Hips2fits new service

astroquery/hips2fits/__init__.py

@@ -0,0 +1,44 @@
+# Licensed under a 3-clause BSD style license - see LICENSE.rst
+"""
+CDS hips2fits Query Tool
+------------------------
+
+:Author: Matthieu Baumann (matthieu.baumann@astro.unistra.fr)
+
+This package is for querying the CDS hips2fits service, primarily hosted at:
+
+* http://alasky.u-strasbg.fr/hips-image-services/hips2fits
+* http://alaskybis.u-strasbg.fr/hips-image-services/hips2fits (mirror)
+
+Note: If the access to hips2fits was helpful for your research
+work, the following acknowledgment would be appreciated::
+
+  This research has made use of the hips2fits, a tool developed at CDS, Strasbourg, France aiming at extracting
+  FITS images from HiPS sky maps with respect to a WCS.
+"""
+
+from astropy import config as _config
+
+
+class Conf(_config.ConfigNamespace):
+    """
+    Configuration parameters for ``astroquery.template_module``.
+    """
+    server = _config.ConfigItem(
+        ["http://alasky.u-strasbg.fr/hips-image-services/hips2fits",
+         "http://alaskybis.u-strasbg.fr/hips-image-services/hips2fits"],
+        'Name of the template_module server to use.')
+
+    timeout = _config.ConfigItem(
+        30,
+        'Time limit for connecting to template_module server.')
+
+
+conf = Conf()
+
+from .core import hips2fits, hips2fitsClass
+
+__all__ = [
+    'hips2fits', 'hips2fitsClass',
+    'Conf', 'conf',
+]

astroquery/hips2fits/tests/test_hips2fits.py

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+# Licensed under a 3-clause BSD style license - see LICENSE.rst
+import sys
+import pytest
+
+from ..core import hips2fits
+
+from astropy import wcs as astropy_wcs
+from astropy.io import fits
+import numpy as np
+
+from astropy.utils.exceptions import AstropyUserWarning
+from matplotlib.colors import Colormap
+
+from astropy.coordinates import Angle, Longitude, Latitude
+import astropy.units as u
+
+class TestHips2fitsRemote(object):
+
+    # Create a new WCS astropy object
+    w = astropy_wcs.WCS(header={
+        'NAXIS1':                 2000,  # Width of the output fits/image
+        'NAXIS2':                 1000,  # Height of the output fits/image
+        'WCSAXES':                   2,  # Number of coordinate axes
+        'CRPIX1':                1000.0, # Pixel coordinate of reference point
+        'CRPIX2':                500.0,  # Pixel coordinate of reference point
+        'CDELT1':                -0.18,  # [deg] Coordinate increment at reference point
+        'CDELT2':                 0.18,  # [deg] Coordinate increment at reference point
+        'CUNIT1': 'deg',                 # Units of coordinate increment and value
+        'CUNIT2': 'deg',                 # Units of coordinate increment and value
+        'CTYPE1': 'GLON-MOL',            # galactic longitude, Mollweide's projection
+        'CTYPE2': 'GLAT-MOL',            # galactic latitude, Mollweide's projection
+        'CRVAL1':                  0.0,  # [deg] Coordinate value at reference point
+        'CRVAL2':                  0.0,  # [deg] Coordinate value at reference point
+    })
+    hips = 'CDS/P/DSS2/red'
+
+    def test_query_jpg(self):
+        result = hips2fits.query_with_wcs(
+            hips=self.hips,
+            wcs=self.w,
+            get_query_payload=True,
+            format='jpg',
+            min_cut=0.5,
+            max_cut=99.5,
+            cmap=Colormap('viridis'),
+        )
+
+        # We must get a numpy array with 3 dimensions, and the last one should be of size 3 (RGB)
+        assert result["format"] == 'jpg' and result["hips"] == "CDS/P/DSS2/red"
+
+    def test_query_no_wcs_fits(self):
+        result = hips2fits.query_without_wcs(
+            hips=self.hips,
+            get_query_payload=True,
+            width=1000,
+            height=500,
+            fov=Angle(20 * u.deg),
+            ra=Longitude(0 * u.deg),
+            dec=Latitude(20 * u.deg),
+            projection="TAN",
+            min_cut=0.5,
+            max_cut=99.5,
+            cmap=Colormap('viridis'),
+        )
+
+        # We must get a numpy array with 3 dimensions, and the last one should be of size 3 (RGB)
+        assert result["format"] == 'fits' and result["hips"] == "CDS/P/DSS2/red"

