From 0fce0e7e8b93c46c50e90e7314baee0dd862e4d6 Mon Sep 17 00:00:00 2001 From: Carlos Quiroz Date: Mon, 4 Dec 2023 16:54:12 -1000 Subject: [PATCH] Update GNIRS blueprint xml --- .../phase2/template/factory/xml/GNIRS_BP.xml | 71 ++++++++++++++----- 1 file changed, 55 insertions(+), 16 deletions(-) diff --git a/bundle/edu.gemini.phase2.skeleton.servlet/src/main/resources/edu/gemini/phase2/template/factory/xml/GNIRS_BP.xml b/bundle/edu.gemini.phase2.skeleton.servlet/src/main/resources/edu/gemini/phase2/template/factory/xml/GNIRS_BP.xml index eef817800b..c8704302ea 100644 --- a/bundle/edu.gemini.phase2.skeleton.servlet/src/main/resources/edu/gemini/phase2/template/factory/xml/GNIRS_BP.xml +++ b/bundle/edu.gemini.phase2.skeleton.servlet/src/main/resources/edu/gemini/phase2/template/factory/xml/GNIRS_BP.xml @@ -2946,7 +2946,7 @@ GNIRS configuration: - + @@ -3096,6 +3096,19 @@ GNIRS configuration: + + + + + If observations in multiple bands are contained within the sequence, for best results: + +Re-acquire after the observation of the source in a given band + associated GCAL calibrations + +There is a possibility that the source can move ~0.1" on the detector when moving back to sky from the GCAL environment due to a number of factors. Since the HR-IFU FoV is small, this can lead to loss of flux with an extended source or a point source that was not originally centered well and/or is observed under poor seeing (without AO). + + + + @@ -3294,7 +3307,7 @@ GNIRS configuration: - + @@ -3437,7 +3450,7 @@ GNIRS configuration: - + @@ -3580,7 +3593,7 @@ GNIRS configuration: - + @@ -3888,7 +3901,7 @@ Note that the target component in the associated spectroscopy observation must b - + @@ -4173,7 +4186,12 @@ Note that the target component in the associated spectroscopy observation must b - If observations in multiple bands are contained within the sequence, for best results, a re-acquisition should occur after the calibrations on a given band. There is a non-repeatability of ~0.1" moving back to sky from the GCAL environment, which can lead to loss of flux with an extended source or a point source that was not originally centered well and/or is observed under poor seeing. + If observations in multiple bands are contained within the sequence, for best results: + +Re-acquire after the observation of the source in a given band + associated GCAL calibrations + +There is a possibility that the source can move ~0.1" on the detector when moving back to sky from the GCAL environment due to a number of factors. Since the HR-IFU FoV is small, this can lead to loss of flux with an extended source or a point source that was not originally centered well and/or is observed under poor seeing (without AO). + @@ -4382,7 +4400,7 @@ Note that the target component in the associated spectroscopy observation must b - + @@ -4532,6 +4550,19 @@ Note that the target component in the associated spectroscopy observation must b + + + + + If observations in multiple bands are contained within the sequence, for best results: + +Re-acquire after the observation of the source in a given band + associated GCAL calibrations + +There is a possibility that the source can move ~0.1" on the detector when moving back to sky from the GCAL environment due to a number of factors. Since the HR-IFU FoV is small, this can lead to loss of flux with an extended source or a point source that was not originally centered well and/or is observed under poor seeing (without AO). + + + + @@ -4787,7 +4818,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -4883,7 +4914,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -4895,7 +4926,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -5087,7 +5118,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -5189,6 +5220,10 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl + + + + @@ -5271,7 +5306,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -5281,6 +5316,10 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl + + + + @@ -5387,7 +5426,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -5491,7 +5530,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -5843,7 +5882,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - + @@ -5919,7 +5958,7 @@ Once you shift the prism, re-read the GNIRS mechanisms file in the cc, and toggl - +