Gotowe bibliografie tematyczne / Cosmic microwave background radiation (CMB)

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji
  6. Raporty organizacyjne

Gotowa bibliografia na temat „Cosmic microwave background radiation (CMB)”

Autor: Grafiati
Data publikacji: 3 czerwca 2025
Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Cosmic microwave background radiation (CMB)"

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Pommerenke, Gerd. "About Cosmic Microwave Background Radiation (CMBR)." Annals of Computational Physics and Material Science 1, no. 2 (2024): 01–42. http://dx.doi.org/10.33140/acpms.01.02.03.

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Because the CMBR follows the PLANCK's radiation law more or less exactly, it should, because of the indistinguishability of individual photons, apply to a whatever black emitter. Therefrom arises the guess, that the existence of an upper cut- off frequency of the vacuum could be the cause for the decrease in the upper frequency range. Since the lower-frequent share of the curve correlates with the frequency response of an oscillating circuit with the Qfactor ½, it is examined, whether it succeeds to approximate the Planck curve by multi-plication of the initial curve with the dynamic, time- de
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Smoot, G. F. "Of Cosmic Background Anisotropies." Symposium - International Astronomical Union 168 (1996): 31–44. http://dx.doi.org/10.1017/s007418090010991x.

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Observations of the Cosmic Microwave Background (CMB) Radiation have put the standard model of cosmology, the Big Bang, on firm footing and provide tests of various ideas of large scale structure formation. CMB observations now let us test the role of gravity and General Relativity in cosmology including the geometry, topology, and dynamics of the Universe. Foreground galactic emissions, dust thermal emission and emission from energetic electrons, provide a serious limit to observations. Nevertheless, observations may determine if the evolution of the Universe can be understood from fundamenta
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BERSHADSKII, A. "SCALING PROPERTIES OF THE COSMIC BACKGROUND PLASMA AND RADIATION." International Journal of Modern Physics D 12, no. 03 (2003): 509–17. http://dx.doi.org/10.1142/s0218271803003219.

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Scaling properties of the cosmic microwave background (CMB) radiation are studied using satellite (COBE-DMR maps), balloon-borne and ground-based (combined QMASK map) data. Quantitative consistency is found between the multiscaling properties of the COBE-DMR and QMASK CMB maps. Surprisingly, it is found that the observed CMB temperature multiscaling quantitatively resembles the multiscaling properties of fluid turbulence, that indicates primordial plasma turbulence as an origin of the CMB temperature space anisotropy.
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Svishch, V. M. "The Features of the Reference Frame Concomitant to the Cosmic Microwave Background." European Journal of Applied Physics 3, no. 6 (2021): 1–6. http://dx.doi.org/10.24018/ejphysics.2021.3.6.115.

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The features of reference frame, concomitant to the cosmic microwave background, immobile relatively cosmic microwave background, are considered. It is shown that the features of reference frame, concomitant to the cosmic microwave background (CMB), are determined by its properties. Any other object in the Universe and reference frame concomitant to it, is immersed in the CMB and moves relative to the reference frame concomitant to microwave background radiation. The zero pecular velocity of the reference frame concomitant to the microwave background radiation is analogous to the zero temperat
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Smoot, George F. "Antarctic observations of the cosmic microwave background." Highlights of Astronomy 9 (1992): 589. http://dx.doi.org/10.1017/s1539299600022607.

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In the standard cosmology of the Big Bang theory the cosmic microwave background (CMB) is the remnant radiation from the hot early universe. The sky signal is comprised of radiation from the CMB, from Galactic emission, from atmospheric emission, and from instrument sidelobes seeing the ground and man-made interference. One observes in directions of minimum galactic signal. The antarctic polar plateau provides the best site in the world for low atmospheric emission, low horizons, low man-made interference, and reasonable accessibility. The low column density of precipitable water and extreme s
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Ota, Atsuhisa. "Fluctuation-dissipation relation in cosmic microwave background." Journal of Cosmology and Astroparticle Physics 2024, no. 05 (2024): 062. http://dx.doi.org/10.1088/1475-7516/2024/05/062.

