Results 61 to 70 of about 6,884 (245)
Measurements of the Cosmic Background Radiation [PDF]
Measurements of the attributes of the 2.7-K microwave background radiation (CBR) are reviewed, with emphasis on the analytic phase of CBR studies. Methods for the direct measurement of the CBR spectrum are discussed; attention is given to receivers, antennas, absolute receiver calibration, atmospheric emission and absorption, the galactic background ...
openaire +2 more sources
Search for Linear Polarization of the Cosmic Background Radiation [PDF]
We present preliminary measurements of the linear polarization of the cosmic microwave background (3 K blackbody) radiation. These ground-based measurements are made at 9-mm wavelength. We find no evidence for linear polarization, and set an upper limit for a polarized component of 0.8 mK with 95% confidence level. This implies that the present rate of
Lubin, P M, Smoot, G F
openaire +6 more sources
ABSTRACT Chronologic and geomorphic evidence of past glaciations is largely recorded in areas at relatively low elevation and/or landscapes defined by high glacial erosion. As a result, data from areas that did not experience significant glacial erosion and the highest elevation locations are lacking from reconstructions of past ice masses.
Samuel E. Kelley+5 more
wiley +1 more source
CMB-S4: Iterative Internal Delensing and r Constraints
The tightest constraints on the tensor-to-scalar ratio r can only be obtained after removing a substantial fraction of the lensing B -mode sample variance.
Sebastian Belkner+6 more
doaj +1 more source
Recovering Cosmic Microwave Background Polarization Signals with Machine Learning
Primordial B-mode detection is one of the main goals of current and future cosmic microwave background (CMB) experiments. However, the weak B-mode signal is overshadowed by several Galactic polarized emissions, such as thermal dust emission and ...
Ye-Peng Yan+3 more
doaj +1 more source
Measurements of the Cosmic Background Radiation [PDF]
Maps of the large scale structure (θ>6 °) of the cosmic background radiation covering 90% of the sky are now available. The data show a very strong 50–100 σ (statistical error) dipole component, interpreted as being due to our motion, with a direction of α = 11.25 ± 0.15 hours, δ = -5.6 ± 2.0° The inferred direction of the velocity of our galaxy ...
Philip Lubin, Thyrso Villela
openaire +2 more sources
ABSTRACT The evolution of lakes in western Mongolia and their responses to climate changes and glacial meltwater input remain poorly understood. This study evaluates the reliability of multigrain and single‐grain K‐feldspar post‐infrared infrared stimulated luminescence (IRSL) (pIRIR) dating applied to palaeoshoreline sediments at Khyargas Nuur ...
Neda Rahimzadeh+4 more
wiley +1 more source
The Atacama Cosmology Telescope: Systematic Transient Search of 3 Day Maps
We conduct a systematic search for transients in 3 yr of data (2017–2019) from the Atacama Cosmology Telescope (ACT). ACT covers 40% of the sky at three bands spanning from 77–277 GHz. Analysis of 3 day mean-subtracted sky maps, which were match filtered
Yaqiong Li+36 more
doaj +1 more source
Balloon-Based Measurements of the Cosmic Background Radiation [PDF]
We have developed and flown a balloon-borne liquid-heliumcooled spectrometer to measure the cosmic background radiation in the 3 -18-cm/sup -1/ region. It features a cooled horn antenna, a polarizing Michelson interferometer, and a germanium bolometer. These design features and the performance of the instrument are discussed.
Mather, John C.+2 more
openaire +2 more sources
A cross‐correlator‐based timing tool for FemtoMAX
A novel timing tool suited for FemtoMAX is described. This will allow sub‐100 fs time‐resolved measurements at FemtoMAX.We report on the commissioning of an ultrafast timing diagnostic for measuring a time‐offset signal between two different synchronized ultrashort light pulses.
D. Kroon+11 more
wiley +1 more source