Keisuke Osumi

TL;DR: The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrogram, and a novel optical interferometer as discussed by the authors.

TL;DR: In this paper , the authors simplify and refactor the standard TES model to directly relate the detector responsivity calibration and optical time constant to the measured TES current I and the applied bias current I b.

TL;DR: In this article, a demodulation scheme was used to extract the polarization timestreams from the Cosmology Large Angular Scale Surveyor (CLASS) data and applied this method to selected data from the first two years of observations by the 40 GHz CLASS telescope.

TL;DR: The cosmology large angular scale surveyor (CLASS) as mentioned in this paper is a large-scale CMB array that observes the cosmic microwave background (CMB) over 75% of the sky from the Atacama Desert, Chile, at frequency bands centered near 40, 90, 150, and 220 GHz.