Have you familiarized yourself with SMS command set used to control TAURUS-2? If not, please scan the quick-and-dirty SMS guide now. . . .
Next, log in to OBSERVER on aat40a and do a quick system check. This is all you should see. If you happen to catch OBSERVER_1, it does not hang around for very long. If you suspect there are errant processes, type tidy and say yes to any questions. You might want to quickly check that the observer processes you are killing do not belong to some poor sap in coude west, or wherever.
aat40a> sh sys
VAX/VMS V5.5 on node AAT40A 30-AUG-1998
13:36:06.91 Uptime 5 02:18:19
Pid Process Name
State Pri I/O
CPU Page flts Ph.Mem
20400101 SWAPPER
HIB 16
0 0 00:00:37.32
0 0
20400106 CONFIGURE
HIB 9
27 0 00:00:00.04 106
183
20400107 IPCACP
HIB 10
7 0 00:00:00.04 105
173
20400109 ERRFMT
HIB 8 3987
0 00:00:12.61 85
146
2040010A CACHE_SERVER HIB
16 150 0 00:00:00.10
64 121
2040010B CLUSTER_SERVER HIB
9 17 0 00:00:02.85
122 295
2040010C OPCOM
HIB 7 5358
0 00:00:13.55 456
180
2040010D AUDIT_SERVER HIB
10 114 0 00:00:00.67
1365 451
2040010E JOB_CONTROL HIB
9 4554 0 00:00:06.10
160 296
2040010F SMISERVER
HIB 9
34 0 00:00:00.25 284
502
20400110 NETACP
HIB 10 230
0 00:00:01.10 161
376
20400111 EVL
HIB 6
91 0 00:00:01.78 110797
63 N
20400112 LES$ACP
HIB 10 144
0 00:00:00.85 317
684
20400113 REMACP
HIB 8
23 0 00:00:00.05
80 74
20400114 LATACP
HIB 14 11
0 00:00:00.96 271
288
20400115 SYMBIONT_3
HIB 5 58682
0 00:00:08.39 290
177
20400116 SYMBIONT_4
HIB 6
12 0 00:00:00.26 340
96
20400117 BULLCP
LEF 6 141215 0 00:07:40.50
876 849
20400118 MULTINET_SERVER HIB
5 46465 0 00:00:48.06
1431 1065
20400119 SMTP_SYMBIONT HIB
4 10182 0 00:00:47.54
84196 117
2040011A SYMBIONT_6
HIB 5 394
0 00:00:02.21 1963
76
20400376 QUEUE_MANAGER HIB
9 21779 0 00:01:45.22
752 1081
2040057E _VTA70:
LEF 8 1676
0 00:00:07.46 2475 400
204006A5 OBSERVER
CUR 5 950
0 00:00:06.56
aat40a>
xon aatxt?
(?
is a letter like k;
check name at top of terminal)
aat40a>
deckeyshmx (or
"deckeys" if not HMX workstation; only need after terminal reboot)
aat40a>
rvtaurus ccd?(?
is either 1
or 2; check whiteboard
in control room)
What
should greet you now are two windows: a CCD control window and a TAURUS-2
(SMS) control window. When the CCD window
has returned to the idle state, ensure that the cursor is at "startup:"
and hit the ENTER key within the TAURUS window.
| startup: | setup- | run- | operate_ccd- |
| panic_recovery | refresh | maintenance- | finished |
| detector | NONE CCD CCD_SHUFFLE |
| reset_micro | YES NO |
| simulation | OFF ON INTERNAL_ONLY |
| taurus_status_display_terminal | DECW$DISPLAY: |
| taurus_micro_terminal_line | TAURUS_SIF: |
| instrument_seq_terminal_line | INSTSEQ_SIF: |
Select ccd_shuffle and hit the ENTER key. It will take about 5 mins for the main TAURUS-2 report window to come up. In the meantime, type the following commands in the CCD control window.The colours refer to the TAURUS-2 control window or the CCD control window. Recall that the obeyw and load commands are typed after hitting "." (DEL) on the keypad. Of course, you can perform all the same actions with cursor clicks in the SMS control window.
unix_server on (a full description of unix_server is given here)A quick guide to setting up an account on aatssf is given at the bottom of this page.
There is a start up file to set up the most commonly used TAURUS parameters. Hit "." (DEL) on the TAURUS window keypad, and after the ":" prompt, type
The startup.icl file is a little too generic for my taste and may need a lot of editting. What I do is to look for the last start up file that was used, e.g.
We will now do a quick system check to ensure that the CCD, instrument sequencer, TAURUS micro and CS100 are all cross-linked correctly.
CCD charge shuffle multi line
| Csr_Default | disk$user:[observer.cs_files]*.csx |
| Csr_Filename | eighty |
| Preexpose_info | 3_1000_100 |
| Cycle_count | 1 |
| Bias | True False |
| Setup_Array | True False |
| Etalon_Start | 0 |
| Etalon_Increment | 7 |
And this is what you should see:
Figure:
Ne
lamp through R0 (668/21) filter and BTTF at high resolution (Zc=+1,
Zf=0).The RTTF image with the same blocker is essentially identical.
You may be interested to see how we use these image to monitor instrumental stability and to measure six basic system parameters.
Here
are more 80-shuffle examples.
Figure:
CuAr
lamp through R1 (710/26) filter and RTTF at high resolution.
Figure:
D
lamp through R0 (668/21) filter and RTTF at
high resolution (Zc=+1, Zf=0).
The next step is to check the camera focus and plate parallelism.
Fast route. Under aatssf, type the following:
Step by step. Under aatssf, you have access to big scratch areas such as /data_ssf/obsred or /data/ssf/1/obsred. Make a subdirectory called "mkdir ttf", followed by "cd ttf". Now set up iraf with "mkiraf" and answer "xgterm" to the preferred terminal. You will now see the directory "uparm" and file "login.cl" appear in your subdirectory. Edit the latter file and insert a few helpful extra lines. Towards the top of the file, insert "set $stdimage = imt2048" which sets the display window size for "ximtool". At the end of login.cl, and just before the last command, include the word "onedspec" on a line by itself. This pulls in the package with "splot". Of course, you can type all of the commands above within iraf, but then you would need to do this repeatedly every time you enter iraf. Now activate "ximtool &" and iraf using "cl" from the same subdirectory, preferably from an "xgterm" window so that splot works properly, and wait for unix_server to transfer your files.cd /data_ssf/obsred
mkdir ttf
cd ttf
cp ~ttf/iraf/TAR .
tar xvf TAR
chmod +x *
xgterm &
(move into xgterm window and type "cl")