Description: | Script to gather information about the Pytho/numpy/LSL install to help with troubleshooting. |
---|---|
Usage: | gatherDebugging.py |
Options: | None |
Description: | Build LSL-specific FFTW wisdom and save it to a file within the LSL distribution. |
---|---|
Usage: | makeWisdom.py |
Options: | None |
Description: | Update the internal LWA1 SSMIF used by LSL. |
||||||
---|---|---|---|---|---|---|---|
Usage: | updateLSLSSMIF.py [options] |
||||||
Options: |
|
Description: | Application to display rise, transit, and set times for various astronomical sources from LWA-1 for the current date. |
---|---|
Usage: | astroevents.py |
Options: | None |
Description: | Application to calculate real-time ephemeris for a LWA site. |
||||||
---|---|---|---|---|---|---|---|
Usage: | astrostatus.py [options] |
||||||
Options: |
|
Description: | Generate a drift curve for a dipole at LWA-1 observing at a given frequency in MHz. |
||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | driftcurve.py [OPTIONS] |
||||||||||||||||||
Options: |
|
Description: | Estimate the ionospheric contribution to the RM for an observation using the IGS final product and the IGRF. |
||||||
---|---|---|---|---|---|---|---|
Usage: | getIonosphericRM.py [options] RA Dec Start Stop RA: J2000 right ascension in HH:MM:SS[.SSS] Dec: J2000 declination in sDD:MM:SS[.SSS] Start: YYYY/MM/DD HH:MM:SS start time in UTC Stop: YYYY/MM/DD HH:MM:SS stop time in UTC |
||||||
Options: |
|
Description: | Simple LWDA astronomical source catalogue display application. |
||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | lwa_cat_view.py [options] |
||||||||||
Options: |
|
Description: | Given a MCS metadata tarball, print out details of the associated observations. |
---|---|
Usage: | inspectTarball.py metaData |
Options: | None |
Description: | Plot the relative dipole response for both polarizations of an isolated LWA-1 antenna at a particular frequency. |
||||||
---|---|---|---|---|---|---|---|
Usage: | plotAntenna.py [OPTIONS] |
||||||
Options: |
|
Description: | Plot the x, y, and z locations of stands at LWA-1. Also, mark and label particular stands, if requested. |
||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | plotStands.py [OPTIONS] [stand1 [stand2 [...]]] |
||||||||||
Options: |
|
Description: | Randomly select 20 antennae from LWA-1 and plot the uv-plane coverage for a zenith snapshot and the expected beam. Alternatively, select some FRACTION of the stands with installed FEEs to use or use the specified list of stands. |
||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | plotUVCoverage.py [FRACTION | STAND LIST] |
||||||||||
Options: |
|
Description: | Split a TBN file containing multiple seconds into several files |
||||||||
---|---|---|---|---|---|---|---|---|---|
Usage: | splitTBN.py [options] file |
||||||||
Options: |
|
Note
This script does not use a lsl.reader.buffer buffer to try to re-order or verify all packets and simply splits files based on size.
Description: | Split a DRX file containing multiple seconds into several files |
||||||||
---|---|---|---|---|---|---|---|---|---|
Usage: | splitDRX.py [options] file |
||||||||
Options: |
|
Description: | Example script for reading in TBW data and writing it to a TSFITS file. |
---|---|
Usage: | readTBW.py file |
Options: | None |
Description: | Example script for reading in TBN data and writing it to a TSFITS file. |
---|---|
Usage: | readTBN.py file |
Options: | None |
Description: | Example script for reading in DRX data and writing it to a SD-FITS file. |
---|---|
Usage: | readDRX.py file |
Options: | None |
Description: | Given a MCS metadata tarball and a session DRX recording, split the session recording into the individual observations. |
---|---|
Usage: | splitSession.py metaData data |
Options: | None |
Description: | Read and plot the NOSTA_MAPPER table in a FITS IDI file writen by lsl.writer.fitsidi if it exists. |
---|---|
Usage: | plotMapper.py file |
Options: | None |
Description: | Given a TBW file, plot the time averaged spectra for each digitizer input. |
||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | tbwSpectra.py [OPTIONS] file |
||||||||||||||||||||||||||||
Options: |
|
Warning
tbwSpectra.py currently assumed that the system it is running on has enough memory to read in a full TBW capture. Due to data representation and processing overheads this amounts to about 16 GB.
Description: | Given a TBN file, plot the time averaged spectra for each digitizer input. |
||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | tbnSpectra.py [OPTIONS] file |
||||||||||||||||||||||||||
Options: |
|
Description: | Given a DRX file, plot the time averaged spectra for each beam output. |
||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | drxSpectra.py [OPTIONS] file |
||||||||||||||||||||||||
Options: |
|
Description: | Given a DR spectrometer file, plot the time averaged spectra for each beam output. |
||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | drSpecSpectra.py [OPTIONS] file |
||||||||||||||
Options: |
|
Description: | Cross-correlate data in a TBW file |
||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | correlateTBW.py [OPTIONS] file |
||||||||||||||||||
Options: |
|
Description: | Example script that reads in TBN data and runs a cross-correlation on it. The results are saved in the Miriad UV format. |
||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | correlateTBN.py [OPTIONS] file |
||||||||||||||||||||||||||||
Options: |
|
Description: | Script that takes a FITS IDI file and mimics the AIPS task POSSM by plotting average cross-power spectra for all baselines in the FITS IDI file. |
---|---|
Usage: | possm.py file |
Options: | None |
Description: | Script that takes a FITS IDI file and images the data. |
||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Usage: | imageIDI.py file |
||||||||||||||||||||
Options: |
|