def fit_spline(x, y, bins=4, estimator=np.median):
""" Find a smooth function that approximates `x`, `y`.
`bins` is the number of bins into which the sample is split. Returns
a function f(x) that approximates y from min(x) to max(x).
Notes
-----
The sample is split into bins number of sub-samples with evenly
spaced x values. The median x and y value within each subsample is
measured, and a cubic spline is drawn through these subsample
median points.
`x` must be sorted lowest -> highest, but need not be evenly spaced.
"""
x,y = map(np.asarray, (x,y))
good = ~np.isnan(x)
good &= ~np.isnan(y)
x = x[good]
y = y[good]
binedges = np.linspace(x.min(), x.max(), bins+1)
medvals = []
cbins = []
for x0,x1 in zip(binedges[:-1], binedges[1:]):
cond = between(x, x0, x1)
if not cond.any():
continue
cbins.append(estimator(x[cond]))
medvals.append(estimator(y[cond]))
if len(cbins) < 3:
raise RuntimeError('Too few bins')
return AkimaSpline(cbins, medvals)
def editRow(row):
gotChoice = False
while not gotChoice:
utilities.clearScreen()
#print(row); input(); quit()
print('1) Solution Type: %s' % row[2][1][1])
print('2) Distance: %s' % row[0])
interval = utilities.format_time_string(row[1])
if interval[0] == 'interval':
print('3) Time: %s' % interval[1])
else: pass #-> there should be no error from this function
# call - the time is guaranteed to be a float.
choice = input('Which line do you wish to edit ([r] to return)? ')
if choice.lower() == 'r':
gotChoice = True
elif utilities.isInt(choice) and utilities.between(int(choice), 1, 3):
gotChoice = True
else: input('%s is not a valid choice: press [ENTER] to continue' % choice)
if choice == 'r': return
if choice == '3':
row[1] = get_time()
editRow(row)
elif choice == '2':
row[0] = get_distance()
editRow(row)
elif choice == '1':
input('rutwro')
def get_row():
choice = input('Which leg? ')
if choice == 'q': return(0)
if len(choice) > 0 and utilities.isInt(choice):
if utilities.between(int(choice), 1, len(result_set)): return(result_set[int(choice) - 1])
else: input('%s is not a valid choice. Press [Enter] to continue (or [q] to quit)' % choice)
else: input('You must choose a leg between %d through %d. Press [Enter] to continue (or [q] to quit)' % (1, len(result_set)))
def plotlines(z, ax, atmos=None, lines=None, labels=False, ls="dotted", color="k", trim=False, fontsize=10, **kwargs):
""" Draw vertical dotted lines showing expected positions of
absorption and emission lines, given a redshift.
Parameters
----------
atmos : list of float pairs, or True (None)
Regions of atmospheric absorption to plot. If True, it uses an
internal list of regions.
lines : stuctured array, optional
If given, it must be a record array with fields 'name' and 'wa'.
Returns the mpl artists representing the lines.
"""
if lines is None:
lines = readtxt(DATAPATH + "linelists/galaxy_lines", names="wa,name,select")
else:
lines = np.rec.fromrecords([(l["name"], l["wa"]) for l in lines], names="name,wa")
autoscale = ax.get_autoscale_on()
if autoscale:
ax.set_autoscale_on(False)
artists = []
w0, w1 = ax.get_xlim()
wa = lines.wa * (z + 1)
if trim:
c0 = between(wa, w0, w1)
wa = wa[c0]
lines = lines[c0]
artists.append(axvlines(wa, ax=ax, ls=ls, color=color, **kwargs))
if labels:
for i in range(3):
for w, l in zip(wa[i::3], lines[i::3]):
if not (w0 < w < w1) and trim:
continue
# name = l.name + '%.2f' % l.wa
name = l.name
artists.append(
puttext(
w,
0.7 + i * 0.08,
name,
ax,
xcoord="data",
alpha=1,
fontsize=fontsize,
rotation=90,
ha="right",
color=color,
)
)
if atmos:
if atmos == True:
atmos = None
artists.append(plotatmos(ax, atmos=atmos))
if autoscale:
ax.set_autoscale_on(True)
return artists
def update(self):
""" Calculates the new continuum, residuals and updates the plots.
