Changes between Version 2 and Version 3 of docs/CommissioningPlan/SDC2
- Timestamp:
- 01/14/22 13:01:06 (3 years ago)
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docs/CommissioningPlan/SDC2
v2 v3 1 1 == SDC2 Instrument flat field, detector linearity and bad pixels == 2 • **Phase** : Any 3 • **Status** : Draft 4 • **Category** : Daytime calibration (C3) 5 • **Recurrence** : every day, with setup on request. 6 • **Duration** : 20 minutes per configuration 2 3 - **Phase** : Any 4 - **Status** : Draft 5 - **Category** : Daytime calibration (C3) 6 - **Recurrence** : every day, with setup on request. 7 - **Duration** : 20 minutes per configuration 8 7 9 **Description** 8 • Instrument flat field, detector linearity, and bad pixels. 10 - Instrument flat field, detector linearity, and bad pixels. 11 9 12 **Prerequisites** 13 10 14 **Procedure** 11 • Use the calibration flat-field source. 12 • This calibration is performed illuminating the detector uniformly using the instrument FF lamp, for each filter. 13 • It is expected that the detector FF depends on filters, final accumulated charge in the pixels. Thus, a series of exposures will be taken at different count levels (realized via ND filters and/or DIT) for each filter setup. In this case, the template takes the background frames automatically. Comparing different count rates at constant DIT will also yield a linearity map of the detector. 15 - Use the calibration flat-field source. 16 - This calibration is performed illuminating the detector uniformly using the instrument FF lamp, for each filter. 17 - It is expected that the detector FF depends on filters, final accumulated charge in the pixels. Thus, a series of exposures will be taken at different count levels (realized via ND filters and/or DIT) for each filter setup. In this case, the template takes the background frames automatically. Comparing different count rates at constant DIT will also yield a linearity map of the detector. 18 19 **Templates** 20 14 21 **Success criteria** 15 • 95% luminous uniformity at large scale. 16 • 99% luminous uniformity at pixel-to-pixel scale 10-2. 17 • Large scales filtered out, only small detector scale will remain. Effect of the large-scale flat field on DBI (rescaling in flux & wavelength) has negligible impact on DBI performances. 22 - 95% luminous uniformity at a large scale. 23 - 99% luminous uniformity at pixel-to-pixel scale 10-2. 24 - Large scales filtered out, only a small detector scale will remain. Effect of the large-scale flat field on DBI (rescaling in flux & wavelength) has negligible impact on DBI performances. 25 18 26 **Notes** 19 • Same as activity 7.9 in AD4 27 - Same as activity 7.9 in AD4 28 20 29 **LBTO support** 21 30 22 **Associated SHARK-NIR personnel**23 24 31 **Date performed and by whom**