Loading csst_mci_sim/support/MCIinstrumentModel.pydeleted 100644 → 0 +0 −68 Original line number Diff line number Diff line """ VIS Instrument Model ==================== The file provides a function that returns VIS related information such as pixel size, dark current, gain, zeropoint, and sky background. :requires: NumPy :requires: numexpr :version: 0.7 """ # import matplotlib # import matplotlib.pyplot as plt # import datetime, math # import numpy as np # import numexpr as ne def MCIinformation(): """ Returns a dictionary describing MCI CCD. The following information is provided (id: value - reference):: dob: 0 - CDM03 (Short et al. 2010) fwc: 90000 - CCD spec EUCL-EST-RS-6-002 (for CDM03) rdose: 30000000000.0 - derived (above the PLM requirement) sfwc: 730000.0 - CDM03 (Short et al. 2010), see also the CCD spec EUCL-EST-RS-6-002 st: 5e-06 - CDM03 (Short et al. 2010) svg: 1e-10 - CDM03 (Short et al. 2010) t: 0.01024 - CDM03 (Short et al. 2010) trapfile: cdm_euclid.dat - CDM03 (derived, refitted to CCD204 data) vg: 6e-11 - CDM03 (Short et al. 2010) vth: 11680000.0 - CDM03 (Short et al. 2010) :return: instrument model parameters :rtype: dict """ ######################################################################################################### out=dict() out.update({'dob' : 0, 'rdose' : 8.0e9, 'parallelTrapfile' : 'cdm_euclid_parallel.dat', 'serialTrapfile' : 'cdm_euclid_serial.dat', 'beta_s' : 0.6, 'beta_p': 0.6, 'fwc' : 90000, 'vth' : 1.168e7, 't' : 20.48e-3, 'vg' : 6.e-11, 'st' : 5.0e-6, 'sfwc' : 730000., 'svg' : 1.0e-10}) return out # def CCDnonLinearityModel(data, beta=6e-7): # """ # The non-linearity is modelled based on the results presented. # :param data: data to which the non-linearity model is being applied to # :type data: ndarray # :return: input data after conversion with the non-linearity model # :rtype: float or ndarray # """ # out = data-beta*data**2 # return out ################################################################### # if __name__ == '__main__': # print() Loading
csst_mci_sim/support/MCIinstrumentModel.pydeleted 100644 → 0 +0 −68 Original line number Diff line number Diff line """ VIS Instrument Model ==================== The file provides a function that returns VIS related information such as pixel size, dark current, gain, zeropoint, and sky background. :requires: NumPy :requires: numexpr :version: 0.7 """ # import matplotlib # import matplotlib.pyplot as plt # import datetime, math # import numpy as np # import numexpr as ne def MCIinformation(): """ Returns a dictionary describing MCI CCD. The following information is provided (id: value - reference):: dob: 0 - CDM03 (Short et al. 2010) fwc: 90000 - CCD spec EUCL-EST-RS-6-002 (for CDM03) rdose: 30000000000.0 - derived (above the PLM requirement) sfwc: 730000.0 - CDM03 (Short et al. 2010), see also the CCD spec EUCL-EST-RS-6-002 st: 5e-06 - CDM03 (Short et al. 2010) svg: 1e-10 - CDM03 (Short et al. 2010) t: 0.01024 - CDM03 (Short et al. 2010) trapfile: cdm_euclid.dat - CDM03 (derived, refitted to CCD204 data) vg: 6e-11 - CDM03 (Short et al. 2010) vth: 11680000.0 - CDM03 (Short et al. 2010) :return: instrument model parameters :rtype: dict """ ######################################################################################################### out=dict() out.update({'dob' : 0, 'rdose' : 8.0e9, 'parallelTrapfile' : 'cdm_euclid_parallel.dat', 'serialTrapfile' : 'cdm_euclid_serial.dat', 'beta_s' : 0.6, 'beta_p': 0.6, 'fwc' : 90000, 'vth' : 1.168e7, 't' : 20.48e-3, 'vg' : 6.e-11, 'st' : 5.0e-6, 'sfwc' : 730000., 'svg' : 1.0e-10}) return out # def CCDnonLinearityModel(data, beta=6e-7): # """ # The non-linearity is modelled based on the results presented. # :param data: data to which the non-linearity model is being applied to # :type data: ndarray # :return: input data after conversion with the non-linearity model # :rtype: float or ndarray # """ # out = data-beta*data**2 # return out ################################################################### # if __name__ == '__main__': # print()