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implement unit conversion in specviz2d #3253

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@gibsongreen gibsongreen commented Oct 24, 2024

Description

This pull request is to address implementing the Unit Conversion plugin in Specviz2d.

Change log entry

  • Is a change log needed? If yes, is it added to CHANGES.rst? If you want to avoid merge conflicts,
    list the proposed change log here for review and add to CHANGES.rst before merge. If no, maintainer
    should add a no-changelog-entry-needed label.

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  • Are two approvals required? Branch protection rule does not check for the second approval. If a second approval is not necessary, please apply the trivial label.
  • Do the proposed changes actually accomplish desired goals? Also manually run the affected example notebooks, if necessary.
  • Do the proposed changes follow the STScI Style Guides?
  • Are tests added/updated as required? If so, do they follow the STScI Style Guides?
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  • After merge, any internal documentations need updating (e.g., JIRA, Innerspace)?

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codecov bot commented Dec 19, 2024

Codecov Report

Attention: Patch coverage is 87.50000% with 10 lines in your changes missing coverage. Please review.

Project coverage is 87.53%. Comparing base (74e537f) to head (d2411c1).

Files with missing lines Patch % Lines
jdaviz/configs/mosviz/plugins/tools.py 60.00% 6 Missing ⚠️
...plugins/spectral_extraction/spectral_extraction.py 70.00% 3 Missing ⚠️
jdaviz/core/marks.py 92.30% 1 Missing ⚠️

❌ Your patch check has failed because the patch coverage (87.50%) is below the target coverage (90.00%). You can increase the patch coverage or adjust the target coverage.

Additional details and impacted files
@@            Coverage Diff             @@
##             main    #3253      +/-   ##
==========================================
+ Coverage   87.51%   87.53%   +0.02%     
==========================================
  Files         128      128              
  Lines       19901    19957      +56     
==========================================
+ Hits        17416    17469      +53     
- Misses       2485     2488       +3     

☔ View full report in Codecov by Sentry.
📢 Have feedback on the report? Share it here.

@gibsongreen gibsongreen marked this pull request as ready for review December 19, 2024 15:37
self.has_angle = False
self.has_sb = False
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We don't append an angle unit in Specviz right now, see the screenshot when the native unit is Jy. This hides both from displaying in the UI and unexposes them from the API.

Screenshot 2024-12-19 at 4 40 57 PM

@@ -260,7 +260,7 @@ def _create_spectrum1d_cube_with_fluxunit(fluxunit=u.Jy, shape=(2, 2, 4), with_u
wcs_dict = {"CTYPE1": "RA---TAN", "CTYPE2": "DEC--TAN", "CTYPE3": "WAVE-LOG",
"CRVAL1": 205, "CRVAL2": 27, "CRVAL3": 4.622e-7,
"CDELT1": -0.0001, "CDELT2": 0.0001, "CDELT3": 8e-11,
"CRPIX1": 0, "CRPIX2": 0, "CRPIX3": 0,
"CRPIX1": 0, "CRPIX2": 0, "CRPIX3": 0, "PIXAR_SR": 10,
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With this update to the test fixture, in test_spectral_extraction_with_correct_sum_units, the scale factor is no longer the default value of 1, so we need to update the expected values in the test.

CHANGES.rst Outdated Show resolved Hide resolved
Comment on lines 228 to 232
if 'value' in row_info:
# format and cast flux value for Table
row_info['value'] = f"{row_info['value']:.5e}"
else:
row_info['value'] = ''
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why is this necessary? Can/should we move it to as_dict instead?

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There was an issue arising where the value column in the table couldn't be ready properly. This was happening when casting value when it was numpy.float32 to float in coords_info.py. I added a check to only cast if the value is not already float.

spec = self.dataset.selected_spectrum
# Needs Attention:
# should conversion occur before or after call to _apply_subset_masks?
if spec.flux.unit.to_string != self.app._get_display_unit('flux'):
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Isn't this a method? Is it cheaper to compare units instead of casting to string?

Suggested change
if spec.flux.unit.to_string != self.app._get_display_unit('flux'):
if spec.flux.unit.to_string() != self.app._get_display_unit('flux'):

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Good catch! Is it worth converting the display units to astropy.Unit or keep to string comparison?

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I'm not sure, probably fine as is for now

Comment on lines 909 to 914
# Needs Attention:
# should conversion occur before or after call to _apply_subset_masks?
if spec.flux.unit.to_string != self.app._get_display_unit('flux'):
equivalencies = u.spectral_density(self.dataset.selected_spectrum.spectral_axis)
spec = self.dataset.selected_spectrum.with_flux_unit(self.app._get_display_unit('flux'),
equivalencies=equivalencies)
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should this all be moved into the DatasetSelect.selected_spectrum logic so its reusable and cached (and then the cache would need to be invalidated for a change in flux display units)?

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I added some logic to handle_display_unit, and with that, this block is removed and selected_spectrum(use_display_units=True) replaces it.

Comment on lines +441 to +442
self._dict['spectral_axis'] = wave.value
self._dict['spectral_axis:unit'] = wave.unit.to_string()
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where were these handled before (I don't see them in the else 🤔)?

