def test_lightcurve(self):
# make 4 images with different date
images = []
image_datasets = db_subs.generate_timespaced_dbimages_data(n_images=4,
taustart_ts= datetime.datetime(2010, 3, 3)
)
for dset in image_datasets:
image = Image(dataset=self.dataset, data=dset)
images.append(image)
# 3 sources per image, with different coordinates & flux
data_list = []
for i in range(1, 4):
data_list.append({
'ra': 111.11 + i,
'decl': 11.11 + i,
'i_peak': 10. * i ,
'i_peak_err': 0.1,
})
# Insert the 3 sources in each image, while further varying the flux
lightcurves_sorted_by_ra = [[],[],[]]
for im_idx, image in enumerate(images):
# Create the "source finding results"
# Note that we reuse 'i_peak' as both peak & integrated flux.
img_sources = []
for src_idx, data in enumerate(data_list):
src = db_subs.example_extractedsource_tuple(
ra = data['ra'],dec=data['decl'],
peak=data['i_peak']* (1 + im_idx),
flux = data['i_peak']* (1 + im_idx)
)
lightcurves_sorted_by_ra[src_idx].append(src)
img_sources.append(src)
insert_extracted_sources(image._id, img_sources)
associate_extracted_sources(image._id, deRuiter_r=3.7,
new_source_sigma_margin=3)
# updates the dataset and its set of images
self.dataset.update()
self.dataset.update_images()
# update the images and their sets of sources
for image in self.dataset.images:
image.update()
image.update_sources()
# Now pick last image, select the first source (smallest RA)
# and extract its light curve
sources = self.dataset.images[-1].sources
sources = sorted(sources, key=attrgetter('ra'))
lightcurve = ligtcurve_func(sources[0]._id)
# check if the sources are associated in all images
self.assertEqual(len(images), len(lightcurve))
self.assertEqual(lightcurve[0][0], datetime.datetime(2010, 3, 3, 0, 0))
self.assertEqual(lightcurve[1][0], datetime.datetime(2010, 3, 4, 0, 0))
self.assertEqual(lightcurve[2][0], datetime.datetime(2010, 3, 5, 0, 0))
self.assertEqual(lightcurve[3][0], datetime.datetime(2010, 3, 6, 0, 0))
self.assertAlmostEqual(lightcurve[0][2], 10.)
self.assertAlmostEqual(lightcurve[1][2], 20.)
self.assertAlmostEqual(lightcurve[2][2], 30.)
self.assertAlmostEqual(lightcurve[3][2], 40.)
#Check the summary statistics (avg flux, etc)
query = """\
SELECT rf.avg_f_int
,rf.avg_f_int_sq
,avg_weighted_f_int
,avg_f_int_weight
FROM runningcatalog r
,runningcatalog_flux rf
WHERE r.dataset = %(dataset)s
AND r.id = rf.runcat
ORDER BY r.wm_ra
"""
self.database.cursor.execute(query, {'dataset': self.dataset.id})
runcat_flux_entries = get_db_rows_as_dicts(self.database.cursor)
self.assertEqual(len(runcat_flux_entries), len(lightcurves_sorted_by_ra))
for idx, flux_summary in enumerate(runcat_flux_entries):
py_results = db_subs.lightcurve_metrics(lightcurves_sorted_by_ra[idx])
for key in flux_summary.keys():
self.assertAlmostEqual(flux_summary[key], py_results[-1][key])
#Now check the per-timestep statistics (variability indices)
sorted_runcat_ids = columns_from_table('runningcatalog',
where={'dataset':self.dataset.id},
order='wm_ra')
sorted_runcat_ids = [entry['id'] for entry in sorted_runcat_ids]
for idx, rcid in enumerate(sorted_runcat_ids):
db_indices = db_queries.get_assoc_entries(self.database,
rcid)
py_indices = db_subs.lightcurve_metrics(lightcurves_sorted_by_ra[idx])
self.assertEqual(len(db_indices), len(py_indices))
for nstep in range(len(db_indices)):
for key in ('v_int', 'eta_int', 'f_datapoints'):
self.assertAlmostEqual(db_indices[nstep][key],
py_indices[nstep][key],
places=5)
def test_lightcurve(self):
# make 4 * 5 images with different date
images = []
for day in [3, 4, 5, 6]:
data = {'taustart_ts': datetime.datetime(2010, 3, day),
'tau_time': 3600,
'url': '/',
'freq_eff': 80e6,
'freq_bw': 1e6,
'beam_smaj_pix': float(2.7),
'beam_smin_pix': float(2.3),
'beam_pa_rad': float(1.7),
'deltax': float(-0.01111),
'deltay': float(0.01111),
'centre_ra': 111,
'centre_decl': 11,
'xtr_radius' : 3
}
image = Image(dataset=self.dataset, data=data)
images.append(image)
# 3 sources per image, with different coordinates & flux
data_list = []
for i in range(1, 4):
data_list.append({
'ra': 111.11 + i,
'decl': 11.11 + i,
'ra_fit_err': 0.01,
'decl_fit_err': 0.01,
'ra_sys_err': 20,
'decl_sys_err': 20,
'i_peak': 10 * i ,
'i_peak_err': 0.1
# x=0.11, y=0.22, z=0.33, det_sigma=11.1, zone=i
})
# Insert the 3 sources in each image, while further varying the flux
for i, image in enumerate(images):
