Night Plan UT 30-Dec-2020
Split Night: 1st half LBTI, 2nd half D/E (this plan)
Night Center 00:22
Handover 00:16
Morning Astronomical Twilight: 05:53
NO chance to open Due to Snow and Ice
Nightlog in google sheets
here
Night Plan
-
Deploy TCS update after handovoer
- SOUL AO Checkout following problems of 20201220 UT- CRITICAL - 2hours
- OSCO at handover - 30min - NCPA on / NCPA off
- AO Scipts: /home/lbto/Service_Observing/D_E_Time_UT_Dec28_Jan_02/AO_Testing/
- Bin3 Test 0.5-0.75 hr - HIGH priority
- closed loop data 6 positons of the instrument rotator
- test the camera lens limits with new M3 position
- Can use either IDL presets, or AO stars from OT in above directory
- Bin 1-4 tests on-sky - check functionality
- use scripts generated from OT in above directory
- Other Issues:
- IT 8282 - Bin? pupil files issue
- IT 8281 - AGW1 loses star at DETXY 10" offset
- IT 8284 - GOPT issues (pending daytime work too)
- IT 8271 - preset gains for ESM needed - work on creating the necessary values
- Observe ESM fields using full AO but with N375 camera - 1 hour per field
- Additional?
- ESM checkout - (M3 and AO checkout must be completed first) - if not started or completed roll over to another night
- Scripts: /home/lbto/Service_Observing/D_E_Time_UT_Dec28_Jan_02/ESM_Testing
- on-sky checks Bin 2 400Hz (FLAO config) vs Bin 2 100Hz (SOUL config) - 1-2 hrs
- Collect ESM data - <1" seeing - stable - 1hr minmum
- Palomar 2 - if clear take photometric standards - probing sensitivity vs FLAO - sets at 3am
- MODS Checkout - Medium Priority
- Verify Rotator ZP with MOS masks (20min)
- Fields:
- StoneA - sets 10pm
- Stone D1f - midnight-2am
- Stone E1f - midnight-5am
- Stone I - 3am-twilight
- MMS files in mms/ sub-directory
- Collect verification AGW transform (1 hour)
- LBC Technical Work - Medium Priority - unlikely to be useful given the HUGE delta-temp for mirrors and ambient
- 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
- Poor Weather Backups
- ESM data collection: this is different than ESM tests above - this is sytematic data colleciton - above is checking on paramters for optimal use
- Scripts: /home/lbto/Service_Observing/D_E_Time_UT_Dec28_Jan_02/ESM_Testing
- M67 (3 filters and bright and faint AO Ref star)
- NGC 3921 all filters
- ICRF3 Spectroscopy (Rothberg)
- Scripts: /home/lbto/Service_Observing/Nov_Dec_2020_E_D_Nights/Poor_Weather/ICRF3_Rothberg_2020B
- ICR5 93.24-13.51 Highest Priority - cycles through G210 K,H,J, and z (fraternal or mono)
- sets at 3am
- Target can sustain 2mags of extinction or more - uses 0.25" slit - J=12, H=9.5, K=7.2
- Observe telluric first
- Double Check high Dec objects to make sure telluric/science are close spatially
- If clear but poor seeing, please observe standard stars, cycling through z,J,H,K,Ks
- Scripts: /home/lbto/Service_Observing/Nov_Dec_2020_E_D_Nights/Poor_Weather/LUCI_Phot_ZP
- Select stars to use based on visibility - OT file is in directory, export the scripts as needed
- Please observe the same star at least two times at different airmasses
--
BarryRothberg - 29 Dec 2020