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python2-astropy-2.0.3-lp152.3.6 RPM for x86_64

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Name: python2-astropy Distribution: openSUSE Leap 15.2
Version: 2.0.3 Vendor: openSUSE
Release: lp152.3.6 Build date: Wed Oct 9 08:48:51 2019
Group: Development/Languages/Python Build host: lamb07
Size: 30924502 Source RPM: python-astropy-2.0.3-lp152.3.6.src.rpm
Packager: https://bugs.opensuse.org
Url: http://astropy.org
Summary: Community-developed python astronomy tools
Astropy is a package intended to contain core functionality and some
common tools needed for performing astronomy and astrophysics research with
Python. It also provides an index for other astronomy packages and tools for
managing them.

Provides

Requires

License

BSD-3-Clause

Changelog

* Fri Jan 05 2018 alarrosa@suse.com
  - Update to astropy 2.0.3
    * Bugfixes:
    * astropy.coordinates
    - Ecliptic frame classes now support attributes v_x, v_y, v_z when using
      with a Cartesian representation.
    - Added a nicer error message when accidentally calling
      frame.representation instead of frame.data in the context of methods
      that use ._apply().
    - Creating a new SkyCoord from a list of multiple SkyCoord objects now
      yield the correct type of frame, and works at all for non-equatorial
      frames.
    - Improved accuracy of velocity calculation in
      EarthLocation.get_gcrs_posvel.
    - Improved accuracy of radial velocity corrections in
      SkyCoord.radial_velocity_correction`.
    - The precision of ecliptic frames is now much better, after removing the
      nutation from the rotation and fixing the computation of the position
      of the Sun.
    * astropy.extern
    - Version 0.2.1 of pytest-astropy is included as an external package.
    * astropy.io.fits
    - Fix writing the result of fitsdiff to file with --output-file.
    - Fix a minor bug where FITS_rec instances can not be indexed with tuples
      and other sequences that end up with a scalar.
    * astropy.io.misc
    - Fix ImportError when hdf5 is imported first in a fresh Python
      interpreter in Python 3.
    * astropy.nddata
    - Suppress errors during WCS creation in CCDData.read().
    - Fixed a problem with CCDData.read when the extension wasn't given and
      the primary HDU contained no data but another HDU did. In that case the
      header were not correctly combined.
    * astropy.stats
    - Fixed an issue where the biweight statistics functions would sometimes
      cause runtime underflow/overflow errors for float32 input arrays.
    * astropy.table
    - Fixed a problem when printing a table when a column is deleted and
      garbage-collected, and the format function caching mechanism happens to
      re-use the same cache key.
    - Fixed a problem when comparing a unicode masked column (on left side)
      to a bytes masked column (on right side).
    - Fixed a problem in comparing masked columns in bytes and unicode when
      the unicode had masked entries.
    * astropy.tests
    - Fixed a bug that causes tests for rst files to not be run on certain
      platforms.
    - Fixed a bug that caused the doctestplus plugin to not work nicely with
      the hypothesis package.
    - Fixed a bug that meant that the data.astropy.org mirror could not be
      used when using --remote-data=astropy.
    - Support compatibility with new pytest-astropy plugins.
    - When testing, astropy (or the package being tested) is now installed to
      a temporary directory instead of copying the build. This allows entry
      points to work correctly.
    * astropy.time
    - Initialization of Time instances now is consistent for all formats to
      ensure that -0.5 <= jd2 < 0.5.
    * astropy.units
    - Ensure that Quantity slices can be set with objects that have a unit
      attribute (such as Column).
    * astropy.utils
    - download_files_in_parallel now respects the given timeout value.
    - Fixed bugs in remote data handling and also in IERS unit test related
      to path URL, and URI normalization on Windows.
    - Fixed a bug that caused get_pkg_data_fileobj to not work correctly when
      used with non-local data from inside packages.
    - Make sure get_pkg_data_fileobj fails if the URL can not be read, and
      correctly falls back on the mirror if necessary.
