Table 1
Parametric description of CTI-induced bias charge traps of different species cause in the measured sizes d and ellipticities e1 of faint galaxies (black lines in Fig. 4).
| C | D a | D p | D w | G a | G p | G w | |
|
|
|||||||
| MSMI-measured galaxies: degraded images | |||||||
| Δd/dtrue | 0.04350 ± 0.00034 | −0.0235 ± 0.0005 | 1.92 ± 0.02 | 0.39 ± 0.08 | 0.1236 ± 0.0038 | 0.713 ± 0.011 | 0.449 ± 0.017 |
| Δe1 | 0.05356 ± 0.00022 | −0.0360 ± 0.0004 | 1.99 ± 0.02 | 0.38 ± 0.04 | 0.1058 ± 0.0019 | 0.666 ± 0.004 | 0.434 ± 0.008 |
| MSMI-measured galaxies: CTI-corrected images | |||||||
| Δd/dtrue | −0.00249 ± 0.00030 | 0.0005 ± 0.0005 | 1.83 ± 1.27 | 0.82 ± 3.91 | 0.0013 ± 0.0009 | 0.675 ± 0.246 | 0.432 ± 0.372 |
| Δe1 | −0.00107 ± 0.00012 | 0.0002 ± 0.0001 | 1.40 ± 0.50 | 0.10 ± 0.00 | 0.0015 ± 0.0003 | 0.792 ± 0.145 | 0.517 ± 0.141 |
Notes. The measurements assume a density of one trap per pixel, and the astrophysical measurement is fitted as a function of the charge trap’s characteristic release time τ as 
. The parameters in this table correspond to a trap density of 24% of the Euclid end-of-life estimate.
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