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Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
G. Hinshaw, D. Larson, E. Komatsu +18
We present cosmological parameter constraints based on the final nine-year WMAP data, in conjunction with additional cosmological data sets. The WMAP data alone, and in combination…
Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
C. L. Bennett, D. Larson, J. L. Weiland +18
We present the final nine-year maps and basic results from the WMAP mission. We provide new nine-year full sky temperature maps that were processed to reduce the asymmetry of the e…
The Cosmology Large Angular Scale Surveyor (CLASS): 40 GHz optical design
Joseph R. Eimer, Charles L. Bennett, David T. Chuss +3
The Cosmology Large Angular Scale Surveyor (CLASS) instrument will measure the polarization of the cosmic microwave background at 40, 90, and 150 GHz from Cerro Toco in the Atacama…
Detectors and cryostat design for the SuMIRe Prime Focus Spectrograph (PFS)
James E. Gunn, Michael Carr, Stephen A. Smee +20
We describe the conceptual design of the camera cryostats, detectors, and detector readout electronics for the SuMIRe Prime Focus Spectrograph (PFS) being developed for the Subaru…
The metrology cameras for Subaru PFS and FMOS
Shiang-Yu Wang, Yen-Shan Hu, Chi-Hung Yan +11
The Prime Focus Spectrograph (PFS) is a new multi-fiber spectrograph on Subaru telescope. PFS will cover around 1.4 degree diameter field with ~2400 fibers. To ensure precise posit…
Prime Focus Spectrograph - Subaru's future -
Hajime Sugai, Hiroshi Karoji, Naruhisa Takato +51
The Prime Focus Spectrograph (PFS) of the Subaru Measurement of Images and Redshifts (SuMIRe) project has been endorsed by Japanese community as one of the main future instruments…