def _post_initialisation(self):
self.t0 = 2458491.8771169
self.period = 1.2652328
self.k2 = 0.3**2
self.a = 10.
self.phase = fold(self.timea, self.period, self.t0)
self.em = UniformModel()
self.em.set_data(self.timea)
self._mec = self.em.evaluate(sqrt(
self.k2), self.t0 + 0.5 * self.period, self.period, self.a,
0.5 * pi) - 1
self._mec = 1 + self._mec / self._mec.ptp()
phi = 2 * pi * self.phase
self.alpha = a = abs(phi - pi)
self._rff = (sin(a) +
(pi - a) * cos(a)) / pi * self._mec # Reflected light
self._dbf = sin(phi) # Doppler boosting
self._evf = -cos(2 * phi) # Ellipsoidal variations
self._cwl = 1e-9 * tess.wl
self._ctm = tess.tm
self.set_prior('ms', 'NP', star_m.n, star_m.s)
self.set_prior('teffh', 'NP', 3300, 100)
self.set_prior('teffc', 'UP', 100, 3300)
self.set_prior('gp_log10_wn', 'NP', -1.74, 0.15)
def plot_folded_planets(self, bwidth: float = 10):
fig, axs = subplots(1, self.nplanets, figsize=(13, 6), sharey=True)
pv = self.de.minimum_location.copy()
for ipl in range(self.nplanets):
planets = set(arange(self.nplanets))
planets.remove(ipl)
mflux = self.transit_model(pv, planets=[ipl])
rflux = self.transit_model(pv, planets=planets)
oflux = self.ofluxa / rflux
phase = (fold(self.timea, pv[3 + 4 * ipl], pv[2 + 4 * ipl], 0.5) -
0.5) * pv[3 + 4 * ipl]
m = abs(phase) < 0.5 * self.bldur
sids = argsort(phase[m])
phase, mflux, oflux = phase[m][sids], mflux[m][sids], oflux[m][
sids]
bp, bf, be = downsample_time(phase, oflux, bwidth / 24 / 60)
axs[ipl].errorbar(bp, bf, be, fmt='ok')
axs[ipl].plot(phase, oflux, '.', alpha=0.25)
axs[ipl].plot(phase, mflux, 'k')
setp(axs,
xlim=(-0.5 * self.bldur, 0.5 * self.bldur),
ylim=(0.996, 1.004))
fig.tight_layout()
return fig
def read_eleanor(zero_epoch,
period,
bjdrefi,
mask_transits=False,
trwidth=0.053,
contamination=None):
dd = root / 'photometry'
files = sorted(dd.glob('hlsp_eleanor*.fits'))
times, fluxes, wnids, lcids = [], [], [], []
s = 0
for i, f in enumerate(files):
df = Table.read(f)
time = df['TIME'].data + bjdrefi
flux = df['CORR_FLUX'].data
m = isfinite(time) & isfinite(flux)
if mask_transits:
p = (fold(time, period, zero_epoch, 0.5) - 0.5) * period
m &= (abs(p) > 0.5 * trwidth)
flux /= nanmedian(flux)
m &= create_eleanor_sector_mask(flux, i)
if contamination is not None:
flux = decontaminate(flux, contamination[i])
if m.sum() > 0:
s += 1
times.append(time[m])
fluxes.append(flux[m])
lcids.append(full(time[m].size, i, 'int'))
wns = [diff(f).std() / sqrt(2) for f in fluxes]
pbs = s * ['TESS']
return times, fluxes, pbs, wns, pbs, list(arange(len(times)))
def plot_folded_tess_transit(self, method='de', pv=None, figsize=None, ylim=None):
assert method in ('de', 'mc')
if pv is None:
if method == 'de':
pv = self.de.minimum_location
else:
df = self.posterior_samples(derived_parameters=False)
pv = df.median.values
etess = self._ntess
t = self.timea[:etess]
fo = self.ofluxa[:etess]
fm = squeeze(self.transit_model(self.de.population))[self.de.minimum_index, :etess]
bl = squeeze(self.baseline(self.de.population))[self.de.minimum_index, :etess]
fig, ax = subplots(figsize=figsize)
phase = pv[1] * (fold(t, pv[1], pv[0], 0.5) - 0.5)
