General Start-up procedure
Draft of 05/04/06

Arriving at WIRO
Connect the ethernet cable on the rear of the electronics rack in the control room to enable wireless internet bridge between WIRO and UW. Turn on breakers at each of the three breaker boxes; control room breaker(only turn on the water pump), hallway breaker(turn on all switches unless otherwise marked), dome breaker(inside Spectrograph room, turn on all switches unless otherwise marked). DO NOT TOUCH anything else in the spectrograph room!! A lot of work has gone in to calibrating each instrument. Plug in the telescope encoder rack(yellow plug into power strip) at the south end of the dome behind the telescope. Plug in UPS power supply in the rear corner of the control room(there are 2 yellow plugs), turn on computers: Horatio is the telescope control computer.

Filling the dewar
Ensure that the LN2 dewar is ready by making sure there is a compressed dry N2 tank supplying overpressure, this will allow for a faster fill by pushing the LN2 into the CCD dewar. Also, ensure the LN2 dewar top is securely attached and that the safety cord is attached to the body of the dewar in case of over pressurization.
     •Securely attach the end of the tygon fill tube to the fill valve on the rear of the CCD dewar, and flip the black switch on the LN2 dewar up to allow overpressure from the dry N2.
     •Turn on the dry N2 tank by turning the knob on the top of the tank. Turn the regulatory pressure valve on the dry N2 tank to supply ~5-6 psi to the LN2 dewar(any more than this
       may cause the LN2 tank to become over pressurized and make the top pop off(safety cord comes in handy).
     •Turn on the LN2 dewar by turning the black knob, this will start filling the CCD dewar. You should see the fill tube start to freeze and gas being ejected from the overfill tube of the
       CCD dewar. It should take <5 minutes to fill the dewar.
     •While the dewar is filling take the lens cap off the prime focus corrector by loosening the 4 allen screws and twisting the cap and gently pulling it off. DO NOT TOUCH the front lens
       element of the corrector.
     •While the dewar is filling plug in the camera electronics by plugging in the 2 power supplies. There are 2 orange extension cords running along the support truss of the telescope(note
       on the extension cord with 2 available slots: the side slot doesn't work--use the one on the end). The power supply cables should be attached to these extension cords and to the power
       supply boxes mounted on the prime focus ring. Turn on camera power by turning on black switch on the black power supply(just under the power supply cord).
     •Stop filling the dewar when the dewar starts sputtering LN2 from the overfill tube—it is full. Turn off the LN2 tank and flip the black switch to the down position. Turn off the dry N2
       tank and loosen the regulatory valve until loose. Wait until the fill tube is thawed(~2 min) before removing it from the dewar or it may break and place it gently back on the LN2 tank.
       If the tygon tubing has pinhole leaks or is in poor condition it should be replaced by another tube.
If the dry N2 tank is empty it can be replaced with a full N2 tank by swapping the regulator. First, USE CAUTION and THINK before acting. Ensure that the current dry N2 tank is completely off by turning the top knob on top clockwise tighlty. Disconnect the hose leading to the LN2 tank and bleed the remaining pressure between the N2 tank and regulator by turning the regulator knob clockwise. Remove the regulator from the N2 tank carefully, when removing parts from under pressure they tend to 'fly' off, it is a good idea to tie a safety cord to the regulator to keep it from flying far or against a wall. NEVER ATTEMPT to remove the top from the N2 tank itself, it could result in serious injury. Replace the N2 tank by removing it from its wall mount and placing a full N2 tank in its place. Attach the regulator on the new N2 tank and reconnect the hose to the LN2 tank.

