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Axion Dark Matter / Adams, C.B. (Munich, Max Planck Inst. ; Columbia U.) ; Aggarwal, N. (Northwestern U.) ; Agrawal, A. (Chicago U.) ; Balafendiev, R. (Unlisted) ; Bartram, C. (Washington U., Seattle) ; Baryakhtar, M. (Washington U., Seattle) ; Bekker, H. (Helmholtz Inst., Mainz ; Mainz U.) ; Belov, P. (Unlisted) ; Berggren, K.K. (MIT) ; Berlin, A. (Fermilab) et al.
Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. [...]
arXiv:2203.14923 ; FERMILAB-CONF-22-996-PPD-T. - 96.
eConf - Fermilab Library Server - Fulltext - Fulltext

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Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes / Planck Collaboration
The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 100GHz. We exploit the Planck HFI polarization data from 100 to 353GHz to measure the dust angular power spectra $C_\ell^{EE,BB}$ over the range $40<\ell<600$. [...]
arXiv:1409.5738.- 2016-02-09 - 25 p. - Published in : Astron. Astrophys. 586 (2016) A133 Fulltext: PDF; External link: Nature article

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Planck 2013 results. XI. All-sky model of thermal dust emission / Planck Collaboration
This paper presents an all-sky model of dust emission from the Planck 857, 545 and 353 GHz, and IRAS 100 micron data. Using a modified black-body fit to the data we present all-sky maps of the dust optical depth, temperature, and spectral index over the 353-3000 GHz range. [...]
arXiv:1312.1300.- 2014 - 36 p. - Published in : Astron. Astrophys. 571 (2014) A11 External link: Preprint

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Planck 2013 results. XVI. Cosmological parameters / Planck Collaboration
We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. [...]
arXiv:1303.5076; CERN-PH-TH-2013-129; CERN-PH-TH-2013-129.- 2014-10-29 - 66 p. - Published in : Astron. Astrophys. 571 (2014) A16 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Planck 2013 results. XV. CMB power spectra and likelihood / Planck collaboration
We present the Planck likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations. We use this likelihood to derive the Planck CMB power spectrum over three decades in l, covering 2 <= l <= 2500 [...]
arXiv:1303.5075; CERN-PH-TH-2013-128; CERN-PH-TH-2013-128.- 2014-10-29 - 60 p. - Published in : Astron. Astrophys. 571 (2014) A15 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Planck 2013 results. XIII. Galactic CO emission / Planck collaboration
Rotational transition lines of CO play a major role in molecular radio astronomy and in particular in the study of star formation and the Galactic structure. Although a wealth of data exists in the Galactic plane and some well-known molecular clouds, there is no available CO high sensitivity all-sky survey to date. [...]
arXiv:1303.5073; CERN-PH-TH-2013-126; CERN-PH-TH-2013-126.- 2014-10-29 - 22 p. - Published in : Astron. Astrophys. 571 (2014) A13 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Planck 2013 results. XII. Diffuse component separation / Planck Collaboration
Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwave background (CMB) temperature fluctuations over nearly the full sky, as well as new constraints on Galactic foregrounds. [...]
arXiv:1303.5072; CERN-PH-TH-2013-125; CERN-PH-TH-2013-125.- 2014-10-29 - 31 p. - Published in : Astron. Astrophys. 571 (2014) A12 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Planck 2013 results. V. LFI calibration / Planck Collaboration
We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the Orbital Dipole plus the Solar Dipole, caused respectively by the motion of the Planck spacecraft with respect to the Sun and by motion of the Solar System with respect to the CMB rest frame [...]
arXiv:1303.5066; CERN-PH-TH-2013-119; CERN-PH-TH-2013-119.- 2014-10-29 - 29 p. - Published in : Astron. Astrophys. 571 (2014) A5 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Planck 2013 results. IV. Low Frequency Instrument beams and window functions / Planck Collaboration
This paper presents the characterization of the in-flight beams, the beam window functions and the associated uncertainties for the Planck Low Frequency Instrument (LFI). Knowledge of the beam profiles is necessary for determining the transfer function to go from the observed to the actual sky anisotropy power spectrum. [...]
arXiv:1303.5065; CERN-PH-TH-2013-118; CERN-PH-TH-2013-118.- 2014-10-29 - 22 p. - Published in : Astron. Astrophys. 571 (2014) A4 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Planck 2013 results. III. LFI systematic uncertainties / Planck Collaboration
We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. [...]
arXiv:1303.5064; CERN-PH-TH-2013-117; CERN-PH-TH-2013-117.- 2014-10-29 - 23 p. - Published in : Astron. Astrophys. 571 (2014) A3 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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Vedi anche: autori con nomi simili
10	Jewell, J
15	Jewell, J B
1	Jewell, J E
4	Jewell, J K
1	Jewell, J S
1	Jewell, Jeffrey
3	Jewell, Jeffrey B
1	Jewell, Joseph S

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