ArXiv e-prints, 2014. ,
Looking for a varying ?? in the cosmic microwave background, Physical Review D, vol.62, issue.12, p.123508, 2000. ,
DOI : 10.1103/PhysRevD.62.123508
Baryonic Features in the Matter Transfer Function, The Astrophysical Journal, vol.496, issue.2, p.605, 1998. ,
DOI : 10.1086/305424
Possible constraints on the time variation of the fine structure constant from cosmic microwave background data, Physical Review D, vol.60, issue.2, p.23515, 1999. ,
DOI : 10.1103/PhysRevD.60.023515
The physics of microwave background anisotropies, Nature, vol.386, issue.6620, p.37, 1997. ,
DOI : 10.1038/386037a0
Cosmic Microwave Background Observables and Their Cosmological Implications, The Astrophysical Journal, vol.549, issue.2, p.669, 2001. ,
DOI : 10.1086/319449
TOWARD A NEW GEOMETRIC DISTANCE TO THE ACTIVE GALAXY NGC 4258. III. FINAL RESULTS AND THE HUBBLE CONSTANT, The Astrophysical Journal, vol.775, issue.1, p.13, 2013. ,
DOI : 10.1088/0004-637X/775/1/13
CMB constraints on the simultaneous variation of the fine structure constant and the electron mass, Physical Review D, vol.74, issue.2, p.23515, 2006. ,
DOI : 10.1103/PhysRevD.74.023515
Constraining variations in the fine-structure constant with the cosmic microwave background, Physical Review D, vol.60, issue.2, p.23516, 1999. ,
DOI : 10.1103/PhysRevD.60.023516
from WMAP 7-year data, Astronomy and Astrophysics, vol.517, issue.440, pp.62-2077, 2010. ,
DOI : 10.1051/0004-6361/201014215
A&A, 571, A16 Planck Collaboration XIII. 2015a, A&A, submitted [arXiv:1502, A&A Am. J. Phys, vol.580, issue.71, pp.22-1043, 2003. ,
ArXiv e-prints, 2013. ,
Measuring ?? in the early Universe: cosmic microwave background polarization, re-ionization and the Fisher matrix analysis, Monthly Notices of the Royal Astronomical Society, vol.352, issue.1, p.20, 2004. ,
DOI : 10.1111/j.1365-2966.2004.07832.x
WMAP 5-year constraints on time variation of ?? and <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:msub><mml:mi>m</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:math> in a detailed recombination scenario, Physics Letters B, vol.669, issue.3-4, p.212, 2008. ,
DOI : 10.1016/j.physletb.2008.09.051
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function, Monthly Notices of the Royal Astronomical Society, vol.434, issue.2, p.1792, 2013. ,
DOI : 10.1093/mnras/stt1143
How Exactly Did the Universe Become Neutral?, The Astrophysical Journal Supplement Series, vol.128, issue.2, p.407, 2000. ,
DOI : 10.1086/313388
Progress in Lunar Laser Ranging Tests of Relativistic Gravity, Physical Review Letters, vol.93, issue.26, p.261101, 2004. ,
DOI : 10.1103/PhysRevLett.93.261101