2016 Workshop
Scientific Organizing Committee
L. Sodre (USP, Sao Paulo, Brasil)
M. Makler (ICRA,Rio Janeiro, Brasil)
S. Pedrosa (IAFE, Buenos Aires, Argentina)
D. G. Lambas (IATE, Cordoba, Argentina)
N. Padilla (PUC, Chile)
D. Minniti (UNAB, Chile)
P. Tissera (UNAB, Chile)
V. Motta (Universidad de Valparaiso, Chile)
Local Organizing Committee
Y. Apostolovski (UNAB, Chile)
A. Rojas (UNAB, Chile)
J. Pullen (UNAB, Chile)
P. Tissera (UNAB, Chile)
Main Topics
Galaxies in different environments: Dynamics and Galaxy Populations
The formation of galaxies in hydrodynamical simulations
The VVV Survey
Semi-analytical models for galaxy formation
Monday - November 21, 2016
09:30 - 10:00
10:00 - 10:30
10:30 - 10:50
10:50 - 11:10
11:10 - 11:40
11:40 - 12:00
12:00 - 12:20
12:20 - 12:40
12:40 - 13:00
13:00 - 14:30
14:30 - 14:50
14:50 - 15:10
15:10 - 15:30
15:30 - 15:50
15:50 - 16:10
16:10 - 16:30
16:30
19:30
Registration
Welcome
The two metallicity components of the Galactic bulge.
Status of the J-PAS, J-PLUS and S-PLUS surveys.
Coffee Break
The VVV Extended Survey.
Currents projects at the Numerical Astrophysics Group.
Combining strong lensing and dynamics to probe the mass distribution in galaxy groups/clusters.
Gravitational arcs as cosmological and astrophysical probes: the case of Stripe 82.
Lunch & Discussion
Testing gravity with cosmic voids.
The metallicity gradients of disc galaxies.
Early-type galaxy formation: understanding the role of the environment.
SOXS an optical and infrared spectrograph for the transient universe.
The shell galaxy NGC4104 in a young fossil group.
Coffee Break
Discussion SAN
Dinner to be confirmed (price and place)
M. Zoccali, E. Treister, P. Tissera
Manuela Zoccali
Laerte Sodre
Dante Minniti
Susana Pedrosa
Veronica Motta
Martin Makler
Nelson Padilla
Patricia Tissera
Ricardo Demarco
Giuliano Pignata
Gastão B. Lima
Tuesday - November 22, 2016
10:00 - 10:20
10:20 - 10:40
10:40 - 11:00
11:00 - 11:30
11:30 - 11:50
11:50 - 12:10
12:10 - 12:30
12:30 - 12:50
12:50 - 13:00
13:30
15:00
SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of 'typical' star-forming galaxies at z = 0.8 - 2.2.
The impact of assembly bias in the galaxy clustering.
Dark matter response to galaxy assembly history.
Coffe Break
Testing parametric dark energy models using strong lensing measurements in galaxy clusters.
Non Parametric Morphologies of Mergers in the Illustris Simulation.
Probing the stellar fraction in dark matter haloes of lensing galaxies using microlensing.
Integral Field Spectroscopy of Arcs - Unveiling the hundreds pc of a star-forming galaxy at redshift 0.7-2.5
Conclusions
Lunch & Discussion
Coordinators Meeting
Juan Molina
Sergio Contreras
Celeste Artale
Juan Magaña
Lucas Bignone
Karina Rojas
Damian Mast
Program
Participants
Damian Mast
Giuliano Pignata
Ezequiel Triester
Juan Molina
Andres Meza
Catalina Mora
Astrid San Martin
Manuela Zoccali
Patricia Tissera
Ricardo Demarco
Catalina Flores
Katherine Montenegro
Gastão B. Lima Neto
Lucas Bignone
Emanuel Sillero
Karina Rojas
Juan Magaña
Martin Makler
Joaquín Armijo Torres
Roberto Gonzalez
Dante Minniti
Veronica Motta
Alejandra Rojas Lilayu
Maria Celeste Artale
Laerte Sodre
Yordanka Apostolovski
Susana Pedrosa
Sergio Contreras Hantke
Nelson Padilla
Observatorio Astronómico de Córdoba
UNAB
PUC
Universidad de Chile
Universidad Andrés Bello
Universidad Andrés Bello
UNAB
P. Universidad Católica de Chile
UNAB
Universidad de Concepción
UNAB - MAS
UNAB - MAS
IAG - USP
IAFE (UBA/CONICET), Argentina
IATE
Instituto de Física y Astronomía, Universidad de Valparaíso
Valparaiso University
Brazilian Center for Physics Research
PUC
AIUC
UNAB CATA MAS VO
Universidad de Valparaiso
UNAB
IAFE (CONICET-UBA)
IAG - USP
UNAB
IAFE
Universidad Católica de Chile
PUC
Venue
Universidad Andrés Bello
Campus Casona Las Condes
Auditorio C6
Fernandez Concha 700, Las Condes.
Santiago, Chile
How to get to Campus La Casona by public transport:
- Metro 1 (Estacion Manquehue) + bus C01c
- Metro 1 (Estacion Los Dominicos) + bus C09
From Av. Las Condes (the Mall Sport at the corner of Fernandez Concha) you have to walk 2 blocks to the entrance.
Webpage
Contact Number
Cellphone Number
