The meeting is aimed to i) foster close interactions between researchers working on individual pulsar timing array (PTA) experiments ii) provide detailed hands-on training for young researchers on the nuances of gravitational wave data analysis and ii) to develop links with the wider gravitational wave community. A status update from the established PTAs and the emerging PTAs will be presented along with detailed discussions on various data sharing and data combination issues relevant for the IPTA consortium. During the first week (the "student week"), experts in the field will share their knowledge and organize hands-on exercises to explore the data-sets and data challenges. During the second week, the active researchers in the field will help to advance the frontiers of our understanding through presentations and discussions on the road ahead that include various challenges and strategies. Apart from invited and contributed talks, updates from IPTA working groups and panel discussion on policy issues regarding the sharing of data and resources are included in the science program. A one day visit to upgraded GMRT is part of the program.
The program targets the advanced students, PhD students and young researchers specializing in theoretical astrophysics. The purpose of the School is to provide modern physical basis in major topics in theory of galaxy formation and evolution and in theory of core-collapse supernovae and stellar explosions. The school will take place at the «SIRIUS” Education Centre (Sochi). 45 minutes drive time from Sochi International Airport.
With this meeting we aim to foster a discussion between the scientists who have been studying galaxies and cosmology in the dark matter and Milgromian frameworks which constitute two fundamentally different hypotheses. The aim is to achieve an exchange notably also on the technical challenges in applying both hypothesis to computational astrophysics problems in view of recent advances in understanding stellar populations, which are important for quantifying feedback processes.
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