def test_alt_unit(self):
layer = self.client.layers.add_table_layer(table=self.table)
# Using a string
layer.alt_unit = 'm'
# Using a string of an imperial unit
layer.alt_unit = 'inch'
# Using an astropy unit
layer.alt_unit = u.km
# Using a unit that is equal but not identical to one of the accepted ones
layer.alt_unit = u.def_unit('same_as_km', 1000 * u.m)
# Using an invalid string
with pytest.raises(ValueError) as exc:
layer.alt_unit = 'banana'
assert exc.value.args[0].strip().startswith(
"'banana' did not parse as unit: At col 0, banana is not a valid unit."
)
# Using an unsupported unit
with pytest.raises(ValueError) as exc:
layer.alt_unit = u.kg
assert exc.value.args[0].strip(
) == "alt_unit should be one of AU/Mpc/ft/inch/km/lyr/m/mi/pc"
# Using a non-equal custom unit
with pytest.raises(ValueError) as exc:
layer.alt_unit = u.def_unit('same_as_half_km', 500 * u.m)
assert exc.value.args[0].strip(
) == "alt_unit should be one of AU/Mpc/ft/inch/km/lyr/m/mi/pc"
def setup_registered_units():
"""
Function to setup predefined units.
This should run once when the module
is imported.
"""
global FORMATTED_UNITS
# Load up configurations from yaml file
with open(DEFAULT_FLUX_UNITS_CONFIGS, 'r') as yamlfile:
cfg = yaml.load(yamlfile)
# Define and add new units to astropy
for new_unit_key in cfg["new_units"]:
new_unit = cfg["new_units"][new_unit_key]
try:
u.Unit(new_unit["name"])
except ValueError:
if "base" in new_unit:
new_astropy_unit = u.def_unit(new_unit["name"],
u.Unit(new_unit["base"]))
else:
new_astropy_unit = u.def_unit(new_unit["name"])
register_new_unit(new_astropy_unit)
new_physical_types = [[(u.Jy / u.degree**2), 'SFD_over_solid_angle'],
[(u.Jy / u.pix), 'SFD_over_pix']]
for model_unit, name in new_physical_types:
try:
u.def_physical_type(model_unit, name)
except ValueError:
continue
FORMATTED_UNITS = cfg["formatted_units"]
def test_lon_unit(self):
layer = self.client.layers.add_table_layer(table=self.table)
# Using a string
layer.lon_unit = 'deg'
# Using an astropy unit
layer.lon_unit = u.hourangle
# Using a unit that is equal but not identical to one of the accepted ones
layer.lon_unit = u.def_unit('same_as_deg', 3600 * u.arcsec)
# Using an invalid string
with pytest.raises(ValueError) as exc:
layer.lon_unit = 'banana'
assert exc.value.args[0].strip().startswith(
"'banana' did not parse as unit: At col 0, banana is not a valid unit."
)
# Using an unsupported unit
with pytest.raises(ValueError) as exc:
layer.lon_unit = u.kg
assert exc.value.args[0].strip(
) == "lon_unit should be one of deg/h/hourangle"
# Using a non-equal custom unit
with pytest.raises(ValueError) as exc:
layer.lon_unit = u.def_unit('same_as_arcmin', 60 * u.arcsec)
assert exc.value.args[0].strip(
) == "lon_unit should be one of deg/h/hourangle"
def __init__(self, cubeviz_layout=None):
self.cubeviz_layout = cubeviz_layout
# Load up configurations from yaml file
with open(DEFAULT_FLUX_UNITS_CONFIGS, 'r') as yamlfile:
cfg = yaml.load(yamlfile)
# Define and add new units to astropy
for new_unit_key in cfg["new_units"]:
new_unit = cfg["new_units"][new_unit_key]
try:
u.Unit(new_unit["name"])
except ValueError:
if "base" in new_unit:
new_astropy_unit = u.def_unit(new_unit["name"], u.Unit(new_unit["base"]))
else:
new_astropy_unit = u.def_unit(new_unit["name"])
self.register_new_unit(new_astropy_unit)
self._define_new_physical_types()
# Formatted units
self.formatted_units = cfg["formatted_units"]
self.data = None
self.wcs = None
self._components = {}
def set_units(self,
velocity_in_cm_per_s=1e5,
lenght_in_cm=3.085678e24,
mass_in_g=1.989e43):
"""Set gadget internal units
Args:
velocity_in_cm_per_s: unit velocity un cm/s
lenght_in_cm: unit lenght in cm
mass_in_g: unit mass in grams
Note:
Default values result in:
- velocity units in km/s
- lenght units in kpc/h
- mass units in 1e10 * solMass/h
Where H0 = 100 * h Km s^{-1} Mpc^{-1} is the Hubble constant
"""
unit_velocity_in_cm_per_s = velocity_in_cm_per_s * u.cm / u.s
unit_lenght_in_cm = lenght_in_cm * u.cm
unit_mass_in_g = mass_in_g * u.gram
h = self.h
vel = u.def_unit("gadget_velocity",
unit_velocity_in_cm_per_s.to("km/s"))
lenght = u.def_unit("gadget_lenght", unit_lenght_in_cm.to("kpc") / h)
mass = u.def_unit("gadget_mass", unit_mass_in_g.to("solMass") / h)
time = lenght / vel
self.gadget_velocity = vel
self.gadget_lenght = lenght
self.gadget_mass = mass
self.gadget_time = time
self.gadget_sfr = mass / time
def __init__(self, _frequency, luminosity):
# Check for correct inputs
if not _frequency.shape[0] == luminosity.shape[0] + 1:
raise ValueError(
"shape of '_frequency' and 'luminosity' are not compatible"
f": '{_frequency.shape[0]}' and '{luminosity.shape[0]}'"
)
self._frequency = _frequency.to("Hz", u.spectral())
self.luminosity = luminosity.to("erg / s")
l_nu_unit = u.def_unit("erg\ s^{-1}\ Hz^{-1}", u.Unit("erg/(s Hz)"))
l_lambda_unit = u.def_unit(
"erg\ s^{-1}\ \\AA^{-1}", u.Unit("erg/(s AA)")
)
self.frequency = self._frequency[:-1]
self.delta_frequency = self._frequency[1] - self._frequency[0]
self.wavelength = self.frequency.to("angstrom", u.spectral())
self.luminosity_density_nu = (
self.luminosity / self.delta_frequency
).to(l_nu_unit)
self.luminosity_density_lambda = self.f_nu_to_f_lambda(
self.luminosity_density_nu,
).to(l_lambda_unit)
def setup_registered_units():
"""
Function to setup predefined units.
This should run once when the module
is imported.
