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Bases: object
Generic class to represent FITS files which contain one or more light curves.
astropy.io.fits.HDUList objectLocal path or remote url of a lightcurve FITS file.Also accepts a FITS file object already opened using AstroPy.
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Keyword arguments to be passed to astropy.io.fits.open.
Attributes Summary
Returns a |
Returns a |
Returns a |
The file's |
Declination as recorded in the header's |
Right Ascension as recorded in the header's |
The file's |
Methods Summary
| Plot the light curve file using matplotlib's |
| Returns the metadata embedded in the file. Cfs software crack. |
| Returns a header keyword value. |
| DEPRECATED. |
| Plot the light curve file using matplotlib's |
| Plot the light curve file using matplotlib's |
Attributes Documentation
FLUX¶Returns a LightCurve object based on thecontents of the FLUX column in the file, if that column exists.
PDCSAP_FLUX¶Returns a LightCurve object based on thecontents of the PDCSAP_FLUX column in the file, if that column exists.
SAP_FLUX¶Returns a LightCurve object based on thecontents of the SAP_FLUX column in the file, if that column exists.
cadenceno¶The file's CADENCENO column.
dec¶Declination as recorded in the header's DEC_OBJ keyword.
ra¶Right Ascension as recorded in the header's RA_OBJ keyword.
time¶The file's TIME column.
Methods Documentation
errorbar(self, flux_types=None, style='lightkurve', **kwargs)¶Plot the light curve file using matplotlib's errorbar method.
AxesA matplotlib axes object to plot into. If no axes is provided,a new one will be generated.
Which fluxes in the LCF to plot. Default is lcf._flux_types().For Kepler this is PDCSAP and SAP flux. Pass a list to change fluxtypes.
Normalize the lightcurve before plotting?
Plot x axis label
Plot y axis label
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Plot set_title
Path or URL to a matplotlib style file, or name of one ofmatplotlib's built-in stylesheets (e.g. ‘ggplot').Lightkurve's custom stylesheet is used by default.
Dictionary of arguments to be passed to matplotlib.pyplot.plot.
AxesThe matplotlib axes object.
get_header(self, ext=0)¶Returns the metadata embedded in the file.
Light Curve Files contain embedded metadata headers spread across threedifferent FITS extensions:
The 'PRIMARY' extension (
ext=0) provides a metadata headerproviding details on the target and its CCD position.The 'LIGHTCURVE' extension (
ext=1) provides details on thedata columns and the systematics removal.The 'APERTURE' extension (
ext=2) provides details on theaperture pixel mask and the expected coordinate system (WCS).
FITS extension name or number.
HeaderHeader object containing metadata keywords.
get_keyword(self, keyword, hdu=0, default=None)¶Returns a header keyword value.
If the keyword is Undefined or does not exist,then return default instead.
header(self, ext=0)¶DEPRECATED. Please use get_header() instead.
plot(self, flux_types=None, style='lightkurve', **kwargs)¶Plot the light curve file using matplotlib's plot method.
AxesA matplotlib axes object to plot into. If no axes is provided,a new one will be generated.
Which fluxes in the LCF to plot. Default is lcf._flux_types().For Kepler this is PDCSAP and SAP flux. Pass a list to change fluxtypes.
Path or URL to a matplotlib style file, or name of one ofmatplotlib's built-in stylesheets (e.g. ‘ggplot').Lightkurve's custom stylesheet is used by default.
Dictionary of arguments to be passed to matplotlib.pyplot.plot.
AxesThe matplotlib axes object.
get_header(self, ext=0)¶Returns the metadata embedded in the file.
Light Curve Files contain embedded metadata headers spread across threedifferent FITS extensions:
The 'PRIMARY' extension (
ext=0) provides a metadata headerproviding details on the target and its CCD position.The 'LIGHTCURVE' extension (
ext=1) provides details on thedata columns and the systematics removal.The 'APERTURE' extension (
ext=2) provides details on theaperture pixel mask and the expected coordinate system (WCS).
FITS extension name or number.
HeaderHeader object containing metadata keywords.
get_keyword(self, keyword, hdu=0, default=None)¶Returns a header keyword value.
If the keyword is Undefined or does not exist,then return default instead.
header(self, ext=0)¶DEPRECATED. Please use get_header() instead.
plot(self, flux_types=None, style='lightkurve', **kwargs)¶Plot the light curve file using matplotlib's plot method.
AxesA matplotlib axes object to plot into. If no axes is provided,a new one will be generated.
Which fluxes in the LCF to plot. Default is lcf._flux_types().For Kepler this is PDCSAP and SAP flux. Pass a list to change fluxtypes.
Normalize the lightcurve before plotting?
Plot x axis label
Plot y axis label
Plot set_title
Path or URL to a matplotlib style file, or name of one ofmatplotlib's built-in stylesheets (e.g. ‘ggplot').Lightkurve's custom stylesheet is used by default.
Dictionary of arguments to be passed to matplotlib.pyplot.plot.
AxesThe matplotlib axes object.
scatter(self, flux_types=None, style='lightkurve', **kwargs)¶Plot the light curve file using matplotlib's scatter method.
AxesA matplotlib axes object to plot into. If no axes is provided,a new one will be generated.
Which fluxes in the LCF to plot. Default is lcf._flux_types().For Kepler this is PDCSAP and SAP flux. Pass a list to change fluxtypes.
Normalize the lightcurve before plotting?
Plot x axis label
Plot y axis label
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Path or URL to a matplotlib style file, or name of one ofmatplotlib's built-in stylesheets (e.g. ‘ggplot').Lightkurve's custom stylesheet is used by default.
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Dictionary of arguments to be passed to matplotlib.pyplot.plot.
AxesThe matplotlib axes object.
