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Lick Planet Search - Hamilton setup
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Fischer, version: 21 Jan 2009
Updated by Julien Spronck in August 2009
Updated by Kelsey Clubb on 23 Dec 2010
- Fill the dewar every afternoon
Setting up the Hamilton
Camera room (four things)
1) open echelle grating
2) open collimator – put in mask
3) open cross-disperser (slide out front and lift side panels)
4) fill the dewar
Is the CCD controller temp correct? (-120 for dewar 8, -116 for dewar 6)
Slit room
1) Check I2-cell orientation on first night with laser
2) Fan on medium, drawing air
Set up computers
Select "Remote Observation Startup for Hamilton" from pull-down Hamilton menu
Type 'yes' in the xterm that appears asking to confirm the start of all Hamilton GUIs
The following windows should appear (if not, select them individually from pull-down menu):
1) Data Taker
2) Hamilton Motor Controller
3) Showmidpt (can no longer rely on showmidpt2 for setting an exposure to end after a specific number of counts have been collected)
4) Slitroom_fe
5) Event sounds
6) Coords
7) Telcoc
8) Guider
NOTE: The previous controller, Hamit, has been decommissioned in favor of a more user-friendly GUI.
To change the setup, click on the box with the letters/numbers to get a pull down menu (not the
downward arrow/check mark). The downward arrow/check mark gives more detailed options for
making changes. Also note that when you change something such as a filter from open to bg12, for
example, the box will turn yellow and you must click the right arrow that appears to the right of the
yellow box or else the change will not take place!
Warm-up Iodine Cell
No longer done manually from slit room!
From the Hamilton motor control GUI, choose "On" from the "Power:" pull-down options (If this fails, open an xterm and type: modify -s hammotor omegapower=on)
After a few minutes or so, the setpoint should reflect 50.0 (degrees C) and it takes 20 minutes to fully warm-up
Logsheet
Open an xterm window on catpc. Type 'logsheets' to get to the logsheets directory (/local/u/user/planets/logsheets). Copy last logsheet to current one and edit.
Data Taker Window
2nd Level Tab, verify and/or change the following:
Directory: /data/shane
Root: run number plus '.' (e.g. i73.)
Suffix: fits
Enter appropriate observer name
Amplifier: Left
Monitor temperature: No (unless briefly checking temperature)
Desired CCD temperature: -120.0 (for Dewar 8)
Focus
1) Hamilton motor control GUI:
Calibration Lamp: ThAr
Aperture plate: 100:2.5
Slit (microns): 2200
Science Filter: open
2) Data-taking window:
Exposure time: 20 (seconds)
Display size: nr=1700 nc=1851, sr=0 sc=100
Shutter: open
Binning = row: 1, column: 1
Read Speed = Fast
Don’t Record (written to scratch directory, necessary for foc.pro)
Object Name: focus
Take exposure
3) Data Taker Control window:
Select "clip" (the oval will turn yellow)
Decrease flux range to something more like ~850-3200 (rather than 0-65535)
Select "lock" (again, the oval will turn yellow)
Right-click on the circle between the two squares and above the flux range (this will show a zoomed-in version of the image when the mouse is in the dtake image window)
Is the ThAr “A” line in the proper position at 759, 1248?
If not, tweak the Grating and Height as necessary to get close (or foc.pro won't work)
NOTE: Click on the downward arrow/check mark to get a new window that allows you to change the position of the grating/height/focus.
You would type your desired move (in stepper counts) in the "relative move:" box
NOTE: To incerase the row by 1, decrease the height by 9 stepper counts. To increase the column by 1, decrease the grating by 1-2 stepper counts.
4) In /local/u/user/observers/lowe/Hamilton on catpc, run foc.pro:
idl> foc, /plt, /mark, /hi_rho, /shane
If necessary, tweak the Grating and Height as directed by foc.pro
Tweak Dewar Focus (by stepper counts, not microns) until FWHM is within range (as specified by foc.pro)
NOTE: Previous grating/height/ccd focus settings are now meaningless (such as never going below 500,000 for CCD focus position)
Once the best focus has been found, turn Recording on and and save the best focus image
5) Update the logsheet with current CCD Focus, Grating, Height settings.
Wideflats
Take test exposures with the BG12 filter until you find an exposure time that results in ~17,000 peak counts for a column cut of column 1000. Repeat for BG13.
1) Hamilton motor control GUI:
Calibration Lamp: PolarQuartz
Aperture plate: 640:5.0
Slit (microns): 2200
Science Filter: BG12 or BG13
2) Data-taking window:
Exposure time: see note above, but a starting point would be 7 seconds for BG12 and 1.5 seconds for BG13
Display size: nr=1700 nc=1851, sr=0 sc=100
Shutter: open
Binning = row: 1, column: 1
Read Speed = Fast
Don't Record (only for the test exposures to find appropriate exp time)
Object Name: wideflat
Take exposure
3) Make sure there are no I2 lines in the data taker images! Iodine Cell Position should be "Out" on GUI
4) Once you have the desired exposure times for each filter:
TURN RECORDING ON!!!
