Changes between Version 6 and Version 7 of docs/CommissioningPlan/P3.18
- Timestamp:
- 01/14/22 19:05:51 (3 years ago)
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docs/CommissioningPlan/P3.18
v6 v7 1 == P3.18 Atmospheric calibration and absolute flux calibration == 2 • **Phase** : 3 3 • **Status** : Draft 4 • **Category** : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6) 5 • **Recurrence** : once at commissioning and then for each LSS observation. 6 • **Duration** : 4 hours 1 == P3.18 Center the slit == 2 3 - **Phase** : 3 4 - **Status** : Draft 5 - **Category** : Nighttime testing (functionality and operability) (C5) 6 - **Recurrence** : once at commissioning 7 - **Duration** : 2 nights 8 7 9 **Description** 8 • Atmospheric calibration to remove telluric atmospheric features from the stellar spectrum and get absolute flux calibration per spectral resolution element. 10 - This activity will center the long slit. 11 9 12 **Prerequisites** 10 • Authorize SHARK-NIR on the SX side.11 • Atmospheric conditions: AO working conditions.12 • Bad pixel map, Background or Dark, Flat-field, wavelength calibration. 13 - Atmospheric conditions: AO working conditions. 14 - Authorize SHARK-NIR on the SX side. 15 13 16 **Procedure** 14 • Observe the spectrum of a featureless (and/or standard) star at a similar airmass that of the science target. 17 - Point to known binary stars and then offset the telescope and the rotators to get to the nominal (known) position of the planet or introducing a bright speckle by using secondary mirrors at the same parallactic angle of the planet in order to align the slit. 18 - TBD 19 20 **Templates** 21 15 22 **Success criteria** 16 • Better than 10% for absolute flux calibration and for average residuals from telluric removal. 23 - xxx 24 17 25 **Notes** 18 • Same as activity 7.4 in AD4 26 19 27 **LBTO support** 20 • AO support 21 **Associated SHARK-NIR personnel** 28 - AO support 22 29 23 30 **Date performed and by whom**