESI planetarium film
  • Dusty views of the southwestern sky
  • Sneaking around with DESI data
  • Lightning and a lunar eclipse over Kitt Peak
  • Untangling the cosmic web
  • Recovery effort update two months after the Contreras Fire
  • First batch of Year 1 Key Project 1 papers
  • Contreras Fire threatens DESI and Kitt Peak National Observatory
  • One year and 12.8 million galaxy redshifts
  • DESI on a T-shirt (and stickers of course!)
  • Selecting targets for the DESI survey
  • The old is new again: social distancing while mapping the universe
  • Congratulations to Frank Valdes
  • The DESI peculiar velocity survey
  • DESI breaking records
  • A DIY guide for upgrading your $100 million world-class astronomical instrument
  • An upgraded DESI returns to the sky
  • Cosmic cartography
  • Diversity of DESI SV quasars
  • The beginnings of the 3-dimensional map
  • What do DESI’s 5000 eyes see?
  • Plugging away
  • DESI begins search for elusive dark energy
  • DESI begins its “One-Percent Survey”
  • DESI embarks on Survey Validation
  • An undergrad perspective on DESI
  • Women in DESI on International Women’s Day
  • Hunting the oxygen doublet in distant galaxies
  • Congratulations to David Weinberg
  • DESI imaging leaves a legacy at infrared wavelengths
  • DESI target selection
  • DESI successfully completes commissioning phase

Footer

TEAM LOGIN

twitter   instagram   facebook

Copyright © 2018 Dark Energy Spectroscopic Instrument [DESI]

Copyright © 2025 · Parallax Pro DESI on Genesis Framework · WordPress · Log in