def test_const_match(w0_test, cosmo_input):
"""test w_matcher gets constant w cosmology correct"""
cosmo_start = cosmo_input[0]
wm = cosmo_input[3]
zs = cosmo_input[5]
w_use_int = w0_test
cosmo_match_a = cosmo_start.copy()
cosmo_match_a['de_model'] = 'jdem'
cosmo_match_a['w0'] = w_use_int
cosmo_match_a['wa'] = 0.
cosmo_match_a['w'] = w_use_int
for i in range(0, 36):
cosmo_match_a['ws36_' + str(i).zfill(2)] = w_use_int
cosmo_match_b = cosmo_match_a.copy()
cosmo_match_b['de_model'] = 'w0wa'
cosmo_match_c = cosmo_match_a.copy()
cosmo_match_c['de_model'] = 'constant_w'
C_match_a = cp.CosmoPie(cosmology=cosmo_match_a, p_space='jdem')
C_match_b = cp.CosmoPie(cosmology=cosmo_match_b, p_space='jdem')
C_match_c = cp.CosmoPie(cosmology=cosmo_match_c, p_space='jdem')
w_a = wm.match_w(C_match_a, zs)
w_b = wm.match_w(C_match_b, zs)
w_c = wm.match_w(C_match_c, zs)
mult_a = wm.match_growth(C_match_a, zs, w_a)
mult_b = wm.match_growth(C_match_b, zs, w_b)
mult_c = wm.match_growth(C_match_c, zs, w_c)
error_a_1 = np.linalg.norm(w_a - C_match_a.de_object.w_of_z(zs)) / w_a.size
error_a_2 = np.linalg.norm(w_use_int - w_a) / zs.size
error_b_1 = np.linalg.norm(w_b - C_match_b.de_object.w_of_z(zs)) / w_b.size
error_b_2 = np.linalg.norm(w_use_int - w_b) / zs.size
error_c_1 = np.linalg.norm(w_c - C_match_c.de_object.w_of_z(zs)) / w_c.size
error_c_2 = np.linalg.norm(w_use_int - w_c) / zs.size
#should usually do more like 1.e-12 or better if no grid issues
atol_loc = 1.e-10
assert error_a_1 < atol_loc
assert error_a_2 < atol_loc
assert error_b_1 < atol_loc
assert error_b_2 < atol_loc
assert error_c_1 < atol_loc
assert error_c_2 < atol_loc
assert np.allclose(w_a, C_match_a.de_object.w_of_z(zs))
assert np.allclose(w_b, C_match_b.de_object.w_of_z(zs))
assert np.allclose(w_c, C_match_c.de_object.w_of_z(zs))
assert np.allclose(w_a, w_use_int)
assert np.allclose(w_b, w_use_int)
assert np.allclose(w_c, w_use_int)
assert np.allclose(mult_a, mult_b)
assert np.allclose(mult_a, mult_c)
assert np.allclose(mult_b, mult_c)
def __init__(self,C_fid,wmatcher_params):
""" C_fid: the fiducial CosmoPie, w(z) irrelevant because it will be ignored
wmatcher_params:
w_step: resolution of w grid
w_min: minimum w to consider
w_max: maximum w to consider
a_step: resolution of a grid
a_min: minimum a to consider
a_max: maximum a to consider
"""
#appears only use of C_fid to extract cosmology
#CosmoPie appears to be used to extract G_norm,G, and Ez
self.C_fid = C_fid
self.cosmo_fid = self.C_fid.cosmology.copy()
self.cosmo_fid['w'] = -1.
self.cosmo_fid['de_model'] = 'constant_w'
self.w_step = wmatcher_params['w_step']
self.w_min = wmatcher_params['w_min']
self.w_max = wmatcher_params['w_max']
self.ws = np.arange(self.w_min,self.w_max,self.w_step)
self.n_w = self.ws.size
self.a_step = wmatcher_params['a_step']
self.a_min = wmatcher_params['a_min']
self.a_max = wmatcher_params['a_max']
self.a_s = np.arange(self.a_max,self.a_min-self.a_step/10.,-self.a_step)
self.n_a = self.a_s.size
self.zs = 1./self.a_s-1.
self.cosmos = np.zeros(self.n_w,dtype=object)
self.integ_Es = np.zeros((self.n_w,self.n_a))
self.Gs = np.zeros((self.n_w,self.n_a))
for i in range(0,self.n_w):
self.cosmos[i] = self.cosmo_fid.copy()
self.cosmos[i]['w'] = self.ws[i]
C_i = cp.CosmoPie(cosmology=self.cosmos[i],p_space=self.cosmo_fid['p_space'],silent=True)
E_as = C_i.Ez(self.zs)
self.integ_Es[i] = cumtrapz(1./(self.a_s**2*E_as)[::-1],self.a_s[::-1],initial=0.)
self.Gs[i] = C_i.G(self.zs)
self.G_interp = RectBivariateSpline(self.ws,self.a_s[::-1],self.Gs[:,::-1],kx=3,ky=3)
self.ind_switches = np.argmax(np.diff(self.integ_Es,axis=0)<0,axis=0)+1
#there is a purely numerical issue that causes the integral to be non-monotonic, this loop eliminates the spurious behavior
for i in range(1,self.n_a):
if self.ind_switches[i]>1:
if self.integ_Es[self.ind_switches[i]-1,i]-self.integ_Es[0,i]>=0:
self.integ_Es[0:(self.ind_switches[i]-1),i] = self.integ_Es[self.ind_switches[i]-1,i]
else:
raise RuntimeError( "Nonmonotonic integral, solution is not unique at "+str(self.a_s[i]))
self.integ_E_interp = RectBivariateSpline(self.ws,self.a_s[::-1],self.integ_Es,kx=3,ky=3)
def test_jdem_w0wa_match(w0_test, wa_test, cosmo_input):
"""check w_matcher gets w0wa cosmology compatible with binned w(z) cosmology"""
cosmo_start = cosmo_input[0]
wm = cosmo_input[3]
zs = cosmo_input[5]
w0_use = w0_test
wa_use = wa_test
cosmo_match_w0wa = cosmo_start.copy()
cosmo_match_jdem = cosmo_start.copy()
cosmo_match_w0wa['de_model'] = 'w0wa'
cosmo_match_w0wa['w0'] = w0_use
cosmo_match_w0wa['wa'] = wa_use
cosmo_match_w0wa['w'] = w0_use #+0.9*wa_use
cosmo_match_jdem['de_model'] = 'jdem'
cosmo_match_jdem['w'] = w0_use + 0.9 * wa_use
a_jdem = 1. - 0.025 * np.arange(0, 36)
for i in range(0, 36):
cosmo_match_jdem[
'ws36_' +
str(i).zfill(2)] = w0_use + (1. -
(a_jdem[i] - 0.025 / 2.)) * wa_use
C_match_w0wa = cp.CosmoPie(cosmology=cosmo_match_w0wa, p_space='jdem')
C_match_jdem = cp.CosmoPie(cosmology=cosmo_match_jdem, p_space='jdem')
w_w0wa = wm.match_w(C_match_w0wa, zs)
w_jdem = wm.match_w(C_match_jdem, zs)
mult_w0wa = wm.match_growth(C_match_w0wa, zs, w_w0wa)
mult_jdem = wm.match_growth(C_match_jdem, zs, w_jdem)
error_w0wa_jdem = np.linalg.norm(w_w0wa - w_jdem) / w_jdem.size
error_mult_w0wa_jdem = np.linalg.norm(mult_w0wa - mult_jdem) / w_jdem.size
assert error_w0wa_jdem < 4.e-4
assert error_mult_w0wa_jdem < 1.e-3
def test_change_params():
"""test rotation function work"""
C_fid = cp.CosmoPie(defaults.cosmology.copy(),'jdem')
f_set_in1 = np.zeros(3,dtype=object)
for i in range(0,3):
f_set1 = np.random.rand(6,6)
f_set1 = np.dot(f_set1.T,f_set1)
f_set1 = f_set1+np.diag(np.random.rand(6))
f_set_in1[i] = f_set1
f_set_in2 = rotate_jdem_to_lihu(f_set_in1,C_fid)
f_set_in3 = rotate_lihu_to_jdem(f_set_in2,C_fid)
f_set_in4 = rotate_jdem_to_lihu(f_set_in3,C_fid)
for i in range(0,3):
assert np.allclose(f_set_in1[i],f_set_in3[i])
assert np.allclose(f_set_in2[i],f_set_in4[i])
def test_vary_1_parameter(param_set, param_vary):
"""test variation of parameters for halofit and linear match expectations from camb"""
atol_rel = 1.e-8
rtol = 3.e-3
eps = 0.1
camb_params = defaults.camb_params.copy()
camb_params['force_sigma8'] = param_set[0]
camb_params['leave_h'] = param_set[1]
power_params = defaults.power_params.copy()
power_params.camb = camb_params
cosmo_fid = defaults.cosmology.copy()
if param_set[2] == 'halofit':
nonlinear_model = camb.model.NonLinear_both
else:
nonlinear_model = camb.model.NonLinear_none
if isinstance(cosmo_fid[param_vary], float):
cosmo_pert = cosmo_fid.copy()
cosmo_pert[param_vary] *= (1. + eps)
print(cosmo_pert['Omegar'])
C_pert = cp.CosmoPie(cosmo_pert, p_space='jdem')
P_pert = mps.MatterPower(C_pert, power_params)
k_pert = P_pert.k
C_pert.k = k_pert
P_res1 = P_pert.get_matter_power(np.array([0.]),
pmodel=param_set[2])[:, 0]
k_res2, P_res2 = camb_pow(C_pert.cosmology,
zbar=np.array([0.]),
camb_params=camb_params,
nonlinear_model=nonlinear_model)
atol_power = np.max(P_res1) * atol_rel
atol_k = np.max(k_pert) * atol_rel
assert np.allclose(k_res2, k_pert, atol=atol_k, rtol=rtol)
assert np.allclose(P_res1, P_res2, atol=atol_power, rtol=rtol)
def cosmo_input():
"""get cosmology for test"""
cosmo_start = defaults.cosmology.copy()
cosmo_start['w'] = -1
cosmo_start['de_model'] = 'constant_w'
C_start = cp.CosmoPie(cosmology=cosmo_start, p_space='jdem')
#base set
#params = {'w_step':0.005,'w_min':-3.50,'w_max':0.1,'a_step':0.001,'a_min':0.000916674,'a_max':1.00}
#mod se
params = {
'w_step': 0.005,
'w_min': -3.5,
'w_max': 0.1,
'a_step': 0.001,
'a_min': 0.000916674,
'a_max': 1.00
}
wm = WMatcher(C_start, params)
a_grid = np.arange(1.00, 0.001, -0.01)
zs = 1. / a_grid - 1.