# Create the "source finding results"
# Note that we reuse 'i_peak' as both peak & integrated flux.
sources = []
for data in data_list:
source = (data['ra'], data['decl'],
data['ra_fit_err'], data['decl_fit_err'], # Gaussian fit errors
data['i_peak'] * (1 + i), data['i_peak_err'], # Peak
data['i_peak'] * (1 + i), data['i_peak_err'], # Integrated
10., # Significance level
1, 1, 0, # Beam params (width arcsec major, width arcsec minor, parallactic angle)
data['ra_sys_err'], data['decl_sys_err']) # Systematic errors
sources.append(source)
# Insert the sources
image.insert_extracted_sources(sources)
# Run the association for each list of source for an image
image.associate_extracted_sources(deRuiter_r=3.7)
# updates the dataset and its set of images
self.dataset.update()
self.dataset.update_images()
# update the images and their sets of sources
for image in self.dataset.images:
image.update()
image.update_sources()
# Now pick any image, select the first source (smallest RA)
# and extract its light curve
sources = self.dataset.images.pop().sources
sources = sorted(sources, key=attrgetter('ra'))
lightcurve = sources[0].lightcurve()
# check if the sources are associated in all images
self.assertEqual(len(images), len(lightcurve))
self.assertEqual(lightcurve[0][0], datetime.datetime(2010, 3, 3, 0, 0))
self.assertEqual(lightcurve[1][0], datetime.datetime(2010, 3, 4, 0, 0))
self.assertEqual(lightcurve[2][0], datetime.datetime(2010, 3, 5, 0, 0))
self.assertEqual(lightcurve[3][0], datetime.datetime(2010, 3, 6, 0, 0))
self.assertAlmostEqual(lightcurve[0][2], 10.)
self.assertAlmostEqual(lightcurve[1][2], 20.)
self.assertAlmostEqual(lightcurve[2][2], 30.)
self.assertAlmostEqual(lightcurve[3][2], 40.)
# Since the light curves are very similar, only eta_nu is different
results = dbtransients._select_updated_variability_indices(self.dataset.images[-1].id)
results = sorted(results, key=itemgetter('eta_int'))
for result, eta_nu in zip(results, (16666.66666667, 66666.666666667,
150000.0)):
self.assertEqual(result['f_datapoints'], 4)
self.assertAlmostEqual(result['eta_int'], eta_nu)
self.assertAlmostEqual(result['v_int'], 0.516397779494)
def test_lightsurface(self):
images = []
# make 4 * 5 images with different frequencies and date
for frequency in [80e6, 90e6, 100e6, 110e6, 120e6]:
for day in [3, 4, 5, 6]:
data = {'taustart_ts': datetime.datetime(2010, 3, day),
'tau_time': 3600,
'url': '/',
'freq_eff': frequency,
'freq_bw': 1e6,
'beam_smaj_pix': float(2.7),
'beam_smin_pix': float(2.3),
'beam_pa_rad': float(1.7),
'deltax': float(-0.01111),
'deltay': float(0.01111),
'centre_ra': 111,
'centre_decl': 11,
'xtr_radius' : 3
}
image = Image(dataset=self.dataset, data=data)
images.append(image)
# 3 sources per image, with different coordinates & flux
data_list = []
for i in range(1, 4):
data_list.append({
'ra': 111.111 + i,
'decl': 11.11 + i,
'ra_fit_err': 0.01,
'decl_fit_err': 0.01,
'ew_sys_err': 20,
'ns_sys_err': 20,
'i_peak': 10*i,
'i_peak_err': 0.1,
'error_radius': 10.0
# x=0.11, y=0.22, z=0.33, det_sigma=11.1, zone=i
})
# Insert the 3 sources in each image, while further varying the flux
for i, image in enumerate(images):
# Create the "source finding results"
sources = []
for data in data_list:
source = (data['ra'], data['decl'],
data['ra_fit_err'], data['decl_fit_err'],
data['i_peak']*(1+i), data['i_peak_err'],
data['i_peak']*(1+i), data['i_peak_err'],
10., # Significance level
1, 1, 0, # Beam params (width arcsec major, width arcsec minor, parallactic angle)
data['ew_sys_err'], data['ns_sys_err'], # Systematic errors
data['error_radius'])
sources.append(source)
# Insert the sources
image.insert_extracted_sources(sources)
# Run the association for each list of source for an image
image.associate_extracted_sources(deRuiter_r=3.7)
# updates the dataset and its set of images
self.dataset.update()
self.dataset.update_images()
# update the images and their sets of sources
for image in self.dataset.images:
image.update()
image.update_sources()