    - Fix the finddiff option in find_current_module to properly deal with
      submodules.
    - Fixed pyreadline import in utils.console.isatty for older IPython
      versions on Windows.
    * astropy.visualization
    - Fixed the vertical orientation of the fits2bitmap output bitmap image
      to match that of the FITS image.
    - Added a workaround for a bug in matplotlib so that the fits2bitmap
      script generates the correct output file type.
    * Other Changes and Additions
    * No longer require LaTeX to build the documentation locally and use
      mathjax instead.
    * Fixed broken links in the documentation.
    * Ensured that all tests use the Astropy data mirror if needed.
* Thu Dec 14 2017 alarrosa@suse.com
  - Remove test bcond since it wasn't really used at all
* Mon Dec 11 2017 alarrosa@suse.com
  - Update to astropy 2.0.2 . Astropy 2.0 is a major release that adds
    significant new functionality since the 1.3.x series of releases:
    * New unit support for most models
    * New image class CCDData added
    * Experimental velocity support in astropy.coordinates
    * New functionality in astropy.stats
    * Easier use of efficient bytestring Table columns in Python 3
    * New way to instantiate a BinTableHDU directly from a Table
    * New printdiff convenience function for FITS
    * New molar_mass_amu unit equivalency
    * Store astropy core object types in ASCII ECSV table file
    * Improvements to astropy.convolution
    * No relativistic species by default in cosmological models
    * Renamed/removed functionality
    The full changelog can be read at
    http://docs.astropy.org/en/stable/changelog.html .
* Fri Jun 23 2017 alarrosa@suse.com
  - The latest astropy version requires liberfa 1.3.0 even if
    it builds fine with 1.2.0 since it requires the eraEceq06 symbol.
* Thu May 25 2017 toddrme2178@gmail.com
  - Implement single-spec version
  - Fix source URL
  - Update to version 1.3.2
    * Lots of changes (see CHANGES.rst for details).
* Fri Nov 18 2016 asterios.dramis@gmail.com
  - Replace cfitsio-devel, liberfa-devel, libexpat-devel and
    libwcs-devel build requirements with pkgconfig() ones.
* Sat Jul 16 2016 asterios.dramis@gmail.com
  - Update to version 1.2.1:
    * Lots of changes (see CHANGES.rst for details).
  - Added new build requirements python-Jinja2, python-PyYAML,
    python-bleach, python-jupyter_ipython, python-mpmath,
    python-psutil and python-scikit-image.
  - Updated python-numpy-devel build requirement and python-numpy
    runtime requirement to version >= 1.7.0.
  - Updated python-six build and runtime requirement to version
    >= 1.7.3.
  - Removed not needed build requirements python-astropy-helpers and
    python-numpy (indirect dependency).
  - Removed not needed runtime requirements python-astropy-helpers.
  - Added new Recommend entries python-PyYAML and
    python-scikit-image.
* Tue Feb 02 2016 toddrme2178@gmail.com
  - Add python-astropy-helpers and python-pandas dependencies.
* Thu Jan 28 2016 toddrme2178@gmail.com
  - update to version 1.1.1
    + New Features
    - ``astropy.io.registry``
    * Allow ``pathlib.Path`` objects (available in Python 3.4 and later) for
      specifying the file name in registry read / write functions. [#4405]
    - ``astropy.utils``
    * ``console.human_file_size`` now accepts quantities with byte-equivalent
      units [#4373]
    + Bug Fixes
    - ``astropy.analytic_functions``
    * Fixed the blackbody functions' handling of overflows on some platforms
      (Windows with MSVC, older Linux versions) with a buggy ``expm1`` function.