return [cosmo_start, C_start, params, wm, a_grid, zs]
def test_casarini_match(cosmo_input):
"""check code matches results extracted from a figure"""
cosmo_start = cosmo_input[0]
wm = cosmo_input[3]
#zs = cosmo_input[5]
#should match arXiv:1601.07230v3 figure 2
cosmo_match_a = cosmo_start.copy()
cosmo_match_a['de_model'] = 'w0wa'
cosmo_match_a['w0'] = -1.2
cosmo_match_a['wa'] = 0.5
cosmo_match_a['w'] = -1.2
cosmo_match_b = cosmo_match_a.copy()
cosmo_match_b['w0'] = -0.6
cosmo_match_b['wa'] = -1.5
cosmo_match_b['w'] = -0.6
C_match_a = cp.CosmoPie(cosmology=cosmo_match_a, p_space='jdem')
C_match_b = cp.CosmoPie(cosmology=cosmo_match_b, p_space='jdem')
weff_2 = np.loadtxt('test_inputs/wmatch/weff_2.dat')
ws_a_pred = weff_2[:, 1]
zs_a_pred = weff_2[:, 0]
weff_1 = np.loadtxt('test_inputs/wmatch/weff_1.dat')
ws_b_pred = weff_1[:, 1]
zs_b_pred = weff_1[:, 0]
z_max_a = np.max(zs_a_pred)
z_max_b = np.max(zs_b_pred)
z_min_a = np.min(zs_a_pred)
z_min_b = np.min(zs_b_pred)
zs_a = np.arange(z_min_a, z_max_a, 0.05)
zs_b = np.arange(z_min_b, z_max_b, 0.05)
ws_a = wm.match_w(C_match_a, zs_a)
ws_b = wm.match_w(C_match_b, zs_b)
ws_a_interp = InterpolatedUnivariateSpline(zs_a_pred,
ws_a_pred,
k=1,
ext=2)(zs_a)
ws_b_interp = InterpolatedUnivariateSpline(zs_b_pred,
ws_b_pred,
k=1,
ext=2)(zs_b)
ws_a = wm.match_w(C_match_a, zs_a)
ws_b = wm.match_w(C_match_b, zs_b)
mse_w_a = np.linalg.norm(
(ws_a - ws_a_interp) / ws_a_interp) / ws_a_interp.size
mse_w_b = np.linalg.norm(
(ws_b - ws_b_interp) / ws_b_interp) / ws_b_interp.size
print(mse_w_a, mse_w_b)
assert mse_w_a < 7.e-4
assert mse_w_b < 7.e-3
sigma_a_in = np.loadtxt('test_inputs/wmatch/sigma_2.dat')
sigma_b_in = np.loadtxt('test_inputs/wmatch/sigma_1.dat')
zs_a_pred_2 = sigma_a_in[:, 0]
zs_b_pred_2 = sigma_a_in[:, 0]
z_max_a_2 = np.max(zs_a_pred_2)
z_max_b_2 = np.max(zs_b_pred_2)
z_min_a_2 = np.min(zs_a_pred_2)
z_min_b_2 = np.min(zs_b_pred_2)
zs_a_2 = np.arange(z_min_a_2, z_max_a_2, 0.05)
zs_b_2 = np.arange(z_min_b_2, z_max_b_2, 0.05)
pow_mults_a = wm.match_growth(C_match_a, zs_a_2, ws_a)
pow_mults_b = wm.match_growth(C_match_b, zs_b_2, ws_b)
sigma_a_interp = InterpolatedUnivariateSpline(sigma_a_in[:, 0],
sigma_a_in[:, 1],
k=3,
ext=2)(zs_a_2)
sigma_b_interp = InterpolatedUnivariateSpline(sigma_b_in[:, 0],
sigma_b_in[:, 1],
k=3,
ext=2)(zs_b_2)
sigma_a = np.sqrt(pow_mults_a) * 0.83
sigma_b = np.sqrt(pow_mults_b) * 0.83
mse_sigma_a = np.linalg.norm(
(sigma_a - sigma_a_interp) / sigma_a_interp) / sigma_a_interp.size
mse_sigma_b = np.linalg.norm(
(sigma_b - sigma_b_interp) / sigma_b_interp) / sigma_b_interp.size
print(mse_sigma_a, mse_sigma_b)
assert mse_sigma_a < 5.e-4
assert mse_sigma_b < 5.e-4
print(mse_sigma_a, mse_sigma_b)
assert mse_sigma_a < 5.e-4
assert mse_sigma_b < 5.e-4
if __name__ == '__main__':
do_test_battery = False
do_other_tests = True
if do_test_battery:
pytest.cmdline.main(['w_matcher_tests.py'])
if do_other_tests:
cosmo_start = defaults.cosmology.copy()
cosmo_start['w'] = -1
cosmo_start['de_model'] = 'constant_w'
C_start = cp.CosmoPie(cosmology=cosmo_start, p_space='jdem')
params = {
'w_step': 0.01,
'w_min': -3.50,
'w_max': 0.1,
'a_step': 0.001,
'a_min': 0.000916674,
'a_max': 1.00
}
do_convergence_test_w0wa = False
do_convergence_test_jdem = False
do_match_casarini = True
do_plots = True
fails = 0
def test_hmf():
"""run various hmf tests as a block"""
cosmo_fid = defaults.cosmology.copy()
cosmo_fid['h'] = 0.65
cosmo_fid['Omegamh2'] = 0.148
cosmo_fid['Omegabh2'] = 0.02
cosmo_fid['OmegaLh2'] = 0.65 * 0.65**2
cosmo_fid['sigma8'] = 0.92
cosmo_fid['ns'] = 1.
cosmo_fid = cp.add_derived_pars(cosmo_fid, p_space='basic')
power_params = defaults.power_params.copy()
power_params.camb['force_sigma8'] = True
power_params.camb['npoints'] = 1000
power_params.camb['maxkh'] = 20000.
power_params.camb['kmax'] = 100. #0.899999976158
power_params.camb['accuracy'] = 2.
C = cp.CosmoPie(cosmo_fid, 'basic')
P = mps.MatterPower(C, power_params)
C.set_power(P)
params = defaults.hmf_params.copy()
params['z_min'] = 0.0
params['z_max'] = 5.0
params['log10_min_mass'] = 6
params['log10_max_mass'] = 18.63
params['n_grid'] = 1264
params['n_z'] = 5. / 0.5
hmf = ST_hmf(C, params=params)
Ms = hmf.mass_grid
do_sanity_checks = True
if do_sanity_checks:
print("sanity")
#some sanity checks
zs = np.arange(0.001, 5., 0.1)
Gs = C.G_norm(zs)
#arbitrary input M(z) cutoff
m_z_in = np.exp(np.linspace(np.log(np.min(Ms)), np.log(1.e15),
zs.size))
m_z_in[0] = Ms[0]
#check normalized to unity (all dark matter is in some halo)
# f_norm_residual = trapz(hmf.f_sigma(Ms,Gs).T,np.log(hmf.sigma[:-1:]**-1),axis=1)
#assert np.allclose(np.zeros(Gs.size)+1.,norm_residual)
_, _, dndM = hmf.mass_func(Ms, Gs)
n_avgs_alt = np.zeros(zs.size)
bias_n_avgs_alt = np.zeros(zs.size)
dndM_G_alt = np.zeros((Ms.size, zs.size))
for i in range(0, zs.size):
n_avgs_alt[i] = hmf.n_avg(m_z_in[i], zs[i])
bias_n_avgs_alt[i] = hmf.bias_n_avg(m_z_in[i], zs[i])
dndM_G_alt[:, i] = hmf.dndM_G(Ms, Gs[i])
dndM_G = hmf.dndM_G(Ms, Gs)
#consistency checks for vector method
assert np.allclose(dndM_G, dndM_G_alt)
n_avgs = hmf.n_avg(m_z_in, zs)
bias_n_avgs = hmf.bias_n_avg(m_z_in, zs)
assert np.allclose(n_avgs, n_avgs_alt)
assert np.all(n_avgs >= 0.)
assert np.allclose(bias_n_avgs, bias_n_avgs_alt)
#check integrating dn/dM over all M actually gives n
assert np.allclose(trapz(dndM.T, Ms, axis=1),
hmf.n_avg(np.zeros(zs.size) + Ms[0], zs))
test_xs = np.outer(hmf.nu_of_M(Ms), 1. / Gs**2)
test_integrand = hmf.f_sigma(Ms, Gs) * hmf.bias_G(
Ms, Gs, hmf.bias_norm(Gs))
#not sure why, but this is true (if ignore h)
#test_term = np.trapz(test_integrand,test_xs,axis=0)*hmf.f_norm(Gs)
#assert np.allclose(1.,test_term,rtol=1e-3)
b_norm_residual = np.trapz(test_integrand, test_xs, axis=0)
assert np.allclose(np.zeros(zs.size) + 1., b_norm_residual)
#b_norm_residual_alt = np.trapz(hmf.f_sigma(Ms,Gs)*hmf.bias_G(Ms,Gs),test_xs,axis=0)
b_norm_residual_alt2 = np.trapz(hmf.f_sigma(Ms, Gs) *
hmf.bias_G(Ms, Gs, 1.),
test_xs,
axis=0)
#check including norm_in behaves appropriately does not matter
#assert np.allclose(b_norm_residual_alt,b_norm_residual_alt2)
assert np.allclose(b_norm_residual,
b_norm_residual_alt2 / hmf.bias_norm(Gs))
#hcekc all the matter in a halo if include normalization factor
assert np.allclose(
np.trapz(hmf.f_sigma(Ms, 1., 1.), np.log(1. / hmf.sigma[:-1:])),
hmf.f_norm(1.))
#sanity check M_star
assert np.round(np.log10(hmf.M_star())) == 13.
assert np.isclose(C.sigma_r(0., 8. / C.h),
cosmo_fid['sigma8'],
rtol=1.e-3)
assert np.isclose(C.sigma_r(1., 8. / C.h),
C.G_norm(1.) * cosmo_fid['sigma8'],
rtol=1.e-3)
#M_restrict = 10**np.linspace(np.log10(4.*10**13),16,100)
#n_restrict = hmf.n_avg(M_restrict,0.)
nu = hmf.nu_of_M(Ms)
bias_nu = hmf.bias_nu(nu)
bias_G = hmf.bias_G(Ms, 1.)
bias_z = hmf.bias(Ms, 0.)
assert np.allclose(bias_nu, bias_G)
assert np.allclose(bias_nu, bias_z)
assert np.allclose(bias_G, bias_z)
assert np.all(bias_nu >= 0)
# dndm = hmf.dndM_G(Ms,1.)
# bias_avg = np.trapz(bias_nu*dndm,Ms)
n_avg2 = hmf.n_avg(Ms, 0.)
assert np.all(n_avg2 >= 0.)
# bias_n_avg1 = bias_nu*n_avg2
#bias_n_avg2 = hmf.bias_n_avg(Ms)
# integ_pred = np.trapz(hmf.f_sigma(Ms,1.,1.),np.log(1./hmf.sigma[:-1:]))
# integ_res = np.trapz(Ms*hmf.dndM_G(Ms,1.),Ms)/C.rho_bar(0.)
#assert np.isclose(integ_res,integ_pred,rtol=1.e-2)
#xs n#np.linspace(np.log(np.sqrt(nu[0])),np.log(nu[-1]),10000)
#xs = np.exp(np.linspace(np.log(np.sqrt(nu[0]),np.log(1.e36),10000))
#F = -cumtrapz(1./np.sqrt(2.*np.pi)*np.exp(-xs[::-1]**2/2.),xs[::-1])[::-1]
#cons_res = np.trapz(hmf.dndM_G(Ms,1.)*Ms*hmf.bias(Ms,1.),Ms)/C.rho_bar(0.)
assert np.isclose(np.trapz(bias_nu * hmf.f_nu(nu), np.sqrt(nu)),
1.,
rtol=1.e-1)
#assert np.isclose(np.trapz(hmf.f_nu(nu)/np.sqrt(nu),np.sqrt(nu)),1.,rtol=2.e-1)
#bias_avg = np.trapz(hmf.dndM_G(Ms,1.)*hmf.bias_G(Ms,1.),Ms)/np.trapz(hmf.dndM_G(Ms,1.),Ms)
#check for various edge cases of n_avg and bias_n_avg
z2s = np.array([0., 1.])
m2s = np.array([1.e8, 1.e9])
n1 = hmf.n_avg(m2s[0], z2s[0])
n2 = hmf.n_avg(m2s[0], z2s)
n3 = hmf.n_avg(m2s, z2s[0])
n4 = hmf.n_avg(m2s, z2s)
n5 = hmf.n_avg(m2s[1], z2s[1])
n6 = hmf.n_avg(m2s[1], z2s[0])
n7 = hmf.n_avg(m2s[0], z2s[1])
assert np.isclose(n1, n2[0])
assert np.isclose(n1, n3[0])
assert np.isclose(n1, n4[0])
assert np.isclose(n5, n4[1])
assert np.isclose(n2[1], n7)
assert np.isclose(n3[1], n6)
bn1 = hmf.bias_n_avg(m2s[0], z2s[0])
bn2 = hmf.bias_n_avg(m2s[0], z2s)
bn3 = hmf.bias_n_avg(m2s, z2s[0])
bn4 = hmf.bias_n_avg(m2s, z2s)
bn5 = hmf.bias_n_avg(m2s[1], z2s[1])
bn6 = hmf.bias_n_avg(m2s[1], z2s[0])
bn7 = hmf.bias_n_avg(m2s[0], z2s[1])
assert np.isclose(bn1, bn2[0])
assert np.isclose(bn1, bn3[0])
assert np.isclose(bn1, bn4[0])
assert np.isclose(bn5, bn4[1])
assert np.isclose(bn2[1], bn7)
assert np.isclose(bn3[1], bn6)
n_avgs_0 = hmf.n_avg(hmf.mass_grid, 0.)
n_avgs_1 = np.zeros(hmf.mass_grid.size)
for itr in range(0, hmf.mass_grid.size):
n_avgs_1[itr] = hmf.n_avg(hmf.mass_grid[itr], 0.)
assert np.allclose(n_avgs_0, n_avgs_1)
bn_avgs_0 = hmf.bias_n_avg(hmf.mass_grid, 0.)
bn_avgs_1 = np.zeros(hmf.mass_grid.size)
for itr in range(0, hmf.mass_grid.size):
bn_avgs_1[itr] = hmf.bias_n_avg(hmf.mass_grid[itr], 0.)
assert np.allclose(bn_avgs_0, bn_avgs_1)
print("PASS: sanity passed")
do_plot_test2 = True
if do_plot_test2:
#Ms = 10**(np.linspace(11,14,500))
# dndM_G=hmf.dndM_G(Ms,Gs)
do_jenkins_comp = True
#should look like dotted line in figure 3 of arXiv:astro-ph/0005260
if do_jenkins_comp:
print("jenkins_comp")
zs = np.array([0.])
