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Fix units JSON units error in notebook #3206

Merged
merged 18 commits into from
Oct 4, 2024
2 changes: 1 addition & 1 deletion CHANGES.rst
Original file line number Diff line number Diff line change
Expand Up @@ -6,7 +6,7 @@ New Features

- Added flux/surface brightness translation and surface brightness
unit conversion in Cubeviz and Specviz. [#2781, #2940, #3088, #3111, #3113, #3129,
#3139, #3149, #3155, #3178, #3185, #3187, #3190, #3156, #3200, #3192]
#3139, #3149, #3155, #3178, #3185, #3187, #3190, #3156, #3200, #3192, #3206]

- Plugin tray is now open by default. [#2892]

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4 changes: 2 additions & 2 deletions jdaviz/app.py
Original file line number Diff line number Diff line change
Expand Up @@ -53,9 +53,9 @@
from jdaviz.utils import (SnackbarQueue, alpha_index, data_has_valid_wcs, layer_is_table_data,
MultiMaskSubsetState, _wcs_only_label, flux_conversion,
spectral_axis_conversion)
from jdaviz.core.custom_units import SPEC_PHOTON_FLUX_DENSITY_UNITS
from jdaviz.core.validunits import (check_if_unit_is_per_solid_angle,
combine_flux_and_angle_units,
locally_defined_flux_units,
supported_sq_angle_units)

__all__ = ['Application', 'ALL_JDAVIZ_CONFIGS', 'UnitConverterWithSpectral']
Expand All @@ -75,7 +75,7 @@ class UnitConverterWithSpectral:
def equivalent_units(self, data, cid, units):
if cid.label == "flux":
eqv = u.spectral_density(1 * u.m) # Value does not matter here.
all_flux_units = locally_defined_flux_units() + ['ct']
all_flux_units = SPEC_PHOTON_FLUX_DENSITY_UNITS + ['ct']
angle_units = supported_sq_angle_units()
all_sb_units = combine_flux_and_angle_units(all_flux_units, angle_units)

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Original file line number Diff line number Diff line change
Expand Up @@ -5,8 +5,7 @@
from regions import PixCoord, CirclePixelRegion
from specutils import Spectrum1D

from jdaviz.core.custom_units import PIX2
from jdaviz.core.validunits import locally_defined_flux_units
from jdaviz.core.custom_units import PIX2, SPEC_PHOTON_FLUX_DENSITY_UNITS


def cubeviz_wcs_dict():
Expand Down Expand Up @@ -36,19 +35,42 @@ def test_basic_unit_conversions(cubeviz_helper, angle_unit):

# load cube with flux units of MJy
w, wcs_dict = cubeviz_wcs_dict()
flux = np.zeros((30, 20, 3001), dtype=np.float32)
flux = np.zeros((3, 4, 5), dtype=np.float32)
cube = Spectrum1D(flux=flux * u.MJy / angle_unit, wcs=w, meta=wcs_dict)
cubeviz_helper.load_data(cube, data_label="test")

# get all available flux units for translation. Since cube is loaded
# in Jy, this will be all items in 'locally_defined_flux_units'

all_flux_units = locally_defined_flux_units()
# in Jy, this will be all items in 'spectral_and_photon_flux_density_units'

uc_plg = cubeviz_helper.plugins['Unit Conversion']

for flux_unit in all_flux_units:
for flux_unit in SPEC_PHOTON_FLUX_DENSITY_UNITS:
uc_plg.flux_unit = flux_unit
assert cubeviz_helper.app._get_display_unit('spectral_y') == flux_unit


