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Colin Slater6/10/26, 9:00 AM
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Tomas Cabrera (Carnegie Mellon University)6/10/26, 9:25 AM
Gravitational wave follow-up requires iterative observation, analysis, and decision-making on the order of hours in the most extreme of cases. To this extent, it is a subfield where throughput is defined not only by the amount of pertinent data, but rather the speed at which the information in the data can be synthesized into a human-digestible format. In this talk I will present the...
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Alessandra Corsi (John Hopkins University)6/10/26, 9:50 AM
In this talk, I will discuss current and future opportunities in the radio follow-up of gravitational-wave (GW) events using interferometric, PI-driven facilities such as the Karl G. Jansky Very Large Array (VLA) and the future next-generation VLA (ngVLA). I will highlight lessons learned from recent GW observing runs, and strategies for identifying and characterizing relativistic ejecta and...
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Mark Lacy6/10/26, 10:10 AM
The VLA Sky Survey images the whole sky at 2-4GHz in the radio with angular resolution comparable to optical telescopes, providing a unique reference survey for the radio sky. Multi-epoch data allows variable sources and transients to be found and characterized and spectral and polarimetric information is also recorded. Processing the large amount of data from this survey is a significant...
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