sids = argsort(phase)
phase = phase[sids]
bp, bf, be = downsample_time(phase, (fo / bl)[sids], 4 / 24 / 60)
ax.plot(phase, (fo / bl)[sids], 'k.', alpha=0.2)
ax.errorbar(bp, bf, be, fmt='ko')
ax.plot(phase, fm[sids], 'k')
setp(ax, ylim=ylim, xlabel='Time', ylabel='Normalised flux')
return fig
def __call__(self):
self.logger = getLogger(
f"{self.name}:{self.ts.name.lower().replace('_','-')}")
self.logger.info(
"Testing for a significant non-transit-like periodic variability")
self.time_before = self.ts.time
self.flux_before = self.ts.flux
self.time_after = self.ts.time
phase = fold(self.time_before, self.ts.ls.period)
bp, bf = running_median(phase, self.flux_before, 0.05, 100)
pv = interp1d(bp, bf)(phase)
df = abs(diff(pv) / diff(self.time_before))
ps = percentile(df, [80, 99.5])
pv_amplitude = bf.ptp()
bfn = -bf
bfn -= bfn.min() - 1e-12
bfn /= bfn.sum()
pv_entropy = -(bfn * log(bfn)).sum()
max_slope = df.max()
slope_percentile_ratio = ps[0] / ps[1]
self._bp = bp
self._bf = bf
self.phase = phase * self.ts.ls.period
self.model = pv
self.spr = slope_percentile_ratio
self.amplitude = pv_amplitude
self.entropy = pv_entropy
self.max_slope = max_slope
self.peak_siginifance = dip_significance(24 * self.ts.ls.period * bp,
bf)
self.is_sigificant = pv_amplitude > 0.001
self.is_transit_like = (slope_percentile_ratio < 0.1
or self.peak_siginifance > 3.0)
if self.is_sigificant and not self.is_transit_like:
self.logger.info("Found and removed a periodic signal")
self.model_removed = True
flux = self.ts.flux - self.model + 1
self.flux_after = flux
self.ts.update_data('pvarstep', self.ts.time, flux, self.ts.ferr)
else:
self.flux_after = self.ts.flux
self.model_removed = False
if self.is_sigificant:
self.logger.info(
"Found a periodic signal but it's too transit-like to be removed"
)
else:
self.logger.info(
"Didn't find any significant periodic signals")
def plot_folded_tess_transit(self,
method: str = 'de',
pv: ndarray = None,
binwidth: float = 1,
plot_model: bool = True,
plot_unbinned: bool = True,
plot_binned: bool = True,
xlim: tuple = None,
ylim: tuple = None,
ax=None,
figsize: tuple = None):
assert method in ('de', 'mc')
if pv is None:
if method == 'de':
pv = self.de.minimum_location
else:
df = self.posterior_samples(derived_parameters=False)
pv = df.median().values
if ax is None:
fig, ax = subplots(figsize=figsize)
else:
fig, ax = None, ax
ax.autoscale(enable=True, axis='x', tight=True)
etess = self._ntess
t = self.timea[:etess]
fo = self.ofluxa[:etess]
fm = squeeze(self.transit_model(pv))[:etess]
bl = squeeze(self.baseline(pv))[:etess]
phase = 24 * pv[1] * (fold(t, pv[1], pv[0], 0.5) - 0.5)
sids = argsort(phase)
phase = phase[sids]
bp, bf, be = downsample_time(phase, (fo / bl)[sids], binwidth / 60)
if plot_unbinned:
ax.plot(phase, (fo / bl)[sids], 'k.', alpha=0.1, ms=2)
if plot_binned:
ax.errorbar(bp, bf, be, fmt='ko', ms=3)
if plot_model:
ax.plot(phase, fm[sids], 'k')
setp(ax,
ylim=ylim,
xlim=xlim,
xlabel='Time - T$_c$ [h]',
ylabel='Normalised flux')
if fig is not None:
fig.tight_layout()
return fig
def __init__(self, name: str):
times, fluxes, _, _, _, _ = read_tess(tess_file,
