The Institute of Astronomy plans to host one large summer conference each year. Below is a list of upcoming and previous meetings at the IoA.
We are planning to host up to 150 registered participants and the main focus of the conference will be on theoretical and numerical modelling of physical processes relevant for galaxy formation. The programme is designed to be of scientific interest to non-numericists who want to learn about the scientific issues surrounding galaxy formation and evolution.
We aim to have participants from different scientific communities and extensive discussion of theoretical and numerical challenges will provide a common ground for close interaction.
The Large Synoptic Survey Telescope (LSST) project is at an exciting phase, with first light planned for 2019 and science operations to start in 2021. This major conference will bring together LSST and European scientists to consider the scientific opportunities of LSST, its current status, the role of European expertise and facilities in partnership with LSST, and the science challenges.
ESO has recently released an Instrumentation Roadmap for the E-ELT that foresees a high-resolution spectrograph either as Instrument Nr.4 or Nr.5. The optimal balance of the major science drivers for such an instrument need still to be defined. The aim of the workshop is to (further) define the science cases and science requirements for E-ELT HIRES, by bringing together people interested in the matter. This should be a rather informal meeting of about 50 participants.
Topics to be covered:
Invited speakers will include: Frank Bertoldi, Jamie Bolton, Rychard Bouwens, Joanna Dunkley, Richard Ellis, Steven Furlanetto, Piero Madau, Matthew McQuinn, Masami Ouchi, Dominik Reichers, Michael Shull, Brian Siana, Chris Willott and Saleem Zaroubi.
The Institute of Astronomy, Cambridge, summer conference will focus on Dark Matter, bring together recent progress in astrophysical studies, direct and indirect detection experiemnts, and the LHC.
We invite applications for contributed talks and posters to fill an expanded format for the Darkness Visible meeting to be held at the Institute of Astronomy, Cambridge (UK). This meeting will bring together particle- and astro - physicists (theoretical, experimental and observational) to present recent advances in our understanding of dark matter at scales ranging from particle pysics to cosmology.
The aim of this conference is to bring together an outstanding group of young researchers to discuss theoretical and observational progress toward understanding accretion disc physics in Young Stellar Objects, compact binaries, and galactic nuclei.
Observations of the later evolutionary stages of discs around young stars offer the best opportunity to study planet formation from an observational perspective. Localised clearing of dust and gas in discs can be inferred from a variety of imaging/spectroscopic diagnostics and is often interpreted as evidence for planet formation; alternatively, such clearing results from some other process which needs to be taken into account when assessing the environment in which planets form.
Large-scale starbursts are very common features of early galaxy evolution. At high redshifts, the majority of the present-day "normal" galaxy progenitors either appear to be undergoing violent gravitational interactions, or experience very active star formation throughout.