Changes between Version 3 and Version 4 of docs/CommissioningPlan/P3.18
- Timestamp:
- 01/19/21 18:04:34 (4 years ago)
Legend:
- Unmodified
- Added
- Removed
- Modified
-
docs/CommissioningPlan/P3.18
v3 v4 1 == P3.0 Large spatial scale instrument and telescope flat field == 1 2 == P3.18 Atmospheric calibration and absolute flux calibration == 2 3 • **Phase** : 3 3 4 • **Status** : Draft 4 5 • **Category** : Nighttime testing (functionality and operability) (C4) 5 • **Recurrence** : before every night observations (valid for all observing modes). 2/day for CI (BB filter only).6 • **Duration** : 2 hours6 • **Recurrence** : once at commissioning and then for each LSS observation observations. 7 • **Duration** : 1 hour 7 8 **Description** 8 • Flat field taken during twilight9 • Atmospheric calibration to remove telluric atmospheric features from the stellar spectrum and get absolute flux calibration per spectral resolution element. 9 10 **Prerequisites** 10 11 • Authorize SHARK-NIR on the SX side. 11 12 • Atmospheric conditions: AO working conditions. 12 • Bad pixel map, Background or Dark .13 • Bad pixel map, Background or Dark, Flat-field, wavelength calibration. 13 14 **Procedure** 14 • This calibration is performed by sky observation combined with pointing scan in order to record a flat (that include telescope large scale transmission variations) on the detector. 15 • Single integration times for a given setup, using various flux level with natural light with no coronagraph. 15 • Observe the spectrum of a featureless (and/or standard) star at similar airmass that of the science target. 16 16 **Success criteria** 17 • Width of flux distribution: 3.10-217 • Better than 10% for absolute flux calibration and for average residuals from telluric removal. 18 18 **Notes** 19 • Same as activity 7. 5in AD419 • Same as activity 7.4 in AD4 20 20 **LBTO support** 21 • Dome open during twilight 22 21 • SOUL-AO support 23 22 **Associated SHARK-NIR personnel** 24 23