Open an xterm on gouda and, in IDL type: IDL> autoflat,number=30,/time
Number can be as small as 10 if time is short
The program will prompt you for the BG12/BG13 exposure times
The program then takes a set of 30 BG12 wideflats, followed by 30 BG13 wideflats
An alternative to "autoflat" is "igetham"
Open an xterm on gouda and type: igetham 30
This will take a set of 30 exposures without observer intervention
You will have to manually change the filter for the second set, however...
Iodine
1) Insert I2 cell by choosing Position: "In" on Hamilton motor control GUI
(or, in the slitroom_fe window, pull down “function” window and insert I2 cell)
(did you turn on the temp controller? Does the temp controller read 50C?)
2) Hamilton motor control GUI:
Calibration Lamp: PolarQuartz
Aperture plate: 640:2.0
Slit (microns): 2200
Science Filter: BG12, then switch to BG13 after pausing exposure (see note below)
3) Data-taking window:
Exposure time: will vary (see note below)
Display size: nr=1700 nc=1851, sr=0 sc=100
Shutter: open
Binning = row: 1, column: 1
Read Speed = Fast
Record
Object Name: iodine
Take exposure
NOTE: The Iodine exposure has two steps since only one filter can be in at a time.
Choose BG12. Enter an exposure time of 4 seconds as a first guess. Start the exposure. After ~2.5 seconds or so, PAUSE the exposure. Switch to the BG13 filter and resume the exposure.
Repeat varying the total exposure time and the individual exposure times per filter until a column cut of column 1000 results in peaks ranging between ~5,000-10,000dn
4) Check the spectrum – I2 lines present? 20-30% deep?
ThAr
1) Hamilton motor control GUI:
Calibration Lamp: ThAr
Aperture plate: 640:2.0
Slit (microns): 2200
Science Filter: open
2) Data-taking window:
Exposure time: 3 (seconds)
Display size: nr=1700 nc=1851, sr=0 sc=100
Shutter: open
Binning = row: 1, column: 1
Read Speed = Fast
Record
Object Name: thar
Take exposure
Observing
1) In slit room: Turn on photon integrator: flip 2 switches, dial to 705 V, pull plunger (Also, remove polar axis plug if on 3m)
2) On gouda: be sure you have “coords” window up and read in observing script (note: “yes” enable POCO on gouda)
upload starlist to both gouda (TT) and shard (observer)
3) Be sure “showmidpt” program is up and running
CAT
a) Open up the CAT telescope (housing, then siderostat, upper shutter then mirror cover, pull and twist ceiling cover, put in 5th mirror, turn on tracking)
b) Start guider (click “CAT” on bottom menu bar, “reset to default values in parameter window, check that guiding apertures are over slit and that TV camera is focused)
c) Set on Bstar, 10 minutes before 12 degree twilight
d) Check telescope focus
e) Start autoguider (“Start CAT Guiding,” enable auto-guider by flipping toggle on instrument panel)
3m
a) direct the telescope operator to the starlist
b) select target star and “Send to POCO”
4) Update exposure times and object names in data-taker
5) Update logsheets (spaces, no tabs in logsheet)
End of the night
1) If no Bstar observed at the beginning of the night, observe one now
CAT
a) toggle off autoguider
b) turn off software guider tracking
c) stow telescope
d) close housing (mirror cover, upper shutter, siderostat cover, housing, swing out 5th mirror, twist ceiling cover to close)
2) In slit room: Turn off photon integrator: push in plunger, dial down voltage, flip two switches (Also, put polar axis plug back in if on 3m)
3) Take one I2 observation
4) Take one ThAr observation
5) Take a second set of wide flats
6) Check (and fix) logsheets
on catpc, in /local/u/user/planets/logsheets: idl> kclogchecker
Advanced observers:
a) ftp logsheets to Berkeley, SFSU, and Yale
b) run barylog
c) set up raw reduction script at SFSU
d) start ftp’ing raw data to SFSU and Yale
7) go to sleep!
Advanced observers:
e) run raw reduction script after waking up
End of the run
1) In the slit room: turn off fan
2) Close up the optics in the camera room
3) Turn off power to Iodine cell temperature controller via the Hamilton motor control GUI (If this fails, open an xterm and type: modify -s hammotor omegapower=off)
4) Have all data been ftp’d to SFSU? All logsheets?
Advanced observers:
Has barylog been run on all logsheets?
Is the latest and greatest bcvel.ascii file at SFSU?
Have all raw reductions been run?
Has barystruct been run on the SFSU bcvel.ascii file?