Computer Interface
Log onto Horatio: user and password are posted. Open a terminal and log in as super-user, password is posted.
[horatio~]\$su
Set the current time
[horatio~]\#date MMDDHHmmYY.ss
where this is local time, date -u MMDDHHmmYY.ss is in universal time. Note YY is not a necessary input parameter and need not be present(YY is the suffix assuming 20YY). Log off super-user.
[horatio~]\#exit
Start the tracking loop for the computer
[horatio~]\$start
The lights on the IO Tech Micro 488 interface(little black box at the bottom of electronics rack in the control room) should come on and blink, and the last thing you should see in the terminal is 'entering trackloop'. If this is the case the telescope display on the shelf should come to life with all the pertinent information about the telescope and you can hit enter to return to a command line. If this is not the case, at the terminal type kill all occurances of track,
[horatio~]\$ps -ef | grep track
[horatio~]\$kill ###
then unplug the encoder rack(yellow plug from power strip) behind the telescope, cycle the power on the IO Tech Micro 488 box(black button at left rear), and plug the encoder rack back in. A bunch of red lights should come on on the south rack and the ethernet interface on the south rack should have good status(no light indicating an error). Type start again,
[horatio~]\$start
if this didn't work try again.

Telescope Control
This is only a brief overview of telescope controls more information can be found in the WIRO General Manual(White binder on the shelf). Flip the switch on the bottom side of the South pier(controls at the base of the telescope) up to supply power to the telescope. Make sure there is nothing that will obstruct the motion of the telescope off the platform(ie. hold-down straps, chairs, fill tube) then push the green 'ON' button on the console. If the telescope is too low and the white override button is not depressed an alarm will go off and the telescope will not move. If power does not come on and the breakers are on open the front panel of the South pier. Along the top there is a thermistor that cuts off power to the telescope if the weather is too cold for too long. With the switch to the pier in the up position hold the thermistor for a few seconds to warm it up and try pressing the green 'ON' button again and the power should come on. Hold down the override button and switch to local control and slew the telescope north to zenith then let go of the override and switch to remote. From the observing platform switch to local telescope motion control and line up the fiducial marks on the telescope axes(RA and DEC) to line up with the 'Index' arrows on the telescope mount by holding the center white button and either N,S,E,W to move the telescope, once aligned switch to remote. Using either the computer on the platform or in the control room type:
[horatio~]\$zero ; zenith ; index
[horatio~]\$g
The telescope should move so that the telescope fiducials now line up with the 'Zenith' arrows, if the telescope did not move make sure both the south pier and observing platform controls are set to remote and that the breaker powering the telescope is on. If the RA arrows don't line up, the telescope may have lost a turn.
[horatio~]\$turn-ra
This should bring the arrows pretty close if not try either turn-ra, turn+ra, and similarly turn+dec, turn-dec if the declination axes don't line up. Alternatively, one could try again by moving to index and re-issuing the zero ; zenith ; index ; g command. If the arrows still don't line up try again.

Useful Telescope Commands
zenith ................................................................. moves telescope to zenith and stays there.
service ............................................................... moves telescope to service position and stays there.
nn ## ................................................................. moves the telescope north in DEC ## arcseconds.
ss ## ................................................................... moves the telescope south in DEC ## arcseconds.
ee ## .................................................................. move the telescope east in RA ## arcseconds.
ww ## ................................................................ move the telescope west in RA ## arcseconds.
icol ..................................................................... computer will use current offsets when moving(makes desired position actual position).
follow ## ............................................................slews to and tracks to item ## in current loaded catalog
fixed xx.xxxxxx yy.yyyyyy ................................moves telescope to HA of xx.xxxxxx and DEC of yy.yyyyyy
fixed xx.xxxxxx yy.yyyyyy follow .................... moves to RA of xx.xxxxxx and DEC of yy.yyyyyy and tracks (Note: xx.xxxxxx is expressed in decimal hours and yy.yyyyyy is
                                                                             expressed in decimal degrees).
clrusr .................................................................. clears user commands from the bottom of the screen.
s .......................................................................... stop - turns telescope off.
g ......................................................................... go - turns telescope on.
dome init .............................................................initializes dome azimuth to current telescope azimuth.
dome on ..............................................................turns dome on so that it moves to the desired telescope azimuth.
dome off ..............................................................turns dome off.

