IRAC High Precision Photometry
This is a list of potentially useful resources already hosted by the SSC for designing actual observations
- Code to calculate expected signal to noise ratio of any target
- Star- pet: 3.6 & 4.5 micron flux estimator for stellar point sources
- Estimator of predicted transit depth
- Warm IRAC saturation limits (number 11): useful for determing appropriate expsoure times