Gs = C.G_norm(zs)
dndM_G = hmf.f_sigma(Ms, Gs)
input_dndm = np.loadtxt('test_inputs/hmf/dig_jenkins_fig3.csv',
delimiter=',')
res_j = np.exp(input_dndm[:, 1])
res_i = InterpolatedUnivariateSpline(1. / hmf.sigma[:-1:],
dndM_G,
k=3,
ext=2)(np.exp(input_dndm[:,
0]))
assert np.all(np.abs((res_j / res_i - 1.)[0:19]) < 0.03)
print("PASS: jenkins_comp")
do_sheth_bias_comp1 = True
#agrees pretty well, maybe as well as it should
#compare to rightmost arXiv:astro-ph/9901122 figure 3
if do_sheth_bias_comp1:
print("sheth_bias_comp1")
cosmo_fid2 = cosmo_fid.copy()
cosmo_fid2['Omegamh2'] = 0.3 * 0.7**2
cosmo_fid2['Omegabh2'] = 0.05 * 0.7**2
cosmo_fid2['OmegaLh2'] = 0.7 * 0.7**2
cosmo_fid2['sigma8'] = 0.9
cosmo_fid2['h'] = 0.7
cosmo_fid2['ns'] = 1.0
cosmo_fid2 = cp.add_derived_pars(cosmo_fid2, p_space='basic')
C2 = cp.CosmoPie(cosmo_fid2, 'basic')
P2 = mps.MatterPower(C2, power_params)
C2.set_power(P2)
params2 = params.copy()
hmf2 = ST_hmf(C2, params=params2)
zs = np.array([0., 1., 2., 4.])
Gs = C2.G_norm(zs)
input_bias = np.loadtxt('test_inputs/hmf/dig_sheth_fig3.csv',
delimiter=',')
bias = hmf2.bias_G(10**input_bias[:, 0], Gs)
error = np.abs(1. - 10**input_bias[:, 1:5] / bias**2)
error_max = np.array([0.06, 0.4, 0.2, 0.4])
assert np.all(np.max(error, axis=0) < error_max)
print("PASS: sheth_bias_comp1")
do_sheth_bias_comp2 = True
#agrees well
#compare to bottom arXiv:astro-ph/9901122 figure 4
if do_sheth_bias_comp2:
print("sheth_bias_comp2")
cosmo_fid2 = cosmo_fid.copy()
cosmo_fid2['Omegamh2'] = 0.3 * 0.7**2
cosmo_fid2['Omegabh2'] = 0.05 * 0.7**2
cosmo_fid2['OmegaLh2'] = 0.7 * 0.7**2
cosmo_fid2['sigma8'] = 0.9
cosmo_fid2['h'] = 0.7
cosmo_fid2['ns'] = 1.0
cosmo_fid2 = cp.add_derived_pars(cosmo_fid2, p_space='basic')
C2 = cp.CosmoPie(cosmo_fid2, 'basic')
P2 = mps.MatterPower(C2, power_params)
C2.set_power(P2)
C2.k = P2.k
params2 = params.copy()
hmf2 = ST_hmf(C2, params=params2)
input_bias = np.loadtxt('test_inputs/hmf/dig_sheth2.csv',
delimiter=',')
bias = hmf2.bias_nu(10**input_bias[:, 0])
observable = 1. + (bias - 1.) * hmf2.delta_c
error = np.abs(1. - 10**input_bias[:, 1] / observable)
error_max = 0.07
assert np.all(np.max(error) < error_max)
print("PASS: sheth_bias_comp2")
#should agree, does
#match fig 2 arXiv:astro-ph/0203169
do_hu_bias_comp2 = True
if do_hu_bias_comp2:
print("hu_bias_comp2")
zs = np.array([0.])
Gs = C.G_norm(zs)
bias = hmf.bias_G(Ms, Gs, 1.)[:, 0] #why 1
#maybe should have k pivot 0.01
input_bias = np.loadtxt('test_inputs/hmf/dig_hu_bias2.csv',
delimiter=',')
# masses = 10**np.linspace(np.log10(10**11),np.log10(10**16),100)
bias_hu_i = 10**input_bias[:,
1] #InterpolatedUnivariateSpline(10**input_bias[:,0],10**input_bias[:,1])(masses)
bias_i = hmf.bias_G(10**input_bias[:, 0], Gs, 1.)[:, 0]
assert np.max(np.abs(bias_hu_i / bias_i - 1.)) < 0.06
print("PASS: hu_bias_comp2 passed")
#should agree, does
#match fig 1 arXiv:astro-ph/0203169
do_hu_sigma_comp = True
if do_hu_sigma_comp:
print("hu_sigma_comp")
assert np.isclose(hmf.M_star(), 1.2 * 10**13, rtol=1.e-1)
input_sigma = np.loadtxt('test_inputs/hmf/dig_hu_sigma.csv',
delimiter=',')
res_sigma = InterpolatedUnivariateSpline(hmf.R,
hmf.sigma,
k=3,
ext=2)(10**input_sigma[:,
0])
assert np.all(
np.abs((res_sigma / 10**input_sigma[:, 1])[4::] - 1.) < 0.02)
print("PASS: hu_sigma_comp")
def test_super_survey(de_model):
"""run some eigenvalue tests of SuperSurvey pipeline"""
t1 = time()
z_max = 1.35
l_max = 50
camb_params = defaults.camb_params.copy()
camb_params['force_sigma8'] = False
camb_params['kmax'] = 5.
camb_params['npoints'] = 1000
cosmo_fid = defaults.cosmology_jdem.copy()
cosmo_fid['w'] = -1.
cosmo_fid['w0'] = cosmo_fid['w']
cosmo_fid['wa'] = 0.
cosmo_fid['de_model'] = de_model
if cosmo_fid['de_model'] == 'jdem':
for i in range(0, 36):
cosmo_fid['ws36_' + str(i).zfill(2)] = cosmo_fid['w']
C = cp.CosmoPie(cosmology=cosmo_fid, p_space='jdem')
power_params = defaults.power_params.copy()
power_params.camb = camb_params
P = mps.MatterPower(C, power_params)
C.set_power(P)
r_max = C.D_comov(z_max)
print('this is r max and l_max', r_max, l_max)
phi1s = np.array([
-19., -19., -11., -11., 7., 25., 25., 43., 43., 50., 50., 50., 24., 5.,
5., 7., 7., -19.
]) * np.pi / 180.
theta1s = np.array([
-50., -35., -35., -19., -19., -19., -15.8, -15.8, -40., -40., -55.,
-78., -78., -78., -55., -55., -50., -50.
]) * np.pi / 180. + np.pi / 2.
phi_in1 = 7. / 180. * np.pi
theta_in1 = -35. * np.pi / 180. + np.pi / 2.
theta0 = np.pi / 4.
theta1 = 3. * np.pi / 4.
phi0 = 0.
phi1 = 3.074096023740458
phi2 = np.pi / 3.
phi3 = phi2 + (phi1 - phi0)
theta2s = np.array([theta0, theta1, theta1, theta0, theta0])
phi2s = np.array([phi0, phi0, phi1, phi1, phi0]) - phi1 / 2.
theta_in2 = np.pi / 2.
phi_in2 = 0.
res_choose = 7
Theta1 = [theta0, theta1]
Phi1 = [phi0, phi1]
Theta2 = [theta0, theta1]
Phi2 = [phi2, phi3]
zs = np.array([0.2, 0.43, .63, 0.9, 1.3])
z_fine = np.linspace(0.001, np.max(zs), 2000) #use linspace
use_poly = True
use_poly2 = True
if use_poly:
if use_poly2:
geo1 = PolygonGeo(zs, theta1s, phi1s, theta_in1, phi_in1, C,
z_fine, l_max, defaults.polygon_params.copy())
geo2 = PolygonGeo(zs, theta2s, phi2s, theta_in2, phi_in2, C,
z_fine, l_max, defaults.polygon_params.copy())
else:
geo1 = PolygonPixelGeo(zs, theta1s, phi1s, theta_in1, phi_in1, C,
z_fine, l_max, res_choose)
geo2 = PolygonPixelGeo(zs, theta2s, phi2s, theta_in2, phi_in2, C,
z_fine, l_max, res_choose)
else:
geo1 = RectGeo(zs, Theta1, Phi1, C, z_fine)
geo2 = RectGeo(zs, Theta2, Phi2, C, z_fine)
len_params = defaults.lensing_params.copy()
len_params['pmodel'] = 'halofit'
lenless_defaults = defaults.sw_survey_params.copy()
lenless_defaults['needs_lensing'] = False
if cosmo_fid['de_model'] == 'w0wa':
cosmo_par_list = np.array(
['ns', 'Omegamh2', 'Omegabh2', 'OmegaLh2', 'LogAs', 'w0', 'wa'])
cosmo_par_eps = np.array(
[0.002, 0.0005, 0.0001, 0.0005, 0.1, 0.01, 0.07])
elif cosmo_fid['de_model'] == 'constant_w':
cosmo_par_list = np.array(
['ns', 'Omegamh2', 'Omegabh2', 'OmegaLh2', 'LogAs', 'w'])
cosmo_par_eps = np.array([0.002, 0.0005, 0.0001, 0.0005, 0.1, 0.01])
elif cosmo_fid['de_model'] == 'jdem':
cosmo_par_list = ['ns', 'Omegamh2', 'Omegabh2', 'OmegaLh2', 'LogAs']
cosmo_par_list.extend(cp.JDEM_LIST)
cosmo_par_list = np.array(cosmo_par_list, dtype=object)
cosmo_par_eps = np.full(41, 0.5)
cosmo_par_eps[0:5] = np.array([0.002, 0.0005, 0.0001, 0.0005, 0.1])
else:
raise ValueError('not prepared to handle ' +
str(cosmo_fid['de_model']))
#note that currently (poorly implemented derivative) in jdem,
#OmegaLh2 and LogAs are both almost completely unconstrained but nondegenerate,
#while in basic, h and sigma8 are not constrained but are almost completely degenerate
nz_params = defaults.nz_params_wfirst_lens.copy()
from nz_wfirst import NZWFirst
nz_matcher = NZWFirst(nz_params)
len_params['smodel'] = 'nzmatcher'
sw_params = defaults.sw_survey_params.copy()
obs_list = defaults.sw_observable_list.copy()
survey_1 = SWSurvey(geo1, 's1', C, sw_params, cosmo_par_list,
cosmo_par_eps, obs_list, len_params, nz_matcher)
surveys_sw = np.array([survey_1])
geos = np.array([geo1, geo2])
k_cut = 0.005
basis = SphBasisK(r_max,
C,
k_cut,
defaults.basis_params.copy(),
l_ceil=100)
lw_param_list = defaults.lw_param_list.copy()
lw_observable_list = defaults.lw_observable_list.copy()
survey_3 = LWSurvey(geos,
'lw_survey1',
basis,
C,
defaults.lw_survey_params.copy(),
observable_list=lw_observable_list,
param_list=lw_param_list)
surveys_lw = np.array([survey_3])
print('main: this is r_max: ' + str(r_max))
SS = SuperSurvey(surveys_sw,
surveys_lw,
basis,
C,
defaults.prior_fisher_params.copy(),
get_a=False,
do_unmitigated=True,
do_mitigated=True,
include_sw=True)
t2 = time()
print("main: total run time " + str(t2 - t1) + " s")
mit_eigs_sw = SS.eig_set[0, 1]
no_mit_eigs_sw = SS.eig_set[0, 0]
mit_eigs_par = SS.eig_set[1, 1]
no_mit_eigs_par = SS.eig_set[1, 0]
#TODO check eigenvalue interlace for this projection
SS.print_standard_analysis()
