3.5m
Differences
This shows you the differences between two versions of the page.
| 3.5m [2022/03/11 16:35] – created holtz | 3.5m [2026/01/30 05:45] (current) – external edit 127.0.0.1 | ||
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| - | ===== Telescope, etc. information ===== | + | ===== Telescope information ===== |
| + | |||
| + | The ARC 3.5m telescope is controlled using the [[https:// | ||
| + | which is software written in Python using a Tk graphical interface. | ||
| + | |||
| + | The telescope can also be controlled with command line commands and scripts, which | ||
| + | can be run through TUI. TUI includes some built-in scripts, but users can also provide | ||
| + | their own. | ||
| ==== How To Track Solar System (Or Otherwise Moving) Objects ==== | ==== How To Track Solar System (Or Otherwise Moving) Objects ==== | ||
| Line 5: | Line 12: | ||
| Steps 1 and 2 are advance preparation before your observing run. | Steps 1 and 2 are advance preparation before your observing run. | ||
| - | 1) Get raw ephemerides from JPL Horizons | + | 1) Get raw ephemerides from JPL Horizons. |
| - | + | | |
| - | These are more accurate than our in-house ephemeris program can provide. | + | |
| - | Go to the Horizons page (http:// | + | |
| - | web-interface | + | |
| - | for each target of interest: timestamp, astrometric RA and Dec (airless, | + | |
| - | in decimal degrees, J2000.0), RA and DEC rates. You can get additional | + | |
| - | info if you want, but those are the ones that we really need. | + | |
| - | + | ||
| - | Example settings for JPL ephemeris | + | |
| - | + | ||
| - | Ephemeris Type [change] : OBSERVER | + | |
| - | + | ||
| - | Target Body [change] : Saturn [699] | + | |
| - | + | ||
| - | Observer Location [change] : Apache Point [705] ( 254°10' | + | |
| - | + | ||
| - | Time Span [change] : Start=2008-04-24, | + | |
| - | + | ||
| - | Table Settings [change] : QUANTITIES=1, | + | |
| - | + | ||
| - | Display/ | + | |
| Then Generate Ephemeris, which outputs something like: | Then Generate Ephemeris, which outputs something like: | ||
| + | < | ||
| Date(UT)HR: | Date(UT)HR: | ||
| - | |||
| $$SOE | $$SOE | ||
| - | |||
| ..... Daylight Cut-off Requested .....< | ..... Daylight Cut-off Requested .....< | ||
| - | |||
| 2008-Apr-24 02:00:00 C 154.3057447 12.5867617 -2.52 0.61 | 2008-Apr-24 02:00:00 C 154.3057447 12.5867617 -2.52 0.61 | ||
| - | |||
| 2008-Apr-24 03:00:00 A 154.3050264 12.5869290 -2.52 0.60 | 2008-Apr-24 03:00:00 A 154.3050264 12.5869290 -2.52 0.60 | ||
| - | |||
| 2008-Apr-24 04:00:00 154.3043103 12.5870917 -2.51 0.58 | 2008-Apr-24 04:00:00 154.3043103 12.5870917 -2.51 0.58 | ||
| - | |||
| ... | ... | ||
| - | |||
| ..... Daylight Cut-off Requested .....< | ..... Daylight Cut-off Requested .....< | ||
| - | |||
| $$EOE | $$EOE | ||
| + | </ | ||
| - | 2) Massage ephemerides into the format you want | + | 2) Write a script to convert the ephemeris numbers into the correct command |
| - | + | ||
| - | Write a script to convert the ephemeris numbers into the correct command | + | |
| syntax. The BIG, IMPORTANT difference is that JPL gives dRA and dDec in | syntax. The BIG, IMPORTANT difference is that JPL gives dRA and dDec in | ||
| arcsec/ | arcsec/ | ||
| DIVIDE THE SPEED BY 12960000 or you will get no data and track the | DIVIDE THE SPEED BY 12960000 or you will get no data and track the | ||
| - | telescope into the ground. | + | telescope into the ground. |
| - | also where you would substitute Jupiter' | + | |
| - | moon's velocity. The timestamps aren't needed in the command, but it's | + | |
| - | useful to make a file with multiple commands, each one marked by a | + | |
| timestamp so as to pick a command depending on what time one actually | timestamp so as to pick a command depending on what time one actually | ||
| - | issues the slew command. Here' | + | issues the slew command. Here' |
| + | < | ||
| + | tcc track 136.72666, | ||
| tcc track 136.72666, | tcc track 136.72666, | ||
| - | ^ | + | tcc track 136.72478, |
| + | </ | ||
| where the first four numbers are: RA(decimal degrees), | where the first four numbers are: RA(decimal degrees), | ||
| - | Here are a couple of example lines: | + | From the JPL ephemeris example above, one line would convert to: |
