The list available features and capabilities will continuously grow with each iterative deployment. Here we describe the features and capabilities as of September 2013.
GMOS Imaging
Processing of acquisition images
Processing of science observations
Processing of biases, to create processed biases
Processing of imaging flats, to create processed flats
Processing of science observations, to create processed fringe frames
Variance and DQ planes propagation
Display of current image and stacked image, if available (ds9)
- Calibration request supported:
- Retrieval of processed bias matching overscan and trim status
- Retrieval of processed imaging flats
- Retrieval of processed fringe frame
- Data reduction steps supported:
- Overscan correction
- Trim overscan section
- Bias correction
- Flat correction
- Fringe correction
- Detection of point sources
- Registration and alignment of images from same observation
- Stacking of images from same observation
- CCDs support
- Current (Aug 2012) EEV CCDs and E2V CCDs
Note that stacking has been removed from the standard recipe for the time being. The CL task used to stack is too slow. Stacking will be re-enable once a more performant Python or C/C++ version is available. (No plans yet.)
This includes seeing and PSF ellipticity.
Available for:
This is available for:
This includes zero-points and extinction
This is available for:
This is available for:
This is available for: