Attachment 'Pako_helpv10.txt'
Download 1 PAKO preparation for 2012 run5
2 -------------------------
3 ; v9 is at the start of 2012 (copy of v8)
4 ; v10 is rearranged v9 for the preparation of November 2012, run5
5
6 --------- XEphem usage -------------------------------------------------
7 !! preliminary: if you want to use xephem with the position of the telescope displayed in real time
8 ! run the following sequence from the command prompt
9 slogin mrt-lx3
10 ps xa |grep azElToXephem.py & ! check if the script is already running, if not do the following
11 useNCS
12 azElToXephem.py &
13 ! once the script is running type:
14 /vis/xephem/xephem
15
16 ------- Managing Imbfits file -----------------------------------------------
17 ; Telescope fits are in mrt-lx1
18 /ncsServer/mrt/ncs/data/imbfits/
19 het or bol
20 ; There is a script to copy imbfits files locally e.g.
21 ; Backup_telescope.bash
22 ; Edit that file
23
24 ; To process NIKA raw data files onto fits files and imbfits files
25 ; log in sami on a dedicated window
26 idl
27 convert_fits_files2
28
29 ---------- Pako usage ----------------------------------------------
30 !!!!
31 Interface to NCS
32 Summary of PAKO user's manual
33
34
35 ! starts a comment line
36 - command is continued
37 @ filename to execute the script filename
38
39 ; To start pako
40 ssh t21@mrt-
41 gopako
42 pakodisplay
43 pako
44
45 !!! Check that the NCS knows the current project is t21
46 !!! otherwise the telescope will not obey you pako commands !
47 !!! --> look at the OperatorControl screen and/or ask the operator
48
49 set project t21
50 set pi "Alain"
51 set observer "Nika observer" ! your name here, Nika needs you
52
53 ! If not sending commands (outside normal run) do:
54 SET DOSUBMIT NO
55
56 SET LEVEL 0 0 ! very verbose
57 SET LEVEL 1 1 ! chatty
58 SET LEVEL 3 3 ! less
59 SET LEVEL 5 5 ! none
60
61 ! Choose one of the 2 azimuth topology possibilities to decide on which end of the
62 ! azimuth overlap you want to set the origin of the 360 degrees azimuth circle
63 ! May be usefull to avoid a complete turn (>8min) to go from one source ot another
64 SET TOPOLOGY LOW ! selects to use the azimuth range 60 to 420 degrees
65 SET TOPOLOGY HIGH ! selects to use the azimuth range 100 to 460 degrees
66
67 SET ANGLEUNIT arcsec ! make sure angle units are arcsec.
68
69 ! Remember to reset offsets!
70 !!!!!!!!!!!!!!!!!!!!!!!!!!!!!
71 OFFSETS /Clear
72
73 ! total power (no secondary wobbler)
74 SWTOTAL
75
76 ! Choose a well known heterodyne instrument or bolometer for pointing purpose
77 ! ASK Samuel
78 RECEIVER /CLEAR
79 !
80 ! RECEIVER BOLO ! set pointing mobel of MAMBO2
81 !! Normaly the default backend for bolo is ABBA (MAMBO2 backend) but thide doesn't exist anymore
82 !! As a consequence NCS does not record FITS files !!!
83 !
84 ! Attention if there's an incompatibility between RECEIVER and BACKEND IMBFITS are not created either !!!
85 ! So do can't choose a heterodyne backend with bolo.
86 ! To do for Oct 2011 (will be different in the future when NIKA will be integrated to Pako):
87 RECEIVER E090 /Default
88 BACKEND /Clear
89 BACKEND BBC /Default
90 !
91 ! prepare a catalog
92 ! NIKA.sou (see wiki web) to put in the directory :
93 ! t21/pako
94
95 ! Choose a catalog with a .sou extension
96 CATALOG SOURCE NIKA
97 HELP source
98
99 ! select a source
100 ! No case matching, but name must be full
101 SOURCE W3OH
102
103 ! or a planet
104 SOURCE Mars
105
106 ! to check the catalog
107 HELP SOURCE
108
109 ! Catalog of Pointing source from IRAM
110 CATALOG SOURCE iram-J2000
111
112 ! Once you have entered an observing mode (See below)
113 ! if you want that the telescope executes your commands do no forget
114 SET DOSUBMIT YES
115
116 ! start an observation (MAKE SURE you want that)
117 START
118 ! (if you still have DOSUBMIT NO, nothing happens, but the commands
119 ! are in the queue and they will be executed when SET DOSUBMIT YES)
120
121 !!!!!!!!! Observing modes !!!!!!!
