コード例 #1
0
 def as_miller_arrays(self,
                      crystal_symmetry=None,
                      force_symmetry=False,
                      merge_equivalents=True,
                      base_array_info=None,
                      anomalous=None):
     from cctbx import miller
     from cctbx import crystal
     if (crystal_symmetry is None):
         crystal_symmetry = crystal.symmetry()
     if (base_array_info is None):
         base_array_info = miller.array_info(source_type="shelx_hklf")
     miller_set = miller.set(crystal_symmetry=crystal_symmetry,
                             indices=self.indices(),
                             anomalous_flag=anomalous)
     if anomalous is None:
         miller_set = miller_set.auto_anomalous()
     miller_arrays = []
     obs = (miller.array(
         miller_set=miller_set, data=self.data(),
         sigmas=self.sigmas()).set_info(
             base_array_info.customized_copy(labels=["obs", "sigmas"])))
     miller_arrays.append(obs)
     if (self.alphas() is not None):
         miller_arrays.append(
             miller.array(
                 miller_set=miller_set, data=self.alphas()).set_info(
                     base_array_info.customized_copy(labels=["alphas"])))
     return miller_arrays
コード例 #2
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 def phase_transfer(miller_array, phase_source):
     tmp = miller.array(
         miller_set=miller_array,
         data=flex.double(miller_array.indices().size(),
                          1)).phase_transfer(phase_source=phase_source)
     return miller.array(miller_set=miller_array,
                         data=miller_array.data() * tmp.data())
コード例 #3
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    def calculate_cc_int(self, odd_reflections, even_reflections):
        odd_reflections_merged = reflection_table_utils.merge_reflections(
            odd_reflections, self.params.merging.minimum_multiplicity)
        even_reflections_merged = reflection_table_utils.merge_reflections(
            even_reflections, self.params.merging.minimum_multiplicity)

        # Create target symmetry
        if self.params.merging.set_average_unit_cell:
            assert 'average_unit_cell' in (self.params.statistics).__dict__
            unit_cell = self.params.statistics.__phil_get__(
                'average_unit_cell')
        else:
            unit_cell = self.params.scaling.unit_cell
        target_symm = symmetry(
            unit_cell=unit_cell,
            space_group_info=self.params.scaling.space_group)

        # Build miller arrays
        miller_indices_odd = miller.set(target_symm,
                                        odd_reflections_merged['miller_index'],
                                        True)
        intensities_odd = miller.array(
            miller_indices_odd, odd_reflections_merged['intensity'],
            flex.double(odd_reflections_merged.size(), 1.0))

        miller_indices_even = miller.set(
            target_symm, even_reflections_merged['miller_index'], True)
        intensities_even = miller.array(
            miller_indices_even, even_reflections_merged['intensity'],
            flex.double(even_reflections_merged.size(), 1.0))

        # Calculate crosss-correlation
        self.Total_CC_OneHalf_Table = self.calculate_cross_correlation(
            intensities_odd, intensities_even)
コード例 #4
0
ファイル: analysis.py プロジェクト: ndevenish/dials-fork
def reflection_tables_to_batch_dependent_properties(reflection_tables,
                                                    experiments,
                                                    scaled_array=None):
    """Extract batch dependent properties from a reflection table list."""
    offsets = calculate_batch_offsets(experiments)
    reflection_tables = assign_batches_to_reflections(reflection_tables,
                                                      offsets)
    # filter bad refls and negative scales
    batches = flex.int()
    scales = flex.double()
    for r in reflection_tables:
        sel = ~r.get_flags(r.flags.bad_for_scaling, all=False)
        sel &= r["inverse_scale_factor"] > 0
        batches.extend(r["batch"].select(sel))
        scales.extend(r["inverse_scale_factor"].select(sel))
    if not scaled_array:
        scaled_array = scaled_data_as_miller_array(reflection_tables,
                                                   experiments)
    ms = scaled_array.customized_copy()
    batch_array = miller.array(ms, data=batches)

    batch_ranges = get_batch_ranges(experiments, offsets)
    batch_data = [{"id": i, "range": r} for i, r in enumerate(batch_ranges)]

    properties = batch_dependent_properties(batch_array, scaled_array,
                                            miller.array(ms, data=scales))

    return properties + (batch_data, )
コード例 #5
0
ファイル: hklf.py プロジェクト: keitaroyam/cctbx_fork
 def as_miller_arrays(self,
       crystal_symmetry=None,
       force_symmetry=False,
       merge_equivalents=True,
       base_array_info=None):
   from cctbx import miller
   from cctbx import crystal
   if (crystal_symmetry is None):
     crystal_symmetry = crystal.symmetry()
   if (base_array_info is None):
     base_array_info = miller.array_info(source_type="shelx_hklf")
   miller_set = miller.set(
     crystal_symmetry=crystal_symmetry,
     indices=self.indices()).auto_anomalous()
   miller_arrays = []
   obs = (miller.array(
     miller_set=miller_set,
     data=self.data(),
     sigmas=self.sigmas())
     .set_info(base_array_info.customized_copy(labels=["obs", "sigmas"])))
   miller_arrays.append(obs)
   if (self.alphas() is not None):
     miller_arrays.append(miller.array(
       miller_set=miller_set,
       data=self.alphas())
       .set_info(base_array_info.customized_copy(labels=["alphas"])))
   return miller_arrays
コード例 #6
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    def from_reflections_and_experiments(cls, reflection_tables, experiments,
                                         params):
        """Construct the resolutionizer from native dials datatypes."""
        # add some assertions about data

        # do batch assignment (same functions as in dials.export)
        offsets = calculate_batch_offsets(experiments)
        reflection_tables = assign_batches_to_reflections(
            reflection_tables, offsets)
        batches = flex.int()
        intensities = flex.double()
        indices = flex.miller_index()
        variances = flex.double()
        for table in reflection_tables:
            if "intensity.scale.value" in table:
                table = filter_reflection_table(table, ["scale"],
                                                partiality_threshold=0.4)
                intensities.extend(table["intensity.scale.value"])
                variances.extend(table["intensity.scale.variance"])
            else:
                table = filter_reflection_table(table, ["profile"],
                                                partiality_threshold=0.4)
                intensities.extend(table["intensity.prf.value"])
                variances.extend(table["intensity.prf.variance"])
            indices.extend(table["miller_index"])
            batches.extend(table["batch"])

        crystal_symmetry = miller.crystal.symmetry(
            unit_cell=determine_best_unit_cell(experiments),
            space_group=experiments[0].crystal.get_space_group(),
            assert_is_compatible_unit_cell=False,
        )
        miller_set = miller.set(crystal_symmetry,
                                indices,
                                anomalous_flag=False)
        i_obs = miller.array(miller_set,
                             data=intensities,
                             sigmas=flex.sqrt(variances))
        i_obs.set_observation_type_xray_intensity()
        i_obs.set_info(miller.array_info(source="DIALS", source_type="refl"))

        ms = i_obs.customized_copy()
        batch_array = miller.array(ms, data=batches)

        if params.reference is not None:
            reference, _ = miller_array_from_mtz(params.reference,
                                                 anomalous=params.anomalous,
                                                 labels=params.labels)
        else:
            reference = None

        return cls(i_obs, params, batches=batch_array, reference=reference)
コード例 #7
0
    def _get_unique_Hi(self):
        COMM.barrier()
        if COMM.rank == 0:
            from cctbx.crystal import symmetry
            from cctbx import miller
            from cctbx.array_family import flex as cctbx_flex

            ii = list(self.Modelers.keys())[0]
            uc = self.Modelers[ii].ucell_man
            params = uc.a, uc.b, uc.c, uc.al * 180 / np.pi, uc.be * 180 / np.pi, uc.ga * 180 / np.pi
            if self.params.refiner.force_unit_cell is not None:
                params = self.params.refiner.force_unit_cell
            symm = symmetry(unit_cell=params, space_group_symbol=self.symbol)
            hi_asu_flex = cctbx_flex.miller_index(self.Hi_asu_all_ranks)
            mset = miller.set(symm, hi_asu_flex, anomalous_flag=True)
            marr = miller.array(mset)
            binner = marr.setup_binner(
                d_max=self.params.refiner.stage_two.d_max,
                d_min=self.params.refiner.stage_two.d_min,
                n_bins=self.params.refiner.stage_two.n_bin)
            from collections import Counter
            print("Average multiplicities:")
            print("<><><><><><><><><><><><>")
            for i_bin in range(self.params.refiner.stage_two.n_bin - 1):
                dmax, dmin = binner.bin_d_range(i_bin + 1)
                F_in_bin = marr.resolution_filter(d_max=dmax, d_min=dmin)
                multi_in_bin = np.array(
                    list(Counter(F_in_bin.indices()).values()))
                print("%2.5g-%2.5g : Multiplicity=%.4f" %
                      (dmax, dmin, multi_in_bin.mean()))
                for ii in range(1, 100, 8):
                    print("\t %d refls with multi %d" %
                          (sum(multi_in_bin == ii), ii))

            print("Overall completeness\n<><><><><><><><>")
            symm = symmetry(unit_cell=params, space_group_symbol=self.symbol)
            hi_flex_unique = cctbx_flex.miller_index(
                list(set(self.Hi_asu_all_ranks)))
            mset = miller.set(symm, hi_flex_unique, anomalous_flag=True)
            self.binner = mset.setup_binner(
                d_min=self.params.refiner.stage_two.d_min,
                d_max=self.params.refiner.stage_two.d_max,
                n_bins=self.params.refiner.stage_two.n_bin)
            mset.completeness(use_binning=True).show()
            marr_unique_h = miller.array(mset)
            print("Rank %d: total miller vars=%d" %
                  (COMM.rank, len(set(self.Hi_asu_all_ranks))))
        else:
            marr_unique_h = None

        marr_unique_h = COMM.bcast(marr_unique_h)
        return marr_unique_h
コード例 #8
0
    def read_file(self, hklin):
        assert self.symm is not None  # XXX more careful check
        fin = open(hklin)
        line = fin.readline()  # first line

