def compute_XD_results(n_components=10, max_iter=500):
clf = XDGMM(n_components,
max_iter=max_iter,
tol=1e-03,
verbose=False,
random_state=None)
clf.fit(Z, Zerr)
return clf
def XD_filter(y , yerr):
clf = XDGMM(n_components = 2 , n_iter = 4)
Y = y.reshape(y.shape[0] , 1)
Yerr = np.zeros((y.shape[0] , 1, 1))
#diag = np.arange(Y.shape[-1])
Yerr[:, 0, 0] = yerr ** 2
clf.fit(Y , Yerr)
return clf.mu, clf.V
def __init__(self,algorithm='XD',n_comp = 20):
if algorithm == 'XD':
self.algorithm='XD'
self.lQSO_model = XDGMM(n_components=n_comp,verbose=True)
self.dud_model = XDGMM(n_components=n_comp,verbose=True)
elif algorithm == 'RandomForest':
self.algorithm = 'RandomForest'
self.trialRF = RandomForestClassifier()
self.RF_params = {'n_estimators':(10,50,200),"max_features": ["auto",2,4],
'criterion':["gini","entropy"],"min_samples_leaf": [1,2]}
return
def _xdFit(X, XErr, nGauss, n_iter=10):
gmm = GMM(nGauss, n_iter=n_iter, covariance_type='full').fit(X)
amp = gmm.weights_
mean = gmm.means_
covar = gmm.covars_
xd.extreme_deconvolution(X, XErr, amp, mean, covar)
clf = XDGMM(nGauss)
clf.alpha = amp
clf.mu = mean
clf.V = covar
return clf
def compute_XD_results(x, y, dx, dy, n_components=6, n_iter=50):
X = np.vstack([x,y]).T
Xerr = np.zeros(X.shape + X.shape[-1:])
diag = np.arange(X.shape[-1])
Xerr[:, diag, diag] = np.vstack([dx ** 2, dy ** 2]).T
clf = None
while clf is None:
try:
clf = XDGMM(n_components, n_iter=n_iter,verbose=True)
clf.fit(X, Xerr)
except:
print('Error: Singular Matrix. Retrying...')
clf = None
return clf
def initialise(self):
nmeas, ndim = self.data.shape
lower_idxs = np.tril_indices(ndim, k=-1)
if self.data_covariances is not None:
xdgmm = XDGMM(1, 1000, verbose=True)
xdgmm.fit(self.data, self.data_covariances)
guess_mu = xdgmm.mu[0]
guess_Sigma = xdgmm.V[0]
else:
gmm = GaussianMixture(1, max_iter=1000, covariance_type='full').fit(self.data)
guess_mu = gmm.means_[0]
guess_Sigma = gmm.covariances_[0]
guess_chol = np.linalg.cholesky(guess_Sigma)
guess_packed_chol = guess_chol[lower_idxs]
return guess_mu, guess_Sigma, guess_packed_chol, guess_chol
def check_single_gaussian(N=100, D=3, sigma=0.1):
np.random.seed(0)
mu = np.random.random(D)
V = np.random.random((D, D))
V = np.dot(V, V.T)
X = np.random.multivariate_normal(mu, V, size=N)
Xerr = np.zeros((N, D, D))
Xerr[:, range(D), range(D)] = sigma ** 2
X += np.random.normal(0, sigma, X.shape)
xdgmm = XDGMM(1)
xdgmm.fit(X, Xerr)
# because of sample variance, results will be similar
# but not identical. We'll use a fudge factor of 0.1
assert_allclose(mu, xdgmm.mu[0], atol=0.1)
assert_allclose(V, xdgmm.V[0], atol=0.1)
def check_single_gaussian(N=100, D=3, sigma=0.1):
np.random.seed(0)
mu = np.random.random(D)
V = np.random.random((D, D))
V = np.dot(V, V.T)
X = np.random.multivariate_normal(mu, V, size=N)
Xerr = np.zeros((N, D, D))
Xerr[:, range(D), range(D)] = sigma**2
X += np.random.normal(0, sigma, X.shape)
xdgmm = XDGMM(1)
xdgmm.fit(X, Xerr)
# because of sample variance, results will be similar
# but not identical. We'll use a fudge factor of 0.1
assert_allclose(mu, xdgmm.mu[0], atol=0.1)
assert_allclose(V, xdgmm.V[0], atol=0.1)
def getMarginalClf(self, cols=None):
if cols is None:
raise ValueError(
"You have to specify the columns you want to keep so that I can marginalizse over the rest."
