This is the full list of commands available inside pamela. If you are new to the program you may find it easier to search using the command classes first of all.
| debias | -- | debiasses a series of frames |
| extnor | -- | normal spectrum extraction. |
| extopt | -- | Horne's optimal extraction. |
| faker | -- | fakes up test data. |
| fixhead | -- | fixes headers into a standard form |
| idtype | -- | determines data type, 'arc', 'flat' or 'data'. |
| lsnosdf | -- | list files without trailing .sdf |
| makebias | -- | makes a mean bias frame |
| medprf | -- | median collapse of an image. |
| noise | -- | calibrates noise model of detector. |
| optext | -- | optimal extraction from curved spectra. |
| pamela | -- | general info on pamela. |
| picstat | -- | computes useful statistics on a file. |
| polfit | -- | fits splines to spectra. |
| pplot | -- | plots slices of data. |
| profit | -- | fits profile to curved spectra. |
| recomp | -- | recomputes fraction file for a new spectrum. |
| reduce | -- | grand reduction script |
| regpic | -- | interactive selection of sky/object regions. |
| renumber | -- | renames frames to their run number |
| rotate | -- | rotate frames |
| skew | -- | straightens/tilts a spectrum. |
| skyfit | -- | makes poly fits to the sky background. |
| skymov | -- | moves regions to account for drift along slit. |
| splfit | -- | fits splines to spectra. |
| splitbysource | -- | divides up data according to type (arc, flat etc) |
| track | -- | measures and fits the spectrum curvature. |
| ultradas | -- | converts from ultradas to standard format sdf |