Changes between Initial Version and Version 1 of NightOperations/Commissioning/Plans/20170709

Timestamp:

Jul 8, 2017 8:12:36 PM (7 years ago)

Author:

shetrone

Comment:

--

NightOperations/Commissioning/Plans/20170709

@@ +1 @@
+= 20170709 =
+
+
+== Any new changes: ==
+
+ *  The problems with WCS last night were the crpix1 and crpix2 were set wrong.    We hope this is fixed now.
+ *  We may have fixed the WFS software problem.
+ *  We have a new version of shuffle installed so we are ready to resume testing of non-optimal Az setups.
+ *  Sergey has fixed the auto numbering in cal and vlexp
+ *  pivot on VIRUS now runs vhc automatically.   
+
+== Twilight Tests ==
+
+Note:  Twilight exposures are critical science calibrations for LRS and VIRUS and if possible should be done every night that science data is taken.
+
+ === twilights with VIRUS with different tracker positions ===
+
+Purpose:  There is some interest in seeing what the long term illumination correction changes look like including what different track positions do to them.    The script is "specialtwilight" in /home/mcs/astronomer/bin/.    It takes a single argument which is the Observation number.
+
+Procedure:  
+ *  Despite of pressures at the start of the night try to get the twilights.
+ *  Setup the guide camera for sky twilight (GC2, 0.1 sec, B filter)
+ *  When you hit the correct flux level (biased to a slight higher value, perhaps 5k) execute the specialtwilight script
+
+
+
+== Mirror Team Training ==
+
+We may have the mirror team come in for training on stacking the mirror any night between Friday and Tuesday (probably Saturday for Amanda night and Monday night for Katie).  These should be hands-on experiences with the mirror team actually sitting in the TO chair and running the code, if possible.     This should be a very high priority taking priority over anything but P0 TOO targets and any current trimester dark time science that can be done at the start of the night early next week.
+
+Here are some suggestions that one might consider:[[BR]]
+1)  Save a cur file before stacking[[BR]]
+2)  Push one mirror out a bit so the mirror team can see mirror recovery with HEFI[[BR]]
+3)  Save a 2nd cur file[[BR]]
+4)  Have the mirror team watch as the TO stacks.[[BR]]
+5)  When done stacking apply cur file number 2 [[BR]]
+6)  Have the mirror team stack.[[BR]]
+
+== On-sky science: ==
+
+If we get any TOO targets during the engineering run which can be done with the current moon conditions this would be the highest priority.    Regular science targets should be the lowest priority.
+
+
+== On-sky engineering: ==
+
+This should be the 2nd highest priority (after any TOO targets).  The priority of the tests is in the order given below.
+
+=== Test the WFS ===
+
+Purpose:  To make sure that the WFS is in good working condition.
+
+Procedure: 
+ * Select a star to setup on using do_shuffle.
+ * Setup on the star and get both WFS centered.
+ * Watch the WFS and see if it is stable
+ * Offset focus by 0.15 mm and look for a response from the WFS.
+
+Report any irregularities to Randy.
+
+=== Standards in each IFU ===
+
+Purpose:  We wish to get spectrophotometric standards in each of the IFU if the conditions are near photometric and you are within the middle portion of the track (in tracker X and tracker Y).   Just give the IFU number to shuffle and then setup like a normal HETDEX observation.   Please use the dither script.  The exposure time will vary but will likely be less than 1 minute.   Please check for saturation.
+
+=== Testing of the ACAM position ===
+
+Purpose:  We want to see if the ACAM position changes with respect to the IHMP over time.  We want this data about 2 times per week and when ever we get an unusually high or low temperature. 
+
+Determine the Center of the BIB:
+  *  Select a 14th mag star in a reasonably rich field with shuffle for the BIB
+  *  Setup on the very center of the BIB field of view (79, 98)  and save an image.
+  *  Guide on one of the guide probes
+  *  Put in the ACAM and save an shallow image with the target star not saturated.
+  *  Report on the position of the BIB in the night report and on [wiki:NightOperations/Commissioning/Results]
+  *  Save a deeper image which should show more than a dozen stars.
+
+Determine the Center of LRS2-B
+  *  Select a 14th mag star in a reasonably rich field with shuffle for the LRS2-B
+  *  Setup on LRS2-B and start guiding on one of the guiders
+  *  Take LRS2-B spectrum, probably 60 seconds.  
+  *  Adjust the position so that the star is at the center of LRS2-B IFU using lmap until the offsets are less than 0.3"
+  *  Confirm the star is at the center of the IFU by taking a spectrum.
+  *  Once it is as the center of the IFU put in the ACAM and take a shallow image so that the star is not saturated.
+  *  Report on the position of the LRS2-B in the night report and on [wiki:NightOperations/Commissioning/Results]
+  *  Take a deeper image so that there are large number of stars.
+
+Determine the Center of LRS2-R
+  *  Select a 14th mag star in a reasonably rich field with shuffle for the LRS2-R
+  *  Setup on LRS2-R and start guiding on one of the guiders
+  *  Take LRS2-R spectrum, probably 60 seconds.  
+  *  Adjust the position so that the star is at the center of LRS2-R IFU using lmap until the offsets are less than 0.3"