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Abstract We study the fluctuation-dissipation relation for sound waves in the cosmic microwave background (CMB), employing effective field theory (EFT) for fluctuating hydrodynamics. Treating sound waves as the linear response to thermal radiation, we establish the fluctuation-dissipation relation within a cosmological framework. While dissipation is elucidated in established linear cosmological perturbation theory, the standard Boltzmann theory overlooks the associated noise, possibly contributing to inconsistencies in Lambda Cold Dark Matter (ΛCDM) cosmology. This paper employs EFT for fluct
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Hofmann, Ralf, and Janning Meinert. "Frequency–Redshift Relation of the Cosmic Microwave Background." Astronomy 2, no. 4 (2023): 286–99. http://dx.doi.org/10.3390/astronomy2040019.

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We point out that a modified temperature–redshift relation (T-z relation) of the cosmic microwave background (CMB) cannot be deduced by any observational method that appeals to an a priori thermalisation to the CMB temperature T of the excited states in a probe environment of independently determined redshift z. For example, this applies to quasar-light absorption by a damped Lyman-alpha system due to atomic as well as ionic fine-splitting transitions or molecular rotational bands. Similarly, the thermal Sunyaev-Zel’dovich (thSZ) effect cannot be used to extract the CMB’s T-z relation. This is
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WINSTEIN, B. "CMB POLARIZATION: THE NEXT DECADE." International Journal of Modern Physics D 16, no. 12b (2007): 2563–71. http://dx.doi.org/10.1142/s0218271807011796.

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I review the exciting science that awaits cosmologists in precision measurements of the cosmic microwave background radiation, particularly its polarization. The conclusions of the Interagency Taskforce ("Weiss Panel") will also be presented. I conclude with an update based primarily on the new WMAP results from their three-year analysis.
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S., Subramanian. "Complete Solution to the Hubble tension from Cosmic Microwave Background Radiation Temperature." Journal of Emerging Technologies and Innovative Research 11, no. 9 (2024): d160—d167. https://doi.org/10.5281/zenodo.14161961.

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   This paper presents a complete solution to the current issue of Hubble tension that arises between Planck 2018 team and SHOES team. Herein we introduce a new constant named as "Dark Constant." Dark Constant is the ratio of X-Energy with the energy of Cosmic Microwave Background Radiation. While estimating X-Energy, we also show the relationship between X-Energy and Hubble's constant (Ho). In the same way we show relationship between Hubble's constant (Ho) and Cosmic Microwave Background Temperature (T). There by we derive a solution to the Hubble tension/issue, estimate the value
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Sakamoto, Hina, Kyungjin Ahn, Kiyotomo Ichiki, Hyunjin Moon, and Kenji Hasegawa. "Probing the Early History of Cosmic Reionization by Future Cosmic Microwave Background Experiments." Astrophysical Journal 930, no. 2 (2022): 140. http://dx.doi.org/10.3847/1538-4357/ac6668.

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Abstract Cosmic reionization imprints its signature on the temperature and polarization anisotropies of the cosmic microwave background (CMB). Advances in CMB telescopes have already placed a significant constraint on the history of reionization. As near-future CMB telescopes target the maximum sensitivity, or observations limited only by the cosmic variance (CV), we hereby forecast the potential of future CMB observations in constraining the history of reionization. In this study, we perform Markov Chain Monte Carlo analysis for CV-limited E-mode polarization observations such as the Lite (Li
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Rozprawy doktorskie na temat "Cosmic microwave background radiation (CMB)"

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Memari, Yasin. "Cosmological parameter estimation with QUaD CMB polarization and temperature experiment." Thesis, University of Edinburgh, 2009. http://hdl.handle.net/1842/4075.

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In this thesis we examine the theoretical origin and statistical features of the Cosmic Microwave Background radiation. We particularly focus on the CMB power spectra and cosmological parameter estimation from QUaD CMB experiment data in order to derive implications for the concordance cosmological model. In chapter 4 we present a detailed parameter estimation analysis of the combined polarization and temperature power spectra from the second and third season observations of the QUaD experiment. QUaD has for the first time detected multiple acoustic peaks in the polarization spectrum, allowing
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O'Sullivan, Creidhe Margaret Mary. "Observations of anisotropies in the CMBR at 15 GHz with the CAT." Thesis, University of Cambridge, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.389958.

