[4]
Amanullah, R. et al., “Spectra and Hubble Space Telescope light curves of six Type Ia supernovae at 0.511
[5]
Bahcall, N. A., “Large-Scale Structure in the Universe Indicated by Galaxy Clusters”, Annual Review of Astronomy and Astrophysics, Vol. 26, 1988, pp. 631-686.
[6]
Bahcall, N. A. & Soneira, R. M., “A ~300Mpc void of rich clusters of galaxies?” The Astrophysical Journal, Vol. 262, 1982, pp. 419-423.
[7]
Bahcall, N. A. & Soneira, R. M., “A supercluster catalog”, The Astrophysical Journal, Vol. 277, 1984, pp. 27-37.
[8]
Coles, P. and Lucchin, F., “Cosmology”, John Wiley & Sons Ltd, 1995, p. 93.
[9]
Courteau S. and van den Bergh S., “The solar motion relative to the Local Group”, The Astronomical Journal, Vol. 118, 1999, pp. 337-345.
[10]
Cox, A. N., “Allen Astrophysical Quantities”, 2000, p. 661, AIPn Press-Springer.
[11]
Dirac, P. A. M., “The cosmological constants”, Vol. 139, 1937, p. 323.
[12]
Dirac, P. A. M., “A new basis for cosmology”, Proceedings of the Royal Society of London, Series A., Vol. 165, Issue 921, 1938, pp. 199-208.
[13]
Faber, S. M. et al., “Spetroscopy and photometry of elliptical galaxies. VI – Sample selection and data summary”, The Astrophysical Journal Supplement Series, Vol. 69, 1989, pp. 763-808.
[14]
Hoessel, J. C., Gunn, J. E., Thuan, T. X., “The photometric properties of bright cluster galaxies. I. Absolute magnitudes in 116 nearby Abell clusters”, The Astrophysical Journal, Vol. 241, 1980, pp. 486-492.
[15]
Hoffman, Y., Pomarède, D., Tully, R. B., Courtois, H. M., “The dipole repeller”, arXiv:1702.02483v1 8 Feb 2018, Nature Astronomy, Letters, Vol. 1, 2017, A. n. 36, pp. 1-5.
[16]
Hubble, E. P., “The Realm of the Nebulae”. New Haven: Yale University Press, 1936.
[17]
Knop, R. A. et al., “New constraints on ΩM, Ωʌ and w from an independent set of eleven high-redshifts supernovae observed with HST”, The Astrophysical Journal, Vol. 598, 2003, pp. 102-137.
[18]
Kowalski, M. et al., “Improved cosmological constraints from new, old and combined supernova data sets”, The Astrophysical Journal, Vol. 686, 2008, pp. 749-778.
[19]
Lopez-Corredoira, M. 2017a (private communication).
[20]
Lopez-Corredoira, M., “Tests and problems of the standard model in Cosmology”, arXiv:1701.08720v1 30 Jan 2017.
[21]
Lorenzi, L., “The Hubble expansion and a simple Big Bang hypothesis”, Centro Studi Astronomia - Mondovì, Contributo No. 0, 1989, DOI: 10.13140/RG.2.1.1698.8564
[22]
Lorenzi, L., “The huge void of Bahcall & Soneira as a possible great expander”, Centro Studi Astronomia - Mondovì, Contributo No. 1, 1991, www.researchgate.net/profile/Luciano_Lorenzi2
[23]
Lorenzi, L., “A cosmic diplole pointed towards the center of the huge void of Bahcall & Soneira”, Memorie della Società Astronomica Italiana, Vol. 66, No. 1, 1995, pp. 249-252.
[24]
Lorenzi, L., “Abell test of a modelled Hubble expansion from the Bahcall & Soneira void center”, Astrophysical Letters and Communications, Vol. 33, 1996, pp. 143-152.
[25]
Lorenzi, L., “The expanding Universe from the huge void center: Theory & modelling”, Memorie della Società Astronomica Italiana, Vol. 71, No. 4, 2000, pp. 1163-1181 (reprinted in MemSAIt, Vol. 74, No. 3, 2003), http://arxiv.org/abs/astro-ph/9906290 17 Jun 1999 (paper I).
[26]
Lorenzi, L., “Local solution of a spherical homogeneous and isotropic Universe radially decelerated towards the expansion center: Tests on historic data sets”, Memorie della Società Astronomica Italiana, Vol. 71, No. 4, 2000, pp. 1183-1197 (reprinted in MemSAIt, Vol. 74, No. 3, 2003), http://arxiv.org/abs/astro-ph/9906292 17 June 1999 (paper II).
[27]
Lorenzi, L., “Universe outline by the expansion center model according to Dirac”, Memorie della Società Astronomica Italiana, Vol. 74, 2003, pp. 480-481 (paper III).
[28]
Lorenzi, L., “The expansion center model as a challenge to cosmology – based on data, results and 3 historical models”, 47th Annual Meeting of the Italian Astronomical Society – Trieste 2003, http://sait.oat.ts.astro.it/MSAIS/3/POST/Lorenzi_poster.pdf (paper V).
[29]
Lorenzi, L., “Cosmic mechanics of the nearby Universe within the expansion center model with angular momentum conserved”, 52th Annual Meeting of the Italian Astronomical Society - Teramo 2008, http://terri1.oa-teramo.inaf.it/sait08/slides/I/ecmcm9b.pdf (paper VII).
