Dark Energy Survey

E76900

The Dark Energy Survey is a large international astronomical project that uses a wide-field camera on a Chilean telescope to map hundreds of millions of galaxies and study the nature of dark energy and cosmic acceleration.

All labels observed (5)

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Statements (70)

Predicate Object
instanceOf astronomical survey
cosmology experiment
international scientific collaboration
abbreviation DES
cameraFieldOfView approximately 3 square degrees
cameraResolution about 570 megapixels
collaborationSize over 400 scientists
cosmologicalProbe Type Ia supernovae
baryon acoustic oscillations
cluster counts
weak lensing and galaxy clustering
countryOfLeadInstitution United States of America
surface form: United States
countryOfObservation Chile
dataPolicy public data releases
dataRelease Dark Energy Survey self-linksurface differs
surface form: DES Data Release 1

Dark Energy Survey self-linksurface differs
surface form: DES Data Release 2

Dark Energy Survey self-linksurface differs
surface form: DES Data Release 3
endYear 2019
field astrophysics
observational cosmology
filter Y-band
g-band
i-band
r-band
z-band
fundingAgency U.S. Department of Energy
National Science Foundation
surface form: U.S. National Science Foundation
goal constrain the equation of state of dark energy
discover thousands of Type Ia supernovae
map hundreds of millions of galaxies
measure the growth of cosmic structure
test models of cosmic acceleration
hemisphere southern sky
hostObservatoryOperator National Optical Astronomy Observatory
instrumentAbbreviation Dark Energy Camera
surface form: DECam
leadInstitution Fermi National Accelerator Laboratory
numberOfFilters 5
numberOfInstitutions over 25 institutions
participatingRegions Australia
Europe
South America
United States of America
surface form: United States
producedCatalog cluster catalogs
galaxy catalogs
supernova light-curve catalogs
weak lensing shear catalogs
relatedProject Dark Energy Spectroscopic Instrument
Legacy Survey of Space and Time
researchArea Milky Way
surface form: Milky Way structure

cosmic acceleration
dark energy
galaxy clustering
galaxy evolution
large-scale structure of the Universe
near-Earth objects
supernova cosmology
weak gravitational lensing
skyCoverage about 5000 square degrees
startYear 2013
supernovaFields 10 fields
surveyDuration 6 years
surveyPhase main survey
science verification phase
supernova survey
telescope Víctor M. Blanco 4-meter Telescope
surface form: Víctor M. Blanco Telescope
telescopeLocation Cerro Tololo Inter-American Observatory
usesInstrument Dark Energy Camera
wavelengthRange near-infrared
optical
website https://www.darkenergysurvey.org/

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Referenced by (14)

Full triples — surface form annotated when it differs from this entity's canonical label.

CTIO hostsProject Dark Energy Survey
Dark Energy Camera developedBy Dark Energy Survey
this entity surface form: Dark Energy Survey collaboration
Dark Energy Camera operatedFor Dark Energy Survey
Dark Energy Camera scienceProgram Dark Energy Survey
Dark Energy Survey dataRelease Dark Energy Survey self-linksurface differs
this entity surface form: DES Data Release 1
Dark Energy Survey dataRelease Dark Energy Survey self-linksurface differs
this entity surface form: DES Data Release 2
Dark Energy Survey dataRelease Dark Energy Survey self-linksurface differs
this entity surface form: DES Data Release 3
DES fullName Dark Energy Survey
DES acronymFor Dark Energy Survey
DECam Legacy Survey relatedProject Dark Energy Survey