        #TODO support other format.
        assert "CrystFEL reflection list version 2.0" in line

        line = fin.readline()  # second line
        sym_str = line[line.find(":") + 1:].strip()
        print "HKL pointgroup:", sym_str,

        anomalous_flag = None
        if sym_str == self.symm.space_group().laue_group_type():
            anomalous_flag = False
        elif sym_str == self.symm.space_group().point_group_type():
            anomalous_flag = True
        else:
            Sorry("Incompatible symmetry: %s and %s" %
                  (sym_str, self.symm.space_group().info()))
        print "Anomalous:", anomalous_flag

        line = fin.readline()  # third line
        assert "   h    k    l          I    phase   sigma(I)   nmeas" in line

        indices, Is, sigIs, ns = [], [], [], []
        for l in fin:
            if l.startswith("End of reflections"):
                break

            h, k, l, i, phase, sigi, nmeas = l.strip().split()
            h, k, l, nmeas = map(int, (h, k, l, nmeas))
            i, sigi = map(float, (i, sigi))
            indices.append((h, k, l))
            Is.append(i)
            sigIs.append(sigi)
            ns.append(nmeas)

        miller_set = miller.set(crystal_symmetry=self.symm,
                                indices=flex.miller_index(indices),
                                anomalous_flag=anomalous_flag)

        self.array = miller.array(
            miller_set=miller_set,
            data=flex.double(Is),
            sigmas=flex.double(sigIs)).set_observation_type_xray_intensity()

        self.redundancies = miller.array(miller_set=miller_set,
                                         data=flex.int(ns))
コード例 #9
0
ファイル: hkl.py プロジェクト: harumome/kamo
    def read_file(self, hklin):
        assert self.symm is not None # XXX more careful check
        fin = open(hklin)
        line = fin.readline() # first line
        
        #TODO support other format.
        assert "CrystFEL reflection list version 2.0" in line

        line = fin.readline() # second line
        sym_str = line[line.find(":")+1:].strip()
        print "HKL pointgroup:",sym_str,

        anomalous_flag = None
        if sym_str == self.symm.space_group().laue_group_type():
            anomalous_flag = False
        elif sym_str == self.symm.space_group().point_group_type():
            anomalous_flag = True
        else:
            Sorry("Incompatible symmetry: %s and %s" % (sym_str, self.symm.space_group().info()))
        print "Anomalous:", anomalous_flag

        line = fin.readline() # third line
        assert "   h    k    l          I    phase   sigma(I)   nmeas" in line

        indices, Is, sigIs, ns = [], [], [], []
        for l in fin:
            if l.startswith("End of reflections"):
                break

            h,k,l,i,phase,sigi,nmeas = l.strip().split()
            h,k,l,nmeas = map(int, (h,k,l,nmeas))
            i,sigi = map(float, (i,sigi))
            indices.append((h,k,l))
            Is.append(i)
            sigIs.append(sigi)
            ns.append(nmeas)
        
        miller_set = miller.set(crystal_symmetry=self.symm,
                                indices=flex.miller_index(indices),
                                anomalous_flag=anomalous_flag)

        self.array = miller.array(miller_set=miller_set,
                                  data=flex.double(Is),
                                  sigmas=flex.double(sigIs)
                                  ).set_observation_type_xray_intensity()

        self.redundancies = miller.array(miller_set=miller_set,
                                  data=flex.int(ns))
コード例 #10
0
ファイル: ScaleAndMerge.py プロジェクト: Anthchirp/xia2
    def reflections_as_miller_arrays(self, combined=False):
        from dials.util.batch_handling import (
            # calculate_batch_offsets,
            # get_batch_ranges,
            assign_batches_to_reflections, )
        from dials.report.analysis import scaled_data_as_miller_array

        # offsets = calculate_batch_offsets(experiments)
        reflection_tables = []
        for id_ in set(self._reflections["id"]).difference({-1}):
            reflection_tables.append(
                self._reflections.select(self._reflections["id"] == id_))

        offsets = [expt.scan.get_batch_offset() for expt in self._experiments]
        reflection_tables = assign_batches_to_reflections(
            reflection_tables, offsets)

        if combined:
            # filter bad refls and negative scales
            batches = flex.int()
            scales = flex.double()

            for r in reflection_tables:
                sel = ~r.get_flags(r.flags.bad_for_scaling, all=False)
                sel &= r["inverse_scale_factor"] > 0
                batches.extend(r["batch"].select(sel))
                scales.extend(r["inverse_scale_factor"].select(sel))
            scaled_array = scaled_data_as_miller_array(reflection_tables,
                                                       self._experiments)
            batch_array = miller.array(scaled_array, data=batches)
            scale_array = miller.array(scaled_array, data=scales)
            return scaled_array, batch_array, scale_array

        else:
            scaled_arrays = []
            batch_arrays = []
            scale_arrays = []
            for expt, r in zip(self._experiments, reflection_tables):
                sel = ~r.get_flags(r.flags.bad_for_scaling, all=False)
                sel &= r["inverse_scale_factor"] > 0
                batches = r["batch"].select(sel)
                scales = r["inverse_scale_factor"].select(sel)
                scaled_arrays.append(scaled_data_as_miller_array([r], [expt]))
                batch_arrays.append(
                    miller.array(scaled_arrays[-1], data=batches))
                scale_arrays.append(
                    miller.array(scaled_arrays[-1], data=scales))
            return scaled_arrays, batch_arrays, scale_arrays
コード例 #11
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def pha2mtz(phain, xs, mtzout):
    hkl, f, fom, phi, sigf = [], [], [], [], []

    for l in open(phain):
        sp = l.split()
        if len(sp) != 7: break
        hkl.append(tuple(map(int, sp[:3])))
        f.append(float(sp[3]))
        fom.append(float(sp[4]))
        phi.append(float(sp[5]))
        sigf.append(float(sp[6]))

    if not hkl:
        return

    f_array = miller.array(miller.set(xs, flex.miller_index(hkl)),
                           data=flex.double(f),
                           sigmas=flex.double(sigf))
    mtz_ds = f_array.as_mtz_dataset(
        column_root_label="ANOM", column_types="FQ"
    )  # To open with Coot, column type F is required (not D)
    mtz_ds.add_miller_array(f_array.customized_copy(data=flex.double(phi),
                                                    sigmas=None),
                            column_root_label="PANOM",
                            column_types="P")
    mtz_ds.add_miller_array(f_array.customized_copy(data=flex.double(fom),
                                                    sigmas=None),
                            column_root_label="FOM",
                            column_types="W")

    mtz_ds.mtz_object().write(mtzout)
コード例 #12
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def load_sfall(fname):
    """
    special script for loading the structure factor file generated in main()
    :param fname: file generated in the main method above.. 
    :return: mil_ar, energies
        mil_ar: dict of miller arrays (complex) 
        energies: array of xray energies in electron volts
        such that  mil_ar[0] is Fhkl at energy energies[0]
    """

    f = h5py.File(fname, "r")
    data = f["data"][()]
    indices = f["indices"][()]
    hall = f["hall_symbol"][()]
    ucell_param = f["ucell_tuple"][()]
    energies = f["energies"][()]
    sg = sgtbx.space_group(hall)
    Symm = crystal.symmetry(unit_cell=ucell_param, space_group=sg)
    indices_flex = tuple(map(tuple, indices))
    mil_idx = flex.miller_index(indices_flex)
    mil_set = miller.set(crystal_symmetry=Symm,
                         indices=mil_idx,
                         anomalous_flag=True)

    mil_ar = {}  # load a dict of "sfall at each energy"
    for i_chan, data_chan in enumerate(data):
        data_flex = flex.complex_double(np.ascontiguousarray(data_chan))
        mil_ar[i_chan] = miller.array(mil_set, data=data_flex)

    return mil_ar, energies
コード例 #13
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ファイル: utils.py プロジェクト: zhuligs/cctbx_project
def random_f_calc(space_group_info,
                  n_scatterers,
                  d_min,
                  anomalous_flag,
                  verbose=0):
    if (anomalous_flag and space_group_info.group().is_centric()):
        return None
    structure = random_structure.xray_structure(space_group_info,
                                                elements=["const"] *
                                                n_scatterers,
                                                volume_per_atom=500,
                                                min_distance=2.,
                                                general_positions_only=True)
    if (0 or verbose):
        structure.show_summary().show_scatterers()
    f_calc = structure.structure_factors(
        d_min=d_min, anomalous_flag=anomalous_flag).f_calc()
    f_calc = miller.array(miller_set=f_calc,
                          data=f_calc.data() /
                          flex.mean(flex.abs(f_calc.data())))
    if (f_calc.anomalous_flag()):
        selection = flex.bool(f_calc.indices().size(), True)
        for i in xrange(f_calc.indices().size() // 10):
            j = random.randrange(f_calc.indices().size())
            selection[j] = False
        f_calc = f_calc.select(selection)
    return f_calc
コード例 #14
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    def as_mtz(self,scale_factor,prefix):
    #This reads in an hkl map and returns a .mtz map
        #Read in hkl file and populate miller array
        inf = open(self.diffuse_file, 'r')
        indices = flex.miller_index()
        i_obs = flex.double()
        sig_i = flex.double()
        for line in inf.readlines():
            assert len(line.split())==4
            line = line.strip().split()
            #####ATTENTION:SCALE FACTOR##############
            i_obs_ = float(line[3])/scale_factor #is a uniform scale factor meant to re-size all diffuse intensities (normally too large for scalepack)
            sig_i_ = math.sqrt(i_obs_) 
            #if(abs(i_obs_)>1.e-6): # perhaps you don't want zeros
            indices.append([int(line[0]),int(line[1]),int(line[2])])
            i_obs.append(i_obs_)
            sig_i.append(sig_i_)
        inf.close()

      # get miller array object
        cs = self.symmetry
        ma = miller.array(miller_set=miller.set(cs, indices), data=i_obs, sigmas=sig_i)
        ma.set_observation_type_xray_intensity()
        mtz_dataset = ma.as_mtz_dataset(column_root_label="I")
        mtz_dataset.mtz_object().write(prefix + '.mtz')
コード例 #15
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def amplitude_quasi_normalisations(ma, d_star_power=1, set_to_minimum=None):
    epsilons = ma.epsilons().data().as_double()
    mean_f_sq_over_epsilon = flex.double()
    for i_bin in ma.binner().range_used():
      sel = ma.binner().selection(i_bin)
      #sel_f_sq = flex.pow2(ma.data().select(sel))
      sel_f_sq = ma.data().select(sel)
      if (sel_f_sq.size() > 0):
        sel_epsilons = epsilons.select(sel)
        sel_f_sq_over_epsilon = sel_f_sq / sel_epsilons
        mean_f_sq_over_epsilon.append(flex.mean(sel_f_sq_over_epsilon))
      else:
        mean_f_sq_over_epsilon.append(0)
    mean_f_sq_over_epsilon_interp = ma.binner().interpolate(
      mean_f_sq_over_epsilon, d_star_power)
    if set_to_minimum and not mean_f_sq_over_epsilon_interp.all_gt(0):
      # HACK NO REASON THIS SHOULD WORK
      sel = (mean_f_sq_over_epsilon_interp <= set_to_minimum)
      mean_f_sq_over_epsilon_interp.set_selected(sel,-mean_f_sq_over_epsilon_interp)
      sel = (mean_f_sq_over_epsilon_interp <= set_to_minimum)
      mean_f_sq_over_epsilon_interp.set_selected(sel,set_to_minimum)
    assert mean_f_sq_over_epsilon_interp.all_gt(0)
    from cctbx.miller import array
    #return array(ma, flex.sqrt(mean_f_sq_over_epsilon_interp))
    return array(ma, mean_f_sq_over_epsilon_interp)
コード例 #16
0
ファイル: cctbx_utils.py プロジェクト: apeck12/cryoetX
def mtz_to_miller_array(mtz_object):
    """
    Recombine intensities and phases (under 'IMEAN' and 'PHIB' labels, respectively)
    from input MTZ file into a Miller array object. Probably there's a CCTBX utility
    to accomplish this, but I haven't been able to locate it.
    
