Changes between Version 87 and Version 88 of PublicPages/MayallZbandLegacy/NotesforObservers
- Timestamp:
- Feb 10, 2016 8:13:04 PM (9 years ago)
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PublicPages/MayallZbandLegacy/NotesforObservers
v87 v88 105 105 Log into the mzls account on the mayall-idl machine. 106 106 107 Update the code, log files and most importantly the tile file: 107 Update the code, log files and most importantly the tile file: (if people have been working on the code and tile file during the day, this step may not be necessary) 108 108 {{{ 109 109 cd ~/products/mosaic3 … … 197 197 2. Take 10 zero exposures [[BR]] 198 198 3. Turn on low dome flat field lamps at 100% intensity (~50V) [[BR]] 199 4. Create a dome flat script using the NGUI interface. Exposure times as follows: [[BR]] 199 4. Create a test script using the NGUI interface to take a 5 second exposure through the zd filter. Run this with TEST.sh in the exec/ directory, and check that the counts you receive are ~9000 ADU in the real-time display. If they are much higher, you will want to adjust the lamp intensity or flat field exposure time to compensate. [[BR]] 200 5. Look for the script DFLATS_MZLS_zd.sh in the exec/ directory and run it if it exists. You can also create your own dome flat script using the NGUI interface. Exposure times as follows: [[BR]] 200 201 z-band : 20 sec [[BR]] 201 202 r-band : 25 sec [[BR]] … … 207 208 = [8] Just before observing = 208 209 209 1. Start the automated script for updating the tile file210 1. Start the may all-idl:1 VNC session. This session should automatically start MUPTILES and MOSSTAT. If it doesn't, open a terminal in the VNC session and start the automated script for updating the tile file: 210 211 211 212 The FITS file listing which tiles have been completed should be updated throughout the night. … … 233 234 234 235 1. Take a zero image to ensure everything is working 235 2. At start of night, check telescope pointing and zero the telescope coordinates using a bright star placed on the telescope boresight (defined as the center of the mosaic3 focal plane). 236 3. Move to the beginning of the first MzLS tile position 236 2. At start of night, check telescope pointing and zero the telescope coordinates using a bright star placed on the telescope boresight (defined as the center of the mosaic3 focal plane). When taking the image of the bright star, make sure to create an OBJECT script with NGUI (not a TEST, because MOSSTAT will ignore it), zd filter, 1 - 5 sec exposure. Watch for MOSSTAT to process the image and report the RA, Dec offsets. Give these offsets to the OA with **opposite** sign. You can take another OBJECT frame if you want to check to make sure the offset went in the right direction. 237 3. Move to the beginning of the first MzLS tile position. What position is that, you ask? One way to find out is to run mosbot.py (see step 5 below), and look for RA, DEC in expose-1.sh in the exec/mosbot/ directory. Tell these coordinates to the OA to move the telescope. 237 238 4. Focus the telescope 238 - create a focus script using the NGUI 239 - create a focus script using the NGUI: exposure time 5 or 10 seconds, zd filter, -100 micron focus steps, click Midpoint to *on*, 9 exposures. 239 240 - run the focus script from the /home/observer/exec directory 240 241 - analyze the focus image using mscstarfocus 241 242 - edit the mscfoc.cl script to correct the name of the image that needs to be analyzed 242 - mark about 10 stars around the image; mark the top star in eachsequence using "m"; "q" to quit243 - mark about 10 stars around the image; to get a quick idea if you have covered the right focus range mark "g" on the top star in a sequence which will pop up a graph that you will need to type "q" to get out of; mark the top star in each remaining sequence using "m"; "q" to quit 243 244 - log the Truss temperature 244 - set the telescope focus 245 - set the telescope focus in the Configuration Monitor: Enter the value in Pedestal focus, **hit return**, and then hit Apply. If you forget the return, it will do nothing. 245 246 - focus the guiders; this way you can use the guider images to monitor focus drifts 246 247 … … 259 260 See [wiki:MayallZbandLegacy/NotesforObservers/MosBot] 260 261 262 Note that if you need to escape the script at some point during the night (see below), you will need to CTRL-C to stop mosbot.py and **restart** it when you are ready to start up again. If you forget this, you will be observing tiles that you already observed earlier in the night. 263 261 264 6. From the observer@mayall-3 xterm window, start taking exposures using the top-level observing script (tonight.sh): 262 265 {{{ … … 277 280 See [wiki:MayallZbandLegacy/NotesforObservers/Copilot] 278 281 279 8. Monitor focus by checking the image quality on each frame. Keep track of the truss temperature variation and modify the focus as needed. The Mayall has astigmatism, so one cantell from the shape of the images which way to move the focus. To stop and do a focus sequence:282 8. Monitor focus by checking the image quality on each frame. Keep track of the truss temperature variation and use the information to modify the focus as needed. Note that the focus may not respond quickly to changes in temperature, so monitor the images carefully before adjusting focus. The Mayall has astigmatism, so one can sometimes tell from the shape of the images which way to move the focus. To stop and do a focus sequence: 280 283 - Create a file to tell obsbot to quit 281 284 {{{ … … 285 288 - Run a focus sequence (DESCRIBE THIS) 286 289 - [wiki:MayallZbandLegacy/NotesforObservers/FocusInfo Example of a focus sequence] 287 - Re-start the observing as described above. * IMPORTANT* make sure to re-run `mosbot.py` so that you don’t repeat exposures from the beginning of the night!290 - Re-start the observing as described above. **IMPORTANT** make sure to re-run `mosbot.py` so that you don’t repeat exposures from the beginning of the night! 288 291 289 292 Keep an eye on the CCD and dewar temps (should be around 173C and 90C respectively)