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fix input for background.traces, raise error in FlatTrace for negativ…
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…e trace

- Changed FitTrace to allow only the 'omit' and 'filter' masking options.
- Changed the FitTrace tests to check that 'zero-fill' masking option is not allowed any more.
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cshanahan1 committed Dec 12, 2024
1 parent 140e817 commit 6eb9720
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7 changes: 6 additions & 1 deletion CHANGES.rst
Original file line number Diff line number Diff line change
Expand Up @@ -78,7 +78,12 @@ Bug Fixes
peaks. Previously for Gaussian, the entire fit failed. [#205, #206]

- Fixed input of `traces` in `Background`. Added a condition to 'FlatTrace' that
trace position must be a positive number. [#211]

- Fix in FitTrace to set fully-masked column bin peaks to NaN. Previously, for
peak_method='max' these were set to 0.0, and for peak_method='centroid' they
were set to the number of rows in the image, biasing the final fit to all bin
peaks. [#206]


Other changes
^^^^^^^^^^^^^
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93 changes: 78 additions & 15 deletions specreduce/background.py
Original file line number Diff line number Diff line change
Expand Up @@ -32,9 +32,9 @@ class Background(_ImageParser):
----------
image : `~astropy.nddata.NDData`-like or array-like
image with 2-D spectral image data
traces : trace, int, float (single or list)
traces : List, `specreduce.tracing.Trace`, int, float
Individual or list of trace object(s) (or integers/floats to define
FlatTraces) to extract the background. If None, a FlatTrace at the
FlatTraces) to extract the background. If None, a ``FlatTrace`` at the
center of the image (according to `disp_axis`) will be used.
width : float
width of extraction aperture in pixels
Expand All @@ -44,8 +44,22 @@ class Background(_ImageParser):
pixels.
disp_axis : int
dispersion axis
[default: 1]
crossdisp_axis : int
cross-dispersion axis
[default: 0]
mask_treatment : string, optional
The method for handling masked or non-finite data. Choice of ``filter``,
``omit``, or ``zero-fill``. If ``filter`` is chosen, masked and non-finite
data will not contribute to the background statistic that is calculated
in each column along `disp_axis`. If `omit` is chosen, columns along
disp_axis with any masked/non-finite data values will be fully masked
(i.e, 2D mask is collapsed to 1D and applied). If ``zero-fill`` is chosen,
masked/non-finite data will be replaced with 0.0 in the input image,
and the mask will then be dropped. For all three options, the input mask
(optional on input NDData object) will be combined with a mask generated
from any non-finite values in the image data.
[default: ``filter``]
"""
# required so numpy won't call __rsub__ on individual elements
# https://stackoverflow.com/a/58409215
Expand All @@ -57,6 +71,8 @@ class Background(_ImageParser):
statistic: str = 'average'
disp_axis: int = 1
crossdisp_axis: int = 0
mask_treatment: str = 'filter'
_valid_mask_treatment_methods = ('filter', 'omit', 'zero-fill')

# TO-DO: update bkg_array with Spectrum1D alternative (is bkg_image enough?)
bkg_array = deprecated_attribute('bkg_array', '1.3')
Expand All @@ -82,8 +98,29 @@ def __post_init__(self):
dispersion axis
crossdisp_axis : int
cross-dispersion axis
mask_treatment : string
The method for handling masked or non-finite data. Choice of `filter`,
`omit`, or `zero-fill`. If `filter` is chosen, masked/non-finite data
will be filtered during the fit to each bin/column (along disp. axis) to
find the peak. If `omit` is chosen, columns along disp_axis with any
masked/non-finite data values will be fully masked (i.e, 2D mask is
collapsed to 1D and applied). If `zero-fill` is chosen, masked/non-finite
data will be replaced with 0.0 in the input image, and the mask will then
be dropped. For all three options, the input mask (optional on input
NDData object) will be combined with a mask generated from any non-finite
values in the image data.
"""
self.image = self._parse_image(self.image)

# Parse image, including masked/nonfinite data handling based on
# choice of `mask_treatment`. Any uncaught nonfinte data values will be
# masked as well. Returns a Spectrum1D.
self.image = self._parse_image(self.image, disp_axis=self.disp_axis,
mask_treatment=self.mask_treatment)

