[Alumnos-ii-cs] [Nuevo Horario] Coloquio Departamental, Martes 2 de Diciembre 12:30, F106 CC y Sala de Reuniones CSJ

[Claudio Torres L.]

Estimad at s,

(*_Nuevo Horario_*)

Este *Martes 2 de Diciembre a las _*12:30*_* tendremos nuestro *último* 
coloquio departamental del 2014 en la F-106 (La charla se transmitirá en 
videoconferencia a la sala de reuniones, Campus Santiago, San Joaquín). 
En esta ocasión *Amelia Bayo, Ph.D.* nos presentará su trabajo titulado: 
"Studying low-mass stars in the VO and other things!".

*Resumen:* After over ten years of the first implementations, the 
Virtual Observatory is still far too little exploited in the everyday 
work of astronomers. A very important problem is the lack of 
"advertizing" in the non-technical community and the lack of bridges 
between the developers and users of algorithms, protocols, and pieces of 
software. In this talk I will review (in a biased way that allows me to 
go into more details) science cases that have benefited immensely from 
VO-techniques and tools. I will also try to be as critical as possible 
regarding problems that are still not solved in the "VO-world", where 
the interactions with the users/astronomers is vital for a successful 
development.

*Mini Bio:* Graduated with minors in Mathematics, Geodesy and Astronomy 
from Universidad Complutense (Madrid). Master in astrophysics and PhD in 
physics and cosmology from Universidad Autonoma (Madrid, 2009). PhD 
supervised by Dr. Barrado at the Laboratory for Fundamental Physics and 
Astronomy (hosted at the European Space Agency, ESA, campus), with one 
year as Spitzer undergrad fellow at Caltech (Pasadena, California). 
Awarded the European Southern Observatory (ESO) fellowship for three 
years in Chile and the fourth year as visiting researcher at the 
Max-Plank Institut fuer Astronomie (MPIA, Heidelberg, Germany). MPIA 
independent fellow researcher for one year and since August 2014, 
Associate Professor at the Instituto de Astronomia from Universidad de 
Valparaiso.
The lines of research can be separated in "purely astrophysical": 
mechanism of formation of substellar objects and disk evolution through 
the whole stellar mass spectrum, in particular paying attention to the 
dependence on the mass of the central object. And "data-driven": in 
particular the homogeneous analysis of large amounts of multi-wavelength 
data of young stars. In this context, Amelia Bayo is the PI of VOSA 
(Virtual observatory SED analyzer, used in ~60 refereed papers), a 
publicly available software for the compilation and analysis of spectral 
energy distributions of different kinds of objects, merging seamlessly 
public and private data.

¡Quedan todos cordialmente invitados!

Cordiales Saludos,

Comité de Coloquio




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