# print("main: unmitigated sw lambda1,2: "+str(no_mit_eigs_sw[0][-1])+","+str(no_mit_eigs_sw[0][-2]))
# print("main: mitigated sw lambda1,2: "+str(mit_eigs_sw[0][-1])+","+str(mit_eigs_sw[0][-2]))
# print("main: n sw mit lambda>1.00000001: "+str(np.sum(np.abs(mit_eigs_sw[0])>1.00000001)))
# print("main: n sw no mit lambda>1.00000001: "+str(np.sum(np.abs(no_mit_eigs_sw[0])>1.00000001)))
# print("main: unmitigated par lambda1,2: "+str(no_mit_eigs_par[0][-1])+","+str(no_mit_eigs_par[0][-2]))
# print("main: mitigated par lambda1,2: "+str(mit_eigs_par[0][-1])+","+str(mit_eigs_par[0][-2]))
# print("main: n par mit lambda>1.00000001: "+str(np.sum(np.abs(mit_eigs_par[0])>1.00000001)))
# print("main: n par no mit lambda>1.00000001: "+str(np.sum(np.abs(no_mit_eigs_par[0])>1.00000001)))
v_no_mit_par = np.dot(SS.f_set_nopriors[0][2].get_cov_cholesky(),
no_mit_eigs_par[1])
v_mit_par = np.dot(SS.f_set_nopriors[0][2].get_cov_cholesky(),
mit_eigs_par[1])
v_no_mit_sw = np.dot(SS.f_set_nopriors[0][1].get_cov_cholesky(),
no_mit_eigs_sw[1])
v_mit_sw = np.dot(SS.f_set_nopriors[0][1].get_cov_cholesky(),
mit_eigs_sw[1])
test_v = True
v_test_fails = 0
if test_v:
m_mat_no_mit_par = np.identity(mit_eigs_par[0].size) + np.dot(
SS.f_set_nopriors[1][2].get_covar(),
SS.f_set_nopriors[0][2].get_fisher())
m_mat_mit_par = np.identity(mit_eigs_par[0].size) + np.dot(
SS.f_set_nopriors[2][2].get_covar(),
SS.f_set_nopriors[0][2].get_fisher())
if not np.allclose(
np.dot(m_mat_no_mit_par, v_no_mit_par) /
(1. + no_mit_eigs_par[0]), v_no_mit_par):
v_test_fails += 1
warn('some no mit eig vectors may be bad')
if not np.allclose(
np.dot(m_mat_mit_par, v_mit_par) /
(1. + mit_eigs_par[0]), v_mit_par):
v_test_fails += 1
warn('some mit eig vectors may be bad')
if v_test_fails == 0:
print("PASS: eigenvector decomposition checks passed")
else:
raise RuntimeError('FAIL: ' + str(v_test_fails) +
' eigenvector decomposition checks failed')
get_hold_mats = False
if get_hold_mats:
no_prior_hold = SS.f_set[0][2].get_fisher()
if C.de_model == 'jdem':
no_prior_project = prior_fisher.project_w0wa(
no_prior_hold, defaults.prior_fisher_params.copy(),
prior_fisher.JDEM_LABELS)
print('main: r diffs', np.diff(geo1.rs))
print('main: theta width',
(geo1.rs[1] + geo1.rs[0]) / 2. * (Theta1[1] - Theta1[0]))
print('main: phi width',
(geo1.rs[1] + geo1.rs[0]) / 2. * (Phi1[1] - Phi1[0]) * np.sin(
(Theta1[1] + Theta1[0]) / 2))
test_perturbation = True
pert_test_fails = 0
if test_perturbation:
#TOLERANCE below which an eigenvalue less than TOLERANCE*max eigenvalue is considered 0
REL_TOLERANCE = 10**-8
f0 = SS.multi_f.get_fisher(mf.f_spec_no_mit,
mf.f_return_lw)[0].get_fisher()
f1 = SS.multi_f.get_fisher(mf.f_spec_mit,
mf.f_return_lw)[0].get_fisher()
if not np.all(f0.T == f0):
pert_test_fails += 1
warn("unperturbed fisher matrix not symmetric, unacceptable")
if not np.all(f1.T == f1):
pert_test_fails += 1
warn("perturbed fisher matrix not symmetric, unacceptable")
#get eigenvalues and set numerically zero values to 0
eigf0 = np.linalg.eigh(f0)[0]
eigf0[np.abs(eigf0) < REL_TOLERANCE * np.max(np.abs(eigf0))] = 0.
eigf1 = np.linalg.eigh(f1)[0]
eigf1[np.abs(eigf1) < REL_TOLERANCE * np.max(np.abs(eigf1))] = 0.
#check positive semidefinite
if np.any(eigf0 < 0.):
pert_test_fails += 1
warn(
"unperturbed fisher matrix not positive definite within tolerance, unacceptable"
)
if np.any(eigf1 < 0.):
pert_test_fails += 1
warn(
"perturbed fisher matrix not positive definite within tolerance, unacceptable"
)
#check nondecresasing
diff_eig = eigf1 - eigf0
diff_eig[np.abs(diff_eig) < REL_TOLERANCE *
np.max(np.abs(diff_eig))] = 0
if np.any(diff_eig < 0):
pert_test_fails += 1
warn("some eigenvalues decreased within tolerance, unacceptable")
#check interlace theorem satisfied (eigenvalues cannot be reordered by more than rank of perturbation)
n_offset = SS.surveys_lw[0].get_total_rank()
rolled_eig = (eigf1[::-1][n_offset:eigf0.size] -
eigf0[::-1][0:eigf0.size - n_offset])
rolled_eig[np.abs(rolled_eig) < REL_TOLERANCE *
np.max(np.abs(rolled_eig))] = 0.
if np.any(rolled_eig > 0):
pert_test_fails += 1
warn("some eigenvalues fail interlace theorem, unacceptable")
c0 = SS.multi_f.get_fisher(mf.f_spec_no_mit,
mf.f_return_lw)[0].get_covar()
c1 = SS.multi_f.get_fisher(mf.f_spec_mit,
mf.f_return_lw)[0].get_covar()
if not np.all(c0 == c0.T):
pert_test_fails += 1
warn("unperturbed covariance not symmetric, unacceptable")
if not np.all(c1 == c1.T):
warn("perturbed covariance not symmetric, unacceptable")
eigc0 = np.linalg.eigh(c0)[0]
eigc1 = np.linalg.eigh(c1)[0]
if np.any(eigc0 < 0):
pert_test_fails += 1
warn(
"unperturbed covariance not positive semidefinite, unacceptable"
)
if np.any(eigc1 < 0):
pert_test_fails += 1
warn(
"perturbed covariance not positive semidefinite, unacceptable")
fdiff_eigc = (eigc1 - eigc0) / eigc0
fdiff_eigc[np.abs(fdiff_eigc) < REL_TOLERANCE] = 0.
if np.any(fdiff_eigc > 0):
pert_test_fails += 1
warn("some covariance eigenvalues increase, unacceptable")
if pert_test_fails == 0:
print("PASS: All fisher matrix sanity checks passed")
else:
raise RuntimeError("FAIL: " + str(pert_test_fails) +
" fisher matrix sanity checks failed")
test_eigs = True
eig_test_fails = 0
if test_eigs:
REL_TOLERANCE = 10**-8
c_ssc0 = SS.multi_f.get_fisher(
mf.f_spec_SSC_no_mit,
mf.f_return_sw)[1].get_covar() #SS.covs_sw[0].get_ssc_covar()
if not np.allclose(c_ssc0, c_ssc0.T):
eig_test_fails += 1
warn("unperturbed result covariance not symmetric, unacceptable")
c_ssc1 = SS.multi_f.get_fisher(
mf.f_spec_SSC_mit,
mf.f_return_sw)[1].get_covar() #SS.covs_sw[0].get_ssc_covar()
if not np.allclose(c_ssc1, c_ssc1.T):
eig_test_fails += 1
warn("perturbed result covariance not symmetric, unacceptable")
eigsys_ssc0 = np.linalg.eigh(c_ssc0)
eigsys_ssc1 = np.linalg.eigh(c_ssc1)
eig_ssc0 = eigsys_ssc0[0].copy()
eig_ssc1 = eigsys_ssc1[0].copy()
eig_ssc0[np.abs(eig_ssc0) < np.max(np.abs(eig_ssc0)) *
REL_TOLERANCE] = 0
eig_ssc1[np.abs(eig_ssc0) < np.max(np.abs(eig_ssc0)) *
REL_TOLERANCE] = 0
if np.any(eig_ssc0 < 0):
eig_test_fails += 1
warn(
"unperturbed result cov not positive semidefinite, unacceptable"
)
if np.any(eig_ssc1 < 0):
eig_test_fails += 1
warn(
"perturbed result cov not positive semidefinite, unacceptable")
cg = SS.f_set_nopriors[0][1].get_covar()
eigsys_cg = np.linalg.eigh(cg)
eig_mitprod = np.real(
np.linalg.eig(np.dot(np.linalg.inv(c_ssc0 + cg), c_ssc1 + cg))[0])
eig_mitprod[np.abs(eig_mitprod - 1.) < REL_TOLERANCE] = 1.
if np.any(eig_mitprod > 1):
eig_test_fails += 1
warn("mitigation making covariance worse, unacceptable")
n_offset = SS.surveys_lw[0].get_total_rank()
if np.sum(eig_mitprod < 1.) > n_offset:
eig_test_fails += 1
warn("mitigation changing too many eigenvalues, unacceptable")
eig_diff = eig_ssc1 - eig_ssc0
eig_diff[np.abs(eig_diff) < np.max(np.abs(eig_diff)) *
REL_TOLERANCE] = 0.
if np.any(eig_diff > 0):
eig_test_fails += 1
warn("mitigation making covariance worse, unacceptable")
if eig_test_fails == 0:
print("PASS: All sw eigenvalue sanity checks passed")
else:
raise RuntimeError("FAIL: " + str(pert_test_fails) +
" eigenvalue sanity checks failed")
do_eig_interlace_check = True
if do_eig_interlace_check:
eig_interlace_fails_mit = 0
eig_interlace_fails_no_mit = 0
n_sw = mit_eigs_sw[0].size
n_par = mit_eigs_par[0].size
d_n = n_sw - n_par
eig_l_mit_par = mit_eigs_par[0][::-1]
eig_l_no_mit_par = no_mit_eigs_par[0][::-1]
eig_l_mit_sw = mit_eigs_sw[0][::-1]
eig_l_no_mit_sw = no_mit_eigs_sw[0][::-1]
for i in range(0, n_par):
if eig_l_mit_par[i] > eig_l_mit_sw[i]:
eig_interlace_fails_mit += 1
if eig_l_no_mit_par[i] > eig_l_no_mit_sw[i]:
eig_interlace_fails_no_mit += 1
if eig_l_mit_par[i] < eig_l_mit_sw[i + d_n]:
eig_interlace_fails_mit += 1
if eig_l_no_mit_par[i] < eig_l_no_mit_sw[i + d_n]:
eig_interlace_fails_no_mit += 1
if eig_interlace_fails_mit == 0 and eig_interlace_fails_no_mit == 0:
print("PASS: All parameter eigenvalue interlace tests passed")
else:
raise RuntimeError(
"FAIL: " + str(eig_interlace_fails_mit) +
" mitigation and " + str(eig_interlace_fails_no_mit) +
" no mitigation failures in parameter eigenvalue interlace tests"
)
def test_agreement_with_sigma8():
"""test sigma8 works basic to jdem"""
cosmo_base = defaults.cosmology_wmap.copy()
cosmo_base = cp.add_derived_pars(cosmo_base, 'jdem')
cosmo_base['de_model'] = 'constant_w'
cosmo_base['w'] = -1.
cosmo_base['sigma8'] = 0.7925070693605805
power_params = defaults.power_params.copy()
power_params.camb['maxkh'] = 3.
power_params.camb['kmax'] = 10.