      [#4393]
    - ``astropy.io.fits``
    * Fixed an bug where updates to string columns in FITS tables were not saved
      on Python 3. [#4452]
    + Other Changes and Additions
    - Updated bundled astropy-helpers to v1.1.1. [#4413]
  - update to version 1.1
    + New Features
    - ``astropy.config``
    - Added new tools ``set_temp_config`` and ``set_temp_cache`` which can be
      used either as function decorators or context managers to temporarily
      use alternative directories in which to read/write the Astropy config
      files and download caches respectively.  This is especially useful for
      testing, though ``set_temp_cache`` may also be used as a way to provide
      an alternative (application specific) download cache for large data files,
      rather than relying on the default cache location in users' home
      directories. [#3975]
    - ``astropy.constants``
    - Added the Thomson scattering cross-section. [#3839]
    - ``astropy.convolution``
    - Added Moffat2DKernel. [#3965]
    - ``astropy.coordinates``
    - Added ``get_constellation`` function and ``SkyCoord.get_constellation``
      convenience method to determine the constellation that a coordinate
      is in. [#3758]
    - Added ``PrecessedGeocentric`` frame, which is based on GCRS, but precessed
      to a specific requested mean equinox. [#3758]
    - Added ``Supergalactic`` frame to support de Vaucouleurs supergalactic
      coordinates. [#3892]
    - ``SphericalRepresentation`` now has a ``._unit_representation`` class attribute to specify
      an equivalent UnitSphericalRepresentation. This allows subclasses of
      representations to pair up correctly. [#3757]
    - Added functionality to support getting the locations of observatories by
      name. See ``astropy.coordinates.EarthLocation.of_site``. [#4042]
    - Added ecliptic coordinates, including ``GeocentricTrueEcliptic``,
      ``BarycentricTrueEcliptic``, and ``HeliocentricTrueEcliptic``. [#3749]
    - ``astropy.cosmology``
    - Add Planck 2015 cosmology [#3476]
    - Distance calculations now > 20-40x faster for the supplied
      cosmologies due to implementing Cython scalar versions of
      ``FLRW.inv_efunc``.[#4127]
    - ``astropy.io.ascii``
    - Automatically use ``guess=False`` when reading if the file ``format`` is
      provided and the format parameters are uniquely specified.  This update
      also removes duplicate format guesses to improve performance. [#3418]
    - Calls to ascii.read() for fixed-width tables may now omit one of the keyword
      arguments ``col_starts`` or ``col_ends``. Columns will be assumed to begin and
      end immediately adjacent to each other. [#3657]
    - Add a function ``get_read_trace()`` that returns a traceback of the
      attempted read formats for the last call to ``astropy.io.ascii.read``. [#3688]
    - Supports LZMA decompression via ``get_readable_fileobj`` [#3667]
    - Allow ``-`` character is Sextractor format column names. [#4168]
    - Improve DAOphot reader to read multi-aperture files [#3535, #4207]
    - ``astropy.io.fits``
    - Support reading and writing from bzip2 compressed files. i.e. ``.fits.bz2``
      files. [#3789]
    - Included a new command-line script called ``fitsinfo`` to display
      a summary of the HDUs in one or more FITS files. [#3677]
    - ``astropy.io.misc``
    - Support saving all meta information, description and units of tables and columns
      in HDF5 files [#4103]
    - ``astropy.io.votable``
    - A new method was added to ``astropy.io.votable.VOTable``,
      ``get_info_by_id`` to conveniently find an ``INFO`` element by its
      ``ID`` attribute. [#3633]
    - Instances in the votable tree now have better ``__repr__``
      methods. [#3639]
    - ``astropy.logger.py``
    - Added log levels (e.g., DEBUG, INFO, CRITICAL) to ``astropy.log`` [#3947]
    - ``astropy.modeling``
    - Added a new ``Parameter.validator`` interface for setting a validation
      method on individual model parameters.  See the ``Parameter``
      documentation for more details. [#3910]
    - The projection classes that are named based on the 3-letter FITS
      WCS projections (e.g. ``Pix2Sky_TAN``) now have aliases using
      longer, more descriptive names (e.g. ``Pix2Sky_Gnomonic``).