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López-Caniego, Alcarria Marcos. "Detection of point sources in maps of the cosmic microwave background radiation by means of optimal filters." Doctoral thesis, Universidad de Cantabria, 2006. http://hdl.handle.net/10803/10647.

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Cuando observamos el cielo con los instrumentos más avanzados en la frecuencia de las microondas, los fotones que vemos fueron originados en regiones muy diferentes del universo. La mayoría proceden de nuestra propia galaxia (emisión difusa de sincrotrón, free-free y polvo), otros se originan en galaxias y cúmulos de galaxias muy lejanos, y, finalmente, una fracción tendrá su origen en la radiación del Big Bang, conocida como la Radiación del Fondo Cósmico de Microondas. Esta radiación está contaminada por las otras y su separación de ellas de una forma satisfactoria sigue siendo un problema a
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Kumar, Saurabh. "Radiating Macroscopic Dark Matter: Searching for Effects in Cosmic Microwave Background and Recombination History." Case Western Reserve University School of Graduate Studies / OhioLINK, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=case1606996786558263.

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Inman, Casey Ann. "A measurement of the cosmic microwave background radiation (CMBR) anisotropy at the half degree angular scale." Thesis, Massachusetts Institute of Technology, 1996. http://hdl.handle.net/1721.1/38384.

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Louis, Thibaut. "High resolution CMB physics." Thesis, University of Oxford, 2014. http://ora.ox.ac.uk/objects/uuid:b0d62439-37b8-4aa8-8d17-70141a70572a.

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This thesis presents the measurement of the cosmic microwave background (CMB) power spectrum for the Atacama Cosmology Telescope (ACT) experiment and its polarized upgrade, ACTPol. I present the tools that I have developed for constructing unbiased and nearly optimal statistical estimators. I discuss how to separate the cosmological and the astrophysical signal and how to characterize instrumental systematics. The goal of this work is to obtain accurate power spectra measurement that can be used for cosmological parameter estimation. I first present the analysis of the complete ACT data set. T
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Hancock, Stephen. "Detections of structure in the cosmic microwave background." Thesis, University of Cambridge, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.338307.

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Nazer, Mohammad Ahsan. "Cosmic microwave background anisotropies in an inhomogeneous universe." Thesis, University of Canterbury. Physics and Astronomy, 2015. http://hdl.handle.net/10092/10199.

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The timescape cosmology represents a potentially viable alternative to the standard homogeneous and isotropic Friedmann--Lemaître--Robertson--Walker (FLRW) cosmology, without the need for dark energy. This thesis first extends the previous work on the timescape cosmology to include a radiation component in the evolution equations for the timescape cosmology and tests of the timescape model are then performed against the Cosmic Microwave Background (CMB) temperature anisotropies from the Planck satellite. Although average cosmic evolution in the timescape scenario only differs substantial
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Dineen, Patrick. "Peculiar features in the cosmic microwave background radiation." Thesis, University of Nottingham, 2005. http://eprints.nottingham.ac.uk/10133/.

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In this thesis, I develop statistics capable of detecting peculiar features in current observations of the cosmic microwave background (CMB) radiation. Such tools scrutinise the very foundations of standard cosmological models. Evidence of peculiar features in the CMB may require a reassessment of these building blocks. More likely, any features may be artefacts of some non-cosmological signal. Nevertheless, whether the origin of these strange attributes is primordial or local, their discovery would be instructive. Existing statistical tools focus on the amplitude of the spherical harmonic coe
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Hervias, Caimapo Carlos. "Cosmology with CMB polarization : impact of foreground residuals." Thesis, University of Manchester, 2018. https://www.research.manchester.ac.uk/portal/en/theses/cosmology-with-cmb-polarization-impact-of-foreground-residuals(88d01ac3-65eb-43b5-a92d-fbbc28a59ff3).html.