Updates the following attributes:
self.markers
self.continuum
"""
wa,fl,er = (self.spec[key] for key in 'wa fl er'.split())
co = np.empty(len(wa))
co.fill(np.nan)
for b0,b1 in zip(self.breaks[:-1], self.breaks[1:]):
cpts = [(x,y) for x,y in self.contpoints if b0 <= x <= b1]
if len(cpts) == 0:
continue
spline = AkimaSpline(*zip(*cpts))
i,j = wa.searchsorted([b0,b1])
co[i:j] = spline(wa[i:j])
resid = (fl - co) / er
# histogram
bins = np.arange(0, 5+0.1, 0.2)
w0,w1 = self.fig.axes[1].get_xlim()
x,_ = np.histogram(resid[between(wa, w0, w1)],
bins=bins)
b = np.repeat(bins, 2)
X = np.concatenate([[0], np.repeat(x,2), [0]])
Xmax = X.max()
X = 0.05 * X / Xmax
self.markers['hist_left'].set_data(X, b)
self.markers['contpoints'].set_data(zip(*self.contpoints))
nbin = self.nbin
self.markers['cont'].set_data(wa[::nbin], co[::nbin])
self.markers['resid'].set_data(wa[::nbin], resid[::nbin])
if self.smoothby is not None:
sfl = convolve_psf(fl, self.smoothby)
self.art_fl.set_data(wa, sfl)
else:
self.art_fl.set_data(wa, fl)
self.continuum = co
saveobj('_knots.sav', self.contpoints, overwrite=True)
self.fig.canvas.draw()
def calc_iontau(wa, ion, zp1, logN, b, debug=False, ticks=False, maxdv=1000.,
label_tau_threshold=0.01, vpad=500., verbose=True):
""" Returns tau values at each wavelength for transitions in ion.
Parameters
----------
wa : array of floats
wavelength array
ion : atom.data entry
ion entry from readatom output dictionary
zp1 : float
redshift + 1
logN : float
log10(column density in cm**-2)
b : float
b parameter (km/s). Assumes thermal broadening.
maxdv : float (default 1000)
For performance reasons, only calculate the Voigt profile for a
single line to +/- maxdv. Increase this if you expect DLA-type
extended wings. None for no maximum.
vpad : float (default 500)
Include transitions that are within vpad km/s of either edge of
the wavelength array.
Returns
-------
tau : array of floats
Array of optical depth values.
"""
z = zp1 - 1
if debug:
i = int(len(wa)/2)
psize = c_kms * (wa[i] - wa[i-1]) / wa[i]
print 'approx pixel width %.1f km/s at %.1f Ang' % (psize, wa[i])
#select only ions with redshifted central wavelengths inside wa,
#+/- the padding velocity range vpad.
obswavs = ion.wa * zp1
wmin = wa[0] * (1 - vpad / c_kms)
wmax = wa[-1] * (1 + vpad / c_kms)
trans = ion[between(obswavs, wmin, wmax)]
if debug:
if len(trans) == 0:
print 'No transitions found overlapping with wavelength array'
tickmarks = []
sumtau = np.zeros_like(wa)
i0 = i1 = None
for i,(wav0,osc,gam) in enumerate(trans):
refwav = wav0 * zp1
dv = (wa - refwav) / refwav * c_kms
if maxdv is not None:
i0,i1 = dv.searchsorted([-maxdv, maxdv])
tau = calctau(dv[i0:i1], wav0, osc, gam, logN, btemp=b,
debug=debug, verbose=verbose)
if ticks and tau.max() > label_tau_threshold:
tickmarks.append((refwav, z, wav0, i))
sumtau[i0:i1] += tau
if ticks:
return sumtau, tickmarks
else:
return sumtau