power_params.camb['npoints'] = 1000
power_params.camb['accuracy'] = 2
power_params.camb['leave_h'] = False
power_params_jdem = deepcopy(power_params)
power_params_jdem.camb['force_sigma8'] = False
power_params_basi = deepcopy(power_params)
power_params_basi.camb['force_sigma8'] = True
cosmo_jdem = cosmo_base.copy()
cosmo_jdem['p_space'] = 'jdem'
C_fid_jdem = cp.CosmoPie(cosmo_jdem, 'jdem')
P_jdem = mps.MatterPower(C_fid_jdem, power_params_jdem)
C_fid_jdem.set_power(P_jdem)
cosmo_basi = cosmo_base.copy()
cosmo_basi['p_space'] = 'basic'
C_fid_basi = cp.CosmoPie(cosmo_basi, 'basic')
P_basi = mps.MatterPower(C_fid_basi, power_params_basi)
C_fid_basi.set_power(P_basi)
zs = np.arange(0.2, 1.41, 0.40)
z_fine = np.linspace(0.001, 1.4, 1000)
geo_jdem = FullSkyGeo(zs, C_fid_jdem, z_fine)
geo_basi = FullSkyGeo(zs, C_fid_basi, z_fine)
jdem_pars = np.array(
['ns', 'Omegamh2', 'Omegabh2', 'OmegaLh2', 'LogAs', 'w'])
jdem_eps = np.array([0.002, 0.00025, 0.0001, 0.00025, 0.01, 0.01])
basi_pars = np.array(['ns', 'Omegamh2', 'Omegabh2', 'h', 'sigma8', 'w'])
basi_eps = np.array([0.002, 0.00025, 0.0001, 0.00025, 0.001, 0.01])
sw_params = defaults.sw_survey_params.copy()
len_params = defaults.lensing_params.copy()
sw_observable_list = defaults.sw_observable_list.copy()
nz_wfirst_lens = NZWFirstEff(defaults.nz_params_wfirst_lens.copy())
prior_params = defaults.prior_fisher_params.copy()
basis_params = defaults.basis_params.copy()
sw_survey_jdem = sws.SWSurvey(geo_jdem, 'wfirst', C_fid_jdem, sw_params,
jdem_pars, jdem_eps, sw_observable_list,
len_params, nz_wfirst_lens)
sw_survey_basi = sws.SWSurvey(geo_basi, 'wfirst', C_fid_basi, sw_params,
basi_pars, basi_eps, sw_observable_list,
len_params, nz_wfirst_lens)
#need to fix As because the code cannot presently do this
for itr in range(0, basi_pars.size):
for i in range(0, 2):
cosmo_alt_basi = sw_survey_basi.len_pow.Cs_pert[
itr, i].cosmology.copy()
n_As = 10
logAs = np.linspace(cosmo_alt_basi['LogAs'] * 0.9,
cosmo_alt_basi['LogAs'] * 1.1, n_As)
As = np.exp(logAs)
sigma8s = np.zeros(n_As)
for itr2 in xrange(0, n_As):
cosmo_alt_basi['As'] = As[itr2]
cosmo_alt_basi['LogAs'] = logAs[itr2]
sigma8s[itr2] = camb_sigma8(cosmo_alt_basi,
power_params_basi.camb)
logAs_interp = InterpolatedUnivariateSpline(sigma8s[::-1],
logAs[::-1],
ext=2,
k=3)
sw_survey_basi.len_pow.Cs_pert[
itr, i].cosmology['LogAs'] = logAs_interp(
sw_survey_basi.len_pow.Cs_pert[itr, i].cosmology['sigma8'])
sw_survey_basi.len_pow.Cs_pert[itr, i].cosmology['As'] = np.exp(
sw_survey_basi.len_pow.Cs_pert[itr, i].cosmology['LogAs'])
dO_dpar_jdem = sw_survey_jdem.get_dO_I_dpar_array()
dO_dpar_basi = sw_survey_basi.get_dO_I_dpar_array()
response_pars = np.array([
'ns', 'Omegach2', 'Omegabh2', 'Omegamh2', 'OmegaLh2', 'h', 'LogAs',
'w', 'sigma8'
])
l_max = 24
r_max_jdem = geo_jdem.r_fine[-1]
k_cut_jdem = 30. / r_max_jdem
basis_jdem = SphBasisK(r_max_jdem,
C_fid_jdem,
k_cut_jdem,
basis_params,
l_ceil=l_max,
needs_m=True)
SS_jdem = SuperSurvey(np.array([sw_survey_jdem]),
np.array([]),
basis_jdem,
C_fid_jdem,
prior_params,
get_a=False,
do_unmitigated=True,
do_mitigated=False)
r_max_basi = geo_basi.r_fine[-1]
k_cut_basi = 30. / r_max_basi
basis_basi = SphBasisK(r_max_basi,
C_fid_basi,
k_cut_basi,
basis_params,
l_ceil=l_max,
needs_m=True)
SS_basi = SuperSurvey(np.array([sw_survey_basi]),
np.array([]),
basis_basi,
C_fid_basi,
prior_params,
get_a=False,
do_unmitigated=True,
do_mitigated=False)
#dO_dpar_jdem_to_basi = np.zeros_like(dO_dpar_jdem)
#dO_dpar_basi_to_jdem = np.zeros_like(dO_dpar_basi)
project_basi_to_jdem = np.zeros((jdem_pars.size, basi_pars.size))
response_derivs_jdem = np.zeros((response_pars.size, jdem_pars.size))
response_derivs_basi = np.zeros((response_pars.size, basi_pars.size))
for i in range(0, response_pars.size):
for j in range(0, jdem_pars.size):
response_derivs_jdem[i, j] = (
sw_survey_jdem.len_pow.Cs_pert[j,
0].cosmology[response_pars[i]] -
sw_survey_jdem.len_pow.Cs_pert[j, 1].cosmology[
response_pars[i]]) / (jdem_eps[j] * 2.)
response_derivs_basi[i, j] = (
sw_survey_basi.len_pow.Cs_pert[j,
0].cosmology[response_pars[i]] -
sw_survey_basi.len_pow.Cs_pert[j, 1].cosmology[
response_pars[i]]) / (basi_eps[j] * 2.)
project_jdem_to_basi = np.zeros((basi_pars.size, jdem_pars.size))
project_basi_to_jdem = np.zeros((jdem_pars.size, basi_pars.size))
for itr1 in range(0, basi_pars.size):
for itr2 in range(0, response_pars.size):
if response_pars[itr2] in jdem_pars:
name = response_pars[itr2]
i = np.argwhere(jdem_pars == name)[0, 0]
project_jdem_to_basi[itr1, i] = response_derivs_basi[itr2,
itr1]
for itr1 in range(0, jdem_pars.size):
for itr2 in range(0, response_pars.size):
if response_pars[itr2] in basi_pars:
name = response_pars[itr2]
i = np.argwhere(basi_pars == name)[0, 0]
project_basi_to_jdem[itr1, i] = response_derivs_jdem[itr2,
itr1]
assert np.allclose(np.dot(dO_dpar_jdem, project_jdem_to_basi.T),
dO_dpar_basi,
rtol=1.e-3,
atol=np.max(dO_dpar_basi) * 1.e-4)
assert np.allclose(np.dot(dO_dpar_basi, project_basi_to_jdem.T),
dO_dpar_jdem,
rtol=1.e-3,
atol=np.max(dO_dpar_jdem) * 1.e-4)
#basi p_space cannot currently do priors by itself
f_p_priors_basi = np.dot(
project_jdem_to_basi,
np.dot(SS_jdem.multi_f.fisher_priors.get_fisher(),
project_jdem_to_basi.T))
for i in range(0, 1):
f_np_jdem = SS_jdem.f_set_nopriors[i][2].get_fisher().copy()
f_np_basi = SS_basi.f_set_nopriors[i][2].get_fisher().copy()
f_np_jdem_to_basi = np.dot(project_jdem_to_basi,
np.dot(f_np_jdem, project_jdem_to_basi.T))
f_np_basi_to_jdem = np.dot(project_basi_to_jdem,
np.dot(f_np_basi, project_basi_to_jdem.T))
assert np.allclose(f_np_jdem_to_basi, f_np_basi, rtol=1.e-2)
assert np.allclose(f_np_basi_to_jdem, f_np_jdem, rtol=1.e-2)
f_p_jdem = SS_jdem.f_set[i][2].get_fisher().copy()
f_p_basi = SS_basi.f_set_nopriors[i][2].get_fisher().copy(
) + f_p_priors_basi.copy()
f_p_jdem_to_basi = np.dot(project_jdem_to_basi,
np.dot(f_p_jdem, project_jdem_to_basi.T))
f_p_basi_to_jdem = np.dot(project_basi_to_jdem,
np.dot(f_p_basi, project_basi_to_jdem.T))
assert np.allclose(f_p_jdem_to_basi, f_p_basi, rtol=1.e-2)
assert np.allclose(f_p_basi_to_jdem, f_p_jdem, rtol=1.e-2)
print(f_np_jdem / f_np_basi_to_jdem)
print(f_np_basi / f_np_jdem_to_basi)
def __init__(self):
""" do power derivative comparison"""
power_params = defaults.power_params.copy()
power_params.camb['force_sigma8'] = True
power_params.camb['leave_h'] = False
power_params.camb['npoints'] = 1000
C = cp.CosmoPie(cosmology=COSMOLOGY_CHIANG, p_space='basic')
epsilon = 0.01
P_a = mps.MatterPower(C, power_params)
k_a = P_a.k
C.k = k_a
k_a_h = P_a.k / C.cosmology['h']
d_chiang_halo = np.loadtxt('test_inputs/dp_1/dp_chiang_halofit.dat')
k_chiang_halo = d_chiang_halo[:, 0] * C.cosmology['h']
dc_chiang_halo = d_chiang_halo[:, 1]
dc_ch1 = interp1d(k_chiang_halo, dc_chiang_halo,
bounds_error=False)(k_a)
d_chiang_lin = np.loadtxt('test_inputs/dp_1/dp_chiang_linear.dat')
k_chiang_lin = d_chiang_lin[:, 0] * C.cosmology['h']
dc_chiang_lin = d_chiang_lin[:, 1]
dc_ch2 = interp1d(k_chiang_lin, dc_chiang_lin, bounds_error=False)(k_a)
d_chiang_fpt = np.loadtxt('test_inputs/dp_1/dp_chiang_oneloop.dat')
k_chiang_fpt = d_chiang_fpt[:, 0] * C.cosmology['h']
dc_chiang_fpt = d_chiang_fpt[:, 1]
dc_ch3 = interp1d(k_chiang_fpt, dc_chiang_fpt, bounds_error=False)(k_a)
do_plots = True
if do_plots:
import matplotlib.pyplot as plt
zbar = np.array([3.])
dcalt1, p1a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='linear',
epsilon=epsilon)
dcalt2, p2a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='halofit',
epsilon=epsilon)
dcalt3, p3a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='fastpt',
epsilon=epsilon)
if do_plots:
ax = plt.subplot(221)
plt.xlim([0., 0.4])
plt.ylim([1.2, 3.2])
plt.grid()
plt.title('z=3.0')
ax.plot(k_a_h, abs(dcalt1 / p1a))
ax.plot(k_a_h, abs(dcalt2 / p2a))
ax.plot(k_a_h, abs(dcalt3 / p3a))
zbar = np.array([2.])
dcalt1, p1a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='linear',
epsilon=epsilon)
dcalt2, p2a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='halofit',
epsilon=epsilon)
dcalt3, p3a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='fastpt',
epsilon=epsilon)
if do_plots:
ax = plt.subplot(222)
plt.xlim([0., 0.4])
plt.ylim([1.2, 3.2])
plt.grid()
plt.title('z=2.0')
ax.plot(k_a_h, abs(dcalt1 / p1a))
ax.plot(k_a_h, abs(dcalt2 / p2a))
ax.plot(k_a_h, abs(dcalt3 / p3a))
zbar = np.array([1.])
