The GMRT EoR experiment: limits on polarized sky brightness at 150 MHz (2009)
Pen, Ue-Li, Chang, Tzu-Ching, Hirata, Christopher M., Peterson, Jeffrey B., Roy, Jayanta, Gupta, Yashwant, ...
The Giant Metrewave Radio Telescope (GMRT) reionization effort aims to map out the large-scale structure of the Universe during the epoch of reionization (EoR). Removal of polarized Galactic emission...
A real-time software backend for the GMRT (2009)
Roy, Jayanta, Gupta, Yashwant, Pen, Ue-Li, Peterson, Jeffrey B., Kudale, Sanjay, Kodilkar, Jitendra
The new era of software signal processing has had a large impact on radio astronomy instrumentation. Our design and implementation of a 32 antennae, 33 MHz, dual polarization, fully real-time...
21 cm Intensity Mapping (2009)
Peterson, Jeffrey B., Aleksan, Roy, Ansari, Reza, Bandura, Kevin, Bond, Dick, Bunton, John, ...
Using the 21 cm line, observed all-sky and across the redshift range from 0 to 5, the large scale structure of the Universe can be mapped in three dimensions. This can be accomplished by studying...
The Yuan-Tseh Lee Array for Microwave Background (2009)
Pablo Altamirano, Chia-hao Chang, Shu-hao Chang, Su-wei Chang, Chung-cheng Chen, ...
The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the first interferometer dedicated to studying the cosmic microwave background (CMB) radiation at 3mm wavelength. The choice of...
The Yuan-Tseh Lee Array for Microwave Background Anisotropy (2008)
Ho, Paul T. P., Altamirano, Pablo, Chang, Chia-Hao, Chang, Shu-Hao, Chang, Su-Wei, Chen, Chung-Cheng, ...
The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the first interferometer dedicated to studying the cosmic microwave background (CMB) radiation at 3mm wavelength. The choice of...
The GMRT EoR Experiment: Limits on Polarized Sky Brightness at 150 MHz (2008)
Pen, Ue-Li, Chang, Tzu-Ching, Peterson, Jeffrey B., Roy, Jayanta, Gupta, Yashwant, Hirata, Christopher M., ...
The GMRT reionization effort aims to map out the large scale structure of the Universe during the epoch of reionization (EoR). Removal of polarized Galactic emission is a difficult part of any 21 cm...
Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy (2007)
Chang, Tzu-Ching, Pen, Ue-Li, Peterson, Jeffrey B., McDonald, Patrick
The expansion of the universe appears to be accelerating, and the mysterious anti-gravity agent of this acceleration has been called ``dark energy''. To measure the dynamics of dark energy, Baryon...
Paolo G. Calisse, Michael G. Burton, Michael A. Phillips, ...
Abstract: We have developed a 350 µm radiometer to perform automated site testing in remote regions of Antarctica. In summer 2000–2001 the instrument operated at Concordia, a new station under...
Plans for a 10-m Submillimeter-wave Telescope at the South Pole (1998)
Stark, Antony A., Carlstrom, John E., Israel, Frank P., Menten, Karl M., Peterson, Jeffrey B., Phillips, T. G., ...
A 10 meter diameter submillimeter-wave telescope has been proposed for the NSF Amundsen-Scott South Pole Station. Current evidence indicates that the South Pole is the best submillimeter-wave...
The spectrum of the cosmic background radiation from 2.3 cm⁻¹ to 11.0 cm⁻¹ / (1985)
Thesis (Ph. D.)--University of California, Berkeley, 1985.
The spectrum of the cosmic background radiation from 2.3cm±¹ to 11.0cm±¹ / (1985)
Thesis (Ph. D. in Physics)--University of California, Berkeley, May 1985.