Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ
îðèãèíàëüíîãî äîêóìåíòà
: http://www.atnf.csiro.au/vlbi/dokuwiki/doku.php/difx/difx2fits
Äàòà èçìåíåíèÿ: Unknown Äàòà èíäåêñèðîâàíèÿ: Sun Apr 10 17:39:30 2016 Êîäèðîâêà: IBM-866 Ïîèñêîâûå ñëîâà: ï ï ï ï ï ï ï ï ï ï ï ï ï ï ï ð ï ð ï ð ï |
Program difx2fits creates a FITS output file from the DIFX (also known as SWIN) format visibilities created by mpifxcorr and several other files carrying information about the observation. When run, difx2fits requires the following files to be present:
.difx/
.input
.uvw
.delay
This minimal requirement means that difx2fits can be used for correlator jobs not created with the job2difx or vex2difx, though it is possible that certain combinations of different configurations within the .input
file will not be properly supported at this time. Several other files are optional and are typically used to populate calibration and ancillary tables:
.calc/
.rates/
.im/
.flag/
flags
pcal
tsys
weather
$GAIN_CURVE_PATH
With the exception of the gain curve files, all the input files to difx2fits are expected to be in the current working directory. As the visibility file (.difx
) is read, any records that are all zero are omitted. The number count of these dropped records is reported as invalid records when difx2fits finishes writing the UV
table. With difx2fits versions since 2.0 multiple correlator output files can be combined into a single destination FITS file; this feature is still new, so please check the results carefully!
difx2fits should be invoked from the command line as follows:
difx2fits
[ options ] [ baseFilename1 [ òÀæ baseFilenameN ]] [ outFile ]
options can include:
-a
chanavg or òÀÓaverage
chanavg : average chanavg spectral channels-b
chan or òÀÓbeginchan
chan : convert channels starting at zero-based channel chan-h
or òÀÓhelp
: print usage information and exit-n
or òÀÓno-model
: don't write model (ML) table-o
nchan or òÀÓoutchans
nchan : write a total of nchan channels to FITS-s
scale or òÀÓscale
scale : scale visibility data by scale-t
interval or òÀÓdeltat
interval : set the time interval (in seconds) of jobmatrix files-v
or òÀÓverbose
: increase verbosity of output; use twice or thrice to get even more-d
or òÀÓdifx
: run on all .difx
files found in the directory-k
or òÀÓkeep-order
: don't sort the antennas by name-1
or òÀÓdont-combine
: make a separate FITS file for each input job-x
or òÀÓdont-sniff
: don't generate sniffer output filesòÀÓoverride-version
: ignore difx version clashes
baseFilenameX is the prefix of a jobfile to convert; it is OK to use the .difx
filename instead
outFile is the name of the FITS file to produce; if not provided one will be made based on the project code
difx2fits job9020.000 9020.FITS
difx2fits -v -v -d
Unless disabled with the òÀÓdont-sniff
or -x
flag, four sniffer output files (with suffixes .acb
, .apd
, .wts
and .xcb
) will be written for each FITS file produced. These files are used by difxsniff and its associated programs to produce data plots that are used to assess data quality.
Unless disabled by setting interval to a non-positive number with the -t
or òÀÓdeltat
option, an output file with suffix .jobmatrix
will be produced.
This file contains an ASCII art diagram of which jobs contributed to each .FITS
file produced as a function of both time and antenna.