zero_epoch,
period,
use_pdc=True,
baseline_duration_d=period)
phase, time, flux = [], [], []
for t, f in zip(times, fluxes):
ph = (fold(t, period.n, zero_epoch.n, 0.5) - 0.5) * period.n
mask = abs(ph) > 0.03
phase.append(ph[mask])
time.append(t[mask])
flux.append(f[mask])
super().__init__(name, ['TESS'],
time,
flux,
wnids=arange(len(flux)),
lnlikelihood='celerite')
def plot_folded_tess_transit(self, solution: str = 'de', pv: ndarray = None, binwidth: float = 1,
plot_model: bool = True, plot_unbinned: bool = True, plot_binned: bool = True,
xlim: tuple = None, ylim: tuple = None, ax=None, figsize: tuple = None):
if pv is None:
if solution.lower() == 'local':
pv = self._local_minimization.x
elif solution.lower() in ('de', 'global'):
pv = self.de.minimum_location
elif solution.lower() in ('mcmc', 'mc'):
pv = self.posterior_samples().median().values
else:
raise NotImplementedError("'solution' should be either 'local', 'global', or 'mcmc'")
if ax is None:
fig, ax = subplots(figsize=figsize)
else:
fig, ax = None, ax
ax.autoscale(enable=True, axis='x', tight=True)
etess = self._ntess
t = self.timea[:etess]
fo = self.ofluxa[:etess]
fm = squeeze(self.transit_model(pv))[:etess]
bl = squeeze(self.baseline(pv))[:etess]
phase = 24 * pv[1] * (fold(t, pv[1], pv[0], 0.5) - 0.5)
sids = argsort(phase)
phase = phase[sids]
bp, bf, be = downsample_time(phase, (fo / bl)[sids], binwidth / 60)
if plot_unbinned:
ax.plot(phase, (fo / bl)[sids], 'k.', alpha=0.1, ms=2)
if plot_binned:
ax.errorbar(bp, bf, be, fmt='ko', ms=3)
if plot_model:
ax.plot(phase, fm[sids], 'k')
setp(ax, ylim=ylim, xlim=xlim, xlabel='Time - T$_c$ [h]', ylabel='Normalised flux')
if fig is not None:
fig.tight_layout()
return fig
def plot_rv_vs_phase(self,
planet: int,
method='de',
pv=None,
nsamples: int = 200,
ntimes: int = 500,
axs=None):
if axs is None:
fig, axs = subplots(2,
1,
gridspec_kw={'height_ratios': (3, 1)},
sharex='all')
else:
fig, axs = None, axs
if pv is None:
if method == 'de':
if self.lpf.de is None:
raise ValueError(
"The global optimizer hasn't been initialized.")
pvp = None
pv = self.lpf.de.minimum_location
elif method == 'mcmc':
if self.lpf.sampler is None:
raise ValueError("The sampler hasn't been initialized.")
df = self.lpf.posterior_samples()
pvp = permutation(df.values)[:nsamples, :]
pv = median(pvp, 0)
else:
if pv.ndim == 1:
pvp = None
pv = pv
else:
pvp = permutation(pv)[:nsamples, :]
pv = median(pvp, 0)
rv_time = linspace(self._timea.min() - 1,
self._timea.max() + 1,
num=ntimes)
all_planets = set(range(self.nplanets))
other_planets = all_planets.difference([planet])
if pvp is None:
rv_model = self.rv_model(pv,
rv_time + self._tref, [planet],
add_sv=False)
rv_others = self.rv_model(pv, planets=other_planets, add_sv=False)
rv_model_limits = None
else:
rv_percentiles = percentile(
self.rv_model(pvp,
rv_time + self._tref, [planet],
add_sv=False), [50, 16, 84, 2.5, 97.5], 0)
rv_model = rv_percentiles[0]
rv_model_limits = rv_percentiles[1:]
rv_others = median(
self.rv_model(pvp, planets=other_planets, add_sv=False), 0)
period = pv[self.ps.names.index(f'p_{planet + 1}')]
