Visualisation gallery at AIP
This page is still under construction.
Flight around the 3D distribution of ~ 22,000 target stars for the Kepler2 mission.
StarHorse 2019
“Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G=18” by F.Anders et al. is published in Astronomy & Astrophysics.
HoloGalaxies@AIP
New website with several holographic videos and “do it yourself” templates.
MUSE: "Zahnarzt Sessel"
MUSE datacube.
processed by P.Weilbacher,
visualization:A.Khalatyan
Dunkle Materie Halos in 3D fusionieren
A merger tree in 3D: the spheres correspond to positions and sizes of dark matter halos that merge from redshift z~5 to z=0 to the most massive halo in the MDR1 cosmological simulation.
Simulierte Clustering-Daten
Click here to download datasets
Data: R.Winkler
DM->GAS->STERNE->HTSMock Rotation von LG64 M31 Kandidat
Simulation: Box=64Mpc/h, eff-resolution=4096^3
Redshift: ~0.9
Color coding: stars HST mock image- UVB=>RGB
Rendering region: R1~512kpc/h, R2~64kpc/h
Gasverteilung in lokaler Gruppe, CLUES B64_WM3
The image/movie shows the distribution of gas in the CLUESsimulation B64_WM3_186592, a resimulation with 4096 3particles, rendered with PMViewer.
Orion Nebel mit MUSE
The MUSE spectrograph produces data cubes, consisting of image slices at different wave lengths. A number of such slices (fitted to characteristic emission lines) is shown in this movie.