CAID: MIPS-241 | Title: 70 um spectral leak check | |
System: MIPS | Principal: mrieke | Deputy: krs |
Objective: | To check the MIPS filters for short-wavelength leaks. |
Description: | Place a bright star in the FOV of the 70um array. Scan the mirror in small steps (1/4 pixel) for a total of 80 steps to obtain the 1D PSF. Repeat at different spacecraft offset for redundancy and repeat using a much colder object. |
Day: 45.8763888888934 | Suggested Order: H400 | ||
Must be preceded by these activities (list by CAID): MIPS-322, MIPS-121 | |||
Place in Schedule: After dust cover off | |||
Priority: Critical | |||
Conditions | |||
Maximum telescope temperature: | 12 K | ||
Minimum telescope temperature: | 5.5 K | ||
Should activity be repeated if focus changes? | Yes Repeat if focus changes by 0 mm | ||
Maximum absolute pointing uncertainty: | 10 arcsec (1 sigma radial) | ||
Maximum precision offset uncertainty: | 10 arcsec (1 sigma radial) | ||
Observatory configuration: | pointing at a star | ||
Go/No Go criteria: | Scan mirror and array readout must be functional. | ||
Duration: 50 minutes
| Real time downlink:
 
No | |
Data Volume (uncompressed): 3 Mbits | |||
List Blocks, AORs, SERs, IERs, or unique sequences required (uplink): Specialized IET | |||
List Analysis tools required (downlink): Data analysis of the PSF power spectrum to detive the high frequency components | |||
Estimate of data turn around: 48 hours | |||
Description: Scans of 1-D PSF at 70um taken with hot and cold sources | |||
Can proceed in parallel with other activity: No | |||
Must outcome be confirmed before next activity: No | |||
Method of Confirmation: Data analysis | |||
Success criteria: obtained well-exposed data | |||
Contingency plan: Repeat with different star, change integration time | |||
Comments | |||
References: | |||
Additional Comments:
Must be careful in choosing stars as saturation must be avoided and extended sources must be avoided | |||
This activity last updated: 7/2/2002 3:36:30 PM |