    Inputs:
    -------
    mtz_object: a CCTBX MTZ object (from mtz.object(file_name=filename.mtz))
    
    Outputs:
    --------
    ma: a CCTBX Miller array object of complex structure factors
    """
    
    # extract Miller arrays and crystal symmetry
    I_ma = mtz_object.as_miller_arrays_dict()[('crystal', 'dataset', 'IMEAN')]
    p_ma = mtz_object.as_miller_arrays_dict()[('crystal', 'dataset', 'PHIB')]
    assert list(I_ma.indices()) == list(p_ma.indices())
    cs = mtz_object.crystals()[1].crystal_symmetry()
    
    # compute complex structure factors
    I, p = np.array(I_ma.data()), np.deg2rad(np.array(p_ma.data()))
    A, B = np.sqrt(I) * np.cos(p), np.sqrt(I) * np.sin(p)
    indices = I_ma.indices()
    sf_data = flex.complex_double(flex.double(A), flex.double(B))

    # convert complex structure factors to CCTBX-style Miller array
    ma = miller.array(miller_set = miller.set(cs, indices, anomalous_flag=False), data = sf_data)
    
    return ma
コード例 #17
0
def random_hkl_selection(cs, resolution, completeness):
    """
    Retrieve a list of random Miller indices to achieve the desired completeness
    in P1, assuming no anomalous signal.
    
    Inputs:
    -------
    cs: CCTBX crystal symmetry object
    resolution: high-resolution limit
    completeness: desired P1 completeness
    
    Outputs:
    --------
    hkl_sel: list of Miller indices to retain   
    """
    # get list of P1 reflections, assuming no anomalous signal
    hkl_p1 = list(
        cs.build_miller_set(anomalous_flag=False,
                            d_min=resolution).expand_to_p1().indices())

    # retrieve random list of reflections and their friedel mates
    n_est = int(np.around(completeness * len(hkl_p1)))
    hkl_sel = random.sample(hkl_p1, n_est)
    fhkl_sel = [(-1 * h[0], -1 * h[1], -1 * h[2]) for h in hkl_sel]
    hkl_sel += fhkl_sel

    # print information about P1 and SG completeness
    for cs_obj, tag in zip([cs, cs.cell_equivalent_p1()], ['SG', 'P1']):
        ma_calc = miller.array(miller_set=miller.set(
            cs_obj, flex.miller_index(hkl_sel), anomalous_flag=False),
                               data=flex.double(np.ones_like(hkl_sel)))
        print "%s completeness: %.2f" % (
            tag, ma_calc.merge_equivalents().array().completeness())

    return hkl_sel
コード例 #18
0
def calculate_exp_i_two_phi_peaks(xray_structure, d_min,
                                  min_peak_distance,
                                  max_reduced_peaks):
  f_h = xray_structure.structure_factors(
    anomalous_flag=False,
    d_min=d_min).f_calc()
  two_i_phi_h = miller.array(
    miller_set=f_h,
    data=flex.polar(1, flex.arg(f_h.data())*2))
  fft_map = two_i_phi_h.fft_map(
    d_min=d_min,
    symmetry_flags=maptbx.use_space_group_symmetry)
  real_map = fft_map.real_map()
  real_map = maptbx.copy(real_map, flex.grid(real_map.focus()))
  stats = maptbx.statistics(real_map)
  if (stats.max() != 0):
    real_map /= abs(stats.max())
  grid_tags = maptbx.grid_tags(real_map.focus())
  grid_tags.build(fft_map.space_group_info().type(), fft_map.symmetry_flags())
  grid_tags.verify(real_map)
  peak_list = maptbx.peak_list(
    data=real_map,
    tags=grid_tags.tag_array(),
    max_peaks=10*max_reduced_peaks,
    interpolate=True)
  reduced_peaks = peak_cluster_reduction(
    crystal_symmetry=xray_structure,
    peak_list=peak_list,
    min_peak_distance=min_peak_distance,
    max_reduced_peaks=max_reduced_peaks)
  return reduced_peaks
コード例 #19
0
ファイル: tst.py プロジェクト: keitaroyam/cctbx_fork
def exercise_recycle(space_group_info, anomalous_flag, n_scatterers=8, d_min=2.5, verbose=0):
    f_calc = random_f_calc(
        space_group_info=space_group_info,
        n_scatterers=n_scatterers,
        d_min=d_min,
        anomalous_flag=anomalous_flag,
        verbose=verbose,
    )
    if f_calc is None:
        return
    recycle(f_calc, "f_calc", verbose=verbose)
    for column_root_label, column_types in [("f_obs", None), ("Ework", "E")]:
        if anomalous_flag and column_types == "E":
            continue
        recycle(
            miller_array=abs(f_calc), column_root_label=column_root_label, column_types=column_types, verbose=verbose
        )
    if not anomalous_flag:
        recycle(abs(f_calc), "f_obs", column_types="R", verbose=verbose)
    for column_root_label, column_types in [("f_obs", None), ("Ework", "EQ")]:
        if anomalous_flag and column_types == "EQ":
            continue
        recycle(
            miller_array=miller.array(
                miller_set=f_calc, data=flex.abs(f_calc.data()), sigmas=flex.abs(f_calc.data()) / 10
            ),
            column_root_label=column_root_label,
            column_types=column_types,
            verbose=verbose,
        )
    recycle(f_calc.centric_flags(), "cent", verbose=verbose)
    recycle(generate_random_hl(miller_set=f_calc), "prob", verbose=verbose)
コード例 #20
0
def exercise(space_group_info, anomalous_flag,
             n_scatterers=8, d_min=2, verbose=0):
  structure = random_structure.xray_structure(
    space_group_info,
    elements=["const"]*n_scatterers)
  f_calc = structure.structure_factors(
    d_min=d_min, anomalous_flag=anomalous_flag).f_calc()
  f = abs(f_calc)
  f = miller.array(miller_set=f, data=f.data(), sigmas=flex.sqrt(f.data()))
  f = f.f_as_f_sq()
  g = f.expand_to_p1()
  merger_p1 = xray.merger( g.indices(),
                              g.data(),
                              g.sigmas(),
                              g.space_group(),
                              g.anomalous_flag(),
                              g.unit_cell() )
  p1_bic = merger_p1.bic()
  p1_r = merger_p1.r_abs()

  merger_nat = xray.merger( g.indices(),
                              g.data(),
                              g.sigmas(),
                              f.space_group(),
                              g.anomalous_flag(),
                              g.unit_cell() )
  nat_bic = merger_nat.bic()
  nat_r = merger_nat.r_abs()
  assert nat_bic >= p1_bic
  assert p1_r <= 1e-8
コード例 #21
0
    def extend_symmetry(self,scale_factor,prefix):
    #This reads in an hkl map and returns a .sca map
        #Read in hkl file and populate miller array
        inf = open(self.diffuse_file, 'r')
        indices = flex.miller_index()
        i_obs = flex.double()
        sig_i = flex.double()
        for line in inf.readlines():
            assert len(line.split())==4
            line = line.strip().split()
            #####ATTENTION:SCALE FACTOR##############
            i_obs_ = float(line[3])/scale_factor #is a uniform scale factor meant to re-size all diffuse intensities (normally too large for scalepack)
            sig_i_ = math.sqrt(i_obs_) 
            #if(abs(i_obs_)>1.e-6): # perhaps you don't want zeros
            indices.append([int(line[0]),int(line[1]),int(line[2])])
            i_obs.append(i_obs_)
            sig_i.append(sig_i_)
        inf.close()

      # get miller array object
        cs = self.symmetry
        ma = miller.array(miller_set=miller.set(cs, indices), data=i_obs, sigmas=sig_i)
        ma.set_observation_type_xray_intensity()
        ma_anom = ma.customized_copy(anomalous_flag=False)
        ma_p1 = ma_anom.expand_to_p1()

        merge.write(file_name= prefix + '.sca', miller_array=ma_p1)

        self.p1_map = prefix + '.sca'
コード例 #22
0
def exercise(space_group_info,
             anomalous_flag,
             n_scatterers=8,
             d_min=2,
             verbose=0):
    structure = random_structure.xray_structure(space_group_info,
                                                elements=["const"] *
                                                n_scatterers)
    f_calc = structure.structure_factors(
        d_min=d_min, anomalous_flag=anomalous_flag).f_calc()
    f = abs(f_calc)
    f = miller.array(miller_set=f, data=f.data(), sigmas=flex.sqrt(f.data()))
    f = f.f_as_f_sq()
    g = f.expand_to_p1()
    merger_p1 = xray.merger(g.indices(), g.data(), g.sigmas(), g.space_group(),
                            g.anomalous_flag(), g.unit_cell())
    p1_bic = merger_p1.bic()
    p1_r = merger_p1.r_abs()

    merger_nat = xray.merger(g.indices(), g.data(),
                             g.sigmas(), f.space_group(), g.anomalous_flag(),
                             g.unit_cell())
    nat_bic = merger_nat.bic()
    nat_r = merger_nat.r_abs()
    assert nat_bic >= p1_bic
    assert p1_r <= 1e-8
コード例 #23
0
ファイル: merge.py プロジェクト: cctbx/cctbx-playground
 def as_miller_array(self,
       crystal_symmetry=None,
       force_symmetry=False,
       merge_equivalents=True,
       base_array_info=None):
   if (base_array_info is None):
     base_array_info = miller.array_info(source_type="scalepack_merge")
   crystal_symmetry_from_file = self.crystal_symmetry()
   if (self.anomalous):
     labels = ["I(+)", "SIGI(+)", "I(-)", "SIGI(-)"]
   else:
     labels = ["I", "SIGI"]
   return (miller.array(
     miller_set=miller.set(
       crystal_symmetry=crystal_symmetry_from_file.join_symmetry(
         other_symmetry=crystal_symmetry,
         force=force_symmetry),
       indices=self.miller_indices,
       anomalous_flag=self.anomalous),
     data=self.i_obs,
     sigmas=self.sigmas)
     .set_info(base_array_info.customized_copy(
       labels=labels,
       crystal_symmetry_from_file=crystal_symmetry_from_file))
     .set_observation_type_xray_intensity())
コード例 #24
0
ファイル: blend.py プロジェクト: keitaroyam/yamtbx
    def cluster_completeness(self, clno, anomalous_flag, calc_redundancy=True):
        if clno not in self.clusters:
            print "Cluster No. %d not found" % clno
            return

        cls = self.clusters[clno][3]
        msets = map(lambda x: self.miller_sets[self.files[x-1]], cls)
        num_idx = sum(map(lambda x: x.size(), msets))
        all_idx = flex.miller_index()
        all_idx.reserve(num_idx)
        for mset in msets: all_idx.extend(mset.indices())

