Exemplo n.º 1
0
                    if len(indices[0]) != 2:
                        print("SKIIIIIIIIIIIIPUH")
                        continue


                    
                    # Initiate third sublist of F for distinguishing between different aperture radii
                    F_3lst, sigmaF_3lst = [], [] 
                    for l, R in enumerate(r_range):  

                        # Lists for temporary storage of aperture sum values and corresponding shotnoise levels
                        apsum_lst, shotnoise_lst = [], []
                        for ind in indices[0]:
                        
                            # Compute cumulative counts within aperture
                            apsum = aper.apersum(data, xcoords[ind], ycoords[ind], R)
                            apsum_lst.append(apsum)
                            # Compute photon shot noise within aperture 
                            shotnoise = np.sqrt(apsum)
                            shotnoise_lst.append(shotnoise)

                        # Compute normalised flux differences for current aperture size
                        F, sigmaF = fluxdiff_norm(apsum_lst[1], apsum_lst[0], shotnoise_lst[1], shotnoise_lst[0]) 




                        # Append results to third sublist
                        F_3lst.append(F), sigmaF_3lst.append(sigmaF)
                    # Append the third sublist to the second sublist
                    F_2lst.append(F_3lst), sigmaF_2lst.append(sigmaF_3lst)
Exemplo n.º 2
0
                    # TODO THERE MIGHT STILL BE THE POSSIBILITY THAT FALSE SOURCES ARE TAKEN INTO ACCOUNT, IF THERE ARE TWO WITHIN <=5 PIXELS PROXIMITY FROM EACH OTHER
                    if len(indices[0]) != 2:
                        print("Possible Artefact!")
                        xcs_lstDEL = np.delete(xcs_lst, q, 0)
                        continue

                    # Initiate third sublist of F for distinguishing between different aperture radii
                    F_3lst, sigmaF_3lst = [], []
                    for l, R in enumerate(r_range):

                        # Lists for temporary storage of aperture sum values and corresponding shotnoise levels
                        apsum_lst, shotnoise_lst = [], []
                        for ind in indices[0]:

                            # Compute cumulative counts within aperture
                            apsum = aper.apersum(data, xcs_lst[ind],
                                                 ycs_lst[ind], R)
                            apsum_lst.append(apsum)
                            # Compute photon shot noise within aperture
                            shotnoise = np.sqrt(apsum)
                            shotnoise_lst.append(shotnoise)

                        # Compute normalised flux differences for current aperture size
                        F, sigmaF = fluxdiff_norm(apsum_lst[1], apsum_lst[0],
                                                  shotnoise_lst[1],
                                                  shotnoise_lst[0])

                        # Append results to third sublist
                        F_3lst.append(F), sigmaF_3lst.append(sigmaF)
                    # Append the third sublist to the second sublist
                    F_2lst.append(F_3lst), sigmaF_2lst.append(sigmaF_3lst)
            print("\t\t\tF_2lst:\t{}".format(len(F_2lst)))