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Python ui.clean函数代码示例

本文整理汇总了Python中sherpa.astro.ui.clean函数的典型用法代码示例。如果您正苦于以下问题:Python clean函数的具体用法?Python clean怎么用?Python clean使用的例子?那么恭喜您, 这里精选的函数代码示例或许可以为您提供帮助。


在下文中一共展示了clean函数的15个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。

示例1: test_xspecvar_no_grouping_comparison_xspec

def test_xspecvar_no_grouping_comparison_xspec(make_data_path,
                                               l, h, ndp, ndof, statval):
    """Compare chi2xspecvar values for a data set to XSPEC.

    The data set has a background. See
    test_xspecvar_no_grouping_no_bg_comparison_xspec

    The XSPEC version used was 12.9.0o.
    """

    dset = create_xspec_comparison_dataset(make_data_path,
                                           keep_background=True)

    # Lazy, so add it to "bad" channels too
    dset.counts += 5
    dset.get_background().counts += 3

    ui.clean()
    ui.set_data(dset)
    ui.subtract()

    ui.set_source(ui.powlaw1d.pl)
    ui.set_par('pl.ampl', 5e-4)

    ui.set_stat('chi2xspecvar')
    ui.set_analysis('energy')

    validate_xspec_result(l, h, ndp, ndof, statval)
    ui.clean()
开发者ID:DougBurke,项目名称:sherpa,代码行数:29,代码来源:test_astro_pha_scale.py

示例2: test_cstat_comparison_xspec

def test_cstat_comparison_xspec(make_data_path, l, h, ndp, ndof, statval):
    """Compare CSTAT values for a data set to XSPEC.

    This checks that the "UI layer" works, although ideally there
    should be a file that can be read in rather than having to
    manipulate it (the advantage here is that it means there is
    no messing around with adding a file to the test data set).

    The XSPEC version used was 12.9.0o.
    """

    dset = create_xspec_comparison_dataset(make_data_path,
                                           keep_background=False)

    ui.clean()
    ui.set_data(dset)
    # use powlaw1d rather than xspowerlaw so do not need XSPEC
    ui.set_source(ui.powlaw1d.pl)
    ui.set_par('pl.ampl', 1e-4)

    ui.set_stat('cstat')
    ui.set_analysis('channel')

    validate_xspec_result(l, h, ndp, ndof, statval)
    ui.clean()
开发者ID:DougBurke,项目名称:sherpa,代码行数:25,代码来源:test_astro_pha_scale.py

示例3: test_xspecvar_no_grouping_no_bg_comparison_xspec

def test_xspecvar_no_grouping_no_bg_comparison_xspec(make_data_path,
                                                     l, h, ndp, ndof, statval):
    """Compare chi2xspecvar values for a data set to XSPEC.

    The data set has no background.

    See test_cstat_comparison_xspec. Note that at present
    Sherpa and XSPEC treat bins with 0 values in them differently:
    see https://github.com/sherpa/sherpa/issues/356
    so for this test all bins are forced to have at least one
    count in them (source -> 5 is added per channel,background ->
    3 is added per channel).

    The XSPEC version used was 12.9.0o.
    """

    dset = create_xspec_comparison_dataset(make_data_path,
                                           keep_background=False)

    # Lazy, so add it to "bad" channels too
    dset.counts += 5

    ui.clean()
    ui.set_data(dset)

    ui.set_source(ui.powlaw1d.pl)
    ui.set_par('pl.ampl', 5e-4)

    ui.set_stat('chi2xspecvar')
    ui.set_analysis('energy')

    validate_xspec_result(l, h, ndp, ndof, statval)
    ui.clean()
开发者ID:DougBurke,项目名称:sherpa,代码行数:33,代码来源:test_astro_pha_scale.py

示例4: check_integrals

def check_integrals():
    """Check that Sherpa normed models integrate to 1."""
    from sherpa.astro import ui
    from sherpa.astro.ui import normgauss2d
    from models import normdisk2d, normshell2d
    
    ui.clean()
    
    g = normgauss2d('g')
    g.xpos, g.ypos, g.ampl, g.fwhm = 100, 100, 42, 5
    
    d = normdisk2d('d')
    d.xpos, d.ypos, d.ampl, d.r0 = 100, 100, 42, 50
    
    s = normshell2d('s')
    s.xpos, s.ypos, s.ampl, s.r0, s.width = 100, 100, 42, 30, 20
    
    models = [g, d, s]
    
    ui.dataspace2d((200, 200))
    for model in models:
        ui.set_model(model)
        # In sherpa normed model values are flux per pixel area.
        # So to get the total flux (represented by the `ampl` parameter)
        # one can simply sum over all pixels, because a pixel has area 1 pix^2.
        # :-) 
        integral = ui.get_model_image().y.sum()
        print model.name, integral
开发者ID:Cadair,项目名称:gammapy,代码行数:28,代码来源:test_models.py

示例5: setUp

 def setUp(self):
     datastack.clear_stack()
     datastack.set_template_id("__ID")
     ui.clean()
     self.ds = datastack.DataStack()
     self.loggingLevel = logger.getEffectiveLevel()
     logger.setLevel(logging.ERROR)
开发者ID:OrbitalMechanic,项目名称:sherpa,代码行数:7,代码来源:test_datastack.py

示例6: tearDown

    def tearDown(self):
        ui.clean()

        try:
            logger.setLevel(self._old_logger_level)
        except AttributeError:
            pass
开发者ID:DougBurke,项目名称:sherpa,代码行数:7,代码来源:test_wstat.py

示例7: clean_astro_ui

def clean_astro_ui():
    """Ensure sherpa.astro.ui.clean is called before AND after the test.

