lightkurve.KeplerTargetPixelFile.plot#
- KeplerTargetPixelFile.plot(ax=None, frame=0, cadenceno=None, bkg=False, column='FLUX', aperture_mask=None, show_colorbar=True, mask_color='red', title=None, style='lightkurve', **kwargs)#
Plot the pixel data for a single frame (i.e. at a single time).
The time can be specified by frame index number (
frame=0
will show the first frame) or absolute cadence number (cadenceno
).- Parameters
- ax
Axes
A matplotlib axes object to plot into. If no axes is provided, a new one will be generated.
- frameint
Frame number. The default is 0, i.e. the first frame.
- cadencenoint, optional
Alternatively, a cadence number can be provided. This argument has priority over frame number.
- bkgbool
If True and
column="FLUX"
, background will be added to the pixel values.- columnstr
Choose the FITS data column to be plotted. May be one of (‘FLUX’, ‘FLUX_ERR’,’FLUX_BKG’,’FLUX_BKG_ERR’,’COSMIC_RAYS’,’RAW_CNTS’).
- aperture_maskndarray or str
Highlight pixels selected by aperture_mask.
- show_colorbarbool
Whether or not to show the colorbar
- mask_colorstr
Color to show the aperture mask
- stylestr
Path or URL to a matplotlib style file, or name of one of matplotlib’s built-in stylesheets (e.g. ‘ggplot’). Lightkurve’s custom stylesheet is used by default.
- kwargsdict
Keywords arguments passed to
plot_image
.
- ax
- Returns
- ax
Axes
The matplotlib axes object.
- ax