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Python ui.get_data函数代码示例

本文整理汇总了Python中sherpa.astro.ui.get_data函数的典型用法代码示例。如果您正苦于以下问题:Python get_data函数的具体用法?Python get_data怎么用?Python get_data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get_data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: __init__

    def __init__(self, name, filename):  # name means datid!!
        self.name = name
        sau.load_pha(name, filename)
        self.data = sau.get_data(name)
        self.arf = sau.get_data(name)
        self.rmf = sau.get_data(name)

        try:  # Read keywords from pha header
            self.threshold = self.data.header['ETH']
        except KeyError:
            print(" ! WARNING: no threshold found, using 200 GeV")
            self.threshold = 2e8  # default value 200 GeV
        self.emax = 1e11  # default value 100 TeV

        try:
            self.zenith = self.data.header['ZENITH']
        except KeyError:
            print("WARNING: no mean zenith angle found, using 45 deg")
            self.zenith = 45.0  # default value 200 GeV

        try:
            self.offset = self.data.header['OFFSET']
        except KeyError:
            print("WARNING: no offset angle found, using 1.0 deg")
            self.offset = 1.0  # default value 200 GeV

        try:
            self.telcode = self.data.header['TELCODE']
        except KeyError:
            print("WARNING: no telcode found, using 0")
            self.telcode = 0  # default value 200 GeV
开发者ID:JonathanDHarris,项目名称:gammapy,代码行数:31,代码来源:read_spectra.py

示例2: __init__

    def __init__(self, name, filename=None):
        self.name = name
        if filename is not None:
            sau.load_pha(name, filename)
            self.data = sau.get_data(name)
            self.arf = self.data.get_arf()
            self.rmf = self.data.get_rmf()

            # Read keywords from pha header
            try:
                self.threshold = self.data.header['ETH']
            except KeyError:
                print("WARNING: no threshold found using 200 GeV")
                self.threshold = 2e8  # default value 200 GeV
                self.emax = 1e11  # default value 100 TeV

            try:
                self.zenith = self.data.header['ZENITH']
            except KeyError:
                print("WARNING: no mean zenith angle found using 45 deg")
                self.zenith = 45.0  # default value 45 deg

            try:
                self.offset = self.data.header['OFFSET']
            except KeyError:
                print("WARNING: no offset angle found using 1.0 deg")
                self.offset = 1.0  # default value 1 deg

            try:
                self.n_tels = self.data.header['N_TELS']
            except KeyError:
                print("WARNING: no number of telescopes found using 0")
                self.n_tels = 0  # default value

            try:
                self.eff = self.data.header['EFFICIEN']
            except KeyError:
                print("WARNING: no efficiency found using 1.0")
                self.eff = 1.00  # default value

            try:
                self.tstart = self.data.header['TSTART']
            except KeyError:
                print("WARNING: no tstart found using 0")
                self.tstart = 0.  # default value

            try:
                self.tstop = self.data.header['TSTOP']
            except KeyError:
                print("WARNING: no tstop found using tsart+1800")
                self.tstop = self.tstart + 1800  # default value

        else:
            self.data = sau.get_data(name)
            self.arf = self.data.get_arf()
            self.rmf = self.data.get_rmf()
开发者ID:astrofrog,项目名称:gammapy,代码行数:56,代码来源:specsource.py

示例3: query

 def query(self, func):
     output = []
     for dataset in self.filter_datasets():
         id = dataset['id']
         if func(ui.get_data(id)):
             output.append(id)
     return output
开发者ID:anetasie,项目名称:sherpa,代码行数:7,代码来源:__init__.py

示例4: center_psf

    def center_psf(self):
        """Set ``xpos`` and ``ypos`` of the PSF to the dataspace center."""
        import sherpa.astro.ui as sau
        try:
            ny, nx = sau.get_data().shape
            for _ in ['psf1', 'psf2', 'psf3']:
                par = sau.get_par(_ + '.xpos')
                par.val = nx / 2.

                par = sau.get_par(_ + '.ypos')
                par.val = ny / 2.
        except:
            raise Exception('PSF is not centered.')
开发者ID:dlennarz,项目名称:gammapy,代码行数:13,代码来源:psf_core.py

示例5: setUp

    def setUp(self):

        self._old_logger_level = logger.getEffectiveLevel()
        logger.setLevel(logging.ERROR)

        ui.set_stat('wstat')

        infile = self.make_path('3c273.pi')
        ui.load_pha(1, infile)

        # Change the backscale value slightly so that the
        # results are different to other runs with this file.
        #
        nbins = ui.get_data(1).get_dep(False).size
        bscal = 0.9 * np.ones(nbins) * ui.get_backscal(1)
        ui.set_backscal(1, backscale=bscal)

        ui.set_source(1, ui.powlaw1d.pl)

        # The powerlaw slope and normalization are
        # intended to be "a reasonable approximation"
        # to the data, just to make sure that any statistic
        # calculation doesn't blow-up too much.
        #
        ui.set_par("pl.gamma", 1.7)
        ui.set_par("pl.ampl", 1.7e-4)
开发者ID:DougBurke,项目名称:sherpa,代码行数:26,代码来源:test_wstat.py

示例6: validate_pha

    def validate_pha(self, idval):
        """Check that the PHA dataset in id=idval is
        as expected.
        """

        self.assertEqual(ui.list_data_ids(), [idval])

        pha = ui.get_data(idval)
        self.assertIsInstance(pha, DataPHA)

        arf = ui.get_arf(idval)
        self.assertIsInstance(arf, ARF1D)

        rmf = ui.get_rmf(idval)
        self.assertIsInstance(rmf, RMF1D)

        bpha = ui.get_bkg(idval, bkg_id=1)
        self.assertIsInstance(bpha, DataPHA)

        barf = ui.get_arf(idval, bkg_id=1)
        self.assertIsInstance(barf, ARF1D)

        brmf = ui.get_rmf(idval, bkg_id=1)
        self.assertIsInstance(brmf, RMF1D)

        # normally the background data set would have a different name,
        # but this is a  PHA Type 3 file.
        # self.assertEqual(pha.name, bpha.name)
        self.assertEqual(arf.name, barf.name)
        self.assertEqual(rmf.name, brmf.name)
开发者ID:abigailStev,项目名称:sherpa,代码行数:30,代码来源:test_astro_ui_io.py

示例7: test_load_table_fits

 def test_load_table_fits(self):
     # QUS: why is this not in the sherpa-test-data repository?
     this_dir = os.path.dirname(os.path.abspath(__file__))
     ui.load_table(1, os.path.join(this_dir, 'data', 'two_column_x_y.fits.gz'))
     data = ui.get_data(1)
     self.assertEqualWithinTol(data.x, [1, 2, 3])
     self.assertEqualWithinTol(data.y, [4, 5, 6])
开发者ID:spidersaint,项目名称:sherpa,代码行数:7,代码来源:test_astro_ui.py

示例8: setUp

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

        self._id = 1
        fname = self.make_path('3c273.pi')
        ui.load_pha(self._id, fname)
        self._pha = ui.get_data(self._id)
开发者ID:OrbitalMechanic,项目名称:sherpa,代码行数:9,代码来源:test_astro_ui.py

示例9: _check_stat

    def _check_stat(self, nbins, expected):

        # check the filter sizes (mainly so that these tests
        # get flagged as in need of a look if anything changes
        # in other parts of the code, such as filtering and binning
        #
        self.assertEqual(nbins, ui.get_data().get_dep(True).size)

        stat = ui.calc_stat()
        self.assertAlmostEqual(expected, stat, places=7)
开发者ID:DougBurke,项目名称:sherpa,代码行数:10,代码来源:test_wstat.py

示例10: testReadImplicit

    def testReadImplicit(self):
        """Exclude .gz from the file name"""

        idval = "13"
        fname = self.head + '_pha3.fits'
        ui.load_pha(idval, fname)

        self.validate_pha(idval)

        pha = ui.get_data(idval)
        bpha = ui.get_bkg(idval, bkg_id=1)
        self.assertEqual(pha.name, bpha.name)
开发者ID:abigailStev,项目名称:sherpa,代码行数:12,代码来源:test_astro_ui_io.py

示例11: center_psf

 def center_psf(self):
     """Set xpos and ypos of the PSF to the dataspace center"""
     import sherpa.astro.ui as sau
     try:
         ny, nx = sau.get_data().shape
         for par in sau.get_psf().kernel.pars:
             if par.name is 'xpos':
                 par.val = (nx + 1) / 2.
             elif par.name is 'ypos':
                 par.val = (ny + 1) / 2.
     except:
         logging.warning('PSF is not centered.')
开发者ID:ignasi-reichardt,项目名称:gammapy,代码行数:12,代码来源:psf.py

