Software Tasks
Before Observing
- Target selection, including merging disjoint projects
- Coordinate generation
- Mask optimization
- Mask generation
At the Telescope
- Mask selection and scheduling
- Mask insertion
- Target acquisition
- Mask alignment
- Data acquisition
- CCD control
- Data display
- Save the bits
- Write data to medium (DVD?)
- Calibrations
- Standard Star selection
- Arc and Flat lamp control
- Flexure compensation?
- Standard star slit-to-slit "hop and observe"
Pipeline Processing
- CCDPROC
- IMCOMBINE
- Wavelength calibration
- Extinction calibration
- Flux calibration
- Reddening determination and correction
- Extraction and/or sky subtraction
- Fringe removal
- Removal of atmospheric (Telluric) lines
Science Pipeline
- Classification
- Stars vs galaxies vs nebulae vs unknown
- Spectral types (MK classes)
- Stellar Measurements
- Reddening
- Velocity
- Equivalent widths
- Nebular Measurements
- Reddening
- Velocity
- Line strengths
- Galaxy Measurements
- Velocity and velocity dispersion
- Classification: "normal", emission-line, active (QSO, AGN)
Expert Software
- Statistical testing on database: correlations in N-space for data with uncertainties
- Automatic astrophysical analysis
- Stellar atmospheric abundances
- Nebular photoionization models
Archive Ingest and Query
- Read from Save-the-Bits
- Generate header summaries
- Simple queries based on position
- Complex queries based on position, wavelength coverage, resolution, etc
- Multi-form (spectra, imaging), multi-wavelength (optical, x-ray) queries
Updated on May 25, 2022, 10:12 am