"""
global FORMATTED_UNITS
# Load up configurations from yaml file
with open(DEFAULT_FLUX_UNITS_CONFIGS, 'r') as yamlfile:
cfg = yaml.load(yamlfile)
# Define and add new units to astropy
for new_unit_key in cfg["new_units"]:
new_unit = cfg["new_units"][new_unit_key]
try:
u.Unit(new_unit["name"])
except ValueError:
if "base" in new_unit:
new_astropy_unit = u.def_unit(new_unit["name"], u.Unit(new_unit["base"]))
else:
new_astropy_unit = u.def_unit(new_unit["name"])
register_new_unit(new_astropy_unit)
new_physical_types = [
[(u.Jy / u.degree ** 2), 'SFD_over_solid_angle'],
[(u.Jy / u.pix), 'SFD_over_pix']
]
for model_unit, name in new_physical_types:
try:
u.def_physical_type(model_unit, name)
except ValueError:
continue
FORMATTED_UNITS = cfg["formatted_units"]
def generateSpecialUnits(qMass, qR, gR):
linearRg = (qMass.to('kg') * const.G / const.c / const.c).to('m')
angleRg = linearRg / cosmo.angular_diameter_distance(qR)
rgUnit = u.def_unit('r_g', angleRg.value * u.rad)
thetaE = 4 * const.G * u.Quantity(0.5, 'solMass').to('kg') * _scaleFactor(
qR, gR) / const.c / const.c
thetaEUnit = u.def_unit('theta_E', math.sqrt(thetaE.value) * u.rad)
return [thetaEUnit, rgUnit]
def __init__(self,fp=None,pool=None,length_unit=1.0*kpc,mass_unit=1.0e10*Msun,velocity_unit=1.0*km/s,header_kwargs=dict()):
self.pool = pool
self._length_unit = length_unit.to(cm).value
self._mass_unit = mass_unit.to(g).value
self._velocity_unit = velocity_unit.to(cm/s).value
if fp is not None:
self.fp = fp
#Load the header
self._header = self.getHeader(**header_kwargs)
#Check that header has been loaded correctly
self._check_header()
#Hubble parameter
h = self._header["h"]
#Define the Mpc/h, and kpc/h units for convenience
if h>0.0:
self.kpc_over_h = def_unit("kpc/h",kpc/self._header["h"])
self.Mpc_over_h = def_unit("Mpc/h",Mpc/self._header["h"])
#Scale box to kpc/h
self._header["box_size"] *= self.kpc_over_h
#Convert to Mpc/h
self._header["box_size"] = self._header["box_size"].to(self.Mpc_over_h)
#Read in the comoving distance
if "comoving_distance" in self._header:
self._header["comoving_distance"] = (self._header["comoving_distance"] / 1.0e3) * self.Mpc_over_h
else:
self._header["box_size"] *= kpc
logging.debug("Warning! Hubble parameter h is zero!!")
#Scale masses to correct units
if h>0.0:
self._header["masses"] *= (self._mass_unit / self._header["h"])
self._header["masses"] = (self._header["masses"]*g).to(Msun)
#Scale Hubble parameter to correct units
self._header["H0"] = self._header["h"] * 100 * km / (s*Mpc)
#Update the dictionary with the number of particles per side
self._header["num_particles_total_side"] = int(np.round(self._header["num_particles_total"]**(1/3)))
#Once all the info is available, add a wCDM instance as attribute to facilitate the cosmological calculations
if h>0.0:
self.cosmology = w0waCDM(H0=self._header["H0"],Om0=self._header["Om0"],Ode0=self._header["Ode0"],w0=self._header["w0"],wa=self._header["wa"])
#Set particle number limits that this instance will handle
self.setLimits()
def test_load_w_quantity(self):
try:
from astropy import units as u
from pvl.decoder import OmniDecoder
pvl_file = 'tests/data/pds3/units1.lbl'
km_upper = u.def_unit('KM', u.km)
m_upper = u.def_unit('M', u.m)
u.add_enabled_units([km_upper, m_upper])
label = pvl.load(pvl_file,
decoder=OmniDecoder(quantity_cls=u.Quantity))
self.assertEqual(label['FLOAT_UNIT'], u.Quantity(0.414, 'KM'))
except ImportError:
pass
def setup_bases(self):
"""Set the standard, non-dimensional bases"""
temperature_unit = u.def_unit("Box-delta-T", np.abs(self.deltaT))
length_unit = u.def_unit("Box-D", self.depth)
viscosity_unit = u.def_unit("kappa", self.primary_viscosity)
time_unit = length_unit**2 / viscosity_unit
self.add_bases("nondimensional", set([temperature_unit, length_unit, viscosity_unit, time_unit]))
temperature_unit = self.deltaT.unit
length_unit = self.depth.unit
time_unit = type(self).Time.unit
viscosity_unit = length_unit**2 / time_unit
self.add_bases("standard", set([temperature_unit, length_unit, time_unit, viscosity_unit]))
def test_represents():
assert u.m.represents is u.m
assert u.km.represents.scale == 1000.
assert u.km.represents.bases == [u.m]
assert u.Ry.scale == 1.0 and u.Ry.bases == [u.Ry]
assert_allclose(u.Ry.represents.scale, 13.605692518464949)
assert u.Ry.represents.bases == [u.eV]
bla = u.def_unit('bla', namespace=locals())
assert bla.represents is bla
blabla = u.def_unit('blabla', 10 * u.hr, namespace=locals())
assert blabla.represents.scale == 10.
assert blabla.represents.bases == [u.hr]
assert blabla.decompose().scale == 10 * 3600
assert blabla.decompose().bases == [u.s]
def test_represents():
assert u.m.represents is u.m
assert u.km.represents.scale == 1000.
assert u.km.represents.bases == [u.m]
assert u.Ry.scale == 1.0 and u.Ry.bases == [u.Ry]
assert_allclose(u.Ry.represents.scale, 13.605692518464949)
assert u.Ry.represents.bases == [u.eV]
bla = u.def_unit('bla', namespace=locals())
assert bla.represents is bla
blabla = u.def_unit('blabla', 10 * u.hr, namespace=locals())
assert blabla.represents.scale == 10.
assert blabla.represents.bases == [u.hr]
assert blabla.decompose().scale == 10 * 3600
assert blabla.decompose().bases == [u.s]
def __init__(self, scdata, inputs, params=None, dphi=1*u.deg, **kwargs):
"""Initializes the LOSResult and runs the model if necessary"""
if params is None:
params = {'quantity': 'radiance'}
else:
pass
scdata.set_frame('Model')
super().__init__(inputs, params)
# Basic information
self.species = scdata.species
self.query = scdata.query
self.type = 'LineOfSight'
self.dphi = dphi.to(u.rad).value
self._oedge = np.min([self.inputs.options.outeredge*2, 100])
self.fitted = self.inputs.options.fitted
nspec = len(scdata)
self.radiance = pd.Series(np.zeros(nspec), index=scdata.data.index)
self.radiance_unit = u.def_unit('kR', 1e3*u.R)
self.sourcemap = None
self.modelfiles = None
self.goodness_of_fit = None
self.mask = None
self.masking = kwargs.get('masking', None)
self.fit_method = kwargs.get('fit_method', None)
self.label = kwargs.get('label', 'LOSResult')
if self.fitted:
self.unfit_outid = None
self.unfit_outputfiles = None
else:
pass
def _get_unit(cls, t):
# match as normal
try:
return cls._parse_unit(t.value)
except ValueError as exc:
name = t.value
sname = name[:-1] if name.endswith('s') else ''
# parse alternative units from the error message
match = cls.re_closest_unit.search(str(exc))
try: # split 'A, B, or C' -> ['A', 'B', 'C']
alts = cls.re_closest_unit_delim.split(match.groups()[0])[::2]
except AttributeError:
alts = []
alts = list(set(alts))
# match uppercase to titled (e.g. MPC -> Mpc)
if name.title() in alts:
alt = name.title()
# match titled unit to lower-case (e.g. Amp -> amp)
elif name.lower() in alts:
alt = name.lower()
# match plural to singular (e.g. meters -> meter)
elif sname in alts:
alt = sname
elif sname.lower() in alts:
alt = sname.lower()
else:
warnings.warn('{0} Mathematical operations using this unit '
'should work, but conversions to other units '
'will not.'.format(str(exc).rstrip(' ')),
category=units.UnitsWarning)
return units.def_unit(name, doc='Unrecognized unit')
return cls._parse_unit(alt)
def get_y_units(y_data, filename, header):
"""finds flux/reflectance units
inputs: y_data, spectrum file
outputs: scaled flux with Units
"""
y_factor = 1
if 'BUNIT' in header:
try:
y_units = u.Unit(header['BUNIT'])
except ValueError:
print("Could not parse flux units from header.")
