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The Astrophysical Multimessenger Observatory Network (AMON) aims to virtually connect the world's leading high-energy and multimessenger observatories. AMON's objective are to evoke the discovery of new multimessenger phenomena, exploit these phenomena as tools for fundamental physics and astrophysics, and explore archival datasets in search of multimessenger activity. I'll summarize some of the main results from AMON including recent ones from the Neutrino-Electromagnetic (NuEM) channel. I'll also talk about the future projects for AMON.
I'm an Assitant Research Professor working on Astrophysics at the Pennsylvania State University under my advisors Dr. Doug Cowen and Dr. Miguel Mostafa.
I'm involved in several projects related to high-energy astrophysics. I study high-energy gamma rays with the HAWC Observatory, located in Mexico.
The second project I'm involved with is a multimessenger framework called AMON, which looks for coincidences of events obtained by different detectors or observatories. This is a pioneer project in the search of multimessenger sources.
I earned my PhD at Michigan Technological University. My thesis was about observations of high-energy gamma-rays from the Northern Fermi Bubble Region with the HAWC Observatory, advised by Dr. Petra Huentemeyer.