@pytest.mark.parametrize("flux_unit, expected_choices", [(u.count, ['ct']),
(u.Jy, SPEC_PHOTON_FLUX_DENSITY_UNITS),
(u.nJy, SPEC_PHOTON_FLUX_DENSITY_UNITS + ['nJy'])]) # noqa
def test_flux_unit_choices(cubeviz_helper, flux_unit, expected_choices):
"""
Test that cubes loaded with various flux units have the expected default
flux unit selection in the unit conversion plugin, and that the list of
convertable flux units in the dropdown is correct.
"""

w, wcs_dict = cubeviz_wcs_dict()
flux = np.zeros((3, 4, 5), dtype=np.float32)
# load cube in flux_unit, will become cube in flux_unit / pix2
cube = Spectrum1D(flux=flux * flux_unit, wcs=w, meta=wcs_dict)
cubeviz_helper.load_data(cube)

uc_plg = cubeviz_helper.plugins['Unit Conversion']

assert uc_plg.angle_unit.selected == 'pix2' # will always be pix2

assert uc_plg.flux_unit.selected == flux_unit.to_string()
assert uc_plg.flux_unit.choices == expected_choices


@pytest.mark.parametrize("angle_unit", [u.sr, PIX2])
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2 changes: 1 addition & 1 deletion jdaviz/configs/default/plugins/viewers.py
Original file line number Diff line number Diff line change
Expand Up @@ -736,7 +736,7 @@ def _plot_uncertainties(self):
self.figure.marks = list(self.figure.marks) + [error_line_mark]

def set_plot_axes(self):
# Set y axes labels for the spectrum viewer
# Set x and y axes labels for the spectrum viewer
y_display_unit = self.state.y_display_unit
y_unit = (
u.Unit(y_display_unit) if y_display_unit and y_display_unit != 'None'
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Original file line number Diff line number Diff line change
Expand Up @@ -4,6 +4,8 @@
from astropy.nddata import InverseVariance
from specutils import Spectrum1D

from jdaviz.core.custom_units import SPEC_PHOTON_FLUX_DENSITY_UNITS


# On failure, should not crash; essentially a no-op.
@pytest.mark.parametrize(
Expand Down Expand Up @@ -133,3 +135,22 @@ def test_non_stddev_uncertainty(specviz_helper):
np.abs(viewer.figure.marks[-1].y - viewer.figure.marks[-1].y.mean(0)),
stddev
)


@pytest.mark.parametrize("flux_unit, expected_choices", [(u.count, ['ct']),
(u.Jy, SPEC_PHOTON_FLUX_DENSITY_UNITS),
(u.nJy, SPEC_PHOTON_FLUX_DENSITY_UNITS + ['nJy'])]) # noqa
def test_flux_unit_choices(specviz_helper, flux_unit, expected_choices):
"""
Test that cubes loaded with various flux units have the expected default
flux unit selection in the unit conversion plugin, and that the list of
convertable flux units in the dropdown is correct.
"""

spec = Spectrum1D([1, 2, 3] * flux_unit, [4, 5, 6] * u.um)
specviz_helper.load_data(spec)

uc_plg = specviz_helper.plugins['Unit Conversion']

assert uc_plg.flux_unit.selected == flux_unit.to_string()
assert uc_plg.flux_unit.choices == expected_choices
Original file line number Diff line number Diff line change
Expand Up @@ -6,7 +6,6 @@
from traitlets import List, Unicode, observe, Bool

from jdaviz.configs.default.plugins.viewers import JdavizProfileView
from jdaviz.core.custom_units import PIX2
from jdaviz.core.events import GlobalDisplayUnitChanged, AddDataMessage
from jdaviz.core.registries import tray_registry
from jdaviz.core.template_mixin import (PluginTemplateMixin, UnitSelectPluginComponent,
Expand Down Expand Up @@ -133,14 +132,16 @@ def __init__(self, *args, **kwargs):
items='flux_unit_items',
selected='flux_unit_selected')
# NOTE: will switch to count only if first data loaded into viewer in in counts
self.flux_unit.choices = create_flux_equivalencies_list(u.Jy, u.Hz)
# initialize flux choices to empty list, will be populated when data is loaded
self.flux_unit.choices = []

