13:20  J3-1  WHAT WILL THE NEXT GENERATION OF 21 CM EXPERIMENTS TEACH US ABOUT THE EPOCH OF REIONIZATION?

Jonathan C. Pober*¹, Joshua S. Dillon², Adrian Liu³

¹Department of Physics, University of Washington, Seattle, WA
²Department of Physics, Massachusetts Institute of Technology, Boston, MA
³Department of Astronomy, University of California Berkeley, Berkeley, CA

13:40  J3-2  HOW THE UW IMAGING PIPELINE PREPARES 350 HOURS OF MWA OBSERVATIONS FOR EOR POWER SPECTRUM MEASUREMENTS

Adam P. Beardsley*, Ian S. Sullivan, Bryna J. Hazelton, Miguel F. Morales

Department of Physics, University of Washington, Seattle, WA

14:00  J3-3  UW EOR POWER SPECTRUM PIPELINE

Bryna J. Hazelton*, Miguel F. Morales, Adam P. Beardsley, Ian S. Sullivan

Physics, University of Washington, Seattle

14:20  J3-4  APPLICATIONS OF FAST 21 CM POWER SPECTRUM ESTIMATION

Joshua S. Dillon*

Department of Physics, Massachusetts Institute of Technology, Cambridge, MA

14:40  J3-5  SHEDDING LIGHT ON FOREGROUNDS WITH NEW MWA AND PAPER DATA

Daniel Jacobs*, Judd Bowman

Arizona State University, Tempe

15:20  J3-6  RESULTS FROM THE GREEN BANK TELESCOPE 21 CM INTENSITY SURVEY

Eric R. Switzer*

NASA Goddard, Greenbelt MD

15:40  J3-7  ANALYSING TRANSIT TELESCOPES WITH THE M-MODE FORMALISM

Richard Shaw*¹, Kris Sigurdson², Ue-Li Pen¹, Albert Stebbins³, Michael Sitwell²

¹Canadian Institute for Theoretical Astrophysics, Toronto, ON, CANADA
²Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, CANADA
³Theoretical Astrophysics Group, Fermi National Accelerator Laboratory, Batavia, IL

16:00  J3-8  CHARTING MOLECULAR GAS THROUGH COSMOLOGICAL TIME: PRESENT RESULTS AND FUTURE DIRECTIONS

Garrett K. Keating*¹, Geoffrey C. Bower¹, David R. DeBoer¹, Daniel Marrone²

¹Dept. of Astronomy, University of California, Berkeley, Berkeley, CA
²Dept. of Astronomy, University of Arizona, Tuscon, AZ

16:20  J3-9  PROBABILISTIC IMAGE RECONSTRUCTION FOR RADIO INTERFEROMETERS

Paul M. Sutter*, Benjamin D. Wandelt

Paris Institute of Astrophysics, Paris, FRANCE

16:40  J3-10  SPT-3G: A NEXT-GENERATION COSMIC MICROWAVE BACKGROUND POLARIZATION EXPERIMENT ON THE SOUTH POLE TELESCOPE

Jason E. Austermann*¹, for the SPT Collaboration²

¹Center for Astrophysics and Space Astronomy, Boulder
²Kavli Institute for Cosmological Physics, University of Chicago, Chicago

17:00  J3-11  Redundant and Non-Imaging Calibration of the Precision Array for Probing the Epoch of Reionization (PAPER)

James E. Aguirre*¹, Aaron R. Parsons², Rich F. Bradley³, Christopher L. Carilli⁴, David R. DeBoer⁵, Zaki S. Ali², Adrian Liu², Daniel C. Jacobs⁶, David F. Moore¹, Jonathan C. Pober⁷, Irina I. Stefan⁸

¹University of Pennsylvania, Philadelphia, PA
²University of California, Berkeley, Berkeley, CA
³National Radio Astronomy Observatory, Charlottesville, VA
⁴National Radio Astronomy Observatory, Socorro, NM
⁵Radio Astronomy Laboratory, Berkeley, CA
⁶Arizona State University, Tempe, AZ
⁷University of Washington, Seattle, WA
⁸Cavendish Laboratory, Cambridge, UNITED KINGDOM

17:20  J3-12  HOW DO POLARIZED FOREGROUNDS AFFECT 21 CM EOR POWER SPECTRUM DETECTION?

David F. Moore*¹, James E. Aguirre¹, Aaron R. Parsons², Richard F. Bradley³, Christopher L. Carilli⁴, David R. DeBoer⁵, Zaki S. Ali², Adrian Liu², Daniel C. Jacobs⁶, Jonathan C. Pober⁷, Irina I. Stefan⁸

¹Department of Physics, University of Pennsylvania, Philadelphia, PA
²Department of Astronomy, Univesity of California, Berkeley, Berkeley, CA
³National Radio Astronomy Observatory, Charlottesville, VA
⁴National Radio Astronomy Observatory, Socorro, NM
⁵Radio Astronomy Laboratory, Berkeley, CA
⁶School of Earth and Space Exploration, Arizona State University, TEMPE, AZ
⁷Department of Physics, University of Washington, Seattle, WA
⁸Cavendish Lab, Cambridge, UNITED KINGDOM