dcalt1, p1a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='linear',
epsilon=epsilon)
dcalt2, p2a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='halofit',
epsilon=epsilon)
dcalt3, p3a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='fastpt',
epsilon=epsilon)
if do_plots:
ax = plt.subplot(223)
plt.xlim([0., 0.4])
plt.ylim([1.2, 3.2])
plt.grid()
plt.title('z=1.0')
ax.set_xlabel('k h Mpc^-1')
ax.set_ylabel('dln(P)/ddeltabar')
ax.plot(k_a_h, abs(dcalt1 / p1a))
ax.plot(k_a_h, abs(dcalt2 / p2a))
ax.plot(k_a_h, abs(dcalt3 / p3a))
ax.plot(k_a_h, dc_ch1)
ax.plot(k_a_h, dc_ch2)
ax.plot(k_a_h, dc_ch3)
plt.legend([
'linear', 'halofit', 'fastpt', 'halo_chiang', "lin_chiang",
"fpt_chiang"
],
loc=4)
mask_mult = (k_a_h > 0.) * (k_a_h < 0.4)
rat_halofit = (dc_ch1 / abs(dcalt2 / p2a)[:, 0])[mask_mult]
rat_linear = (dc_ch2 / abs(dcalt1 / p1a)[:, 0])[mask_mult]
rat_fpt = (dc_ch3 / abs(dcalt3 / p3a)[:, 0])[mask_mult]
zbar = np.array([0.])
dcalt1, p1a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='linear',
epsilon=epsilon)
dcalt2, p2a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='halofit',
epsilon=epsilon)
dcalt3, p3a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='fastpt',
epsilon=epsilon)
if do_plots:
ax = plt.subplot(224)
plt.xlim([0., 0.4])
plt.ylim([1.2, 3.2])
plt.grid()
plt.title('z=0.0')
ax.plot(k_a_h, abs(dcalt1 / p1a))
ax.plot(k_a_h, abs(dcalt2 / p2a))
ax.plot(k_a_h, abs(dcalt3 / p3a))
#plt.legend(['linear','halofit','fastpt'],loc=4)
if do_plots:
plt.show()
k_a_halofit = k_a_h[mask_mult][~np.isnan(rat_halofit)]
k_a_linear = k_a_h[mask_mult][~np.isnan(rat_linear)]
k_a_fpt = k_a_h[mask_mult][~np.isnan(rat_fpt)]
dkh = 0.05
halofit_bins = np.zeros(7)
linear_bins = np.zeros(7)
fpt_bins = np.zeros(7)
for itr in range(1, 8):
mask_loc_hf = (k_a_halofit < dkh *
(itr + 1.)) * (k_a_halofit >= dkh * itr)
mask_loc_lin = (k_a_linear < dkh *
(itr + 1.)) * (k_a_linear >= dkh * itr)
mask_loc_fpt = (k_a_fpt < dkh *
(itr + 1.)) * (k_a_fpt >= dkh * itr)
halofit_bins[itr - 1] = np.average(
rat_halofit[~np.isnan(rat_halofit)][mask_loc_hf])
linear_bins[itr - 1] = np.average(
rat_linear[~np.isnan(rat_linear)][mask_loc_lin])
fpt_bins[itr - 1] = np.average(
rat_fpt[~np.isnan(rat_fpt)][mask_loc_fpt])
#print(np.abs(halofit_bins-1.))
#print(np.abs(linear_bins-1.))
#print(np.abs(fpt_bins-1.))
fails = 0
if np.all(np.abs(halofit_bins - 1.) < 0.02):
print("PASS: smoothed z=1 halofit matches chiang")
else:
fails += 1
print("FAIL: smoothed z=1 halofit does not match chiang")
if np.all(np.abs(linear_bins - 1.) < 0.02):
print("PASS: smoothed z=1 linear matches chiang")
else:
fails += 1
print("FAIL: smoothed z=1 linear does not match chiang")
if np.all(np.abs(fpt_bins - 1.) < 0.02):
print("PASS: smoothed z=1 fastpt matches chiang")
else:
fails += 1
print("FAIL: smoothed z=1 fastpt does not match chiang")
if fails == 0:
print("PASS: all tests satisfactory")
else:
print("FAIL: " + str(fails) + " tests unsatisfactory")
#for some reason the discrepancy is a function of pivot_scalar and is minimizaed around pivot_scalar=0.01-0.0001
rtol = 3.e-3
eps = 0.01
cosmo_fid = defaults.cosmology.copy()
camb_params = defaults.camb_params.copy()
camb_params['force_sigma8'] = param[0]
camb_params['leave_h'] = param[1]
camb_params['npoints'] = 3000
camb_params['kmax'] = 2.
camb_params['maxkh'] = 2.
power_params = defaults.power_params.copy()
power_params.camb = camb_params
#camb_params['minkh'] = 1e-3
C_fid = cp.CosmoPie(cosmo_fid, p_space='jdem')
P_fid = mps.MatterPower(C_fid, power_params)
k_fid = P_fid.k
C_fid.set_power(P_fid)
P_lin1 = P_fid.get_matter_power(np.array([0.]), pmodel='linear')[:,
0]
P_res1 = P_fid.get_matter_power(np.array([0.]), pmodel=param[2])[:,
0]
if param[2] == 'halofit':
nonlinear_model = camb.model.NonLinear_both
else:
nonlinear_model = camb.model.NonLinear_none
k_res2, P_res2 = camb_pow(C_fid.cosmology,
zbar=np.array([0.]),
def test_cosmosis_match():
"""test agreement with modified cosmosis demo 15 results
assuming gaussian matter distribution with sigma=0.4 and average z=1
use halofit power spectrum grid"""
TOLERANCE_MAX = 0.2
TOLERANCE_MEAN = 0.2
power_params = defaults.power_params.copy()
power_params.camb['force_sigma8'] = True
power_params.camb['maxkh'] = 25000
power_params.camb['kmax'] = 100.
power_params.camb['npoints'] = 3200
C = cp.CosmoPie(cosmology=COSMOLOGY_COSMOSIS2.copy(), p_space='jdem')
P_in = mps.MatterPower(C, power_params)
#k_in = P_in.k
C.set_power(P_in)
zs = np.loadtxt('test_inputs/proj_2/z.txt')
zs[0] = 10**-3
ls = np.loadtxt('test_inputs/proj_2/ell.txt')
f_sky = np.pi / (3. * np.sqrt(2.))
params = defaults.lensing_params.copy()
params['zbar'] = 1.0
params['sigma'] = 0.40
params['smodel'] = 'gaussian'
params['l_min'] = np.min(ls)
params['l_max'] = np.max(ls)
params['n_l'] = ls.size
params['n_gal'] = 118000000 * 6.
params['pmodel'] = 'halofit'
sh_pow1 = np.loadtxt('test_inputs/proj_2/ss_pow.txt')
sh_pow1_gg = np.loadtxt('test_inputs/proj_2/gg_pow.txt')
sh_pow1_sg = np.loadtxt('test_inputs/proj_2/sg_pow.txt')
sh_pow1_mm = np.loadtxt('test_inputs/proj_2/mm_pow.txt') / C.h
sp2 = sp.ShearPower(C, zs, f_sky, params, mode='power')
q_sh = lw.QShear(sp2)
q_num = lw.QNum(sp2)
q_mag = lw.QMag(sp2)
sh_pow2 = sp.Cll_q_q(sp2, q_sh, q_sh).Cll()
sh_pow2_gg = sp.Cll_q_q(sp2, q_num, q_num).Cll()
sh_pow2_sg = sp.Cll_q_q(sp2, q_sh, q_num).Cll()
sh_pow2_mm = sp.Cll_q_q(sp2, q_mag, q_mag).Cll()
#get ratio of calculated value to expected value from cosmosis
#use -np.inf as filler for interpolation when l value is not in ls*C.h,filter it later
ss_rat = (sh_pow2 - sh_pow1) / sh_pow2
gg_rat = (sh_pow2_gg - sh_pow1_gg) / sh_pow2_gg
sg_rat = (sh_pow2_sg - sh_pow1_sg) / sh_pow2_sg
mm_rat = (sh_pow2_mm - sh_pow1_mm) / sh_pow2_mm
print(sh_pow2)
mean_ss_err = np.mean(abs(ss_rat)[abs(ss_rat) < np.inf])
mean_gg_err = np.mean(abs(gg_rat)[abs(gg_rat) < np.inf])
mean_sg_err = np.mean(abs(sg_rat)[abs(sg_rat) < np.inf])
mean_mm_err = np.mean(abs(mm_rat)[abs(mm_rat) < np.inf])
max_ss_err = max((abs(ss_rat))[abs(ss_rat) < np.inf])
max_gg_err = max((abs(gg_rat))[abs(gg_rat) < np.inf])
max_sg_err = max((abs(sg_rat))[abs(sg_rat) < np.inf])
max_mm_err = max((abs(mm_rat))[abs(mm_rat) < np.inf])
print("ss agreement within: " + str(max_ss_err * 100.) + "%" +
" mean agreement: " + str(mean_ss_err * 100.) + "%")
print("gg agreement within: " + str(max_gg_err * 100.) + "%" +
" mean agreement: " + str(mean_gg_err * 100.) + "%")
print("sg agreement within: " + str(max_sg_err * 100.) + "%" +
" mean agreement: " + str(mean_sg_err * 100.) + "%")
print("mm agreement within: " + str(max_mm_err * 100.) + "%" +
" mean agreement: " + str(mean_mm_err * 100.) + "%")
assert max_ss_err < TOLERANCE_MAX
assert max_gg_err < TOLERANCE_MAX
assert max_sg_err < TOLERANCE_MAX
assert max_mm_err < TOLERANCE_MAX
assert mean_ss_err < TOLERANCE_MEAN
assert mean_gg_err < TOLERANCE_MEAN
assert mean_sg_err < TOLERANCE_MEAN
assert mean_mm_err < TOLERANCE_MEAN
def get_perturbed_cosmopies(C_fid,
pars,
epsilons,
log_par_derivs=None,
override_safe=False):
"""get set of 2 perturbed cosmopies, above and below (including camb linear power spectrum) for getting partial derivatives
using central finite difference method
inputs:
C_fid: the fiducial CosmoPie
pars: an array of the names of parameters to change
epsilons: an array of step sizes correspondings to pars
log_par_derivs: if True for a given element of pars will do log derivative in the parameter
override_safe: if True do not borrow the growth factor or power spectrum from C_fid even if we could
"""
cosmo_fid = C_fid.cosmology.copy()
P_fid = C_fid.P_lin
k_fid = C_fid.k
power_params = P_fid.power_params.copy()
#default assumption is ordinary derivative, can do log deriv in parameter also
#if log_par_derivs[i]==True, will do log deriv
if log_par_derivs is not None and log_par_derivs.size != pars.size:
raise ValueError('invalid input log_par_derivs ' + str(log_par_derivs))
elif log_par_derivs is None:
log_par_derivs = np.zeros(pars.size, dtype=bool)
Cs_pert = np.zeros((pars.size, 2), dtype=object)
for i in range(0, pars.size):
cosmo_a = get_perturbed_cosmology(cosmo_fid, pars[i], epsilons[i],
log_par_derivs[i])
cosmo_b = get_perturbed_cosmology(cosmo_fid, pars[i], -epsilons[i],
log_par_derivs[i])
#set cosmopie power spectrum appropriately
#avoid unnecessarily recomputing growth factors if they won't change. If growth factors don't change neither will w matching
if pars[i] in cp.GROW_SAFE and not override_safe:
C_a = cp.CosmoPie(cosmo_a,
p_space=cosmo_fid['p_space'],
G_safe=True,
G_in=C_fid.G_p)
C_b = cp.CosmoPie(cosmo_b,
p_space=cosmo_fid['p_space'],
G_safe=True,
G_in=C_fid.G_p)
P_a = mps.MatterPower(C_a,
power_params,
k_in=k_fid,
wm_in=P_fid.wm,
de_perturbative=True)
P_b = mps.MatterPower(C_b,
power_params,
k_in=k_fid,
wm_in=P_fid.wm,
de_perturbative=True)
else:
C_a = cp.CosmoPie(cosmo_a, p_space=cosmo_fid['p_space'])
C_b = cp.CosmoPie(cosmo_b, p_space=cosmo_fid['p_space'])
#avoid unnecessarily recomputing WMatchers for dark energy related parameters, and unnecessarily calling camb
if pars[i] in cp.DE_SAFE and not override_safe:
P_a = mps.MatterPower(C_a,
power_params,
k_in=k_fid,
wm_in=P_fid.wm,
P_fid=P_fid,
camb_safe=True)
P_b = mps.MatterPower(C_b,
power_params,
k_in=k_fid,
wm_in=P_fid.wm,
P_fid=P_fid,
camb_safe=True)
else:
P_a = mps.MatterPower(C_a,
power_params,
k_in=k_fid,
de_perturbative=True)
P_b = mps.MatterPower(C_b,
power_params,
k_in=k_fid,
de_perturbative=True)
#k_a = P_a.k
#k_b = P_b.k
C_a.set_power(P_a)
C_b.set_power(P_b)
Cs_pert[i, 0] = C_a
Cs_pert[i, 1] = C_b
return Cs_pert
def test_pipeline_consistency():
"""test full pipeline consistency with rotation jdem vs lihu"""
cosmo_base = defaults.cosmology_wmap.copy()
cosmo_base = cp.add_derived_pars(cosmo_base, 'jdem')
cosmo_base['de_model'] = 'constant_w'
cosmo_base['w'] = -1.
