Commit dd1608ee authored by Yan Zhaojun's avatar Yan Zhaojun
Browse files

debug

parent a5489f19

csst_ifs_sim/csst_ifs_sim.py

+30 −55
Original line number Original line Diff line number Diff line
@@ -22,23 +22,11 @@ from scipy.signal import fftconvolve 
from scipy import ndimage

from scipy import ndimage

import cmath

import cmath

import configparser as ConfigParser

import configparser as ConfigParser



# from support import IFSinstrumentModel

# from support import cosmicrays

# from support import logger as lg

# from CTI import CTI



import os

import os

from scipy.interpolate import interp1d

from scipy.interpolate import interp1d

import astropy.coordinates as coord

import astropy.coordinates as coord

import ctypes

import ctypes

import sys

import sys



# from csst_ifs_sim.support import IFSinstrumentModel

# from csst_ifs_sim.support import cosmicrays

# from csst_ifs_sim.support import logger as lg

# from csst_ifs_sim.CTI import CTI



sys.path.append('./csst_ifs_sim')

sys.path.append('./csst_ifs_sim')

conf.auto_max_age = None

conf.auto_max_age = None
@@ -91,6 +79,9 @@ Note:: This class is Python 3 compatible. 




"""

"""

######################## functions definition ################################

######################## functions definition ################################





class CDM03bidir():

    """

    """

    Charge Transfer Inefficiency

    Charge Transfer Inefficiency

    ============================

    ============================
@@ -103,11 +94,6 @@ parameters in parallel and serial direction. 
    :requires: NumPy

    :requires: NumPy

    :requires: CDM03 (FORTRAN code, f2py -c -m cdm03bidir cdm03bidir.f90)

    :requires: CDM03 (FORTRAN code, f2py -c -m cdm03bidir cdm03bidir.f90)





"""



#CDM03bidir

class CDM03bidir():

    """

    Class to run CDM03 CTI model, class Fortran routine to perform the actual CDM03 calculations.

    Class to run CDM03 CTI model, class Fortran routine to perform the actual CDM03 calculations.





     :param settings: input parameters

     :param settings: input parameters
@@ -181,8 +167,6 @@ class CDM03bidir(): 
        Set up the logger.

        Set up the logger.

        """

        """

        self.logger = True

        self.logger = True

        # if self.log is None:

        #     self.logger = False









    def applyRadiationDamage(self, data, iquadrant=0):

    def applyRadiationDamage(self, data, iquadrant=0):
@@ -309,6 +293,8 @@ def lg(log_filename, loggername='logger'): 








##############################################################################

##############################################################################



def IFSinformation():

    """

    """

    IFS Instrument Model

    IFS Instrument Model

    ====================

    ====================
@@ -316,13 +302,8 @@ IFS Instrument Model 
    The file provides a function that returns IFS related information such as pixel

    The file provides a function that returns IFS related information such as pixel

    size, dark current, gain...

    size, dark current, gain...

    

    

"""

    Returns a dictionary describing VIS. The following information is provided 



    (id: value - reference)::

def IFSinformation():

    """

    Returns a dictionary describing VIS. The following information is provided (id: value - reference)::









    :return: instrument model parameters

    :return: instrument model parameters

    :rtype: dict

    :rtype: dict
@@ -353,7 +334,12 @@ def CCDnonLinearityModel(data, beta=6e-7): 
    return out

    return out





#############################################################################

#############################################################################



from scipy.interpolate import InterpolatedUnivariateSpline



class cosmicrays():

    """

    """

    

    Cosmic Rays

    Cosmic Rays

    ===========

    ===========
@@ -365,18 +351,7 @@ The energy of the cosmic ray events can also be set to constant for 
    testing purposes. The class can be used to draw a single cosmic ray

    testing purposes. The class can be used to draw a single cosmic ray

    event or up to a covering fraction.

    event or up to a covering fraction.





:requires: NumPy

:requires: SciPy



:version: 0.2



"""



from scipy.interpolate import InterpolatedUnivariateSpline







class cosmicrays():

    """

    Cosmic ray generation class. Can either draw events from distributions or

    Cosmic ray generation class. Can either draw events from distributions or

    set the energy of the events to a constant.

    set the energy of the events to a constant.