tc = pv[self.ps.names.index(f'tc_{planet + 1}')] - self._tref
phase = (fold(self._timea, period, tc, 0.5) - 0.5) * period
phase_model = (fold(rv_time, period, tc, 0.5) - 0.5) * period
msids = argsort(phase_model)
if pvp is not None:
axs[0].fill_between(phase_model[msids],
rv_model_limits[2, msids],
rv_model_limits[3, msids],
facecolor='blue',
alpha=0.15)
axs[0].fill_between(phase_model[msids],
rv_model_limits[0, msids],
rv_model_limits[1, msids],
facecolor='darkblue',
alpha=0.25)
axs[0].errorbar(phase,
self._rva - rv_others - self.rv_shifts(pv),
self._rvea,
fmt='ok')
axs[0].plot(phase_model[msids], rv_model[msids], 'k')
axs[1].errorbar(phase,
self._rva - self.rv_model(pv),
self._rvea,
fmt='ok')
setp(axs[0], ylabel='RV [m/s]')
setp(axs[1], xlabel='Phase [d]', ylabel='O-M [m/s]')
axs[0].autoscale(axis='x', tight=True)
if fig is not None:
fig.tight_layout()
return fig
def phase(self) -> Optional[ndarray]:
if self.zero_epoch is not None:
return fold(self.time, self.period, self.zero_epoch, 0.5) * self.period
else:
return None
def __call__(self, npop: int = 40, de_niter: int = 1000, mcmc_niter: int = 200, mcmc_repeats: int = 3, initialize_only: bool = False):
self.logger = getLogger(f"{self.name}:{self.ts.name.lower().replace('_','-')}")
self.logger.info(f"Fitting {self.mode} transits")
self.ts.transit_fits[self.mode] = self
epochs = epoch(self.ts.time, self.ts.zero_epoch, self.ts.period)
if self.mode == 'all':
mask = ones(self.ts.time.size, bool)
elif self.mode == 'even':
mask = epochs % 2 == 0
elif self.mode == 'odd':
mask = epochs % 2 == 1
else:
raise NotImplementedError
mask &= abs(self.ts.phase - 0.5*self.ts.period) < 4 * 0.5 * self.ts.duration
self.ts.transit_fit_masks[self.mode] = self.mask = mask
self.epochs = epochs = epochs[mask]
self.time = self.ts.time[mask]
self.fobs = self.ts.flux[mask]
tref = floor(self.time.min())
tm = QuadraticModelCL(klims=(0.01, 0.60)) if self.use_opencl else QuadraticModel(interpolate=False)
self.lpf = lpf = SearchLPF(times=self.time, fluxes=self.fobs, epochs=epochs, tm=tm,
nsamples=self.nsamples, exptimes=self.exptime, tref=tref)
# TODO: V-shaped transits are not always modelled well. Need to set smarter priors (or starting population)
# for the impact parameter and stellar density.
lpf.set_prior('rho', 'UP', 0.01, 25)
if self.mode == 'all':
d = min(self.ts.depth, 0.75)
lpf.set_prior('tc', 'NP', self.ts.zero_epoch, 0.01)
lpf.set_prior('p', 'NP', self.ts.period, 0.001)
lpf.set_prior('k2', 'UP', max(0.01**2, 0.5*d), min(max(0.08**2, 4*d), 0.75**2))
else:
pr = self.ts.tf_all.parameters
lpf.set_prior('tc', 'NP', pr.tc.med, 5*pr.tc.err)
lpf.set_prior('p', 'NP', pr.p.med, pr.p.err)
lpf.set_prior('k2', 'UP', max(0.01**2, 0.5 * pr.k2.med), max(0.08**2, min(0.6**2, 2 * pr.k2.med)))
lpf.set_prior('q1', 'NP', pr.q1.med, pr.q1.err)
lpf.set_prior('q2', 'NP', pr.q2.med, pr.q2.err)
# TODO: The limb darkening table has been computed for TESS. Needs to be made flexible.
if self.ts.teff is not None:
ldcs = Table.read(Path(__file__).parent / "data/ldc_table.fits").to_pandas()
ip = interp1d(ldcs.teff, ldcs[['q1', 'q2']].T)
q1, q2 = ip(clip(self.ts.teff, 2000., 12000.))