power_params = defaults.power_params.copy()
power_params.camb['maxkh'] = 1.
power_params.camb['kmax'] = 1.
power_params.camb['npoints'] = 1000
power_params.camb['accuracy'] = 2
power_params.camb['leave_h'] = False
cosmo_jdem = cosmo_base.copy()
cosmo_jdem['p_space'] = 'jdem'
C_fid_jdem = cp.CosmoPie(cosmo_jdem, 'jdem')
P_jdem = mps.MatterPower(C_fid_jdem, power_params.copy())
C_fid_jdem.set_power(P_jdem)
cosmo_lihu = cosmo_base.copy()
cosmo_lihu['p_space'] = 'lihu'
C_fid_lihu = cp.CosmoPie(cosmo_lihu, 'lihu')
P_lihu = mps.MatterPower(C_fid_lihu, power_params.copy())
C_fid_lihu.set_power(P_lihu)
zs = np.arange(0.2, 1.41, 0.40)
z_fine = np.linspace(0.001, 1.4, 1000)
geo_jdem = FullSkyGeo(zs, C_fid_jdem, z_fine)
geo_lihu = FullSkyGeo(zs, C_fid_lihu, z_fine)
jdem_pars = np.array(
['ns', 'Omegamh2', 'Omegabh2', 'OmegaLh2', 'LogAs', 'w'])
jdem_eps = np.array([0.002, 0.00025, 0.0001, 0.00025, 0.1, 0.01])
lihu_pars = np.array(['ns', 'Omegach2', 'Omegabh2', 'h', 'LogAs', 'w'])
lihu_eps = np.array([0.002, 0.00025, 0.0001, 0.00025, 0.1, 0.01])
sw_params = defaults.sw_survey_params.copy()
len_params = defaults.lensing_params.copy()
sw_observable_list = defaults.sw_observable_list.copy()
nz_wfirst_lens = NZWFirstEff(defaults.nz_params_wfirst_lens.copy())
prior_params = defaults.prior_fisher_params.copy()
basis_params = defaults.basis_params.copy()
sw_survey_jdem = sws.SWSurvey(geo_jdem, 'wfirst', C_fid_jdem, sw_params,
jdem_pars, jdem_eps, sw_observable_list,
len_params, nz_wfirst_lens)
sw_survey_lihu = sws.SWSurvey(geo_lihu, 'wfirst', C_fid_lihu, sw_params,
lihu_pars, lihu_eps, sw_observable_list,
len_params, nz_wfirst_lens)
#dO_dpar_jdem = sw_survey_jdem.get_dO_I_dpar_array()
#dO_dpar_lihu = sw_survey_lihu.get_dO_I_dpar_array()
response_pars = np.array([
'ns', 'Omegach2', 'Omegabh2', 'Omegamh2', 'OmegaLh2', 'h', 'LogAs', 'w'
])
response_derivs_jdem_pred = np.array(
[[1., 0., 0., 0., 0., 0., 0., 0.],
[0., 1., 0., 1., 0., 1. / (2. * C_fid_jdem.cosmology['h']), 0., 0.],
[0., -1., 1., 0., 0., 0., 0., 0.],
[0., 0., 0., 0., 1., 1. / (2. * C_fid_jdem.cosmology['h']), 0., 0.],
[0., 0., 0., 0., 0., 0., 1., 0.], [0., 0., 0., 0., 0., 0., 0., 1.]]).T
response_derivs_lihu_pred = np.array(
[[1., 0., 0., 0., 0., 0., 0., 0.], [0., 1., 0., 1., -1., 0., 0., 0.],
[0., 0., 1., 1., -1., 0., 0., 0.],
[0., 0., 0., 0., 2. * C_fid_lihu.cosmology['h'], 1., 0., 0.],
[0., 0., 0., 0., 0., 0., 1., 0.], [0., 0., 0., 0., 0., 0., 0., 1.]]).T
l_max = 24
r_max_jdem = geo_jdem.r_fine[-1]
k_cut_jdem = 30. / r_max_jdem
basis_jdem = SphBasisK(r_max_jdem,
C_fid_jdem,
k_cut_jdem,
basis_params,
l_ceil=l_max,
needs_m=True)
SS_jdem = SuperSurvey(np.array([sw_survey_jdem]),
np.array([]),
basis_jdem,
C_fid_jdem,
prior_params,
get_a=False,
do_unmitigated=True,
do_mitigated=False)
r_max_lihu = geo_lihu.r_fine[-1]
k_cut_lihu = 30. / r_max_lihu
basis_lihu = SphBasisK(r_max_lihu,
C_fid_lihu,
k_cut_lihu,
basis_params,
l_ceil=l_max,
needs_m=True)
SS_lihu = SuperSurvey(np.array([sw_survey_lihu]),
np.array([]),
basis_lihu,
C_fid_lihu,
prior_params,
get_a=False,
do_unmitigated=True,
do_mitigated=False)
#dO_dpar_jdem_to_lihu = np.zeros_like(dO_dpar_jdem)
#dO_dpar_lihu_to_jdem = np.zeros_like(dO_dpar_lihu)
project_lihu_to_jdem = np.zeros((jdem_pars.size, lihu_pars.size))
#f_g_jdem_to_lihu = np.zeros((lihu_pars.size,lihu_pars.size))
#f_g_lihu_to_jdem = np.zeros((jdem_pars.size,jdem_pars.size))
response_derivs_jdem = np.zeros((response_pars.size, jdem_pars.size))
response_derivs_lihu = np.zeros((response_pars.size, lihu_pars.size))
for i in range(0, response_pars.size):
for j in range(0, jdem_pars.size):
response_derivs_jdem[i, j] = (
sw_survey_jdem.len_pow.Cs_pert[j,
0].cosmology[response_pars[i]] -
sw_survey_jdem.len_pow.Cs_pert[j, 1].cosmology[
response_pars[i]]) / (jdem_eps[j] * 2.)
response_derivs_lihu[i, j] = (
sw_survey_lihu.len_pow.Cs_pert[j,
0].cosmology[response_pars[i]] -
sw_survey_lihu.len_pow.Cs_pert[j, 1].cosmology[
response_pars[i]]) / (lihu_eps[j] * 2.)
assert np.allclose(response_derivs_jdem, response_derivs_jdem_pred)
assert np.allclose(response_derivs_lihu, response_derivs_lihu_pred)
project_jdem_to_lihu = np.zeros((lihu_pars.size, jdem_pars.size))
project_lihu_to_jdem = np.zeros((jdem_pars.size, lihu_pars.size))
for itr1 in range(0, lihu_pars.size):
for itr2 in range(0, response_pars.size):
if response_pars[itr2] in jdem_pars:
name = response_pars[itr2]
i = np.argwhere(jdem_pars == name)[0, 0]
project_jdem_to_lihu[itr1, i] = response_derivs_lihu[itr2,
itr1]
for itr1 in range(0, jdem_pars.size):
for itr2 in range(0, response_pars.size):
if response_pars[itr2] in lihu_pars:
name = response_pars[itr2]
i = np.argwhere(lihu_pars == name)[0, 0]
project_lihu_to_jdem[itr1, i] = response_derivs_jdem[itr2,
itr1]
#assert np.allclose(np.dot(dO_dpar_jdem,project_jdem_to_lihu.T),dO_dpar_lihu,rtol=1.e-3,atol=np.max(dO_dpar_lihu)*1.e-4)
#assert np.allclose(np.dot(dO_dpar_lihu,project_lihu_to_jdem.T),dO_dpar_jdem,rtol=1.e-3,atol=np.max(dO_dpar_jdem)*1.e-4)
#lihu p_space cannot currently do priors by itself
f_p_priors_lihu = np.dot(
project_jdem_to_lihu,
np.dot(SS_jdem.multi_f.fisher_priors.get_fisher(),
project_jdem_to_lihu.T))
f_set_jdem_in = np.zeros(3, dtype=object)
f_set_lihu_in = np.zeros(3, dtype=object)
for i in range(0, 3):
f_set_jdem_in[i] = SS_jdem.f_set_nopriors[i][2].get_fisher().copy()
f_set_lihu_in[i] = SS_lihu.f_set_nopriors[i][2].get_fisher().copy()
f_np_lihu2 = rotate_jdem_to_lihu(f_set_jdem_in, C_fid_jdem)
f_np_jdem2 = rotate_lihu_to_jdem(f_set_lihu_in, C_fid_lihu)
f_np_lihu3 = rotate_jdem_to_lihu(f_np_jdem2, C_fid_jdem)
f_np_jdem3 = rotate_lihu_to_jdem(f_np_lihu2, C_fid_lihu)
for i in range(0, 3):
f_np_jdem = SS_jdem.f_set_nopriors[i][2].get_fisher().copy()
f_np_lihu = SS_lihu.f_set_nopriors[i][2].get_fisher().copy()
f_np_jdem_to_lihu = np.dot(project_jdem_to_lihu,
np.dot(f_np_jdem, project_jdem_to_lihu.T))
f_np_lihu_to_jdem = np.dot(project_lihu_to_jdem,
np.dot(f_np_lihu, project_lihu_to_jdem.T))
assert np.allclose(f_set_lihu_in[i], f_np_lihu3[i])
assert np.allclose(f_set_jdem_in[i], f_np_jdem3[i])
assert np.allclose(f_np_jdem_to_lihu, f_np_lihu2[i])
assert np.allclose(f_np_lihu_to_jdem, f_np_jdem2[i])
assert np.allclose(f_np_jdem_to_lihu, f_np_lihu, rtol=1.e-3)
assert np.allclose(f_np_lihu_to_jdem, f_np_jdem, rtol=1.e-3)
assert np.allclose(f_set_lihu_in[i], f_np_lihu2[i], rtol=1.e-3)
assert np.allclose(f_set_jdem_in[i], f_np_jdem2[i], rtol=1.e-3)
assert np.allclose(f_np_jdem3[i], f_np_jdem2[i], rtol=1.e-3)
assert np.allclose(f_np_lihu3[i], f_np_lihu2[i], rtol=1.e-3)
f_p_jdem = SS_jdem.f_set[i][2].get_fisher().copy()
f_p_lihu = SS_lihu.f_set_nopriors[i][2].get_fisher().copy(
) + f_p_priors_lihu.copy()
f_p_jdem_to_lihu = np.dot(project_jdem_to_lihu,
np.dot(f_p_jdem, project_jdem_to_lihu.T))
f_p_lihu_to_jdem = np.dot(project_lihu_to_jdem,
np.dot(f_p_lihu, project_lihu_to_jdem.T))
assert np.allclose(f_p_jdem_to_lihu, f_p_lihu, rtol=1.e-3)
assert np.allclose(f_p_lihu_to_jdem, f_p_jdem, rtol=1.e-3)
def test_power_derivative():
"""test that the power derivatives agree with chiang&wagner arxiv:1403.3411v2 figure 4-5"""
power_params = defaults.power_params.copy()
power_params.camb['force_sigma8'] = True
power_params.camb['leave_h'] = False
power_params.camb['npoints'] = 1000
C = cp.CosmoPie(cosmology=COSMOLOGY_CHIANG, p_space='basic')
#d = np.loadtxt('camb_m_pow_l.dat')
#k_in = d[:,0]
epsilon = 0.01
#k_a,P_a = cpow.camb_pow(cosmo_a)
P_a = mps.MatterPower(C, power_params)
k_a = P_a.k
C.k = k_a
k_a_h = P_a.k / C.cosmology['h']
pmodels = ['linear', 'halofit', 'fastpt']
for pmodel in pmodels:
z0 = 0.
hold0 = shp.dp_ddelta(P_a, z0, C, pmodel, epsilon)
z1 = np.array([0.])