122
123 ! procedure to focus
124 ! to set focus
125 SET FOCUS 0
126
127 ! On the fly mode (cover all array pixels) for pointing and alignment. Expensive.
128 OTFMAP -180 -180 180 -180 - ! offsets at start and end of first otf subscan
129 /notf 61 ! number of subscans
130 /step 0 6 ! steps between subscans in arcsecond
131 /system truehorizon ! projection AzEl is used to define the map
132 /totf 36 ! time of a subscan
133 /zigzag ! go back and forth
134 /reference no ! not necessary except if there's a conflict with /system
135
136 !! Attention to the tracking speed (= subscan length / totf) if you choos >10"/s keep an eye
137 !! on the tracking errors trackAz and trackEl in real time on the telescope control screen
138 !! this information is also stored in the FITs files
139
140 ! Correct pointing to center on the array by giving a and b
141 OFFSET a b /SYSTEM Nasmyth
142
143 ! correct the focus
144 SET FOCUS -1
145
146 ! Small map to check the focus quickly
147 OTFMAP -48 -48 48 -48 - ! offsets at start and end of first otf subscan
148 /notf 17 ! number of subscans
149 /step 0 6 ! steps between subscans in arcsecond
150 /system truehorizon ! projection AzEl is used to define the map
151 /totf 10 ! time of a subscan
152 /zigzag ! go back and forth
153
154 ! 4 switching modes (3 useful for bolometers)
155 ! total power
156 SWTOTAL
157 ! Beam switching
158 SWBEAM
159 ! wobbler switching negAmplitude posAmplitude 0.6 seconds per phase!
160 SWWOBBLER -30 +30 /TPHASE 0.6
161
162 ! Observing modes
163 CALIBRATE
164
165 ! pointing cross of given length (in trueHorizon system)
166 POINTING 120
167
168 ! skydip
169 ! stop wobbler
170 SWTOTAL /tphase 0.6
171 ! tip at azimuth 180, scan airmass from 1.1 to 4.1 by steps of 0.6
172 TIP 180 /airmass 1.1 4.1 0.6 /tsubscan 12.0
173
174 ! position switching
175 ONOFF !
176 ! example (give ON offsets and OFF offsets, 2 positions each, 2 systems)
177 ONOFF 30 40 /reference -600 -700 projection /SYSTEM projection
178 ! other options (30 seconds per subscan):
179 /nsubscans 12 /symmetric /tsubscan 30
180
181 ! projection is RADEC system here
182 ! can use /SYSTEM trueHorizon too
183
184 ! if wobbler on use the following special mode
185 ! in that case the off position is automatically on the off wobbler position
186 ONOFF /swwobbler /nsubscans 12 /symmetric /tsubscan 30
187
188 ! not used by bolometers
189 TRACK
190
191 ! everything in J2000
192 ! x=(l-lsource)*cos(b)
193 ! y=b-bsource
194 ! to define the source
195 SOURCE
196 ! if needs to offset from source use
197 OFFSET a b /SYSTEM projection
198 ! then it is in x and y as above
199
200 ! or
201
202 OFFSET a b /SYSTEM trueHorizon
203 ! then Delta az= (az-azsource)*cos(elev)
204 ! and Delta el= elev-elevsource
205
206 ! or
207 OFFSET a b /SYSTEM Nasmyth
208
209 ! Remember to reset offsets!
210 !!!!!!!!!!!!!!!!!!!!!!!!!!!!!
211 OFFSETS /Clear
212
213 !options
214 /t... refers to time
215 /n... refers to number
216 /f... refers to frequency
217 /temp... refers to temperature
218
219 ! See example of startup p21
220
221 ! Pointing
222 SWBEAM
223 POINTING /default
224 START
225
226 ! Set the corrections
227 SET POINTING 3.4 -1.2
228
229 ! Focus (length in mm)
230 FOCUS 2 /nsubscans 6 /tsubscans 12
231 START
232
233 ! enter the correction
234 SET FOCUS -2.1
235
236 ! Useful in a script
237 PAUSE "Sequence Something OK to start ? [c/q]" ! a chance to check
238
239 ! and also
240 SAY " blabla "
241
242 ! save last command
243 SAVE name
244 ! retrieve a command
245 @ command_name
246
247
248 ! To erase graphics in greg
249 Clear
Attached Files
To refer to attachments on a page, use attachment:filename, as shown below in the list of files. Do NOT use the URL of the [get] link, since this is subject to change and can break easily.You are not allowed to attach a file to this page.