Conference-Service.com met à la disposition de ses visiteurs des listes de conférences et réunions dans le domaine scientifique. Ces listes sont publiées pour le bénéfice des personnes qui cherchent une conférence, mais aussi, bien sûr, pour celui des organisateurs. Noter que, malgré tout le soin que nous apportons à la vérification des données entrées dans nos listes, nous ne pouvons accepter de responsabilité en ce qui concerne leur exactitude ou étendue. Pensez donc à vérifier les informations présentées avec les organisateurs de la conférence ou de la réunion avant de vous engager à y participer!
Les organisateurs peuvent soumettre une réunion ou une conférence pour inclusion dans nos listes, et ceci gratuitement.
astrochemistry. Additionally, during the symposium, we will have two hands-on workshops: One focused in experimental astrochemistry and other focused on observations. The hands-on workshops will have activities on the proposal submissions to the LNLS (Brazilian Synchrotron Light Laboratory) laboratory, data reduction and to LLAMA (Large Latin American Millimeter Array) and ALMA (Atacama Large Millimeter Array) radio observatories. During this meeting we will also have an opportunity to follow a real astrochemical experiment (in real time) at one of the beamlines of the LNLS that simulates the interaction between UV and soft X-rays with
astrophysical ice analogs.
In recent years there has been significant improvement in our knowledge of both the distribution of galaxies through comprehensive redshift surveys and the deviant motions of galaxies through measurements of distances. These observational advances have stimulated interest in methods of interpretation. The constraints on the distribution of matter and cosmological parameters are becoming increasingly precise. Yet major questions remain.
The conference will consist of plenary sessions for in depth oral presentations (review talks and specialized talks on specific topics) and posters. The contributions are either solicited or selected among submitted abstracts. The program will be available after the deadline of abstracts submission (March 3rd, 2016).
Students will be given the opportunity to present their own research work by bringing a poster to the School. The School provides an opportunity for the young researchers to network with fellow students and lecturers, thereby promoting awareness of areas outside the main specialization of the student, and potential cross-fertilization of techniques and concepts.
The School covers two scientific topics that share many synergies and resources: Asteroseismology and Exoplanets. Therefore, the program aims at building opportunities for cooperation and sharing of methods that will benefit both communities. This cooperation has experienced great success in the context of past space missions such as CoRoT and Kepler. Upcoming photometry and astrometry from space, as well as complementary data from ground-based networks, will continue to foster this cooperation. Observations of bright stars and clusters in the ecliptic plane are being made by the repurposed K2 mission, and NASA's TESS and ESA's CHEOPS missions will soon start obtaining similar data over the entire sky. ESA's PLATO mission will then build upon these successes by providing photometric light curves on a wealth of stars. Ground-based spectroscopy from the Stellar Observations Network Group (SONG) will complement the satellite data for the brightest stars in the sky, as will also be the case with the new generation of high-precision spectrographs being developed for the ESO, like the Echelle SPectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO).
UC Santa Barbara. Though extensive hands-on labs, participants will gain familiarity with MESA and learn how to make better use of MESA in their own work. Featured science topics include gravity-mode oscillations of massive stars (Connie Aerts), transport by waves (Jim Fuller), pulsations (Alfred Gautschy),
massive stars (Norbert Langer), and much more.
• Fundamental aspects, structure and spectroscopy
• Collisions with electrons, ions, atoms and molecules
• Interaction with clusters, surfaces and solids
• Interaction with photons and plasmas
• Strong field and ultrafast processes
• Production, experimental developments and applications
The school will look at the principles of inference and methods of astronomical data analysis and data mining. We will cover a range of numerical and statistical techniques and their application to different types of astronomical data.
Building on the latest results from Great Observatories (in orbit and on the ground), we will discuss the nature and evolution of high redshift galaxies, with a particular emphasis on the consistency between the star-formation and the mass assembly processes. We aim at bringing together members of the CANDELS and the GOODS-Herschel collaborations, as well as external scientists interested in the topics, to present their latest results and the perspectives for the next future.
To fully realise the potential of the SKA as a machine for fundamental physics, the SKA organisation seeks to engage the theoretical physics community in the science case and design considerations for the full array. To initiate this discussion, we will be holding a focused workshop in May 2017, in which we aim to bring together radio astronomers and theorists to jointly consider ways in which the SKA can test and explore fundamental physics.
The meeting will place GC systems in the context of their host galaxy and the interplay between them.
Dernière mise à jour: 22 Juin 2016