astroquery/hips2fits/tests/test_hips2fits_remote.py

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+# -*- coding: utf-8 -*
+
+# Licensed under a 3-clause BSD style license - see LICENSE.rst
+import sys
+import pytest
+
+from ..core import hips2fits
+
+from astropy import wcs as astropy_wcs
+from astropy.io import fits
+import numpy as np
+
+from astropy.utils.exceptions import AstropyUserWarning
+from matplotlib.colors import Colormap
+
+@pytest.mark.remote_data
+class TestHips2fitsRemote(object):
+
+    # Create a new WCS astropy object
+    w = astropy_wcs.WCS(header={
+        'NAXIS1':                 2000,  # Width of the output fits/image
+        'NAXIS2':                 1000,  # Height of the output fits/image
+        'WCSAXES':                   2,  # Number of coordinate axes
+        'CRPIX1':                1000.0,  # Pixel coordinate of reference point
+        'CRPIX2':                500.0,  # Pixel coordinate of reference point
+        'CDELT1':                -0.18,  # [deg] Coordinate increment at reference point
+        'CDELT2':                 0.18,  # [deg] Coordinate increment at reference point
+        'CUNIT1': 'deg',                 # Units of coordinate increment and value
+        'CUNIT2': 'deg',                 # Units of coordinate increment and value
+        'CTYPE1': 'GLON-MOL',            # galactic longitude, Mollweide's projection
+        'CTYPE2': 'GLAT-MOL',            # galactic latitude, Mollweide's projection
+        'CRVAL1':                  0.0,  # [deg] Coordinate value at reference point
+        'CRVAL2':                  0.0,  # [deg] Coordinate value at reference point
+    })
+    hips = 'CDS/P/DSS2/red'
+
+
+    def test_query_jpg(self):
+        result = hips2fits.query_with_wcs(
+            hips=self.hips,
+            wcs=self.w,
+            get_query_payload=False,
+            format='jpg',
+            min_cut=0.5,
+            max_cut=99.5,
+            cmap=Colormap('viridis'),
+        )
+
+
+        #import matplotlib.cm as cm
+        #import matplotlib.pyplot as plt
+
+        #im = plt.imshow(result)
+        #plt.show(im)
+
+        # We must get a numpy array with 3 dimensions, and the last one should be of size 3 (RGB)
+        assert isinstance(result, np.ndarray) and result.shape[2] == 3
+
+    def test_query_jpg_no_wcs(self):
+        from astropy.coordinates import Longitude
+        from astropy.coordinates import Latitude
+        from astropy.coordinates import Angle
+        import astropy.units as u
+
+        result = hips2fits.query_without_wcs(
+            hips=self.hips,
+            width=1000,
+            height=500,
+            fov=Angle(20 * u.deg),
+            ra=Longitude(0 * u.deg),
+            dec=Latitude(20 * u.deg),
+            projection="TAN",
+            get_query_payload=False,
+            format='jpg',
+            min_cut=0.5,
+            max_cut=99.5,
+            cmap=Colormap('viridis'),
+        )
+
+
+        import matplotlib.cm as cm
+        import matplotlib.pyplot as plt
+
+        im = plt.imshow(result)
+        plt.show(im)
+
+        # We must get a numpy array with 3 dimensions, and the last one should be of size 3 (RGB)
+        assert isinstance(result, np.ndarray) and result.shape[2] == 3
+
+
+    def test_bad_strech(self):
+        with pytest.raises(AttributeError):
+            result = hips2fits.query_with_wcs(
+                hips=self.hips,
+                wcs=self.w,
+                get_query_payload=False,
+                format='jpg',
+                stretch="azs",
+                min_cut=0.5,
+                max_cut=99.5,
+                cmap=Colormap('viridis'),
+            )
+
+    def test_query_fits(self):
+        result = hips2fits.query_with_wcs(
+            hips=self.hips,
+            wcs=self.w,
+            get_query_payload=False,
+        )
+
+        assert isinstance(result, fits.HDUList)
+
+    def test_query_fits(self):
+        result = hips2fits.query_with_wcs(
+            hips=self.hips,
+            wcs=self.w,
+            # Here we send additional keywords incompatible with
+            # the fits output format
+            min_cut=1.5,
+            max_cut=96,
+            stretch='asinh',
+            cmap='twilight',
+        )
+
+        import pdb
+        pdb.set_trace()
+
+    def test_query_png(self):
+        result = hips2fits.query_with_wcs(
+            hips=self.hips,
+            wcs=self.w,
+            get_query_payload=False,
+            format='png'
+        )
+        # We must get a numpy array with 3 dimensions, and the last one should be of size 4 (RGBA)
+        assert isinstance(result, np.ndarray) and result.shape[2] == 4
+
+    def test_bad_format_asked(self):
+        with pytest.raises(AttributeError):
+            result = hips2fits.query_with_wcs(
+                hips=self.hips,
+                wcs=self.w,
+                get_query_payload=False,
+                format='sdfsg'
+            )

