Source code for jwst.saturation.x_irs2

from collections import namedtuple

import numpy as np

from jwst.lib import pipe_utils

# This is the interface:
#     mask = make_mask(input_model)
#         Create a mask for extracting normal pixels; used by from_irs2 and
#         to_irs2.
#         n and r can be specified as keyword arguments to override the
#         default values.  This option is primarily useful if `input_model`
#         is a numpy.ndarray rather than a jwst.datamodels object.
#     shape = normal_shape(input_model, n=n, r=r)
#         The shape of the data array when excluding interleaved reference
#         pixels.
#         n and r can be specified as keyword arguments.
#     normal_data = from_irs2(irs2_data, mask, detector)
#         Extract the normal pixels from data in IRS2 format.
#     to_irs2(irs2_data, normal_data, mask, detector)
#         Insert an array of normal pixels back into data in IRS2 format.

#     Note that `input_model` may be either a jwst.datamodels object or a
#     numpy.ndarray (though in the latter case the parameters will be
#     assigned default values, unless specified explicitly).


ReadoutParam = namedtuple("ReadoutParam", ["refout", "n", "r"])

__all__ = ["normal_shape", "make_mask", "from_irs2", "to_irs2"]


def _get_irs2_parameters(input_model, n=None, r=None):
    """
    Get the parameters describing IRS2 readout format.

    Parameters
    ----------
    input_model : `~stdatamodels.jwst.datamodels.JwstDataModel` or ndarray
        Model from which we retrieve the width of the reference
        output and the values of NRS_NORM and NRS_REF. If the input_model
        is a ndarray the parameters will be assigned default values.

    n : int or None
        The number of "normal" (as opposed to reference) pixels read
        out before jumping to the reference pixel region.

    r : int or None
        The number of reference pixels read out before jumping back to
        the normal pixel region.

    Returns
    -------
    param : ReadoutParam object
        ReadoutParam objects contains the following information:

        param.refout: int
            The length (in the last image axis) of the reference output
            section.  The reference output is assumed to be on the left
            side of the IRS2-format image.

        param.n : int
            The number of "normal" (as opposed to reference) pixels read
            out before jumping to the reference pixel region.

        param.r : int
            The number of reference pixels read out before jumping back to
            the normal pixel region.
    """
    try:
        # Try to get keyword values
        n_norm = input_model.meta.exposure.nrs_normal
        n_ref = input_model.meta.exposure.nrs_reference
    except AttributeError:
        # If keywords are missing, use default values
        n_norm = 16
        n_ref = 4

    # Check for user-supplied values
    if n is not None:
        n_norm = n
    if r is not None:
        n_ref = r

    param = ReadoutParam(refout=(512 + 512 // n_norm * n_ref), n=n_norm, r=n_ref)

