def plot_misclass(epoch=10, plotdir='../../plots/phot_and_morph/'):
"""
Just plot the single epoch `galaxies` that turned out to be
stars in the coadd - its weird that this happens at bright mags.
"""
single, coadd = fetch_mixed_epoch(epoch)
mags = coadd['psfmag_r']
singlepmm = single['psfmag_r'] - single['modelmag_r']
coaddpmm = coadd['psfmag_r'] - coadd['modelmag_r']
ind = (single['type'] == 3) & (coaddpmm < 0.03) & (coaddpmm > -0.03)
f = pl.figure()
pl.plot(mags[ind], singlepmm[ind], '.k', alpha=0.3)
f.savefig(plotdir + 'misclassed_gals.png')
def plot_misclass(epoch=10, plotdir='../../plots/phot_and_morph/'):
"""
Just plot the single epoch `galaxies` that turned out to be
stars in the coadd - its weird that this happens at bright mags.
"""
single, coadd = fetch_mixed_epoch(epoch)
mags = coadd['psfmag_r']
singlepmm = single['psfmag_r'] - single['modelmag_r']
coaddpmm = coadd['psfmag_r'] - coadd['modelmag_r']
ind = (single['type'] == 3) & (coaddpmm < 0.03) & (coaddpmm > -0.03)
f = pl.figure()
pl.plot(mags[ind], singlepmm[ind], '.k', alpha=0.3)
f.savefig(plotdir + 'misclassed_gals.png')
def one_epoch_class_check(epoch=10, plotdir='../../plots/phot_and_morph/'):
"""
Check out the change in classification from the single epoch to the coadd.
"""
single, coadd = fetch_mixed_epoch(epoch)
ind = np.random.permutation(single['objid'].size)[0]
assert single['coadd_objid'][ind] == coadd['objid'][ind], 'Object mismatch'
mags = coadd['psfmag_r']
singlepmm = single['psfmag_r'] - single['modelmag_r']
coaddpmm = coadd['psfmag_r'] - coadd['modelmag_r']
fs = 5
alpha = 0.3
colors = ['#CC6600', '#990099']
titles = ['single epoch ', 'coadd ']
classes = [single['type'], coadd['type']]
xlabel = 'Coadd psfmag r'
ylabel = 'psf - model r'
xlim = (18, 22)
ylim = (-0.1, 0.5)
f = pl.figure(figsize=(4 * fs, 2 * fs))
pl.subplots_adjust(wspace=0.25, right=0.8)
xticks = []
for i in range(10):
if i % 2 == 0:
xticks.append('%0.0f' % (18 + 0.5 * i))
else:
xticks.append('')
types = [3, 6]
crit = [0.145, 0.03]
for i in range(2):
for j in range(2):
ind = classes[i] == types[j]
ax = pl.subplot(2, 4, 4 * i + j * 2 + 1)
pl.plot(mags[ind], singlepmm[ind], '.', alpha=alpha, color=colors[j])
pl.plot([18, 22], [crit[0], crit[0]], 'k', lw=2.5)
pl.plot([18, 22], [-crit[0], -crit[0]], 'k', lw=2.5)
pl.xlabel(xlabel)
pl.ylabel(titles[0] + ylabel)
pl.title(titles[i] + 'type')
pl.xlim(xlim)
pl.ylim(ylim)
ax.set_xticklabels(xticks)
ax = pl.subplot(2, 4, 4 * i + j * 2 + 2)
pl.plot(mags[ind], coaddpmm[ind], '.', alpha=alpha, color=colors[j])
pl.plot([18, 22], [crit[1], crit[1]], 'k', lw=2.5)
pl.plot([18, 22], [-crit[1], -crit[1]], 'k', lw=2.5)
pl.xlabel(xlabel)
pl.ylabel(titles[1] + ylabel)
pl.title(titles[i] + 'type')
pl.xlim(xlim)
pl.ylim(ylim)
ax.set_xticklabels(xticks)
rfnotes = 'RF:\n - Why are there single epoch "stars"\n so far above 0.145? '
rfnotes += 'This seems to be\n true regardless of "single epoch type"\n or '
rfnotes += '"coadd type". Is the single epoch\n data crummier than normal SDSS?\n\n'
rfnotes += '- It is plain to see that "type" from single\n epoch data is calling some '
rfnotes += 'small\n fraction of stars "galaxies" and vice versa.\n\n'
rfnotes += '- The coadd classification clears things up,\n but there must still be a '
rfnotes += 'fair bit of label\n error. "Galaxies" are piling up near 0.03\n in the coadd '
rfnotes += 'and the dist. of stars is\n asymmetric at the faint end.\n\n'
rfnotes += '- Note the downward trend of the stellar\n locus in the single epoch data. '
rfnotes += 'This bias\n is likely arises from the noise model used\n in the psf fitting. '
rfnotes += 'This is also seen in the\n coadd if you go to faint depths. '
rfnotes += 'This\n motivates not forcing axis alignment in all\n XD "star" clusters.'
