@prefix ns0: <https://gcmd.earthdata.nasa.gov/kms#> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

<https://gcmd.earthdata.nasa.gov/kms/concept/f81fffc6-6742-4d69-b30a-c125fde64738>
  ns0:reference [ ] ;
  skos:changeNote """2023-07-14 07:59:14.0 [tstevens]  
insert AltLabel (id: null
category: primary
text: Hyperspectral Thermal Emission Spectrometer
language code: en); 
insert Definition (id: null
text: The Hyperspectral Thermal Emissions Spectrometer (HyTES) instrument has 512 pixels across track with pixel sizes in the range of 5 to 50 m depending on aircraft flying height and 256 spectral channels between 7.5 and 12 µm. The HyTES design is built upon a Quantum Well Infrared Photodetector (QWIP) focal plane array (FPA), a cryo-cooled Dyson Spectrometer and a high-efficiency, concave blazed grating, produced using E-beam lithography. HyTES was originally developed to support the Hyperspectral Infrared Imager (HyspIRI) mission. HyTES is useful for a number of applications, including high-resolution surface temperature and emissivity measurements, point sources of air pollution, and volcano observations.
language code: en); 
""", """2023-07-14 14:09:01.0 [tstevens]  
update Definition (The Hyperspectral Thermal Emission Spectrometer (HyTES) instrument has 512 pixels across track with pixel sizes in the range of 5 to 50 m depending on aircraft flying height and 256 spectral channels between 7.5 and 12 µm. The HyTES design is built upon a Quantum Well Infrared Photodetector (QWIP) focal plane array (FPA), a cryo-cooled Dyson Spectrometer and a high-efficiency, concave blazed grating, produced using E-beam lithography. HyTES was originally developed to support the Hyperspectral Infrared Imager (HyspIRI) mission. HyTES is useful for a number of applications, including high-resolution surface temperature and emissivity measurements, point sources of air pollution, and volcano observations.); 
""", """2023-07-14 08:01:02.0 [tstevens]  
update Definition (https://airbornescience.nasa.gov/instrument/hytes; https://hytes.jpl.nasa.gov/); 
""", """2023-07-14 07:59:56.0 [tstevens]  
update Definition (https://airbornescience.nasa.gov/instrument/hytes                                                                    https://hytes.jpl.nasa.gov/); 
""", """2023-07-14 07:57:49.0 [tstevens] Insert Concept 
add broader relation (HyTES [f81fffc6-6742-4d69-b30a-c125fde64738,1380223] - Imaging Spectrometers/Radiometers [944b7691-af37-4fb4-9393-c114e7997829,1371941]); 
""" ;
  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/944b7691-af37-4fb4-9393-c114e7997829> ;
  ns0:altLabel [ ] ;
  skos:definition "The Hyperspectral Thermal Emission Spectrometer (HyTES) instrument has 512 pixels across track with pixel sizes in the range of 5 to 50 m depending on aircraft flying height and 256 spectral channels between 7.5 and 12 µm. The HyTES design is built upon a Quantum Well Infrared Photodetector (QWIP) focal plane array (FPA), a cryo-cooled Dyson Spectrometer and a high-efficiency, concave blazed grating, produced using E-beam lithography. HyTES was originally developed to support the Hyperspectral Infrared Imager (HyspIRI) mission. HyTES is useful for a number of applications, including high-resolution surface temperature and emissivity measurements, point sources of air pollution, and volcano observations."@en ;
  skos:inScheme <https://gcmd.earthdata.nasa.gov/kms/concepts/concept_scheme/instruments> ;
  skos:prefLabel "HyTES"@en ;
  a skos:Concept .

<https://gcmd.earthdata.nasa.gov/kms/concept/944b7691-af37-4fb4-9393-c114e7997829>
  skos:prefLabel "Imaging Spectrometers/Radiometers"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/f81fffc6-6742-4d69-b30a-c125fde64738> .