Commit 3351be22 authored by Wei Chengliang's avatar Wei Chengliang
Browse files

update codestyle-PEP8

parent 8fd9723d

observation_sim/mock_objects/Quasar.py

+1 −1
Original line number Original line Diff line number Diff line
@@ -98,7 +98,7 @@ class Quasar(MockObject): 
        del self.sed

        del self.sed





    def getGSObj(self, psf, g1=0, g2=0, flux=None, filt=None, tel=None, exptime=150.):

    def getGSObj(self, psf, g1=0, g2=0, flux=None, filt=None, tel=None, exptime=150.):

        if flux == None:

        if flux is None:

            flux = self.getElectronFluxFilt(filt, tel, exptime)

            flux = self.getElectronFluxFilt(filt, tel, exptime)

        qso = galsim.Gaussian(sigma=1.e-8, flux=1.)

        qso = galsim.Gaussian(sigma=1.e-8, flux=1.)

        qso = qso.withFlux(flux)

        qso = qso.withFlux(flux)

observation_sim/mock_objects/Stamp.py

+1 −1
Original line number Original line Diff line number Diff line
@@ -21,7 +21,7 @@ class Stamp(MockObject): 
        del self.sed

        del self.sed





    def drawObj_multiband(self, tel, pos_img, psf_model, bandpass_list, filt, chip, nphotons_tot=None, g1=0, g2=0, exptime=150., fd_shear=None):

    def drawObj_multiband(self, tel, pos_img, psf_model, bandpass_list, filt, chip, nphotons_tot=None, g1=0, g2=0, exptime=150., fd_shear=None):

        if nphotons_tot == None:

        if nphotons_tot is None:

            nphotons_tot = self.getElectronFluxFilt(filt, tel, exptime)

            nphotons_tot = self.getElectronFluxFilt(filt, tel, exptime)





        try:

        try:

observation_sim/mock_objects/Star.py

+2 −2
Original line number Original line Diff line number Diff line
@@ -22,7 +22,7 @@ class Star(MockObject): 
        del self.sed

        del self.sed





    def getGSObj(self, psf, g1=0, g2=0, flux=None, filt=None, tel=None, exptime=150.):

    def getGSObj(self, psf, g1=0, g2=0, flux=None, filt=None, tel=None, exptime=150.):

        if flux == None:

        if flux is None:

            flux = self.getElectronFluxFilt(filt, tel, exptime)

            flux = self.getElectronFluxFilt(filt, tel, exptime)

        # star = galsim.Gaussian(sigma=1.e-8, flux=1.)

        # star = galsim.Gaussian(sigma=1.e-8, flux=1.)

        star = galsim.DeltaFunction()

        star = galsim.DeltaFunction()
@@ -35,7 +35,7 @@ class Star(MockObject): 
            raise ValueError(

            raise ValueError(

                "!!!The number of PSF profiles and the number of bandpasses must be equal.")

                "!!!The number of PSF profiles and the number of bandpasses must be equal.")

        objs = []

        objs = []

        if nphotons_tot == None:

        if nphotons_tot is None:

            nphotons_tot = self.getElectronFluxFilt(filt, tel, exptime)

            nphotons_tot = self.getElectronFluxFilt(filt, tel, exptime)





        try:

        try:

tests/test_SpecDisperse.py

+2 −2
Original line number Original line Diff line number Diff line
@@ -428,8 +428,8 @@ class TestSpecDisperse(unittest.TestCase): 
        plt.xlim(6200, 10000)

        plt.xlim(6200, 10000)

        plt.ylim(1, 4)

        plt.ylim(1, 4)

        plt.yscale('log')

        plt.yscale('log')

        plt.xlabel('$\lambda$')

        plt.xlabel(r'$\lambda$')

        plt.ylabel('$F\lambda$')

        plt.ylabel(r'$F\lambda$')

        plt.legend(['one spec', 'split in 8000 A'])

        plt.legend(['one spec', 'split in 8000 A'])

        plt.show()

        plt.show()

tests/test_Straylight.py

+1 −1
Original line number Original line Diff line number Diff line
@@ -192,7 +192,7 @@ class TestStraylight(unittest.TestCase): 
        plt.figure()

        plt.figure()

        plt.plot(spec['WAVELENGTH'], spec['FLUX'], 'r')

        plt.plot(spec['WAVELENGTH'], spec['FLUX'], 'r')

        plt.xlabel('WAVELENGTH')

        plt.xlabel('WAVELENGTH')

        plt.ylabel('F$\lambda$(erg/s/cm2/A/arcsec2)')

        plt.ylabel(r'F$\lambda$(erg/s/cm2/A/arcsec2)')

        plt.xlim(2000, 10000)

        plt.xlim(2000, 10000)

        plt.show()

        plt.show()

        median = np.median(sl_e_pix[0:tnum])

        median = np.median(sl_e_pix[0:tnum])