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Hot-wiring the Transient Universe III

Hot-wiring the Transient Universe 3 will explore opportunities and challenges of massively parallel time domain surveys coupled with rapid coordinated multi-wavelength follow-up observations. The interdisciplinary agenda includes future and ongoing science investigations, information infrastructure for publishing observations in real time, as well as novel data science to classify events and systems to optimize follow-up campaigns. Time domain astronomy is at the fore of modern astrophysics and crosses fields from solar physics and solar system objects, through stellar variability, to explosive phenomena at galactic and cosmological distances. Recent rapid progress by instruments in space and on the ground has been toward a continuous record of the electromagnetic sky with ever increasing coverage, sensitivity, and temporal resolution. With the advent of gravitational wave and neutrino observatories we are witnessing the birth of multi-messenger astronomy.
When 13 November 2013 08:55 AM to
15 November 2013 06:55 PM
Where Santa Fe NM USA
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Organizing Committee:

Przemek Wozniak, Los Alamos National Laboratory
Tom Vestrand, Los Alamos National Laboratory
Josh Bloom, University of California, Berkeley
Matthew Graham, California Institute of Technology
Lynne Jones, University of Washington
Mansi Kasliwal, Carnegie Observatories
Ashish Mahabal, California Institute of Technology
Tom Matheson, National Optical Astronomy Observatory
Andrej Prsa, Villanova University
Rob Seaman, National Optical Astronomy Observatory
Rachel Street, Las Cumbres Observatory Global Telescope Network
John Swinbank, Low-Frequency Array for Radio Astronomy
Lucianne Walkowicz, Princeton University
Roy Williams, Laser Interferometer Gravitational Wave Observatory

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