MIPS_150a 24um Throughput


IOC-MIPS_150a     10560C,10700C            
Title:   Determination of MIPS Radiometric Throughput at 24um              
                   
Objective:   Measure the fluxes of known celestial objects to calibrate the absolute throughput.              
                   
Description:                  
including flow / state diagram                  
      For each module and mode in MIPS, a celestial standard will be observed.            
      At 24 microns a nominal sensitivity of 100:1 will be achieved.            
      The observed fluxes will be compared to the modelled throughput of MIPS            
      and will be used to update subsequent estimates of sensitivity and integration times required .            
                 
      I. Throughput in Scan Map mode            
        Make scan maps at each scan rate (slow,medium,fast)          
      Repeat the fast scan rate map to insure ~35sec integration.          
        Use the scan map AOT.          
      II. Throughput in Photometry Mode            
        Place star on the 24um array . Take data in a 12 position          
        dither pattern using 3,10, and 30 secs exposure at          
        at each position. Repeat the entire pattern a total of 3 times.          
        Use the photometry AOT.          
                   
Required Conditions:     MIPS detector aliveness and electronics checks must have been performed.            
      Pointing must support placing a star in the central 50% of the array.            
      For 24um, background must be less than 4.0e-6 W/m^2/sr.            
      or T<38K            
                   
Resources: duration (best estimate)         1 hr      
  real time downlink (Y / N)         No      
  special post event actions (Y / N)         No      
  Generates ~234 DCEs depending on the amount of ovescan.                
                   
Outcome:                  
  description         Revised throughput numbers      
  can proceed in parallel with other activity         No, dedicated observing.      
  must outcome be confirmed before next event / test /activity         Outcome must be confirmed before tests of ultimate sensitivity can      
            be executed.      
  method of confirmation (sensor TLM, data analysis, etc.)         Data analysis      
  estimate of data turn around if required for confirmation         48 hrs      
                   
Unique or included in planned AOT?                  
      Planned AOTs but with non-standard pipeline processing as calibration data            
      will not yet be available            
                   
Contingency Plan:                  
"What if..."     If throughput is radically different than pre-launch estimates, further analysis and            
      tests to pin point the nature of the problem will be required (eg., are other instruments            
      affected similarly, are backgrounds as expected and so on).            
                   
IOC Critical     Y            
                   
References:                  
                   
Template last updated:     7-Sep-99            
      M. Rieke            
                   
                   


Last Updated on 10/7/99
By Marcia Rieke
Email: mrieke@as.arizona.edu