hold1 = shp.dp_ddelta(P_a, z1, C, pmodel, epsilon)
z2 = np.array([0., 0.001])
hold2 = shp.dp_ddelta(P_a, z2, C, pmodel, epsilon)
z3 = np.arange(0., 1., 0.001)
hold3 = shp.dp_ddelta(P_a, z3, C, pmodel, epsilon)
assert np.allclose(hold0[0], hold1[0][:, 0])
assert np.allclose(hold1[0][:, 0], hold2[0][:, 0])
assert np.allclose(hold1[0][:, 0], hold3[0][:, 0])
assert np.allclose(hold2[0][:, 1], hold3[0][:, 1])
assert np.allclose(hold1[1][:, 0], hold1[1][:, 0])
assert np.allclose(hold1[1][:, 0], hold2[1][:, 0])
assert np.allclose(hold1[1][:, 0], hold3[1][:, 0])
assert np.allclose(hold2[1][:, 1], hold3[1][:, 1])
d_chiang_halo = np.loadtxt('test_inputs/dp_1/dp_chiang_halofit.dat')
k_chiang_halo = d_chiang_halo[:, 0] * C.cosmology['h']
dc_chiang_halo = d_chiang_halo[:, 1]
dc_ch1 = interp1d(k_chiang_halo, dc_chiang_halo, bounds_error=False)(k_a)
d_chiang_lin = np.loadtxt('test_inputs/dp_1/dp_chiang_linear.dat')
k_chiang_lin = d_chiang_lin[:, 0] * C.cosmology['h']
dc_chiang_lin = d_chiang_lin[:, 1]
dc_ch2 = interp1d(k_chiang_lin, dc_chiang_lin, bounds_error=False)(k_a)
d_chiang_fpt = np.loadtxt('test_inputs/dp_1/dp_chiang_oneloop.dat')
k_chiang_fpt = d_chiang_fpt[:, 0] * C.cosmology['h']
dc_chiang_fpt = d_chiang_fpt[:, 1]
dc_ch3 = interp1d(k_chiang_fpt, dc_chiang_fpt, bounds_error=False)(k_a)
zbar = np.array([1.])
dcalt1, p1a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='linear',
epsilon=epsilon)
dcalt2, p2a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='halofit',
epsilon=epsilon)
dcalt3, p3a = shp.dp_ddelta(P_a,
zbar,
C=C,
pmodel='fastpt',
epsilon=epsilon)
mask_mult = (k_a_h > 0.) * (k_a_h < 0.4)
rat_halofit = (dc_ch1 / abs(dcalt2 / p2a)[:, 0])[mask_mult]
rat_linear = (dc_ch2 / abs(dcalt1 / p1a)[:, 0])[mask_mult]
rat_fpt = (dc_ch3 / abs(dcalt3 / p3a)[:, 0])[mask_mult]
k_a_halofit = k_a_h[mask_mult][~np.isnan(rat_halofit)]
k_a_linear = k_a_h[mask_mult][~np.isnan(rat_linear)]
k_a_fpt = k_a_h[mask_mult][~np.isnan(rat_fpt)]
dkh = 0.05
halofit_bins = np.zeros(7)
linear_bins = np.zeros(7)
fpt_bins = np.zeros(7)
for itr in range(1, 8):
mask_loc_hf = (k_a_halofit < dkh *
(itr + 1.)) * (k_a_halofit >= dkh * itr)
mask_loc_lin = (k_a_linear < dkh *
(itr + 1.)) * (k_a_linear >= dkh * itr)
mask_loc_fpt = (k_a_fpt < dkh * (itr + 1.)) * (k_a_fpt >= dkh * itr)
halofit_bins[itr - 1] = np.average(
rat_halofit[~np.isnan(rat_halofit)][mask_loc_hf])
linear_bins[itr - 1] = np.average(
rat_linear[~np.isnan(rat_linear)][mask_loc_lin])
fpt_bins[itr - 1] = np.average(
rat_fpt[~np.isnan(rat_fpt)][mask_loc_fpt])
assert np.all(np.abs(halofit_bins - 1.) < 0.02)
assert np.all(np.abs(linear_bins - 1.) < 0.02)
assert np.all(np.abs(fpt_bins - 1.) < 0.02)
def test_power_agreement():
"""test agreement of powers extracted in two different cosmological parametrizations"""
cosmo_base = defaults.cosmology_wmap.copy()
cosmo_base = cp.add_derived_pars(cosmo_base, 'jdem')
cosmo_base['de_model'] = 'constant_w'
cosmo_base['w'] = -1.
power_params = defaults.power_params.copy()
power_params.camb['maxkh'] = 3.
power_params.camb['kmax'] = 10.
power_params.camb['npoints'] = 1000
power_params.camb['accuracy'] = 2
power_params.camb['leave_h'] = False
cosmo_jdem = cosmo_base.copy()
cosmo_jdem['p_space'] = 'jdem'
C_fid_jdem = cp.CosmoPie(cosmo_jdem, 'jdem')
P_jdem = mps.MatterPower(C_fid_jdem, power_params.copy())
C_fid_jdem.set_power(P_jdem)
cosmo_lihu = cosmo_base.copy()
cosmo_lihu['p_space'] = 'lihu'
C_fid_lihu = cp.CosmoPie(cosmo_lihu, 'lihu')
P_lihu = mps.MatterPower(C_fid_lihu, power_params.copy())
C_fid_lihu.set_power(P_lihu)
jdem_pars = np.array(['ns', 'Omegamh2', 'Omegabh2', 'OmegaLh2', 'LogAs'])
jdem_eps = np.array([0.002, 0.00025, 0.0001, 0.00025, 0.1])
C_pert_jdem = ppr.get_perturbed_cosmopies(C_fid_jdem, jdem_pars, jdem_eps)
lihu_pars = np.array(['ns', 'Omegach2', 'Omegabh2', 'h', 'LogAs'])
lihu_eps = np.array([0.002, 0.00025, 0.0001, 0.00025, 0.1])
C_pert_lihu = ppr.get_perturbed_cosmopies(C_fid_lihu, lihu_pars, lihu_eps)
response_pars = np.array(
['Omegach2', 'Omegabh2', 'Omegamh2', 'OmegaLh2', 'h'])
response_derivs_jdem = np.zeros((response_pars.size, 3))
response_derivs_jdem_pred = np.array(
[[1., 0., 1., 0., 1. / (2. * C_fid_jdem.cosmology['h'])],
[-1., 1., 0., 0., 0.],
[0., 0., 0., 1., 1. / (2. * C_fid_jdem.cosmology['h'])]]).T
response_derivs_lihu = np.zeros((response_pars.size, 3))
response_derivs_lihu_pred = np.array(
[[1., 0., 1., -1., 0.], [0., 1., 1., -1., 0.],
[0., 0., 0., 2. * C_fid_lihu.cosmology['h'], 1.]]).T
for i in range(0, response_pars.size):
for j in range(1, 4):
response_derivs_jdem[i, j - 1] = (
C_pert_jdem[j, 0].cosmology[response_pars[i]] -
C_pert_jdem[j, 1].cosmology[response_pars[i]]) / (jdem_eps[j] *
2.)
response_derivs_lihu[i, j - 1] = (
C_pert_lihu[j, 0].cosmology[response_pars[i]] -
C_pert_lihu[j, 1].cosmology[response_pars[i]]) / (lihu_eps[j] *
2.)
assert np.allclose(response_derivs_jdem_pred, response_derivs_jdem)
assert np.allclose(response_derivs_lihu_pred, response_derivs_lihu)
power_derivs_jdem = np.zeros((3, C_fid_jdem.k.size))
power_derivs_lihu = np.zeros((3, C_fid_lihu.k.size))
for pmodel in ['linear', 'fastpt', 'halofit']:
for j in range(1, 4):
power_derivs_jdem[
j - 1] = (C_pert_jdem[j, 0].P_lin.get_matter_power(
[0.], pmodel=pmodel)[:, 0] -
C_pert_jdem[j, 1].P_lin.get_matter_power(
[0.], pmodel=pmodel)[:, 0]) / (jdem_eps[j] * 2.)
power_derivs_lihu[
j - 1] = (C_pert_lihu[j, 0].P_lin.get_matter_power(
[0.], pmodel=pmodel)[:, 0] -
C_pert_lihu[j, 1].P_lin.get_matter_power(
[0.], pmodel=pmodel)[:, 0]) / (lihu_eps[j] * 2.)
assert np.allclose((power_derivs_jdem[1] + power_derivs_jdem[0] -
power_derivs_jdem[2]),
power_derivs_lihu[1],
rtol=1.e-2,
atol=1.e-4 * np.max(np.abs(power_derivs_lihu[1])))
assert np.allclose((power_derivs_jdem[0] - power_derivs_jdem[2]),
power_derivs_lihu[0],
rtol=1.e-2,
atol=1.e-4 * np.max(np.abs(power_derivs_lihu[0])))
assert np.allclose(power_derivs_jdem[2] * 2 *
C_fid_lihu.cosmology['h'],
power_derivs_lihu[2],
rtol=1.e-2,
atol=1.e-4 * np.max(np.abs(power_derivs_lihu[2])))
def get_matter_power(self,
zs_in,
pmodel='linear',
const_pow_mult=1.,
get_one_loop=False):
"""get a matter power spectrum P(z)
Inputs:
pmodel: nonlinear power spectrum model to use, options are 'linear','halofit', and 'fastpt'
const_pow_mult: multiplier to adjust sigma8 without creating a whole new power spectrum
get_one_loop: If True and pmodel=='fastpt', return the one loop contribution in addition to the nonlinear power spectrum
"""
if isinstance(zs_in, np.ndarray):
zs = zs_in
else:
zs = np.array([zs_in])
n_z = zs.size
G_norms = self.C.G_norm(zs)
if self.use_match_grid:
w_match_grid = self.w_match_interp(zs)
pow_mult_grid = self.growth_match_interp(zs) * const_pow_mult
Pbases = np.zeros((self.k.size, n_z))
if self.use_camb_grid:
for i in range(0, n_z):
Pbases[:, i] = pow_mult_grid[i] * self.camb_w_interp(
self.k, w_match_grid[i]).flatten()
else:
Pbases = np.outer(self.P_lin, pow_mult_grid)
else:
Pbases = np.outer(self.P_lin, np.full(n_z, 1.)) * const_pow_mult
P_nonlin = np.zeros((self.k.size, n_z))
if pmodel == 'linear':
P_nonlin = Pbases * G_norms**2
elif pmodel == 'halofit':
if self.use_match_grid:
for i in range(0, n_z):
cosmo_hf_i = self.cosmology.copy()
cosmo_hf_i['de_model'] = 'constant_w'
cosmo_hf_i['w'] = w_match_grid[i]
G_hf = InterpolatedUnivariateSpline(self.C.z_grid,
self.wm.growth_interp(
w_match_grid[i],
self.C.a_grid),
ext=2,
k=3)
hf_C_calc = cp.CosmoPie(cosmo_hf_i,
self.C.p_space,
silent=True,
G_safe=True,
G_in=G_hf)
hf_C_calc.k = self.k
hf_calc = halofit.HalofitPk(hf_C_calc, Pbases[:, i],
self.power_params.halofit,
self.camb_params['leave_h'])
P_nonlin[:, i] = 2. * np.pi**2 * (
hf_calc.D2_NL(self.k, zs[i]).T / self.k**3)
else:
hf_calc = halofit.HalofitPk(self.C,
self.P_lin * const_pow_mult,
self.power_params.halofit,
self.camb_params['leave_h'])
P_nonlin = 2. * np.pi**2 * (hf_calc.D2_NL(self.k, zs).T /
self.k**3).T
elif pmodel == 'fastpt':
if self.use_match_grid:
one_loops = np.zeros((self.k.size, n_z))
for i in range(0, n_z):
G_i = G_norms[i]
one_loops[:, i] = self.fpt.one_loop(
Pbases[:, i],
C_window=self.power_params.fpt['C_window']) * G_i**4
P_nonlin[:, i] = Pbases[:, i] * G_i**2 + one_loops[:, i]
else:
one_loops = np.outer(
self.fpt.one_loop(
self.P_lin,
C_window=self.power_params.fpt['C_window']),
G_norms**4)
P_nonlin = np.outer(self.P_lin, G_norms**2) + one_loops
if pmodel == 'fastpt' and get_one_loop:
return P_nonlin, one_loops
elif get_one_loop:
raise ValueError(
'could not get one loop power spectrum for pmodel ' +
str(pmodel))
else:
return P_nonlin
