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W. H. Press and P. Schechter, Astrophys. J. 187
1974
Earlier work this paper cites.
N. Kaiser, ApJL 284
1984
Earlier work this paper cites.
S. D. Landy and A. S. Szalay, Astrophys. J. 412
1993
Earlier work this paper cites.
H. J. Mo and S. D. M. White, MNRAS 282
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk, and S. D. M. White, Astrophys. J. 462
1996
Earlier work this paper cites.
R. K. Sheth, H. J. Mo, and G. Tormen, MNRAS 323
2001
Earlier work this paper cites.
A. Cooray and R. Sheth, Phys. Rep. 372
2002
Earlier work this paper cites.
C. Hirata and U. Seljak, MNRAS 343
2003
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R. K. Sheth and G. Tormen, MNRAS 350
2004
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L. Gao, V. Springel, and S. D. M. White, MNRAS 363
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Earlier work this paper cites.
R. Mandelbaum, C. M. Hirata, U. Seljak, J. Guzik, N. Padmanabhan, C. Blake, M. R. Blanton, R. Lupton, and J. Brinkmann, MNRAS 361
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Earlier work this paper cites.
R. H. Wechsler, A. R. Zentner, J. S. Bullock, A. V. Kravtsov, and B. Allgood, Astrophys. J. 652
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2015

Miyatake, Hironao, More, Surhud, Takada, Masahiro et al.

We present significant evidence of halo assembly bias for SDSS redMaPPer galaxy clusters in the redshift range $[0.1, 0.33]$.

By dividing the 8,648 clusters into two subsamples based on the average member galaxy separation from the cluster center, we first show that the two subsamples have very similar halo mass of $M_{\rm 200m}\simeq 1.9\times 10^{14}~h^{-1}M_\odot$ based on the weak lensing signals at small radii $R<\sim 10~h^{-1}{\rm Mpc}$.
However, their halo bias inferred from both the large-scale weak lensing and the projected auto-correlation functions differs by a factor of $\sim$1.5, which is a signature of assembly bias.
The same bias hypothesis for the two subsamples is excluded at 2.5$\sigma$ in the weak lensing and 4.4$\sigma$ in the auto-correlation data, respectively.

W. H. Press and P. Schechter, Astrophys. J. 187
1974
Earlier work this paper cites.
N. Kaiser, ApJL 284
1984
Earlier work this paper cites.
S. D. Landy and A. S. Szalay, Astrophys. J. 412
1993
Earlier work this paper cites.
H. J. Mo and S. D. M. White, MNRAS 282
1996
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk, and S. D. M. White, Astrophys. J. 462
1996
Earlier work this paper cites.
R. K. Sheth, H. J. Mo, and G. Tormen, MNRAS 323
2001
Earlier work this paper cites.
A. Cooray and R. Sheth, Phys. Rep. 372
2002
Earlier work this paper cites.
C. Hirata and U. Seljak, MNRAS 343
2003
Earlier work this paper cites.
R. K. Sheth and G. Tormen, MNRAS 350
2004
Earlier work this paper cites.
L. Gao, V. Springel, and S. D. M. White, MNRAS 363
2005
Earlier work this paper cites.
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2005
Earlier work this paper cites.
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2006
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Cited alongside, same era.
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2006
Cited alongside, same era.
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2007
Cited alongside, same era.
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2007
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2008
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