Statements (91)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:spectrometer
|
| gptkbp:analyzes |
cosmic structures
|
| gptkbp:associated_with |
gptkb:Subaru_Telescope
|
| gptkbp:collaborated_with |
global astronomical community
|
| gptkbp:collaborates_with |
international research teams
|
| gptkbp:collaboration |
international research teams
|
| gptkbp:collaborator |
gptkb:National_Astronomical_Observatory_of_Japan
|
| gptkbp:contributes_to |
exoplanet studies
cosmology research |
| gptkbp:designed_for |
gptkb:astronomy
|
| gptkbp:developed_by |
gptkb:international_collaboration
gptkb:Subaru_Telescope |
| gptkbp:enables |
large-scale surveys
redshift measurements |
| gptkbp:enhances |
observational astronomy
understanding of the universe spectroscopic capabilities |
| gptkbp:features |
fiber optic technology
|
| gptkbp:first_light_achieved |
gptkb:2019
|
| gptkbp:frequency |
0.38 to 1.8 micrometers
|
| gptkbp:has_component |
detectors
optical fibers gratings |
| gptkbp:has_function |
spectral data
|
| gptkbp:has_view_of |
1.3 degrees
|
| https://www.w3.org/2000/01/rdf-schema#label |
Prime Focus Spectrograph
|
| gptkbp:improves |
data collection efficiency
|
| gptkbp:improves_understanding_of |
galaxy formation
|
| gptkbp:include |
new insights into dark matter
|
| gptkbp:input_output |
spectra
|
| gptkbp:instrument |
gptkb:CD-ROM
state-of-the-art technology |
| gptkbp:is_a |
gptkb:scientific_instruments
|
| gptkbp:is_aimed_at |
understanding cosmic expansion
|
| gptkbp:is_capable_of |
multi-object spectroscopy
wide-field observations spectroscopic redshift measurements |
| gptkbp:is_designed_for |
large-scale galaxy surveys
|
| gptkbp:is_designed_to |
observe faint objects
|
| gptkbp:is_equipped_with |
spectral resolution capabilities
|
| gptkbp:is_expected_to |
future astronomical research.
produce significant discoveries |
| gptkbp:is_funded_by |
gptkb:Japanese_government
|
| gptkbp:is_integrated_with |
Subaru Telescope's optics
|
| gptkbp:is_located_at |
gptkb:Hawaii
|
| gptkbp:is_optimized_for |
wide-field observations
|
| gptkbp:is_part_of |
astronomical survey projects
Subaru Strategic Program Subaru Telescope project large telescope initiative |
| gptkbp:is_significant_for |
cosmology research
|
| gptkbp:is_studied_for |
stellar evolution
|
| gptkbp:is_used_for |
stellar evolution research
stellar population studies stellar population synthesis supernova observations intergalactic medium studies dark matter studies time-domain astronomy quasar research high-redshift galaxy studies stellar dynamics research chemical composition analysis stellar kinematics research chemical enrichment studies extragalactic surveys spectral line studies nearby galaxy studies galactic archaeology galaxy cluster analysis |
| gptkbp:is_utilized_for |
mapping the universe
|
| gptkbp:is_utilized_in |
galactic archaeology
|
| gptkbp:lighting |
gptkb:2020
|
| gptkbp:location |
Mauna Kea, Hawaii
|
| gptkbp:number_of_fibers |
4000
|
| gptkbp:operated_by |
gptkb:National_Astronomical_Observatory_of_Japan
|
| gptkbp:operational_since |
gptkb:2020
|
| gptkbp:provides |
high-resolution spectra
high-throughput spectroscopy |
| gptkbp:provides_support_for |
gptkb:dark_matter
|
| gptkbp:resolution |
up to 10000
|
| gptkbp:scientific_goals |
exoplanet studies
dark energy research study of galaxy formation |
| gptkbp:supports |
large surveys
|
| gptkbp:used_by |
gptkb:Mauna_Kea_Observatory
|
| gptkbp:uses |
multi-object spectroscopy
|
| gptkbp:uses_technology |
fiber optics
|
| gptkbp:utilizes |
advanced optics
advanced detectors |
| gptkbp:view |
1.5 degrees
|