elif "ctiostan" in filename and '.dat' in filename: # from ESO aaareadme.ctio
y_units = u.erg / (u.cm**2) / u.s / u.AA
y_factor = 10**16
elif .001 < np.median(y_data) < 10: # Probably Normalized
y_units = u.def_unit("Normalized_Reflectance",
u.dimensionless_unscaled)
elif '_2df_ex.fits' in filename: # from FLOYDS
y_factor = 10**20
y_units = u.erg / (u.cm**2) / u.s / u.AA
else:
print("Could not parse flux units from file. Assuming erg/cm^2/s/A")
y_units = u.erg / (u.cm**2) / u.s / u.AA
yyy = np.array(y_data)
flux = ((yyy / y_factor) * y_units)
return flux
def astro_dist(mass):
"""
Function for turning distance into astronomical perspective.
"""
value = (G.value * mass) / (c.value ** 2)
astro_dist = u.def_unit("astro-m(GM/c2)", u.m / value)
return astro_dist
def astro_sec(mass):
"""
Function for turning time into astronomical perspective.
"""
value = (G.value * mass) / (c.value ** 3)
astro_sec = u.def_unit("astro-sec(GM/c3)", u.s / value)
return astro_sec
def test_with_custom_units_qtable(self, tmpdir):
# Test only for QTable - for Table's Column, new units are dropped
# (as is checked in test_write_drop_nonstandard_units).
filename = str(tmpdir.join('test_with_units.fits'))
unit = u.def_unit('bandpass_sol_lum')
t = QTable()
t['l'] = np.ones(5) * unit
with pytest.warns(AstropyUserWarning) as w:
t.write(filename, overwrite=True)
assert len(w) == 1
assert 'bandpass_sol_lum' in str(w[0].message)
# Just reading back, the data is fine but the unit is not recognized.
with pytest.warns(u.UnitsWarning,
match="'bandpass_sol_lum' did not parse") as w:
t2 = QTable.read(filename)
assert len(w) == 1
assert isinstance(t2['l'].unit, u.UnrecognizedUnit)
assert str(t2['l'].unit) == 'bandpass_sol_lum'
assert np.all(t2['l'].value == t['l'].value)
# But if we enable the unit, it should be recognized.
with u.add_enabled_units(unit):
t3 = QTable.read(filename)
assert t3['l'].unit is unit
assert equal_data(t3, t)
# Regression check for #8897; write used to fail when a custom
# unit was enabled.
with pytest.warns(AstropyUserWarning):
t3.write(filename, overwrite=True)
def test_auto_lon_unit(self):
self.table['longitude'] = [1, 4, 5] * u.hour
self.table['longitude2'] = [1, 4, 5] * u.def_unit(
'same_as_deg', 3600 * u.arcsec)
self.table['flux'].unit = u.kg
layer = self.client.layers.add_table_layer(table=self.table)
assert layer.lon_att == 'ra'
assert layer.lon_unit is u.deg
layer.lon_att = 'longitude'
assert layer.lon_unit is u.hour
layer.lon_att = 'longitude2'
assert layer.lon_unit is u.deg
expected_warning = (
'Column flux has units of kg but this is not a '
'valid unit of longitude - set the unit directly with '
'lon_unit')
with pytest.warns(UserWarning, match=expected_warning):
layer.lon_att = 'flux'
def __init__(self, coords):
valid_coords = ['KRTP', 'KSM', 'KSO', 'RTN']
if coords not in valid_coords:
raise ValueError('coords must be one of {}'.format(valid_coords))
self.coords = coords
Rs = u.def_unit('saturnRad', 60268 * u.km)
if (coords == 'KRTP'):
self.units = OrderedDict([('Bx', u.nT), ('By', u.nT), ('Bz', u.nT),
('X', Rs), ('|B|', u.nT),
('Y', u.deg),
('Z', u.deg),
('Local hour', u.dimensionless_unscaled),
('n points', u.dimensionless_unscaled)])
if (coords == 'RTN'):
self.units = OrderedDict([('Bx', u.nT), ('By', u.nT), ('Bz', u.nT),
('X', u.AU), ('Y', u.AU), ('Z', u.AU),
('|B|', u.nT),
('Local hour', u.dimensionless_unscaled),
('n points', u.dimensionless_unscaled)])
if (coords == 'KSM' or coords == 'KSO'):
self.units = OrderedDict([('Bx', u.nT), ('By', u.nT), ('Bz', u.nT),
('X', Rs), ('Y', Rs), ('Z', Rs),
('|B|', u.nT),
('Local hour', u.dimensionless_unscaled),
('n points', u.dimensionless_unscaled)])
def test_read_cdf_empty_variable():
# This tests that:
# - A CDF file with an empty column can be read
# - Unknown unit handling works as expected
result = sunpy.net.Fido.search(a.Time('2020-01-01', '2020-01-02'),
a.cdaweb.Dataset('AC_H6_SWI'))
filename = Fido.fetch(result[0, 0])
# Temporarily reset sunpy.io.cdf registry of known unit conversions
import sunpy.io.cdf as sunpy_cdf
known_units = sunpy_cdf._known_units
sunpy_cdf._known_units = {}
with pytest.warns(SunpyUserWarning, match='Assigning dimensionless units'):
ts = sunpy.timeseries.TimeSeries(filename)
assert ts.quantity('nH').unit == u.dimensionless_unscaled
# Put back known unit registry, and check that units are recognised
sunpy_cdf._known_units = known_units
ts = sunpy.timeseries.TimeSeries(filename)
assert ts.quantity('nH').unit == u.cm**-3
# Reset again to check that registring units via. astropy works too
sunpy_cdf._known_units = {}
u.add_enabled_units([u.def_unit('#/cm^3', represents=u.cm**-3)])
ts = sunpy.timeseries.TimeSeries(filename)
assert ts.quantity('nH').unit == u.cm**-3
sunpy_cdf._known_units = known_units
def __init__(self,cosmoModel=cosmology.WMAP9):
assert isinstance(cosmoModel,cosmology.FLRW),"cosmoModel should be a valid astropy cosmology instance!"
self.cosmoModel = cosmoModel
#Define also the Mpc/h units for convenience
self.Mpc_over_h = def_unit("Mpc/h",Mpc/self.cosmoModel.h)
def aspcapStar_loader(file_obj, **kwargs):
"""
Loader for APOGEE aspcapStar files.
