Changes between Version 2 and Version 3 of NightOperations/Commissioning/Plans/20161026
- Timestamp:
- Oct 25, 2016 11:12:14 PM (8 years ago)
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NightOperations/Commissioning/Plans/20161026
v2 v3 35 35 Procedure: 36 36 * Tell the RA that you are going to take the images (will move the probes but won't interfere with anything). 37 * Retract the ACAM and CWFS 37 38 * On a jove terminal Move the probes to the home5 position with the command {{{home5}}} 38 * Save a few 5 secondexposures which are not saturated with both WFS1 and WFS2.39 * Save a few exposures which are not saturated with both WFS1 and WFS2. 39 40 * On a jove terminal Move the probes to the home3 position with the command {{{home3}}} 40 * Save a few 5 secondexposures which are not saturated with both WFS1 and WFS2.41 * Save a few exposures which are not saturated with both WFS1 and WFS2. 41 42 * On a jove terminal Move the probes to the home1 position with the command {{{home1}}} 42 * Save a few 5 secondexposures which are not saturated with both WFS1 and WFS2.43 * Save a few exposures which are not saturated with both WFS1 and WFS2. 43 44 * Move back to the home3 and home5 positions each in a row (this keeps the probes from getting confused and slow. 44 45 * On a jove terminal Move the probes to the home8 position with the command {{{home8}}} 45 * Save a few 5 secondexposures which are not saturated with both WFS1 and WFS2.46 * Save a few exposures which are not saturated with both WFS1 and WFS2. 46 47 47 48 === OWFS on the blue sky as a function of rho === … … 51 52 Procedure: 52 53 * Tell the RA that you are going to take the images (will move the probes but won't interfere with anything). 54 * Retract the ACAM and CWFS 53 55 * Move to center position 0,0,0,0,0 but select rho to be -20 54 56 * Save a few exposures which are not saturated with both WFS1 and WFS2. … … 76 78 Procedure: 77 79 * Tell the RA that you are going to take the images (will move the probes but won't interfere with anything). 80 * Retract the ACAM and CWFS 78 81 * Move to center position 0,0,0,0,0 79 82 * Set exposure times so that WFS1 and WFS2 are not saturating … … 95 98 Purpose: We want to calibrate the OWFS using DWFS8 or CWFS (depending on what stage of the testing we are in, Feedback from Hanshin) on a sidereal trajectory at one of the following Az: 96 99 97 '''a normal star for Az 180, 234, 292, 335, 0''' 100 '''a normal star for Az 180, 234, 292, 335, 0''' We want two more sets of these Az to be complete. 98 101 99 102 * setup on an 11 mag star on the IHMP … … 146 149 * Close the PFIP shutter {{{ syscmd -P -v 'CloseShutter()' }}} 147 150 148 Repeat test: choosing a new star at the next Az in the list: 180, 234, 292, 335, 0. 149 150 151 === doing globular clusters with VIRUS === 152 153 Purpose: We need to fill the IFU with lots of stars. Take a bright GC and move it to four different positions in the IFU array: 084, 085, 094 and 095. '''NOTE: all of the CCAS free GC are in the 1st half of the night.''' 154 155 Procedure: 156 * Select a bright globular cluster near the beginning of track (try to avoid the CCAS tower). 157 * Using do_shuffle put the center of the GC in one of the IFUs 084, 085, 094 and 095. 158 * What ever method is used to setup on the the cluster, save the IHMP clearly in the RA logs. 159 * setup on the target 160 * save an ACAM image to document the setup. 161 * go through a series of dithers with 180 second exposure at each dither. 162 * when done with this setup, setup on the next IFU. '''Note if required this test could be split over nights.''' 163 * contact Karl that the test is complete. 151 Repeat test: choosing a new star at the next Az in the list: 180, 234, 292, 335, 0. We want two more sets of these Az to be complete. 164 152 165 153 == Science with LRS2-R and VIRUS Engineering ==