[30]
Lorenzi, L., “Steps towards the expansion center cosmology”, 53th Annual Meeting of the Italian Astronomical Society - Pisa 2009, http://astro.df.unipi.it/sait09/presentazioni/AulaMagna/08AM/lorenzi.pdf (paper VIII).
[31]
Lorenzi, L., “The new wedge-shaped Hubble diagram of 398 SCP supernovae according to the expansion center model”, 54th Annual Meeting of the Italian Astronomical Society – Naples 2010, arXiv:1006.2112v3 17 Jun 2010 (paper IX).
[32]
Lorenzi, L., “A crucial dipole test of the expansion center Universe – based on high-z SCP Union & Union2 supernovae”, 55th Annual Meeting of the Italian Astronomical Society – Palermo 2011 & European Week ofAstronomy and Space Science – Rome 2012, arXiv:1105.3697v4 20 Sep 2012 (paper XV(X+XII)).
[33]
Lorenzi, L., “Dipole & absolute magnitude analysis of the SCP Union supernovae within the expansion center model”, 55th Annual Meeting of the Italian Astronomical Society – Palermo 2011 & European Week of Astronomy and Space Science – Rome 2012, arXiv:1105.3699v3 20 Sep 2012 (paper XVI(XI+XIII)).
[34]
Lorenzi, L., “A briefing on the expansion center universe”, International Journal of Astronomy, Astrophysics and Space Science, Vol. 1, No. 1, 2014, pp. 1-5 (paper XVII).
[35]
Lorenzi, L., “Big Bang as a big crush?”, International Journal of Astronomy, Astrophysics and Space Science, Vol. 1, No. 1, 2014, pp. 6-10 (paper XIV).
[36]
Lorenzi, L., “A new RFR effect at the mean redshift ≥ 1”, December 2015, DOI: 10.13140/RG.2.1.4782.2167 (paper XVIII).
[37]
Lorenzi, L., “RFR z-test on 5 historic surveys: confirming the expansion center model”, December 2015, DOI: 10.13140/RG.2.1.1767.5605 (paper XIX).
[38]
Lorenzi, L., “The cosmic dipole of the expansion center universe”, European Week of Astronomy and Space Science – La Laguna, Tenerife, June 2015, www.iac.es/galeria/martinlc/EWASS2015/176.pdf (paper XX).
[39]
Lorenzi, L., “Preliminary solution of the CMB dipole within the ECM rotating Universe: A sample test on the historic G7 survey”, European Week of Astronomy and Space Science – Athens, July 2016, DOI: 10.13140/RG.2.1.1896.2164, www.astro.noa.gr/ewass/Site/FilesRepo/131_lorenzi_2016_06_16_10_35_00.pdf (paper XXI).
[40]
Lorenzi, L., “The ECM rotating Universe with CMB dipole solved”, An informal presentation at “Institute de Astrofisica de Canarias”, La Laguna, Tenerife – December 14th, 2016, DOI: 10.13140/RG.2.2.36762.85441/3 (paper XXII).
[41]
Lorenzi, L., “COSMIC DIPOLE: A macroscopic proof of the deceleration of the Hubble flow”, January 2018, DOI: 10.13140/RG.2.2.29853.82405/1 (paper XXIII).
[42]
Lorenzi, L., “The Aaronson catalog supports a CMB origin at the mean redshift 0.0050”, January 2018, DOI: 10.13140/RG.2.2.13076.60805 (paper XXIV).
[43]
Lucey, J. R. and Carter, D., “Distances to five nearby southern galaxy clusters and the absolute motion of the Local Group”, Monthly Notices of the Royal Astronomical Society, Vol. 235, 1988, pp. 1177-1201.
[44]
Nottale, L., Pecker, J. C., Vigier, J. P. et Yourgrau, W., “La constant de Hubble mise en question”, La Recherce 68, Vol. 7, 1976, pp. 529-540.
[45]
Perlmutter, S. et al., “Measurements of Omega and Lambda from 42 High-Redshift Supernovae”, The Astrophysical Journal, Vol. 517, No. 2, 1999, pp. 565-586.
[46]
Rubin, V. C., Ford, W. K. and Rubin, J. S., “A curious distribution of radial velocities of ScI galaxies with 14.0 ≤ m ≤ 15.0”, The Astrophysical Journal, Vol. 183, 1973, L111-L115.
[47]
Sandage, A. & Tammann G. A., “Steps towards the Hubble constant. V. The Hubble constant from nearby galaxies and the regularity of the local velocity field”, The Astrophysical Journal, Vol. 196, 1975, pp. 313-328.
[48]
Sandage, A. & Tammann, G. A., “Steps towards the Hubble constant. VI. The Hubble constant determined from redshifts and magnitudes of remote ScI galaxies: The value of q0”, The Astrophysical Journal, Vol. 197, 1975, pp. 265-280.
[49]
Suzuki, N. et al., “The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z > 1 and Building an Early Type-Hosted Supernova Sample”, arXiv:1105.3470v1 17 May 2011. The Astrophysical Journal, Vol. 746, 2012, pp. 85-109.
[50]
Vaucouleurs, G., in “Galaxies and the Universe”, Vol. IX of Stars and Stellar Systems, 1975, p. 598, The University of Chicago Press.