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Table 1.

Bad pixel flags used in the MUSE pipeline.

Flag value Bit-shift Data quality condition
0 0 Good pixel – no flaw detected
1 1 Affected by telluric feature (corrected) (a)
2 1 ≪ 1 Affected by telluric feature (uncorrected) (a)
32 1 ≪ 5 Cosmic ray (unremoved) (b)
64 1 ≪ 6 Low QE pixel (< 20% of the average sensitivity; e.g., defective CCD coating, vignetting)
256 1 ≪ 8 Hot pixel (> 5σ median dark)
512 1 ≪ 9 Dark pixel (permanent CCD charge trap)
4096 1 ≪ 12 A/D converter saturation (signal irrecoverable, but known to exceed the A/D full-scale signal)
8192 1 ≪ 13 Permanent camera defect (such as blocked columns, dead pixels)
16384 1 ≪ 14 Bad pixel not fitting into any other category (c)
230 1 ≪ 30 Missing data (pixel was lost)
231 1 ≪ 31 Outside data range (e.g., outside of spectral range, inactive detector area, mosaic gap)

Notes.

(a)

In the MUSE pipeline telluric features are only marked in the standard star processing, but never propagated to science data.

(b)

The corresponding “removed” cosmic ray from the Euro3D specifications is not used.

(c)

In the MUSE pipeline this is used for non-positive pixels in flat-field images.

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