Table 1.
PAUS W3 (0.1 < zphot. < 0.8) and GAMA sample characteristics.
Sample | ⟨z⟩ | ⟨L/Lpiv⟩ | Nshapes | Npositions |
---|---|---|---|---|
PAUS W3 red | 0.48 | 0.48 | 43725 | 43824 |
PAUS W3 red (Qz50) | 0.47 | 0.62 | 27427 | 27460 |
PAUS W3 blue | 0.47 | 0.22 | 145100 | 145514 |
PAUS W3 blue (Qz50) | 0.44 | 0.24 | 66991 | 67209 |
GAMA red | 0.25 | 0.77 | 69920 | 78165 |
GAMA blue | 0.24 | 0.52 | 93156 | 89064 |
Notes. The table lists: mean redshifts ⟨z⟩, mean r-band luminosities relative to the pivot Lpiv = L(Mr = −22), the number of galaxies used as tracers of the intrinsic shear field Nshapes, and the number of density field tracer galaxies Npositions – we do not apply colour-selections to positional tracers for our intrinsic alignment correlations, using the full sample to trace the density field (see Sect. 4.2). Samples labelled ‘Qz50’ are defined from the best 50% of photo-z in all of PAUS W3 (i.e. selected on photo-z quality prior to the colour-cut). GAMA galaxies are those analysed by Johnston et al. (2019), who limited the blue density sample objects to Mr ≤ −18.9, causing the blue sample to have more shapes than density tracers.
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