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SEMINARIOS Y EVENTOS EN EL DAS

Constantemente se están realizando diversas actividades, seminarios y eventos en nuestro centro astronómico, te invitamos a formar parte de esta gran oportunidad de expandir tus conocimientos de la mano de grandes exponentes, científicos de todo el mundo nos visitan, visitanos tu también.

Listado de Seminarios y Eventos

El horario de los Seminarios esta sujeta a cambios. Por favor revisar regularmente.
Finalizado
27May 2022

Probing chemical evolution of galactic gas reservoirs with quasars

The chemical enrichment of the Universe is a key signature of how stellar populations and galaxies evolved across cosmic time, from quantifying the properties of Population III stars to constraining the strength of feedback processes in galaxies....
Trystyn Berg
ESO-Chile / DAS
Hora: 00:15 hrs.
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Finalizado
13May 2022

La Comisión Chilena de Energía Nuclear: Investigación en un instituto tecnológico público

La Comisión Chilena de Energía Nuclear (CCHEN) es un instituto tecnológico de investigación público creado en 1964 y que mantiene, entre otras facilidades, un reactor nuclear de investigación de 5 MW....
Hora: 12:15 hrs.
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SIN IMAGEN
Finalizado
17Mar 2022

Science with the CCAT-prime Observatory: From Galactic Star Formation to the Edge of the Universe

The CCAT-prime collaboration are currently constructing the Fred Young Submillimeter Telescope (FYST), a wide-field, 6-m aperture telescope to be located sited at more than 5600 meters elevation on Cerro Chajnantor in northern Chile....
Dominik A. Riechers
University of Cologne
Hora: 00:15 hrs.
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SIN IMAGEN
Finalizado
13Ene 2022

Seminario: SDSS-V Chile

The Sloan Digital Sky Survey (SDSS) has been one of the most successful worldwide collaborations in astronomy. In its current fifth stage, SDSS-V will provide multi-epoch optical and IR spectroscopy using facilities in the United States and Chile and...
Ivan Lacerna
Instituto de Astronomía y Ciencias Planetarias, Universidad de Atacama
Hora: 12:15 hrs.
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SIN IMAGEN
Finalizado
02Dic 2021

Exoplanet Demographics: Population Statistics of Hot Super-Earths and Cold Jupiters

Exoplanets are a diverse population reflecting the range in possible outcomes of the planet formation process. Yet there are also patterns in the observed properties of planets and planetary systems that reveal common formation pathways....
Gijs Mulder
Universidad Adolfo Ibañez
Hora: 12:15 hrs.
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SIN IMAGEN
Finalizado
18Nov 2020

Arids 2021: the birth of a meteor shower

Meteor showers are caused by meteoroid released by comets, each entering our atmosphere and creating individual meteors. They are recognized by identifying their radiant (location in the sky where they seem to come from) or directly from their orbit....
Jeremie Vaubaillon
Institut de Mecanique Celeste et de Calcul des Ephemerides, Paris.
Hora: 00:15 hrs.
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SIN IMAGEN
Finalizado
11Nov 2021

PASSAGES: A Multi-J CO and [CI] line study of single dish observations of the lensed Planck selected starbursts at cosmic noon

The peak epoch of cosmic star formation also coincides with the peak in the cosmic co-moving molecular gas mass density, at z ~2. Even with sensitive interferometers, only strongly lensed galaxies offer the feasibility to efficiently and systematical...
Kevin Harrington
APEX and ALMA Fellow at ESO/Chile
Hora: 12:15 hrs.
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SIN IMAGEN
Finalizado
28Oct 2021

The SOFIA Legacy Project FEEDBACK

FEEDBACK is a Stratospheric Observatory for Infrared Astronomy (SOFIA) legacy project using the upGREAT heterodyne receiver to map the [CII] 158μm line in Galactic molecular clouds. It aims to study the interaction of massive stars with their enviro...
Pablo Garcia
Researcher and Project Assistant at the National Astronomical Observatories of China, and Instituto de Astronomía, Universidad Católica del Norte.
Hora: 12:15 hrs.
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SIN IMAGEN
Finalizado
14Oct 2021

The Process of Planning and Implementing SDSS-V projects in the era of robotic Focal Plane System (FPS)

The Sloan Digital Sky Survey has recently reached its fifth generation SDSS-V which consists of the projects Milky Way Mapper (MWM), Black Hole Mapper (BHM), and Local Volume Mapper (LVM). The main difference of this generation is the use of Fiber Po...
Felipe Santana
Departamento de Astronomía, Universidad de de Chile
Hora: 12:15 hrs.
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SIN IMAGEN
Finalizado
07Oct 2021

Planetary remnants around white dwarfs

White dwarfs are the final fate of 95 per cent of all stars, including our Sun. Planets and planetary bodies that survived thismetamorphosis of their host star can venture close to the left-over stellar cores (i.e. white dwarf) where tidal force resu...
Odette Toloza
Núcleo Milenio de Formación Planetaria
Hora: 10:30 hrs.
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