docs/hips2fits/hips2fits.rst

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+.. doctest-skip-all
+
+.. _astroquery.hips2fits:
+
+******************************************
+HiPS2fits Service (`astroquery.hips2fits`)
+******************************************
+
+Getting started
+===============
+
+Query the `CDS hips2fits service <http://alasky.u-strasbg.fr/hips-image-services/hips2fits>`_
+
+The `CDS hips2fits service <http://alasky.u-strasbg.fr/hips-image-services/hips2fits>`_ offers a way
+to extract FITS images from HiPS sky maps. HiPS is an IVOA standard that combines individual images in
+order to produce a progressive hierarchical sky map describing the whole survey. Please refer to the 
+`IVOA paper <http://www.ivoa.net/documents/HiPS/20170519/REC-HIPS-1.0-20170519.pdf>`_ for more info.
+
+Given an astropy user-defined WCS with an HiPS name 
+(see the list of valid HiPS names hosted in CDS `here <http://aladin.unistra.fr/hips/list>`_),
+hips2fits will return you the corresponding FITS image (JPG/PNG output formats are also implemented).
+
+This package implements two methods:
+
+* :meth:`~astroquery.hips2fits.hips2fitsClass.query_with_wcs` extracting a FITS image from a HiPS and an astropy ``wcs.WCS``.
+    See `here <http://aladin.unistra.fr/hips/list>`_ all the valid HiPS names hosted in CDS.
+* :meth:`~astroquery.hips2fits.hips2fitsClass.query_without_wcs` extracting a FITS image from a HiPS given the output image pixel size, the center of projection, the type of projection and the field of view.
+    See `here <http://aladin.unistra.fr/hips/list>`_ all the valid HiPS names hosted in CDS.
+
+
+Examples
+========
+
+With an user defined astropy WCS
+~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
+
+.. code-block:: python
+
+    >>> from astroquery.hips2fits import hips2fits
+    >>> import matplotlib.pyplot as plt
+    >>> from matplotlib.colors import Colormap
+    >>> from astropy import wcs as astropy_wcs
+    >>> # Create a new WCS astropy object
+    >>> w = astropy_wcs.WCS(header={
+    ...     'NAXIS1':                 2000,  # Width of the output fits/image
+    ...     'NAXIS2':                 1000,  # Height of the output fits/image
+    ...     'WCSAXES':                   2,  # Number of coordinate axes
+    ...     'CRPIX1':                1000.0, # Pixel coordinate of reference point
+    ...     'CRPIX2':                500.0,  # Pixel coordinate of reference point
+    ...     'CDELT1':                -0.18,  # [deg] Coordinate increment at reference point
+    ...     'CDELT2':                 0.18,  # [deg] Coordinate increment at reference point
+    ...     'CUNIT1': 'deg',                 # Units of coordinate increment and value
+    ...     'CUNIT2': 'deg',                 # Units of coordinate increment and value
+    ...     'CTYPE1': 'GLON-MOL',            # galactic longitude, Mollweide's projection
+    ...     'CTYPE2': 'GLAT-MOL',            # galactic latitude, Mollweide's projection
+    ...     'CRVAL1':                  0.0,  # [deg] Coordinate value at reference point
+    ...     'CRVAL2':                  0.0,  # [deg] Coordinate value at reference point
+    ... })
+    >>> hips = 'CDS/P/DSS2/red'
+    >>> result = hips2fits.query_with_wcs(
+    ...    hips=hips,
+    ...    wcs=w,
+    ...    get_query_payload=False,
+    ...    format='jpg',
+    ...    min_cut=0.5,
+    ...    max_cut=99.5,
+    ...    cmap=Colormap('viridis'),
+    ... )
+    >>> im = plt.imshow(result)
+    >>> plt.show(im)
+
+.. image:: ./query_wcs.png
+
+Without WCS
+~~~~~~~~~~~
+
+    >>> from astroquery.hips2fits import hips2fits
+    >>> import matplotlib.pyplot as plt
+    >>> from matplotlib.colors import Colormap
+    >>> import astropy.units as u
+    >>> from astropy.coordinates import Longitude, Latitude, Angle
+    >>> hips = 'CDS/P/DSS2/red'
+    >>> result = hips2fits.query_without_wcs(
+    ...    hips=hips,
+    ...    width=1000,
+    ...    height=500,
+    ...    ra=Longitude(0 * u.deg),
+    ...    dec=Latitude(20 * u.deg),
+    ...    fov=Angle(80 * u.deg),
+    ...    projection="AIT",
+    ...    get_query_payload=False,
+    ...    format='jpg',
+    ...    min_cut=0.5,
+    ...    max_cut=99.5,
+    ...    cmap=Colormap('viridis'),
+    ... )
+    >>> im = plt.imshow(result)
+    >>> plt.show(im)
+
+.. image:: ./query_no_wcs.png
+
+Reference/API
+=============
+
+.. automodapi:: astroquery.hips2fits
+    :no-inheritance-diagram:
+
+
+.. _hips2fits: http://alasky.u-strasbg.fr/hips-image-services/hips2fits
+

docs/index.rst

@@ -172,6 +172,7 @@ The following modules have been completed using a common API:
   gama/gama.rst
   gemini/gemini.rst
   heasarc/heasarc.rst
+  hips2fits/hips2fits.rst
   hitran/hitran.rst
   ibe/ibe.rst
   irsa/irsa.rst