Monday 3rd and Tuesday 4th: You can register from 8:30 to 9:00 am in the hall of the Conference Room.
Monday 3rd: Opening from 9:00 to 9:20.
Final program:


Time Monday 3 Tuesday 4 Wednesday 5 Thursday 6 Friday 7
09:00
to
09:20
Opening
Radostin Kurtev
VVV astrometry, proper motions and parallaxes

Alvaro Alvarez-Candal
What we (don't) know about the trans-Neptunian objects

Michael Balogh
Satellite galaxies and the baryon cycle

Yan-Chuan Cai
Cosmology with Cosmic Voids
09:20
to
10:00

Stefan Gottlöber
From Large Volumes to Near Field Cosmology
10:00
to
10:20

Virginia Cúneo
30 years of optical spectroscopy from the symbiotic binary PU Vulpeculae

Cristian Giuppone
Kozai resonance in coorbital planets

Maria Argudo-Fernández
Spatially resolved SFH of isolated spiral galaxies

Carlos Correa
Determining cosmological parameters with cosmic voids
10:20
to
10:40

Cecilia Scannapieco
The formation of disk galaxies in computer simulations

Karla Peña Ramírez
Low mass stellar and substellar population in young star forming regions: the Sigma Orionis case

Alejandro Esquivel
Modeling the interaction of an exoplanet and its host star: the case of HD 209458b

Graeme Candlish
Tidal effects in galaxy clusters

Laura Ceccarelli
The motion of emptiness: Dynamics of cosmic voids
10:40
to
11:00

Horacio Dottori
The History of Star Formation in the Barred Galaxy NGC 7020

Heliana Luparello
Voids and Superstructures: correlations and induced large–scale velocity flows
11:00
to
11:30
Coffee Break Coffee Break Coffee Break Coffee Break Coffee Break
11:30
to
12:10

Sebastián Nuza
Gas accretion onto MW-like galaxies and the Local Group

Jura Borissova
Star clusters in the VVV survey

Adrián Rovero
What VHE gamma-ray astronomy can do about the IGMF

Sofía Cora
Catalogs of simulated galaxies: MultiDark Galaxies

Yolanda Jiménez Teja
CHEF bases for astronomical data analysis
12:10
to
12:30

Ismael Ferrero
Abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE

Tali Palma
Two New VVV Discoveries: A Dwarf Galaxy and a Globular Cluster

Federico Stasyszyn
Faraday Rotation Measures dependence with galaxy clusters dynamics

Martín de los Rios
Measuring the cosmological parameters spatial distribution
Maria Chira
Environmental Dependence of Dark Matter Halo Abundances
12:30
to
12:50

Gian Luigi Granato
On dust obscured simulations

Sebastián Ramírez Alegría
Near-infrared eyes to observe obscured and massive young stellar clusters

Bruno Sánchez
Bogus/Real implementation on new Image Subtraction algorithm

Poster
Session IV

Manolis Plionis
Using HII galaxies as a tracer of the high-z Hubble expansion
12:50
to
13:10

Poster
Session III
13:10
to
14:30
Lunch Lunch Lunch Lunch Lunch
14:30
to
15:10

Gustavo Yepes
The MUSIC of galaxy clusters

Javier Alonso García
The inner Galactic globular clusters

Ariel Rossanigo
My scientific python toolbox

Gastão Lima Neto
Galaxy cluster collisions
15:10
to
15:30

Diego Pallero
Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation

Andrea Ahumada
Integrated spectroscopy of 16 Large Magellanic Cloud stellar clusters

Juan Pedro Fisanotti
Current ecosystem for ANNs in Python

Elizabeth Gonzalez
Weak lensing mass determinations
15:30
to
15:50

Poster
Session I

Martin Chalela
A weak lensing analysis of Compact Groups
15:50
to
16:20
Coffee Break Coffee Break Excursion to
Alta Gracia
and
Estación Astrofísica
de Bosque Alegre
Coffee Break Coffee Break
16:20
to
17:00

Yara Jaffé
The impact of ram-pressure stripping in cluster and group galaxies

Marcelo Arnal
LLAMA: A new "road" for astronomical observing research

Nicolás Wolowick & Antonio Russo
How and why do we have to exploit a CPU/GPU?

Martín Makler
Gravitational arcs as cosmological and astrophysical probes: the case of Stripe 82
17:00
to
17:20

Nelson Padilla
Asymmetric star formation efficiency due to ram pressure stripping

Francesco Di Mille
Las Campanas Observatory: past, present and future

Gastón Avila
Git for scientists, an introduction

Ezequiel Boero
Gravitational lensing and exact geometrical models for astrophysical systems in the cosmological contexts
17:20
to
17:40
Closing Session
17:40
to
18:00

Poster
Session II


Posters Session

Posters shall be portrait shaped: width = 0.80 m MAX, height = 1.20 m MAX.

Poster Session I


Poster Session II

Poster Session III

Poster Session IV