Computer header sharing program
Currently the tracking computer(horatio) does not communicate with the image acquisition computer(claudius). To initiate a program that dumps the telescope tracking information into a core file that is read by the acquisition computer do the following.
   1. On Claudius as root user run the program server located in /home/observer/WIRO/WIRO_information_sharing_program/testing.
       [claudius~]\$cd /home/observer/WIRO/WIRO_information_sharing_program/testing
       [claudius~]\$./server 9999
         'listening to socket' should appear indicating a successful execution.
   2. On Horatio run the program client located in the same directory as above from the directory /home/observer/wiro/track.
       [horatio~]\$
cd /home/observer/wiro/track
       [horatio~]\$/home/observer/WIRO/WIRO_information_sharing_program/testing/client 10.212.212.110 9999
         'data sent successfully' should appear repeatedly indicating that the core file is being sent successfully.
The terminals running the program should be left running and monitored to ensure they are working. This program does not excuse keeping regular observing logs, the program is fallable and should only be used as a tool for writing some of the header information, it should be scrutinized before trusting.

Dome slit and wind screen operation
Upon arrival the dome orientation should be such that the slit is in the E-W direction. Both windscreens should be overlapping at the top of the dome. Rotate the dome to the south from the observing platform by aligning the center of the upper wind screen(denoted by a joint in the dome) to the apex of the North polar axis support structure while the telescope is at zenith. The azimuth of the telescope at zenith is 180°(south). On Horatio initialize the dome,
[horatio~]\$dome init
this will initialize the dome's azimuth to 180°. Turn the dome on.
[horatio~]\$dome on
Tthis will enable the dome to automatically rotate to the telescope desired azimuth. It is worth checking from time to time the the dome slit and the telescope are aligned, if the dome occults the primary in any way it will result in bad data. Open the dome slit(on observing platform or service platform) with the windscreens still overlapping above the telescope and with the mirror covers closed to protect the mirror from possible falling stuff. Lower the lower wind screen from the service platform while the dome is facing south and watch the cables as it is lowering and check that the cables don't do anything bad if you have ANY doubts stop and consult with the other observer or call for assistance. Move to the observing platform and raise the upper wind screen, again watch the cables, if you have ANY doubts stop and consult with the other observer or call for assistance. Open the mirror covers(either south pier or observing platform) and make sure both shutters open, if only one opens close the mirror covers and try opening again.

Dome Flat Screen
To use the dome white spot for dome flats the dome needs to initialized. The dome should be rotated to an azimuth of 142°
and the telescope should be moved to an hour angle of 0.0 and a declination of -25° i.e. [horatio~]\$fixed 0.0 -25.0
There are four neutral density filters lamps on the front end ring of the telescope. The lamps are controlled with a rheostat in the control room. If any of the bulbs burn out, there are replacements in the WIRO lab(do not touch the lamps when replacing, hold them with the packaging they come with). Taking flat fields with any filter varies, however here are some documented settings:
Filter          Setting           Exposure           Counts
   U               100V                   2s                ~32,000
   B                60V                    1s                ~21,000
   V                40V                    4s                ~36,000
   R                40V                    1s                ~40,000
    I                 20V                    2s               ~32,000
 OIII               70V                    5s               ~27,000
 5200             70V                    3s                ~22,000

 8132             35V                    5s                ~15,000
 8199             35V                    5s                ~15,000
 8615             35V                    5s                ~17,000
 8685             35V                    5s                ~18,000

Collimating the Telescope
Collimating the telescope should be done each time there is a top end ring change in going from cassegrain to prime focus. It will be easiest to collimate on a star near the zenith, this way the collimation screws on the rear cell of the telescope are more accessible from the observation platform. There are three collimation screws located in the primary mirror cell I will denote E, NW and SW(cardinal direction). Each screw is locked in place by use of a nut and has a limited range of motion. It will be necessary to move the camera(guider for cass and the main imager for prime) far enough out of focus to see the donut(actually the image of the primary mirror) well defined with the central obstruction and spider vanes--it will be necessary to adjust the exposure time to get a good enough signal so use a moderate to bright star. The goal is to place the central obstruction as close to the center as possible. This means, as you get closer, measure how close the central obstruction is to the edge of the 'donut'(be cautious of measuring from the bottom since the filter wheel juts out a little) along the edges to determine its position precisely.

