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References:
[1] Alpher, R. A., Bethe, H., Gamow, G.: The Origin of Chemical Elements. Physical Review, Vol. 73 (1948), Issue 7, 803–804.
[2] Bennett, C. L.: Four-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results. Astrophysical Journal Letters, Vol. 464 (1996), L1.
[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.
[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.
[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.
[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.
[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.
[8] Fixsen, D. J.: The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set. Astrophysical Journal, Vol. 473 (1996), 576.
[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.
[10] Hinshaw, G.: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis. eprint arXiv:astro-ph/0603451 (2006).
[11] Hoyle, F., Tayler, R. J.: The Mystery of the Cosmic Helium Abundance. Nature, Vol. 203 (1964), 1108.
[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).
[13] Kogut, A.: Microwave Emission at High Galactic Latitudes in the Four-Year DMR Sky Maps. Astrophysical Journal Letters, Vol. 464 (1996), L5.
[14] Kovac, J. M.: Detection of Polarization in the Cosmic Microwave Background using DASI. Nature, Vol. 420 (2002), Issue 6917, 772–787.
[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.
[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.
[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.
[18] McKellar, A.: Wave Lenghts of the CH Band Lines. Publications of the Astronomical Society of the Pacific, Vol. 52 (1940), No. 309, 312.
[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.
[20] Peebles, P. J. E.: The Blackbody Radiation Content of the Universe and the Fomation of Galaxies. Astrophysical Journal, Vol. 142 (1965), 1317.
[21] Penzias, A. A., Wilson, R. W.: A Measurement of Excess Antenna Temperature at 4080 Mc/s. Astrophysical Journal, Vol. 142 (1965), 419–421.
[22] Penzias, A. A., Wilson, R. W.: Isotropy of Cosmic Background Radiation at 4080 Megahertz. Science, Vol. 156 (1967), Issue 3778, 1100–1101.
[23] Readhead, A. C. S.: Extended Mosaic Observations with the Cosmic Background Imager. Astrophysical Journal, Vol. 609 (2004), Issue 2, 498–512.
[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.
[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.
[26] Smoot, G. F.: Large-Angular-Scale Anisotropy in the Cosmic Background Radiation. D. Reidel Publishing Co. (1980), 321–328.
[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.
[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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