CAID: MIPS-924 | Title: Routine 160 um Flux Standard | |
System: MIPS | Principal: dhines | Deputy: cengelbracht, dfrayer, SStolovy |
Objective: | Flux Calibration to be done at the beginning and end of every campaign after instrument checkout and calibration has reached a certain level. This task is repeated 4 times with different STIM flash amplitudes to test for linearity in the transfer from DN/s to Jy on the sky. |
Description: | Same basic procedure as MIPS 920, but with stars bright enough to get 25:1 on the photosphere at 160. 160 um flux standard - 11 min Total - 11 min Ph/SR AOT used for all observations. This will be repeated 3 more times but before each repeat, an IER will execute to change the STIM flash amplitude for that AOR. |
Day: 68.2104166666686 | Suggested Order: | ||
Must be preceded by these activities (list by CAID): | |||
Place in Schedule: | |||
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: | 5 arcsec (1 sigma radial) | ||
Maximum precision offset uncertainty: | 0.4 arcsec (1 sigma radial) | ||
Observatory configuration: | |||
Go/No Go criteria: | |||
Duration: 16 minutes
| Real time downlink:
 
No | |
Data Volume (uncompressed): 20 Mbits | |||
List Blocks, AORs, SERs, IERs, or unique sequences required (uplink): | |||
List Analysis tools required (downlink): | |||
Estimate of data turn around: 48 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: | |||
Comments | |||
References: | |||
Additional Comments:
To be scheduled at the beginning and end of every campaign after instrument checkout and calibration has reached a certain level. | |||
This activity last updated: 6/9/2002 11:33:17 PM |