        # Calc median cell
        cells = numpy.array(map(lambda x: x.unit_cell().parameters(), msets))
        median_cell = map(lambda i: numpy.median(cells[:,i]), xrange(6))
        symm = msets[0].customized_copy(unit_cell=median_cell)

        assert anomalous_flag is not None
        # XXX all must belong to the same Laue group and appropriately reindexed..
        all_set = miller.set(indices=all_idx,
                             crystal_symmetry=symm, anomalous_flag=anomalous_flag)
        all_set = all_set.resolution_filter(d_min=self.d_min)

        # dummy for redundancy calculation. dirty way..
        if calc_redundancy:
            dummy_array = miller.array(miller_set=all_set, data=flex.int(all_set.size()))
            merge = dummy_array.merge_equivalents()
            cmpl = merge.array().completeness()
            redun = merge.redundancies().as_double().mean()
            return cmpl, redun
        else:
            cmpl = all_set.unique_under_symmetry().completeness()
            return cmpl
コード例 #25
0
def exercise():
  ma = miller.array(
    miller.set(crystal.symmetry(unit_cell=(5,5,5, 90, 90, 90),
                                space_group=sgtbx.space_group('P 2x')),
               indices=flex.miller_index(
                 [(1,0,0), (0,1,0), (0,0,1),
                  (-1,0,0), (0,-1,0), (0,0,-1),
                  (1,1,0), (1,0,1), (0,1,1),
                  (-1,-1,0), (-1,0,-1), (0,-1,-1),
                  (1,-1,0), (1,0,-1), (0,1,-1),
                  (-1,1,0), (-1,0,1), (0,-1,1),
                  (1,1,1), (-1,1,1), (1,-1,1), (1,1,-1),
                  (-1,-1,-1), (1,-1,-1), (-1,1,-1), (-1,-1,1)])),
    data=flex.complex_double(flex.random_double(26), flex.random_double(26)))
  f_at_h = dict(zip(ma.indices(), ma.data()))
  for op in ("-x, y+1/2, -z", "x+1/2, -y, z-1/2"):
    op = sgtbx.rt_mx(op)
    original, transformed = ma.common_sets(
      ma.change_basis(sgtbx.change_of_basis_op(op.inverse())))
    for h, f in original:
      assert f == f_at_h[h]
    for h, op_f in transformed:
      assert approx_equal(
        op_f,
        f_at_h[h*op.r()]*exp(1j*2*pi*row(h).dot(col(op.t().as_double()))))
コード例 #26
0
def exercise_SFweight_spline_core(structure, d_min, verbose=0):
  structure.scattering_type_registry(d_min=d_min)
  f_obs = abs(structure.structure_factors(
    d_min=d_min, anomalous_flag=False).f_calc())
  if (0 or verbose):
    f_obs.show_summary()
  f_obs = miller.array(
    miller_set=f_obs,
    data=f_obs.data(),
    sigmas=flex.sqrt(f_obs.data()))
  partial_structure = xray.structure(
    crystal_symmetry=structure,
    scatterers=structure.scatterers()[:-2])
  f_calc = f_obs.structure_factors_from_scatterers(
    xray_structure=partial_structure).f_calc()
  test_set_flags = (flex.random_double(size=f_obs.indices().size()) < 0.1)
  sfweight = clipper.SFweight_spline_interface(
    unit_cell=f_obs.unit_cell(),
    space_group=f_obs.space_group(),
    miller_indices=f_obs.indices(),
    anomalous_flag=f_obs.anomalous_flag(),
    f_obs_data=f_obs.data(),
    f_obs_sigmas=f_obs.sigmas(),
    f_calc=f_calc.data(),
    test_set_flags=test_set_flags,
    n_refln=f_obs.indices().size()//10,
    n_param=20)
  if (0 or verbose):
    print "number_of_spline_parameters:",sfweight.number_of_spline_parameters()
    print "mean fb: %.8g" % flex.mean(flex.abs(sfweight.fb()))
    print "mean fd: %.8g" % flex.mean(flex.abs(sfweight.fd()))
    print "mean phi: %.8g" % flex.mean(sfweight.centroid_phases())
    print "mean fom: %.8g" % flex.mean(sfweight.figures_of_merit())
  return sfweight
コード例 #27
0
def run(lstin):
    data = []
    for l in open(lstin):
        xdsasc = l.strip()
        xa = XDS_ASCII(xdsasc, sys.stdout, i_only=True)
        ma = miller.array(miller_set=xa.as_miller_set(anomalous_flag=False),
                          data=xa.iobs)
        data.append((xdsasc, ma))

    print "index filename"
    for i, d in enumerate(data):
        print i, d[0]

    print "i j n.i n.j n.common cc"
    for i in xrange(len(data) - 1):
        for j in xrange(i + 1, len(data)):
            di, dj = data[i][1].common_sets(data[j][1],
                                            assert_is_similar_symmetry=False)
            print i, j, data[i][1].data().size(), data[j][1].data().size(),
            if len(di.data()) == 0:
                print 0, "nan"
            else:
                corr = flex.linear_correlation(di.data(), dj.data())
                assert corr.is_well_defined()
                cc = corr.coefficient()
                print len(di.data()), cc
コード例 #28
0
def generate_table(complex_data, indices, numpy_args=False, anom=True):
    """

    :param complex_data: structure factors
    :param indices: miller indices in a list, Nx3
    :param numpy_args: are the complex data and indices numpy type, if not
        assume flex
    :param anom: return a miller array with +H and -H ?
    :return: dictionary whose keys are miller index tuple and values are structure fact
    """
    sg = sgtbx.space_group(" P 4nw 2abw")
    Symm = crystal.symmetry(unit_cell=(79, 79, 38, 90, 90, 90), space_group=sg)
    if numpy_args:
        assert type(indices) == tuple
        assert (type(indices[0]) == tuple)
        indices = flex.miller_index(indices)

    mil_set = miller.set(crystal_symmetry=Symm,
                         indices=indices,
                         anomalous_flag=anom)
    if numpy_args:
        complex_data = flex.complex_double(np.ascontiguousarray(complex_data))
    mil_ar = miller.array(mil_set, data=complex_data)

    mil_dict = {h: val for h, val in izip(mil_ar.indices(), mil_ar.data())}
    return mil_dict
コード例 #29
0
def exercise_recycle(space_group_info,
                     anomalous_flag,
                     n_scatterers=8,
                     d_min=2.5,
                     verbose=0):
    f_calc = random_f_calc(space_group_info=space_group_info,
                           n_scatterers=n_scatterers,
                           d_min=d_min,
                           anomalous_flag=anomalous_flag,
                           verbose=verbose)
    if (f_calc is None): return
    recycle(f_calc, "f_calc", verbose=verbose)
    for column_root_label, column_types in [("f_obs", None), ("Ework", "E")]:
        if (anomalous_flag and column_types == "E"): continue
        recycle(miller_array=abs(f_calc),
                column_root_label=column_root_label,
                column_types=column_types,
                verbose=verbose)
    if (not anomalous_flag):
        recycle(abs(f_calc), "f_obs", column_types="R", verbose=verbose)
    for column_root_label, column_types in [("f_obs", None), ("Ework", "EQ")]:
        if (anomalous_flag and column_types == "EQ"): continue
        recycle(miller_array=miller.array(miller_set=f_calc,
                                          data=flex.abs(f_calc.data()),
                                          sigmas=flex.abs(f_calc.data()) / 10),
                column_root_label=column_root_label,
                column_types=column_types,
                verbose=verbose)
    recycle(f_calc.centric_flags(), "cent", verbose=verbose)
    recycle(generate_random_hl(miller_set=f_calc), "prob", verbose=verbose)
コード例 #30
0
def scale_data(indices, iobs, scale_ref, parameter, calc_cc):
    k, b, cc = 1, float("nan"), float("nan")

    sortp = yamtbx_utils_ext.sort_permutation_fast_less(indices)
    indices = indices.select(sortp)
    iobs = iobs.select(sortp)

    sel0, sel1 = yamtbx_utils_ext.my_common_indices(scale_ref.indices(), indices)
    #indices = indices.select(sel1)
    iobs_c = iobs.select(sel1)
    ref_c = scale_ref.data().select(sel0)

    if iobs_c.size() < 10 and ref_c.size() < 10:
        return k, b, cc

    if parameter == "k":
        k = flex.sum(ref_c*iobs_c) / flex.sum(flex.pow2(iobs_c))
    elif parameter == "kb":
        from yamtbx.dataproc.scale_data import kBdecider
        kbd = kBdecider(scale_ref,
                        miller.array(scale_ref.customized_copy(indices=indices),data=iobs))
        k, b = kbd.run()
    else:
        raise "Never reaches here"
    
    if calc_cc:
        corr = flex.linear_correlation(ref_c, iobs_c)
        if corr.is_well_defined(): cc = corr.coefficient()

