Statements (52)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:can_detect |
gamma rays
|
| gptkbp:contains |
gptkb:Chandra_X-ray_Observatory
gptkb:Fermi_Gamma-ray_Space_Telescope HESS (High Energy Stereoscopic System) MAGIC (Major Atmospheric Gamma Imaging Cherenkov Telescope) VERITAS (Very Energetic Radiation Imaging Telescope Array System) |
| gptkbp:contributes_to |
gptkb:dark_matter
gptkb:Supernova cosmic rays stellar evolution the early universe exotic astrophysical phenomena |
| gptkbp:has_contributed_to_discoveries_of |
new cosmic phenomena
new astrophysical sources |
| gptkbp:has_limitations |
background noise
data processing challenges instrument sensitivity |
| gptkbp:has_role |
gptkb:space_exploration
gptkb:scientific_research |
| https://www.w3.org/2000/01/rdf-schema#label |
gamma-ray telescope
|
| gptkbp:is_affected_by |
atmospheric conditions
|
| gptkbp:is_analyzed_in |
astrophysicists
|
| gptkbp:is_designed_to |
maximize sensitivity
improve resolution increase field of view |
| gptkbp:is_essential_for |
gamma-ray astronomy
understanding the universe |
| gptkbp:is_funded_by |
government grants
private donations |
| gptkbp:is_observed_in |
gptkb:active_galactic_nuclei
supernovae black holes gamma-ray bursts pulsars |
| gptkbp:is_part_of |
international collaborations
multi-wavelength astronomy |
| gptkbp:is_studied_for |
the universe's most energetic processes
|
| gptkbp:launched_in |
gptkb:space
|
| gptkbp:operated_by |
research institutions
space agencies |
| gptkbp:operates_in |
high-energy astronomy
|
| gptkbp:provides_information_on |
cosmic events
|
| gptkbp:requires |
high-altitude locations
|
| gptkbp:used_in |
astrophysics
|
| gptkbp:uses |
gptkb:Earth
|
| gptkbp:uses_technology |
semiconductor detectors
scintillation detectors Cherenkov radiation detection |
| gptkbp:bfsParent |
gptkb:Spektr-M
gptkb:Electromagnetic_Telescopes |
| gptkbp:bfsLayer |
6
|