Statements (43)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:astronomy
|
| gptkbp:analysis |
used for astrophysics research
|
| gptkbp:collaborates_with |
international research institutions
|
| gptkbp:contributes_to |
understanding of dark matter
understanding of black holes understanding of supernova remnants understanding of active galactic nuclei |
| gptkbp:designed_by |
gptkb:H._E._S._S._collaboration
|
| gptkbp:diameter |
28 meters
|
| gptkbp:has_ability |
detects very high energy gamma rays
|
| gptkbp:has_technology |
multi-wavelength observations
high-speed data acquisition advanced trigger systems imaging atmospheric Cherenkov technique sophisticated analysis software |
| https://www.w3.org/2000/01/rdf-schema#label |
H. E. S. S. II telescope
|
| gptkbp:is_funded_by |
gptkb:European_Union
|
| gptkbp:is_observed_in |
cosmic rays
gamma rays |
| gptkbp:lighting |
gptkb:2012
|
| gptkbp:location |
gptkb:Namibia
|
| gptkbp:notable_galaxies |
gptkb:5
|
| gptkbp:operated_by |
gptkb:H._E._S._S._collaboration
|
| gptkbp:operational_since |
gptkb:2012
|
| gptkbp:part_of |
gptkb:H._E._S._S._array
|
| gptkbp:scientific_goals |
collaborate with other observatories
map the distribution of dark matter publish research findings search for new physics investigate the nature of gamma-ray bursts monitor variable sources conduct long-term monitoring of sources develop new technologies for astronomy educate the public about astrophysics explore the origin of cosmic rays study cosmic accelerators support graduate and postdoctoral research train new scientists in observational techniques enhance international collaboration in astrophysics |
| gptkbp:type |
very high energy gamma-ray observatory
|
| gptkbp:view |
5 degrees
|
| gptkbp:bfsParent |
gptkb:High_Energy_Astronomical_Observatory-2
|
| gptkbp:bfsLayer |
6
|