--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 6.3. | |
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 6.2 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 6.1 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. | |