)
rowsV, colsV = np.meshgrid(cols, cols, indexing='ij')
xdMarginal = XDClf(ngStar=self.ngStar,
ngGal=self.ngGal,
priorStar=self.priorStar)
xdMarginal.clfStar = XDGMM(self.ngStar)
xdMarginal.clfStar.alpha = self.clfStar.alpha
xdMarginal.clfStar.mu = self.clfStar.mu[:, cols]
xdMarginal.clfStar.V = self.clfStar.V[:, rowsV, colsV]
xdMarginal.clfGal = XDGMM(self.ngGal)
xdMarginal.clfGal.alpha = self.clfGal.alpha
xdMarginal.clfGal.mu = self.clfGal.mu[:, cols]
xdMarginal.clfGal.V = self.clfGal.V[:, rowsV, colsV]
if self.priorStar == 'auto':
xdMarginal._priorStar = self._priorStar
return xdMarginal
def main(ps1_file, g_lim):
try:
ps1 = np.load(ps1_file)
except:
ps1 = ascii.read(ps1_file)
cut_ps1 = cut_func(ps1, g_lim=g_lim)
ps1_c = coord.SkyCoord(ra=cut_ps1['ra']*u.degree,
dec=cut_ps1['dec']*u.degree)
cut_ps1 = cut_ps1[ps1_c.separation(cluster_c) > (0.12*u.degree)]
# feature and covariance matrices
X,Xcov = data_to_X_cov(cut_ps1)
n_clusters = 8
n_iter = 512
xd_clf = XDGMM(n_clusters, n_iter=n_iter, tol=1E-4, verbose=True)
xd_clf.fit(X[::100], Xcov[::100])
# pickle this thing! xd_clf
with open("xd_control_clf.pickle", "wb") as f:
pickle.dump(xd_clf, f)
def test_XDGMM_1D_gaussian(N=100, sigma=0.1):
np.random.seed(0)
mu = 0
V = 1
X = np.random.normal(mu, V, size=(N, 1))
X += np.random.normal(0, sigma, size=(N, 1))
Xerr = sigma**2 * np.ones((N, 1, 1))
xdgmm = XDGMM(1).fit(X, Xerr)
# because of sample variance, results will be similar
# but not identical. We'll use a fudge factor of 0.1
assert_allclose(mu, xdgmm.mu[0], atol=0.1)
assert_allclose(V, xdgmm.V[0], atol=0.1)
def TryModel(nGaussiansStar, nGaussiansGalaxy):
print 'Star Gaussians: {0}'.format(nGaussiansStar)
print 'Galaxy Gaussians: {0}'.format(nGaussiansGalaxy)
#convolving
print 'Estimating Gaussians'
GMMStar = GMM(nGaussiansStar, n_iter = 10, covariance_type='full').fit(XTrainStar)
GMMGalaxy = GMM(nGaussiansGalaxy, n_iter=10, covariance_type='full').fit(XTrainGalaxy)
ampstar = GMMStar.weights_
meanstar = GMMStar.means_
covarstar = GMMStar.covars_
ampgalaxy = GMMGalaxy.weights_
meangalaxy = GMMGalaxy.means_
covargalaxy = GMMGalaxy.covars_