| - | 12:00: tcc track 136.72666, | + | < |
| - | + | ||
| - | 12:15 tcc track 136.72478, | + | |
| - | + | ||
| - | From the JPL ephemeris | + | |
| 2008-Apr-24 04:00:00 154.3043103 12.5870917 -2.51 0.58 | 2008-Apr-24 04:00:00 154.3043103 12.5870917 -2.51 0.58 | ||
| tcc track 154.3043103, | tcc track 154.3043103, | ||
| + | </ | ||
| - | 3) Slew to the planet with desired rate and rotation | + | 3) Slew to the planet with desired rate and rotation. |
| Notify the observing specialist that you are about to issue a | Notify the observing specialist that you are about to issue a | ||
| non-sidereal tracking rate to the telescope and get their permission to | non-sidereal tracking rate to the telescope and get their permission to | ||
| do so before doing the following. If the slew rate is wrong it can cause | do so before doing the following. If the slew rate is wrong it can cause | ||
| the telescope to slew too fast, and the observing specialist can stop | the telescope to slew too fast, and the observing specialist can stop | ||
| - | the telescope before it goes out of control. The telescope | + | the telescope before it goes out of control. The telescope |
| - | check your numbers. When in doubt, ask the observing specialist to | + | automatically |
| double check your numbers and they can issue the tcc track command for | double check your numbers and they can issue the tcc track command for | ||
| - | you as well [http:// | + | you as well. |
| Paste your pre-prepared commands into the TUI Log window. When in doubt | Paste your pre-prepared commands into the TUI Log window. When in doubt | ||
| about anything (if your offsets get tangled up, for example), reslew. | about anything (if your offsets get tangled up, for example), reslew. | ||
| This is the motivation for making all those pre-prepared commands. They | This is the motivation for making all those pre-prepared commands. They | ||
| - | WILL come in useful. | + | **will** |
| - | 4) Take images often to see what's going on | + | 4) Take images often to see what's going on. This is just generally good policy. It should be safe to run the guider |
| - | + | ||
| - | This is just generally good policy. It should be safe to run the guider | + | |
| even if you have a non-stellar tracking rate. | even if you have a non-stellar tracking rate. | ||
| - | |||
| - | Last updated 12-20-2007 JMD | ||
| ==== Some useful observing object catalogs ==== | ==== Some useful observing object catalogs ==== | ||
| Line 110: | Line 85: | ||
| ==== Useful Observing Resources ==== | ==== Useful Observing Resources ==== | ||
| + | |||
| + | [root@astronomy pages]# vi start.txt | ||
| + | [root@astronomy pages]# vi 3.5m.txt | ||
| + | [root@astronomy pages]# vi tui.txt | ||
| + | |||
| + | ==== TUI information ==== | ||
| + | |||
| + | Some (probably obsolete!) information about building TUI from source | ||
| + | on a Linux machine. | ||
| + | |||
| + | === Python dependencies for linux users === | ||
| + | |||
| + | TUI has strict python dependencies. | ||
| + | displaying guider or slitviewer images because they have the wrong | ||
| + | version of one or more packages. | ||
| + | running it from the wrong directory might result in a different | ||
| + | package being loaded. | ||
| + | vary widely, the same solution might not work for everyone. | ||
| + | here are some solutions that have worked for some people. | ||
| + | |||
| + | === Pre-built TUI 2.6.0 === | ||
| + | |||
| + | Download a copy of TUI pre-built for linux as of December 2017 at | ||
| + | |||
| + | http:// | ||
| + | |||
| + | Future TUI versions will be linked from the TUI-images web page so | ||
| + | be sure to check there also. | ||
| + | |||
| + | === Install from the ground up === | ||
| + | |||
| + | |||
| + | - install miniconda2 using the usual installer | ||
| + | - in miniconda2/ | ||
| + | - create a file " | ||
| + | - in miniconda2/ | ||
| + | - add line "numpy ==1.8.2" | ||
| + | - in miniconda2/ | ||
| + | - in miniconda2/ | ||
| + | - in miniconda2/ | ||
| + | - in miniconda2/ | ||
| + | - in miniconda2/ | ||
| + | |||
| + | |||
| + | === Forcing package version at runtime === | ||
3.5m.1647016544.txt.gz · Last modified: by holtz
