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Table 5.
Setups for further MCMC test runs.
| No. | Setup | Difference w.r.t. fiducial setup |
|---|---|---|
| 1 | sDIR | sDIR (smoothed version of DIR) n(z) |
| 2 | DIR-w/o-COSMOS | DIR n(z) based on all spec-z except COSMOS |
| 3 | DIR-w/o-COSMOS&VVDS | DIR n(z) based on all spec-z except COSMOS and VVDS |
| 4 | DIR-w/o-VVDS | DIR n(z) based on all spec-z except VVDS |
| 5 | DIR-w/o-DEEP2 | DIR n(z) based on all spec-z except DEEP2 |
| 6 | DIR-C15 | DIR n(z) based on the COSMOS-2015 photo-z |
| 7 | CC-fit | n(z) from GMM fit to small-scale clustering-z (CC; Appendix C.2) |
| 8 | CC-shift | DIR n(z) shifted to best fit CC measurements |
| 9 | OQE-shift | DIR n(z) shifted to best fit large-scale clustering-z (OQE; Appendix C.3) |
| 10 | no-deltaz | Redshift uncertainty switched off, i.e. δzi = 0 |
| 11 | IA-Gauss | Informative Gaussian prior on AIA |
| 12 | IA-linear-PS | Using the linear power spectrum in Eq. (9) |
| 13 | IA-z-evolution | Allowing for redshift evolution in the IA model |
| 14 | No-baryons | Baryon feedback switched off, i.e. B = 3.13 |
| 15 | Wide-baryons | Wide prior on baryon feedback, B ∈ [1.4, 4.8], η0 ∈ [0.4, 0.9] |
| 16 | No-systematics | No marginalisation over nuisance parameters, no error on m |
| 17 | No-systematics_merr | Same as 16 but including a σm = 0.02 uncertainty in the m-bias |
| 18 | All-xip | All scales  used for ξ+ |
| 19 | nu0 | Massless neutrinos |
| 20 | nu0p26 | One massive neutrino with m = 0.26 eV and two massless neutrinos |
| 21 | No-bin1 | Using tomographic bins 2, 3, 4, and 5 only |
| 22 | No-bin2 | Using tomographic bins 1, 3, 4, and 5 only |
| 23 | No-bin3 | Using tomographic bins 1, 2, 4, and 5 only |
| 24 | No-bin4 | Using tomographic bins 1, 2, 3, and 5 only |
| 25 | No-bin5 | Using tomographic bins 1, 2, 3, and 4 only |
| 26 | iterative-covariance | analytical covariance based on the best-fit fiducial cosmology |
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