lpf.set_prior('q1', 'NP', q1, 1e-5)
lpf.set_prior('q2', 'NP', q2, 1e-5)
if initialize_only:
return
else:
lpf.optimize_global(niter=de_niter, npop=npop, use_tqdm=self.use_tqdm, plot_convergence=False)
lpf.sample_mcmc(mcmc_niter, repeats=mcmc_repeats, use_tqdm=self.use_tqdm, leave=False)
df = lpf.posterior_samples(derived_parameters=True)
df = pd.DataFrame((df.median(), df.std()), index='med err'.split())
pv = lpf.posterior_samples(derived_parameters=False).median().values
self.phase = fold(self.time, pv[1], pv[0], 0.5) * pv[1] - 0.5 * pv[1]
self.fmod = lpf.flux_model(pv)
self.ftra = lpf.transit_model(pv)
self.fbase = lpf.baseline(pv)
# Calculate the per-orbit log likelihood differences
# --------------------------------------------------
ues = unique(epochs)
lnl = zeros(ues.size)
err = 10 ** pv[7]
def lnlike_normal(o, m, e):
npt = o.size
return -npt * log(e) - 0.5 * npt * log(2. * pi) - 0.5 * sum((o - m) ** 2 / e ** 2)
for i, e in enumerate(ues):
m = epochs == e
lnl[i] = lnlike_normal(self.fobs[m], self.fmod[m], err) - lnlike_normal(self.fobs[m], 1.0, err)
self.parameters = df
self.dll_epochs = ues
self.dll_values = lnl
self.zero_epoch = df.tc.med
self.period = df.p.med
self.duration = df.t14.med
self.depth = df.k2.med
if self.mode == 'all':
self.delta_bic = self.ts.dbic = delta_bic(lnl.sum(), 0, 9, self.time.size)
self.ts.update_ephemeris(self.zero_epoch, self.period, self.duration, self.depth)
def plot_folded_planets(self,
passband: str,
method: str = 'de',
bwidth: float = 10,
axs=None,
pv: ndarray = None,
nsamples: int = 100,
limp=(2.5, 97.5, 16, 84),
limc: str = 'darkblue',
lima: float = 0.15,
ylines=None):
from pytransit.lpf.tesslpf import downsample_time
if axs is None:
fig, axs = subplots(1, self.nplanets, sharey='all')
else:
fig, axs = None, axs
if pv is None:
if method == 'de':
if self.de is None:
raise ValueError(
"The global optimizer hasn't been initialized.")
pvp = None
pv = self.de.minimum_location
elif method == 'mcmc':
if self.sampler is None:
raise ValueError("The sampler hasn't been initialized.")
df = self.posterior_samples(derived_parameters=False)
pvp = permutation(df.values)[:nsamples, :]
pv = median(pvp, 0)
else:
if pv.ndim == 1:
pvp = None
pv = pv
else:
pvp = permutation(pv)[:nsamples, :]
pv = median(pvp, 0)
is_pb = self.pbids == self.passbands.index(passband)
pbmask = zeros(self.timea.size, 'bool')
for sl, cpb in zip(self.lcslices, is_pb):
if cpb:
pbmask[sl] = 1
tcids = [
self.ps.names.index(f'tc_{i + 1}') for i in range(self.nplanets)
]
prids = [
self.ps.names.index(f'p_{i + 1}') for i in range(self.nplanets)
]
t0s = pv[tcids]
prs = pv[prids]
for ipl in range(self.nplanets):
planets = set(arange(self.nplanets))
planets.remove(ipl)
if pvp is None:
mflux = squeeze(self.transit_model(pv, planets=[ipl]))[pbmask]
rflux = squeeze(self.transit_model(pv,
planets=planets))[pbmask]
mflim = None
fbline = self.baseline(pv)[pbmask]
else:
mfluxes = self.transit_model(pvp, planets=[ipl])[:, pbmask]
rfluxes = self.transit_model(pvp, planets=planets)[:, pbmask]
fblines = self.baseline(pvp)[:, pbmask]
mflux = median(mfluxes, 0)
mflim = percentile(mfluxes, limp, 0)
rflux = median(rfluxes, 0)
fbline = median(fblines, 0)
oflux = self.ofluxa[pbmask] / rflux / fbline
phase = (fold(self.timea[pbmask], prs[ipl], t0s[ipl], 0.5) -
0.5) * prs[ipl]
m = abs(phase) < 0.5 * self.bldur
sids = argsort(phase[m])
if m.sum() > 0:
phase, mflux, oflux = phase[m][sids], mflux[m][sids], oflux[m][
sids]
bp, bf, be = downsample_time(phase, oflux, bwidth / 24 / 60)
if mflim is not None:
for il in range(mflim.shape[0] // 2):
axs[ipl].fill_between(phase,
mflim[2 * il, m][sids],
mflim[2 * il + 1, m][sids],
fc=limc,
alpha=lima)
axs[ipl].errorbar(bp, bf, be, fmt='ok')
axs[ipl].plot(phase, oflux, '.', alpha=0.25)
axs[ipl].plot(phase, mflux, 'k')
if ylines is not None:
axs[ipl].fill_between(phase, mflux, 1, fc='w', zorder=-99)
for yl in ylines:
axs[ipl].axhline(yl,
lw=1,
ls='--',
c='k',
alpha=0.5,
zorder=-100)
setp(axs,
xlim=(-0.5 * self.bldur, 0.5 * self.bldur),
ylim=(0.996, 1.004))
if fig is not None:
fig.tight_layout()
return fig
def plot_gb_transits(self,
method='de',
pv: ndarray = None,
remove_baseline: bool = True,
figsize: tuple = (14, 2),
axes=None,
ncol: int = 4,
xlim: tuple = None,
ylim: tuple = None,
nsamples: int = 200):
if pv is None:
if method == 'de':
if self.de is None:
raise ValueError(
"The global optimizer hasn't been initialized.")
