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This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlations of CMB data, using the hybrid approach employed previously: pixel-based at $\ell<30$ and a Gaussian approximation to the distribution of spectra at higher $\ell$.
Pryke, C., Ade, P., Bock, J., et al., Second and Third Season QUaD Cosmic Microwave Background Temperature and Polarization Power Spectra. 2009, ApJ, 692, 1247, 0805.1944
1944
Earlier work this paper cites.
James, F. & Roos, M., Minuit - a system for function minimization and analysis of the parameter errors and correlations. 1975, Computer Physics Communications, 10, 343
1975
Earlier work this paper cites.
Haslam, C. G. T., Salter, C. J., Stoffel, H., & Wilson, W. E., A 408 MHz all-sky continuum survey. II - The atlas of contour maps. 1982, A&AS, 47, 1
1982
Earlier work this paper cites.
Scott, D. & White, M. 1994, in CMB Anisotropies Two Years after COBE: Observations, Theory and the Future, ed. L. M. Krauss, 214
1994
Earlier work this paper cites.
Wright, E. L., Bennett, C. L., Górski, K., Hinshaw, G., & Smoot, G. F., Angular Power Spectrum of the Cosmic Microwave Background Anisotropy Seen by the COBE DMR. 1996, The Astrophysical Journal Letters, 464, L21
1996
Earlier work this paper cites.
Hancock, S. & Rocha, G. 1997, in Microwave Background Anisotropies, ed. F. R. Bouchet, R. Gispert, B. Guiderdoni, & J. Trân Thanh Vân, 179–188
1997
Earlier work this paper cites.
Hu, W., Sugiyama, N., & Silk, J., The physics of microwave background anisotropies. 1997, Nature, 386, 37, astro-ph/9504057
1997
Earlier work this paper cites.
Hu, W. & White, M., CMB anisotropies: Total angular momentum method. 1997, Phys. Rev. D, 56, 596, astro-ph/9702170
1997
Earlier work this paper cites.
Kamionkowski, M., Kosowsky, A., & Stebbins, A., Statistics of cosmic microwave background polarization. 1997, Phys. Rev. D, 55, 7368, astro-ph/9611125
1997
Earlier work this paper cites.
Netterfield, C. B., Devlin, M. J., Jarosik, N., Page, L., & Wollack, E. J., A Measurement of the Angular Power Spectrum of the Anisotropy in the Cosmic Microwave Background. 1997, ApJ, 474, 47, astro-ph/9601197
1997
Earlier work this paper cites.
Seljak, U., Measuring Polarization in the Cosmic Microwave Background. 1997, ApJ, 482, 6
1997
Earlier work this paper cites.
Tegmark, M., How to measure CMB power spectra without losing information. 1997, Phys. Rev. D, 55, 5895, arXiv:astro-ph/9611174
1997
Earlier work this paper cites.
1997
Earlier work this paper cites.
Hanany, S., Ade, P. A. R., Balbi, A., et al., MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10 arcmin–5 degree. 2000, ApJ, 545, L5
2000
Earlier work this paper cites.
Knox, L. & Page, L., Characterizing the Peak in the Cosmic Microwave Background Angular Power Spectrum. 2000, Physical Review Letters, 85, 1366, astro-ph/0002162
2000
Earlier work this paper cites.
Souradeep, T. & Ratra, B., Window Function for Noncircular Beam Cosmic Microwave Background Anisotropy Experiment. 2001, The Astrophysical Journal, 560, 28
2001
Earlier work this paper cites.
Tegmark, M. & de Oliveira-Costa, A., How to measure CMB polarization power spectra without losing information. 2001, Phys. Rev. D, 64, 063001, arXiv:astro-ph/0012120
2001
Earlier work this paper cites.
Wandelt, B. D., Hivon, E., & Górski, K. M., Cosmic microwave background anisotropy power spectrum statistics for high precision cosmology. 2001, Phys. Rev. D, 64, 083003, arXiv:astro-ph/0008111
2001
Earlier work this paper cites.
de Bernardis, P., Ade, P. A. R., Bock, J. J., et al., Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology. 2002, ApJ, 564, 559, astro-ph/0105296
2002
Earlier work this paper cites.
Hansen, F. K., Górski, K. M., & Hivon, E., Gabor transforms on the sphere with applications to CMB power spectrum estimation. 2002, MNRAS, 336, 1304, arXiv:astro-ph/0207464
2002
Earlier work this paper cites.
Hivon, E., Górski, K. M., Netterfield, C. B., et al., MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets. 2002, ApJ, 567, 2, arXiv:astro-ph/0105302
2002
Earlier work this paper cites.