# always work with masked array, even if there is no masked
# or nonfinite data, in case padding is needed. if not, mask will be
# dropped at the end and a regular array will be returned.
img = np.ma.masked_array(self.image.data, self.image.mask)

if self.width < 0:
raise ValueError("width must be positive")
Expand All @@ -95,9 +132,13 @@ def __post_init__(self):

bkg_wimage = np.zeros_like(self.image.data, dtype=np.float64)
for trace in self.traces:
# note: ArrayTrace can have masked values, but if it does a MaskedArray
# will be returned so this should be reflected in the window size here
# (i.e, np.nanmax is not required.)
windows_max = trace.trace.data.max() + self.width/2
windows_min = trace.trace.data.min() - self.width/2
if windows_max >= self.image.shape[self.crossdisp_axis]:

if windows_max > self.image.shape[self.crossdisp_axis]:
warnings.warn("background window extends beyond image boundaries " +
f"({windows_max} >= {self.image.shape[self.crossdisp_axis]})")
if windows_min < 0:
Expand All @@ -115,27 +156,26 @@ def __post_init__(self):
raise ValueError("background regions overlapped")
if np.any(np.sum(bkg_wimage, axis=self.crossdisp_axis) == 0):
raise ValueError("background window does not remain in bounds across entire dispersion axis") # noqa
# check if image contained within background window is fully-nonfinite and raise an error
if np.all(img.mask[bkg_wimage > 0]):
raise ValueError("Image is fully masked within background window determined by `width`.") # noqa

if self.statistic == 'median':
# make it clear in the expose image that partial pixels are fully-weighted
bkg_wimage[bkg_wimage > 0] = 1

self.bkg_wimage = bkg_wimage

# mask user-highlighted and invalid values (if any) before taking stats
or_mask = (np.logical_or(~np.isfinite(self.image.data), self.image.mask)
if self.image.mask is not None
else ~np.isfinite(self.image.data))

if self.statistic == 'average':
image_ma = np.ma.masked_array(self.image.data, mask=or_mask)
self._bkg_array = np.ma.average(image_ma,
self._bkg_array = np.ma.average(img,
weights=self.bkg_wimage,
axis=self.crossdisp_axis).data
axis=self.crossdisp_axis)

elif self.statistic == 'median':
med_mask = np.logical_or(self.bkg_wimage == 0, or_mask)
image_ma = np.ma.masked_array(self.image.data, mask=med_mask)
self._bkg_array = np.ma.median(image_ma, axis=self.crossdisp_axis).data
# combine where background weight image is 0 with image masked (which already
# accounts for non-finite data that wasn't already masked)
img.mask = np.logical_or(self.bkg_wimage == 0, self.image.mask)
self._bkg_array = np.ma.median(img, axis=self.crossdisp_axis)
else:
raise ValueError("statistic must be 'average' or 'median'")

Expand Down Expand Up @@ -204,7 +244,19 @@ def two_sided(cls, image, trace_object, separation, **kwargs):
dispersion axis
crossdisp_axis : int
cross-dispersion axis
mask_treatment : string
The method for handling masked or non-finite data. Choice of `filter`,
`omit`, or `zero-fill`. If `filter` is chosen, masked/non-finite data
will be filtered during the fit to each bin/column (along disp. axis) to
find the peak. If `omit` is chosen, columns along disp_axis with any
masked/non-finite data values will be fully masked (i.e, 2D mask is
collapsed to 1D and applied). If `zero-fill` is chosen, masked/non-finite
data will be replaced with 0.0 in the input image, and the mask will then
be dropped. For all three options, the input mask (optional on input
NDData object) will be combined with a mask generated from any non-finite
values in the image data.
"""

image = _ImageParser._get_data_from_image(image) if image is not None else cls.image
kwargs['traces'] = [trace_object-separation, trace_object+separation]
return cls(image=image, **kwargs)
Expand Down Expand Up @@ -241,6 +293,17 @@ def one_sided(cls, image, trace_object, separation, **kwargs):
dispersion axis
crossdisp_axis : int
cross-dispersion axis
mask_treatment : string
The method for handling masked or non-finite data. Choice of `filter`,
`omit`, or `zero-fill`. If `filter` is chosen, masked/non-finite data
will be filtered during the fit to each bin/column (along disp. axis) to
find the peak. If `omit` is chosen, columns along disp_axis with any
masked/non-finite data values will be fully masked (i.e, 2D mask is
collapsed to 1D and applied). If `zero-fill` is chosen, masked/non-finite
data will be replaced with 0.0 in the input image, and the mask will then
be dropped. For all three options, the input mask (optional on input
NDData object) will be combined with a mask generated from any non-finite
values in the image data.
"""
image = _ImageParser._get_data_from_image(image) if image is not None else cls.image
kwargs['traces'] = [trace_object+separation]
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