Man

Matias Ambrosio Vidal Navarro

Profesor Investigador

Universidad Autónoma de Chile

Santiago, Chile

Líneas de Investigación


Interstellar Medium; CMB foregrounds; Radio emission, Astrochemistry

Educación

  •  Licenciatura en Ciencias, Mencion Astronomia, UNIVERSIDAD DE CHILE. Chile, 2007
  •  Magister en Astronomia, UNIVERSIDAD DE CHILE. Chile, 2009
  •  Ph.D Astrophysics, THE UNIVERSITY OF MANCHESTER. Reino Unido, 2014

Experiencia Académica

  •   Research Associate (Postdoc) Full Time

    THE UNIVERSITY OF MANCHESTER

    Manchester, Reino Unido

    2014 - 2015

  •   Profesor Investigador Full Time

    UNIVERSIDAD AUTONOMA DE CHILE

    Ingenieria

    santiago, Chile

    2020 - A la fecha

Experiencia Profesional

  •   Research Associate

    University of Manchester

    Reino Unido

    2014 - A la fecha

  •   Investigador Postdoctoral Full Time

    Universidad de Chile

    Santiago, Chile

    2016 - A la fecha

Premios y Distinciones

  •   FONDECYT Postdoctoral Grant.

    FONDECYT

    Chile, 2016

    FONDECYT 2016 Postdoctoral Grant.


 

Article (14)

Cm-wavelength observations of MWC758=> resolved dust trapping in a vortex and intra-cavity signal
The State-of-Play of Anomalous Microwave Emission (AME) research
A new polarization amplitude bias reduction method
Planck 2015 results I. Overview of products and scientific results
Planck 2015 results XXV. Diffuse low-frequency Galactic foregrounds
Polarized radio filaments outside the Galactic plane
THE Q/U IMAGING EXPERIMENT=> POLARIZATION MEASUREMENTS OF THE GALACTIC PLANE AT 43 AND 95 GHz
Studies of Anomalous Microwave Emission (AME) with the SKA
Dust-correlated centimetre-wave radiation from the M78 reflection nebula
Dust-correlated cm wavelength continuum emission from translucent clouds zeta Oph and LDN 1780
New constraints on the polarization of anomalous microwave emission in nearby molecular clouds
New constraints on the polarization of anomalous microwave emission in nearby molecular clouds
Galaxy clusters in the line of sight to background quasars. I. Survey design and incidence of MgII absorbers at cluster redshifts
Galaxy clusters in the line of sight to background quasars. I. Survey design and incidence of MgII absorbers at cluster redshifts

BookWhole (1)

Diffuse Radio Foregrounds

Proyecto (4)

RADIO/SUBMM CONTINUUM EMISSION FROM THE ISM
A STUDY OF CORE-COLLAPSE SUPERNOVAE IN THE LOCAL UNIVERSE.
QUASAR ABSORPTION LINE SYSTEMS AS A PROBE OF HIGH-REDSHIFT GALAXIES.
STARDUST AND THE STRUCTURE OF THE INTERSTELLAR MEDIUM.
6
Matias Vidal

Profesor Investigador

Universidad Autónoma de Chile

Santiago, Chile

1
Simon Casassus

Profesor Titular

Astronomía

DEPARTAMENTO DE ASTRONOMÍA, UNIVERSIDAD DE CHILE

Santiago, Chile