# Now pick any image, select the first source (smallest RA)
# and extract its light curve
# TODO: aaarch this is so ugly. Because this a set we need to pop it.
sources = self.dataset.images.pop().sources
#sources = self.dataset.images[-1].sources
sources = sorted(sources, key=attrgetter('ra'))
extracted_source = sources[0].id
lightcurve = tkp.db.general.lightcurve(extracted_source)
def test_lightsurface(self):
images = []
# make 4 * 5 images with different frequencies and date
for frequency in [80e6, 90e6, 100e6, 110e6, 120e6]:
for day in [3, 4, 5, 6]:
img_data = db_subs.example_dbimage_data_dict(
taustart_ts=datetime.datetime(2010, 3, day),
freq_eff=frequency)
image = Image(dataset=self.dataset, data=img_data)
images.append(image)
# 3 sources per image, with different coordinates & flux
data_list = []
for i in range(1, 4):
data_list.append({
'ra': 111.111 + i,
'decl': 11.11 + i,
'ra_fit_err': 0.01,
'decl_fit_err': 0.01,
'i_peak': 10. * i,
'i_peak_err': 0.1,
'error_radius': 10.0,
'fit_type': 1,
# x=0.11, y=0.22, z=0.33, det_sigma=11.1, zone=i
})
# Insert the 3 sources in each image, while further varying the flux
for i, image in enumerate(images):
# Create the "source finding results"
sources = []
for data in data_list:
source = db_subs.example_extractedsource_tuple(
ra=data['ra'],
dec=data['decl'],
ra_fit_err=data['ra_fit_err'],
dec_fit_err=data['decl_fit_err'],
peak=data['i_peak'] * (1 + i),
peak_err=data['i_peak_err'],
flux=data['i_peak'] * (1 + i),
flux_err=data['i_peak_err'],
fit_type=data['fit_type'])
sources.append(source)
# Insert the sources
insert_extracted_sources(image._id, sources)
# Run the association for each list of source for an image
associate_extracted_sources(image._id,
deRuiter_r=3.7,
new_source_sigma_margin=3)
# updates the dataset and its set of images
self.dataset.update()
self.dataset.update_images()
# update the images and their sets of sources
for image in self.dataset.images:
image.update()
image.update_sources()
# Now pick any image, select the first source (smallest RA)
# and extract its light curve
# TODO: aaarch this is so ugly. Because this a set we need to pop it.
sources = self.dataset.images.pop().sources
#sources = self.dataset.images[-1].sources
sources = sorted(sources, key=attrgetter('ra'))
extracted_source = sources[0].id
lightcurve = tkp.db.general.lightcurve(extracted_source)
def test_lightsurface(self):
images = []
# make 4 * 5 images with different frequencies and date
for frequency in [80e6, 90e6, 100e6, 110e6, 120e6]:
for day in [3, 4, 5, 6]:
img_data = db_subs.example_dbimage_data_dict(
taustart_ts=datetime.datetime(2010, 3, day),
freq_eff = frequency
)
image = Image(dataset=self.dataset, data=img_data)
images.append(image)
# 3 sources per image, with different coordinates & flux
data_list = []
for i in range(1, 4):
data_list.append({
'ra': 111.111 + i,
'decl': 11.11 + i,
'ra_fit_err': 0.01,
'decl_fit_err': 0.01,
'i_peak': 10.*i,
'i_peak_err': 0.1,
'error_radius': 10.0,
'fit_type': 1,
# x=0.11, y=0.22, z=0.33, det_sigma=11.1, zone=i
})
# Insert the 3 sources in each image, while further varying the flux
for i, image in enumerate(images):
# Create the "source finding results"
sources = []
for data in data_list:
source = db_subs.example_extractedsource_tuple(
ra=data['ra'], dec=data['decl'],
ra_fit_err=data['ra_fit_err'],
dec_fit_err= data['decl_fit_err'],
peak = data['i_peak']*(1+i),
peak_err = data['i_peak_err'],
flux = data['i_peak']*(1+i),
flux_err = data['i_peak_err'],
fit_type=data['fit_type']
)
sources.append(source)
# Insert the sources
insert_extracted_sources(image._id, sources)
# Run the association for each list of source for an image
associate_extracted_sources(image._id, deRuiter_r=3.7,
new_source_sigma_margin=3)
# updates the dataset and its set of images
self.dataset.update()
self.dataset.update_images()
# update the images and their sets of sources
for image in self.dataset.images:
image.update()
image.update_sources()
# Now pick any image, select the first source (smallest RA)
# and extract its light curve
# TODO: aaarch this is so ugly. Because this a set we need to pop it.
sources = self.dataset.images.pop().sources
#sources = self.dataset.images[-1].sources
sources = sorted(sources, key=attrgetter('ra'))
extracted_source = sources[0].id
lightcurve = tkp.db.general.lightcurve(extracted_source)