• Facets (new session)
• Description
• Metadata
• Settings
  • Rule: ActivityStreamsMapasEquivalentb3sb3sifpdbprdf-labelfacetshttp://dbpedia.org/resource/inference/rules/dbpedia#http://dbpedia.org/resource/inference/rules/opencyc#http://dbpedia.org/resource/inference/rules/umbel#http://dbpedia.org/resource/inference/rules/yago#http://dbpedia.org/schema/property_rules#http://www.ontologyportal.org/inference/rules/SUMO#http://www.ontologyportal.org/inference/rules/WordNet#http://www.w3.org/2002/07/owl#ldpoplwebskos-transurn:det:rdf:labelvirtrdf-labelvirtrdf-urlNone
    
  • Inverse Functional Properties: Disabled (fastest) Apply to subjects only Apply to objects only Apply to both subjects and objects
  • "Same As": Disabled (fastest) Apply to subjects only Apply to objects only Apply to both subjects and objects (recommended) Apply to subjects, objects and predicates (not recommended on big datasets) Apply to predicates only (special use cases only)

About: Robotic Lunar Observatory     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatDefunctAstronomicalObservatories, within Data Space : dbpedia.org associated with source document(s)

Type: placeyago:WikicatAstronomicalObservatoriesInArizonayago:WikicatBuildingsAndStructuresInFlagstaff,Arizonageo:SpatialThingyago:Artifact100021939yago:Building102913152yago:Object100002684yago:Observatory103839671yago:PhysicalEntity100001930yago:YagoGeoEntityyago:YagoPermanentlyLocatedEntityyago:Structure104341686yago:Whole100003553yago:WikicatDefunctAstronomicalObservatories New Facet based on Instances of this Class

The Robotic Lunar Observatory (ROLO) is an astronomical observatory funded by NASA and located at the United States Geological Survey Flagstaff Science Campus atop McMillan Mesa in Flagstaff, Arizona. Its purpose is to enable the Moon to be used as a radiometric calibration reference for Earth-orbiting remote-sensing spacecraft instruments. The ROLO project is currently ongoing, but the program ceased observations in September 2003. The facility is maintained for calibration and instrument characterization purposes. It consists of two 20 cm (7.9 in) Ritchey-Chrétien telescopes attached to an equatorial mount made by DFM Engineering. One telescope is fitted with a sensor optimized for visible and near-infrared (VNIR) wavelengths, while the other is tuned to short-wavelength infrared (SWIR)