CAID: MIPS-337 | Title: 160 um PSF | |
System: MIPS | Principal: krs | Deputy: dhines |
Objective: | Characterize the MIPS 160 micron PSF |
Description: | A bright stellar PSF will be moved in a 1x3 grid of positions over the 160 micron array. At each position 3 sec integrations will be taken in an 8x8 grid stepping by 1/4 pixel, in order to sub-sample the PSF. |
Day: 85.6763888888963 | Suggested Order: W100 | ||
Must be preceded by these activities (list by CAID): MIPS-307, MIPS-324 | |||
Place in Schedule: | |||
Priority: Desired | |||
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: | 0 arcsec (1 sigma radial) | ||
Maximum precision offset uncertainty: | 0 arcsec (1 sigma radial) | ||
Observatory configuration: | |||
Go/No Go criteria: | |||
Duration: 45 minutes
| Real time downlink:
 
No | |
Data Volume (uncompressed): 46 Mbits | |||
List Blocks, AORs, SERs, IERs, or unique sequences required (uplink): | |||
List Analysis tools required (downlink): | |||
Estimate of data turn around: 0 hours | |||
Description: | |||
Can proceed in parallel with other activity: No | |||
Must outcome be confirmed before next activity: No | |||
Method of Confirmation: | |||
Success criteria: | |||
Contingency plan: repeat with brighter/fainter star | |||
Comments | |||
References: | |||
Additional Comments:
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This activity last updated: 7/2/2002 4:53:59 PM |