sensitivity_gamma_efficiency

lstchain.mc.sensitivity.sensitivity_gamma_efficiency(dl2_file_g, dl2_file_p, ntelescopes_gammas, ntelescopes_protons, n_bins_energy, gamma_eff_gammaness, gamma_eff_theta2, noff, obstime=<Quantity 180000. s>)

Main function to calculate the sensitivity for cuts based on gamma efficiency

Parameters:

dl2_file_g: `string` path to h5 file of reconstructed gammas

dl2_file_p: `string’ path to h5 file of reconstructed protons

ntelescopes_gammas: `int` number of telescopes used

ntelescopes_protons: `int` number of telescopes used

n_bins_energy: `int` number of bins in energy

gamma_eff_gammaness: `float` between 0 and 1 %/100

of gammas to be left after cut in gammaness

gamma_eff_theta2: `float` between 0 and 1 %/100

of gammas to be left after cut in theta2

noff: `float` ratio between the background and the signal region

obstime: `Quantity` Observation time in seconds

Returns:

energy: array center of energy bins

sensitivity: array sensitivity per energy bin