INT/IDS Troubleshooter
- Starting the system
- Shutting down the system
- Bad Pointing
- Closing down fast
- Faults - In General
- Autoguider window disappears
- Guide camera in the lightpath?
- No available guide stars
- Observing at low elevation
- Data acquisition problems
- Problems with IDS control
- Problems with Acquistions Guidance
Box (AGB) control
- Restarting inttv
- Starting up the data reduction PC
- Restarting the meteorological data screen
- Power cuts
- TCS Screens Hang
- Cenwave value fluctuating in the IDS mimic
- Acknowledgements
| Note: The following
operations should be done in the order as indicated below
|
Start
TCS
- Login to the TCS system using the username and password written
on the top of the monitor.
- Upon logging in 2 windows appear: the DAS (orange) and the TCS on
LPAS2 (white). If the TCS window disappears. You can bring back the
TCS window again by double clicking on the INT TCS icon.
- If this icon is not present you will need to open a terminal
window and type >telnet inttcs
and log in using the int_login
account.
.
On the LPAS2 window (white):
- Logon using the int_login
account.
> start
This brings up the TCS Display and the
User interface. Note: In case there is no 'start' in the menu, then press 'stop' followed by 'start'.
Start TV acquisition camera
On the DAS window (orange):
inttv@miranda> obssys
- From the available options choose:
1 - manual camera selection
1 - manual camera selection.
- Ensure the camera server is not running by executing
DAS6@miranda> shutdownobssys
- Start the camera
server using
DAS6@miranda> startobssys
- Start the TV acquisition system:
DAS6@miranda> startag AG0
Choose
option:
station: 4 - Cassegrain Focus
- When asked to start ds9 respond y.
- Still in the DAS terminal execute > bin 3 3.
- Acquire an image with the Acquisition camera by pressing Field.
It will be just noise but it's not important. It's only so that you can
load regions on ds9 by going to Region -> Load Regions and
select the most recent "IDS_centres_bin3" file (for 3x3 binning).
- This should result in the green and blue overlays being
displayed on the ds9 screen.
- Flip the ds9 image in Y by doing Zoom -> Invert y.
Start the Observing System
On the intics machine (lpss7):
- Log in with the intobs account (within the OpenWindows
desktop)
- Start the detector and instrument
control systems.
In the orange IDS window (intobs@proteo): DAS5@proteo> obssys
(refer to the whiteboard for the option
number)
DAS5@proteo> startobssys
- In the pink Observing System window:
lpss7> obssys
(same option number as
before)
SYS> startobssys
2. Shutting down the system
| Note:
The TCS and ICS systems are independent, but if you need to restart the
system, you should first shut down the ICS *then* the TCS. Then restart
the TCS followed by the ICS. Doing otherwise might cause you to lose
the apertures for the acquisition camera. |
On the lpss7 computer:
On the inttv computer:
Note: If the TCS is
restarted at any point, the zeroset
of the telescope must be redone.
|
3. Bad Pointing
If stars are not visible on the TV
or appear way off centre, repeat the ZEROSET procedure at zenith. If
the pointing still seems poor, follow this procedure to recalculate the
pointing model:
- Make sure the TV is test on the slit (SYS> tvcenter)
- Select the default pointing model using the command: USER>
cal default
- When
the HANDSET menu appears, center the star on the slit using the cursor
keys. Once centered, hit the HANDSET button again to proceed to next
star.
- Once all seven stars have been centered, a prompt appears
asking if all stars have been centered - answer Y.
- The rms is typically between 2 and 5, answer Y to accept the
result.
- Reacquire the stars with new corrections using the command: USER>
next
4. Closing down fast
- Stop the exposure by typing SYS> finish. If doing
a multrun then it's SYS> abort.
- Switch the TCS to engineering mode: USER> eng
- Close the primary mirror cover.
