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2017
The kinematic dipole in galaxy redshift surveys Maartens, Roy, Clarkson, Chris, Chen, Song
Understand In the concordance model of the Universe, the matter distribution - as observed in galaxy number counts or the intensity of line emission (such as the 21cm line of neutral hydrogen) - should have a kinematic dipole due to the Sun's motion relative to the CMB rest-frame.
This dipole should be aligned with the kinematic dipole in the CMB temperature. Accurate measurement of the direction of the matter dipole will become possible with future galaxy surveys, and this will be a critical test of the foundations of the concordance model. The amplitude of the matter dipole is also a potential cosmological probe. The kinematic dipole in galaxy redshift surveys · Around
Built on G. F. R. Ellis and J. E. Baldwin, “On the Expected Anisotropy of Radio Source Counts,” Mon. Not. Roy. Astron. Soc. 206
1984
Earlier work this paper cites.
C. Bonvin, R. Durrer and M. Kunz, “The dipole of the luminosity distance: a direct measure of H(z),” Phys. Rev. Lett. 96
Original
2006
Earlier work this paper cites.
A. Challinor and A. Lewis, “The linear power spectrum of observed source number counts,” Phys. Rev. D 84
Original
2011
Earlier work this paper cites.
C. Gibelyou and D. Huterer, “Dipoles in the Sky,” Mon. Not. Roy. Astron. Soc. 427
Original
2012
Earlier work this paper cites.
D. Jeong, F. Schmidt and C. M. Hirata, “Large-scale clustering of galaxies in general relativity,” Phys. Rev. D 85
Original
2012
Earlier work this paper cites.
C. Bonvin, R. Durrer and M. A. Gasparini, “Fluctuations of the luminosity distance,” Phys. Rev. D 73
2012
Earlier work this paper cites.
A. Hall, C. Bonvin and A. Challinor, “Testing General Relativity with 21-cm intensity mapping,” Phys. Rev. D 87
Original
2013
Earlier work this paper cites.
Similar N. Aghanim et al
Original
2014
Cited alongside, same era.
D. J. Schwarz et al
Original
2015
Cited alongside, same era.
M. Yoon and D. Huterer, “Kinematic dipole detection with galaxy surveys: forecasts and requirements,” Astrophys. J. 813
Original
2015
Cited alongside, same era.
D. Alonso, P. Bull, P. G. Ferreira, R. Maartens and M. Santos, “Ultra large-scale cosmology in next-generation experiments with single tracers,” Astrophys. J. 814
Original
2015
Cited alongside, same era.
R. Maartens et al
Original
2015
Then P. Tiwari and A. Nusser, “Revisiting the NVSS number count dipole,” JCAP 1603
Original
2016
Later among the works it cites.
S. Ghosh, P. Jain, G. Kashyap, R. Kothari, S. Nadkarni-Ghosh and P. Tiwari, “Probing statistical isotropy of cosmological radio sources using SKA,” J. Astrophys. Astron. 37
Original
2016
Later among the works it cites.
C. A. P. Bengaly, A. Bernui, J. S. Alcaniz, H. S. Xavier and C. P. Novaes, “Is there evidence for anomalous dipole anisotropy in the large-scale structure?,” Mon. Not. Roy. Astron. Soc. 464
Original
2017
Closest in time.
J. Colin, R. Mohayaee, M. Rameez and S. Sarkar, “High redshift radio galaxies and divergence from the CMB dipole,” Mon. Not. Roy. Astron. Soc. 471
Original
2017
Closest in time.
A. Slosar, “Dipole of the Epoch of Reionization 21-cm signal,” Phys. Rev. Lett. 118
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