Table 1
Intrinsic alignment amplitudes from model fits to LOWZ and MICE galaxies.
| LOWZ | MICE | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| AIA (2 pt) | ⟨Mr⟩ | ⟨z⟩ | AIA (3pt, large scales) | AIA (3 pt, all) | ⟨Mr⟩ | ⟨z⟩ | AIA (3pt, large scales) | AIA (3 pt, all) | |
| All | 4.6 ± 0.5 | −21.88 | 0.28 | 4.40 ± 0.93 | 3.99 ± 0.53 | −21.84 | 0.26 | 4.20 ± 0.59 | 3.90 ± 0.56 |
| L1 | 8.5 ± 0.9 | −22.42 | 0.28 | 8.3 ± 1.4 | 7.02 ± 0.76 | −22.43 | 0.29 | 7.4 ± 1.3 | 6.65 ± 0.72 |
| L2 | 5.0 ± 1.0 | −22.05 | 0.28 | 5.3 ± 1.0 | 4.57 ± 0.58 | −22.08 | 0.28 | 3.84 ± 0.83 | 4.39 ± 0.48 |
| L3 | 4.7 ± 1.0 | −21.86 | 0.28 | 5.01 ± 0.99 | 3.58 ± 0.45 | −21.87 | 0.27 | 3.88 ± 0.70 | 4.77 ± 0.46 |
| L4 | 2.2 ± 0.9 | −21.55 | 0.28 | 2.01 ± 0.56 | 1.88 ± 0.31 | −21.41 | 0.24 | 3.05 ± 0.51 | 2.33 ± 0.31 |
Notes. The AIA were obtained by Singh et al. (2015) from second-order statistics (second column), the third-order measurements at R > 6 h−1 Mpc (fifth and ninth column), and at all scales (sixth and tenth column). Also shown are the average absolute magnitude ⟨Mr⟩ and the average redshift ⟨z⟩ of the samples. Bold denotes values that differ more than 1σ from the second-order estimates.
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