Clippy

class dorado.Clippy[source] [edit on github]

Bases: object

Methods Summary

delcacheObj(fname[, subcache])

diread(dirarray)

dirscan(dirarray)

enter_dordir()

exit_dordir()

force16(hdu)

getDateString(cr)

get_night()

get_night obtains a timestring for the most recent(previous) night based on local/hardware time provided by datetime.

init_dir()

mkBias(biasIFC)

mkBias takes a list of bias images to construct a combined bias image. ————> this needs to be corrected for the new image storage format Parameters ———- biasIFC: array[CCDdata] array of raw bias images.

mkFlat(flats)

mkFlat takes a list of flats to construct a calibrated flatfield image.

mkcacheObj(object[, subcache])

mkceres(date[, sub, target, calibrated, aligned])

mkwrk(cr)

newdat()

plate_solve(dirarray[, data, writearray])

saveWCS(cr[, filters])

savewrk(cr[, filters])

Methods Documentation

delcacheObj(fname, subcache=False)[source] [edit on github]
diread(dirarray)[source] [edit on github]
dirscan(dirarray)[source] [edit on github]
enter_dordir()[source] [edit on github]
exit_dordir()[source] [edit on github]
force16(hdu)[source] [edit on github]
getDateString(cr)[source] [edit on github]
get_night()[source] [edit on github]

get_night obtains a timestring for the most recent(previous) night based on local/hardware time provided by datetime. The format follows yyyy-mm-(dd-1)+dd where (dd-1) is last nights day of the month. This currently does not support dates at which the start of the observing night was the last day of the month.

Parameters
None
Returns
night: str

Timestring for the most recent night.

init_dir()[source] [edit on github]
mkBias(biasIFC)[source] [edit on github]

mkBias takes a list of bias images to construct a combined bias image. ————> this needs to be corrected for the new image storage format Parameters ———- biasIFC: array[CCDdata]

array of raw bias images.

Returns
bias: CCDdata

The combined bias image.

mkFlat(flats)[source] [edit on github]

mkFlat takes a list of flats to construct a calibrated flatfield image.

Parameters
flats: array[CCDdata]

array of raw flatfields. ————> this needs to be corrected for the new image storage format

Returns
flat: CCDdata

The combined calibrated flatfield image.

mkcacheObj(object, subcache=False)[source] [edit on github]
mkceres(date, sub='raw', target=None, calibrated=False, aligned=False)[source] [edit on github]
mkwrk(cr)[source] [edit on github]
newdat()[source] [edit on github]
plate_solve(dirarray, data=None, writearray=False)[source] [edit on github]
saveWCS(cr, filters=None)[source] [edit on github]
savewrk(cr, filters=None)[source] [edit on github]