    return k, b, cc
コード例 #31
0
ファイル: read_ascii.py プロジェクト: dials/cctbx
 def as_miller_array(self,
       crystal_symmetry=None,
       force_symmetry=False,
       merge_equivalents=True,
       base_array_info=None,
       anomalous=None):
   if (base_array_info is None):
     base_array_info = miller.array_info(source_type="xds_ascii")
   crystal_symmetry_from_file = self.crystal_symmetry()
   array = (miller.array(
     miller_set=self.miller_set(
       crystal_symmetry=crystal_symmetry,
       force_symmetry=force_symmetry,
       anomalous=anomalous,
     ),
     data=self.iobs,
     sigmas=self.sigma_iobs)
     .set_info(base_array_info.customized_copy(
       labels=["iobs", "sigma_iobs"],
       crystal_symmetry_from_file=crystal_symmetry_from_file,
       wavelength=self.wavelength))
     .set_observation_type_xray_intensity())
   if (merge_equivalents):
     info = array.info()
     info.merged = True
     array = array.merge_equivalents().array().set_info(info)
   return array
コード例 #32
0
def generate_mtz_files(space_group_info, anomalous_flag):
    crystal_symmetry = crystal.symmetry(
        unit_cell=space_group_info.any_compatible_unit_cell(volume=1000),
        space_group_info=space_group_info)
    miller_set = miller.build_set(crystal_symmetry=crystal_symmetry,
                                  anomalous_flag=anomalous_flag,
                                  d_min=1)
    miller_array = miller.array(
        miller_set=miller_set,
        data=flex.random_double(size=miller_set.indices().size()))
    miller_array_p1 = miller_array.expand_to_p1()
    miller_arrays = []
    file_names = []
    subgrs = subgroups.subgroups(space_group_info).groups_parent_setting()
    for i_subgroup, subgroup in enumerate(subgrs):
        subgroup_miller_array = miller_array_p1.customized_copy(
          space_group_info=sgtbx.space_group_info(group=subgroup)) \
            .merge_equivalents() \
            .array() \
            .as_reference_setting() \
            .set_observation_type_xray_intensity()
        file_name = "tmp_refl_stats%d.mtz" % i_subgroup
        mtz_object = subgroup_miller_array.as_mtz_dataset(
            column_root_label="FOBS").mtz_object().write(file_name=file_name)
        miller_arrays.append(
            subgroup_miller_array.f_sq_as_f().expand_to_p1().map_to_asu())
        file_names.append(file_name)
    return miller_arrays, file_names
コード例 #33
0
  def __init__(self, obs,
               is_amplitude=True,
               weighting=None
               ):
    """
    Construct a least-square residuals

    .. |Sigma|  unicode:: U+003A3 .. GREEK CAPITAL LETTER SIGMA

    |Sigma|:sub:`i`  w[i] ( f_obs.data[i] - k abs(f_calc.data[i]) )^2
    /  |Sigma|:sub:`i` w[i] f_obs.data[i]^2

    or

    |Sigma|:sub:`i` w[i] ( f_obs_square.data[i] - k abs(f_calc.data[i])^2 )^2
    /  |Sigma|:sub:`i` w[i] f_obs_square.data[i]^2

    depending on which of f_obs and f_obs_square is not None.

    Note that
      - the sums are over the indices i of the reflections,
      - f_calc is to be passed to the __call__ method,
      - the weights w and the scale factor k are discussed below.

    :Parameters:

      obs : real miller.array
        the observed reflections, with F and sigma(F) (or F^2 and sigma(F^2))
        respectively in obs.data() and obs.sigmas()

      is_amplitude : bool
        a flag to discriminate the type of data in obs if the latter does not
        spell out whether it contains amplitudes or intensities;
        the default means that amplitudes is the default when data type is
        unknown.

      weighting
        a weighting scheme for the data (c.f. cctbx.xray.weighting for common
        ones) or None, which means no weights
    """
    if not(obs.is_xray_amplitude_array() or obs.is_xray_intensity_array()):
      self._obs = miller.array(obs, data=obs.data(), sigmas=obs.sigmas())
      if is_amplitude:
        self._obs.set_observation_type_xray_amplitude()
      else:
        self._obs.set_observation_type_xray_intensity()
    else:
      self._obs = obs
    assert(self._obs.is_xray_amplitude_array()
           or self._obs.is_xray_intensity_array())
    if self.obs().is_xray_amplitude_array():
      self._ext_ls_residual = ext.targets_least_squares_residual
      default_weighting = weighting_schemes.amplitude_unit_weighting()
    elif self.obs().is_xray_intensity_array():
      self._ext_ls_residual = ext.targets_least_squares_residual_for_intensity
      default_weighting = weighting_schemes.intensity_quasi_unit_weighting()
    if weighting is None: weighting = default_weighting
    self._weighting = weighting
    self._weighting.observed = self._obs
    self._scale_factor = None
コード例 #34
0
 def as_miller_array(self,
       crystal_symmetry=None,
       force_symmetry=False,
       merge_equivalents=True,
       base_array_info=None):
   if (base_array_info is None):
     base_array_info = miller.array_info(
       source_type="scalepack_no_merge_original_index")
   crystal_symmetry_from_file = self.crystal_symmetry()
   crystal_symmetry = crystal_symmetry_from_file.join_symmetry(
     other_symmetry=crystal_symmetry,
     force=force_symmetry)
   result = miller.array(
     miller_set=self.unmerged_miller_set(
       crystal_symmetry=crystal_symmetry,
       force_symmetry=True),
     data=self.i_obs,
     sigmas=self.sigmas)
   if (merge_equivalents):
     result = result.merge_equivalents().array()
   return (result
     .set_info(base_array_info.customized_copy(
       labels=["I(+)", "SIGI(+)", "I(-)", "SIGI(-)"],
       merged=merge_equivalents,
       crystal_symmetry_from_file=crystal_symmetry_from_file))
     .set_observation_type_xray_intensity())
コード例 #35
0
def df2m(df, cell, spgr, data=None, sigmas=None):
    """Constructs a miller.array from the columns specified by data/sigmas in the dataframe,
    if both are None, returns just the indices.
    needs cell and spgr to generate a symmetry object."""
    anomalous_flag = False

    if isinstance(df, pd.DataFrame):
        try:
            sel = df[data].notnull()  # select notnull data items for index
        except ValueError:
            index = df.index
        else:
            index = df.index[sel]
    else:
        index = df

    indices = flex.miller_index(index)

    if data:
        data = flex.double(df[data][sel])
    if sigmas:
        sigmas = flex.double(df[sigmas][sel])

    symm = make_symmetry(cell, spgr)
    ms = miller.set(
        crystal_symmetry=symm, indices=indices, anomalous_flag=anomalous_flag)
    return miller.array(ms, data=data, sigmas=sigmas)
コード例 #36
0
ファイル: reformat_gsas_rfl.py プロジェクト: rwgk/focus
def as_miller_array(gsas_exp, gsas_rfl, divide_pr, phase_id=1, histogram_id=1):
    from cctbx import miller
    from cctbx import crystal
    from cctbx.array_family import flex
    from scitbx.python_utils import easy_pickle
    info = gsas_exp.DESCR
    if (divide_pr):
        info += ", FIPS partitioning"
    indices = flex.miller_index()
    data = flex.double()
    if (not divide_pr):
        sigmas = flex.double()
        for r in gsas_rfl.records:
            indices.append(r.ihkl)
            data.append(r.fosq)
            sigmas.append(r.sig)
    else:
        sigmas = None
        for r in divide_pr.records:
            indices.append(r.hkl)
            data.append(r.fnew**2)
    miller_array = miller.array(
        miller_set=miller.set(crystal_symmetry=crystal.symmetry(
            unit_cell=gsas_exp.get_unit_cell_parameters(phase_id),
            space_group_symbol=gsas_exp.get_space_group_symbol(phase_id)),
                              indices=indices,
                              anomalous_flag=00000),
        data=data,
        sigmas=sigmas).set_info(info).set_observation_type_xray_intensity()
    miller_array.show_comprehensive_summary()
    print "Writing file: miller_array.pickle"
    easy_pickle.dump("miller_array.pickle", miller_array)
コード例 #37
0
ファイル: xds_pairwise_cc.py プロジェクト: harumome/kamo
def run(lstin):
    data = []
    for l in open(lstin):
        xdsasc = l.strip()
        xa = XDS_ASCII(xdsasc, sys.stdout, i_only=True)
        ma = miller.array(miller_set=xa.as_miller_set(anomalous_flag=False),
                          data=xa.iobs)
        data.append((xdsasc, ma))

    print "index filename"
    for i, d in enumerate(data):
        print i, d[0]

    print "i j n.i n.j n.common cc"
    for i in xrange(len(data)-1):
        for j in xrange(i+1, len(data)):
            di, dj = data[i][1].common_sets(data[j][1], assert_is_similar_symmetry=False)
            print i, j, data[i][1].data().size(), data[j][1].data().size(), 
            if len(di.data()) == 0:
                print 0, "nan"
            else:
                corr = flex.linear_correlation(di.data(), dj.data())
                assert corr.is_well_defined()
                cc =  corr.coefficient()
                print len(di.data()), cc
コード例 #38
0
def read_x(xfile, take_full=False):
    """
    according to http://www.hkl-xray.com/denzo-output

Regular (film output file, Denzo _ip) imaging plate output format (i.e. the format you would you to read in in FORTRAN) is:

format (3i4,i2,2f8.0,f7.0,f6.0,f6.0,2f7.0,f6.0,f8.0)
h,k,l
Flag 0 - full 1 - partial
Intensity (F**2) by profile fitting
s of intensity (F**2)
c2 of profile fitting
Intensity (F**2) by profile summation
Cosine of incidence angle at detector
Predicted pixel position of spot centroid (slow, fast) directions
Lorentz, polarization, obliquity combined factor
Strength of averaged profile in arbitrary units
    """

    lines = open(xfile).readlines()

    indices = flex.miller_index()
    data = flex.double()
    sigmas = flex.double()
    full_flags = flex.bool()
    cell, sg_str = None, None

    read_hkl = True

    for l in lines[5:]:
        if l.startswith(" 999") and len(l.split()) == 3:
            read_hkl = False

        if read_hkl:
            hkl = map(int, (l[0:4], l[4:8], l[8:12]))
            ispart = int(l[13])
            iobs, sigma = map(float, (l[14:22], l[22:30]))

            indices.append(hkl)
            data.append(iobs)
            sigmas.append(sigma)
            full_flags.append(ispart==0)
        else:
            if l.startswith("unit cell"):
                cell = map(float, l.split()[2:])
            elif l.startswith("space group"):
                sg_str = l.split()[-1]

    #sg_str="p1"
    symm = crystal.symmetry(unit_cell=cell, space_group=sg_str)

    array = miller.array(miller_set=miller.set(crystal_symmetry=symm,
                                               indices=indices,
                                               anomalous_flag=True),
                         data=data, sigmas=sigmas).set_observation_type_xray_intensity()

    if take_full:
        array = array.select(full_flags)

    return array
コード例 #39
0
ファイル: combat.py プロジェクト: vanbenschoten/combat
def aniso_convert(uc,sg,map,res):

  os.system('hkl2vtk %s_friedel.hkl %s_friedel.vtk %s_raw.vtk' %(map,map,map))
  os.system('vtk2lat %s_friedel.vtk %s_friedel.lat' %(map,map))
  os.system('avgrlt %s_friedel.lat %s_friedel.rf' %(map,map))
  os.system('subrflt %s_friedel.rf %s_friedel.lat anisotropic.lat' %(map,map))
  os.system('lat2hkl anisotropic.lat anisotropic.hkl')

