ahbackscal |
- Corrects BACKSCAL keyword in a spectrum extracted with xselect |
ahcalcl32ti |
- Compute L32TI from S_TIME |
ahfilecaldb |
- Creates a FITS file from a set of text files |
ahgainfit |
- Calculate the time-dependent energy gain corrections using known calibration lines |
ahgetvector |
- Extracts vectors from a FITS file and outputs to a text file |
ahgtigen |
- Create and/or merge GTI files |
ahmodhkext |
- Merges extensions of FITS file into single extension |
ahscreen |
- Screens a science event file |
ahsysinfo |
- Displays system build information about an executable and/or information about the current system |
ahtimeconv |
- Converts mission time in different formats |
xaarfgen |
- Makes an ancillary response function (ARF) file for XRISM Resolve or Xtend using xaxmaarfgen |
xacalctime |
- Re-runs the XRISM timing tools on an output directory from the XRISM pipeline |
xaexpmap |
- Generates an exposure map for XRISM Resolve or Xtend instrument |
xafilter |
- Generates an EHK file and a MKF filter file for XRISM |
xamkehk |
- Makes an extended housekeeping (EHK) file using XRISM orbit and attitude data to construct time series columns |
xamkregion |
- Creates region files showing the fields of view of all XRISM instruments |
xamktim |
- Calculates the relation of XRISM time invariant (TI) vs. TIME and the GTI for when the GPS is on |
xapipeline |
- XRISM Resolve/Xtend reprocessing tool |
xatime |
- Calculates times and populates the TIME column for all XRISM science and housekeeping data |
xatrendtemp |
- Calculates the quartz clock frequency vs. temperature relation for the on-board clock on XRISM |
xaxmaarfgen |
- Creates an ancillary response function (ARF) file for the XRISM Resolve or Xtend instruments |
xrismversion |
- Reports version string for XRISM tools |
rsladrgti |
- Calculates ADR GTI and constructs ADR GTI file |
rslanticolc |
- Extracts XRISM Resolve antico light curve(s), with optional spectra |
rslanticopi |
- Assigns PHA and PI columns to XRISM Resolve anticoincidence events |
rslbranch |
- Computes rates and branching ratios for each XRISM Resolve event grade |
rslctsfluct |
- Calculates CTS Control and Monitor thermometer temperature fluctuations |
rslflagpix |
- Flags XRISM Resolve events for antico and MXS event coincidence, temporal proximity, and crosstalk |
rslgain |
- Calculates the time-dependent energy correction for XRISM Resolve events from comparison with known calibration lines |
rslmkrmf |
- Creates a XRISM Resolve redistribution matrix file (RMF) for selected Resolve pixels and grade combinations |
rslmxsgti |
- Generates coarse and fine MXS GTI files for XRISM Resolve using rslmxstime, inverts GTI, and merges GTI |
rslmxstime |
- Generates coarse and fine GTI files for the XRISM MXS and populates HK columns with LED start and stop times |
rslnxbgen |
- Creates a non-X-ray background (NXB) spectrum for the XRISM Resolve instrument |
rslpha2pi |
- Calculates the PI values for events in XRISM Resolve event files |
rslpipeline |
- XRISM Resolve reprocessing tool |
rslpixgti |
- Combines pixel-dependent and pixel-independent Resolve GTI |
rslplsclip |
- Calculates Resolve event pulse clipping flag |
rslrmf |
- Creates an XRISM Resolve redistribution matrix file (RMF) file for selcted pixels and grades with weighting factors |
rslsamcnt |
- Calculates the local time at fine resolution in XRISM Resolve for later synchronization wth GPS-related time |
rslseccor |
- Corrects PHA for mid-resolution secondary grade XRISM Resolve events |
rslsecid |
- Associates XRISM Resolve secondary events with primary events in groups, optionally reassigning event grades |
arftable |
- Creates an ancillary response function (ARF), or effective area file from the output events from the raytracing code xrtraytrace, not including any detector efficiencies
|
dustmodeleffarea |
- For X-ray point sources with dust halos, makes an effective area correction (or modifier) file, with the option of inputting raytracing event files made by the tool dustyarfmod |
dustyarfmod |
- For X-ray point sources with dust halos, makes an effective area correction (or modifier) file, with the option of running raytracing simulations for the calculations |
eeftable |
- Creates an encircled energy function (EEF) file based on the output history file from the raytracing tool xrtraytrace
|
xrtraytrace |
- Performs raytracing simulations of X-ray telescopes, calculating photon paths, PSF, EEF, and effective area |
xrtreftable |
- Calculates the probability of reflection and transmission of a ray upon a surface, and mass absorption coefficients for mirror surface |
barycen |
- Applies barycenter corrections to X-ray timing data |