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In this thesis, I present my work related to the characterization of diffuse Galactic foregrounds for observing the polarization of the Cosmic Microwave Background (CMB) radiation, and the impact of these foregrounds on the measurement of cosmological parameters. One of the most important future challenges for cosmology is the potential detection of polarization B-modes of the CMB. Inflation is a theory that explains the extremely early Universe, and solves several problems that were present in classical cosmology. It describes the anisotropies observed in the current Universe as primordial qu
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Książki na temat "Cosmic microwave background radiation (CMB)"

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H, Lineweaver C., North Atlantic Treaty Organization. Scientific Affairs Division., and NATO Advanced Study Institute on the Cosmological Background Radiation (1996 : Strasbourg, France), eds. The cosmic microwave background. Kluwer Academic Publishers, 1997.

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Partridge, R. B. 3 K: The cosmic microwave background radiation. Cambridge University Press, 1995.

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Angelica, De Oliveira-Costa, Tegmark Max, and Sloan Summit on Origins (1998-1999 : Princeton, N.J.), eds. Microwave foregrounds. Astronomical Society of the Pacific, 1999.

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International School of Physics "Enrico Fermi." (2004 July 6-16 Varenna, Italy). Background microwave radiation and intracluster cosmology. IOS Press, 2005.

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Giovannini, Massimo. A primer on the physics of the cosmic microwave background. World Scientific, 2008.

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Center, Goddard Space Flight, ed. Microwave anisotrophy probe, MAP. NASA's Goddard Space Flight Center, 1997.

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United States. National Aeronautics and Space Administration. Map Project Office., ed. MAP, microwave anisotropy probe. MAP Project Office, 1997.

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Laboratory, Fermi National Accelerator, and United States. National Aeronautics and Space Administration., eds. Non-gaussian microwave background fluctuations from nonlinear gravitational effects. Fermi National Accelerator Laboratory, 1991.

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Laboratory, Fermi National Accelerator, and United States. National Aeronautics and Space Administration., eds. Non-gaussian microwave background fluctuations from nonlinear gravitational effects. Fermi National Accelerator Laboratory, 1991.

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CMB Polarization Workshop (2008 : Batavia, Ill.), ed. CMB polarization workshop: Theory and foregrounds : CMBPol mission concept study : Batavia, IL, 23-26 June 2008. American Institute of Physics, 2009.

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Części książek na temat "Cosmic microwave background radiation (CMB)"

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Shiraishi, Maresuke. "Fluctuations in Cosmic Microwave Background Radiation." In Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum. Springer Japan, 2013. http://dx.doi.org/10.1007/978-4-431-54180-6_3.

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Năstase, Horaţiu. "The Cosmic Microwave Background Radiation (CMBR) Anisotropy." In Fundamental Theories of Physics. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-15077-8_7.

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Jackson Kimball, Derek F., and Dmitry Budker. "Introduction to Dark Matter." In The Search for Ultralight Bosonic Dark Matter. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-95852-7_1.

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AbstractTo set the stage for our study of ultralight bosonic dark matter (UBDM), we review the evidence for the existence of dark matter: galactic and stellar dynamics, gravitational lensing studies, measurements of the cosmic microwave background radiation (CMB), surveys of the large-scale structure of the universe, and the observed abundance of light elements. This diverse array of observational evidence informs what we know about dark matter: its universal abundance, its spatial and velocity distribution, and that its explanation involves physics beyond the Standard Model. But what we know
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Smoot, George F. "The CMB Spectrum." In The Cosmic Microwave Background. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-009-0051-6_8.

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Smoot, George F. "The CMB Anisotropy Experiments." In The Cosmic Microwave Background. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-009-0051-6_6.

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Reimberg, Paulo H. "A Path-Integral Approach to CMB." In The Cosmic Microwave Background. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-44769-8_12.

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Quartin, Miguel. "Peculiar Velocity Effects on the CMB." In The Cosmic Microwave Background. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-44769-8_7.

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Verkhodanov, O. V. "Problems of CMB Data Registration and Analysis." In The Cosmic Microwave Background. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-44769-8_4.

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Spatschek, Karl-Heinz. "Cosmic Microwave Background Radiation." In Astrophysics. Springer Berlin Heidelberg, 2024. http://dx.doi.org/10.1007/978-3-662-66648-7_13.