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X-axis conversions were not previously handled in Specviz2d, so they were previously always using the native units and value when mousing over

Comment on lines +226 to +227
# Note: spectra2d Wave loaded in meters, but we respect one spectral unit, so the meters in
# converted to Angstrom (the spectra1d spectral unit).
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Can you explain this a little more? Is it that a previous data entry was in angstroms or just that that is the default spectral display unit?

Suggested change
# Note: spectra2d Wave loaded in meters, but we respect one spectral unit, so the meters in
# converted to Angstrom (the spectra1d spectral unit).
# Note: spectra2d Wave loaded in meters, but we respect one spectral unit, so the meters is
# converted to Angstrom (the spectra1d spectral unit).

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So the loaded 1D and 2D spectra have different native spectral units, with one in meters and one in angstroms and app-wide we're respecting one choice for spectral unit.

Comment on lines 117 to 118
# TODO [specviz2d, mosviz] x_display_unit is not implemented in glue for image viewer
# used by spectrum-2d-viewer
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is this still relevant?

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For the MosvizImageView, I will make sure to update the comment to reflect this!

@rosteen rosteen modified the milestones: 4.1, 4.2 Dec 23, 2024
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When testing this with the specviz2d example notebook, the option to change flux unit disappears when you load the data. The screen shots below show an empty specviz instance, with the 'Flux' option appearing under the unit conversion plugin, and then after loading data when that dropdown disappears

Screenshot 2024-12-23 at 1 59 21 PM Screenshot 2024-12-23 at 2 08 54 PM

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What is included in the scope here for surface brightness logic, including coercing flux units to surface brightness, handling square pixel, and toggling the spectral axis? (Are images of 2d spectra even typically or commonly in surface brightness units?)

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gibsongreen commented Dec 23, 2024

What is included in the scope here for surface brightness logic, including coercing flux units to surface brightness, handling square pixel, and toggling the spectral axis? (Are images of 2d spectra even typically or commonly in surface brightness units?)

  • There will be no coercing for pix^2 in Specviz2d, but I think it will be applicable for the image viewers in Mosviz and Imviz.
  • We only apply the scale factor in Cubeviz since it is stored in the metadata when we extract the cube using the plugin (so no translations here)
  • I did some research into 2d spectra before starting and to my knowledge, they should only be in Flux units. Specviz2d will still be able to load surface brightness units in steradian, if applicable.

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kecnry commented Jan 24, 2025

Probably could be a follow-up - but do we want to invert the x-axis on the 2d spectrum to align with the 1d spectrum when switching between wavelength and frequency units?

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Huge effort - just a few small comments and then I think this is good to go in and build on and hopefully didn't miss too many bugs that might slip through 🤞

@@ -18,12 +19,43 @@ def _is_matched_viewer(self, viewer):
return isinstance(viewer, (MosvizProfile2DView, MosvizProfileView))

def _map_limits(self, from_viewer, to_viewer, limits={}):
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any (reasonable) way to increase test coverage in this method?

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I'm not sure if codecov will be satisfied, but, I should be able to add to an existing test where the data_collection entry doesn't have the cids that were looking for.

A second addition could be to manually recreate the conversion with the pixel_to_world_limits and vis versa in the test itself and assert whether the results are the same (but it will pretty much be identical to the logic in the method).

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I added a second test for when the data loaded doesn't have the Wave nor Wavelength component (I tried using data_collection[0].remove_component('Wave') to no avail). I'm open to adding the pixel_to_world_limits test if coverage doesn't increase much from this recent test addition.

Comment on lines 25 to 36
for key in components.keys():
if 'Wavelength' in str(key):
cid = str(key)
break
elif 'Wave' in str(key):
cid = str(key)
break

if cid is not None:
native_unit = u.Unit(self.viewer.state.data_collection[0].get_component(cid).units)
else:
native_unit = ''
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We could condense this a bit (but existing is fine too if you'd rather keep it)

Suggested change
for key in components.keys():
if 'Wavelength' in str(key):
cid = str(key)
break
elif 'Wave' in str(key):
cid = str(key)
break
if cid is not None:
native_unit = u.Unit(self.viewer.state.data_collection[0].get_component(cid).units)
else:
native_unit = ''
for key in components.keys():
strkey = str(key)
if 'Wavelength' in strkey or 'Wave' in strkey:
native_unit = u.Unit(self.viewer.state.data_collection[0].get_component(strkey).units)
break
else:
# no matches found
native_unit = ''

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I was thinking too that casting each check was overkill, will be included in the next commit!

Comment on lines 94 to 95
cube = spectrum1d_cube_custom_fluxunit(fluxunit=u.Jy / sq_angle_unit,
cube = spectrum1d_cube_custom_fluxunit(fluxunit=u.MJy / sq_angle_unit,
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why the change here?

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I just double-checked and will revert this with an update below where the flux_unit is changed (with the scientific notation for the updated values check).

@@ -708,6 +708,7 @@ def import_trace(self, trace):
else: # pragma: no cover
raise NotImplementedError(f"trace of type {trace.__class__.__name__} not supported")

# UPDATE HERE
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can this be removed or do we need a follow-up ticket for something?

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This was just a note to myself that slipped through the cracks, will be removed shortly

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4 participants