Cookbook for MIPS-2010: Tracking Flat (24micron) and IC (Ge:Ga) Measurements

Principal: Almudena Alonso
Deputy: Karl Gordon
Data Monkey(s):
Priority:
Downlink Priority: Normal
Analysis Time: Entire duration of IOC and SV
Last Updated: 

Objective

To track quality of Flatfields (24micron) and Illumination Corrections (70, 160micron) taken during IOC and SV.

Description

Flatfields and IC will be obtained during every campaign in IOC and SV as part of the calibration routines. This meta-task will track the qualitiy of such flatfields and ICs taken with tasks: MIPS-914, 915, 916, 917, 918, 919, 305, 306, 307 and MIPS-313 (fine-scale 70 micron ICs). Since flatfields and ICs will be observed using different regions of the sky, this meta-task will also be used to track the quality of regions used. For instance we will answer questions such as: do the chosen regions of the sky produce enough S/N? Does the Region of sky saturate at one or more wavelengths?  Are there bright sources in FOV? etc.

Data Collected

Data Reformatting Requirements

Array Data Desired:
 
Data Reformatting Option:
Special Instructions:

Task Dependencies

Calibration Dependencies

Output and Deliverable Products


Flatfield/IC S/N (statistical quality) in terms of number of DCEs.
Comparison of quality of Flatfields/ICs obtained in photometry and scan modes.
We will construct "super-flatfields and super-ICs" with high S/N. According to simulations:

at 24microns 40-60DCEs or more DCEs (depending on zodi brightness) will produce flatfields to better than 0.5%RMS
at 70micron 200DCEs or more will produce Ics to better than 0.5%
at 160microns we will need ~500DCEs to produce an IC to better than 1%

Data Analysis

Software Requirements

Actions Following Analysis

Failure Modes and Responses

Additional Notes