    This also resets the XSPEC settings (if XSPEC support is provided).

    See Also
    --------
    clean_ui

    Notes
    -----
    It does NOT change the logging level; perhaps it should, but the
    screen output is useful for debugging at this time.
    """
    from sherpa.astro import ui

    if has_xspec:
        old_xspec = xspec.get_xsstate()
    else:
        old_xspec = None

    ui.clean()
    yield

    ui.clean()
    if old_xspec is not None:
        xspec.set_xsstate(old_xspec)
开发者ID:DougBurke,项目名称:sherpa,代码行数:27,代码来源:conftest.py

示例8: cleanup_astro_session

def cleanup_astro_session(request):
    """Ensure sherpa.astro.ui is cleaned before and after the test."""
    ui.clean()

    def fin():
        ui.clean()

    request.addfinalizer(fin)
开发者ID:DougBurke,项目名称:sherpa,代码行数:8,代码来源:test_astro_data_rosat_unit.py

示例9: setUp

    def setUp(self):
        # hide warning messages from file I/O
        self._old_logger_level = logger.level
        logger.setLevel(logging.ERROR)

        ui.clean()

        self.head = self.make_path('acisf01575_001N001_r0085')
开发者ID:abigailStev,项目名称:sherpa,代码行数:8,代码来源:test_astro_ui_io.py

示例10: tearDown

 def tearDown(self):
     datastack.clear_stack()
     ui.clean()
     datastack.set_template_id("__ID")
     os.remove(self.lisname)
     os.remove(self.name1)
     os.remove(self.name2)
     datastack.set_stack_verbose(False)
     logger.setLevel(self.loggingLevel)
开发者ID:OrbitalMechanic,项目名称:sherpa,代码行数:9,代码来源:test_datastack.py

示例11: run_thread

 def run_thread(self, name, scriptname='fit.py'):
     ui.clean()
     ui.set_model_autoassign_func(self.assign_model)
     self.locals = {}
     cwd = os.getcwd()
     os.chdir(self.make_path('ciao4.3', name))
     try:
         execfile(scriptname, {}, self.locals)
     finally:
         os.chdir(cwd)
开发者ID:spidersaint,项目名称:sherpa,代码行数:10,代码来源:test_nan.py

示例12: test_load_xstable_model_fails_with_dir

def test_load_xstable_model_fails_with_dir():
    """Check that the function fails with invalid input: directory

    The temporary directory is used for this (the test is skipped if
    it does not exist).
    """

    ui.clean()
    assert ui.list_model_components() == []
    with pytest.raises(IOError):
        ui.load_xstable_model('tmpdir', tmpdir)

    assert ui.list_model_components() == []
开发者ID:DougBurke,项目名称:sherpa,代码行数:13,代码来源:test_astro_ui_utils_unit.py

示例13: test_load_table_model_fails_with_dev_null

def test_load_table_model_fails_with_dev_null():
    """Check that load_table_model fails with invalid input: /dev/null

    This simulates an empty file (and relies on the system
    containing a /dev/null file that reads in 0 bytes).
    """

    ui.clean()
    assert ui.list_model_components() == []

    # The error depends on the load function
    with pytest.raises(ValueError):
        ui.load_table_model('devnull', '/dev/null')

    assert ui.list_model_components() == []
开发者ID:DougBurke,项目名称:sherpa,代码行数:15,代码来源:test_astro_ui_utils_unit.py

示例14: clean

def clean():
    """Remove the models and data from the data stack and Sherpa.

    This function clears out the models and data set up in the data
    stack and in the Sherpa session.

    See Also
    --------
    clear_models, clear_stack
    sherpa.astro.ui.clean
    """
    DATASTACK.clear_models()
    DATASTACK.clear_stack()
    ui.clean()
    logger.warning("clean() will invalidate any existing DataStack instances by removing all the datasets from the " +
                   "Sherpa session")
开发者ID:OrbitalMechanic,项目名称:sherpa,代码行数:16,代码来源:__init__.py

示例15: run_hspec_fit

    def run_hspec_fit(self, model, thres_low, thres_high):
        """Run the gammapy.hspec fit

        Parameters
        ----------
        model : str
            Sherpa model
        thres_high : `~gammapy.spectrum.Energy`
            Upper threshold of the spectral fit
        thres_low : `~gammapy.spectrum.Energy`
            Lower threshold of the spectral fit
        """

        log.info("Starting HSPEC")
        import sherpa.astro.ui as sau
        from ..hspec import wstat
        from sherpa.models import PowLaw1D

        if model == 'PL':
            p1 = PowLaw1D('p1')
            p1.gamma = 2.2
            p1.ref = 1e9
            p1.ampl = 6e-19
        else:
            raise ValueError('Desired Model is not defined')

        thres = thres_low.to('keV').value
        emax = thres_high.to('keV').value

        sau.freeze(p1.ref)
        sau.set_conf_opt("max_rstat", 100)

        list_data = []
        for obs in self.observations:
            datid = obs.phafile.parts[-1][7:12]
            sau.load_data(datid, str(obs.phafile))
            sau.notice_id(datid, thres, emax)
            sau.set_source(datid, p1)
            list_data.append(datid)
        wstat.wfit(list_data)
        sau.covar()
        fit_val = sau.get_covar_results()
        fit_attrs = ('parnames', 'parvals', 'parmins', 'parmaxes')
        fit = dict((attr, getattr(fit_val, attr)) for attr in fit_attrs)
        fit = self.apply_containment(fit)
        sau.clean()
        self.fit = fit
开发者ID:JouvinLea,项目名称:gammapy,代码行数:47,代码来源:spectrum_analysis.py


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