      [#3583]
    - All of the standard FITS WCS projection types have been
      implemented in ``astropy.modeling.projections`` (by wrapping
      WCSLIB). [#3906]
    - Added ``Sersic1D`` and ``Sersic2D`` model classes. [#3889]
    - Added the Voigt profile to existing models. [#3901]
    - Added ``bounding_box`` property and ``render_model`` function [#3909]
    - ``astropy.nddata``
    - Added ``block_reduce`` and ``block_replicate`` functions. [#3453]
    - ``extract_array`` now offers different options to deal with array
      boundaries [#3727]
    - Added a new ``Cutout2D`` class to create postage stamp image cutouts
      with optional WCS propagation. [#3823]
    - ``astropy.stats``
    - Added ``sigma_lower`` and ``sigma_upper`` keywords to
      ``sigma_clip`` to allow for unsymmetric clipping. [#3595]
    - Added ``cenfunc``, ``stdfunc``, and ``axis`` keywords to
      ``sigma_clipped_stats``. [#3792]
    - ``sigma_clip`` automatically masks invalid input values (NaNs, Infs) before
      performing the clipping [#4051]
    - Added the ``histogram`` routine, which is similar to ``np.histogram`` but
      includes several additional options for automatic determination of optimal
      histogram bins. Associated helper routines include ``bayesian_blocks``,
      ``friedman_bin_width``, ``scott_bin_width``, and ``knuth_bin_width``.
      This functionality was ported from the astroML_ library. [#3756]
    - Added the ``bayesian_blocks`` routine, which implements a dynamic algorithm
      for locating change-points in various time series. [#3756]
    - A new function ``poisson_conf_interval()`` was added to allow easy calculation
      of several standard formulae for the error bars on the mean of a Poisson variable
      estimated from a single sample.
    - ``astropy.table``
    - ``add_column()`` and ``add_columns()`` now have ``rename_duplicate``
      option to rename new column(s) rather than raise exception when its name
      already exists. [#3592]
    - Added ``Table.to_pandas`` and ``Table.from_pandas`` for converting to/from
      pandas dataframes. [#3504]
    - Initializing a ``Table`` with ``Column`` objects no longer requires
      that the column ``name`` attribute be defined. [#3781]
    - Added an ``info`` property to ``Table`` objects which provides configurable
      summary information about the table and its columns. [#3731]
    - Added an ``info`` property to column classes (``Column`` or mixins).  This
      serves a dual function of providing configurable summary information about
      the column, and acting as a manager of column attributes such as
      name, format, or description. [#3731]
    - Updated table and column representation to use the ``dtype_info_name``
      function for the dtype value.  Removed the default "masked=False"
      from the table representation. [#3868, #3869]
    - Updated row representation to be consistent with the corresponding
      table representation for that row.  Added HTML representation so a
      row displays nicely in IPython notebook.
    - Added a new table indexing engine allowing for the creation of
      indices on one or more columns of a table using ``add_index``. These
      indices enable new functionality such as searching for rows by value
      using ``loc`` and ``iloc``, as well as increased performance for
      certain operations. [#3915]
    - Added capability to include a structured array or recarray in a table
      as a mixin column.  This allows for an approximation of nested tables.
