The Simons Observatory: Design, Integration, and Testing of the Small Aperture Telescopes
The Simons Observatory (SO) is a cosmic microwave background survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5200 m in the Atacama Desert in Chile.
Nicholas Galitzki+81 more
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Observations of the cosmic background radiation at 1440 angstroms
F. Paresco+3 more
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Angular Momentum Transport in Early‐formed Objects by Cosmic Background Radiation: Radiation‐hydrodynamical Approach [PDF]
Tohru Tsuribe, Masayuki Umemura
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Measurement and Modeling of Polarized Atmosphere at the South Pole with SPT-3G
We present the detection and characterization of fluctuations in linearly polarized emission from the atmosphere above the South Pole. These measurements make use of data from the SPT-3G receiver on the South Pole Telescope in three frequency bands ...
A. Coerver+104 more
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A map of the cosmic background radiation at 3 millimeters
P. M. Lubin+3 more
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Excess Ultraviolet Emission at High Galactic Latitudes: A New Horizons View
We present new observations of the cosmic ultraviolet background (CUVB) at high Galactic latitudes (∣ b ∣ > 40 ^∘ ), made using the Alice UV spectrograph on board the New Horizons spacecraft.
Jayant Murthy+13 more
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New measurements of the cosmic background radiation temperature at 3.3 millimeter wavelength
C. Witebsky+3 more
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Anisotropy of the cosmic background radiation implies the violation of the strong energy condition in Bianchi type I universe [PDF]
Takeshi Chiba+2 more
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In our previous study, we introduced a machine learning technique, namely Cosmic Microwave Background Foreground Subtraction with Convolutional Neural Networks ( CMBFSCNN ), for the removal of foreground contamination in cosmic microwave background (CMB)
Ye-Peng Yan+4 more
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Measurements of the cosmic microwave background radiation temperature at 90 GHz
Marco Bersanelli+6 more
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