Built on

P. Zhang, M. Liguori, R. Bean, and S. Dodelson, Phys.Rev.Lett. 99
Original
1932
Earlier work this paper cites.
C. Deffayet, S. Deser, and G. Esposito-Farese, Phys.Rev. D80
Original
1967
Earlier work this paper cites.
J. Merten, M. Cacciato, M. Meneghetti, C. Mignone, and M. Bartelmann, Astron.Astrophys. 500
Original
1967
Earlier work this paper cites.
A. Vainshtein, Phys. Lett. B 39
1972
Earlier work this paper cites.
G. W. Horndeski, Int.J.Theor.Phys. 10
1974
Earlier work this paper cites.
M. Bartelmann, Astron.Astrophys. 313
1996
Earlier work this paper cites.
J. Kneib, R. Ellis, I. Smail, W. Couch, and R. Sharples, Astrophys.J. 471
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk, and S. D. White, Astrophys.J. 490
1997
Earlier work this paper cites.
C. Oaxaca Wright and T. G. Brainerd, ArXiv Astrophysics e-prints(Aug. 1999), astro-ph/9908213
1999
Earlier work this paper cites.
G. Dvali, G. Gabadadze, and M. Porrati, Phys.Lett. B485
2000
Earlier work this paper cites.
M. Bartelmann and P. Schneider, Phys.Rept. 340
2001
Earlier work this paper cites.
J. G. Williams, S. G. Turyshev, and D. H. Boggs, Phys.Rev.Lett. 93
2004
Earlier work this paper cites.
T. J. Broadhurst et al. (ACS Collaboration), Astrophys.J. 621
2005
Earlier work this paper cites.
G. P. Smith, J.-P. Kneib, I. Smail, P. Mazzotta, H. Ebeling, et al. , Mon.Not.Roy.Astron.Soc. 359
2005
Earlier work this paper cites.
A. Halkola, S. Seitz, and M. Pannella, Mon.Not.Roy.Astron.Soc. 372
2006
Earlier work this paper cites.
S. Deser and R. Woodard, Phys.Rev.Lett. 99
Original
2007
Earlier work this paper cites.
E. Jullo, J.-P. Kneib, M. Limousin, A. Eliasdottir, P. Marshall, et al. , New J.Phys. 9
Original
2007
Earlier work this paper cites.
A. F. Neto, L. Gao, P. Bett, S. Cole, J. F. Navarro, et al. , Mon.Not.Roy.Astron.Soc. 381
Original
2007
Earlier work this paper cites.
B. Jain and P. Zhang, Phys.Rev. D78
Original
2008
Earlier work this paper cites.
S. Nojiri and S. D. Odintsov, Phys.Lett. B659
Original
2008
Earlier work this paper cites.
A. R. Duffy, J. Schaye, S. T. Kay, and C. Dalla Vecchia, Mon.Not.Roy.Astron.Soc. 390
Original
2008
Earlier work this paper cites.
T. L. Smith, ArXiv e-prints(Jul. 2009), arXiv:0907.4829 [astro-ph.CO]
Original
2009
Earlier work this paper cites.
F. Schmidt, A. Vikhlinin, and W. Hu, PRD 80
Original
2009
Earlier work this paper cites.
A. Nicolis, R. Rattazzi, and E. Trincherini, Phys. Rev. D 79
2009
Earlier work this paper cites.
C. Deffayet, G. Esposito-Farèse, and A. Vikman, Phys. Rev. D 79
2009
Earlier work this paper cites.
G. Gabadadze, Phys.Lett. B681
Original
2009
Earlier work this paper cites.
E. Babichev, C. Deffayet, and R. Ziour, Int.J.Mod.Phys. D18
Original
2009
Earlier work this paper cites.
G.-B. Zhao, L. Pogosian, A. Silvestri, and J. Zylberberg, Phys.Rev. D79
Original
2009
Earlier work this paper cites.
S. Capozziello, E. Elizalde, S. Nojiri, and S. D. Odintsov, Phys.Lett. B671
Original
2009
Earlier work this paper cites.
N. Koshelev, Grav.Cosmol. 15
Original
2009
Earlier work this paper cites.
A. Zitrin, T. Broadhurst, K. Umetsu, D. Coe, N. Benítez, B. Ascaso, L. Bradley, H. Ford, J. Jee, E. Medezinski, Y. Rephaeli, and W. Zheng, MNRAS 396
Original
2009
Earlier work this paper cites.
T. P. Sotiriou and V. Faraoni, Rev.Mod.Phys. 82
Original
2010
Earlier work this paper cites.
F. Schmidt, PRD 81
Original
2010
Earlier work this paper cites.
J. Schwab, A. S. Bolton, and S. A. Rappaport, APJ 708
Original
2010
Earlier work this paper cites.
C. de Rham, Phys.Lett. B688
Original
2010
Earlier work this paper cites.
C. de Rham and G. Gabadadze, Phys.Lett. B693
Original
2010
Earlier work this paper cites.
C. de Rham and G. Gabadadze, Phys.Rev. D82
Original
2010
Earlier work this paper cites.
K. Umetsu, ArXiv e-prints(Feb. 2010), arXiv:1002.3952 [astro-ph.CO]
Original
2010
Earlier work this paper cites.
M. Bartelmann, Classical and Quantum Gravity 27
Original
2010
Earlier work this paper cites.
T. S. Koivisto, AIP Conf.Proc. 1206
Original
2010
Earlier work this paper cites.
M. Oguri, PASJ 62
Original
2010
Earlier work this paper cites.
C. de Rham, G. Gabadadze, and A. J. Tolley, Phys.Rev.Lett. 106
Original
2011
Earlier work this paper cites.

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Original
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Cited alongside, same era.
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Later among the works it cites.
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Later among the works it cites.

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2015

Galaxy cluster lensing masses in modified lensing potentials

Barreira, Alexandre, Li, Baojiu, Jennings, Elise et al.

Understand

We determine the concentration-mass relation of 19 X-ray selected galaxy clusters from the CLASH survey in theories of gravity that directly modify the lensing potential.

We model the clusters as NFW haloes and fit their lensing signal, in the Cubic Galileon and Nonlocal gravity models, to the lensing convergence profiles of the clusters.
We discuss a number of important issues that need to be taken into account, associated with the use of nonparametric and parametric lensing methods, as well as assumptions about the background cosmology.
Our results show that the concentration and mass estimates in the modified gravity models are, within the errorbars, the same as in $\Lambda$CDM.