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[PDF] Top 20 Data analysis of and results from observations of the cosmic microwave background with the Cosmic Background Imager

Has 10000 "Data analysis of and results from observations of the cosmic microwave background with the Cosmic Background Imager" found on our website. Below are the top 20 most common "Data analysis of and results from observations of the cosmic microwave background with the Cosmic Background Imager".

Data analysis of and results from observations of the cosmic microwave background with the Cosmic Background Imager

Data analysis of and results from observations of the cosmic microwave background with the Cosmic Background Imager

... Even if the Karhunen-Loeve compression were computationally feasible, it suffers from another drawback. Namely, though it is optimal at maximizing the expected SNR, for typical CMB behav- iors, it is bad at ... See full document

167

H_o from Cosmic Background Imager observations of the Sunyaev-Zeldovich effect in nearby clusters

H_o from Cosmic Background Imager observations of the Sunyaev-Zeldovich effect in nearby clusters

... Ben Mazin’s no-nonsense point of view helped me keep things in perspective over the years. Dave Vakil has become a true friend, someone I can always count on, even though we almost killed each other when we first ... See full document

131

A limit on the polarization of the cosmic microwave background radiation

A limit on the polarization of the cosmic microwave background radiation

... departures from uniform behavior would affect the interpretation of the cross polarized visibilities for extended ...example, from the il- lumination pattern of the ...polarization observations of ... See full document

308

Observation of Cosmic Microwave Background Polarization with BICEP

Observation of Cosmic Microwave Background Polarization with BICEP

... PSB-differenced data. Stability data taken shortly before deploying the instrument indicated that the FRMs introduced excess white noise, and the power spectral densities of the FRM-demodulated bolometer ... See full document

156

Dark Energy Stars and the Cosmic Microwave Background

Dark Energy Stars and the Cosmic Microwave Background

... the cosmic seed eventually lead to the production of primordial dark energy stars with masses −10 3 M O ...the cosmic seed, which accounts for the overall isotropy and homogeneity of the observable ...the ... See full document

7

Balloon-borne Cosmic Microwave Background experiments

Balloon-borne Cosmic Microwave Background experiments

... range from a few kg to more than two tons, depending on the balloons size, ranging from a few thousands cubic meters volume at float, to more than 1 million cubic ...development: from the idea, to ... See full document

7

Peculiar Features in the Cosmic Microwave Background Radiation

Peculiar Features in the Cosmic Microwave Background Radiation

... century; from a view limited to our Galaxy to a cosmos with billions of sim- ilar ...Recent observations of the large scale structure ...Wilkinson Microwave Anisotropy Probe (WMAP; Bennett et al., ... See full document

111

CiteSeerX — STATISTICAL CHALLENGES IN THE ANALYSIS OF COSMIC MICROWAVE BACKGROUND RADIATION

CiteSeerX — STATISTICAL CHALLENGES IN THE ANALYSIS OF COSMIC MICROWAVE BACKGROUND RADIATION

... evidence from WMAP data that isotropy may fail, that is, some authors have suggested that data on CMB radiation may show some asymmetries which would be inconsistent with isotropy [see, ...causes. ... See full document

36

Cosmological parameters from velocities, cosmic microwave background and supernovae

Cosmological parameters from velocities, cosmic microwave background and supernovae

... ± cosmic microwave background ± cosmological parameters ± cosmology: observations ± cosmology: theory ± large-scale structure of ...simultaneous analysis of the constraints placed on ... See full document

8

Semi analytic calculation of cosmic microwave background anisotropies from wiggly and superconducting cosmic strings

Semi analytic calculation of cosmic microwave background anisotropies from wiggly and superconducting cosmic strings

... our results for network evolution and in figure 3 the corresponding CMB anisotropies com- puted in our modified version of ...corresponding results of the original CMBact code [43] for ...our ... See full document

20

A Search for Cosmic Microwave Background Anisotropies on Arcminute Scales

A Search for Cosmic Microwave Background Anisotropies on Arcminute Scales

... Cluster Observations Since November 2006, we have observed nine clusters and one blank test field at 150 GHz with Bolocam at the CSO, and each cluster has been observed for a total of approximately ten ...noise ... See full document

251

Cosmic microwave background science at commercial airline altitudes

Cosmic microwave background science at commercial airline altitudes

... (9 km) with further modifications and testing, and careful operation from a suitable 8–10 000 feet operating base. There are several features of Airlander 10 that lend it well to CMB observations. Airlander ... See full document

5

The Cosmic Microwave Background and the Big Bang Theory of the Universe

The Cosmic Microwave Background and the Big Bang Theory of the Universe

... light from the stars shifted to lower frequencies as the stars ...Hubble’s data were so scattered in 1929 that it is amazing that he could have made the conclusions he ...the results have ... See full document

8

LiteBIRD: an all-sky cosmic microwave background probe of inflation

LiteBIRD: an all-sky cosmic microwave background probe of inflation

... sky observations at many different timescales and a large-angle coverage for most of the pixels on the ...Planck data, since it allows instantaneous estimation of Stokes ... See full document

17

Square Kilometre Array and cosmic microwave background spectral distortions

Square Kilometre Array and cosmic microwave background spectral distortions

... 2. The Square Kilometre Array The Square Kilometre Array (SKA) is a huge, new technology radio telescope that, with an extension of ∼ 3000 km and a collecting area of ∼ 1 km 2 , has been designed to provide a significant ... See full document

Large Scale Cosmic Microwave Background Anisotropies and Dark Energy

Large Scale Cosmic Microwave Background Anisotropies and Dark Energy

... scale cosmic microwave background ...constraints from cosmic microwave background experiments change if this is ...Combining cosmic microwave back- ground ... See full document

7

Cosmology from galaxy clusters with cosmic microwave background lensing mass calibration

Cosmology from galaxy clusters with cosmic microwave background lensing mass calibration

... unbiased results given the presence of selection ...mock observations obtained from an N -body ...deviations from the commonly- assumed log-normality in the ...(e.g., from CMB-S4), in ... See full document

224

Studying Heavy Ion Collisions Using Methods From Cosmic Microwave Background (CMB) Analysis

Studying Heavy Ion Collisions Using Methods From Cosmic Microwave Background (CMB) Analysis

... Figure 4. Left panel: power spectra for the map from Fig.3. The black histogram shows the total power spectrum, the blue dots are for the m = 0 mode only and the red histogram shows the power associated with m ≥ 1 ... See full document

9

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP*) Observations: Bayesian Estimation Of Cosmic Microwave Background Polarization Maps

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP*) Observations: Bayesian Estimation Of Cosmic Microwave Background Polarization Maps

... WMAP data we find a consistent result compared to template cleaning, with τ = ...0.019 from this method and 0.086 ± 0.016 from the standard template-cleaning ... See full document

10

Polarized cosmic microwave background map recovery   with sparse component separation

Polarized cosmic microwave background map recovery with sparse component separation

... cosmological microwave background are an invaluable source of information for cosmology and a unique window to probe the energy scale of ...information from microwave surveys requires ... See full document

13

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