Commit 9b95b859 authored by Fang Yuedong's avatar Fang Yuedong
Browse files

Merge branch 'develop' into sim_scheduler

parents 4f32a363 86563808
...@@ -5,4 +5,5 @@ conda install numpy==1.26.4 ...@@ -5,4 +5,5 @@ conda install numpy==1.26.4
conda install cython==3.0.6 conda install cython==3.0.6
conda install sep==1.2.1 conda install sep==1.2.1
conda install mpi4py==3.1.6 conda install mpi4py==3.1.6
pip install -e . python3 setup.py install --user
\ No newline at end of file pip install -e .
...@@ -10,4 +10,5 @@ h5py==3.11.0 ...@@ -10,4 +10,5 @@ h5py==3.11.0
Cython==3.0.6 Cython==3.0.6
numba==0.59.1 numba==0.59.1
psutil==5.9.8 psutil==5.9.8
toml==0.10.2 toml==0.10.2
\ No newline at end of file lmfit==1.2.2
\ No newline at end of file
...@@ -98,7 +98,7 @@ setup(name='CSSTSim', ...@@ -98,7 +98,7 @@ setup(name='CSSTSim',
'ObservationSim.Instrument.data.sls_conf': ['*.conf', '*.fits'], 'ObservationSim.Instrument.data.sls_conf': ['*.conf', '*.fits'],
'ObservationSim.Instrument.data.flatCube': ['*.fits'], 'ObservationSim.Instrument.data.flatCube': ['*.fits'],
'Catalog.data': ['*.fits','*.so'], 'Catalog.data': ['*.fits','*.so'],
'ObservationSim.Config.Header':['*.header','*.lst'], 'ObservationSim.Config.Header':['*.fits','*.lst'],
'ObservationSim.Straylight.data': ['*.dat'], 'ObservationSim.Straylight.data': ['*.dat'],
'ObservationSim.Straylight.data.sky': ['*.dat'], 'ObservationSim.Straylight.data.sky': ['*.dat'],
'ObservationSim.Straylight.lib': ['*'], 'ObservationSim.Straylight.lib': ['*'],
......
...@@ -138,15 +138,15 @@ class DetTest(unittest.TestCase): ...@@ -138,15 +138,15 @@ class DetTest(unittest.TestCase):
newimg.write(os.path.join(self.outDataFn,'test_badlines.fits')) newimg.write(os.path.join(self.outDataFn,'test_badlines.fits'))
del newimg,img del newimg,img
def test_cte(self): # def test_cte(self):
img = galsim.Image(200,200,init_value=1000) # img = galsim.Image(200,200,init_value=1000)
img.array[50,80] = 1e4 # img.array[50,80] = 1e4
img.array[150,150] = 3e4 # img.array[150,150] = 3e4
newimgcol = Effects.CTE_Effect(copy.deepcopy(img),direction='column') # newimgcol = Effects.CTE_Effect(copy.deepcopy(img),direction='column')
newimgrow = Effects.CTE_Effect(copy.deepcopy(img),direction='row') # newimgrow = Effects.CTE_Effect(copy.deepcopy(img),direction='row')
newimgcol.write(os.path.join(self.outDataFn,'test_ctecol.fits')) # newimgcol.write(os.path.join(self.outDataFn,'test_ctecol.fits'))
newimgrow.write(os.path.join(self.outDataFn,'test_cterow.fits')) # newimgrow.write(os.path.join(self.outDataFn,'test_cterow.fits'))
del img,newimgcol,newimgrow # del img,newimgcol,newimgrow
def test_readnoise(self): def test_readnoise(self):
img = galsim.Image(200,200,init_value=1000) img = galsim.Image(200,200,init_value=1000)
......
...@@ -231,16 +231,16 @@ class TestSpecDisperse(unittest.TestCase): ...@@ -231,16 +231,16 @@ class TestSpecDisperse(unittest.TestCase):
ids1 = wave_pix[ids] > 6500 ids1 = wave_pix[ids] > 6500
print('Spec disperse flux test') print('Spec disperse flux test')
self.assertTrue(np.mean((wave_flux[ids][ids1] - sed_i(wave_pix[ids][ids1]))/sed_i(wave_pix[ids][ids1]))<0.004) self.assertTrue(np.mean((wave_flux[ids][ids1] - sed_i(wave_pix[ids][ids1]))/sed_i(wave_pix[ids][ids1]))<0.004)
plt.figure() # plt.figure()
plt.plot(wave_pix, wave_flux) # plt.plot(wave_pix, wave_flux)
plt.plot(sed['WAVELENGTH'], sed['FLUX']) # plt.plot(sed['WAVELENGTH'], sed['FLUX'])
plt.xlim(6200, 10000) # plt.xlim(6200, 10000)
plt.ylim(1, 3) # plt.ylim(1, 3)
plt.yscale('log') # plt.yscale('log')
plt.xlabel('$\lambda$') # plt.xlabel('$\lambda$')
plt.ylabel('$F\lambda$') # plt.ylabel('$F\lambda$')
plt.legend(['extracted', 'input']) # plt.legend(['extracted', 'input'])
plt.show() # plt.show()
def test_Specdistperse2(self): def test_Specdistperse2(self):
...@@ -303,16 +303,16 @@ class TestSpecDisperse(unittest.TestCase): ...@@ -303,16 +303,16 @@ class TestSpecDisperse(unittest.TestCase):
self.assertTrue(fwhmx/deltLamda_pix*pix_scale - psf_fwhm < np.abs(0.02)) self.assertTrue(fwhmx/deltLamda_pix*pix_scale - psf_fwhm < np.abs(0.02))
# print('error is ',np.mean((wave_flux[ids][ids1] - sed_i(wave_pix[ids][ids1]))/sed_i(wave_pix[ids][ids1]))) # print('error is ',np.mean((wave_flux[ids][ids1] - sed_i(wave_pix[ids][ids1]))/sed_i(wave_pix[ids][ids1])))
# self.assertTrue(np.mean((wave_flux[ids][ids1] - sed_i(wave_pix[ids][ids1]))/sed_i(wave_pix[ids][ids1]))<0.004) # self.assertTrue(np.mean((wave_flux[ids][ids1] - sed_i(wave_pix[ids][ids1]))/sed_i(wave_pix[ids][ids1]))<0.004)
plt.figure() # plt.figure()
plt.plot(wave_pix, wave_flux) # plt.plot(wave_pix, wave_flux)
plt.plot(sed['WAVELENGTH'], sed['FLUX']) # plt.plot(sed['WAVELENGTH'], sed['FLUX'])
plt.xlim(6200, 10000) # plt.xlim(6200, 10000)
plt.ylim(1, 75) # plt.ylim(1, 75)
plt.yscale('log') # plt.yscale('log')
plt.xlabel('$\lambda$') # plt.xlabel('$\lambda$')
plt.ylabel('$F\lambda$') # plt.ylabel('$F\lambda$')
plt.legend(['extracted', 'input']) # plt.legend(['extracted', 'input'])
plt.show() # plt.show()
def test_Specdistperse3(self): def test_Specdistperse3(self):
......
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