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Page, Lyman, and David Wilkinson. "Cosmic Microwave Background Radiation." In More Things in Heaven and Earth. Springer New York, 1999. http://dx.doi.org/10.1007/978-1-4612-1512-7_18.

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Streszczenia konferencji na temat "Cosmic microwave background radiation (CMB)"

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Leitner, Matthaeus, Jessica N. Aguilar, Zeeshan Ahmed, et al. "Project overview of the Stage-4 Cosmic Microwave Background experiment (CMB-S4)." In Ground-based and Airborne Telescopes X, edited by Heather K. Marshall, Jason Spyromilio, and Tomonori Usuda. SPIE, 2024. http://dx.doi.org/10.1117/12.3018095.

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Dekker, Gerald A., John Moreland, and Jatila van der Veen. "Developing the Planck Mission Simulation as a Multi-Platform Immersive Application." In ASME 2011 World Conference on Innovative Virtual Reality. ASMEDC, 2011. http://dx.doi.org/10.1115/winvr2011-5575.

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Planck is an international mission led by the European Space Agency with significant contribution by NASA, designed to measure the anisotropy of the Cosmic Microwave Background (CMB), the oldest radiation of the universe, with the greatest accuracy and precision of any such CMB experiment to date. The present work was completed as part of the Planck Education and Public Outreach (E/PO) effort to communicate the results of Planck science to the public. The Planck Mission Simulation is a multiplatform, interactive visualization of the mission, from launch to orbital insertion to data gathering o
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Zaldarriaga, Matias, Loris Colombo, Eiichiro Komatsu, et al. "Reionization Science with the Cosmic Microwave Background." In CMB POLARIZATION WORKSHOP: THEORY AND FOREGROUNDS: CMBPol Mission Concept Study. AIP, 2009. http://dx.doi.org/10.1063/1.3160887.

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Lasenby, Anthony N. "Observations of the cosmic microwave background and CMB interferometers." In Cosmology and particle physics. AIP, 2001. http://dx.doi.org/10.1063/1.1363508.

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Kovac, John. "The Next Generation Cosmic Microwave Background Experiment -- CMB-S4." In XXXVth URSI General Assembly and Scientific Symposium. URSI – International Union of Radio Science, 2023. http://dx.doi.org/10.46620/ursigass.2023.3597.lmxg8219.

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BASKARAN, DEEPAK, LEONID P. GRISHCHUK, and WEN ZHAO. "PRIMORDIAL GRAVITATIONAL WAVES AND COSMIC MICROWAVE BACKGROUND RADIATION." In Proceedings of the MG12 Meeting on General Relativity. WORLD SCIENTIFIC, 2012. http://dx.doi.org/10.1142/9789814374552_0034.

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DETTMANN, C. P., J. P. KEATING, and S. D. PRADO. "STOCHASTIC STABILIZATION OF THE COSMIC MICROWAVE BACKGROUND RADIATION." In Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF). World Scientific Publishing Company, 2006. http://dx.doi.org/10.1142/9789812704030_0219.

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Spergel, David N. "Extracting Cosmology from the Cosmic Microwave Background Radiation." In Proceedings of Nobel Symposium 109. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812810434_0017.

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Ganga, Ken, E. Hivon, Peter A. R. Ade, et al. "Recent results from the cosmic microwave background radiation." In International Europhysics Conference on High Energy Physics. Sissa Medialab, 2001. http://dx.doi.org/10.22323/1.007.0283.

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Barron, Darcy, Amy Bender, Ian Birdwell, et al. "Large Satellite Constellations and the Next-Generation Ground-Based Cosmic Microwave Background Survey, CMB-S4." In XXXVth URSI General Assembly and Scientific Symposium. URSI – International Union of Radio Science, 2023. http://dx.doi.org/10.46620/ursigass.2023.3501.woao9381.

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Raporty organizacyjne na temat "Cosmic microwave background radiation (CMB)"

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Mukhopadhyay, Shomeek. 3D printing of High Precision Radiation Filters for next generation Cosmic Background (CMB) studies. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1663377.

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Levin, S. M. A measurement of the low frequency spectrum of the cosmic microwave background radiation. Office of Scientific and Technical Information (OSTI), 1987. http://dx.doi.org/10.2172/6463884.

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