Changes between Version 219 and Version 220 of docs/CommissioningPlan

Timestamp:

01/14/22 18:03:58 (3 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan

@@ -144 +144 @@
 ||P2.5||[wiki:/docs/CommissioningPlan/P2.5 SOUL AO system test]||Day||5||C3 + C4||Authorize SHARK-NIR on SX side. Permission to use the Argos Swing Arm. If not the Argos swing arm, RR will be required on the SX side. AO support.||
 ||P2.6||[wiki:/docs/CommissioningPlan/P2.6 NCPA measurements]||Day||8||C3 + C4||Authorize SHARK-NIR on SX side. Permission to use the Argos Swing Arm. When not using the Argos swing arm and for different elevation angle tests, RR will be required on the SX side. AO support.||
-||P2.65 / P3.12 / E1||[wiki:/docs/CommissioningPlan/P3.12 Star center Fourier mode images]||Day||2||C3||Authorize SHARK-NIR on SX side. Permission to use the Argos Swing Arm. When not using the Argos swing arm and for different elevation angle tests, RR will be required on the SX side. AO support.||
-||P2.7||[wiki:/docs/CommissioningPlan/P2.7 Checking pointing offset between SHARK-NIR and SOUL-AO]||Day||1||C3 + C4||Authorize SHARK-NIR on the SX side. RR mounted on the SX side. AO support.||
-||P2.8||[wiki:/docs/CommissioningPlan/P2.8 Science detector calibrations (on the telescope)]||Day||1||C3 + C4||-||
-||P2.9||[wiki:/docs/CommissioningPlan/P2.9 Cryostat warm up check]||Day||2||C3||-||
+||P2.7 / NE1||[wiki:/docs/CommissioningPlan/P2.7 Star center Fourier mode images]||Day||2||C3||Authorize SHARK-NIR on SX side. Permission to use the Argos Swing Arm. When not using the Argos swing arm and for different elevation angle tests, RR will be required on the SX side. AO support.||
+||P2.8||[wiki:/docs/CommissioningPlan/P2.8 Checking pointing offset between SHARK-NIR and SOUL-AO]||Day||1||C3 + C4||Authorize SHARK-NIR on the SX side. RR mounted on the SX side. AO support.||
+||P2.9||[wiki:/docs/CommissioningPlan/P2.9 Science detector calibrations (on the telescope)]||Day||1||C3 + C4||-||
+||P2.10||[wiki:/docs/CommissioningPlan/P2.10 Cryostat warm up check]||Day||2||C3||-||
 ||Total||(4 days of) contingency (15%) included within || ||34 days || || ||
 
@@ -156 +156 @@
 Phase 3 is further divided into 5 runs. Run 1 consists of essential common activities essential for every observing case. This will be the first to be tested on-sky. Run 2-5 blocks represent the nighttime technical commissioning of a set of 17 observing cases. For each of the observing cases, only one target will be tested. The contrast obtained from the data will be used as the merit function or success criterion. If contrast is not an option, a similar (or another) merit function will be used. After the completion of each of these runs, SHARK-NIR will be ready for Phase 4 (science verification) of the respective observing cases.
 
-It is important to note that Run 2-5 are interchangeable. It is currently sorted to have the software complexity in the increasing order and also considering the science interest. Note that "Run N" does not mean that it is the Nth visit to the observatory. For example, Run 1 can be completed in 1 or 2 visits to the observatory, depending on the allotted time. Note also that, for individual runs (2-5), the time taken for other basic activities (such as moving from one target to another, setting up the telescope, closing the AO loop, etc.) are not explicitly mentioned in the table. For example, we anticipate, it may take between 10-20 minutes to move and set the telescope and close the AO loop from one target to another (numbers from the LUCI overheads table). This extra duration required will be mostly covered within the 20% contingency and/or the rounding up of the total nights.
+It is important to note that __Run 2-5 are interchangeable__. It is currently sorted to have the software complexity in the increasing order and also considering the science interest. Note that "Run N" does not mean that it is the Nth visit to the observatory. For example, Run 1 can be completed in 1 or 2 visits to the observatory, depending on the allotted time. Note also that, for individual runs (2-5), the time taken for other basic activities (such as moving from one target to another, setting up the telescope, closing the AO loop, etc.) are not explicitly mentioned in the table. For example, we anticipate, it may take between 10-20 minutes to move and set the telescope and close the AO loop from one target to another (numbers from the LUCI overheads table). This extra duration required will be mostly covered within the 20% contingency and/or the rounding up of the total nights.
 
 Every evening of the nighttime commissioning, all the required calibrations (including dark, bias, flat-field, etc. for all the filters required) will be taken using the SHARK-NIR calibration unit.