Kovac, J. M., Leitch, E. M., Pryke, C., et al., Detection of polarization in the cosmic microwave background using DASI. 2002, Nature, 420, 772
2002
Earlier work this paper cites.
Lewis, A. & Bridle, S., Cosmological parameters from CMB and other data: a Monte- Carlo approach. 2002, Phys. Rev., D66, 103511, astro-ph/0205436
2002
Earlier work this paper cites.
Benoît, A., Ade, P., Amblard, A., et al., Cosmological constraints from Archeops. 2003, A&A, 399, L25, astro-ph/0210306
2003
Earlier work this paper cites.
Bond, J. R., Contaldi, C., & Pogosyan, D., Cosmic microwave background snapshots: pre-WMAP and post-WMAP. 2003, Royal Society of London Philosophical Transactions Series A, 361, 2435, astro-ph/0310735
2003
Earlier work this paper cites.
Durrer, R., Novosyadlyj, B., & Apunevych, S., Acoustic Peaks and Dips in the Cosmic Microwave Background Power Spectrum: Observational Data and Cosmological Constraints. 2003, ApJ, 583, 33, astro-ph/0111594
2003
Earlier work this paper cites.
Grainge, K., Carreira, P., Cleary, K., et al., The cosmic microwave background power spectrum out to l= 1400 measured by the Very Small Array. 2003, MNRAS, 341, L23, astro-ph/0212495
2003
Earlier work this paper cites.
Hinshaw, G., Spergel, D. N., Verde, L., et al., First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: The Angular Power Spectrum. 2003, ApJS, 148, 135, astro-ph/0302217
2003
Earlier work this paper cites.
Hu, W., Hedman, M. M., & Zaldarriaga, M., Benchmark parameters for CMB polarization experiments. 2003, Phys. Rev. D, 67, 043004, arXiv:astro-ph/0210096v1
2003
Earlier work this paper cites.
Kogut, A., Spergel, D. N., Barnes, C., et al., First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature-Polarization Correlation. 2003, ApJS, 148, 161, astro-ph/0302213
2003
Earlier work this paper cites.
Page, L., Nolta, M. R., Barnes, C., et al., First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks. 2003, ApJS, 148, 233, astro-ph/0302220
2003
Earlier work this paper cites.
Pearson, T. J., Mason, B. S., Readhead, A. C. S., et al., The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager. 2003, ApJ, 591, 556, astro-ph/0205388
2003
Earlier work this paper cites.
Peiris, H. V., Komatsu, E., Verde, L., et al., First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications For Inflation. 2003, ApJS, 148, 213, astro-ph/0302225
2003
Earlier work this paper cites.
Chon, G., Challinor, A., Prunet, S., Hivon, E., & Szapudi, I., Fast estimation of polarization power spectra using correlation functions. 2004, MNRAS, 350, 914, astro-ph/0303414v2
2004
Earlier work this paper cites.
Efstathiou, G., Myths and truths concerning estimation of power spectra: the case for a hybrid estimator. 2004, MNRAS, 349, 603, arXiv:astro-ph/0307515
2004
Earlier work this paper cites.
Eriksen, H. K., O’Dwyer, I. J., Jewell, J. B., et al., Power Spectrum Estimation from High-Resolution Maps by Gibbs Sampling. 2004, ApJS, 155, 227, arXiv:astro-ph/0407028
2004
Earlier work this paper cites.
Readhead, A. C. S., Myers, S. T., Pearson, T. J., et al., Polarization Observations with the Cosmic Background Imager. 2004, Science, 306, 836, astro-ph/0409569
2004
Earlier work this paper cites.
Challinor, A. & Chon, G., Error analysis of quadratic power spectrum estimates for cosmic microwave background polarization: sampling covariance. 2005, MNRAS, 360, 509, astro-ph/0410097
2005
Earlier work this paper cites.
Chu, M., Eriksen, H. K., Knox, L., et al., Cosmological parameter constraints as derived from the Wilkinson Microwave Anisotropy Probe data via Gibbs sampling and the Blackwell-Rao estimator. 2005, Phys. Rev. D, 71, 103002, arXiv:astro-ph/0411737
2005
Earlier work this paper cites.
Górski, K. M., Hivon, E., Banday, A. J., et al., HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere. 2005, ApJ, 622, 759, astro-ph/0409513
2005
Earlier work this paper cites.
Polenta, G., Marinucci, D., Balbi, A., et al., Unbiased estimation of an angular power spectrum. 2005, J. Cosmology Astropart. Phys., 11, 1, arXiv:astro-ph/0402428
2005
Earlier work this paper cites.
Efstathiou, G., Hybrid estimation of cosmic microwave background polarization power spectra. 2006, MNRAS, 370, 343, arXiv:astro-ph/0601107
2006
Earlier work this paper cites.
