Preferred Name |
Optical astronomy |
Definitions |
Optical astronomy is the part of astronomy that uses optical instruments (mirrors, lenses, and solid-state detectors) to observe light from near-infrared to near-ultraviolet wavelengths. Visible-light astronomy, using wavelengths detectable with the human eyes (about 400–700 nm), falls in the middle of this spectrum. |
ID |
http://www.ivoa.net/rdf/uat#visible-astronomy |
broader | |
definition |
Optical astronomy is the part of astronomy that uses optical instruments (mirrors, lenses, and solid-state detectors) to observe light from near-infrared to near-ultraviolet wavelengths. Visible-light astronomy, using wavelengths detectable with the human eyes (about 400–700 nm), falls in the middle of this spectrum. |
exactMatch | |
prefLabel |
Optical astronomy |
related |
Delete | Mapping To | Ontology | Source |
---|---|---|---|
http://data.europa.eu/8mn/euroscivoc/cd9d6c59-4bf8-45cc-8a9c-8e465d2e526d | EUROSCIVOC | LOOM | |
http://astrothesaurus.org/uat/1776 | UAT | LOOM |