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