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MKID development for SuperSpec: an on-chip, mm-wave, filter-bank spectrometer
Erik Shirokoff, Peter S. Barry, Charles M. Bradford +16
SuperSpec is an ultra-compact spectrometer-on-a-chip for millimeter and submillimeter wavelength astronomy. Its very small size, wide spectral bandwidth, and highly multiplexed rea…
SuperSpec: design concept and circuit simulations
Attila Kovács, Peter S. Barry, Charles M. Bradford +14
SuperSpec is a pathfinder for future lithographic spectrometer cameras, which promise to energize extra-galactic astrophysics at (sub)millimeter wavelengths: delivering 200--500 km…
Multi-chroic dual-polarization bolometric detectors for studies of the Cosmic Microwave Background
Aritoki Suzuki, Kam Arnold, Jennifer Edwards +12
We are developing multi-chroic antenna-coupled TES detectors for CMB polarimetry. Multi-chroic detectors increase the mapping speed per focal plane area and provide greater discrim…
Antenna-coupled TES bolometers for the Keck Array, Spider, and Polar-1
R. O'Brient, P. A. R. Ade, Z. Ahmed +50
Between the BICEP2 and Keck Array experiments, we have deployed over 1500 dual polarized antenna coupled bolometers to map the Cosmic Microwave Background's polarization. We have b…
Optimization and sensitivity of the Keck Array
S. Kernasovskiy, P. A. R. Ade, R. W. Aikin +41
The Keck Array (SPUD) began observing the cosmic microwave background's polarization in the winter of 2011 at the South Pole. The Keck Array follows the success of the predecessor…
Optical Characterization of the Keck Array Polarimeter at the South Pole
A. G. Vieregg, P. A. R. Ade, R. Aikin +37
The Keck Array (SPUD) is a set of microwave polarimeters that observes from the South Pole at degree angular scales in search of a signature of Inflation imprinted as B-mode polari…