References for data used in current DOLPHOT module

- Zero Points: ABmag from STIPS Development Team et al. (2024) PASP 136 124502.  Note, these zero points are approximately 0.04 magnitudes higher than those implemented in STIPS v2.2.2.  VegaMag from STIPS v2.2.2 outputs, aside from F213 (not implemented in STIPS v2.2.2) which is set equal to ABmag.
- PSFs: Generated using STPSF version 2.1 using distorted PSF models and exit pupil normalization.  Key inputs for these PSFs were 9x oversampling, and an input spectrum of a G2V model from the Phoenix stellar library. Input spectrum is sampled over 25 points for all filters, except 45 points for F062 and F146.
- Encircled Energy: Calculated from the PSFs
- Distortions: N/A
- Pixel Area: N/A
- Gain: N/A - STIPS images are written in electrons
- Readout noise: read from STIPS image
- Data quality: N/A

NOTE: The current DOLPHOT module is intended to be compatible with images generated by STIPS.  This tool assumes no geometric distortion (aside from as reflected in the PSFs), uniform pixel area map, and no bad pixels.
