We present a visual analytics tool, based on the VisIVO suite, to exploit a combination of all new-generation surveys of the Galactic Plane to study the star formation process of the Milky Way. The tool has been developed within the VIALACTEA project, founded by the 7th Framework Programme of the European Union, that creates a common forum for the major new-generation surveys of the Milky Way Galactic Plane from the near-infrared to the radio, both in thermal continuum and molecular lines. Massive volumes of data are produced by space missions and ground-based facilities and the ability to collect and store them is increasing at a higher pace than the ability to analyze them. This gap leads to new challenges in the analysis pipeline to discover information contained in the data. Visual analytics focuses on handling these massive, heterogeneous, and dynamic volumes of information accessing the data previously processed by data mining algorithms and advanced analysis techniques with highly interactive visual interfaces offering scientists the opportunity for in-depth understanding of massive, noisy, and high-dimensional data.
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Tag
ASI
Astri
campo magnetico
catalogo
CHEOPS
Cherenkov
corona solare
coronografo
Cta
ESA
ESO
esopianeti
Etna
eventi-seminari
evoluzione
formazione planetaria
GAIA
galassie
GAPS
Giove
HARPS-N
idrogeno
Inaf
jwst
Metis
migrazione
plasma
Plato
radio
radiotelescopio
raggi gamma
Serra La Nave
Sistema Solare
SKA
Solar Orbiter
Sole
space weather
stelle
TESS
test
TNG
transito
ultravioletto
velocità radiale
Via Lattea