Wrote tests for image parsing methods + codestyle

specreduce/background.py

@@ -6,7 +6,6 @@
 import numpy as np
 from astropy.nddata import NDData
 from astropy.units import UnitTypeError
-from astropy import units as u
 from specutils import Spectrum1D
 
 from specreduce.core import _ImageParser

specreduce/extract.py

@@ -9,7 +9,7 @@
 from astropy.modeling import Model, models, fitting
 from astropy.nddata import NDData, VarianceUncertainty
 
-from specreduce.core import _ImageParser, SpecreduceOperation
+from specreduce.core import SpecreduceOperation
 from specreduce.tracing import Trace, FlatTrace
 from specutils import Spectrum1D
 

specreduce/tests/test_background.py

@@ -2,7 +2,7 @@
 import numpy as np
 
 import astropy.units as u
-from astropy.nddata import CCDData, VarianceUncertainty
+from astropy.nddata import VarianceUncertainty
 from specutils import Spectrum1D
 
 from specreduce.background import Background

specreduce/tests/test_extract.py

@@ -144,7 +144,6 @@ def test_horne_variance_errors():
     # single negative value raises error
     err = image.uncertainty.array
     err[0][0] = -1
-    mask = np.zeros_like(image)
     with pytest.raises(ValueError, match='variance must be fully positive'):
         # remember variance, mask, and unit args are only checked if image
         # object doesn't have those attributes (e.g., numpy and Quantity arrays)

specreduce/tests/test_image_parsing.py

@@ -0,0 +1,104 @@
+import numpy as np
+
+from astropy import units as u
+from astropy.io import fits
+from astropy.nddata import CCDData, NDData, VarianceUncertainty
+from astropy.utils.data import download_file
+
+from specreduce.extract import HorneExtract
+from specreduce.tracing import FlatTrace
+from specutils import Spectrum1D, SpectralAxis
+
+# fetch test image
+fn = download_file('https://stsci.box.com/shared/static/exnkul627fcuhy5akf2gswytud5tazmw.fits',
+                   cache=True)
+
+# duplicate image in all accepted formats
+# (one Spectrum1D variant has a physical spectral axis; the other is in pixels)
+img = fits.getdata(fn).T
+flux = img * u.MJy / u.sr
+sax = SpectralAxis(np.linspace(14.377, 3.677, flux.shape[-1]) * u.um)
+unc = VarianceUncertainty(np.random.rand(*flux.shape))
+
+all_images = {}
+all_images['arr'] = img
+all_images['s1d'] = Spectrum1D(flux, spectral_axis=sax, uncertainty=unc)
+all_images['s1d_pix'] = Spectrum1D(flux, uncertainty=unc)
+all_images['ccd'] = CCDData(img, uncertainty=unc, unit=flux.unit)
+all_images['ndd'] = NDData(img, uncertainty=unc, unit=flux.unit)
+all_images['qnt'] = img * flux.unit
+
+# save default values used for spectral axis and uncertainty when they are not
+# available from the image object or provided by the user
+sax_def = np.arange(img.shape[1]) * u.pix
+unc_def = np.ones_like(img)
+
+
+# (for use inside tests)
+def compare_images(key, collection, compare='s1d'):
+    # was input converted to Spectrum1D?
+    assert isinstance(collection[key], Spectrum1D), (f"image '{key}' not "
+                                                     "of type Spectrum1D")
+
+    # do key's fluxes match its comparison's fluxes?
+    assert np.allclose(collection[key].data,
+                       collection[compare].data), (f"images '{key}' and "
+                                                   f"'{compare}' have unequal "
+                                                   "flux values")
+
+    # if the image came with a spectral axis, was it kept? if not, was the
+    # default spectral axis in pixels applied?
+    sax_provided = hasattr(all_images[key], 'spectral_axis')
+    assert np.allclose(collection[key].spectral_axis,
+                       (all_images[key].spectral_axis if sax_provided
+                        else sax_def)), (f"spectral axis of image '{key}' does "
+                                         f"not match {'input' if sax_provided else 'default'}")
+
+    # if the image came with an uncertainty, was it kept? if not, was the
+    # default uncertainty created?
+    unc_provided = hasattr(all_images[key], 'uncertainty')
+    assert np.allclose(collection[key].uncertainty.array,
+                       (all_images[key].uncertainty.array if unc_provided
+                        else unc_def)), (f"uncertainty of image '{key}' does "
+                                         f"not match {'input' if unc_provided else 'default'}")
+
+    # were masks created despite none being given? (all indices should be False)
+    assert (getattr(collection[key], 'mask', None)
+            is not None), f"no mask was created for image '{key}'"
+    assert np.all(collection[key].mask == 0), ("mask not all False "
+                                               f"for image '{key}'")
+
+
+# test consistency of general image parser results
+def test_parse_general():
+    all_images_parsed = {k: FlatTrace._parse_image(object, im)
+                         for k, im in all_images.items()}
+
+    for key in all_images_parsed.keys():
+        compare_images(key, all_images_parsed)
+
+
+# use verified general image parser results to check HorneExtract's image parser
+def test_parse_horne():
+    # HorneExtract's parser is more stringent than the general one, hence the
+    # separate test. Given proper inputs, both should produce the same results.
+    images_collection = {k: {} for k in all_images.keys()}
+
+    for key, col in images_collection.items():
+        img = all_images[key]
+        col['general'] = FlatTrace._parse_image(object, img)
+
+        if hasattr(all_images[key], 'uncertainty'):
+            defaults = {}
+        else:
+            # save default values of attributes used in general parser when
+            # they are not available from the image object. HorneExtract always
+            # requires a variance, so it's chosen here to be on equal footing
+            # with the general case
+            defaults = {'variance': unc_def,
+                        'mask': np.ma.masked_invalid(img).mask,
+                        'unit': getattr(img, 'unit', u.DN)}
+
+        col[key] = HorneExtract._parse_image(object, img, **defaults)
+
+        compare_images(key, col, compare='general')

specreduce/tracing.py

@@ -5,11 +5,9 @@
 import warnings
 
 from astropy.modeling import fitting, models
-from astropy.nddata import NDData, VarianceUncertainty
+from astropy.nddata import NDData
 from astropy.stats import gaussian_sigma_to_fwhm
-from astropy import units as u
 from scipy.interpolate import UnivariateSpline
-from specutils import Spectrum1D
 import numpy as np
 
 from specreduce.core import _ImageParser