Cosmological and nuisance parameters and their priors used in this analysis.
Parameter . | Prior . |
---|---|
Cosmology | |
Ωm | flat (0.1, 0.9) |
As | flat (5 × 10−10, 5 × 10−9) |
ns | flat (0.87, 1.07) |
Ωb | flat (0.03, 0.07) |
h | flat (0.55, 0.90) |
Ωνh2 | flat(5 × 10−4, 10−2) |
Lens galaxy bias | |
bi(i = 1, 5) | flat (0.8, 3.0) |
Intrinsic alignment | |
AIA | flat (−5, 5) |
ηIA | flat (−5, 5) |
Lens photo-z shift (red sequence) | |
|$\Delta z^1_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^2_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^3_{\rm l}$| | Gauss (0.0, 0.006) |
|$\Delta z^4_{\rm l}$| | Gauss (0.0, 0.01) |
|$\Delta z^5_{\rm l}$| | Gauss (0.0, 0.01) |
Source photo-z shift | |
|$\Delta z^1_{\rm s}$| | Gauss (0.0, 0.016) |
|$\Delta z^2_{\rm s}$| | Gauss (0.0, 0.013) |
|$\Delta z^3_{\rm s}$| | Gauss (0.0, 0.011) |
|$\Delta z^4_{\rm s}$| | Gauss (0.0, 0.022) |
Shear calibration | |
mi(i = 1, 4) | Gauss (0.0, 0.023) |
Parameter . | Prior . |
---|---|
Cosmology | |
Ωm | flat (0.1, 0.9) |
As | flat (5 × 10−10, 5 × 10−9) |
ns | flat (0.87, 1.07) |
Ωb | flat (0.03, 0.07) |
h | flat (0.55, 0.90) |
Ωνh2 | flat(5 × 10−4, 10−2) |
Lens galaxy bias | |
bi(i = 1, 5) | flat (0.8, 3.0) |
Intrinsic alignment | |
AIA | flat (−5, 5) |
ηIA | flat (−5, 5) |
Lens photo-z shift (red sequence) | |
|$\Delta z^1_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^2_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^3_{\rm l}$| | Gauss (0.0, 0.006) |
|$\Delta z^4_{\rm l}$| | Gauss (0.0, 0.01) |
|$\Delta z^5_{\rm l}$| | Gauss (0.0, 0.01) |
Source photo-z shift | |
|$\Delta z^1_{\rm s}$| | Gauss (0.0, 0.016) |
|$\Delta z^2_{\rm s}$| | Gauss (0.0, 0.013) |
|$\Delta z^3_{\rm s}$| | Gauss (0.0, 0.011) |
|$\Delta z^4_{\rm s}$| | Gauss (0.0, 0.022) |
Shear calibration | |
mi(i = 1, 4) | Gauss (0.0, 0.023) |
Cosmological and nuisance parameters and their priors used in this analysis.
Parameter . | Prior . |
---|---|
Cosmology | |
Ωm | flat (0.1, 0.9) |
As | flat (5 × 10−10, 5 × 10−9) |
ns | flat (0.87, 1.07) |
Ωb | flat (0.03, 0.07) |
h | flat (0.55, 0.90) |
Ωνh2 | flat(5 × 10−4, 10−2) |
Lens galaxy bias | |
bi(i = 1, 5) | flat (0.8, 3.0) |
Intrinsic alignment | |
AIA | flat (−5, 5) |
ηIA | flat (−5, 5) |
Lens photo-z shift (red sequence) | |
|$\Delta z^1_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^2_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^3_{\rm l}$| | Gauss (0.0, 0.006) |
|$\Delta z^4_{\rm l}$| | Gauss (0.0, 0.01) |
|$\Delta z^5_{\rm l}$| | Gauss (0.0, 0.01) |
Source photo-z shift | |
|$\Delta z^1_{\rm s}$| | Gauss (0.0, 0.016) |
|$\Delta z^2_{\rm s}$| | Gauss (0.0, 0.013) |
|$\Delta z^3_{\rm s}$| | Gauss (0.0, 0.011) |
|$\Delta z^4_{\rm s}$| | Gauss (0.0, 0.022) |
Shear calibration | |
mi(i = 1, 4) | Gauss (0.0, 0.023) |
Parameter . | Prior . |
---|---|
Cosmology | |
Ωm | flat (0.1, 0.9) |
As | flat (5 × 10−10, 5 × 10−9) |
ns | flat (0.87, 1.07) |
Ωb | flat (0.03, 0.07) |
h | flat (0.55, 0.90) |
Ωνh2 | flat(5 × 10−4, 10−2) |
Lens galaxy bias | |
bi(i = 1, 5) | flat (0.8, 3.0) |
Intrinsic alignment | |
AIA | flat (−5, 5) |
ηIA | flat (−5, 5) |
Lens photo-z shift (red sequence) | |
|$\Delta z^1_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^2_{\rm l}$| | Gauss (0.0, 0.007) |
|$\Delta z^3_{\rm l}$| | Gauss (0.0, 0.006) |
|$\Delta z^4_{\rm l}$| | Gauss (0.0, 0.01) |
|$\Delta z^5_{\rm l}$| | Gauss (0.0, 0.01) |
Source photo-z shift | |
|$\Delta z^1_{\rm s}$| | Gauss (0.0, 0.016) |
|$\Delta z^2_{\rm s}$| | Gauss (0.0, 0.013) |
|$\Delta z^3_{\rm s}$| | Gauss (0.0, 0.011) |
|$\Delta z^4_{\rm s}$| | Gauss (0.0, 0.022) |
Shear calibration | |
mi(i = 1, 4) | Gauss (0.0, 0.023) |
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