- At
the same time, the dome can also start to be closed. If the lower
shutter is up, bring it down first: press "LOWER MICRO" while in MAIN
OVER TRAVEL, otherwise "LOWER MAIN". Then "LOWER MICRO" again until it
is fully closed.
- Bring the upper shutter down using the same technique.
- If later you find you will not be opening again, do not forget
to park the telescope. Switch back to computer mode first.
(It's possible to close the dome while in computer mode, by pressing
the DOME SHUTTERS button on the Engineering Console. But remember later
to release it otherwise the dome will not track with the telescope.)
5. Faults - In General
Most of the faults can be cleared by typing:
SYS> shutdownobssys
SYS> startobssys If a sub-system (DAS, TCS or Autoguider) is corrupted
'shutdownobssys' wont help. First the sub-system has to be brought
back, then: SYS> shutdownobssys (if not already done)
SYS> startobssys -- will re-establish contact between the observing system and the
sub-systems. 6. Autoguider window disappears
If the autoguider window disappears, it can be recovered by typing:
SYS> agstart cass 7. Guide camera in the lightpath?
If the light does not go to the
CCD (for example while taking an arc), check that the guide camera does
not obturate the lightpath:
SYS> autopark SYS> tvpark
8. No available guide stars
Sometimes it's not possible to find guide stars near the target
position and for the required Position Angle (PA). When this happens,
the first step one should take is to search with the opposite slit PA
(PA - 180). If this does not resolve the problem and in the case of
long exposures where an
average PA (e.g. average parallactic angle) is usually chosen, small PA changes can be tried (5-10º). If
this also fails, the alternative is to guide manually by opening the
HANDSET tool (F6 on the TCS keyboard) and applying the necessary
corrections to maintain the target over the blue cross inside the slit.
If the target is not visible and there are other stars in the FOV, then
one of them can be used for manual guiding by creating a region around
it and keeping it inside that region during the exposure.
9. Observing at low elevation
If you want to observe at a zenith
distance (ZD) between 57 and 70 degrees (33-20 degrees elevation) then
you need to raise the lower shutter. There will not be any warnings
given from the telescope control, so you will have to check the ZD from
time to time.
- Push the yellow button under SELECT MANUAL CONTROL, labelled
"DOME SHUTRS" to get the control of the shutters.
- On
the engineering rack, under LOWER SHUTTER, push the "RAISE MICRO"
button until the MAIN OVER TRAVEL light underneath goes off.
- Follow
by pushing the "RAISE MAIN" button; while raising, you will hear two
bangs caused by the segments of the shutter catching the next one. Keep
the button pressed until you hear the motor stop. This takes
approximately 30 seconds.
- Depress the "DOME SHUTRS" button, otherwise the dome will no
longer track the object.
You can now observe below 33 degrees elevation. Remember to bring the lower shutter down again when you go to a
new source above 33 degrees elevation. To do this: - Select manual control as before with the "DOME SHUTRS" button.
- Push the "LOWER MAIN" button to bring the shutter down as far
as it goes.
- Push the "LOWER MICRO" button to fully lower the shutter. Keep
the button pressed for approximately 10 seconds to be sure.
- Depress the "DOME SHUTRS" button.
Note:
If the bottom shutter is not fully lowered, then the upper shutter will
not completely seal the dome at the top and rain/wind will penetrate
into the dome.
|
10. Data acquisition problems
'Data acquisition' refers to the
management of an exposure, reading of data from the CCDs and saving to
disk. This may fail in one of several stages, for example:
- Run, Finish, Abort or Re-time commands are not successful
- Run process stops after CCD clearing
- Run spontaneously aborts during readout or transfer to disk
- Transfer to disk does not complete to 100%
- Data on disk is corrupted (e.g. torn frames)
These may or may not be accompanied by a pop-up error
box/alarm. If the error pop-up mentions the (ultra)DAS or "reset the
camera", and you cannot continue observing, then the following
procedure is recommended (pink window):
SYS> dasreset
IDS
(i.e. startobssys is unnecessary) When this completes, try a new run and see if the above fault
reoccurs. If it does, then a lower-level reset of the CCD controller
may be necessary and you need to park the telescope at zenith:
- Power cycle the unit labeled SDSU CCD controller, located to
the left of the cryostat, followed by:
SYS> dasreset IDS
- If this does not resolve the problem, follow the
instructions to shut down the ICS and DAS on the intics screen and then
restart.