Parameters
----------
file_obj: str or file-like
FITS file name or object (provided from name by Astropy I/O Registry).
Returns
-------
data: Spectrum1D
The spectrum that is represented by the data in this table.
"""
with read_fileobj_or_hdulist(file_obj, **kwargs) as hdulist:
header = hdulist[0].header
meta = {'header': header}
wcs = WCS(hdulist[1].header)
data = hdulist[1].data # spectrum in the first extension
unit = def_unit('arbitrary units')
uncertainty = StdDevUncertainty(hdulist[2].data)
# dispersion from the WCS but convert out of logspace
dispersion = 10**wcs.all_pix2world(np.arange(data.shape[0]), 0)[0]
dispersion_unit = Unit('Angstrom')
return Spectrum1D(data=data * unit,
uncertainty=uncertainty,
spectral_axis=dispersion * dispersion_unit,
meta=meta,
wcs=wcs)
def get_y_units(y_data, filename, y_error=[]):
"""finds flux/reflectance units
inputs: y_data, spectrum file
outputs: scaled flux with Units
"""
y_factor = 1
if "ctiostan" in filename and '.dat' in filename: # from ESO aaareadme.ctio
y_units = u.erg/(u.cm**2)/u.s/u.AA
y_factor = 10**16
elif .001 < np.median(y_data) < 10: # Probably Normalized
y_units = u.def_unit("Normalized_Reflectance", u.dimensionless_unscaled)
elif '_2df_ex.fits' in filename: # from FLOYDS
y_factor = 10**20
y_units = u.erg/(u.cm**2)/u.s/u.AA
else:
logger.warning("Could not parse flux units from file. Assuming erg/cm^2/s/A")
y_units = u.erg/(u.cm**2)/u.s/u.AA
yyy = np.array(y_data)
err = np.array(y_error)
flux = ((yyy / y_factor) * y_units)
error = ((err / y_factor) * y_units)
return flux, error
def cdf_dict(unit_string):
"""
Method to obtain the unit denoted by the strings inside the CDF files in
the UNIT attribute.
"""
ionic_charge = u.def_unit('Charged State', 1.6021766 * (10**-19) * u.C)
units = OrderedDict([('ratio', u.dimensionless_unscaled),
('Unitless', u.dimensionless_unscaled),
('unitless', u.dimensionless_unscaled),
('Spacecraft', u.dimensionless_unscaled),
('microW m^-2', u.mW * u.m**-2), ('years', u.yr),
('days', u.d), ('#/cc', u.cm**-3),
('#/cm^3', u.cm**-3), ('cm^{-3}', u.cm**-3),
('particles cm^-3', u.cm**-3),
('n/cc (from moments)', u.cm**-3),
('n/cc (from fits)', u.cm**-3),
('km/sec (from fits)', u.km / u.s),
('km/sec (from moments)', u.km / u.s),
('ionic charge', u.electron),
('earth radii', u.earthRad), ('Re', u.earthRad),
('Degrees', u.deg), ('degrees', u.deg),
('deg (from fits)', u.deg),
('deg (from moments)', u.deg),
('#/{cc*(cm/s)^3}', (u.cm**3 * (u.cm / u.s)**3)**-1),
('sec', u.s), ('seconds', u.s), ('nT GSE', u.nT),
('nT GSM', u.nT), ('nT DSL', u.nT), ('nT SSL', u.nT),
('msec', u.ms), ('ionic charge', ionic_charge)])
try:
return units[unit_string]
except KeyError:
return None
def mkwvl(quantity, base=u.um):
"""Generate a new Wavelength unit.
Parameters
----------
quantity : `float` or `astropy.units.unit`
number of (base) for the wavelength, e.g. quantity=632.8 with base=u.nm for HeNe.
if an astropy unit, simply returned by this function
base : `astropy.units.Unit`
base unit, e.g. um or nm
Returns
-------
`astropy.units.Unit`
new Unit for appropriate wavelength
"""
if quantity is None:
return quantity
elif not isinstance(quantity, u.Unit):
return u.def_unit(['wave', 'wavelength'],
quantity * base,
format={
'latex': r'\lambda',
'unicode': 'λ'
})
else:
return quantity
def test_auto_alt_unit(self):
self.table['altitude'] = [1, 4, 5] * u.au
self.table['altitude2'] = [1, 4, 5] * u.def_unit(
'same_as_km', 1000 * u.m)
self.table['flux'].unit = u.kg
layer = self.client.layers.add_table_layer(table=self.table)
assert layer.alt_att == ''
assert layer.alt_unit is None
layer.alt_att = 'altitude'
assert layer.alt_unit is u.au
layer.alt_att = 'altitude2'
assert layer.alt_unit is u.km
expected_warning = (
'Column flux has units of kg but this is not a '
'valid unit of altitude - set the unit directly with '
'alt_unit')
with pytest.warns(UserWarning, match=expected_warning):
layer.alt_att = 'flux'
def setHeaderInfo(self,Om0=0.26,Ode0=0.74,w0=-1.0,wa=0.0,h=0.72,redshift=100.0,box_size=15.0*u.Mpc/0.72,flag_cooling=0,flag_sfr=0,flag_feedback=0,flag_stellarage=0,flag_metals=0,flag_entropy_instead_u=0,masses=np.array([0,1.03e10,0,0,0,0])*u.Msun,num_particles_file_of_type=None,npartTotalHighWord=np.zeros(6,dtype=np.uint32)):
"""
Sets the header info in the snapshot to write
"""
if num_particles_file_of_type is None:
num_particles_file_of_type = np.array([0,1,0,0,0,0],dtype=np.int32) * self.positions.shape[0]
assert num_particles_file_of_type.sum()==self.positions.shape[0],"The total number of particles must match!!"
