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Title: Nobelova cena za fyziku za rok 2006 (Czech)
Title: Nobel Prize for physics in 2006 (English)
Author: Pitňa, Alexander
Language: Czech
Journal: Pokroky matematiky, fyziky a astronomie
ISSN: 0032-2423
Volume: 52
Issue: 1
Year: 2007
Pages: 1-16
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Category: physics
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Date available: 2010-12-11T21:55:23Z
Last updated: 2012-08-26
Stable URL: http://hdl.handle.net/10338.dmlcz/141336
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Reference: [1] Alpher, R. A., Bethe, H., Gamow, G.: The Origin of Chemical Elements.Physical Review, Vol. 73 (1948), Issue 7, 803–804.
Reference: [2] Bennett, C. L.: Four-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results.Astrophysical Journal Letters, Vol. 464 (1996), L1.
Reference: [3] Bennett, C. L.: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basics Results.Astrophysical Journal Supplement Series, Vol. 148 (2003), Issue 1, 1–27.
Reference: [4] Carpenter, R. L., Gulkis, S., Sato, T.: Search for Small-Scale Anisotropy in the 2.7$^\circ $ K Background Radiation at a Wavelenght of 3.56 Centimetres.Astrophysical Journal, Vol. 182 (1973), p. L61.
Reference: [5] Cheng, E. S., Saulson, P. R., Wilkinson, D. T., Corey, B. E.: Large-Scale Anisotropy in the 2.7$^\circ $ K Radiation.Astrophysical Journal, Part 2, Vol. 232 (1979), p. L139–L143.
Reference: [6] Dicke, R. H., Peebles, P. J. E., Roll, P. G., Wilkinson, D. T.: Cosmic Black-Body Radiation.Astrophysical Journal, Vol. 142 (1965), 414–419.
Reference: [7] Fixsen, D. J.: Cosmic Microwave Background Dipole Spectrum Measured by the COBE FIRAS Instrument.Astrophysical Journal, Part 1, Vol. 420, no. 2 (1994), 445–449.
Reference: [8] Fixsen, D. J.: The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set.Astrophysical Journal, Vol. 473 (1996), 576.
Reference: [9] Field, G. B., Hitchcock, J. L.: The Radiation Temperature of Space at $\lambda $ 2.6 MM and Excitation of Interstellar CN.Astrophysical Journal, Vol. 146 (1996), 1.
Reference: [10] Hinshaw, G.: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis.eprint arXiv:astro-ph/0603451 (2006).
Reference: [11] Hoyle, F., Tayler, R. J.: The Mystery of the Cosmic Helium Abundance.Nature, Vol. 203 (1964), 1108.
Reference: [12] Jones, W. C.: A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERanG.eprint arXiv:astro-ph/0507494 (2005).
Reference: [13] Kogut, A.: Microwave Emission at High Galactic Latitudes in the Four-Year DMR Sky Maps.Astrophysical Journal Letters, Vol. 464 (1996), L5.
Reference: [14] Kovac, J. M.: Detection of Polarization in the Cosmic Microwave Background using DASI.Nature, Vol. 420 (2002), Issue 6917, 772–787.
Reference: [15] Lubin, P. M., Smoot, G. F.: Search for Linear Polarization of the Cosmic Background Radiation.Physical Review Letters, Vol. 42 (1979), Issue 2, 129–132.
Reference: [16] Mason, B. S.: The Anisotropy of the Microwave Background to ${l=3500}$: Deep Field Observations with the Cosmic Background Imager.Astrophysical Journal, Vol. 591 (2003), Issue 2, 540–555.
Reference: [17] Mather, J. C., Fixsen, D. J., Shafer, R. A., Mosier, C., Wilkinson, D. T.: Calibrator Design for the COBE Far-Infrared Absolute Spectrophotometer (FIRAS).Astronomical Journal, Vol. 512 (1999), Issue 2, 511–520.
Reference: [18] McKellar, A.: Wave Lenghts of the CH Band Lines.Publications of the Astronomical Society of the Pacific, Vol. 52 (1940), No. 309, 312.
Reference: [19] Pearson, T. J.: The Anisotropy of the Microwave Background to ${l=3500}$: Mosaic Observations with the Cosmic Background Imager.Astrophysical Journal, Vol. 591 (2003), Issue 2, 556–574.
Reference: [20] Peebles, P. J. E.: The Blackbody Radiation Content of the Universe and the Fomation of Galaxies.Astrophysical Journal, Vol. 142 (1965), 1317.
Reference: [21] Penzias, A. A., Wilson, R. W.: A Measurement of Excess Antenna Temperature at 4080 Mc/s.Astrophysical Journal, Vol. 142 (1965), 419–421.
Reference: [22] Penzias, A. A., Wilson, R. W.: Isotropy of Cosmic Background Radiation at 4080 Megahertz.Science, Vol. 156 (1967), Issue 3778, 1100–1101.
Reference: [23] Readhead, A. C. S.: Extended Mosaic Observations with the Cosmic Background Imager.Astrophysical Journal, Vol. 609 (2004), Issue 2, 498–512.
Reference: [24] Ruhl, J. E.: Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the Cosmic Microwave Background from Two New Analyses of BOOMERanG Observations.Astrophysical Journal, Vol. 599 (2003), Issue 2, 786–805.
Reference: [25] Smoot, G. F., Gorenstein, M. V., Muller, R. A.: Detection of Anisotropy in the Cosmic Blackbody Radiation.Physical Review Letters, Vol. 39 (1977), 898–901.
Reference: [26] Smoot, G. F.: Large-Angular-Scale Anisotropy in the Cosmic Background Radiation.D. Reidel Publishing Co. (1980), 321–328.
Reference: [27] Smoot, G. F.: Statistics and topology of the COBE differential microwave radiometer first-year sky maps.Astrophysical Journal, Part 1, Vol. 437 (1994), no. 1, 1–11.
Reference: [28] Thaddeus, P.: The Short-Wavelenght Spectrum of the Microwave Background.Annual Review of Astronomy and Astrophysics, Vol. 10 (1972), 305.
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