hillas

hipecta._image.hillas()

Make the Hillas reconstruction with a telescope Parameter: ———- tab_signal : one dimension numpy ndarray

signal in the pixels’ telescope

tabX : one dimension numpy ndarray

position of the pixels on the x axis

tabY : one dimension numpy ndarray Return: ——- tulpe conaining twelve elements: - float: gx, X coordinate of the center of gravity of the shower in the camera - float: gy, Y coordinate of the center of gravity of the shower in the camera - float: phi, Orientation angle of Major Axis w.r.t. x-axis - float: width, telescope image width - float: length, telescope image length - float: imageAmplitude, Total aplitude of the signal in all pixels of the telescope - int : nbSelectedPixel, Number of selected pixels - float: skewness, Assymetry of the image - float: skewnessPhi, Assymetry of the shower - float: kurtosis, Kurtosis excess, define the peakedness of the distribution - float: direction, direction, angle of the shower - float: hofmannSeparation, Hofmann Separation; kurtosis along width axis