The organizers seek out up to a few select scientists to be primary lecturers at the school and also participate in content development. A series of secondary lecturers will also be invited, and the diversity of speakers are emphasized. Hands-on sessions will include theory, computation, and data analysis. Students will leave the school having replicated some of the analysis that went into recent discoveries of gravitational waves, interpreted observational data from stellar clusters, and ran a simple computer simulation of star formation. A visit and half-day mini-workshop at the TIFR National Balloon Facility, Hyderabad, where we will do some demonstration of scientific ballooning for astronomical observations along with two day exhaustive workshop on computational astrophysics and data mining.
ISVHECRI is a biennial conference series supported by the International Union of Pure and Applied Physics (IUPAP). Its primary objective is to provide a forum for the discussion of very high energy interaction for the interpretation of cosmic ray data based on the information available from both the accelerator and cosmic ray experiments. This unique series brings together cosmic ray physicists and scientists involved with the high energy accelerators and colliding beam facilities. The scope of the conference has been widened to include interesting and new measurements from related areas of astro-particle physics.
Theoretical investigations are verified experimentally through the timing and spectral properties of the observed sources. In the last years, the observational context has been enormously enhanced due to discovery of gravitational waves, which give independent constraints on the masses (and possibly spins) of the merging compact stars. The multi-wavelength detection of accompanying events of the short GRBs, such as the kilonovae, have brought further important information about the conditions within the post-merger environment. Finally, the fundamental theories of gravity can be tested now with unprecedented precision through the signals from compact objects, such as quasars, supernovae, and gravitational-wave sources.
The goal of the conference is to share the different views from different research communities by balancing contributions from different categories and to encourage collaborations between researchers across the Globe. Ample time is set aside to encourage discussions and collaboration. The meeting consists of invited reviews, invited talks, contributed talks, and posters. The conference also aims at fostering close collaboration via smaller size focus group discussion and excursion. There is also a bootcamp training school prior to the conference for local students.
The IPA2020 conference will bring together experimentalists and theorists to discuss the topics mentioned above with an emphasis on exchange between the different but correlated fields.
In this sense, we would foster inclusiveness in the advancement of astronomy and facilitate the advancement of the next generation of astronomers and scientists, through encouragement of the use of new methods of learning and best practices (including distance education: Moocs) in pedagogy at university level, as well as the use of astronomy for teaching and education at school level, which are part of the definitions of the proposed Office of Astronomy for Education (OAE), which also pursuits the establishment of a Network of Astronomy Education Contacts (NAECs) to provide accessible materials and astronomy literacy guidelines globally. The invited speakers are international leaders in discipline-based education in astronomy and the planetary science, but also in communication, history, inclusion and protection of world’s heritage, including the dark sky.
As with most other sciences, astronomy is being fundamentally transformed by the Information and Computation Technology (ICT) revolution. The data volume is growing exponentially, can be accessed remotely and the observations can be performed even without a real knowledge of a telescope. The new approaches to the data permits the development of new tools, techniques and resources for data analysis and produce discoveries which probably never would be reached with traditional astronomy data analysis period.
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!
Dernière mise à jour: 22 Janvier 2020