# Results are saved in `amp`, `mean`, and `covar`
print 'Deconvolving star'
xd.extreme_deconvolution(XTrainStar, XErrTrainStar, ampstar, meanstar, covarstar)
clfstar = XDGMM(nGaussiansStar)
clfstar.alpha = ampstar
clfstar.mu = meanstar
clfstar.V = covarstar
print 'Deconvolving galaxies'
xd.extreme_deconvolution(XTrainGalaxy, XErrTrainGalaxy, ampgalaxy, meangalaxy, covargalaxy)
clfgalaxy = XDGMM(nGaussiansGalaxy)
clfgalaxy.alpha = ampgalaxy
clfgalaxy.mu = meangalaxy
clfgalaxy.V = covargalaxy
print 'Predicting'
# need to pass XTestStar[i] and XTestGalaxy[i] as np.array([XTestStar[i]]) because internally it assumes 2D matrix
starPredictions = np.array([predictStar(clfstar, clfgalaxy, np.array([XTestStar[i]]), np.array([XErrTestStar[i]]), i) for i in range(starTestNumber)])
galaxyPredictions = np.array([predictStar(clfstar, clfgalaxy, np.array([XTestGalaxy[i]]), np.array([XErrTestGalaxy[i]]), i) for i in range(galaxyTestNumber)])
predictions = np.array(starPredictions.tolist() + galaxyPredictions.tolist())
results = np.array([1 for i in range(len(starPredictions))] + [0 for i in range(len(galaxyPredictions))])
report = generateReport(predictions, results)
return (report['Precision'], report['Recall'], clfstar, clfgalaxy)
def mixture_fitting(args):
'''
component = 0 : u-g, 1: g-r, 2: r-i
'''
zmin, zmax, component = args
zspec, x, xerr, color, color_err = catalog_slicer(zmin, zmax, component)
Y_xd = np.vstack([x,color[component,:]]).T
Yerr_xd = np.zeros((Y_xd.shape[0] , 2 , 2))
Yerr_xd[:,0,0] = xerr
Yerr_xd[:,1,1] = color_err[component,component,:]
#fitting a two component GMM to (mi , color(component) space in the redshift bin)
clf_in = XDGMM(2, n_iter=400)
clf_in.fit(Y_xd, Yerr_xd)
# mixture component associated with the red population
red_index = np.where(clf_in.mu[:,1] == clf_in.mu[:,1].max())[0]
mu_red , V_red= clf_in.mu[red_index] , clf_in.V[red_index][0]
red_line = mu_red[0,1] + V_red[0,1]*(Y_xd[:,0] - mu_red[0,0])/V_red[0,0]
red_scatter = V_red[1,1] - V_red[0,1]**2./V_red[0,0]
chi_red = (Y_xd[:,1] - red_line)**2. / (red_scatter + Yerr_xd[:,1,1])
mask = chi_red < 2
##UPDATE : I have converged on using g-r for masking purposes!!
