The focal plane surveys are being done in three phases: pre-coarse, coarse, and fine. The pre-coarse survey is using first light data and early observations (FPS candidate star observations) to find the location of the frame table entries to a goal of 5 arc seconds. The coarse surveys has a goal of finding the frame table entries to an accuracy of about 1 arc second. While the fine surveys have a goal of 0.28 to 0.14 arc seconds.

Focal Plane Survey Summary Updates

CAID Type of Survey: Taskname Campaign Executed Summary IPF report generated Frame Table Updated
100 Pre-Coarse 24 micron:
24 micron first light 		D1 centroided data for all observations
Sent data to IPF team 		ID01P095.pdf FTU 7
130 Coarse 24 micron F centroided data for all observations
Sent data to IPF team 		ID001095.pdf Combined results with 130G:
FTU 10
130 Coarse 24 micron G centroided data for all observations
Sent data to IPF team 		ID101095.pdf
multi-run: ID01M095.pdf 		Combined results with 130F:
FTU 10
322 and 965 Pre-Coarse 70 WF micron:
70 micron First light and FPS candidate Star		 G Centroided data for first light data and bright candidate star
Sent data to IPF team 		ID01P107.pdf FTU 9
966 Pre-Coarse 70 micron NF:
70 micron NF FPS candidate Star		 G Centroided data for candidate star
Sent data to IPF team 		ID01P118.pdf FTU 10
132 Coarse 70 micron WF micron H S/N not adequate to use for FPS, mosaicked data showed star in the center of the image
132 Coarse 70 micron WF micron I S/N not adequate to use for FPS, mosaicked data showed star in center of the image.
137 Coarse 70 micron NF micron I wrong mirror positions, the mosaicked data showed star in center of the image.
967 Pre-Coarse 160 micron
160 micron candidate star		 I S/N not adequate to use for FPS.
139 Coarse SED I data far from slit center
centroided a single image sent to IPF team		 ID002121.pdf FTU 10
234 160 micron Coarse FPS J S/N not adequate for FPS. Could not mosaic because the WCS header values were incorrect.
139 SED Coarse J centroided data and sent to IPF team ID103121.pdf FTU 12
137 70 micron NF Coarse Survey J centroided 59 images and sent to IPF team
Improved centroiding method and sent more centroids to IPF team 		59 centroids: ID102118.pdf
Improved centroids: ID203118.pdf 		1st run: FTU 12
2nd run: FTU 14
234 160 micron Coarse K rough centroiding sent to IPF ID103087.pdf FTU 12
70 Array changes Changed frames so targets are on high S/N side of the array FTU 13
235 160 micron Fine Q centroiding sent to IPF
target affected by spectral leak
redo with different target 		ID502087.pdf FTU 14
133 70 micron W Fine Q centroided data using IDP3 and sent to IPF team ID201107.pdf FTU 14
130 24 micron Fine Q centroided data and sent to IPF team ID502095.pdf
results differed with cam R, V direction 1 arc second
131 24 micron Fine R centroided data and sent to IPF team ID602095.pdf
results differed with cam Q, V direction 1 arc second		 FTU 15
138 70 NF micron Fine R centroided data and sent to IPF team no IPF report, only 2 columns of data
133 70 WF micron Fine R centroided data and sent to IPF team no IPF report, only 2 columns of data
138 70 NF micron Fine V failure of same task in Cam R, did not centroid data
235 160 micron Fine W Corruption of spectral leak - did not centroid data
139 SED X1 centroided data and sent to IPF team ID504121.pdf
Problem with centroids only on 1/2 array, IPF results not used for FTU
235 160 micron Fine 1MC centroided data and sent to IPF team ID803087.pdf FTU 16