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Table 3.

Goodness of fit of our models given the DES Y3 data vector.

Model χ2/d.o.f.(Nfree) χ2/d.o.f.(Neff)

DES scale cuts All scales DES scale cuts All scales
NLA BCM7 (fiducial) 226.98/204 = 1.11 414.14/377 = 1.1 226.98/224.69 = 1.01 414.14/397.16 = 1.04
NLA GrO 227.98/211 = 1.08 416.46/384 = 1.08 227.98/224.63 = 1.01 416.46/397.37 = 1.05
NLA BCM1 227.58/210 = 1.08 414.23/383 = 1.08 227.58/224.61 = 1.01 414.23/397.11 = 1.04
NLA BCM-extreme 227.24/211 = 1.08 419.03/384 = 1.09 227.24/224.6 = 1.01 419.03/397.77 = 1.05

TATT BCM7 226.28/201 = 1.13 411.22/374 = 1.1 226.28/224.14 = 1.01 411.22/396.21 = 1.04
TATT GrO 226.37/208 = 1.09 410.66/381 = 1.08 226.37/224.28 = 1.01 410.66/396.16 = 1.04
TATT BCM1 225.28/207 = 1.09 407.65/380 = 1.07 225.28/223.87 = 1.01 407.65/396.35 = 1.03
TATT BCM-extreme 227.2/208 = 1.09 408.69/381 = 1.07 227.2/223.77 = 1.02 408.69/396.37 = 1.03

Notes. We calculated the d.o.f. by subtracting the number of parameters Nθ from the number of data points (N𝒟). We used as Nθ either the number of free parameters Nfree or the number of effective parameters Neff as defined in Raveri & Hu (2019). We explored different models, with NLA or TATT intrinsic alignment, gravity-only, or applying a baryonification with one or seven free parameters (BCM1 and BCM7, respectively). We also included a model with an extreme implementation of AGN feedback.

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