  #Read in hkl file and populate miller array
  from cctbx import crystal
  inf = open('anisotropic.hkl', "r")
  indices = flex.miller_index()
  i_obs = flex.double()
  #sig_i = flex.double()
  for line in inf.readlines():
    assert len(line.split())==4
    line = line.strip().split()
    i_obs_ = float(line[3])#/10000 #10000 is a uniform scale factor meant to re-size all diffuse intensities (normally too large for scalepack)
    #sig_i_ = math.sqrt(i_obs_) 
    #if(abs(i_obs_)>1.e-6): # perhaps you don't want zeros

    if i_obs_ != -32768.0:
      indices.append([int(line[0]),int(line[1]),int(line[2])])
      i_obs.append(i_obs_)
    #sig_i.append(sig_i_)
  inf.close()

  #Get miller array object
  cs = crystal.symmetry(unit_cell=(float(uc[0]), float(uc[1]), float(uc[2]), float(uc[3]), float(uc[4]), float(uc[5])), space_group=sg)
  miller_set=miller.set(cs, indices)
  ma = miller.array(miller_set=miller_set, data=i_obs, sigmas=None)
  mtz_dataset = ma.as_mtz_dataset(column_root_label="Amplitude")
  mtz_dataset.mtz_object().write('%s_anisotropic.mtz' %map)
コード例 #40
0
ファイル: blend.py プロジェクト: nsls-ii-mx/yamtbx
    def cluster_completeness(self, clno, anomalous_flag, calc_redundancy=True):
        if clno not in self.clusters:
            print "Cluster No. %d not found" % clno
            return

        cls = self.clusters[clno][3]
        msets = map(lambda x: self.miller_sets[self.files[x-1]], cls)
        num_idx = sum(map(lambda x: x.size(), msets))
        all_idx = flex.miller_index()
        all_idx.reserve(num_idx)
        for mset in msets: all_idx.extend(mset.indices())

        # Calc median cell
        cells = numpy.array(map(lambda x: x.unit_cell().parameters(), msets))
        median_cell = map(lambda i: numpy.median(cells[:,i]), xrange(6))
        symm = msets[0].customized_copy(unit_cell=median_cell)

        assert anomalous_flag is not None
        # XXX all must belong to the same Laue group and appropriately reindexed..
        all_set = miller.set(indices=all_idx,
                             crystal_symmetry=symm, anomalous_flag=anomalous_flag)
        all_set = all_set.resolution_filter(d_min=self.d_min)

        # dummy for redundancy calculation. dirty way..
        if calc_redundancy:
            dummy_array = miller.array(miller_set=all_set, data=flex.int(all_set.size()))
            merge = dummy_array.merge_equivalents()
            cmpl = merge.array().completeness()
            redun = merge.redundancies().as_double().mean()
            return cmpl, redun
        else:
            cmpl = all_set.unique_under_symmetry().completeness()
            return cmpl
コード例 #41
0
ファイル: cctbx_utils.py プロジェクト: apeck12/cryoetX
def convert_to_sf(hkl, intensities, phases, cs):
    """
    Reformat intensities and phases into a CCTBX-style Miller array, with space group
    symmetry enforced. 

    Inputs:
    -------
    hkl: list of Miller indices, formatted as tuples
    intensities: array of intensities, with ordering matching hkl
    phases: array of phases with ordering matching hkl
    cs: CCTBX crystal.symmetry object

    Outputs:
    --------
    ma: CCTBX-style Miller array
    """
    # compute structure factors in complex number format
    if (phases.min() < -1*np.pi) or (phases.max() > np.pi):
        print "Error: Invalid phase values; may be in degrees rather than radians."
    A, B = np.sqrt(intensities)*np.cos(phases), np.sqrt(intensities)*np.sin(phases)
    B[np.abs(B)<1e-12] = 0

    # reformat miller indices and structure factor information into CCTBX format
    indices = flex.miller_index(hkl)
    sf_data = flex.complex_double(flex.double(A),flex.double(B))
    ma = miller.array(miller_set=miller.set(cs, indices, anomalous_flag=False), data=sf_data)

    return ma
コード例 #42
0
    def as_mtz(self, scale_factor, prefix):
        #This reads in an hkl map and returns a .mtz map
        #Read in hkl file and populate miller array
        inf = open(self.diffuse_file, 'r')
        indices = flex.miller_index()
        i_obs = flex.double()
        sig_i = flex.double()
        for line in inf.readlines():
            assert len(line.split()) == 4
            line = line.strip().split()
            #####ATTENTION:SCALE FACTOR##############
            i_obs_ = float(
                line[3]
            ) / scale_factor  #is a uniform scale factor meant to re-size all diffuse intensities (normally too large for scalepack)
            sig_i_ = math.sqrt(i_obs_)
            #if(abs(i_obs_)>1.e-6): # perhaps you don't want zeros
            indices.append([int(line[0]), int(line[1]), int(line[2])])
            i_obs.append(i_obs_)
            sig_i.append(sig_i_)
        inf.close()

        # get miller array object
        cs = self.symmetry
        ma = miller.array(miller_set=miller.set(cs, indices),
                          data=i_obs,
                          sigmas=sig_i)
        ma.set_observation_type_xray_intensity()
        mtz_dataset = ma.as_mtz_dataset(column_root_label="I")
        mtz_dataset.mtz_object().write(prefix + '.mtz')
コード例 #43
0
def merge_obs(indices, iobs, sel, symm, anomalous_flag, d_min, d_max):
    #indices = flex.miller_index(indices)
    #iobs = flex.double(iobs)
    if sel is not None and len(sel) > 0:
        sel = flex.bool(sel)
        indices = indices.select(sel)
        iobs = iobs.select(sel)

    miller_set = miller.set(crystal_symmetry=symm,
                            indices=indices,
                            anomalous_flag=anomalous_flag)

    array = miller.array(miller_set=miller_set,
                         data=iobs,
                         ).set_observation_type_xray_intensity()
    array = array.resolution_filter(d_min=d_min, d_max=d_max)

    ## New way
    #array = array.map_to_asu()
    #
    #merger = yamtbx_dataproc_crystfel_ext.merge_equivalents_crystfel()
    #merger.add_observations(array.indices(), array.data())
    #merger.merge()

    return array.merge_equivalents(algorithm="crystfel") # if sigmas is None, merge_equivalents_real() is used which simply averages.
コード例 #44
0
def generate_mtz_files(space_group_info, anomalous_flag):
  crystal_symmetry = crystal.symmetry(
    unit_cell=space_group_info.any_compatible_unit_cell(volume=1000),
    space_group_info=space_group_info)
  miller_set = miller.build_set(
    crystal_symmetry=crystal_symmetry,
    anomalous_flag=anomalous_flag,
    d_min=1)
  miller_array = miller.array(
    miller_set=miller_set,
    data=flex.random_double(size=miller_set.indices().size()))
  miller_array_p1 = miller_array.expand_to_p1()
  miller_arrays = []
  file_names = []
  subgrs = subgroups.subgroups(space_group_info).groups_parent_setting()
  for i_subgroup, subgroup in enumerate(subgrs):
    subgroup_miller_array = miller_array_p1.customized_copy(
      space_group_info=sgtbx.space_group_info(group=subgroup)) \
        .merge_equivalents() \
        .array() \
        .as_reference_setting() \
        .set_observation_type_xray_intensity()
    file_name = "tmp_refl_stats%d.mtz" % i_subgroup
    mtz_object = subgroup_miller_array.as_mtz_dataset(
      column_root_label="FOBS").mtz_object().write(file_name=file_name)
    miller_arrays.append(
      subgroup_miller_array.f_sq_as_f().expand_to_p1().map_to_asu())
    file_names.append(file_name)
  return miller_arrays, file_names
コード例 #45
0
def amplitude_quasi_normalisations(ma, d_star_power=1, set_to_minimum=None,
    pseudo_likelihood=False):  # Used for pseudo-likelihood calculation
    epsilons = ma.epsilons().data().as_double()
    mean_f_sq_over_epsilon = flex.double()
    for i_bin in ma.binner().range_used():
      sel = ma.binner().selection(i_bin)
      if pseudo_likelihood:
        sel_f_sq = flex.pow2(ma.data().select(sel)) # original method used
      else: # usual
        sel_f_sq = ma.data().select(sel)
      if (sel_f_sq.size() > 0):
        sel_epsilons = epsilons.select(sel)
        sel_f_sq_over_epsilon = sel_f_sq / sel_epsilons
        mean_f_sq_over_epsilon.append(flex.mean(sel_f_sq_over_epsilon))
      else:
        mean_f_sq_over_epsilon.append(0)
    mean_f_sq_over_epsilon_interp = ma.binner().interpolate(
      mean_f_sq_over_epsilon, d_star_power)
    if set_to_minimum and not mean_f_sq_over_epsilon_interp.all_gt(0):
      # HACK NO REASON THIS SHOULD WORK BUT IT GETS BY THE FAILURE
      sel = (mean_f_sq_over_epsilon_interp <= set_to_minimum)
      mean_f_sq_over_epsilon_interp.set_selected(sel,-mean_f_sq_over_epsilon_interp)
      sel = (mean_f_sq_over_epsilon_interp <= set_to_minimum)
      mean_f_sq_over_epsilon_interp.set_selected(sel,set_to_minimum)
    assert mean_f_sq_over_epsilon_interp.all_gt(0)
    from cctbx.miller import array
    return array(ma, flex.sqrt(mean_f_sq_over_epsilon_interp))
コード例 #46
0
 def as_miller_array(self,
       crystal_symmetry=None,
       force_symmetry=False,
       merge_equivalents=True,
       base_array_info=None):
   if (base_array_info is None):
     base_array_info = miller.array_info(
       source_type="scalepack_no_merge_original_index")
   crystal_symmetry_from_file = self.crystal_symmetry()
   crystal_symmetry = crystal_symmetry_from_file.join_symmetry(
     other_symmetry=crystal_symmetry,
     force=force_symmetry)
   result = miller.array(
     miller_set=self.unmerged_miller_set(
       crystal_symmetry=crystal_symmetry,
       force_symmetry=True),
     data=self.i_obs,
     sigmas=self.sigmas)
   if (merge_equivalents):
     result = result.merge_equivalents().array()
   return (result
     .set_info(base_array_info.customized_copy(
       labels=["I(+)", "SIGI(+)", "I(-)", "SIGI(-)"],
       merged=merge_equivalents,
       crystal_symmetry_from_file=crystal_symmetry_from_file))
     .set_observation_type_xray_intensity())
コード例 #47
0
ファイル: simple_strategy.py プロジェクト: dials/dials
  def __init__(self, strategies, n_bins=8, degrees_per_bin=5):
    from cctbx import crystal, miller
    import copy