# at this point we don't care which color component was used for masking
# we keep the masked galaxies (chisq<2) and fit a linear line to the i-colors.
# this step is agnostic about the color component used for masking
# note that we ahve used mu_red[0,0] (the first component of the center of the red galaxies) as m_ref
x_xd = x[mask]
xerr_xd = x[mask]
Y_xd = np.vstack([color[0,mask], color[1,mask], color[2,mask]]).T
Yerr_xd = np.zeros((Y_xd.shape[0] , 3 , 3))
for i in xrange(3):
for j in xrange(3):
Yerr_xd[:,i,j] = color_err[i,j,mask]
# fitting a two component GMM to the remainder of galaxies in the three dimensional colorspace
clf_fi = XDGMM(2, n_iter=400)
clf_fi.fit(Y_xd, Yerr_xd)
pure_index = np.where(clf_fi.mu[:,1] == clf_fi.mu[:,1].max())
mu_pure , V_pure = clf_fi.mu[pure_index] , clf_fi.V[pure_index][0]
dY_pure = Y_xd - mu_pure
P = np.linalg.inv(V_pure + Yerr_xd)
chi = np.einsum('mn,mn->m', np.einsum('ijk,ik->ij', P, dY_pure) , dY_pure)
pure_mask = chi<2
zred = zspec[mask][pure_mask]
zred = zred.reshape(zred.shape[0],1)
ired = x_xd[pure_mask]
ired = ired.reshape(ired.shape[0],1)
eired = xerr_xd[pure_mask]
eired = ired.reshape(eired.shape[0],1)
cred = Y_xd[pure_mask]
ecred = Yerr_xd[pure_mask].reshape(cred.shape[0],cred.shape[1]*cred.shape[1])
return [mu_red[0,0] , np.hstack([zred,ired,eired,cred,ecred])]
def compute_XD(n_clusters=12, rseed=0, n_iter=100, verbose=True):
np.random.seed(rseed)
clf = XDGMM(n_clusters, n_iter=n_iter, tol=1E-5, verbose=verbose)
clf.fit(X, Xcov)
return clf
def compute_XD_results(n_components=10, n_iter=500):
clf = XDGMM(n_components, n_iter=n_iter)
clf.fit(X, Xerr)
return clf
def compute_XD_results(n_components=10, n_iter=500):
clf = XDGMM(n_components, n_iter=n_iter)
clf.fit(X, Xerr)
return clf
def compute_XD(n_clusters=12, rseed=0, max_iter=100, verbose=True):
np.random.seed(rseed)
clf = XDGMM(n_clusters, max_iter=max_iter, tol=1E-5, verbose=verbose)
clf.fit(X, Xcov)
return clf
ampstar = GMMStar.weights_ meanstar = GMMStar.means_ covarstar = GMMStar.covars_ ampgalaxy = GMMGalaxy.weights_ meangalaxy = GMMGalaxy.means_ covargalaxy = GMMGalaxy.covars_ # Results are saved in `amp`, `mean`, and `covar` print 'Deconvolving star' xd.extreme_deconvolution(XTrainStar, XErrTrainStar, ampstar, meanstar, covarstar) clfstar = XDGMM(nGaussiansStar) clfstar.alpha = ampstar clfstar.mu = meanstar clfstar.V = covarstar print 'Deconvolving galaxies' xd.extreme_deconvolution(XTrainGalaxy, XErrTrainGalaxy, ampgalaxy, meangalaxy, covargalaxy) clfgalaxy = XDGMM(nGaussiansGalaxy) clfgalaxy.alpha = ampgalaxy clfgalaxy.mu = meangalaxy clfgalaxy.V = covargalaxy print 'Predicting' # need to pass XTestStar[i] and XTestGalaxy[i] as np.array([XTestStar[i]]) because internally it assumes 2D matrix
class Classifier(object):
def __init__(self,algorithm='XD',n_comp = 20):
if algorithm == 'XD':
self.algorithm='XD'
self.lQSO_model = XDGMM(n_components=n_comp,verbose=True)
self.dud_model = XDGMM(n_components=n_comp,verbose=True)
elif algorithm == 'RandomForest':
self.algorithm = 'RandomForest'
self.trialRF = RandomForestClassifier()
self.RF_params = {'n_estimators':(10,50,200),"max_features": ["auto",2,4],
'criterion':["gini","entropy"],"min_samples_leaf": [1,2]}
return
def train(self,train,truth,covmat=1):
if self.algorithm == 'XD':