assert box_size.unit.physical_type=="length"
assert masses.unit.physical_type=="mass"
#Create the header
self._header = Gadget2Header()
#Fill in
self._header["Om0"] = Om0
self._header["Ode0"] = Ode0
self._header["w0"] = w0
self._header["wa"] = wa
self._header["h"] = h
self._header["H0"] = 100.0*h*u.km/(u.s*u.Mpc)
self._header["redshift"] = redshift
self._header["scale_factor"] = 1.0 / (1.0 + redshift)
self._header["box_size"] = box_size
self._header["flag_cooling"] = flag_cooling
self._header["flag_sfr"] = flag_sfr
self._header["flag_feedback"] = flag_feedback
self._header["flag_stellarage"] = flag_stellarage
self._header["flag_metals"] = flag_metals
self._header["flag_entropy_instead_u"] = flag_entropy_instead_u
self._header["masses"] = masses
self._header["num_particles_file_of_type"] = num_particles_file_of_type
self._header["num_particles_file"] = num_particles_file_of_type.sum()
self._header["num_particles_total_of_type"] = num_particles_file_of_type
self._header["num_particles_total"] = num_particles_file_of_type.sum()
self._header["npartTotalHighWord"] = npartTotalHighWord
#Define the kpc/h and Mpc/h units for convenience
self.kpc_over_h = u.def_unit("kpc/h",u.kpc/self._header["h"])
self.Mpc_over_h = u.def_unit("Mpc/h",u.Mpc/self._header["h"])
#Compute the comoving distance according to the model
cosmo = w0waCDM(H0=100.0*h,Om0=Om0,Ode0=Ode0,w0=w0,wa=wa)
self._header["comoving_distance"] = cosmo.comoving_distance(redshift).to(self.Mpc_over_h)
def setup_bases(self):
"""Set the standard, non-dimensional bases"""
temperature_unit = u.def_unit("Box-delta-T", np.abs(self.deltaT))
length_unit = u.def_unit("Box-D", self.depth)
viscosity_unit = u.def_unit("kappa", self.primary_viscosity)
time_unit = length_unit**2 / viscosity_unit
self.add_bases(
"nondimensional",
set([temperature_unit, length_unit, viscosity_unit, time_unit]))
temperature_unit = self.deltaT.unit
length_unit = self.depth.unit
time_unit = type(self).Time.unit
viscosity_unit = length_unit**2 / time_unit
self.add_bases(
"standard",
set([temperature_unit, length_unit, time_unit, viscosity_unit]))
def static_theta_E(z_s, z_l):
dS = Cosmic.cosmology.angular_diameter_distance(z_s)
dL = Cosmic.cosmology.angular_diameter_distance(z_l)
dLS = Cosmic.cosmology.angular_diameter_distance_z1z2(z_l, z_s)
Msun = 1 * u.solMass
tmp = (4 * const.G * Msun / const.c / const.c) * (dL * dLS / dS)
ret = (tmp**0.5 / dL).to('').value
return u.def_unit('theta_E', ret * u.rad)
def _generate_unit_names():
from astropy import units as u
names = {}
deprecated_names = set()
bases = [
'A', 'C', 'cd', 'eV', 'F', 'g', 'H', 'Hz', 'J',
'Jy', 'K', 'lm', 'lx', 'm', 'mol', 'N', 'ohm', 'Pa',
'pc', 'rad', 's', 'S', 'sr', 'T', 'V', 'W', 'Wb'
]
deprecated_bases = []
prefixes = [
'y', 'z', 'a', 'f', 'p', 'n', 'u', 'm', 'c', 'd',
'', 'da', 'h', 'k', 'M', 'G', 'T', 'P', 'E', 'Z', 'Y'
]
for base in bases + deprecated_bases:
for prefix in prefixes:
key = prefix + base
if keyword.iskeyword(key):
continue
names[key] = getattr(u, key)
for base in deprecated_bases:
for prefix in prefixes:
deprecated_names.add(prefix + base)
simple_units = [
'angstrom', 'arcmin', 'arcsec', 'AU', 'barn', 'bin',
'byte', 'chan', 'count', 'day', 'deg', 'erg', 'G',
'h', 'lyr', 'mag', 'min', 'photon', 'pixel',
'voxel', 'yr'
]
for unit in simple_units:
names[unit] = getattr(u, unit)
# Create a separate, disconnected unit for the special case of
# Crab and mCrab, since OGIP doesn't define their quantities.
Crab = u.def_unit(['Crab'], prefixes=False, doc='Crab (X-ray flux)')
mCrab = u.Unit(10 ** -3 * Crab)
names['Crab'] = Crab
names['mCrab'] = mCrab
deprecated_units = ['Crab', 'mCrab']
for unit in deprecated_units:
deprecated_names.add(unit)
# Define the function names, so we can parse them, even though
# we can't use any of them (other than sqrt) meaningfully for
# now.
functions = [
'log', 'ln', 'exp', 'sqrt', 'sin', 'cos', 'tan', 'asin',
'acos', 'atan', 'sinh', 'cosh', 'tanh'
]
for name in functions:
names[name] = name
return names, deprecated_names, functions
def _generate_unit_names():
from astropy import units as u
names = {}
deprecated_names = set()
bases = [
'A', 'C', 'cd', 'eV', 'F', 'g', 'H', 'Hz', 'J',
'Jy', 'K', 'lm', 'lx', 'm', 'mol', 'N', 'ohm', 'Pa',
'pc', 'rad', 's', 'S', 'sr', 'T', 'V', 'W', 'Wb'
]
deprecated_bases = []
prefixes = [
'y', 'z', 'a', 'f', 'p', 'n', 'u', 'm', 'c', 'd',
'', 'da', 'h', 'k', 'M', 'G', 'T', 'P', 'E', 'Z', 'Y'
]
for base in bases + deprecated_bases:
for prefix in prefixes:
key = prefix + base
if keyword.iskeyword(key):
continue
names[key] = getattr(u, key)
for base in deprecated_bases:
for prefix in prefixes:
deprecated_names.add(prefix + base)
simple_units = [
'angstrom', 'arcmin', 'arcsec', 'AU', 'barn', 'bin',
'byte', 'chan', 'count', 'day', 'deg', 'erg', 'G',
'h', 'lyr', 'mag', 'min', 'photon', 'pixel',
'voxel', 'yr'
]
for unit in simple_units:
names[unit] = getattr(u, unit)
# Create a separate, disconnected unit for the special case of
# Crab and mCrab, since OGIP doesn't define their quantities.
Crab = u.def_unit(['Crab'], prefixes=False, doc='Crab (X-ray flux)')
mCrab = u.Unit(10 ** -3 * Crab)
names['Crab'] = Crab
names['mCrab'] = mCrab
deprecated_units = ['Crab', 'mCrab']
for unit in deprecated_units:
deprecated_names.add(unit)
# Define the function names, so we can parse them, even though
# we can't use any of them (other than sqrt) meaningfully for
# now.
functions = [
'log', 'ln', 'exp', 'sqrt', 'sin', 'cos', 'tan', 'asin',
'acos', 'atan', 'sinh', 'cosh', 'tanh'
]
for name in functions:
names[name] = name
return names, deprecated_names, functions
def t_UNIT(self, t):
r'<[\w*^\-/]+>'
import astropy.units as u
# most astropy units are lower-case versions of the PDS3 units
unit = t.value[1:-1].lower()
# but not all
if unit in self.unit_translate:
unit = self.unit_translate[unit]
_degC = u.def_unit('degC', u.deg_C)
_degc = u.def_unit('degc', _degC)
_w = u.def_unit('w', u.W)
u.add_enabled_units([_degC,_degc,_w])
t.value = u.Unit(unit)
return t
def calculateAvgMassEinsteinRadius(gz, qz):
avgMass = 0.247
# avgMass = 0.20358470458734301
dL = cosmo.angular_diameter_distance(gz).to('m')
dS = cosmo.angular_diameter_distance(qz).to('m')
dLS = cosmo.angular_diameter_distance_z1z2(gz, qz).to('m')
thetaE = 4 * const.G * u.Quantity(
avgMass, 'solMass').to('kg') * dLS / dL / dS / const.c / const.c
thetaEUnit = u.def_unit('theta_E', math.sqrt(thetaE.value) * u.rad)
return thetaEUnit
def setup_bases(self):
"""Setup the standard bases."""
super(MagnetoSystem, self).setup_bases()
magnetic_unit = u.def_unit("B0", self.B0)
mass_unit = magnetic_unit * u.A * u.s**2
self._bases["standard"][u.T.physical_type] = u.T
self._bases["standard"][u.kg.physical_type] = u.kg
self._bases["standard"][u.A.physical_type] = u.A
self._bases["nondimensional"][magnetic_unit.physical_type] = magnetic_unit
self._bases["nondimensional"][mass_unit.physical_type] = mass_unit
self._bases["nondimensional"][u.A.physical_type] = u.A
def _locally_defined_pixel_units():
"""
list of defined spectral pixel units.
