J1.1
Re-channelizing Quantized Polyphase Filter Banks
Stephen Fay, McGill University, Canada
Session:
J1: New Telescopes, Techniques, and Technologies I Lecture
Track:
Commission J: Radio Astronomy
Location:
Room 265
Presentation Time:
Thu, 9 Jan, 08:20 - 08:40 MT (UTC -7)
Session Chair:
Alyson Ford, University of Arizona
Presentation
Discussion
Resources
No resources available.
Session J1
J1.1: Re-channelizing Quantized Polyphase Filter Banks
Stephen Fay, McGill University, Canada
J1.2: Evidence for uncorrected gain factors in Galactic synchrotron template maps
Michael Wilensky, McGill University, Canada; Melis Irfan, University of Cambridge, United Kingdom; Philip Bull, University of Manchester, United Kingdom
J1.3: Cyclic Spectroscopy in Present and Upcoming Radio Telescope Data
Timothy Dolch, Hillsdale College, United States
J1.4: A 400Gbit Ethernet core enabling High Data Rate Streaming from FPGAs to Servers and GPUs in Radio Astronomy
Wei Liu, University of California Berkeley, United States; Mitchell C. Burnett, Brigham Young University, United States; Dan Werthimer, Jonathon Kocz, University of California Berkeley, United States
J1.5: Pulsar Detection Performance using Oversampled Spectrometer: Preliminary Indications
Rebecca Haymore, Mitchell Burnett, Brian Jeffs, Karl Warnick, Brigham Young University, United States
J1.6: High-dynamic Range Radio Astronomy Systems, Interference Mitigation strategies, and a Test Setup for Experimenting Dynamic Spectrum Sharing
Emilio Armas, Connor Westcott, William Dellinger, Nehal Patel, D. Anish Roshi, University of Central Florida, United States; Mitch Burnett, Brigham Young University, United States; Wei Liu, University of California Berkely, United States; Dan Werthimer, University of California Berkeley, United States; Rafael A. Rodríguez-Solís, University of Puerto Rico, United States
J1.7: An Experimental Test-bed for Investigating Spectrum Sharing Strategies Between Passive and Active Users at a Prototype National Radio Dynamic Zone (NRDZ)
Arvind Aradhya, University of Colorado, Boulder, United States; David DeBoer, University of California, Berkeley, United States; Oren Collaco, University of Colorado, Boulder, United States; Wael Farah, SETI Institute, United States; Cole Forrester, University of California, Berkeley, United States; Kevin Gifford, University of Colorado, Boulder, United States; David Johnson, University of Utah, United States; Sylvia Llosa, University of Colorado, Boulder, United States; Alexander Pollak, SETI Institute, United States; Bo Pearce, University of Colorado, Boulder, United States; Mark Ruzindana, University of California, Berkeley, United States; Aarushi Sarbhai, University of Utah, United States; Brockton Stover, University of California, Berkeley, United States; Stefan Tschimben, University of Colorado, Boulder, United States; Jacobus Van der Merwe, Kirk Webb, University of Utah, United States; Georgiana Weihe, University of Colorado, Boulder, United States
J1.8: Detecting VHF satellite emissions using the Orville Wideband Imager
Nicholas Rainville, Scott Palo, University of Colorado Boulder, United States; Gergory Taylor, Jayce Dowell, University of New Mexico, United States
J1.9: Using Meter-Wavelength Lunar Polarimetry to Determine the Accuracy of Estimates of the Ionospheric Faraday Rotation Measure
Richard Perley, Bryan Butler, Lilia Tremou, Eric Greisen, National Radio Astronomy Observatory, United States; Tony Willis, Dominion Radio Astrophysical Observatory, Canada
J1.10: Precision Data Analysis for 21 cm Cosmology with the OVRO-LWA Stage III
Ruby Byrne, Gregg Hallinan, Caltech, United States
Contacts