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Table 1
Detection quality of the best parameters for the simulated data.
| PMAS-LArr | PMAS-PPak | VIMOS MR | |
|
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| CCD size | 4k × 4k | 4k × 4k | 2k × 4k |
| CCD binning | 2 × 2 | 2 × 2 | 1 × 1 |
| grism | R1200(bw) | V500 | MR |
| θ | 1.5 | 2.4 | 3.0 |
| N c | 6386 | 6471 | 11726 |
|
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| DCR | |||
| Pd [%] | 65.6 | 74.6 | 83.6 |
| Pf [%] | 6.2 | 3.1 | 0.5 |
| ϵ [%] | 62.9 | 73.0 | 83.1 |
| I i | 20 × 20 | 10 × 10 | 5 × 20 |
| ξ | 7.0 | 3.0 | 3.0 |
|
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| L.A.Cosmic | |||
| Pd [%] | 95.2 | 86.9 | 94.5 |
| Pf [%] | 3.2 | 39.2 | 3.3 |
| ϵ [%] | 92.8 | 61.4 | 91.5 |
| σ frac | 1.0 | 1.0 | 1.0 |
| f lim | 23 | 27 | 7 |
|
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| PyCosmic | |||
| Pd [%] | 92.9 | 92.5 | 96.1 |
| Pf [%] | 5.5 | 1.3 | 3.5 |
| ϵ [%] | 88.7 | 91.6 | 92.9 |
| w | 1.0 | 2.0 | 1.5 |
| r lim | 1.25 | 1.4 | 1.0 |
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