| 311 | |
| 312 | The evening 'A' calibration sequence includes the LFC and Etalon |
| 313 | frames (and flats) that are necessary to start the nightly drift |
| 314 | calibration. The 'C' calibrations contain the UNe lamps, which are |
| 315 | only present as an emergency backup source in case the LFC is offline. |
| 316 | Taking the 'A' sequence is critical; skipping the 'C' sequence if you |
| 317 | are crunched for time is OK, although that sequence has been timed to |
| 318 | fit within a typical stack time. |
| 319 | |
| 320 | |
| 321 | |
| 322 | |
| 323 | |
| 349 | |
| 350 | We have added an additional script (hpf_takeLFCHRCalExposure.sh) |
| 351 | that will take a LFC exposure through the calibration fiber (~2 minutes |
| 352 | to complete). This should not interfere with any other telescope |
| 353 | operations, as it is entirely internal to HPF. If you find yourself in |
| 354 | a situation similar to last night, you can run this stand alone script |
| 355 | a few times while a different primary operation is happening (e.g. LRS |
| 356 | or VIRUS exposure, slew, or other telescope setup). That will at least |
| 357 | provide a few LFC reference points to tie the drift calculation to. |
| 358 | |
| 359 | The script accepts an optional argument - N - where N is the number of |
| 360 | ramps you wish to take. e.g. {{{ ./hpf_takeLFCHRCalExposure.sh 3 }}} |