Changes between Initial Version and Version 1 of NightOperations/SciencePlans/20170306


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Timestamp:
Mar 5, 2017 12:38:15 PM (7 years ago)
Author:
shetrone
Comment:

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  • NightOperations/SciencePlans/20170306

    v1 v1  
     1= 20170306 =
     2
     3
     4== Twilight Tests ==
     5
     6Note:  Twilight exposures are critical science calibrations for LRS and VIRUS and if possible should be done every night that science data is taken.
     7
     8 === twilights with VIRUS with different tracker positions ===
     9
     10Purpose:  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.
     11
     12Procedure: 
     13 *  Despite of pressures at the start of the night try to get the twilights.
     14 *  Setup the guide camera for sky twilight (GC2, 0.1 sec, B filter)
     15 *  When you hit the correct flux level (biased to a slight higher value, perhaps 5k) execute the specialtwilight script
     16
     17== On-sky science: ==
     18
     19We have a few changes in procedure that are important to note:
     20
     211)   Use shuffle_config_matt6   
     22
     232)   For LRS2 and LRS2+parallelVIRUS use vlexp code as per normal.
     24
     253)   For VIRUS hetdex fields please use the $HET_SRC_ROOT/integration/hetdex-dither.py script which has the new guider dither method built into it.  Note you will have to put in the actual observation number.   We hope to update vlexp in the near future.  You should look at the help pages to remind you how to specify observations.     Here it is repeated for your reading:
     26
     27{{{
     28$HET_SRC_ROOT/integration/hetdex-dither.py -h
     29usage: hetdex-dither.py [-h] -o OBS -O OBJ [-e EXPT] [--dry-run]
     30
     31Execute a 3-dither HETDEX observation.
     32
     33optional arguments:
     34  -h, --help            show this help message and exit
     35  -o OBS, --obs OBS     Observation number.
     36  -O OBJ, --object OBJ  Object descriptor.
     37  -e EXPT, --exptime EXPT
     38                        Exposure time per dither in s. Defaults to 360s.
     39  --dry-run             Print actions without executing commands on the
     40                        hardware
     41}}}
     42
     43Watch out for the moon brightness at the start of the night.   I am not sure that the automatic moon brightness works in htopx so you should set this manually to make sure you don't hit inappropriate targets or miss targets.    After the moon sets just turn off the moon brightness.
     44
     45At the start of the night please try to hit the PSU17-1-002 targets in the West.  Even if that means a short stack after twilights.
     46
     47During any thin parts of the night (few targets) please try to get your standards.
     48
     49When VIRUS targets are available they generally should have priority over regular targets, at least at the same priority.
     50
     51Watch out for the request telluric standards needed just before or after UT17-1-008!
     52
     53== On-sky engineering: ==
     54
     55This should be the lowest priority but could be done when the moon rises or during a hole in the queue (after standards have been taken).   The priority of the tests is in the order given below.
     56
     57
     58=== Globular cluster dither test with VIRUS ===
     59
     60Purpose:  Now that we have eliminated some of the drag problems we would like to test how dithering looks on VIRUS.    Do this on a globular cluster (GC).   Choose a a very rich wide GC.   Want to put the center of the GC on one of the currently active IFU. 
     61
     62Good globulars that we have used in past, that are up now, are:
     63
     64NGC2419 (probably need 5 minute exposure for this)
     65NGC4147
     66NGC5024 = M53
     67NGC5272 = M3
     68
     69NGC5024 and NGC5272 would be ideal for this even though they are only in the East and CCAS will block some of the light.
     70
     71 * Use do_shuffle to set up on a globular cluster on one IFU
     72 * Have TO setup guiding on '''gc1'''.  This will put the guide probe close to the IFUs and will minimize the guider drag.
     73 * offset the nearest bright star onto the BIB with the probes=true option. 
     74    *  '''It is critical that you get a star on the BIB for this test.'''
     75 * while at dither position 1, start saving bib images (you may have to manually open the PFIP shutter) and get the proper exposure time (try to get exposure x coadd >= 3)
     76 * start saving bib images
     77 * record start time in the log
     78 * Run take a parallel exposure with 120 seconds, virus as the prime and dither = true.
     79 * when dither 3 is complete stop saving bib images
     80 * record end time in the log
     81 * setup on the next IFU.
     82
     83repeat with '''gc2''' to maximize the drift.
     84
     85Here are some suggestions that might help.
     86{{{
     87antigc1
     88mgp -cp
     89
     90convert /home/mcs/astronomer/matttmp/ACAMimages/ngc5024_103_E.png /data1/nossy/www/html/noss/htopx2/acam_dss.jpg
     91syscmd -T -v 'load_trajectory(id=4018, ra=13.2169, dec=18.298265, equinox=2000.0, dir="EAST" )'
     92syscmd -T -v 'Guider1_set_position( ra=13.2134, dec=18.151206 )'
     93mgp -mp
     94echo "starting ngc5024_103" >> mattlog
     95date >> mattlog
     96vlexp -i virus -t sci -texp 120 -pobj ngc5024_103 -sobj ngc5024_103 -dither -B
     97echo "ending ngc5024_103" >> mattlog
     98date >> mattlog
     99
     100}}}
     101
     102=== BIB Drag Test ===
     103
     104 * Make sure your stack is pretty good (RSE < 250)
     105 * Make sure GROC is pretty well set
     106 * Select a 13th mag target near the start of the track for all probes and targetted on BIB using shuffle and shuffle_config_matt4
     107 * Setup on BIB and start guiding on BIB.
     108 * Center up both guide probes and start metrology loops.
     109 * Center up at least one OWFS to watch focus.
     110 * set bib exposure to be not saturated but at least 3 seconds ( e.g. 2 seconds with 2 co-add)
     111 * Record a time, GROC and RSE in the log
     112 * Hit "store images" and "Start Metrology Loop"  for GC1, GC2, WFS1, WFS2, TT, BIB
     113 * '''In this test we should NEVER apply X,Y, or GROC offset corrections'''
     114 * Run until the end of track
     115 * when done, record a time, GROC and RSE in the log
     116
     117Run this at several different Az.   Priorities 40, 330, 30, 340, 20, 350, 10, 0.
     118
     119== Closed dome: ==
     120
     121Please look at the long cals and see if there are any that need doing. 
     122
     123[https://hettrac:8001/trac/WFUCommissioning/wiki/NightOperations/SciencePlans/longcals
     124]
     125