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Cosmic Microwave Background Constraints on the Duration and Timing of Reionizati...
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Probing star formation in the dense environments of z ~ 1 lensing haloes aligned...
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A Measurement of the Correlation of Galaxy Surveys with CMB Lensing Convergence...
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Planck intermediate results. XLIV. Structure of the Galactic magnetic field from...
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Planck intermediate results XLVII. Planck constraints on reionization history
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SPIDER: CMB Polarimetry from the Edge of Space
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280 GHz Focal Plane Unit Design and Characterization for the Spider-2 Suborbital...
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A New Limit on CMB Circular Polarization from SPIDER
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Pre-flight integration and characterization of the SPIDER balloon-borne telescop...
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Design and construction of a carbon fiber gondola for the SPIDER balloon-borne t...
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SPIDER: a balloon-borne CMB polarimeter for large angular scales
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Attitude determination for balloon-borne experiments
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BLASTbus electronics: general-purpose readout and control for balloon-borne expe...
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Particle Response of Antenna-Coupled TES Arrays: Results from SPIDERÂ and the La...
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Archeops in-flight performance, data processing, and map making
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A Simulation-based Method for Correcting Mode Coupling in CMB Angular Power Spec...
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Design and pre-flight performance of SPIDER 280 GHz receivers
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Related Subjects
cosmic microwave background
SPIDER
polarization
transition-edge sensor
cosmic background radiation
cosmology
inflation
millimeter wave instrumentation
scientific ballooning
Astronomy and Astrophysics
Astronomy data analysis
Cosmic microwave background radiation
Cosmic microwave background · Inflation · Bolometers · Transition-edge sensors · Polarimetry
Detector packaging · Magnetic shielding · Transition-edge sensors · Scientific ballooning · Cosmic microwave background
Observational cosmology
Space and Planetary Science
Spider
attitude determination
balloon-borne telescope
balloon-borne telescopes
composite materials
cosmic background radiation / dark ages
cosmology: theory
extinction – cosmic background radiation – ISM: magnetic fields
first stars / polarization
galaxies: structure
intergalactic medium
large-scale structure of universe
magnetohydrodynamics (MHD) – polarization – methods: data analysis – dust
methods: data analysis
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