PACS numbers

98.80.Es Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc)
  1. A.V. Toporensky, S.B. Popov “The Hubble flow: an observer’s perspective57 708–713 (2014)
    98.62.Py, 98.80.−k, 98.80.Es (all)
  2. V.G. Kurt, N.N. Shakhvorostova “CMB spectral distortions during the recombination of the primeval plasma in the early Universe57 389–406 (2014)
    52.40.Db, 98.70.Vc, 98.80.Es (all)
  3. B.P. Schmidt “The path to measuring an accelerating Universe56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  4. S. Perlmutter “Measuring the acceleration of the cosmic expansion using supernovae56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  5. O.V. Verkhodanov, A.G. Doroshkevich “Sky pixelization for the analysis of extended emission56 801–812 (2013)
    95.75.−z, 95.85.Bh, 98.80.−k, 98.80.Es (all)
  6. Astrophysics and astronomy (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 26 January 2011)54 1061–1084 (2011)
    01.10.Fv, 04.20.−q, 11.27.+d, 89.60.Gg, 96.30.Cw, 96.30.Ys, 97.60.Jd, 97.60.Lf, 97.80.−d, 97.82.−j, 98.62.Sb, 98.80.Es (all)
  7. O.S. Sazhina, M.V. Sazhin et alSearch for cosmic strings using optical and radio astronomy methods54 1072–1077 (2011)
    11.27.+d, 98.62.Sb, 98.80.Es (all)
  8. D.P. Skulachev “Cosmic microwave background anisotropy data correlation in WMAP and Relikt-1 experiments53 373–376 (2010)
    95.55.−n, 95.75.−z, 98.80.Es (all)
  9. I.D. Novikov “’Big Bang’ echo (cosmic microwave background observations)44 817–818 (2001)
    95.85.Bh, 98.80.Cq, 98.80.Es (all)
  10. I.D. Novikov, I.D. Karachentsev et alScientific session of the Division of General Physics and Astronomy of the Russian Academy of Sciences (28 February, 2001)44 817–818 (2001)
    01.10.Fv, 95.85.Bh, 98.80.Cq, 98.80.Es, 95.35.+d, 98.65.−r, 04.70.-S, 97.80.Jp, 98.35.Jk, 47.37.+q, 97.60.Gb, 97.60.Jd (all)
  11. A.D. Sakharov “Violation of CP in variance, C asymmetry, and baryon asymmetry of the universe34 (5) 392–393 (1991)
    98.80.Cq, 98.80.Es, 11.30.Er, 14.65.−q, 95.30.Cq (all)
  12. A.D. Sakharov “Spectral density of eigenvalues of the wave equation and vacuum polarization34 (5) 395–400 (1991)
    04.20.Fy, 04.50.+h, 98.80.Es (all)
  13. A.D. Sakharov “Baryon asymmetry of the universe34 (5) 417–421 (1991)
    11.30.Er, 98.80.Cq, 12.10.Dm, 98.80.Es (all)
  14. Ya.A. Smorodinskii “The early universe32 943–943 (1989)
    01.30.Vv, 98.80.Es, 98.80.Cq, 95.35.+d (all)
  15. L.P. Grishchuk “Gravitational-wave astronomy31 940–954 (1988)
    04.30.Db, 97.60.Gb, 97.80.Gm, 97.30.Qt, 98.80.Es, 04.60.−m (all)
  16. N.S. Kardashev, V.N. Lukash, I.D. Novikov “Observational cosmology and cosmological models30 82–82 (1987)
    98.80.Es, 98.80.Cq, 98.65.Dx (all)
  17. B.V. Vainer, Yu.A. Shchekinov “The origin of deuterium28 414–431 (1985)
    98.80.Es, 98.80.Ft, 98.80.Bp, 98.80.Cq, 97.10.Cv (all)
  18. Yu.N. Efremov, S.B. Novikov, P.V. Shcheglov “Prospects for development of ground-based optical astronomy18 151–160 (1975)
    98.80.Es, 98.54.Aj, 97.60.Gb, 95.30.Sf, 98.62.Js, 95.55.Cs (all)
  19. A.M. Gal’per, V.G. Kirillov-Ugryumov, B.I. Luchkov “Observational gamma astronomy17 186–198 (1974)
    98.70.Rz, 98.70.Sa, 98.80.Es, 97.60.Gb (all)
  20. P.V. Shcheglov “Astroclimatic Conditions in Central Asia and Kazakhstan14 792–794 (1972)
    97.30.Qt, 97.60.Bw, 95.75.De, 97.10.Ri, 98.80.Es, 97.10.Cv (all)
  21. Ya.M. Kramarovskii, V.P. Chechev “Does the charge of the electron vary with the age of the universe?13 628–631 (1971)
    98.80.Es, 98.80.Jk, 98.80.Bp, 95.30.Sf, 98.80.Cq (all)
  22. Ya.B. Zel’dovich “The cosmological constant and the theory of elementary particles11 381–393 (1968)
    98.80.Es, 98.80.Cq, 95.30.Cq, 98.54.Aj (all)
  23. Ya.B. Zel’dovich “The "hot" model of the Universe9 602–617 (1967)
    98.80.Cq, 95.30.Qd, 98.80.Es, 98.62.Ra (all)
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