How To Collimate: Unlock the nut preventing the screw from turning, an adjustable wrench works well(I like a 15/16” wrench). Then turn the screw using a 1/2” wrench. As of 04/22/06 there are fiducial marks on the collimation screws indicating where and how much to turn each bolt to achieve collimation for cass and prime.

The following is a how to in case the marks become unreliable. NOTE: it doesn't take much to change the collimation, only an 1/8 of a turn can be significant! Take an exposure and compare to the previous, if it is better—GREAT! if it is worse undo what you did and try the other direction or a different screw. There is a limited range on each screw, if it starts to get tight and hard to turn—STOP!! the primary may be pinching, if it gets sloppy loose—STOP!! there may be nothing supporting the mirror. Remember you can always go to another screw and do the opposite to achieve a similar result. As collimation proceeds the images will shift around on the display as a result of tilting the primary so try to keep the star centered by using the 'nn','ss','ee','ww' commands. Once the central obstruction is well centered start moving back towards focus. Continue to take images though and watch that the central obstruction remains in the center because as you get closer to focus the 'donut' is more sensitive to collimation. Remember to tighten the locking nuts after you are done.

Shutdown Procedure
Move the telescope to service by first moving it close to the meridian and then issuing the 'service' command. Once the slew is complete type 's' to turn off the telescope and 'dome off' to turn the dome off. The reason for moving it to the meridian first is because from low declination and/or at high hour angles the telescope gets close to hitting the service platform. Close the mirror covers and from the south pier switch to local control and while holding down the white limit switch slew the telescope south until it is almost touching(6 inches) the service platform. Turn off power to the telescope by pushing the switch down on the bottom of the south pier. From the service platform raise the lower windscreen while watching the cables as they wind around the capstan an ensure they are winding properly. Place the cover back on the corrector and tighten the 4 allen screws holding it on. Turn the camera interface off and unplug the camera electronics(2 plugs). From the observing platform lower the upper windscreen until it overlaps the lower windscreen, again watching the cables wrap around the capstan. Close the dome slit and rotate the dome to face East-West. Unplug the encoder rack and turn off the breakers in the dome, the hallway and the control room(unless otherwise marked). Close the camera interface(s) and the filter wheel/focus gui(s) and turn off the CompuMotor controller box and log off all the computers and remove the 2 plugs from the UPS and unplug the ethernet. The purpose is to protect the electronics from possible lightning strike. Make sure all data is copied to CD/DVD before departure, it takes a long time to transfer via sftp/scp/ssh. It is a good idea to have someone check that the shutdown looks good, it easy to forget something at the end of a long run.

Creating a data CD/DVD
Xcdroast is used on Claudius to write data to a CD/DVD.
[claudius~]\$xcdroast
Click on Master tracks and drag the desired folders to the left column. Select the type of media you wish to write to: CD or DVD and the size, type, etc. Click on Master to Image File, this will create a temporary image file on the hard disk. Select the image file just created and click Write Tracks. Verify the tracks were written using Verify Tracks. The software requires a key to burn DVD's, if the key is out of date(last updated 3/7/2006) get an updated key from xcdroast.org and run xcdroast as root and copy/paste the key in the setup location.

Water Pump
The Water supply for WIRO is a 10,000 gallon tank that rests in near the main entrance to WIRO. The water tank is filled via a truck hauling 1,000 gallons of water during the Summer, when the road is easy to pass, requiring multiple trips. The water pump transfers water from the holding tank to two holding tanks under the main entry to WIRO. A water meter gauges the amount of water that is transferred and should be check to ensure water levels. Access to these indoor tanks is obtained through the floor hatch located in the storage area next to the entrance. When the floor panel is removed a light switch is released turning lights on under the floor. There is heat tape wrapped around some of the pipes and a space heater that are constantly running to prevent the water from freezing in the pipes. There is light switch panel that controls the heat tape. If anything seems wrong contact WIRO personnel.

Troubleshooting

If what you are trying to move isn't moving check that the platform you are on is set to local control and that other platform is set to remote. If that is not working check that all breakers were properly switched on.