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Procedure: Afternoon Activities
Contents
- 1. Check Schedules
- 2. Verify Instrument Status
- 3. Data Management
- 4. Enable System
- 5. Align
- 6. Reference Centroids
- 7. Disable System
- 8. Junk File(s) & Delete Exposure Information
- 10. Dome Flat Fields & Calibrations
- 11. Sky Flat Fields & Calibrations
- 12. Process PAM Files
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Check technicians' support
schedule.
Determine if operations are limited, and responsibilities for opening
enclosure prior to sunset.
-
Monitor
current
and
forecast
weather trends:
-
If LGS operations
scheduled, then before 16:00 on a weekday:
If new observing run, then:
-
Execute the following command (enables brushless motors, which can be vulnerable
to power fluctuations, and sets them to default positions):
user@shimmy /u/user/observers/lgs/scripts/daily_startup.tcl
Alternatively, in ShaneAO loop control GUI (saocon_gui):
-
Use Instrument setups option to load approprate configuration, e.g. ngs16cog
-
Verify/set NGS mode explicitly via Python prompt >>> ngs()
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Verify/set WFS camera rate, WFScam rate(Hz) to 250 Hz, e.g. via Python prompt >>> rate(250)
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Verify/set TT Cam rate, TTcam rate(Hz)to 500 Hz, e.g. via Python prompt >>> ttrate(500)
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Optional: Initialize software via Python prompt >>> e.g. init(16)
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Optional: Enable woofer communications via Python prompt >>> woof('on')
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Optional: Enable tweeter communications via Python prompt >>> mems('on')
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Optional: Set centroiding algorithm e.g. via Python prompt >>> cent('bin')
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Optional: Load appropriate refcent file via Python prompt >>> e.g. refcent('data/hs-2014-08-13-BINQUAD_16xLGS.fits')
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In ShaneAO motor control GUI (saomot_gui):
-
Verify/set TT Dichroic to Splitter
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Verify/set Lenslet to 16x
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In ShaneAO Power Controls GUI (saopower_ui), verify/set the following:
B5 |
Woofer |
ON |
B6 |
Heartbeat failsafe |
ON |
B7 |
635nm laser diode |
OFF |
B8 |
White light |
OFF |
C4 |
Argon Lamp |
OFF |
C7 |
Galil 7 |
ON |
-
Refresh mirror shape: Over time, successively saved mirror
flats acquire more and more problems. Therefore, periodically (every
few days, or more frequently if needed), the mirror status must be
refreshed by commanding the actuator voltages on both Woofer and
Tweeter to go to zero in 2 sequential phases.
In ShaneAO loop control GUI:
- Actions...
- Shape...
- Go to bias zero
- Actions...
- Shape...
- Go to zero
-
Align and acquire new mirror flat:
-
In ShaneAO motor controls GUI (saomot_gui):
-
Verify/set TT Dichroic to Splitter
-
Insert calibration stage into the beam.
Cal X |
White Light |
Cal Y |
Open or White Light |
-
Ensure the White light source is OFF, via ShaneAO Power Controls GUI:
-
Acquire new background sample: WFS camera dark background, via ShaneAO loop control GUI. Alternatively (via Python prompt): dark()
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Illuminate the White light source, via ShaneAO Power Controls GUI:
-
Close WFS loop (Gain=0.2 for 16x; Gain=0.1 for 8x), via ShaneAO loop control GUI.
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Ensure woofer values ty and tx are each less than 1.0 via ShaneAO - peeko GUI (peeko).
-
Adjust
Cal X and Cal Y stages in order for
ty and tx to converge to zero, via ShaneAO motor control GUI (saomot_gui):
Cal X adjusts ty, recommended move size: 500 load encoder counts.
Cal Y adjusts tx, recommended move size: 10 load encoder counts.
-
In ShaneAO loop control GUI, acquire new mirror flat:
- Actions...
- Shape...
- Save as flat
Alternatively (via Python prompt >>>) save_flat()
This should set the foc: value in the ShaneAO - peeko GUI near to the expected value of approximately +2.00 (+/- 1.5).
-
Ensure Loops open on completion.
For each mode (16x, BINQUAD; 16x COG; 16x QUAD; 8x, BINQUAD; 8x, COG; 8x, QUAD),
sample performance of ShaneAO + ShARCS.
Determine if image sharpening is required.
-
In ShARCS wheel control GUI (saowheels_gui), set the following:
Filter #1 |
Open |
Filter #2 |
FeII |
Filter #3 |
Open |
-
Ensure the White light source is OFF, via ShaneAO Power Controls GUI:
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In sharcs_fe GUI, set:
-
Exposure 0.11 seconds.
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Ncoadds 3.
-
Window: Select Windows..., Window...
In resulting Sharcs Window GUI, set the following:
start x: 1085
end x: 1184
start y: 700
end y: 799
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In ShaneAO loop control GUI, acquire new background sample: WFS camera dark background.
Alternatively dark()
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In ShaneAO Power Controls GUI, illuminate the White light source:
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In ShaneAO loop control GUI, close WFS loop.
Alternatively close() or gain(0.2),
where 0.3 is the Tweeter+woofer gain.
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In Image Browser GUI, ensure fwhm tool is enabled.
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In sharcs_fe GUI, take exposure: Expose
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In sharcsdisp GUI, inspect resulting image for Airy rings, circularity, aberrations.
-
In sharcsdisplay terminal:
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Inspect values of (x / y)fwhm" for circularity and optimization.
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Inspect values of strehl ratio for optimization.
If strehl ≤ 0.65 perform Image Sharpening using scriptproc.tcl GUI.
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On completion, ensure Loops open.