Jones, W. C., Ade, P. A. R., Bock, J. J., et al., A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG. 2006, ApJ, 647, 823, arXiv:astro-ph/0507494
2006
Earlier work this paper cites.
Percival, W. J. & Brown, M. L., Likelihood techniques for the combined analysis of CMB temperature and polarization power spectra. 2006, MNRAS, 372, 1104, arXiv:astro-ph/0604547
2006
Earlier work this paper cites.
Fendt, W. A. & Wandelt, B. D., Computing High Accuracy Power Spectra with Pico. 2007, ArXiv e-prints, 0712.0194
2007
Earlier work this paper cites.
Fendt, W. A. & Wandelt, B. D., Pico: Parameters for the Impatient Cosmologist. 2007, ApJ, 654, 2
2007
Earlier work this paper cites.
Hinshaw, G., Nolta, M. R., Bennett, C. L., et al., Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis. 2007, ApJS, 170, 288, astro-ph/0603451
2007
Earlier work this paper cites.
Jones, W. C., Montroy, T. E., Crill, B. P., et al., Instrumental and analytic methods for bolometric polarimetry. 2007, A&A, 470, 771
2007
Earlier work this paper cites.
Sievers, J. L., Achermann, C., Bond, J. R., et al., Implications of the Cosmic Background Imager Polarization Data. 2007, ApJ, 660, 976, astro-ph/0509203
2007
Cited alongside, same era.
Corasaniti, P. S. & Melchiorri, A., Testing cosmology with cosmic sound waves. 2008, Phys. Rev. D, 77, 103507, 0711.4119
2008
Cited alongside, same era.
Destri, C., de Vega, H. J., & Sanchez, N. G., CMB quadrupole depression produced by early fast-roll inflation: Monte Carlo Markov chains analysis of WMAP and SDSS data. 2008, Phys. Rev. D, 78, 023013, 0804.2387
2008
Cited alongside, same era.
Eriksen, H. K., Jewell, J. B., Dickinson, C., et al., Joint Bayesian Component Separation and CMB Power Spectrum Estimation. 2008, ApJ, 676, 10, 0709.1058
2008
Cited alongside, same era.
Hamimeche, S. & Lewis, A., Likelihood analysis of CMB temperature and polarization power spectra. 2008, Phys. Rev. D, 77, 103013, 0801.0554
Kitazawa, N. & Sagnotti, A., Pre-inflationary clues from String Theory? 2014, J. Cosmology Astropart. Phys., 4, 17, 1402.1418
2014
Later among the works it cites.
Planck Collaboration VI, Planck
2014
Later among the works it cites.
Planck Collaboration VII, Planck
2014
Later among the works it cites.
Planck Collaboration XI, Planck
2014
Later among the works it cites.
Planck Collaboration XII, Planck
2014
Later among the works it cites.
Planck Collaboration XIII, Planck
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Later among the works it cites.
Planck Collaboration XV, Planck
2014
Later among the works it cites.
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Cited alongside, same era.
Tinker, J., Kravtsov, A. V., Klypin, A., et al., Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality. 2008, ApJ, 688, 709, 0803.2706
2008
Cited alongside, same era.
Dunkley, J., Komatsu, E., Nolta, M. R., et al., Five-Year Wilkinson Microwave Anisotropy Probe Observations: Likelihoods and Parameters from the WMAP Data. 2009, ApJS, 180, 306, 0803.0586
2009
Cited alongside, same era.
Gruppuso, A., de Rosa, A., Cabella, P., et al., New estimates of the CMB angular power spectra from the WMAP 5 year low-resolution data. 2009, MNRAS, 400, 463, 0904.0789
2009
Cited alongside, same era.
Reichardt, C. L., Ade, P. A. R., Bock, J. J., et al., High-Resolution CMB Power Spectrum from the Complete ACBAR Data Set. 2009, ApJ, 694, 1200, 0801.1491
2009
Cited alongside, same era.
Rudjord, Ø., Groeneboom, N. E., Eriksen, H. K., et al., Cosmic Microwave Background Likelihood Approximation by a Gaussianized Blackwell-Rao Estimator. 2009, ApJ, 692, 1669, 0809.4624
2009
Cited alongside, same era.
Arnaud, M., Pratt, G. W., Piffaretti, R., et al., The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y SZ
2010
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Fowler, J. W., Acquaviva, V., Ade, P. A. R., et al., The Atacama Cosmology Telescope: A Measurement of the 600 < ℓ < 8000 600<\ell<8000 Cosmic Microwave Background Power Spectrum at 148 GHz. 2010, ApJ, 722, 1148, 1001.2934
2010
Cited alongside, same era.
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2014
Later among the works it cites.
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