a ߙfb, @szddlZddlZddlmZmZddlmZmZddl m Z m Z ddl m Z dgZddZede eed e edS) N)registryfits)Table MaskedColumn)Time TimeDelta) TimeSerieskepler_fits_readerc Cst|}|djd}|dkr.|d}n*|dkr@|d}ntd|djd|jddkrtd |jd |jd|jd d krtd |jd |jd tj|dd}d|jvr| dd|jD]p}||j }|rt ||t r|| tj||<|dkr"d||_ |dkr6d||_ | ||qt|dj}t|r|tdt|d||}t|jd|jd|jd dd}|t|dj} d| _|d|t| |dS)at This serves as the FITS reader for KEPLER or TESS files within astropy-timeseries. This function should generally not be called directly, and instead this time series reader should be accessed with the :meth:`~astropy.timeseries.TimeSeries.read` method:: >>> from astropy.timeseries import TimeSeries >>> ts = TimeSeries.read('kplr33122.fits', format='kepler.fits') # doctest: +SKIP Parameters ---------- filename : `str` or `pathlib.Path` File to load. Returns ------- ts : `~astropy.timeseries.TimeSeries` Data converted into a TimeSeries. rZtelescopZtessZ LIGHTCURVEZkeplerzL{} is not implemented, only KEPLER or TESS are supported through this readerZEXTVERz,Support for {} v{} files not yet implementedZTELESCOPZTIMESYSZTDBz:Support for {} time scale not yet implemented in {} readerr)formatTZTIMEze-/sz electron/sZpixelsZpixeltimez Ignoring z rows with NaN timesZBJDREFIZBJDREFFZjd)Zscaler Zisot)r data)ropenheaderlowerNotImplementedErrorr rreadZcolnamesZ rename_columnunit isinstancerZfillednpnanZisnanranywarningswarnsumrrZ remove_columncloser) filenameZhdulistZ telescopeZhduZtabZcolnamerZnansZreference_dater r;lib/python3.9/site-packages/astropy/timeseries/io/kepler.pyr sR               z kepler.fitsz tess.fits)rZnumpyrZ astropy.iorrZ astropy.tablerrZ astropy.timerrZastropy.timeseries.sampledr__all__r Zregister_readerrrrrs T