| Type . | Impact . | On . |
|---|---|---|
| SFR/SNR | 20 per cent factor two to three | Pop II |
| IMF | +50 per cent | Pop II |
| Type IIn 1 per cent | 0–10 | CC SN in DD at AB-mag > 28 |
| Type IIn 1 per cent | 0 | CC SN |
| PP SN factor | 0 | PI SN |
| RSG factor 75 per cent | −100 per cent to + 33 per centa | CC SN and PI SN |
| CCSN energy distribution | −100 per cent to +200 per centa | CC SN |
| Detection change threshold (25 per cent) | 0 | WFD |
| Detection change threshold (25 per cent) | 0.01 | ADS |
| ADS cadence if > 1–2 months | 0 | ADS |
| Attenuation Ly α scatter | 100 per cent of Madau | i band |
| Attenuation Ly α scatter | 35 per cent of Madau | z band |
| Attenuation Ly α scatter | 0 | y band |
| Lens Model | −50 per cent to 100 per cent | all |
| Magnification mu 1–2 interpolation | 0 | WFD |
| Magnification mu 1–2 interpolation | 1 | ADS |
| Type . | Impact . | On . |
|---|---|---|
| SFR/SNR | 20 per cent factor two to three | Pop II |
| IMF | +50 per cent | Pop II |
| Type IIn 1 per cent | 0–10 | CC SN in DD at AB-mag > 28 |
| Type IIn 1 per cent | 0 | CC SN |
| PP SN factor | 0 | PI SN |
| RSG factor 75 per cent | −100 per cent to + 33 per centa | CC SN and PI SN |
| CCSN energy distribution | −100 per cent to +200 per centa | CC SN |
| Detection change threshold (25 per cent) | 0 | WFD |
| Detection change threshold (25 per cent) | 0.01 | ADS |
| ADS cadence if > 1–2 months | 0 | ADS |
| Attenuation Ly α scatter | 100 per cent of Madau | i band |
| Attenuation Ly α scatter | 35 per cent of Madau | z band |
| Attenuation Ly α scatter | 0 | y band |
| Lens Model | −50 per cent to 100 per cent | all |
| Magnification mu 1–2 interpolation | 0 | WFD |
| Magnification mu 1–2 interpolation | 1 | ADS |
These are the lower/upper limits on how the results can vary.
| Type . | Impact . | On . |
|---|---|---|
| SFR/SNR | 20 per cent factor two to three | Pop II |
| IMF | +50 per cent | Pop II |
| Type IIn 1 per cent | 0–10 | CC SN in DD at AB-mag > 28 |
| Type IIn 1 per cent | 0 | CC SN |
| PP SN factor | 0 | PI SN |
| RSG factor 75 per cent | −100 per cent to + 33 per centa | CC SN and PI SN |
| CCSN energy distribution | −100 per cent to +200 per centa | CC SN |
| Detection change threshold (25 per cent) | 0 | WFD |
| Detection change threshold (25 per cent) | 0.01 | ADS |
| ADS cadence if > 1–2 months | 0 | ADS |
| Attenuation Ly α scatter | 100 per cent of Madau | i band |
| Attenuation Ly α scatter | 35 per cent of Madau | z band |
| Attenuation Ly α scatter | 0 | y band |
| Lens Model | −50 per cent to 100 per cent | all |
| Magnification mu 1–2 interpolation | 0 | WFD |
| Magnification mu 1–2 interpolation | 1 | ADS |
| Type . | Impact . | On . |
|---|---|---|
| SFR/SNR | 20 per cent factor two to three | Pop II |
| IMF | +50 per cent | Pop II |
| Type IIn 1 per cent | 0–10 | CC SN in DD at AB-mag > 28 |
| Type IIn 1 per cent | 0 | CC SN |
| PP SN factor | 0 | PI SN |
| RSG factor 75 per cent | −100 per cent to + 33 per centa | CC SN and PI SN |
| CCSN energy distribution | −100 per cent to +200 per centa | CC SN |
| Detection change threshold (25 per cent) | 0 | WFD |
| Detection change threshold (25 per cent) | 0.01 | ADS |
| ADS cadence if > 1–2 months | 0 | ADS |
| Attenuation Ly α scatter | 100 per cent of Madau | i band |
| Attenuation Ly α scatter | 35 per cent of Madau | z band |
| Attenuation Ly α scatter | 0 | y band |
| Lens Model | −50 per cent to 100 per cent | all |
| Magnification mu 1–2 interpolation | 0 | WFD |
| Magnification mu 1–2 interpolation | 1 | ADS |
These are the lower/upper limits on how the results can vary.
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