self.has_angle = self.config in ('cubeviz', 'specviz', 'mosviz')
self.angle_unit = UnitSelectPluginComponent(self,
items='angle_unit_items',
selected='angle_unit_selected')
# NOTE: will switch to pix2 only if first data loaded into viewer is in pix2 units
self.angle_unit.choices = create_angle_equivalencies_list(u.sr)
# initialize flux choices to empty list, will be populated when data is loaded
self.angle_unit.choices = []

self.has_sb = self.has_angle or self.config in ('imviz',)
# NOTE: sb_unit is read_only, exposed through sb_unit property
Expand Down Expand Up @@ -219,19 +220,15 @@ def _on_add_data_to_viewer(self, msg):
flux_unit = data_obj.flux.unit if angle_unit is None else data_obj.flux.unit * angle_unit # noqa

if not self.flux_unit_selected:
if flux_unit in (u.count, u.DN, u.electron / u.s):
self.flux_unit.choices = [flux_unit]
elif flux_unit not in self.flux_unit.choices:
# ensure that the native units are in the list of choices
self.flux_unit.choices += [flux_unit]
self.flux_unit.choices = create_flux_equivalencies_list(flux_unit)
try:
self.flux_unit.selected = str(flux_unit)
except ValueError:
self.flux_unit.selected = ''

if not self.angle_unit_selected:
if angle_unit == PIX2:
self.angle_unit.choices = ['pix2']
self.angle_unit.choices = create_angle_equivalencies_list(angle_unit)

try:
if angle_unit is None:
# default to sr if input spectrum is not in surface brightness units
Expand Down
20 changes: 20 additions & 0 deletions jdaviz/core/custom_units.py
Original file line number Diff line number Diff line change
@@ -1,4 +1,24 @@
import astropy.units as u

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___all__ = ["PIX2", "SPEC_PHOTON_FLUX_DENSITY_UNITS"]
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# define custom composite units here
PIX2 = u.pix * u.pix


def _spectral_and_photon_flux_density_units():
"""
This function returns an alphabetically sorted list of string representations
of spectral and photon flux density units. This list represents flux units
that the unit conversion plugin supports conversion to and from if the input
data unit is compatible with items in the list (i.e is equivalent directly
or with u.spectral_density(cube_wave)).
"""
flux_units = ['Jy', 'mJy', 'uJy', 'MJy', 'W / (Hz m2)', 'eV / (Hz s m2)',
'erg / (Hz s cm2)', 'erg / (Angstrom s cm2)',
'ph / (Angstrom s cm2)', 'ph / (Hz s cm2)']

return sorted(flux_units)


SPEC_PHOTON_FLUX_DENSITY_UNITS = _spectral_and_photon_flux_density_units()
73 changes: 31 additions & 42 deletions jdaviz/core/validunits.py
Original file line number Diff line number Diff line change
@@ -1,9 +1,9 @@
from astropy import units as u
import itertools

from jdaviz.core.custom_units import PIX2
from jdaviz.core.custom_units import PIX2, SPEC_PHOTON_FLUX_DENSITY_UNITS

__all__ = ['supported_sq_angle_units', 'locally_defined_flux_units',
__all__ = ['supported_sq_angle_units',
'combine_flux_and_angle_units', 'units_to_strings',
'create_spectral_equivalencies_list',
'create_flux_equivalencies_list', 'check_if_unit_is_per_solid_angle']
Expand All @@ -16,20 +16,6 @@ def supported_sq_angle_units(as_strings=False):
return units


def locally_defined_flux_units():
"""
This function returns a list of string representations of flux units. This
list represents flux units that the unit conversion plugin supports
conversion to and from if the input data unit is compatible with items in the
list (i.e is equivalent directly or with u.spectral_density(cube_wave)).

