La Serena, Chile, March 17 - 18, 2016
Easter Island, Chile, August 9 - 13, 2016
Supernova science has entered a golden age with daily announcements of new discoveries. This rate of discovery is only going to increase as we move to an era of large-scale non-targeted surveys, which will culminate with the LSST. In order to take advantage of this deluge of observations the community needs to evaluate the efficiency and effectiveness of data analysis techniques to ensure that optimal science is achieved. As supernova sample sizes continue to drastically increase, well-observed nearby events will still provide the most direct insights into progenitor properties and explosion mechanisms. Here, the challenge is to obtain multi-wavelength observations at epochs as early as possible post-explosion, where crucial constraints on physics are at their most powerful.
Santiago, Chile, May 16 - 20, 2016
Results from ALMA Long Baseline observations and from SPHERE, GPI and other high-contrast AO instruments have given a taste of what to expect over the next few years in the fields of protoplanetary and debris disks, and planet formation. For the first time, these instruments are enabling us to observe the regions where planets form. Already we are finding gaps, holes, spiral wave patterns, and extreme asymmetries in the disks.
22nd Los Alamos Stellar Pulsation Conference Series Meeting
San Pedro de Atacama, Chile, Nov. 28 - Dec. 2, 2016
Astronomy is undergoing a major revolution in the way it approaches its core subject. With the increase in detector efficiency and size and the availability of ever more powerful computers, wide-field surveys, once few in number, have become increasingly common – and indeed, it is clear that the field will be largely dominated by massive wide-field surveys, photometric and spectroscopic alike, in the not-too-distant future.
At this special transition moment between “classical” and survey-based astronomy, we are faced with important challenges on how to properly handle, process and analyze the increasingly large datasets that are continuously amassed by these surveys. Astronomers must increasingly work together with computer scientists and statisticians. Entirely new fields, such as the booming but fairly young field of Astrostatistics, are emerging in the process.
Astronomy & Astrophysics, EDP Sciences and Sociedad Chilena de Astronomia (SOCHIAS) are glad to announce the registration open for the
4th Scientific Writing for Young Astronomers,
which will be held in Puerto Varas, Chile, from 19th to 22th April, 2016.
The beginning of operations of the Large Synoptic Survey Telescope (LSST), scheduled for ~2020, is approaching very fast. The main motivation for this workshop is to address how prepared are we, as Chilean community, for the avalanche of LSST data and more importantly what research we hope to do with these data. With this in mind, we are organizing a two-days meeting in which members of the Chilean community can present and discuss their ideas to make the best use of the LSST data and multi wavelength follow-up studies, ranging from solar system and planetary science to high redshift galaxies and cosmology.