    sg = strategies[0].experiment.crystal.get_space_group() \
      .build_derived_reflection_intensity_group(anomalous_flag=True)
    cs = crystal.symmetry(
      unit_cell=strategies[0].experiment.crystal.get_unit_cell(), space_group=sg)

    for i, strategy in enumerate(strategies):
      if i == 0:
        predicted = copy.deepcopy(strategy.predicted)
      else:
        predicted_ = copy.deepcopy(strategy.predicted)
        predicted_['dose'] += (flex.max(predicted['dose']) + 1)
        predicted.extend(predicted_)
    ms = miller.set(cs, indices=predicted['miller_index'], anomalous_flag=True)
    ma = miller.array(ms, data=flex.double(ms.size(),1),
                      sigmas=flex.double(ms.size(), 1))
    if 1:
      merging = ma.merge_equivalents()
      o = merging.array().customized_copy(
        data=merging.redundancies().data().as_double()).as_mtz_dataset('I').mtz_object()
      o.write('predicted.mtz')

    d_star_sq = ma.d_star_sq().data()

    binner = ma.setup_binner_d_star_sq_step(
      d_star_sq_step=(flex.max(d_star_sq)-flex.min(d_star_sq)+1e-8)/n_bins)

    dose = predicted['dose']
    range_width = 1
    range_min = flex.min(dose) - range_width
    range_max = flex.max(dose)
    n_steps = 2 + int((range_max - range_min) - range_width)

    binner_non_anom = ma.as_non_anomalous_array().use_binning(
      binner)
    self.n_complete = flex.size_t(binner_non_anom.counts_complete()[1:-1])

    from xia2.Modules.PyChef2 import ChefStatistics
    chef_stats = ChefStatistics(
      ma.indices(), ma.data(), ma.sigmas(),
      ma.d_star_sq().data(), dose, self.n_complete, binner,
      ma.space_group(), ma.anomalous_flag(), n_steps)

    def fraction_new(completeness):
      # Completeness so far at end of image
      completeness_end = completeness[1:]
      # Completeness so far at start of image
      completeness_start = completeness[:-1]
      # Fraction of unique reflections observed for the first time on each image
      return completeness_end - completeness_start

    self.dose = dose
    self.ieither_completeness = chef_stats.ieither_completeness()
    self.iboth_completeness = chef_stats.iboth_completeness()
    self.frac_new_ref = fraction_new(self.ieither_completeness) / degrees_per_bin
    self.frac_new_pairs = fraction_new(self.iboth_completeness) / degrees_per_bin
コード例 #48
0
ファイル: tst_cns_hl.py プロジェクト: cctbx/cctbx-playground
def verify(sg_fcalc, sg_hl, sg_cns, p1_cns):
  sg_phase_integrals = miller.array(
    miller_set=miller.set(
      crystal_symmetry=sg_fcalc,
      indices=sg_cns.miller_indices,
      anomalous_flag=sg_fcalc.anomalous_flag()),
    data=sg_cns.hl).phase_integrals()
  for h, cns_pi, miller_pi in zip(sg_cns.miller_indices,
                                  sg_cns.pi.data,
                                  sg_phase_integrals.data()):
    if (abs(cns_pi - miller_pi) > 1.e-2):
      print "Error:", h, cns_pi, miller_pi
      if (0): return
      raise AssertionError
  #
  p1_phase_integrals = miller.array(
    miller_set=miller.set(
      crystal_symmetry=sg_fcalc.cell_equivalent_p1(),
      indices=p1_cns.miller_indices,
      anomalous_flag=sg_fcalc.anomalous_flag()),
    data=p1_cns.hl).phase_integrals()
  for h, cns_pi, miller_pi in zip(p1_cns.miller_indices,
                                  p1_cns.pi.data,
                                  p1_phase_integrals.data()):
    if (abs(cns_pi - miller_pi) > 1.e-2):
      print "Error:", h, cns_pi, miller_pi
      if (0): return
      raise AssertionError
  #
  space_group = sg_fcalc.space_group()
  asu = sg_fcalc.space_group_info().reciprocal_space_asu()
  lookup_dict = miller.make_lookup_dict(sg_fcalc.indices())
  for p1_i, h in enumerate(p1_cns.miller_indices):
    h_asu = miller.asym_index(space_group, asu, h)
    h_eq = h_asu.one_column(sg_fcalc.anomalous_flag())
    fcalc_asu = h_eq.complex_eq(p1_cns.fcalc.data[p1_i])
    hl_asu = h_eq.hendrickson_lattman_eq(p1_cns.hl[p1_i])
    sg_i = lookup_dict[h_eq.h()]
    assert abs(sg_fcalc.data()[sg_i] - fcalc_asu) < 1.e-2
    if (not approx_equal(sg_hl[sg_i], hl_asu, eps=1.e-2)):
      print "Error:", sg_fcalc.space_group_info()
      print sg_fcalc.indices()[sg_i]
      print "i:", sg_hl[sg_i]
      print "o:", hl_asu
      if (0): return
      raise AssertionError
コード例 #49
0
ファイル: scale.py プロジェクト: cctbx/cctbx-playground
def run(show_plots,args):
  from xfel.command_line.cxi_merge import master_phil
  phil = iotbx.phil.process_command_line(args=args, master_string=master_phil).show()
  work_params = phil.work.extract()
  from xfel.merging.phil_validation import application,samosa
  application(work_params)
  samosa(work_params)
  if ("--help" in args) :
    libtbx.phil.parse(master_phil.show())
    return

  datadir = "."
  written_files = []
  if work_params.levmar.compute_cc_half:

    for half_data_flag in [1,2,0]:
      case = execute_case(datadir, work_params, plot=show_plots, half_data_flag=half_data_flag)
      assert len(case.Fit_I)==len(case.ordered_intensities.indices())==len(case.reference_millers.indices())
      model_subset = case.reference_millers[0:len(case.Fit_I)]
      fitted_miller_array = miller.array (miller_set = model_subset,
                                        data = case.Fit_I, sigmas = case.Fit_I_stddev)
      fitted_miller_array.set_observation_type_xray_intensity()
      output_result = fitted_miller_array.select(case.I_visited==1)
      outfile = "%s_s%1d_levmar.mtz"%(work_params.output.prefix,half_data_flag)
      output_result.show_summary(prefix="%s: "%outfile)
      mtz_out = output_result.as_mtz_dataset(column_root_label="Iobs",title=outfile,wavelength=None)
      mtz_obj = mtz_out.mtz_object()
      mtz_obj.write(outfile)
      written_files.append(outfile)
      print "OK s%1d"%half_data_flag
      #raw_input("OK?")

    """Guest code to retrieve the modified orientations after rotational fitting is done"""
    if "Rxy" in work_params.levmar.parameter_flags:
      all_A = [e.crystal.get_A() for e in case.experiments.get_experiments()]
      all_files = case.experiments.get_files()
      all_x = case.Fit["Ax"]
      all_y = case.Fit["Ay"]

      from scitbx import matrix
      x_axis = matrix.col((1.,0.,0.))
      y_axis = matrix.col((0.,1.,0.))
      out = open("aaaaa","w")
      for x in xrange(len(all_A)):
        Rx = x_axis.axis_and_angle_as_r3_rotation_matrix(angle=all_x[x], deg=True)
        Ry = y_axis.axis_and_angle_as_r3_rotation_matrix(angle=all_y[x], deg=True)
        modified_A = Rx * Ry * all_A[x]
        filename = all_files[x]
        print >>out, filename, " ".join([str(a) for a in modified_A.elems])



    work_params.scaling.algorithm="levmar"
    from xfel.cxi.cxi_cc import run_cc
    run_cc(work_params,work_params.model_reindex_op,sys.stdout)

  else:
    execute_case(datadir, work_params, plot=show_plots)
コード例 #50
0
 def as_miller_arrays(self,
                      crystal_symmetry=None,
                      force_symmetry=False,
                      merge_equivalents=True,
                      base_array_info=None):
   if (base_array_info is None):
     base_array_info = miller.array_info(source_type="xds_integrate_hkl")
   from cctbx.array_family import flex
   from cctbx import crystal, miller, sgtbx
   crystal_symmetry = crystal.symmetry(
     unit_cell=self.unit_cell,
     space_group_info=sgtbx.space_group_info(number=self.space_group))
   indices = flex.miller_index(self.hkl)
   miller_set = miller.set(crystal_symmetry, indices)
   return (miller.array(
     miller_set, data=flex.double(self.iobs), sigmas=flex.double(self.sigma))
           .set_info(base_array_info.customized_copy(
             labels=["iobs", "sigma_iobs"])),
           miller.array(miller_set, data=flex.vec3_double(self.xyzcal))
           .set_info(base_array_info.customized_copy(
             labels=["xyzcal"])),
           miller.array(miller_set, data=flex.vec3_double(self.xyzobs))
           .set_info(base_array_info.customized_copy(
             labels=["xyzobs"])),
           miller.array(miller_set, data=flex.double(self.rlp))
           .set_info(base_array_info.customized_copy(
             labels=["rlp"])),
           miller.array(miller_set, data=flex.double(self.peak))
           .set_info(base_array_info.customized_copy(
             labels=["peak"])),
           miller.array(miller_set, data=flex.double(self.corr))
           .set_info(base_array_info.customized_copy(
             labels=["corr"])),
           miller.array(miller_set, data=flex.double(self.maxc))
           .set_info(base_array_info.customized_copy(
             labels=["maxc"])),
           miller.array(miller_set, data=flex.vec2_double(self.alfbet0))
           .set_info(base_array_info.customized_copy(
             labels=["alfbet0"])),
           miller.array(miller_set, data=flex.vec2_double(self.alfbet1))
           .set_info(base_array_info.customized_copy(
             labels=["alfbet1"])),
           miller.array(miller_set, data=flex.double(self.psi))
           .set_info(base_array_info.customized_copy(
             labels=["psi"])))
コード例 #51
0
ファイル: xds_analyze_overlaps.py プロジェクト: harumome/kamo
def run(files):
    assert len(files) == 2

