[PDF] Top 20 Balloon-borne Cosmic Microwave Background experiments
Has 10000 "Balloon-borne Cosmic Microwave Background experiments" found on our website. Below are the top 20 most common "Balloon-borne Cosmic Microwave Background experiments".
Balloon-borne Cosmic Microwave Background experiments
... the balloon is the same as the surrounding atmospheric ...stratospheric balloon payload is recovered and can be flown again, for improved measurements, after a relatively short amount of time since the ... See full document
7
Cosmic ray nuclei detection in the balloon borne nuclear emulsion gamma ray telescope flight in Australia (GRAINE 2015)
... and implemented at the Fundamental Particle Laboratory (F-lab.) [5,6] in Nagoya University. HTS achieves over 5000 cm 2 per hour scanning speed. Figure 5 is the identified track density map in one HTS scanning command. ... See full document
5
Challenges for cosmic-ray experiments
... the cosmic-ray spectrum.The abundant elements of the primary cosmic- ray spectrum are measured accurately to energies higher than a TeV per nucleon with spectrometers in space ...with balloon- ... See full document
8
Cosmological parameters from velocities, cosmic microwave background and supernovae
... These three data sets directly probe the mass in the Universe, without the need to relate the galaxy distribution to the underlying mass via a `biasing' relation. We include the recent results from the CMB ... See full document
8
Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum
... (CMB, Cosmic Microwave Background, and EBL, Extragalactic Background Light) shape the spectrum of UHECR observed at the Earth and are also responsible for the production of secondary ... See full document
6
Measurement of the Polarization of the Cosmic Microwave Background with the BICEP2 and Keck Array Telescopes
... [5] S. J. Benton, P. A. Ade, M. Amiri, F. E. Angil`e, J. J. Bock, J. R. Bond, S. A. Bryan, H. C. Chiang, C. R. Contaldi, B. P. Crill, M. J. Devlin, B. Dober, O. P. Dor´e, M. Farhang, J. P. Filippini, L. M. Fissel, A. A. ... See full document
152
The Cosmic Stories: Beginning, Evolution and Present Days of the Universe
... the experiments searching for gravitational wave signatures predicted by the simple inflaton ...the cosmic microwave background (CMB) polarization maps [45, 46, ... See full document
131
A Search for Cosmic Microwave Background Anisotropies on Arcminute Scales
... Several experiments are currently, or will soon begin, looking for this B-mode signal, includ- ing BICEP [157], Planck [145] PolarBeaR [105], Spider [133], and Clover ...observational experiments aimed at ... See full document
251
Separation of Correlated Astrophysical Sources Using Multiple-Lag Data Covariance Matrices
... the microwave and millimeter-wave range, the dominant ra- diations are the cosmic microwave background, the galactic dust, the free-free emission and the synchrotron (see ...our ... See full document
13
Detection of Point Sources on Two-Dimensional Images Based on Peaks
... A very challenging aspect of data analysis in astronomy is the detection of pointlike sources embedded in one- and two- dimensional images. Some common examples are the sep- aration of individual stars in crowded optical ... See full document
11
Testing Inflationary Cosmology with the BICEP1 and BICEP2 Experiments
... Abstract Recent observations of the temperature anisotropies of the cosmic microwave background CMB favor an inflationary paradigm in which the scale factor of the universe inflated by m[r] ... See full document
212
Large Scale Cosmic Microwave Background Anisotropies and Dark Energy
... scale cosmic microwave background ...from cosmic microwave background experiments change if this is ...Combining cosmic microwave back- ground with large ... See full document
7
Data analysis of and results from observations of the cosmic microwave background with the Cosmic Background Imager
... or balloon-born experiments has been characterized by high signal-to-noise ratio (SNR) measurements of the CMB spectrum over large ranges of angular ...single experiments to trace out important ... See full document
167
Observation of Cosmic Microwave Background Polarization with BICEP
... other experiments [7–11], thus confirming our basic under- standing of CMB ...wave background, the existence of which is a robust prediction of inflation ... See full document
156
A limit on the polarization of the cosmic microwave background radiation
... initial experiments with the techniques which evolved from this insight focused on a period in early August 2000 which suffered from a lack of polarization ... See full document
308
Comptonization of the cosmic microwave background by relativistic plasma
... to give a marginal (1-sigma) detection of such a supra- thermal electron population in the Coma cluster. Since some other clusters are also expected to contain supra- thermal electrons – e.g. Abell 2256 revealed very ... See full document
15
A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set
... beam uncertainty and the calibration error for both experiments is taken into account by Monte-carlo techniques. The likelihood function is averaged over 1000 realizations under the assumption that each of the ... See full document
158
A Measurement of the Angular Power Spectrum of the Cosmic Microwave Background with a Long Duration Balloon borne Receiver
... A Measurement of the Angular Power Spectrum of the Cosmic Microwave Background with a Long Duration Balloon-borne Receiver Thesis by Brendan P.. In Partial Ful..[r] ... See full document
136
iSEDE demonstrator on high altitude balloon BEXUS : inflatable satellite encompassing disaggregated electronics
... space missions involving large space structure, the development of new deployable structures and the improvement of current designs are of great importance. Applications can be easily envisioned through truss structures, ... See full document
9
Exploring The Universe With The Atacama Cosmology Telescope: Polarization-Sensitive Measurements Of The Cosmic Microwave Background
... collapse became known as the Dark Ages (due to the lack of significant sources of radiation) and lasted until the local matter density became large enough to form the first stars and galaxies - approximately 200 million ... See full document
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