self.XDtrain(train,truth,covmat)
elif self.algorithm == 'RandomForest':
self.RFtrain(train,truth)
return
def RFtrain(self,train,truth):
tunedRF = grid_search.GridSearchCV(self.trialRF, self.RF_params,\
n_jobs = -1, cv = 3,verbose=1)
self.optRF = tunedRF.fit(train, truth)
return
def XDtrain(self,train,truth,covmat=1):
self.lQSO_model.fit(train[truth==1], listify(covmat,np.sum(truth)))
self.dud_model.fit(train[truth==0], listify(covmat,np.sum(1-truth)))
return
def test(self,test,covmat=1):
if self.algorithm == 'XD':
self.XDprobs(test,covmat)
elif self.algorithm == 'RandomForest':
self.RFprobs(test)
return
def RFprobs(self,test):
self.dud_probs = self.optRF.predict_proba(test)[:,0]
self.lQSO_probs = self.optRF.predict_proba(test)[:,1]
return
def XDprobs(self,test,covmat):
lQSO_like = np.sum(np.exp(self.lQSO_model.logprob_a(test, listify(covmat,test.shape[0]))),axis=1)
dud_like= np.sum(np.exp(self.dud_model.logprob_a(test, listify(covmat,test.shape[0]))),axis=1)
self.lQSO_probs = (lQSO_like * lQSO_prior) / (lQSO_like * lQSO_prior + dud_like * dud_prior)
self.dud_probs = (dud_like * dud_prior) / (lQSO_like * lQSO_prior + dud_like * dud_prior)
return
def make_roc(self,truth):
fpr, tpr, _ = metrics.roc_curve(truth,self.lQSO_probs,pos_label=1)
plt.title('ROC Curve')
plt.plot(fpr,tpr,'b--')
plt.xlabel('FPR')
plt.ylabel('TPR')
return fpr,tpr
def save(self,pkl_fname='classifiers.pkl'):
outfile = open(pkl_fname,'wb')
outDict = {}
if hasattr(self,'lQSO_model'):
outDict.update({'lQSO_model':self.lQSO_model})
if hasattr(self,'dud_model'):
outDict.update({'dud_model':self.dud_model})
if hasattr(self,'optRF'):
outDict.update({'optRF':self.optRF})
pickle.dump(outDict,outfile)
outfile.close()
return
def load(self,pkl_fname='classifiers.pkl'):
pkl_in = open(pkl_fname,'rb')
inDict = pickle.load(pkl_in)
pkl_in.close()
if 'lQSO_model' in inDict.keys():
self.lQSO_model = inDict['lQSO_model']
if 'dud_model' in inDict.keys():
self.dud_model = inDict['dud_model']
if 'optRF' in inDict.keys():
self.optRF = inDict['optRF']
return
def compute_XD(n_clusters=2, rseed=0, n_iter=30, verbose=True):
np.random.seed(rseed)
clf = XDGMM(n_clusters, n_iter=n_iter, tol=1E-5, verbose=verbose)
clf.fit(newZ, Zcov)
return clf
gaussian(x, amp3, mu3, sig3, 0)) + y0
#Lee
ids, pmx, pmy, magK, pmex, pmey = np.genfromtxt('PM_final.dat', unpack=True, usecols=(0,3,4,5,8,9))
#Filtra
mag_mask = (magK < max_mag) & (magK > min_mag)
err_mask = (pmex**2 + pmey**2)**0.5 < max_err
dataset = np.vstack([pmx[mag_mask*err_mask], pmy[mag_mask*err_mask]]).T
dataerr = np.zeros(dataset.shape + dataset.shape[-1:])
diag = np.arange(dataset.shape[-1])
dataerr[:, diag, diag] = np.vstack([pmex[mag_mask*err_mask]**2, pmey[mag_mask*err_mask]**2]).T
clf = XDGMM(compo, itera, verbose=True)
clf.fit(dataset, dataerr)
samples = clf.sample(np.sum(mag_mask*err_mask))
clfu = mixture.VBGMM(compo, covariance_type='full', tol=1e-5, n_iter=1000)
clfu.fit((pmx[mag_mask*err_mask])[:,np.newaxis])
meu = np.hstack(clfu.means_)
stu = np.hstack(clfu.precs_)[0]
weu = np.hstack(clfu.weights_)
clfd = XDGMM(compo, itera, verbose=True)
clfd.fit(pmy[mag_mask*err_mask][:,np.newaxis], (pmey[mag_mask*err_mask]**2)[:,np.newaxis,np.newaxis])
samd = clfd.sample(np.sum(mag_mask*err_mask))
print('Centros:\n', clf.mu)
print('Covarianza:\n', clf.V)
