AIPS-to-CASA Cheat Sheet
From CASA Guides
For AIPS users who are learning CASA, it is intuitive to think about equivalent tasks between the two software packages. Below are some AIPS-to-CASA equivalent tasks; note that there is not always a one-to-one transformation between the two packages.
AIPS | CASA | Purpose |
---|---|---|
BLCAL | blcal | Calculate a baseline-based calibration solution (gain or bandpass) |
BPASS | bandpass | Calibrate bandpasses |
CALIB | gaincal | Calibrate gains (amplitudes and phases) |
CLCAL | applycal | Apply calibration to data |
COMB | immath | Combine images |
CPASS | cpass | Calibrate bandpasses by polynomial fitting |
DBCON | concat | Concatenate uv datasets |
DEFAULT | default | Load a task with default parameters |
FILLM | importvla | Import old-format VLA data |
FITLD | importuvfits | Import a uv dataset which is in FITS format |
FITLD | importfits | Import an image which is in FITS format |
FITTP | exportuvfits | Write a uv dataset to FITS format |
FITTP | exportfits | Write an image to FITS format |
FRING | --- | Calibrate group delays and phase rates. |
GETJY | fluxscale | Determine flux densities for other cals |
GO | go | Run a task |
IMAGR | clean | Image and deconvolve |
IMFIT | imfit | Fit gaussian components to an image |
IMHEAD | vishead | View header for uv data |
IMHEAD | imhead | View header for an image |
IMLIN | imcontsub | Subtract continuum in image plane |
IMLOD | importfits | Import a FITS image |
IMSTAT | imstat | Measure statistics on an image |
INP | inp | View task parameters |
JMFIT | imfit | Fit gaussian components to an image |
LISTR | listobs | Print basic data |
MCAT | ls | List image data files |
MOMNT | immoments | Compute moments from an image |
OHGEO | imregrid | Regrids an image onto another image's geometry |
PBCOR | immath | Correct an image for the primary beam |
PCAL | polcal | Calibrate polarization |
POSSM | plotcal | Plot bandpass calibration tables |
POSSM | plotms | Plot spectra |
PRTAN | listobs | Print antenna locations |
PRTAN | plotants | Plot antenna locations |
QUACK | flagdata | Remove first integrations from scans |
RENAME | mv | Rename an image or dataset |
SETJY | setjy | Set flux densities for flux cals |
SMOTH | imsmooth | Smooth an image |
SNPLT | plotcal | Plot gain calibration tables |
SPFLG | viewer | Flag raster image of time v. channel |
SPLIT | split | Write out uv files for individual sources |
TASK | inp | Load a task with current parameters |
TGET | tget | Load a task with parameters last used for that task |
TVALL | viewer | Display image |
TVFLG | viewer | Flag raster image of time v. baseline |
UCAT | ls | List uv data files |
UVFLG | flagdata | Flag data |
UVLIN | UVCONTSUB | Subtract continuum from uv data |
UVLSF | UVCONTSUB | Subtract continuum from uv data |
UVPLT | PLOTMS | Plot UV data |
WIPER | PLOTMS | Plot and flag UV data |
ZAP | RMTABLES | Delete data files |
--Laura Chomiuk 20:32, 10 February 2010 (UTC)