sep.flux_radius¶
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sep.flux_radius(data, x, y, rmax, frac, normflux=None, mask=None, maskthresh=0.0, subpix=5)¶ Return radius of a circle enclosing requested fraction of total flux.
Parameters: data :
ndarray2-d array to be summed.
x, y : array_like
Center coordinates and radius (radii) of aperture(s).
xcorresponds to the second (“fast”) axis of the input array andycorresponds to the first (“slow”) axis.x, y = (0.0, 0.0)corresponds to the center of the first element of the array. Shapes must match.rmax : array_like
Maximum radius to analyze. Used as normalizing flux if
normfluxis None. Shape must match x and y.frac : array_like
Requested fraction of light (in range 0 to 1). Can be scalar or array.
normflux : array_like, optional
Normalizing flux for each position. If not given, the sum within
rmaxis used as the normalizing flux. If given, shape must match x, y and rmax.mask :
ndarray, optionalMask array. If supplied, a given pixel is masked if its value is greater than
maskthresh.maskthresh : float, optional
Threshold for a pixel to be masked. Default is
0.0.subpix : int, optional
Subpixel sampling factor. Default is 5.
Returns: radius :
ndarrayThe sum of the data array within the aperture(s). Shape is same as
x, except iffracis an array; then the dimension offracwill be appended. For example, ifxandfracare both 1-d arrays, the result will be a 2-d array with the trailing dimension corresponding tofrac.flags :
ndarrayInteger giving flags. Same shape as
x. (0 if no flags set.)