Statements (55)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:spacecraft
|
| gptkbp:bfsLayer |
4
|
| gptkbp:bfsParent |
gptkb:Cosmic_Microwave_Background
|
| gptkbp:analysis |
gptkb:Planck_Collaboration
|
| gptkbp:archives |
gptkb:ESA's_Planck_Legacy_Archive
|
| gptkbp:collaborations |
over 200 scientists
scientists from various countries |
| gptkbp:data_type |
HEASARCFITS
|
| gptkbp:frequency |
9 frequency channels
|
| gptkbp:headquarters |
gptkb:Paris,_France
|
| https://www.w3.org/2000/01/rdf-schema#label |
Planck mission
|
| gptkbp:image |
multi-frequency analysis
|
| gptkbp:impact |
understanding of the universe's composition
constraints on neutrino masses improved measurements of the CMB power spectrum new insights into dark matter refined models of the universe |
| gptkbp:instrument |
High Frequency Instrument
Low Frequency Instrument sensitive detectors |
| gptkbp:is_observed_in |
gptkb:spacecraft
gptkb:Monarch temperature fluctuations large scale structure of the universe polarization of the CMB |
| gptkbp:launch_site |
gptkb:Guiana_Space_Centre
|
| gptkbp:launch_vehicle |
gptkb:opera
|
| gptkbp:launched |
May 14, 2009
|
| gptkbp:legacy |
foundation for future missions
|
| gptkbp:mission |
gptkb:Spitzer_Space_Telescope
gptkb:Chandra_X-ray_Observatory gptkb:James_Webb_Space_Telescope gptkb:Fermi_Gamma-ray_Space_Telescope gptkb:Herschel_Space_Observatory gptkb:Euclid gptkb:character October 2013 |
| gptkbp:mission_duration |
approximately 4 years
|
| gptkbp:objective |
map cosmic microwave background radiation
|
| gptkbp:operated_by |
gptkb:spacecraft
|
| gptkbp:products |
high precision
|
| gptkbp:publishes |
over 100 papers
|
| gptkbp:released |
gptkb:2015
|
| gptkbp:research |
atmospheric effects
instrumental noise full sky survey foreground contamination |
| gptkbp:result |
published in 2018
|
| gptkbp:significance |
improved understanding of the universe's age
constraints on cosmological parameters detection of baryon acoustic oscillations evidence for cosmic inflation mapping of the early universe measurement of the Hubble constant |
| gptkbp:successor |
gptkb:WMAP
|