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LSSTAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Prof Ian Kenyon. Recent technological advances have made deep fast optical surveys of large fractions of the sky feasible. LSST is the exemplar. An 8.4m primary mirror with a 10 square degree field of view instrumented by a 3.2 Gigapixel CCD will survey more of the optical universe in one month than all previous telescopes. This will enable astronomical and fundamental physics investigations of the solar system, Milky Way, the transient sky and establish tight constraints on dark energy models. The major features and challenges will be described. This talk is part of the Particle Physics Seminars series. This talk is included in these lists:
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Other listsPIPS - Postgraduate Informal Physics Seminars Condensed Matter Group Meetings Type the title of a new list hereOther talksTBA TBA TBC TBA Ultrafast Spectroscopy and Microscopy as probes of Energy Materials Waveform modelling and the importance of multipole asymmetry in Gravitational Wave astronomy |