Planck 2018 results. II. Low Frequency Instrument data processing

Fixsen, D. J., The Temperature of the Cosmic Microwave Background. 2009, ApJ, 707, 916, 0911.1955

1955

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.

Mo, H. J. & White, S. D. M., An analytic model for the spatial clustering of dark matter haloes. 1996, MNRAS, 282, 347, astro-ph/9512127

1996

Earlier work this paper cites.

Wang, L. & Steinhardt, P. J., Cluster Abundance Constraints for Cosmological Models with a Time-varying, Spatially Inhomogeneous Energy Component with Negative Pressure. 1998, ApJ, 508, 483, astro-ph/9804015

1998

Earlier work this paper cites.

Dame, T. M., Hartmann, D., & Thaddeus, P., The Milky Way in Molecular Clouds: A New Complete CO Survey. 2001, ApJ, 547, 792, astro-ph/0009217

2001

Earlier work this paper cites.

Delabrouille, J., Melin, J.-B., & Bartlett, J. G. 2002, in Astronomical Society of the Pacific Conference Series, Vol. 257, AMiBA 2001: High-Z Clusters, Missing Baryons, and CMB Polarization, ed. L.-W. Chen, C.-P. Ma, K.-W. Ng, & U.-L. Pen, 81

2001

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.

Maino, D., Burigana, C., Górski, K. M., Mandolesi, N., & Bersanelli, M., Removing 1/f noise stripes in cosmic microwave background anisotropy observations. 2002, A&A, 387, 356, astro-ph/0202271

2002

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.

Keihänen, E., Kurki-Suonio, H., & Poutanen, T., MADAM- a map-making method for CMB experiments. 2005, MNRAS, 360, 390, astro-ph/0412517

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

2005

Earlier work this paper cites.

Reinecke, M., Dolag, K., Hell, R., Bartelmann, M., & Enßlin, T. A., A simulation pipeline for the Planck mission. 2006, A&A, 445, 373, astro-ph/0508522

2006

Earlier work this paper cites.

Page, L., Hinshaw, G., Komatsu, E., et al., Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis. 2007, ApJS, 170, 335, astro-ph/0603450

2007

Earlier work this paper cites.

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

Earlier work this paper cites.

Miville-Deschênes, M.-A., Ysard, N., Lavabre, A., et al., Separation of anomalous and synchrotron emissions using WMAP polarization data. 2008, A&A, 490, 1093, 0802.3345

2008

Earlier work this paper cites.

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

Earlier work this paper cites.

Basak, S., Prunet, S., & Benabed, K., Simulating weak lensing of CMB maps. 2009, A&A, 508, 53

2009

Earlier work this paper cites.

Meinhold, P., Leonardi, R., Aja, B., et al., Noise properties of the Planck-LFI receivers. 2009, Journal of Instrumentation, 4, 2009, 1001.4608

2009

Earlier work this paper cites.

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

Earlier work this paper cites.

Bersanelli, M., Mandolesi, N., Butler, R. C., et al., Planck

2010

Earlier work this paper cites.

Keihänen, E., Keskitalo, R., Kurki-Suonio, H., Poutanen, T., & Sirviö, A., Making cosmic microwave background temperature and polarization maps with MADAM. 2010, A&A, 510, A57, 0907.0367

2010

Earlier work this paper cites.

Mennella, A., Bersanelli, M., Butler, R. C., et al., Planck

2010

Earlier work this paper cites.

Blas, D., Lesgourgues, J., & Tram, T., The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes. 2011, J. Cosmology Astropart. Phys., 7, 034, 1104.2933

2011

Earlier work this paper cites.

Fixsen, D. J., Kogut, A., Levin, S., et al., ARCADE 2 Measurement of the Absolute Sky Brightness at 3-90 GHz. 2011, The Astrophysical Journal, 734, 5

2011

Earlier work this paper cites.

Planck Collaboration. 2011, The Explanatory Supplement to the Planck Early Release Compact Source Catalogue (ESA)

2011

Earlier work this paper cites.

Planck Collaboration XIV, Planck

2011

Earlier work this paper cites.

Remazeilles, M., Delabrouille, J., & Cardoso, J.-F., Foreground component separation with generalized Internal Linear Combination. 2011, MNRAS, 418, 467, 1103.1166

2011

Earlier work this paper cites.

Bennett, C. L., Larson, D., Weiland, J. L., et al., Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results. 2013, ApJS, 208, 20, 1212.5225

2013

Earlier work this paper cites.

Cai, Z.-Y., Lapi, A., Xia, J.-Q., et al., A Hybrid Model for the Evolution of Galaxies and Active Galactic Nuclei in the Infrared. 2013, ApJ, 768, 21, 1303.2335

2013

Earlier work this paper cites.

Delabrouille, J., Betoule, M., Melin, J.-B., et al., The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths. 2013, A&A, 553, A96, 1207.3675

2013

Earlier work this paper cites.

Dio, E. D., Montanari, F., Lesgourgues, J., & Durrer, R., The CLASSgal code for relativistic cosmological large scale structure. 2013, J. Cosmology Astropart. Phys., 11, 044

2013

Earlier work this paper cites.

Planck Collaboration I, Planck

2014

Earlier work this paper cites.

Planck Collaboration II, Planck

2014

Earlier work this paper cites.

Planck Collaboration III, Planck

2014

Earlier work this paper cites.

Planck Collaboration IV, Planck

2014

Earlier work this paper cites.

Planck Collaboration V, Planck

2014

Earlier work this paper cites.

Planck Collaboration VI, Planck

2014

Earlier work this paper cites.

Planck Collaboration VII, Planck

2014

Earlier work this paper cites.

Planck Collaboration VIII, Planck

2014

Earlier work this paper cites.

Planck Collaboration IX, Planck

2014

Earlier work this paper cites.

Planck Collaboration X, Planck

2014

Earlier work this paper cites.

Planck Collaboration XI, Planck

2014

Earlier work this paper cites.

Planck Collaboration XII, Planck

2014

Earlier work this paper cites.

Planck Collaboration XIII, Planck

2014

Cited alongside, same era.

Planck Collaboration XIV, Planck

2014

Cited alongside, same era.

Planck Collaboration XV, Planck

2014

Cited alongside, same era.

Planck Collaboration XVI, Planck

2014

Cited alongside, same era.

Planck Collaboration XVII, Planck

2014

Cited alongside, same era.

Planck Collaboration XVIII, Planck

2014

Cited alongside, same era.

Planck Collaboration XIX, Planck

2014

Cited alongside, same era.

Planck Collaboration XXI, Planck

2016

Later among the works it cites.

Planck Collaboration XXII, Planck

2016

Later among the works it cites.

Planck Collaboration XXIII, Planck

2016

Later among the works it cites.

Planck Collaboration XXIV, Planck

2016

Later among the works it cites.

Planck Collaboration XXV, Planck

2016

Later among the works it cites.

Planck Collaboration XXVI, Planck

2016

Later among the works it cites.

Planck Collaboration XXVII, Planck

2016

Later among the works it cites.