Statements (67)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:observatory
|
| gptkbp:area |
X-ray emissions
Cosmic voids Galaxy filaments Baryonic_matter |
| gptkbp:canBe |
gptkb:Telescopes
|
| gptkbp:canEstablish |
Gravitational lensing
Dynamical activity Non-thermal emissions X-ray cooling flows |
| gptkbp:composedOf |
Galaxies
|
| gptkbp:hasInfluenceOn |
Galaxy evolution
Galaxy formation rates |
| https://www.w3.org/2000/01/rdf-schema#label |
Galaxy Clusters
|
| gptkbp:is_featured_in |
Massive structures
|
| gptkbp:isCitedIn |
Cosmology
Galaxy dynamics |
| gptkbp:isCounteredBy |
Spectroscopy
Radio waves Numerical simulations Optical imaging Galaxy redshift surveys Multi-wavelength observations Cluster catalogs Cluster lensing Mass and temperature X-ray luminosity |
| gptkbp:isFoundIn |
Various environments
Large-scale structures |
| gptkbp:isHeldAnnually |
Gravity
|
| gptkbp:isHomeTo |
Supermassive black holes
|
| gptkbp:isImportantFor |
Understanding galaxy formation
Studying cosmic microwave background Studying the evolution of the universe Understanding large-scale structure |
| gptkbp:isLinkedTo |
Galaxy mergers
|
| gptkbp:isLocatedIn |
gptkb:Universe
|
| gptkbp:isMaintainedBy |
Galaxy interactions
Galaxy morphology |
| gptkbp:isOftenMadeWith |
Galaxy clusters mergers
|
| gptkbp:isStudiedIn |
Astrophysics
|
| gptkbp:isUsedFor |
gptkb:Superclusters
General relativity Cosmological parameters Different cosmic epochs Different redshifts Filaments of the cosmic web Galaxy groups Massive versus less massive clusters Morphological types Poor clusters Rich clusters |
| gptkbp:isUsedIn |
Astrophysical research
Dark matter distribution |
| gptkbp:isUtilizedFor |
Galaxy surveys
Gravitational lensing techniques |
| gptkbp:keyIssues |
Understanding the universe's expansion
Studying dark energy Understanding cosmic structure formation Understanding galaxy cluster physics Understanding the large-scale structure of the universe. |
| gptkbp:mayHave |
Computer simulations
Dark matter Astrophysical simulations Gravitational wave observations Hot gas Hundreds of galaxies |