--h option after it, e.g.
dal_attach --h
| Name | Description |
| barycent | Converts time stamps of events or light curves to barycentered times assuming |
| that the data comes from a given source direction. | |
| cat2ds9 | Creates DS9 region file from the list of sources. This can be a catalog extract, |
or a list of sources produced by the analysis. See more details in section . |
|
| cat_merge | Merges two source lists, e.g., two extracts from different catalogs. |
| converttime | Reads input time in a user specified format and converts it to either user |
| specified output format or into all formats known by the converttime. | |
| dal_create | Creates a FITS file according to a template. |
| evts_extract | Creates an instrument independent event list. |
| evts_pick | Combines event data distributed over several Science Windows and tables |
| within the Science Window into a single table. Limited to ISGRI and JEM-X | |
| in this release. | |
| gti_attitude | Creates a GTI depending on attitude stability, see Science Analysis sections of |
| [1], [2],[3],[4] for more details on practical implementations. | |
| gti_create | Generates GTIs depending on housekeeping parameters, see Science Analysis |
| sections of [1], [2],[3],[4] for more details on practical implementations. | |
| gti_data_gaps | Generates GTIs depending on the not missing science data packets, see Science |
| Analysis sections of [1], [2],[3],[4] for more details on practical implementations. | |
| gti_import | Imports User GTIs into the ISDC GTI index files, see Science Analysis sections |
| of [1], [2],[3],[4] for more details on practical implementations. | |
| gti_merge | Merges Good Time Intervals,see Science Analysis sections of [1], [2],[3],[4] for |
| more details on practical implementations. | |
| gti_pick | Creates a user GTI file from ISDC GTIs. |
| gti_user | Creates user GTI table, see for more details. |
| image_mosaic | Combines many count rate sky images into a mosaic count rate image and |
| an exposure map. | |
| lc_pick | Selects lightcurves created for a given source and combines them in a single |
| file. Either as individual tables combined by an Index (the default) or merged | |
| together to a single dataset. See Cookbooks of [1] and[3] for examples on | |
| practical usage. | |
| og_create | Builds the OG from an index of prepared science window groups and observa- |
tion IDs, setting up the complete directory structure; see for more details. |
|
| og_clean | This executable will clean an OG up to a certain level. To do that, it will erase |
| the files from the disk. | |
| To work properly, the group should not have been used to build another OG | |
| or groups of higher level. | |
| og_copy | Copies the OG. |
| q_identify_srcs | Compares sources found by the software with the catalog. |
| spe_pick | Combines the extracted spectra for a given source across multiple Science Win- |
| dows. See Cookbooks of [1] and [3] for examples on practical usage. | |
| src_collect | Combines source data obtained by the imaging analysis for individual Science |
| Windows into a single table covering an Observation Group. It is possible to | |
| retrieve only selected results, e.g., just for a given source. | |
| txt2idx | All DOLs contained in the ASCII list will be added to the index. See Cookbooks |
| of [1] and [3] for examples on practical usage. | |