Participants. Galaxy Modelling with a Gaia mock catalogue
(The number of participants is limited to ~40)
|
Name |
Institute |
Interests |
Lunch |
Dinner |
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29 |
1 |
2 |
29 |
|
Daisuke Kawata |
MSSL,UCL,UK |
Generating Gaia Mock catalogue from N-body simulations. Spiral Structures, pattern speed and stellar motion around spiral arms. |
x |
x |
x |
x |
|
Francesca Figueras |
UB (Spain) |
Kinematic tracers from Spiral Structure models |
x |
x |
x |
x |
|
Mercč Romero-Gómez |
UB (Spain) |
Bar and Spiral Structure models |
x |
x |
x |
x |
|
Luis Aguilar |
UB , UNAM |
|
x |
x |
x |
x |
|
Teresa Antoja |
Kapteyn (Netherlands) |
|
x |
x |
x |
x |
|
Joao Alves |
University of Vienna |
Data visualization. 3D modeling of the local ISM |
x |
x |
x |
x |
|
Andre Moitinho |
SIM - U. Lisbon |
Type C participant. I'm interested in the selection of star clusters; Spiral arms; optically revealed star forming regions (Large scale star formation) |
x |
x |
x |
x |
|
Coryn Bailer-Jones |
MPIA, Heidelberg |
Modelling Gaia data using Bayesian methods (i.e. as participant type B); overview of the expected results/accuracies on the astrophysical parameters from CU8 (i.e. as participant type C). |
x |
x |
x |
x |
|
Andreea Font |
University of Birmingham |
Generating Gaia mock catalogues from numerical simulations and comparisons with the data (groups A and B). |
x |
x |
x |
x |
|
Robyn Sanderson |
Kapteyn Astronomical Institute (Netherlands) |
Constraining the dark matter distribution in the outer Galaxy with [mock] Gaia data (participant type B). |
x |
x |
x |
x |
|
E. Athanassoula |
LAM, Marseille |
The bar/bulge and spirals in the MW |
x |
x |
x |
x |
|
Xavier Luri |
UB - ICC- IEEC |
Luminosity calibrations, distance estimation |
x |
x |
x |
x |
|
Yago Isasi |
UB - ICC - IEEC |
Explotation from the knowledge discovery point of view. Several technical architecture tests. |
x |
x |
x |
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