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gptkbp:instance_of
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gptkb:musical_instruments
|
|
gptkbp:calibration_methods
|
wavelength calibration
flat-fielding
sky subtraction
|
|
gptkbp:collaboration
|
gptkb:Caltech
gptkb:University_of_California
gptkb:NASA
Keck Observatory staff
|
|
gptkbp:collection
|
gptkb:spectroscopy
imaging
|
|
gptkbp:community
|
gptkb:astronomy
astrophysicists
planetary scientists
cosmologists
exoplanet researchers
galaxy formation researchers
stellar evolution researchers
|
|
gptkbp:data_reduction_software
|
MOSFIRE Data Reduction Pipeline
|
|
gptkbp:data_type
|
fits
|
|
gptkbp:designed_for
|
gptkb:astronomy
|
|
gptkbp:developed_by
|
gptkb:California_Institute_of_Technology
|
|
gptkbp:features
|
multi-object spectroscopy
|
|
gptkbp:frequency
|
0.9 to 2.5 micrometers
|
|
gptkbp:funding
|
gptkb:California_Institute_of_Technology
gptkb:National_Science_Foundation
|
|
gptkbp:has_ability
|
high-resolution spectroscopy
simultaneous observations of multiple objects
spectral resolution up to 3600
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
MOSFIRE
|
|
gptkbp:lighting
|
gptkb:2012
|
|
gptkbp:location
|
gptkb:Hawaii
|
|
gptkbp:observational_mode
|
multi-object mode
long-slit mode
|
|
gptkbp:operated_by
|
gptkb:W._M._Keck_Observatory
|
|
gptkbp:operational_status
|
active
|
|
gptkbp:pixel_scale
|
0.18 arcseconds per pixel
|
|
gptkbp:scientific_goals
|
stellar populations
exoplanet atmospheres
study of distant galaxies
|
|
gptkbp:sensor
|
Hawaii 2 RG
|
|
gptkbp:significance
|
important tool for infrared astronomy
|
|
gptkbp:type
|
near-infrared spectrograph
|
|
gptkbp:used_by
|
gptkb:Keck_Observatory
|
|
gptkbp:view
|
6.4 arcminutes
|
|
gptkbp:year
|
gptkb:2012
|
|
gptkbp:bfsParent
|
gptkb:Keck_Observatory
|
|
gptkbp:bfsLayer
|
6
|