Euclid on Sky
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Table 3

NISP detector chain performance.

Mosaic Position SCA 18XXX 11 12 13 14 21 22 23 24 31 32 33 34 41 42 43 44
453 272 632 267 268 285 548 452 280 284 278 269 458 249 221 628
QE (%) YE-band 93 96 88 95 92 94 94 93 91 92 94 94 92 93 96 92
JE-band 95 97 95 96 93 96 95 95 93 94 95 95 96 94 98 95
HE-band 96 98 95 97 94 96 96 95 93 94 95 96 95 94 99 95

Noise (e) Spectro 8.2 9.0 7.8 9.2 8.2 8.9 8.3 8.4 8.1 7.9 8.0 8.7 7.7 7.9 8.1 8.7
Photo 6.0 6.2 5.9 6.4 6.3 6.7 6.4 6.4 5.9 5.8 5.6 6.4 5.7 5.6 6.1 6.1

Disconnected pixels (#) 135 3223 589 252 313 2580 1512 146 1420 269 262 970 198 334 222 255

Notes. Detector chain performance of the flight model NISP focal plane, for all 16 SCS, identified by their SCA number. ‘Position’ refers to position in the 4×4 array as defined in Fig. A.1, ‘QE’ is the quantum efficiency in the respective photometry passbands, with an absolute accuracy of 5% (Waczynski et al. 2016). ‘Noise’ is the read noise in the standard survey MACC modes for photometry and spectroscopy. ‘Disconnected pixels’ gives the number of pixels per detector that do not produce a signal due to a missing or faulty indium bump. If not specified then values given are medians over the array.

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