Check rotator ZP duirng a MODS MOS acquisition (Stone fields) - High Priority - 20min per field - 2 field 01:10-01:50
Fields (MMS files in mms/ sub-directory):
Stone A - sets 10pm (only if science cannot be done)
Stone D1f - sets 2am (only if science cannot be done)
Sone E1f - sets 5am
Stone I - 3am-twlight
Check NS dithers 01:55-02:30?
In /home/lbto/Service_Observing/D_E_Time_UT_Dec28_Jan_02/MODS_NSdithers, there are 3 scripts for end-of-night target, Semele (V<~15), available from 2am to morning:
async.txt - grid of small async dithers
sync+async - large sync dither followed by an updatepointing and a grid of detxy abs dithers
sync+async_rel large sync dither followed by a grid of detxy rel dithers.
Reconfigure for LBCs
LBC Technical Work - Medium Priority 02:50? onwards - O.Kuhn running Technical Work
focus offset checks - stable seeing (1" or better on DIMM) - 1.5hr
scripts in lbto@robs:~/Service_Observing_D_E_Time_UT_Dec28_Jan02/LBC_R_focus
check LBCR R focus, mainly.
Focus/collimate, then run superfoc at V+r, followed by a superfoc at [Us,B,g]+R, followed again by superfoc at V+r. Repeat 3x.
Gain/Linearity checks - 1hr (photometric conditions, but poor seeing OK)
scripts in lbto@robs:~/Service_Observing_D_E_Time_UT_Dec28_Jan02/LBC_Linearity
observe a star field with successively longer exposure times, so that a set of stars will have counts that range from 1000 ADU to saturation.
several star fields will be chosen, with published photometry (SDSS or other) so we can not only examine the linearity but check the sensitivity.
TMS: Run TMS in active mode while collecting a series of pupil images (dfoc = -0.8, Z4/Z11 as sent by fpia) - 2hr any conditions (if above can't be done)