:return: list of unit strings
"""
units = ["pixel"]
spaxel = u.def_unit('spaxel', u.astrophys.pix)
u.add_enabled_units(spaxel)
units.append('spaxel')
return units
def load_units(self):
"""Load all unit definitions as defined in the [units] section
"""
try:
customunits = self.nditems('units')
except configparser.NoSectionError:
return []
else:
new_ = []
for unit, b in customunits:
if b.lower() == 'dimensionless':
b = ''
new_.append(units.def_unit([unit], units.Unit(b)))
units.add_enabled_units(new_)
return new_
def _get_unit(cls, t):
# match as normal
try:
return cls._parse_unit(t.value)
except ValueError as exc:
name = t.value
sname = name[:-1] if name.endswith('s') else ''
# parse alternative units from the error message
match = cls.re_closest_unit.search(str(exc))
try: # split 'A, B, or C' -> ['A', 'B', 'C']
alts = cls.re_closest_unit_delim.split(match.groups()[0])[::2]
except AttributeError:
alts = []
alts = list(set(alts))
# match uppercase to titled (e.g. MPC -> Mpc)
if name.title() in alts:
alt = name.title()
# match titled unit to lower-case (e.g. Amp -> amp)
elif name.lower() in alts:
alt = name.lower()
# match plural to singular (e.g. meters -> meter)
elif sname in alts:
alt = sname
elif sname.lower() in alts:
alt = sname.lower()
else:
if cls.warn:
warnings.warn(
'{0} Mathematical operations using this unit should '
'work, but conversions to other units will '
'not.'.format(str(exc).rstrip(' ')),
category=units.UnitsWarning)
try: # return previously created unit
return UNRECOGNIZED_UNITS[name]
except KeyError: # or create new one now
u = UNRECOGNIZED_UNITS[name] = units.def_unit(
name, doc='Unrecognized unit')
return u
return cls._parse_unit(alt)
def aspcapStar_loader(file_name, **kwargs):
"""
Loader for APOGEE aspcapStar files.
Parameters
----------
file_name: str
The path to the FITS file
Returns
-------
data: Spectrum1D
The spectrum that is represented by the data in this table.
"""
name = os.path.basename(file_name.rstrip(os.sep)).rsplit('.', 1)[0]
hdulist = fits.open(file_name, **kwargs)
header = hdulist[0].header
meta = {'header': header}
wcs = WCS(hdulist[1].header)
data = hdulist[1].data # spectrum in the first extension
unit = def_unit('arbitrary units')
uncertainty = StdDevUncertainty(hdulist[2].data)
# dispersion from the WCS but convert out of logspace
dispersion = 10**wcs.all_pix2world(np.arange(data.shape[0]), 0)[0]
dispersion_unit = Unit('Angstrom')
hdulist.close()
return Spectrum1D(data=data * unit,
uncertainty=uncertainty,
dispersion=dispersion * dispersion_unit,
meta=meta,
wcs=wcs)
"""
from .extern._version import get_versions
__version__ = get_versions()['version']
del get_versions
# Define a few important constants
import astropy.units as u
from astropy.units import si
import astropy.constants as c
import astropy.time as time
import numpy as np
from . import utils
# light-second unit
ls = u.def_unit('ls', c.c * 1.0 * u.s)
# DM unit (pc cm^-3)
dmu = u.def_unit('dmu', u.pc*u.cm**-3)
# define equivalency for astropy units
light_second_equivalency = [(ls, si.second, lambda x: x, lambda x: x)]
dimensionless_cycles = [(u.cycle, None)]
# hourangle_second unit
hourangle_second = u.def_unit('hourangle_second', u.hourangle/np.longdouble(3600.0))
# Following are from here:
# http://ssd.jpl.nasa.gov/?constants (grabbed on 30 Dec 2013)
GMsun = 1.32712440018e20 * u.m**3/u.s**2
# Solar mass in time units (sec)
HC = H * C
SR_PER_ARCSEC2 = u.rad.to(u.arcsec) ** -2 # steradian per arcsec^2
# ------------- #
# synphot units #
# ------------- #
# Default unit of area covered by flux
AREA = u.cm * u.cm
# synphot unitless unit (using def_unit mess up arithmetic result unit string)
THROUGHPUT = u.dimensionless_unscaled
# synphot flux units
PHOTLAM = u.def_unit(
'photlam', u.photon / (u.cm**2 * u.s * u.AA),
format={'generic': 'PHOTLAM', 'console': 'PHOTLAM'})
PHOTNU = u.def_unit(
'photnu', u.photon / (u.cm**2 * u.s * u.Hz),
format={'generic': 'PHOTNU', 'console': 'PHOTNU'})
FLAM = u.def_unit(
'flam', u.erg / (u.cm**2 * u.s * u.AA),
format={'generic': 'FLAM', 'console': 'FLAM'})
FNU = u.def_unit(
'fnu', u.erg / (u.cm**2 * u.s * u.Hz),
format={'generic': 'FNU', 'console': 'FNU'})
OBMAG = u.def_unit(
'obmag', u.mag, format={'generic': 'OBMAG', 'console': 'OBMAG'})
VEGAMAG = u.def_unit(
'vegamag', u.mag, format={'generic': 'VEGAMAG', 'console': 'VEGAMAG'})
# hscimgloader.py
# ALS 2017/05/02
import numpy as np
import os
import requests
import astropy.units as u
from astropy.io import fits
import re
from ..loader import imgLoader
from ...filters import surveysetup
from ..get_credential import getCrendential
from . import hscurl
nanomaggy = u.def_unit('nanomaggy', 3.631e-6*u.Jy)
u.add_enabled_units([nanomaggy])
u.nanomaggy=nanomaggy
class hscimgLoader(imgLoader):
def __init__(self, **kwargs):
"""
hscimgLoader, child of imgLoader
download stamps from HSC DAS Quarry
download psf by either:
(iaa) call sumire to infer psf from calexp and download psf from sumire
(online) download calexp from server and infer psf locally
def test_flatten_to_known():
myunit = u.def_unit("FOOBAR_One", u.erg / u.Hz)
assert myunit.to_string('fits') == 'erg Hz-1'
myunit2 = myunit * u.bit ** 3
assert myunit2.to_string('fits') == 'bit3 erg Hz-1'
def test_flatten_impossible():
myunit = u.def_unit("FOOBAR_Two")
with u.add_enabled_units(myunit), pytest.raises(ValueError):
myunit.to_string('fits')
from glue.lal import (Cache, CacheEntry)
from .array import *
from .array2d import *
from .series import *
# define custom time-series units
try:
from astropy import (__version__ as astropyversion, units)
except ImportError:
pass
else:
from distutils.version import LooseVersion
if LooseVersion(astropyversion) < LooseVersion('0.3'):
units.def_unit(['counts'], represents=units.Unit('count'),
register=True)
units.def_unit(['strain'], represents=units.dimensionless_unscaled,
register=True)
units.def_unit(['coherence'], represents=units.dimensionless_unscaled,
register=True)
else:
units.add_enabled_units([
units.def_unit(['counts'], units.Unit('count')),
units.def_unit(['coherence'], units.dimensionless_unscaled),
units.def_unit(['strain'], units.dimensionless_unscaled),
])
__all__ = ['Array', 'Array2D', 'Series', 'Cache', 'CacheEntry']
import astropy.units as u
import astropy.constants as co
########################################################################
# Define new uv-coordinate units
lambdas = u.def_unit('lambdas', format={'format' : r'\lambda'})
klambdas = u.def_unit('kilolambdas', 1e3 * lambdas, format={'format' : r'k\lambda'})
# equivalency (from_unit, to_unit, forward, backward)
def lambdas_equivalencies(restunit):
try:
restfreq_hz = restunit.to(u.Hz, equivalencies=u.spectral())
except (AttributeError):
raise AttributeError('input \'restfreq\' should be a spectral unit.')
