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The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite.
Planck Collaboration VII, Planck
1906
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Challinor, A. & van Leeuwen, F., Peculiar velocity effects in high-resolution microwave background experiments. 2002, Phys. Rev. D, 65, 103001, astro-ph/0112457
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Kamionkowski, M. & Knox, L., Aspects of the cosmic microwave background dipole. 2003, Phys. Rev. D, 67, 063001, astro-ph/0210165
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Chluba, J., Hütsi, G., & Sunyaev, R. A., Clusters of galaxies in the microwave band: Influence of the motion of the Solar System. 2005, A&A, 434, 811, astro-ph/0409058
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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
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Burles, S. & Rappaport, S., Detecting the Aberration of the Cosmic Microwave Background. 2006, ApJ, 641, L1, astro-ph/0601559
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Desjacques, V., Baryon acoustic signature in the clustering of density maxima. 2008, Phys. Rev. D, 78, 103503, 0806.0007
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Hinshaw, G., Weiland, J. L., Hill, R. S., et al., Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results. 2009, ApJS, 180, 225, 0803.0732
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Bucher, M., van Tent, B., & Carvalho, C. S., Detecting bispectral acoustic oscillations from inflation using a new flexible estimator. 2010, Monthly Notices of the Royal Astronomical Society, 407, 2193, http://oup.prod.sis.lan/mnras/article-pdf/407/4/2193/3195988/mnras0407-2193.pdf
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Komatsu, E., Smith, K. M., Dunkley, J., et al., Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation. 2011, ApJS, 192, 18, 1001.4538
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Planck Collaboration VIII, Planck
2016
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Planck Collaboration XXII, Planck
2016
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Planck Collaboration Int. XLIX, Planck
2016
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Contreras, D., Boubel, P., & Scott, D., Constraints on direction-dependent cosmic birefringence from Planck polarization data. 2017, J. Cosmology Astropart. Phys., 2017, 046, 1705.06387
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Alonso, D., Sanchez, J., Slosar, A., & Collaboration, L. D. E. S., A unified pseudo-C ℓ \ell framework. 2019, Monthly Notices of the Royal Astronomical Society, 484, 4127, http://oup.prod.sis.lan/mnras/article-pdf/484/3/4127/27747342/stz093.pdf
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Remazeilles, M., Delabrouille, J., & Cardoso, J.-F., CMB and SZ effect separation with constrained Internal Linear Combinations. 2011, MNRAS, 410, 2481, 1006.5599
2011
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Bhattacharya, S., Nagai, D., Shaw, L., Crawford, T., & Holder, G. P., Bispectrum of the Sunyaev-Zel’dovich Effect. 2012, ApJ, 760, 5, 1203.6368
2012
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Hurier, G., Macías-Pérez, J. F., & Hildebrandt, S., MILCA, a modified internal linear combination algorithm to extract astrophysical emissions from multifrequency sky maps. 2013, A&A, 558, A118, 1007.1149
2013
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Planck Collaboration XXI, Planck
2014
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Planck Collaboration XXVII, Planck
2014
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Planck Collaboration Int. XIII, Planck
2014
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Notari, A. & Quartin, M., CMB all-scale blackbody distortions induced by linearizing temperature. 2015, ArXiv e-prints, 1510.08793
2015
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Jow, D. L., Contreras, D., Scott, D., & Bunn, E. F., Taller in the saddle: constraining CMB physics using saddle points. 2019a, J. Cosmology Astropart. Phys., 2019, 031, 1811.05629
2019
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Jow, D. L., Contreras, D., Scott, D., & Bunn, E. F., Taller in the saddle: constraining CMB physics using saddle points. 2019b, J. Cosmology Astropart. Phys., 2019, 031, 1811.05629
2019
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Planck Collaboration I, Planck
2019
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Planck Collaboration II, Planck
2019
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Planck Collaboration III, Planck
2019
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Planck Collaboration IV, Planck
2019
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