    return param


[docs] def normal_shape(input_model, n=None, r=None, detector=None): """ Determine the shape of the 'normal' pixel data. Parameters ---------- input_model : `~stdatamodels.jwst.datamodels.JwstDataModel` This is used to get the shape of the input data. n : int or None The number of "normal" (as opposed to reference) pixels read out before jumping to the reference pixel region. r : int or None The number of reference pixels read out before jumping back to the normal pixel region. detector : str Detector of data. Valid values are None, NRS1, or NRS2. Other detector values will result in a RuntimeError. Returns ------- data_shape : ndarray The shape of the 2-D data array when excluding interleaved reference pixels. """ if isinstance(input_model, np.ndarray): shape = input_model.shape else: shape = input_model.data.shape if detector is None: detector = input_model.meta.instrument.detector if not pipe_utils.is_irs2(input_model): # not IRS2 format return shape param = _get_irs2_parameters(input_model, n=n, r=r) if detector is None: irs2_nx = shape[-1] elif detector == "NRS1" or detector == "NRS2": irs2_nx = shape[-2] else: raise RuntimeError(f"Detector {detector} is not supported for IRS2 data.") k = (irs2_nx - param.refout) // (param.n + param.r) n_output = (irs2_nx - param.refout) - k * param.r if detector is None: data_shape = shape[0:-1] + (n_output,) elif detector == "NRS1" or detector == "NRS2": data_shape = shape[0:-2] + (n_output, shape[-1]) return data_shape
[docs] def make_mask(input_model, n=None, r=None): """ Create a mask to extract "normal" pixels. Parameters ---------- input_model : `~stdatamodels.jwst.datamodels.JwstDataModel` or ndarray This is used for getting the IRS2 parameters and the length of the X image axis. n : int or None The number of "normal" (as opposed to reference) pixels read out before jumping to the reference pixel region. r : int or None The number of reference pixels read out before jumping back to the normal pixel region. Returns ------- irs2_mask : ndarray Boolean index mask (1-D) with length equal to the last axis of the data shape. """ param = _get_irs2_parameters(input_model, n=n, r=r) refout = param.refout n_norm = param.n n_ref = param.r if isinstance(input_model, np.ndarray): shape = input_model.shape else: shape = input_model.data.shape # The input may be flipped and/or rotated from detector orientation. irs2_nx = max(shape[-1], shape[-2]) # Number of (n + r) per output, assuming 4 amplifier outputs. k = (irs2_nx - refout) // 4 // (n_norm + n_ref) # Number of normal pixels per amplifier output. n_output = (irs2_nx - refout) // 4 - k * n_ref irs2_mask = np.ones(irs2_nx, dtype=bool) irs2_mask[0:refout] = False # Check that the locations of interspersed reference pixels is # the same regardless of readout direction. if n_output // n_norm * n_norm == n_output: # The interspersed reference pixels are in the same locations # regardless of readout direction. for i in range(refout + n_norm // 2, irs2_nx + 1, n_norm + n_ref): irs2_mask[i : i + n_ref] = False else: # Set the flags for each readout direction separately. nelem = (irs2_nx - refout) // 4 # number of elements per output temp = np.ones(nelem, dtype=bool) for i in range(n_norm // 2, nelem + 1, n_norm + n_ref): temp[i : i + n_ref] = False j = refout irs2_mask[j : j + nelem] = temp.copy() j = refout + nelem irs2_mask[j + nelem - 1 : j - 1 : -1] = temp.copy() j = refout + 2 * nelem irs2_mask[j : j + nelem] = temp.copy() j = refout + 3 * nelem irs2_mask[j + nelem - 1 : j - 1 : -1] = temp.copy() return irs2_mask
[docs] def from_irs2(irs2_data, irs2_mask, detector=None): """ Extract 'normal' pixel data from an IRS2 image. Parameters ---------- irs2_data : ndarray Data in IRS2 format. This can be a slice in the Y direction, but it should include the entire X (last) axis. irs2_mask : ndarray Boolean mask (1-D) to extract the "normal" pixels. This is a 1-D array with length equal to the size of the next-to-last axis (for data in DMS orientation) of ``irs2_data``. detector : str or None For IRS2 data in DMS orientation, this should be either "NRS1" or "NRS2"; NIRSpec is currently the only instrument supported in this module. The mask will be applied to the rows, and for "NRS2" the mask will first be reversed. For IRS2 data in detector orientation, this should be None (the default), and the mask will be applied to the columns. Returns ------- norm_data : ndarray The normal pixel data (i.e., without embedded reference pixels). """ if detector is None: # Select columns. norm_data = irs2_data[..., irs2_mask] elif detector == "NRS1": # Select rows. norm_data = irs2_data[..., irs2_mask, :] elif detector == "NRS2": # Reverse the direction of the mask, and select rows. temp_mask = irs2_mask[::-1] norm_data = irs2_data[..., temp_mask, :] else: raise RuntimeError(f"Detector {detector} is not supported for IRS2 data.") return norm_data
[docs] def to_irs2(irs2_data, norm_data, irs2_mask, detector=None): """ Copy 'normal' pixel data into an IRS2 image. Parameters ---------- irs2_data : ndarray Data in IRS2 format. This will be modified in-place. norm_data : ndarray The normal data, for example previously extracted from ``irs2_data`` but then modified in some way. This will be copied back into ``irs2_data`` in the correct locations, as specified by ``irs2_mask``. irs2_mask : ndarray Boolean mask (1-D) identifying the locations of the "normal" pixels within irs2_data. The length is equal to the size of the next-to-last axis (for data in DMS orientation) of ``irs2_data``. detector : str or None For IRS2 data in DMS orientation, this should be either "NRS1" or "NRS2"; NIRSpec is currently the only instrument supported in this module. The mask will be applied to the rows, and for "NRS2" the mask will first be reversed. For IRS2 data in detector orientation, this should be None (the default), and the mask will be applied to the columns. """ if detector is None: # Mask specifies columns. irs2_data[..., irs2_mask] = norm_data.copy() elif detector == "NRS1": # Mask specifies rows. irs2_data[..., irs2_mask, :] = norm_data.copy() elif detector == "NRS2": # Reverse the direction of the mask, and apply the reversed mask # to the rows. temp_mask = irs2_mask[::-1] irs2_data[..., temp_mask, :] = norm_data.copy() else: raise RuntimeError(f"Detector {detector} is not supported for IRS2 data.")