| CAID: MIPS-235 | Title: 160 um Focal Plane Survey (fine) | |
| System: MIPS | Principal: jkeene | Deputy: |
| Objective: | To measure the pixel sizes and the relative locations ( i.e., array orientation, scale and distortion) as a function of scan mirror angle. |
| Description: | This task will duplicate MIPS-234 - adding another repeat. |
| Day: 61.6687500000044 | Suggested Order: R300 | ||
| Must be preceded by these activities (list by CAID): MIPS-234 | |||
| Place in Schedule: After dust cover off. After initial FPS survey and CSMM calibration. | |||
| Priority: Necessary | |||
Conditions | |||
| Maximum telescope temperature: | 6.5 K | ||
| Minimum telescope temperature: | 5.5 K | ||
| Should activity be repeated if focus changes? | No Repeat if focus changes by 0 mm | ||
| Maximum absolute pointing uncertainty: | 3 arcsec (1 sigma radial) | ||
| Maximum precision offset uncertainty: | 1 arcsec (1 sigma radial) | ||
| Observatory configuration: | standard | ||
| Go/No Go criteria: | CSMM, CE, and detectors must be operational, instrument and telescope temperatures must be stable | ||
Duration: 90 minutes
| | Real time downlink:
No | | |||
| Data Volume (uncompressed): 0 Mbits | |||
| List Blocks, AORs, SERs, IERs, or unique sequences required (uplink): IER or perhaps unique IPP file to apply non-standard CSMM offset to otherwise nominal 3x1 raster AOT. | |||
| List Analysis tools required (downlink): Pipeline output. Centroiding of sources in 160um images -> pixel coordinates of those sources. | |||
| Estimate of data turn around: 60 hours | |||
| Description: Map of the 160 mm pixel locations. | |||
| Can proceed in parallel with other activity: No | |||
| Must outcome be confirmed before next activity: No | |||
| Method of Confirmation: Data analysis | |||
| Success criteria: Source appears on array in all observations. | |||
| Contingency plan: Repeat with brighter star and/or integrating longer. Revise offsets from PCRS to 160FOV for CSMM offssets used. | |||
Comments | |||
| References: | |||
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Additional Comments:
This task verifies field distortions on the 160um array, and determines in detail the orientation and location of the array. Results influence reconstruction of scan-map observations primarily. | |||
| This activity last updated: 7/25/2002 1:56:05 PM | |||