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Ensure the White light source is OFF, via ShaneAO Power Controls GUI:
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Execute the following command (disables brushless motors, making them less vulnerable to power fluctuations):
user@shimmy /u/user/observers/lgs/scripts/daily_shutdown.tcl
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In ShaneAO Power Controls GUI (saopower_ui), verify/set the following:
B5 |
Woofer |
OFF |
B6 |
Heartbeat failsafe |
OFF |
B7 |
635nm laser diode |
OFF |
B8 |
White light |
OFF |
C4 |
Argon Lamp |
OFF |
C7 |
Galil 7 |
OFF |
The ShARCS detector/electronics has the property that when the windowed is re-sized from a small area to a larger or full frame,
spurious electronic signal/noise is introduced into the first data frame following the geometry change.
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In sharcs_fe GUI, set:
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Exposure 1.5 seconds.
-
Ncoadds 1.
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Window: Select Windows..., Window..., Full
In the resulting Sharcs Window, the geometry should be the following:
start x: 0
end x: 2047
start y: 0
end y: 2047
-
Acquire at least one exposure with Object specified as "Junk".
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Delete Exposure Information: Select Take Darks..., Delete Exp Info..., Reload
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Verify status of Shane 3-m Telescope Mirror Cover and Lights.
-
Verify/set diagnonal mirror sdiagmir_fe to position 3.
-
Remove calibration stage from the beam, via ShaneAO motor controls GUI (saomot_gui):
Cal X |
White Light |
Cal Y |
Open |
-
In ShARCS wheel control GUI (saowheels_gui), configure filter(s) and acquire dome flat field exposures:
J |
Red |
45.0 |
H |
Red |
15.0 |
Ks |
Red |
9.0 |
BrG-2.16 |
Sup_Blue Dimmer [100] |
1.5 |
FeII |
Sup_Blue Dimmer [100] |
1.5 |
J + CH4-1.2 |
Sup_Blue Dimmer [100] |
1.5 |
H2-2.122 |
Sup_Blue Dimmer [100] |
1.5 |
CH4-2.4 |
Blue |
6.0 |
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Optional: Acquire accompanying Darks.
-
Configure ShaneAO and ShARCS for sky calibrations and arrange for enclosure to be
opened, e.g. via electronic mail to: mh-techs@ucolick.org.
Optionally, circulate to shane-observers@ucolick.org, notifying of any acquired
dome flat fields and/or dark frame calibrations:
Subject: Conditions permitting, please open 3m + M1 cover ca 1-hr pre-sunset
Conditions permitting, please open Shane enclosure and mirror cover circa 1-hour before sunset to enable enclosure to thermalize and (if desired) observer(s) to acquire sky flat fields.
System is configured for sky flat fields, pending input of observer contact information.
Expect to commence on-sky optimization circa 20--30 minutes post-sunset.
Scheduled observers: Please note the following afternoon calibrations:
0XXX--0XXX Dome Flat J 60.0 s counts~10000 (Red lamp).
0XXX--0XXX Dome Flat H 12.0 s counts~11000 (Red lamp).
0XXX--0XXX Dome Flat BrG-2.16 3.0 s counts~13000--14000 (Sup Blue Dimmer 100%).
0XXX--0XXX Dark 3.0 s.
0XXX--0XXX Dark 12.0 s.
0XXX--0XXX Dark 18.0 s.
0XXX--0XXX Dark 60.0 s.
If LGS operations scheduled, process Predictive Avoidance Authorization
Message (PAM) files.
It is important to process PAM files promptly (before 16:00) to allow for Laser
Clearing House (LCH) to be contacted for a resolution during regular business
hours.
Normal LCH hours are 08:00--17:00 PT Mo-Fr. (805) 605-4763 or (805) 606-7410.
For emergency actions outside regular business hours the phone number is
(805) 605-3514 to request on-call support.
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Save PAM files (e.g. PAM_Lick_589nm_13kHz_T-003_30JUN2023_For_JDAY185_AZEL-1.txt;
PAM_Lick_589nm_13kHz_T-003_30JUN2023_For_JDAY185_RADEC-1.txt;
PAM_Lick_LLAMAS_355nm_T-000_23AUG2023_For_JDAY236_AZEL-1.txt;
PAM_Lick_LLAMAS_355nm_T-000_23AUG2023_For_JDAY236_RADEC-1.txt)
and copy to appropriate destination:
scp PAM_Lick_*_JDAYXXX_*.txt user@shimmy.ucolick.org:/u/user/observers/lgs/PAM/
- Parse PAM files:
user@shimmy.ucolick.org: /usr/local/lick/bin/lsmParse /u/user/observers/lgs/PAM/PAM_Lick_*_JDAYXXX_AZEL-1.txt
user@shimmy.ucolick.org: /usr/local/lick/bin/lsmParse /u/user/observers/lgs/PAM/PAM_Lick_*_JDAYXXX_RADEC-1.txt
- Check UT date vs JDAY:
user@shimmy.ucolick.org: /usr/local/lick/bin/lsmCheck 2023MonXXUT
- Match object names for UT date:
user@shimmy.ucolick.org: /usr/local/lick/bin/lsmNames 2023MonXXUT
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Monitor electronic mail for notifications of additional closures due to
recent space events, circulated to mh-laser.ucolick.org.
Change Log
- 2024-09-18: Updated.
- 2023-08-24: Updated: Change PAM filename root.
- 2023-07-03: Updated: Change PAM filename root.
- 2023-05-07: Updated: Change destination of PAM files.
- 2021-05-29: Updated.
- 2020-10-29: Updated.
- 2019-02-20: Updated.
- 2018-12-22: Updated.
- 2018-10-29: Updated save mirror flat procedure.
- 2017-12-30: Updated LGS file names for 2018.
- 2017-08-05: Updated window.
- 2017-06-09: Updated shimmy replaces shred.
- 2014-05-09: First version.
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