This table compares the shear calibration bias, both multiplicative and additive bias for different simple simulation runs. In each simulation except the first and last row, 5 million objects were simulated. We simulated 15 million objects for the first and last row to obtain sufficiently small uncertainties.
Simulation variants . | Galaxy profile . | PSF profile . | Shear . | Background noise level . | m1 × 102 . | m2 × 102 . | c1 × 104 . | c2 × 104 . |
---|---|---|---|---|---|---|---|---|
Basic-0.02 | Gaussian | Gaussian | 0.02 | 5714.36 e-/arcsec2 | 0.01 ± 0.10 | −0.02 ± 0.10 | −0.02 ± 0.14 | 1.06 ± 0.14 |
Basic-0.05 | Gaussian | Gaussian | 0.05 | 5714.36 e-/arcsec2 | 0.23 ± 0.07 | 0.22 ± 0.07 | 0.05 ± 0.33 | 1.08 ± 0.33 |
Basic-0.1 | Gaussian | Gaussian | 0.1 | 5714.36 e-/arcsec2 | 0.99 ± 0.03 | 0.99 ± 0.03 | 0.13 ± 0.33 | 0.88 ± 0.33 |
Doublesky-0.02 | Gaussian | Gaussian | 0.02 | 11428.72 e-/arcsec2 | −0.12 ± 0.18 | 0.01 ± 0.18 | 0.06 ± 0.36 | 1.04 ± 0.36 |
RomanPSF-0.02 (non-rotated) | Gaussian | Roman | 0.02 | 5714.36 e-/arcsec2 | 0.13 ± 0.10 | 0.18 ± 0.10 | −0.02 ± 0.19 | 5.33 ± 0.19 |
Simulation variants . | Galaxy profile . | PSF profile . | Shear . | Background noise level . | m1 × 102 . | m2 × 102 . | c1 × 104 . | c2 × 104 . |
---|---|---|---|---|---|---|---|---|
Basic-0.02 | Gaussian | Gaussian | 0.02 | 5714.36 e-/arcsec2 | 0.01 ± 0.10 | −0.02 ± 0.10 | −0.02 ± 0.14 | 1.06 ± 0.14 |
Basic-0.05 | Gaussian | Gaussian | 0.05 | 5714.36 e-/arcsec2 | 0.23 ± 0.07 | 0.22 ± 0.07 | 0.05 ± 0.33 | 1.08 ± 0.33 |
Basic-0.1 | Gaussian | Gaussian | 0.1 | 5714.36 e-/arcsec2 | 0.99 ± 0.03 | 0.99 ± 0.03 | 0.13 ± 0.33 | 0.88 ± 0.33 |
Doublesky-0.02 | Gaussian | Gaussian | 0.02 | 11428.72 e-/arcsec2 | −0.12 ± 0.18 | 0.01 ± 0.18 | 0.06 ± 0.36 | 1.04 ± 0.36 |
RomanPSF-0.02 (non-rotated) | Gaussian | Roman | 0.02 | 5714.36 e-/arcsec2 | 0.13 ± 0.10 | 0.18 ± 0.10 | −0.02 ± 0.19 | 5.33 ± 0.19 |
This table compares the shear calibration bias, both multiplicative and additive bias for different simple simulation runs. In each simulation except the first and last row, 5 million objects were simulated. We simulated 15 million objects for the first and last row to obtain sufficiently small uncertainties.
Simulation variants . | Galaxy profile . | PSF profile . | Shear . | Background noise level . | m1 × 102 . | m2 × 102 . | c1 × 104 . | c2 × 104 . |
---|---|---|---|---|---|---|---|---|
Basic-0.02 | Gaussian | Gaussian | 0.02 | 5714.36 e-/arcsec2 | 0.01 ± 0.10 | −0.02 ± 0.10 | −0.02 ± 0.14 | 1.06 ± 0.14 |
Basic-0.05 | Gaussian | Gaussian | 0.05 | 5714.36 e-/arcsec2 | 0.23 ± 0.07 | 0.22 ± 0.07 | 0.05 ± 0.33 | 1.08 ± 0.33 |
Basic-0.1 | Gaussian | Gaussian | 0.1 | 5714.36 e-/arcsec2 | 0.99 ± 0.03 | 0.99 ± 0.03 | 0.13 ± 0.33 | 0.88 ± 0.33 |
Doublesky-0.02 | Gaussian | Gaussian | 0.02 | 11428.72 e-/arcsec2 | −0.12 ± 0.18 | 0.01 ± 0.18 | 0.06 ± 0.36 | 1.04 ± 0.36 |
RomanPSF-0.02 (non-rotated) | Gaussian | Roman | 0.02 | 5714.36 e-/arcsec2 | 0.13 ± 0.10 | 0.18 ± 0.10 | −0.02 ± 0.19 | 5.33 ± 0.19 |
Simulation variants . | Galaxy profile . | PSF profile . | Shear . | Background noise level . | m1 × 102 . | m2 × 102 . | c1 × 104 . | c2 × 104 . |
---|---|---|---|---|---|---|---|---|
Basic-0.02 | Gaussian | Gaussian | 0.02 | 5714.36 e-/arcsec2 | 0.01 ± 0.10 | −0.02 ± 0.10 | −0.02 ± 0.14 | 1.06 ± 0.14 |
Basic-0.05 | Gaussian | Gaussian | 0.05 | 5714.36 e-/arcsec2 | 0.23 ± 0.07 | 0.22 ± 0.07 | 0.05 ± 0.33 | 1.08 ± 0.33 |
Basic-0.1 | Gaussian | Gaussian | 0.1 | 5714.36 e-/arcsec2 | 0.99 ± 0.03 | 0.99 ± 0.03 | 0.13 ± 0.33 | 0.88 ± 0.33 |
Doublesky-0.02 | Gaussian | Gaussian | 0.02 | 11428.72 e-/arcsec2 | −0.12 ± 0.18 | 0.01 ± 0.18 | 0.06 ± 0.36 | 1.04 ± 0.36 |
RomanPSF-0.02 (non-rotated) | Gaussian | Roman | 0.02 | 5714.36 e-/arcsec2 | 0.13 ± 0.10 | 0.18 ± 0.10 | −0.02 ± 0.19 | 5.33 ± 0.19 |
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