+  *  Confirm the star is at the center of the IFU by taking a spectrum.
+  *  Once it is as the center of the IFU put in the ACAM and take a shallow image so that the star is not saturated.
+  *  Report on the position of the LRS2-R in the night report and on [wiki:NightOperations/Commissioning/Results]
+  *  Take a deeper image so that there are large number of stars.
+
+Repeat the above tests a few times at different Az to confirm that the positions are good.
+
+=== Testing non-optimal Az setups with do_shuffle ===
+
+Purpose:  We want to test our new features of shuffle for setting up on a non-optimal Az.   
+
+Procedure: 
+ * Use do_shuffle to set up on a field on the IHMP.
+ * after arriving on the target make note of the Az
+ * see if all guide probes and wfs can be setup on the object.
+ * Once the WFS and guiders are setup save an ACAM image.
+ * abort the trajectory
+ * Use do_shuffle with a new fixed az about 5-10 degrees away from the original Az.
+ * after arriving on the target make note of the Az
+ * see if all guide probes and wfs can be setup on the object.
+ * Once the WFS and guiders are setup save an ACAM image.
+ * abort the trajectory
+
+Try the above test a 2nd time but setup on an LRS2 IFU (056 or 066) and then try a VIRUS IFU.
+
+Here is an example:
+{{{
+do_shuffle -v --use_brightness true 16:57:09.05 " -04:06:01.12" 0 1 095 0 0 star1
+
+do_shuffle -v --az 195.7 --use_brightness true 16:57:09.05 " -04:06:01.12" 0 1 095 0 0 star1_az195.7
+}}}
+
+
+=== test RA scripts ===
+
+Auto-numbering:  Please try all modes of the vlexp to see if auto-numbering is working.   Try vlexp on lrs2, virus and parallel.  Also try auto-numbering in cal script with both lrs2, virus and parallel biases.    
+
+VHC:   Please check to see if VHC is running and that data is transferring out of the RAMDISK for virus.
+
+
+
+=== WFS for New setup of PSU17-2-003 ===
+
+Last night Steve determine a guide star that could be used for the A and B setups for this program.   It would be good to determine a WFS that can make the first jump (from the setup star to A or B).  The A and B exposures are very long so using a WFS for this exposure would be good.   The WFS need not make the jump to the sky position and could be unset at the end of the exposure (while taking the acam image).   
+
+
+=== Testing Probe offsets ===
+
+Purpose:  We want to see how accurately we offset using probe offsets with the same tools that we used for the guide probe measurements.    
+
+Procedure:
+ *  Setup on For VIRUS on IFU 095 for Globular cluster ngc6205 in the east early in the track.
+ *  Setup on GC1  (You can also run a WFS to keep good IQ).
+ *  Expose VIRUS for 180 seconds {{{ syscmd -v -V 'expose( seconds=180, x_binning=2, y_binning=1, type="sci", object="ngc6205_095_E", observation=2, exposure=1 )' }}}
+ *  Wait for the shutter to close {{{ syscmd -V 'wait_for_shutter_close(observation=2, exposure=1  )' }}}
+ *  Move to 2nd dither position with a probe offset move {{{mgp -toff=-0.73,1.27 }}}
+ *  Expose VIRUS for 180 seconds {{{ syscmd -v -V 'expose( seconds=180, x_binning=2, y_binning=1, type="sci", object="ngc6205_095_E", observation=2, exposure=2 )' }}}
+ *  Wait for the shutter to close {{{ syscmd -V 'wait_for_shutter_close(observation=2, exposure=1  )' }}}
+ *  Move to 3rd dither position with a probe offset move {{{mgp -toff=1.46,0.0 }}}
+ *  Expose VIRUS for 180 seconds {{{ syscmd -v -V 'expose( seconds=180, x_binning=2, y_binning=1, type="sci", object="ngc6205_095_E", observation=2, exposure=3 )' }}}
+ *  Wait for the shutter to close {{{ syscmd -V 'wait_for_shutter_close(observation=2, exposure=3  )' }}}
+ *  Move back to the start with a probe offset move {{{mgp -toff=-0.73,-1.27 }}}
+
+ *  Repeat the test but guiding on GC2  '''Be sure to change the observation number to 3'''
+ *  Repeat the test but guiding on GC1  '''Be sure to change the observation number to 4'''
+ *  Repeat the test but guiding on GC2  '''Be sure to change the observation number to 5'''
+
+
+
+=== Refinements to pointing ===
+
+we know there is going to be some small errors in the WCS since the RA and DEC when the telescope finally arrives on trajectory (before any TO offsets) does not match the input load trajectory coordinates.   
+
+ * The idea is to try to start a few trajectories from stars pointed to the IHMP.  
+ * Look at the RA and DEC from TCS (can use a monitor or look at a fits header) and compare that to the target RA and DEC.   
+ * Look at the acam and note the position of the target star
+ * Change the telescope position with telescope offsets so that the telescope RA and DEC now read the same as the target RA and DEC.
+ * Has the position of the target star on the ACAM gotten closer to the IHMP?
+
+Try this for a few different Az.
+
+
+=== Confirmation of readiness for science ===
+
+  * Try some different modes of operations.
+      *  VIRUS observing using {{{ hetdex-dither }}}
+      *  LRS2 observing with VIRUS parallel with {{{ vlexp }}}
+      *  Setting up on stars with all probes including WFS
+      *  Doing LRS2-B -> LRS2-R observing.
+
+
+== Closed dome: ==
+
+Please do the following if you are closed (in order of priority):
+
+  *  200 ldls flats for VIRUS
+  *  dark 1800s x3 for LRS2
+
+
+See the long cals page for more information:
+
+[wiki:NightOperations/SciencePlans/longcals]