SPACEU SYMPOSIUM:

PAPIA TANJIA

We detected 3.3 GHz CH transitions tracing CO-dark molecular gas in the Galactic center using the Arecibo 12 m telescope. To overcome RFI, we are developing a 3.3 GHz multi-antenna system with adaptive post-correlation cancellation and GPU-based real-time and offline mitigation.

UCF | Electrical and Computer Engineering

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