pl.text(1.1, 2.1, rfnotes, transform=ax.transAxes, va='top')
f.savefig(plotdir + 'pminusm_changes_%d.png' % epoch)
def one_epoch_class_check(epoch=10, plotdir='../../plots/phot_and_morph/'):
"""
Check out the change in classification from the single epoch to the coadd.
"""
single, coadd = fetch_mixed_epoch(epoch)
ind = np.random.permutation(single['objid'].size)[0]
assert single['coadd_objid'][ind] == coadd['objid'][ind], 'Object mismatch'
mags = coadd['psfmag_r']
singlepmm = single['psfmag_r'] - single['modelmag_r']
coaddpmm = coadd['psfmag_r'] - coadd['modelmag_r']
fs = 5
alpha = 0.3
colors = ['#CC6600', '#990099']
titles = ['single epoch ', 'coadd ']
classes = [single['type'], coadd['type']]
xlabel = 'Coadd psfmag r'
ylabel = 'psf - model r'
xlim = (18, 22)
ylim = (-0.1, 0.5)
f = pl.figure(figsize=(4 * fs, 2 * fs))
pl.subplots_adjust(wspace=0.25, right=0.8)
xticks = []
for i in range(10):
if i % 2 == 0:
xticks.append('%0.0f' % (18 + 0.5 * i))
else:
xticks.append('')
types = [3, 6]
crit = [0.145, 0.03]
for i in range(2):
for j in range(2):
ind = classes[i] == types[j]
ax = pl.subplot(2, 4, 4 * i + j * 2 + 1)
pl.plot(mags[ind],
singlepmm[ind],
'.',
alpha=alpha,
color=colors[j])
pl.plot([18, 22], [crit[0], crit[0]], 'k', lw=2.5)
pl.plot([18, 22], [-crit[0], -crit[0]], 'k', lw=2.5)
pl.xlabel(xlabel)
pl.ylabel(titles[0] + ylabel)
pl.title(titles[i] + 'type')
pl.xlim(xlim)
pl.ylim(ylim)
ax.set_xticklabels(xticks)
ax = pl.subplot(2, 4, 4 * i + j * 2 + 2)
pl.plot(mags[ind],
coaddpmm[ind],
'.',
alpha=alpha,
color=colors[j])
pl.plot([18, 22], [crit[1], crit[1]], 'k', lw=2.5)
pl.plot([18, 22], [-crit[1], -crit[1]], 'k', lw=2.5)
pl.xlabel(xlabel)
pl.ylabel(titles[1] + ylabel)
pl.title(titles[i] + 'type')
pl.xlim(xlim)
pl.ylim(ylim)
ax.set_xticklabels(xticks)
rfnotes = 'RF:\n - Why are there single epoch "stars"\n so far above 0.145? '
rfnotes += 'This seems to be\n true regardless of "single epoch type"\n or '
rfnotes += '"coadd type". Is the single epoch\n data crummier than normal SDSS?\n\n'
rfnotes += '- It is plain to see that "type" from single\n epoch data is calling some '
rfnotes += 'small\n fraction of stars "galaxies" and vice versa.\n\n'
rfnotes += '- The coadd classification clears things up,\n but there must still be a '
rfnotes += 'fair bit of label\n error. "Galaxies" are piling up near 0.03\n in the coadd '
rfnotes += 'and the dist. of stars is\n asymmetric at the faint end.\n\n'
rfnotes += '- Note the downward trend of the stellar\n locus in the single epoch data. '
rfnotes += 'This bias\n is likely arises from the noise model used\n in the psf fitting. '
rfnotes += 'This is also seen in the\n coadd if you go to faint depths. '
rfnotes += 'This\n motivates not forcing axis alignment in all\n XD "star" clusters.'
pl.text(1.1, 2.1, rfnotes, transform=ax.transAxes, va='top')
f.savefig(plotdir + 'pminusm_changes_%d.png' % epoch)
