COMBO-17 survey

E371575

The COMBO-17 survey is a deep multi-band astronomical imaging and photometric redshift survey designed to study galaxies, quasars, and large-scale structure across cosmic time.

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COMBO-17 survey canonical 1

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Statements (46)

Predicate Object
instanceOf astronomical survey
multi-band imaging survey
photometric redshift survey
fullName Classifying Objects by Medium-Band Observations in 17 filters
hasAnalysisType clustering analysis
galaxy type classification
luminosity function determination
statistical analysis of large samples
hasDataProduct galaxy classification catalogs
multi-band photometric catalogs
photometric redshift catalogs
quasar candidate catalogs
hasKeyFeature classification of objects by spectral energy distribution
deep multi-band imaging
medium-band spectral resolution from photometry
photometric redshift accuracy sufficient for large-scale structure studies
hasMethod photometric redshift estimation
spectral energy distribution fitting
hasObservationType multi-band photometry
optical imaging
hasRelevanceTo galaxy evolution studies
large-scale structure mapping
observational cosmology
quasar evolution studies
hasScienceGoal constrain cosmological parameters
identify quasars
measure photometric redshifts
study galaxies across cosmic time
study galaxy evolution
study large-scale structure of the Universe
study quasars across cosmic time
hasSelectionMethod multi-color selection
hasTemporalScope cosmic time
hasWavelengthRange optical
isDesignedFor cosmological studies
environmental dependence of galaxy properties
galaxy population statistics
quasar demographics
studiesObjectType active galactic nuclei
galaxies
galaxy clusters
large-scale structure
quasars
usesFilterType broad-band filters
medium-band filters
usesNumberOfFilters 17

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

MPG/ESO 2.2 m Telescope hasSurvey COMBO-17 survey