    hkl1 = xds_ascii.XDS_ASCII(files[0], sys.stdout)
    hkl2 = xds_ascii.XDS_ASCII(files[1], sys.stdout)

    hkl1_points = numpy.column_stack((hkl1.xd, hkl1.yd, hkl1.zd))
    tree1 = spatial.cKDTree(hkl1_points)

    n_ovl, n_nonovl = 0, 0

    novl_indices, novl_i, novl_sigma = flex.miller_index(), flex.double(), flex.double()

    for i in xrange(len(hkl2.indices)):
        x, y, z = hkl2.xd[i], hkl2.yd[i], hkl2.zd[i]
        #if z > 180:
        #    continue
        dists, idxs = tree1.query((x,y,z), k=3, p=1)

        overlaps = []
        for dist, idx in zip(dists, idxs):
            idx = int(idx)
            xo, yo, zo = hkl1.xd[idx], hkl1.yd[idx], hkl1.zd[idx]

            if abs(z-zo) < 2.5 and (xo-x)**2+(yo-y)**2 < 15**2: # FIXME MAGIC NUMBER!
                overlaps.append((dist,idx))

        if len(overlaps) == 0:
            novl_indices.append(hkl2.indices[i])
            novl_i.append(hkl2.iobs[i])
            novl_sigma.append(hkl2.sigma_iobs[i])
            n_nonovl += 1
        else:
            print hkl2.indices[i], x, y, z
            for dist, idx in overlaps:
                xo, yo, zo = hkl1.xd[idx], hkl1.yd[idx], hkl1.zd[idx]
                print hkl1.indices[idx], xo, yo, zo
                print dist, idx
            print

    print
    n_ref = len(hkl2.indices)
    print "%.2f%% overlap!" % (100.*(n_ref-n_nonovl)/n_ref)

    novl_array = miller.array(miller_set=miller.set(crystal_symmetry=hkl2.symm, indices=novl_indices),
                              data=novl_i, sigmas=novl_sigma)

    stats = dataset_statistics(novl_array, anomalous=False, sigma_filtering="xds")
    stats.show(out=sys.stdout)

    novl_array = novl_array.customized_copy(anomalous_flag=False).map_to_asu()
    novl_array = novl_array.eliminate_sys_absent()
    novl_array = novl_array.select(novl_array.sigmas() >= 0)

    filtr = filter_intensities_by_sigma(novl_array, "xds")
    hklout = os.path.splitext(os.path.basename(files[1]))[0] + "_novl.mtz"
    filtr.array_merged.set_observation_type_xray_intensity().as_mtz_dataset(column_root_label="IMEAN").mtz_object().write(hklout)
コード例 #52
0
def exercise(space_group_info, anomalous_flag,
             d_min=1.0, reflections_per_bin=200, n_bins=10, verbose=0):
  elements = ("N", "C", "C", "O") * 5
  structure_factors = random_structure.xray_structure(
    space_group_info,
    elements=elements,
    volume_per_atom=50.,
    min_distance=1.5,
    general_positions_only=True,
    use_u_aniso=False,
    u_iso=adptbx.b_as_u(10)
    ).structure_factors(
        anomalous_flag=anomalous_flag, d_min=d_min, algorithm="direct")
  if (0 or verbose):
    structure_factors.xray_structure().show_summary()
  asu_contents = dicts.with_default_value(0)
  for elem in elements: asu_contents[elem] += 1
  f_calc = abs(structure_factors.f_calc())
  f_calc.setup_binner(
    auto_binning=True,
    reflections_per_bin=reflections_per_bin,
    n_bins=n_bins)
  if (0 or verbose):
    f_calc.binner().show_summary()
  for k_given in [1,0.1,0.01,10,100]:
    f_obs = miller.array(
      miller_set=f_calc,
      data=f_calc.data()*k_given).set_observation_type_xray_amplitude()
    f_obs.use_binner_of(f_calc)
    wp = statistics.wilson_plot(f_obs, asu_contents, e_statistics=True)
    if (0 or verbose):
      print "wilson_k, wilson_b:", wp.wilson_k, wp.wilson_b
      print "space group:", space_group_info.group().type().hall_symbol()
      print "<E^2-1>:", wp.mean_e_sq_minus_1

    assert 0.8 < wp.wilson_k/k_given < 1.2
    assert 0.64 < wp.wilson_intensity_scale_factor/(k_given*k_given) < 1.44
    assert 9 < wp.wilson_b < 11
    assert wp.xy_plot_info().fit_correlation == wp.fit_correlation
    if space_group_info.group().is_centric():
      assert 0.90 < wp.mean_e_sq_minus_1 < 1.16
      assert 3.15 < wp.percent_e_sq_gt_2 < 6.5
    else:
      assert 0.65 < wp.mean_e_sq_minus_1 < 0.90
      assert 1.0 < wp.percent_e_sq_gt_2 < 3.15
    assert wp.normalised_f_obs.size() == f_obs.size()
  f_obs = f_calc.array(data=flex.double(f_calc.indices().size(), 0))
  f_obs.use_binner_of(f_calc)
  n_bins = f_obs.binner().n_bins_used()
  try:
    statistics.wilson_plot(f_obs, asu_contents)
  except RuntimeError, e:
    assert not show_diff(str(e), """\
wilson_plot error: %d empty bins:
  Number of bins: %d
  Number of f_obs > 0: 0
  Number of f_obs <= 0: %d""" % (n_bins, n_bins, f_obs.indices().size()))
コード例 #53
0
ファイル: map_tools.py プロジェクト: keitaroyam/cctbx_fork
def anomalous_residual_map_coefficients (fmodel, weighted=False,
    exclude_free_r_reflections=True) :
  """
  EXPERIMENTAL

  Calculates map coefficients showing the difference in anomalous scattering
  between F-obs and F-model.  Similar to the Phaser SAD LLG map, but appears
  to be less sensitive.
  """
  assert (fmodel.f_obs().anomalous_flag())
  f_obs_anom = fmodel.f_obs().anomalous_differences()
  f_model_anom = abs(fmodel.f_model()).anomalous_differences()
  if (weighted) :
    mch = fmodel.map_calculation_helper()
    fom = fmodel.f_obs().customized_copy(
      data=mch.fom, sigmas=None).average_bijvoet_mates()
    alpha = mch.alpha.average_bijvoet_mates()
    fom = fom.common_set(other=f_obs_anom)
    alpha = alpha.common_set(other=f_obs_anom)
    f_obs_anom = f_obs_anom.customized_copy(data=f_obs_anom.data()*fom.data())
    f_model_anom = f_model_anom.customized_copy(
      data=f_model_anom.data()*alpha.data())
  anom_diff_diff = f_obs_anom.customized_copy(
    data=f_obs_anom.data() - f_model_anom.data())
  f_model = fmodel.f_model().as_non_anomalous_array().\
    merge_equivalents().array()
  fmodel_match_anom_diff, anom_diff_diff_common = \
    f_model.common_sets(other =  anom_diff_diff)
  assert (anom_diff_diff_common.indices().size() ==
          anom_diff_diff.indices().size())
  phases_tmp = miller.array(
    miller_set=anom_diff_diff_common,
    data=flex.double(anom_diff_diff_common.indices().size(), 1)
    ).phase_transfer(phase_source=fmodel_match_anom_diff)
  map_coeffs = miller.array(
    miller_set=anom_diff_diff_common,
    data = anom_diff_diff_common.data() * phases_tmp.data())
  if (exclude_free_r_reflections) :
    r_free_flags = fmodel.r_free_flags().average_bijvoet_mates()
    r_free_flags, map_coeffs = r_free_flags.common_sets(map_coeffs)
    map_coeffs = map_coeffs.select(~(r_free_flags.data()))
  return miller.array(
    miller_set=map_coeffs,
    data=map_coeffs.data()/(2j))
コード例 #54
0
    def i_obs(self, anomalous_flag=None):
        assert "IOBS" in self.data
        assert "SIGMA" in self.data

        array_info = miller.array_info(source_type="xds_integrate")#, wavelength=)
        return miller.array(miller_set=miller.set(crystal_symmetry=self.crystal_symmetry(),
                                                  indices=self.hkl,
                                                  anomalous_flag=anomalous_flag),
                            data=self.data["IOBS"],
                            sigmas=self.data["SIGMA"]).set_info(array_info).set_observation_type_xray_intensity()
コード例 #55
0
def exercise_sys_absent_intensity_distribution():
  xs = crystal.symmetry((3,4,5), "F222")
  mi = flex.miller_index(((1,2,3), (1,1,1), (1,2,2), (0,0,4)))
  ms = miller.set(xs, mi)
  data = flex.double((-1,-2,3,4))
  sigmas = flex.double((2,3,4,5))
  f_obs = miller.array(ms, data=data, sigmas=sigmas).set_observation_type_xray_intensity()
  dist = statistics.sys_absent_intensity_distribution(f_obs)
  assert approx_equal(dist.x,(-0.5,0.75))
  assert approx_equal(dist.y,(-1,3))
  assert approx_equal(dist.indices,((1,2,3), (1,2,2)))
コード例 #56
0
ファイル: maxlik.py プロジェクト: cctbx/cctbx-playground
 def alpha_beta_for_each_reflection(self, f_obs=None):
   if f_obs is None: f_obs = self.f_obs
   alpha = flex.double(f_obs.size())
   beta = flex.double(f_obs.size())
   f_obs.setup_binner(n_bins= len(self.alpha_in_zones))
   binner = f_obs.binner()
   if(self.interpolation == True):
     az = flex.double(self.smooth(self.alpha_in_zones))
     bz = flex.double(self.smooth(self.beta_in_zones) )
     alpha = binner.interpolate(az, 0)
     beta  = binner.interpolate(bz, 0)
   elif(self.interpolation == False):
     for i_bin, az, bz in zip(binner.range_used(),self.alpha_in_zones,
                              self.beta_in_zones):
       sel = binner.selection(i_bin)
       alpha.set_selected(sel, az)
       beta.set_selected(sel, bz)
   alpha = miller.array(miller_set=f_obs, data=alpha)
   beta = miller.array(miller_set=f_obs, data=beta)
   return alpha, beta
コード例 #57
0
    def arrays(self):
        ret = {}

        for key in self.data:
            arr = miller.array(miller_set=miller.set(crystal_symmetry=self.crystal_symmetry(),
                                                     indices=self.hkl,
                                                     anomalous_flag=False),
                               data=self.data[key])
            ret[key] = arr

        return ret