pvp = None
pv = self.de.minimum_location
elif method == 'mcmc':
if self.sampler is None:
raise ValueError("The sampler hasn't been initialized.")
df = self.posterior_samples(derived_parameters=False)
pvp = permutation(df.values)[:nsamples, :]
pv = median(pvp, 0)
else:
if pv.ndim == 1:
pvp = None
pv = pv
else:
pvp = permutation(pv)[:nsamples, :]
pv = median(pvp, 0)
if pvp is None:
if remove_baseline:
fobs = self.ofluxa / squeeze(self.baseline(pv))
fmodel = squeeze(self.transit_model(pv))
fbasel = ones_like(self.ofluxa)
else:
fobs = self.ofluxa
fmodel = squeeze(self.flux_model(pv))
fbasel = squeeze(self.baseline(pv))
fmodel_limits = None
else:
if remove_baseline:
fobs = self.ofluxa / squeeze(self.baseline(pv))
fmodels = percentile(self.transit_model(pvp),
[50, 16, 84, 2.5, 97.5], 0)
fbasel = ones_like(self.ofluxa)
else:
fobs = self.ofluxa
fmodels = percentile(self.flux_model(pvp),
[50, 16, 84, 2.5, 97.5], 0)
fbasel = median(self.baseline(pvp), 0)
fmodel = fmodels[0]
fmodel_limits = fmodels[1:]
tcids = [
self.ps.names.index(f'tc_{i + 1}') for i in range(self.nplanets)
]
prids = [
self.ps.names.index(f'p_{i + 1}') for i in range(self.nplanets)
]
t0s = pv[tcids]
prs = pv[prids]
tcs = array([t.mean() for t in self.times[self._stess:]])
tds = array([
abs(fold(tcs, prs[i], t0s[i], 0.5) - 0.5)
for i in range(self.nplanets)
])
pids = argmin(tds, 0)
nlc = self.nlc - self._stess
nrow = int(ceil(nlc / ncol))
if axes is None:
fig, axs = subplots(nrow,
ncol,
figsize=figsize,
sharex='all',
sharey='all',
squeeze=False)
else:
fig, axs = None, axes
[ax.autoscale(enable=True, axis='x', tight=True) for ax in axs.flat]
etess = self._stess
for iax, i in enumerate(range(self.nlc - etess)):
ax = axs.flat[iax]
sl = self.lcslices[etess + i]
t = self.times[etess + i]
e = epoch(t.mean(), t0s[pids[i]], prs[pids[i]])
tc = t0s[pids[i]] + e * prs[pids[i]]
tt = 24 * (t - tc)
if fmodel_limits is not None:
ax.fill_between(tt,
fmodel_limits[2, sl],
fmodel_limits[3, sl],
facecolor='blue',
alpha=0.15)
ax.fill_between(tt,
fmodel_limits[0, sl],
fmodel_limits[1, sl],
facecolor='darkblue',
alpha=0.25)
ax.plot(tt, fobs[sl], 'k.', alpha=0.2)
ax.plot(tt, fmodel[sl], 'k')
setp(axs, xlim=xlim, ylim=ylim)
setp(axs[-1, :], xlabel='Time - T$_c$ [h]')
setp(axs[:, 0], ylabel='Normalised flux')
fig.tight_layout()
return fig
