Purpose: check on the correctness of our calibration. The idea here is that we are calling DR1 "good enough" when the DEGAS pixel values are within 20% of the EMPIRE pixel values for the same galaxy.
Input: DEGAS Cube
Output: plot comparing EMPIRE vs. DEGAS pixel values.
Pieces that need to be built:
- Function to find EMPIRE data corresponding to input DEGAS cube (assume EMPIRE data on local disk)
- Function to smooth DEGAS data to EMPIRE spatial resolution (preserving the units)
- Function to regrid the DEGAS data to EMPIRE pixel scale
- Function to regrid the DEGAS data channels to the EMPIRE channels (Maybe able to be combined with above)
- Function to output the plot
Purpose: check on the correctness of our calibration. The idea here is that we are calling DR1 "good enough" when the DEGAS pixel values are within 20% of the EMPIRE pixel values for the same galaxy.
Input: DEGAS Cube
Output: plot comparing EMPIRE vs. DEGAS pixel values.
Pieces that need to be built: