Source code for yt.frontends.fits.misc

Miscellaneous FITS routines

# Copyright (c) 2013, yt Development Team.
# Distributed under the terms of the Modified BSD License.
# The full license is in the file COPYING.txt, distributed with this software.

import numpy as np
import base64
from yt.extern.six import PY3
from yt.fields.derived_field import ValidateSpatial
from yt.funcs import mylog
from yt.utilities.on_demand_imports import _astropy
from yt.units.yt_array import YTQuantity, YTArray
if PY3:
    from io import BytesIO as IO
    from yt.extern.six.moves import StringIO as IO

import os

def _make_counts(emin, emax):
    def _counts(field, data):
        e = data["event_energy"].in_units("keV")
        mask = np.logical_and(e >= emin, e < emax)
        x = data["event_x"][mask]
        y = data["event_y"][mask]
        z = np.ones(x.shape)
        pos = np.array([x,y,z]).transpose()
        img = data.deposit(pos, method="count")
        if data.has_field_parameter("sigma"):
            sigma = data.get_field_parameter("sigma")
            sigma = None
        if sigma is not None and sigma > 0.0:
            kern = _astropy.conv.Gaussian2DKernel(stddev=sigma)
            img[:,:,0] = _astropy.conv.convolve(img[:,:,0], kern)
        return data.ds.arr(img, "counts/pixel")
    return _counts

[docs]def setup_counts_fields(ds, ebounds, ftype="gas"): r""" Create deposited image fields from X-ray count data in energy bands. Parameters ---------- ds : ~yt.data_objects.static_output.Dataset The FITS events file dataset to add the counts fields to. ebounds : list of tuples A list of tuples, one for each field, with (emin, emax) as the energy bounds for the image. ftype : string, optional The field type of the resulting field. Defaults to "gas". Examples -------- >>> ds = yt.load("evt.fits") >>> ebounds = [(0.1,2.0),(2.0,3.0)] >>> setup_counts_fields(ds, ebounds) """ for (emin, emax) in ebounds: cfunc = _make_counts(emin, emax) fname = "counts_%s-%s" % (emin, emax)"Creating counts field %s." % fname) ds.add_field((ftype,fname), sampling_type="cell", function=cfunc, units="counts/pixel", validators = [ValidateSpatial()], display_name="Counts (%s-%s keV)" % (emin, emax))
[docs]def create_spectral_slabs(filename, slab_centers, slab_width, **kwargs): r""" Given a dictionary of spectral slab centers and a width in spectral units, extract data from a spectral cube at these slab centers and return a `FITSDataset` instance containing the different slabs as separate yt fields. Useful for extracting individual lines from a spectral cube and separating them out as different fields. Requires the SpectralCube ( library. All keyword arguments will be passed on to the `FITSDataset` constructor. Parameters ---------- filename : string The spectral cube FITS file to extract the data from. slab_centers : dict of (float, string) tuples or YTQuantities The centers of the slabs, where the keys are the names of the new fields and the values are (float, string) tuples or YTQuantities, specifying a value for each center and its unit. slab_width : YTQuantity or (float, string) tuple The width of the slab along the spectral axis. Examples -------- >>> slab_centers = {'13CN': (218.03117, 'GHz'), ... 'CH3CH2CHO': (218.284256, 'GHz'), ... 'CH3NH2': (218.40956, 'GHz')} >>> slab_width = (0.05, "GHz") >>> ds = create_spectral_slabs("intensity_cube.fits", ... slab_centers, slab_width, ... nan_mask=0.0) """ from spectral_cube import SpectralCube from yt.visualization.fits_image import FITSImageData from yt.frontends.fits.api import FITSDataset cube = if not isinstance(slab_width, YTQuantity): slab_width = YTQuantity(slab_width[0], slab_width[1]) slab_data = {} field_units = cube.header.get("bunit", "dimensionless") for k, v in slab_centers.items(): if not isinstance(v, YTQuantity): slab_center = YTQuantity(v[0], v[1]) else: slab_center = v"Adding slab field %s at %g %s" % (k, slab_center.v, slab_center.units)) slab_lo = (slab_center-0.5*slab_width).to_astropy() slab_hi = (slab_center+0.5*slab_width).to_astropy() subcube = cube.spectral_slab(slab_lo, slab_hi) slab_data[k] = YTArray(subcube.filled_data[:,:,:], field_units) width = subcube.header["naxis3"]*cube.header["cdelt3"] w = subcube.wcs.copy() w.wcs.crpix[-1] = 0.5 w.wcs.crval[-1] = -0.5*width fid = FITSImageData(slab_data, wcs=w) for hdu in fid: hdu.header.pop("RESTFREQ", None) hdu.header.pop("RESTFRQ", None) ds = FITSDataset(fid, **kwargs) return ds
[docs]def ds9_region(ds, reg, obj=None, field_parameters=None): r""" Create a data container from a ds9 region file. Requires the pyregion package ( to be installed. Parameters ---------- ds : FITSDataset The Dataset to create the region from. reg : string The filename of the ds9 region, or a region string to be parsed. obj : data container, optional The data container that will be used to create the new region. Defaults to ds.all_data. field_parameters : dictionary, optional A set of field parameters to apply to the region. Examples -------- >>> ds = yt.load("m33_hi.fits") >>> circle_region = ds9_region(ds, "circle.reg") >>> print circle_region.quantities.extrema("flux") """ import pyregion if os.path.exists(reg): r = else: r = pyregion.parse(reg) reg_name = reg filter = r.get_filter(header=ds.wcs_2d.to_header()) nx = ds.domain_dimensions[ds.lon_axis] ny = ds.domain_dimensions[ds.lat_axis] mask = filter.mask((ny,nx)).transpose() if ds.events_data: prefix = "event_" else: prefix = "" def _reg_field(field, data): i = data[prefix+"xyz"[ds.lon_axis]].d.astype("int")-1 j = data[prefix+"xyz"[ds.lat_axis]].d.astype("int")-1 new_mask = mask[i,j] ret = np.zeros(data[prefix+"x"].shape) ret[new_mask] = 1. return ret ds.add_field(("gas", reg_name), sampling_type="cell", function=_reg_field) if obj is None: obj = ds.all_data() if field_parameters is not None: for k,v in field_parameters.items(): obj.set_field_parameter(k,v) return obj.cut_region(["obj['%s'] > 0" % (reg_name)])
[docs]class PlotWindowWCS(object): r""" Use the wcsaxes library to plot celestial coordinates on the axes of a on-axis PlotWindow plot. See for details. Parameters ---------- pw : on-axis PlotWindow instance The PlotWindow instance to add celestial axes to. """ def __init__(self, pw): from wcsaxes import WCSAxes if pw.oblique: raise NotImplementedError("WCS axes are not implemented for oblique plots.") if not hasattr(pw.ds, "wcs_2d"): raise NotImplementedError("WCS axes are not implemented for this dataset.") if pw.data_source.axis != pw.ds.spec_axis: raise NotImplementedError("WCS axes are not implemented for this axis.") self.plots = {} = pw for f in pw.plots: rect = pw.plots[f]._get_best_layout()[1] fig = pw.plots[f].figure ax = fig.axes[0] wcs_ax = WCSAxes(fig, rect, wcs=pw.ds.wcs_2d, frameon=False) fig.add_axes(wcs_ax) wcs = pw.ds.wcs_2d.wcs xax = pw.ds.coordinates.x_axis[pw.data_source.axis] yax = pw.ds.coordinates.y_axis[pw.data_source.axis] xlabel = "%s (%s)" % (wcs.ctype[xax].split("-")[0], wcs.cunit[xax]) ylabel = "%s (%s)" % (wcs.ctype[yax].split("-")[0], wcs.cunit[yax]) fp = pw._font_properties wcs_ax.coords[0].set_axislabel(xlabel, fontproperties=fp, minpad=0.5) wcs_ax.coords[1].set_axislabel(ylabel, fontproperties=fp, minpad=0.4) wcs_ax.coords[0].ticklabels.set_fontproperties(fp) wcs_ax.coords[1].ticklabels.set_fontproperties(fp) ax.xaxis.set_visible(False) ax.yaxis.set_visible(False) wcs_ax.set_xlim(pw.xlim[0].value, pw.xlim[1].value) wcs_ax.set_ylim(pw.ylim[0].value, pw.ylim[1].value) wcs_ax.coords.frame._update_cache = [] ax.xaxis.set_visible(False) ax.yaxis.set_visible(False) self.plots[f] = fig
[docs] def keys(self): return self.plots.keys()
[docs] def values(self): return self.plots.values()
[docs] def items(self): return self.plots.items()
def __getitem__(self, key): for k in self.keys(): if k[1] == key: return self.plots[k]
[docs] def show(self): return self
[docs] def save(self, name=None, mpl_kwargs=None): if mpl_kwargs is None: mpl_kwargs = {} mpl_kwargs["bbox_inches"] = "tight", mpl_kwargs=mpl_kwargs)
def _repr_html_(self): from yt.visualization._mpl_imports import FigureCanvasAgg ret = '' for k, v in self.plots.items(): canvas = FigureCanvasAgg(v) f = IO() canvas.print_figure(f) img = base64.b64encode( ret += r'<img style="max-width:100%%;max-height:100%%;" ' \ r'src="data:image/png;base64,%s"><br>' % img return ret