示例12: center_psf

 def center_psf(self):
     """Set ``xpos`` and ``ypos`` of the PSF to the dataspace center."""
     import sherpa.astro.ui as sau
     try:
         ny, nx = sau.get_data().shape
         for par in sau.get_psf().kernel.pars:
             if par.name is 'xpos':
                 par.val = (nx + 1) / 2.
             elif par.name is 'ypos':
                 par.val = (ny + 1) / 2.
     except:
         raise Exception('PSF is not centered.')
开发者ID:mwcraig,项目名称:gammapy,代码行数:12,代码来源:psf.py

示例13: containment_fraction

 def containment_fraction(self, theta, npix=1000):
     """Compute fraction of PSF contained inside theta."""
     import sherpa.astro.ui as sau
     sau.dataspace2d((npix, npix))
     self.set()
     # x_center = get_psf().kernel.pars.xpos
     # y_center = get_psf().kernel.pars.ypos
     x_center, y_center = sau.get_psf().model.center
     x_center, y_center = x_center + 0.5, y_center + 0.5  # shift seen on image.
     x, y = sau.get_data().x0, sau.get_data().x1
     # @note Here we have to use the source image, before I used
     # get_model_image(), which returns the PSF-convolved PSF image,
     # which is a factor of sqrt(2) ~ 1.4 too wide!!!
     p = sau.get_source_image().y.flatten()
     p /= np.nansum(p)
     mask = (x - x_center) ** 2 + (y - y_center) ** 2 < theta ** 2
     fraction = np.nansum(p[mask])
     if 0:  # debug
         sau.get_data().y = p
         sau.save_data('psf_sherpa.fits', clobber=True)
         sau.get_data().y = mask.astype('int')
         sau.save_data('mask_sherpa.fits', clobber=True)
     return fraction
开发者ID:mwcraig,项目名称:gammapy,代码行数:23,代码来源:psf.py

示例14: testReadExplicit

    def testReadExplicit(self):
        """Include .gz in the file name"""

        idval = 12
        fname = self.head + '_pha3.fits.gz'
        ui.load_pha(idval, fname)

        self.validate_pha(idval)

        # TODO: does this indicate that the file name, as read in,
        #       should have the .gz added to it to match the data
        #       read in, or left as is?
        pha = ui.get_data(idval)
        bpha = ui.get_bkg(idval, bkg_id=1)
        self.assertEqual(pha.name, bpha.name + '.gz')
开发者ID:abigailStev,项目名称:sherpa,代码行数:15,代码来源:test_astro_ui_io.py

示例15: test_xmm2

 def test_xmm2(self):
     self.run_thread('xmm2')
     self.assertEqualWithinTol(ui.get_data().channel[0], 1.0, 1e-4)
     self.assertEqual(ui.get_rmf().detchans, 800)
     self.assertEqual(len(ui.get_rmf().energ_lo), 2400)
     self.assertEqual(len(ui.get_rmf().energ_hi), 2400)
     self.assertEqual(len(ui.get_rmf().n_grp), 2400)
     self.assertEqual(len(ui.get_rmf().f_chan), 2394)
     self.assertEqual(len(ui.get_rmf().n_chan), 2394)
     self.assertEqual(len(ui.get_rmf().matrix), 1281216)
     self.assertEqual(ui.get_rmf().offset, 0)
     self.assertEqual(len(ui.get_rmf().e_min), 800)
     self.assertEqual(len(ui.get_rmf().e_max), 800)
     self.assertEqual(len(ui.get_arf().energ_lo), 2400)
     self.assertEqual(len(ui.get_arf().energ_hi), 2400)
     self.assertEqual(len(ui.get_arf().specresp), 2400)
开发者ID:valkenar,项目名称:sherpa,代码行数:16,代码来源:test_astro.py


注:本文中的sherpa.astro.ui.get_data函数示例由纯净天空整理自Github/MSDocs等开源代码及文档管理平台,相关代码片段筛选自各路编程大神贡献的开源项目,源码版权归原作者所有,传播和使用请参考对应项目的License;未经允许,请勿转载。