|
gptkbp:instance_of
|
gptkb:spectrometer
|
|
gptkbp:average_temperature
|
around 40 K
|
|
gptkbp:characteristic
|
Cassegrain design
|
|
gptkbp:collaboration
|
gptkb:ESA
gptkb:Northrop_Grumman
gptkb:Ariane_5
gptkb:NASA
|
|
gptkbp:community
|
gptkb:astronomy
astrophysicists
planetary scientists
cosmologists
space scientists
|
|
gptkbp:cooling_system
|
passive and active systems
cryogenic system
|
|
gptkbp:data_transmission
|
high-speed communication
|
|
gptkbp:data_type
|
FITS
|
|
gptkbp:designed_by
|
gptkb:NASA
|
|
gptkbp:designed_for
|
gptkb:James_Webb_Space_Telescope
|
|
gptkbp:developed_by
|
gptkb:ESA
gptkb:European_Space_Agency
|
|
gptkbp:filter_type
|
broadband filters
narrowband filters
|
|
gptkbp:frequency
|
0.6 to 5.0 micrometers
|
|
gptkbp:grating_types
|
reflection gratings
transmission gratings
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Near Infrared Spectrograph (NIRSpec)
|
|
gptkbp:image_processing
|
onboard processing
ground processing
|
|
gptkbp:is_capable_of
|
multi-object spectroscopy
|
|
gptkbp:launch_date
|
gptkb:2021
|
|
gptkbp:launch_vehicle
|
gptkb:Ariane_5
|
|
gptkbp:lighting
|
gptkb:2022
|
|
gptkbp:mission_duration
|
10 years
|
|
gptkbp:operates_in
|
near-infrared spectrum
|
|
gptkbp:operational_status
|
multi-object spectroscopy
integral field spectroscopy
single-object spectroscopy
|
|
gptkbp:powers
|
approximately 200 watts
|
|
gptkbp:provides
|
spectrum analysis
|
|
gptkbp:resolution
|
up to 3000
|
|
gptkbp:scientific_goals
|
observe distant galaxies
study exoplanets
analyze star formation
investigate cosmic dawn
|
|
gptkbp:sensitivity
|
0.6 to 5 microns
|
|
gptkbp:sensor
|
Hg Cd Te
|
|
gptkbp:storage
|
solid-state drives
|
|
gptkbp:used_for
|
spectroscopy in the near-infrared spectrum
|
|
gptkbp:user_interface
|
web-based interface
|
|
gptkbp:uses
|
gptkb:microshutter_array
|
|
gptkbp:view
|
3.2 arcminutes
|
|
gptkbp:weight
|
approximately 200 kg
|
|
gptkbp:bfsParent
|
gptkb:James_Webb_Space_Telescope
|
|
gptkbp:bfsLayer
|
4
|