eq = [
(lambdas, u.s, lambda x: x/restfreq_hz, lambda x: x*restfreq_hz),
(lambdas, u.m, lambda x: x/restfreq_hz * co.c.to(u.m/u.s).value, lambda x: x/co.c.to(u.m/u.s).value * restfreq_hz),
(u.m, u.s, lambda x: x/co.c.to(u.m/u.s).value, lambda x: x*co.c.to(u.m/u.s).value),
]
return eq
########################################################################
# BINNING
def uv_bin_vector(uvdist, re, im, wt, start='zero', binsize=10, nbins=50, weighted=False):
"""
def make_table(header, section_lines):
"""
From the seperated section lines and the header, clean up the data and
convert to a QTable.
"""
meta_data = get_meta_data(header)
tables = []
for i, lines in enumerate(section_lines):
if lines:
key = list(meta_data['id'].keys())[i]
t1 = astropy.io.ascii.read(lines)
if len(t1) == 0:
col_data_types = {
# ID : <class 'str'>
'Nmbr': np.dtype('i4'),
'Location': np.dtype('U6'),
'Lo': np.dtype('i8'),
'Area': np.dtype('i8'),
'Z': np.dtype('U3'),
'LL': np.dtype('i8'),
'NN': np.dtype('i8'),
'MagType': np.dtype('S4'),
'Lat': np.dtype('i8')
}
for c in t1.itercols():
# Put data types of columns in empty table to correct types,
# or else vstack will fail.
c.dtype = col_data_types[c._name]
t1.add_column(
Column(data=None, name="ID", dtype=('S2')), index=0)
else:
t1.add_column(Column(data=[key] * len(t1), name="ID"), index=0)
tables.append(t1)
out_table = vstack(tables)
# Parse the Location column in Table 1
if 'Location' in out_table.columns:
col_lat, col_lon = parse_location(out_table['Location'])
del out_table['Location']
out_table.add_column(col_lat)
out_table.add_column(col_lon)
# Parse the Lat column in Table 3
if 'Lat' in out_table.columns:
parse_lat_col(out_table['Lat'], out_table['Latitude'])
del out_table['Lat']
# Give columns more sensible names
out_table.rename_column("Nmbr", "Number")
out_table.rename_column("NN", "Number of Sunspots")
out_table.rename_column("Lo", "Carrington Longitude")
out_table.rename_column("MagType", "Mag Type")
out_table.rename_column("LL", "Longitudinal Extent")
# Define a Solar Hemispere Unit
a = {}
u.def_unit(
"SH",
represents=(2 * np.pi * u.solRad**2),
prefixes=True,
namespace=a,
doc="A solar hemisphere is the area of the visible solar disk.")
# Set units on the table
out_table['Carrington Longitude'].unit = u.deg
out_table['Area'].unit = a['uSH']
out_table['Longitudinal Extent'].unit = u.deg
out_table.meta = meta_data
# Number should be formatted in 10000 after 2002-06-15.
if out_table.meta['issued'] > datetime.datetime(2002, 6, 15):
out_table['Number'] += 10000
return QTable(out_table)
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with GWpy. If not, see <http://www.gnu.org/licenses/>.
"""Package to do gravitational wave astrophysics with python
"""
from astropy import table
try:
from astropy.units.quantity import WARN_IMPLICIT_NUMERIC_CONVERSION
except ImportError:
pass
else:
WARN_IMPLICIT_NUMERIC_CONVERSION.set(False)
import warnings
warnings.filterwarnings("ignore", "Module (.*) was already import from")
# set metadata
from . import version
__author__ = "Duncan Macleod <*****@*****.**>"
__version__ = version.version
# register new unit at the top level
from astropy import units
units.def_unit(['counts'], represents=units.Unit('count'), register=True)
units.def_unit(['strain'], represents=units.Unit(''), register=True)
print 'No limits to cancel.'
def __addwindow(self,limlo,limhi):
if limhi < limlo:
limlo,limhi = limhi,limlo
self.windows.append([limlo,limhi])
def __finalise(self):
self.__addwindow(self.__limlo,self.__limhi)
self.__ax.figure.canvas.mpl_disconnect(self.__buttonListener)
self.__ax.figure.canvas.mpl_disconnect(self.__keyListener)
plt.close(self.__ax.figure)
#---------------------
#New units definitions
#---------------------
#the units themselves
unit_t = u.def_unit('transmittance units',doc='Transmittance of radiation')
unit_transmittance = unit_t
unit_abs = u.def_unit('absorbance units',doc='Absorbance of radiation')
unit_absorbance = unit_abs
unit_od = u.def_unit('optical depth units',doc='Optical depth of radiation')
unit_opticaldepth = unit_od
#the equivalencies between the units
equivalencies_absorption = [
(unit_t,unit_abs,lambda x:-np.log10(x),lambda x:10**-x),
(unit_od,unit_abs,lambda x:x/np.log(10),lambda x:x*np.log(10)),
(unit_od,unit_t,lambda x:10**(-x/np.log(10)),lambda x:-np.log10(x)*np.log(10))
]
#------------------------------------------------------
#Functions related to light scattering and transmission
import astropy.units as u
import astropy.constants as ac
import astropy.coordinates.angles as ang
import matplotlib.pyplot as plt
from astropy import log
import time, copy
import collections
try:
from collections import OrderedDict
except ImportError:
from ordereddict import OrderedDict
# Make sure we have the minuteangle and secondangle units
u.minuteangle = u.def_unit('minuteangle', u.hourangle / 60)
u.secondangle = u.def_unit('secondangle', u.minuteangle / 60)
u.lts = u.def_unit(['lightsecond','ls','lts'], ac.c * u.s)
# In the case of a unitless interface, we need to make sure we provide the
# 'correct' tempo2-like units
map_units = {
'F0': u.Hz,
'F1': u.Hz/u.s,
'F2': u.Hz/u.s**2,
'F3': u.Hz/u.s**3,
'F4': u.Hz/u.s**4,
'F5': u.Hz/u.s**5,
'F6': u.Hz/u.s**6,
'F7': u.Hz/u.s**7,
'F8': u.Hz/u.s**8,
# Top-level PINT __init__.py
"""
PINT Is Not TEMPO3!