"""
flux_units = ['Jy', 'mJy', 'uJy', 'MJy', 'W / (Hz m2)', 'eV / (Hz s m2)',
'erg / (Hz s cm2)', 'erg / (Angstrom s cm2)',
'ph / (Angstrom s cm2)', 'ph / (Hz s cm2)']
return flux_units


def combine_flux_and_angle_units(flux_units, angle_units):
"""
Combine (list of) flux_units and angle_units to create a list of string
Expand Down Expand Up @@ -92,36 +78,39 @@ def create_spectral_equivalencies_list(spectral_axis_unit,
return sorted(units_to_strings(local_units)) + spectral_axis_unit_equivalencies_titles


def create_flux_equivalencies_list(flux_unit, spectral_axis_unit):
"""Get all possible conversions for flux from current flux units."""
if ((flux_unit in (u.count, u.dimensionless_unscaled))
or (spectral_axis_unit in (u.pix, u.dimensionless_unscaled))):
return []

# Get unit equivalencies. Value passed into u.spectral_density() is irrelevant.
try:
curr_flux_unit_equivalencies = flux_unit.find_equivalent_units(
equivalencies=u.spectral_density(1 * spectral_axis_unit),
include_prefix_units=False)
except u.core.UnitConversionError:
return []
def create_flux_equivalencies_list(flux_unit):
"""
Get all possible conversions for flux from flux_unit, to populate 'flux'
dropdown menu in the unit conversion plugin.

mag_units = ['bol', 'AB', 'ST']
# remove magnitude units from list
curr_flux_unit_equivalencies = [unit for unit in curr_flux_unit_equivalencies if not any(mag in unit.name for mag in mag_units)] # noqa
If flux_unit is a spectral or photon density (i.e convertable to units in
SPEC_PHOTON_FLUX_DENSITY_UNITS), then the loaded unit and all of the
units in SPEC_PHOTON_FLUX_DENSITY_UNITS.

# Get local flux units.
local_units = [u.Unit(unit) for unit in locally_defined_flux_units()]
If the loaded flux unit is count, dimensionless_unscaled, DN, e/s, then
there will be no additional items available for unit conversion and the
only item in the dropdown will be the native unit.
"""

# Remove overlap units.
curr_flux_unit_equivalencies = list(set(curr_flux_unit_equivalencies)
- set(local_units))
flux_unit_str = flux_unit.to_string()

# Convert equivalencies into readable versions of the units and sort them alphabetically.
flux_unit_equivalencies_titles = sorted(units_to_strings(curr_flux_unit_equivalencies))
# if flux_unit is a spectral or photon flux density unit, then the flux unit
# dropdown options should be the loaded unit (which may have a different
# prefix e.g nJy) in addition to items in SPEC_PHOTON_FLUX_DENSITY_UNITS
equiv = u.spectral_density(1 * u.m) # spec. unit doesn't matter here, we're not evaluating
for un in SPEC_PHOTON_FLUX_DENSITY_UNITS:
if flux_unit.is_equivalent(un, equiv):
if flux_unit_str not in SPEC_PHOTON_FLUX_DENSITY_UNITS:
return SPEC_PHOTON_FLUX_DENSITY_UNITS + [flux_unit_str]
else:
return SPEC_PHOTON_FLUX_DENSITY_UNITS

# Concatenate both lists with the local units coming first.
return sorted(units_to_strings(local_units)) + flux_unit_equivalencies_titles
else:
# for any other units, including counts, DN, e/s, DN /s, etc,
# no other conversions between flux units available as we only support
# conversions to and from spectral and photon flux density flux unit.
# dropdown will only contain one item (the input unit)
return [flux_unit_str]


def create_angle_equivalencies_list(solid_angle_unit):
Expand All @@ -146,7 +135,7 @@ def create_angle_equivalencies_list(solid_angle_unit):

"""

if solid_angle_unit is None:
if solid_angle_unit is None or solid_angle_unit is PIX2:
# if there was no solid angle in the unit when calling this function
# can only represent that unit as per square pixel
return ['pix^2']
Expand Down