11. Problems with IDS control
If the right-hand side of the
mimic shows IDS mechanisms in red, this infers that attempted movements
have either failed or are incomplete. If this occurs the MMS controller
or IDS MMS may need to be power cycled. To do so contact the WHT TO or
your SA. Only they can access the Power Distribution Unit.
12. Problems with Acquisition
Guidance Box (AGB) control
If the left-hand side of the mimic
shows AGB mechanisms in red, this infers that attempted movements have
either failed or are incomplete. If this occurs and the AGB MMS needs
to be power cycled contact the WHT TO or your SA. Only they can access
the Power Distribution Unit to do it.
13. Restarting inttv
If the TV system fails to readout/update, then in the pink window on
inttv:
DAS6@miranda> dasreset AG0
When this completes, try a new TV or 'field' operation. If there
are still problems power cycle the TV CCD controller, followed by
DAS6@miranda> dasreset AG0
If this still does not resolve the problem, try the following:
DAS6@miranda> shutdownag
DAS6@miranda> shutdownobssys
DAS6@miranda> startobssys
DAS6@miranda> startag AG0
DAS6@miranda> bin 3 3
14. Starting up the data reduction
PC
- Log on to the INT Data Reduction PC (INTDRPC1)
Username: intguest Password: ******** (as shown on monitor)
-
Start iraf:
From any terminal window, open an xgterm window ( > xgterm & )
and type:
> iraf (Alternatively, go to the home directory, and type:
> ds9 & [to start
the image display tool]
> ecl [to
start Iraf] )
- In IRAF, move into the "date" directory where the images are
stored. The current date is entered in the format 'yyyymmdd' e.g.
ecl> cd /obsdata/inte/20010225/
15. Restarting the meteorological data
screen
Occasionally the measurements from
one, two or all three of the meteorological stations will fail to reach
the meteorological data screen, leaving all the windows red. If this
continues for more than a few minutes the program can be restated. To
close it type Alt+F4
on the attached keyboard, and reopen by double clicking on the
Meteorological Data Screen icon near the middle of the screen. After a
minute this should update and work as normal.
16. Power cuts
In the case of a power cut, the systems will go on batteries and
moments later the generators will start.
If
this happens the exposure will be interrupted and two alarms will sound
which will have to be acknowledged by pressing a button. One in the
control room, on the Engineering Console, marked with an ACCEPT
sticker. Wait until you're on generator power to do this otherwise the
alarm won't stop. The other is on the ground floor, by the entrance,
opposite to the door and will be flashing red.
Call the WHT TO to know what has happened. After the generators start
it may possible to resume observations.
If you notice the alarm when coming in the afternoon, please let
someone from the Operations Team, INT SA or WHT TO know that the INT is
running on generators.
If later returning to power grid, the control room alarm will sound
again.
17. TCS Communication Issues
In the case of loss of communication between the TCS and the user interface, i.e. if either the TCS USER window stops responding, or the TCS DISPLAY window stops updating, clearing the communications may recover the system:
In the blue band at top of the window, click on Commands --> Clear Communications
18. Cenwave value fluctuating in the IDS mimic
Fluctuations of the central wavelength value at the IDS mimic can be caused by a temporal malfunctioning of the grating encoder. The fluctuating values in the mimic do not mean that the grating actually moves. In case you find this problem, please report the failure to the WHT TO (and at the ING Fault Management System) and continue with your observations.
19. Acknowledgements
Credits should be given to the ING students (2011-2012)
who contributed
recently to improve this manual.
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