"""
import os
# Define a few important constants
import astropy.units as u
import astropy.constants as c
# light-second unit
ls = u.def_unit('ls', c.c * 1.0 * u.s)
# Following are from here:
# http://ssd.jpl.nasa.gov/?constants (grabbed on 30 Dec 2013)
GMsun = 1.32712440018e20 * u.m**3/u.s**2
# Solar mass in time units (sec)
Tsun = (GMsun / c.c**3).to(u.s)
# Planet system(!) masses in time units
Tmercury = Tsun / 6023600.
Tvenus = Tsun / 408523.71
Tearth = Tsun / 328900.56 # Includes Moon!
Tmars = Tsun / 3098708.
Tjupiter = Tsun / 1047.3486
Tsaturn = Tsun / 3497.898
Turanus = Tsun / 22902.98
Tneptune = Tsun / 19412.24
# setup environment
import math, shlex, subprocess, numpy
import astropy.constants as const
import astropy.units as u
from pint.utils import PosVel
from astropy import log
import os
from pinttestdata import testdir, datadir
log.setLevel('ERROR')
# for nice output info, set the following instead
#log.setLevel('INFO')
observatories = obsmod.read_observatories()
ls = u.def_unit('ls', const.c * 1.0 * u.s)
log.info("Reading TOAs into PINT")
ts = toa.get_TOAs(datadir + "/testtimes.tim",usepickle=False)
if log.level < 25:
ts.print_summary()
ts.table.sort('index')
log.info("Calling TEMPO2")
#cmd = 'tempo2 -output general2 -f tests/testtimes.par tests/testtimes.tim -s "XXX {clock0} {clock1} {clock2} {clock3} {tt} {t2tb} {telSSB} {telVel} {Ttt}\n"'
cmd = 'tempo2 -output general2 -f ' + datadir+'/testtimes.par ' + datadir + \
'/testtimes.tim -s "XXX {clock0} {clock1} {clock2} {clock3} {tt} {t2tb} {earth_ssb1} {earth_ssb2} {earth_ssb3} {earth_ssb4} {earth_ssb5} {earth_ssb6} {telEpos} {telEVel} {Ttt}\n"'
args = shlex.split(cmd)
tout = subprocess.check_output(args)
goodlines = [x for x in tout.split("\n") if x.startswith("XXX")]
""" Module for spec widgets
"""
from __future__ import print_function, absolute_import, division, unicode_literals
import numpy as np
import pdb
from PyQt4 import QtGui
from PyQt4 import QtCore
from astropy.units import Quantity
from astropy import constants as const
from astropy import units as u
u.def_unit(['mAA', 'milliAngstrom'], 0.001 * u.AA, namespace=globals()) # mA
from matplotlib.backends.backend_qt4agg import FigureCanvasQTAgg as FigureCanvas
from matplotlib.figure import Figure
from astropy.modeling import models, fitting
from linetools.guis import utils as ltgu
from linetools.guis import line_widgets as ltgl
from linetools.spectra.xspectrum1d import XSpectrum1D
from ..spectralline import AbsLine
from ..analysis import voigt as ltv
class ExamineSpecWidget(QtGui.QWidget):
""" Widget to plot a spectrum and interactively
fiddle about. Akin to XIDL/x_specplot.pro
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with GWpy. If not, see <http://www.gnu.org/licenses/>.
"""This module registers a number of custom units used in GW astronomy.
"""
from .. import version
__author__ = "Duncan Macleod <*****@*****.**>"
__version__ = version.version
from astropy import units
# enable imperial units
units.add_enabled_units(units.imperial)
# -----------------------------------------------------------------------------
# instrumental units
units.add_enabled_units([
units.def_unit(['counts'], represents=units.Unit('count')),
units.def_unit(['undef'], doc='No unit has been defined for these data'),
units.def_unit(['coherence'], represents=units.dimensionless_unscaled),
units.def_unit(['strain'], represents=units.dimensionless_unscaled),
units.def_unit(['Degrees_C'], represents=units.Unit('Celsius')),
units.def_unit(['Degrees_F'], represents=units.Unit('Fahrenheit')),
])
# This file is part of GWSumm.
#
# GWSumm is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# GWSumm is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with GWSumm. If not, see <http://www.gnu.org/licenses/>.
"""Extra units for GW data processing
"""
__author__ = 'Duncan Macleod <*****@*****.**>'
from astropy import units
import gwpy.detector.units # noqa: F401
_ns = {} # collector for new units
# Virgo units
units.def_unit('state', namespace=_ns)
# -- register new units -----
units.add_enabled_units(_ns)
import warnings
import numpy as np
from astropy import units as u
from astropy.utils import lazyproperty
from .utils import get_frame_rate
__all__ = ['u_sample', 'VLBIStreamBase', 'VLBIStreamReaderBase',
'VLBIStreamWriterBase']
u_sample = u.def_unit('sample', doc='One sample from a data stream')
class VLBIStreamBase(object):
"""VLBI file wrapper, allowing access as a stream of data."""
_frame_class = None
def __init__(self, fh_raw, header0, nchan, bps, complex_data, thread_ids,
samples_per_frame, frames_per_second=None,
sample_rate=None):
self.fh_raw = fh_raw
self.header0 = header0
self.nchan = nchan
self.bps = bps
self.complex_data = complex_data
self.thread_ids = thread_ids
self.nthread = nchan if thread_ids is None else len(thread_ids)
self.samples_per_frame = samples_per_frame
if frames_per_second is None:
frames_per_second = sample_rate.to(u.Hz).value / samples_per_frame
# 1) alternative names
registry = units.get_current_unit_registry().registry
for unit, aliases in [
(units.Unit('ct'), ('counts',)),
(units.Unit('Celsius'), ('Degrees_C', 'DegC')),
(units.Unit('Fahrenheit'), ('Degrees_F', 'DegF')),
]:
unit.names.extend(aliases)
for alias in aliases:
registry[alias] = unit
# 2) new units
_ns = {}
# LIGO-Lab standard for 'no unit defined'
units.def_unit(['NONE', 'undef'], namespace=_ns,
doc='No unit has been defined for these data')
# other dimenionless units
units.def_unit('strain', represents=units.Unit(''), namespace=_ns)
units.def_unit('coherence', namespace=_ns)
# alias for 'second' but with prefices
units.def_unit((['sec'], ['sec']), represents=units.second, prefixes=True,
namespace=_ns)
# alternative Pressure unit for LIGO UHV
units.def_unit((['torr'], ['torr']), represents=101325/760.*units.pascal,
prefixes=True, namespace=_ns)
# pounds per square inch gauge
units.def_unit('psig', represents=units.imperial.psi, prefixes=True,
