No evidence for dust B-mode decorrelation in Planck data
暂无分享,去创建一个
[1] U. Seljak,et al. Signature of gravity waves in polarization of the microwave background , 1996, astro-ph/9609169.
[2] Uros Seljak,et al. Measuring Polarization in the Cosmic Microwave Background , 1996, astro-ph/9608131.
[3] C. A. Oxborrow,et al. Planck 2013 results. XVI. Cosmological parameters , 2013, 1303.5076.
[4] Albert Stebbins,et al. A Probe of Primordial Gravity Waves and Vorticity , 1997 .
[5] J. Aumont,et al. Planck intermediate results L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis , 2016, 1606.07335.
[6] David Alonso,et al. The Python Sky Model: software for simulating the Galactic microwave sky , 2016, 1608.02841.
[7] G. W. Pratt,et al. Planck 2015 results Special feature Planck 2015 results XII . Full focal plane simulations , 2016 .
[8] R. W. Ogburn,et al. Joint Analysis of BICEP2/Keck Array and Planck Data , 2015, 1502.00612.
[9] G. W. Pratt,et al. Planck 2013 results. XI. All-sky model of thermal dust emission , 2013, 1312.1300.
[10] V. Pavlidou,et al. Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz? , 2014, 1410.8136.
[11] Scott Dodelson,et al. Line-of-sight extrapolation noise in dust polarization , 2016, 1606.08922.
[12] E. Hivon,et al. Fast estimation of polarization power spectra using correlation functions , 2003, astro-ph/0303414.
[13] C. A. Oxborrow,et al. Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth , 2016, 1605.02985.
[14] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[15] G. W. Pratt,et al. Planck 2015 results Special feature Planck 2015 results VIII . High Frequency Instrument data processing : Calibration and maps , 2016 .
[16] XSPECT, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars , 2004, astro-ph/0405575.
[17] G. W. Pratt,et al. Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies , 2013, 1312.5446.
[18] G. W. Pratt,et al. Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization , 2014, 1405.0874.
[19] Miss A.O. Penney. (b) , 1974, The New Yale Book of Quotations.
[20] G. W. Pratt,et al. Planck intermediate results - XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes , 2014, 1409.5738.
[21] J. Aumont,et al. The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths , 2012, 1207.3675.
[22] Matias Zaldarriaga,et al. Gravitational lensing effect on cosmic microwave background polarization , 1998, astro-ph/9803150.