kepstitch -- Append short cadence months and/or long cadence quarters
kepstitch infiles outfile clobber verbose logfile status
infiles = string
A list of individual FITS files. Most commonly these will
contain data from the same target obtained over different months
or quarters. Short cadence and long cadence data can be mixed
within this list. The list of files provided directly must be
comma-separated. Alternatively an ASCII file containing file
names can parsed to this argument if the path and name of the
file are preceded by a '@' character. The ASCII file must be
formatted to have one FITS filename per line.
outfile = string
The name of the output FITS file with concatenated time series data.
clobber = boolean (optional)
Overwrite the output file? if clobber = no and an existing file has
the same name as outfile then the task will stop with an error.
verbose = boolean (optional)
Print informative messages and warnings to the shell and logfile?
logfile = string (optional)
Name of the logfile containing error and warning messages.
status = integer
Exit status of the script. It will be non-zero if the task halted with an
error. This parameter is set by the task and should not be modified by the
kepstitch takes a list of FITS light curves obtained from
the MAST archive and concatenates them into one long table. Be
aware that this task currently does not sort the table by
time. If users must ensure that the input file list is ordered
by increasing time. Also no attempt is made to correct for
aperture and PSF differences across quarterly rolls. Light
curves spanning multiple quarters are likely to be discontinuous
at the quarterly boundaries. Both issues will be addressed in
- Provide a direct list of Kepler time series files to concatenate:
- Provide a list within an ASCII file of Kepler time series files to concatenate:
- kepstitch infiles=@KeplerFiles.lis outfile=stitched.fits clobber=y
Full completion upon one quarter of Kepler long cadence target using a 3.06
GHz Intel Core 2 Duo Mac running OS 10.6.4 takes a few seconds. Running times
increase by several factors if input data contains NaNs. These will be
filtered out before task execution.
BUGS AND LIMITATIONS
Although the target pixel mask will change from quarter to quarter, kepstitch does not track that change. The target pixel mask in the output file of kepstitch belongs to the first file in the list of input files. The Kepler PyRAF package is privately-developed software made available to
the community through the contributed software page of the GO program at
http://keplergo.arc.nasa.gov/ContributedSoftware.shtml. It is not an
official software product of the Kepler mission. Bugs and errors are not
the responsibility of NASA or the Kepler Team. Please send bug reports and
suggestions to firstname.lastname@example.org.
Initial software release (MS)
Updated for Kepler FITS v2.0 (MS)
Code can now be run from the command line (TB)
more reliable plot rendering on linux operating systems (MS)