      [#3925]
    - Added ``keep_byteorder`` option to ``Table.as_array()``.  See the
      "API Changes" section below. [#4080]
    - Added a new method ``Table.replace_column()`` to replace an existing
      column with a new data column. [#4090]
    - Added a ``tableclass`` option to ``Table.pformat()`` to allow specifying
      a list of CSS classes added to the HTML table. [#4131]
    - New CSS for jsviewer table [#2917, #2982, #4174]
    - Added a new ``Table.show_in_notebook`` method that shows an interactive view
      of a Table (similar to ``Table.show_in_browser(jsviewer=True)``) in an
      Python/Jupyter notebook. [#4197]
    - ``astropy.tests``
    - Added new test config options, ``config_dir`` and ``cache_dir``  (these
      can be edited in ``setup.cfg`` or as extra command-line options to
      py.test) for setting the locations to use for the Astropy config files
      and download caches (see also the related ``set_temp_config/cache``
      features added in ``astropy.config``). [#3975]
    - ``astropy.time``
    - Add support for FITS standard time strings. [#3547]
    - Allow the ``format`` attribute to be updated in place to change the
      default representation of a ``Time`` object. [#3673]
    - Add support for shape manipulation (reshape, ravel, etc.). [#3224]
    - Add argmin, argmax, argsort, min, max, ptp, sort methods. [#3581]
    - Add ``Time.to_datetime`` method for converting ``Time`` objects to
      timezone-aware datetimes. [#4119]
    - ``astropy.units``
    - Added furlong to imperial units. [#3529]
    - Added mil to imperial units. [#3716]
    - Added stone to imperial units. [#4192]
    - Added Earth Mass (``M_earth``) and Jupiter mass (``M_jup``) to units [#3907]
    - Added support for functional units, in particular the logarithmic ones
      ``Magnitude``, ``Decibel``, and ``Dex``. [#1894]
    - Quantities now work with the unit support in matplotlib.  See
      :ref:`plotting-quantities`. [#3981]
    - ``astropy.utils``
    - Added new ``OrderedDescriptor`` and ``OrderedDescriptorContainer`` utility
      classes that make it easier to implement classes with declarative APIs,
      wherein class-level attributes have an inherit "ordering" to them that is
      specified by the order in which those attributes are defined in the class
      declaration (by defining them using special descriptors that have
      ``OrderedDescriptor`` as a base class).  See the API documentation for
      these classes for more details. Coordinate frames and models now use this
      interface. [#3679]
    - The ``get_pkg_data_*`` functions now take an optional ``package`` argument
      which allows specifying any package to read package data filenames or
      content out of, as opposed to only being able to use data from the package
      that the function is called from. [#4079]
    - Added function ``dtype_info_name`` to the ``data_info`` module to provide
      the name of a ``dtype`` for human-readable informational purposes. [#3868]
    - Added ``classproperty`` decorator--this is to ``property`` as
      ``classmethod`` is to normal instance methods. [#3982]
    - ``iers.open`` now handles network URLs, as well as local paths. [#3850]
    - The ``astropy.utils.wraps`` decorator now takes an optional
      ``exclude_args`` argument not shared by the standard library ``wraps``
      decorator (as it is unique to the Astropy version's ability of copying
      the wrapped function's argument signature).  ``exclude_args`` allows
      certain arguments on the wrapped function to be excluded from the signature
      of the wrapper function.  This is particularly useful when wrapping an
      instance method as a function (to exclude the ``self`` argument). [#4017]
    - ``get_readable_fileobj`` can automatically decompress LZMA ('.xz')
      files using the ``lzma`` module of Python 3.3+ or, when available, the
      ``backports.lzma`` package on earlier versions. [#3667]
    - The ``resolve_name`` utility now accepts any number of additional
      positional arguments that are automatically dotted together with the
      first ``name`` argument. [#4083]
    - Added ``is_url_in_cache`` for resolving paths to cached files via URLS
      and checking if files exist. [#4095]
    - Added a ``step`` argument to the ``ProgressBar.map`` method to give
      users control over the update frequency of the progress bar. [#4191]
    - ``astropy.visualization``
    - Added a function / context manager ``quantity_support`` for enabling
      seamless ploting of ``Quantity`` instances in matplotlib. [#3981]
    - Added the ``hist`` function, which is similar to ``plt.hist`` but
      includes several additional options for automatic determination of optimal
      histogram bins. This functionality was ported from the astroML_ library.
      [#3756]
    - ``astropy.wcs``
    - The included version of wcslib has been upgraded to 5.10. [#4239]
      The minimum required version of wcslib in the 4.x series remains 4.24.
      The minimum required version of wcslib in the 5.x series is
      5.8.  Building astropy against a wcslib 5.x prior to 5.8
      will raise an ``ImportError`` when ``astropy.wcs`` is imported.
      The wcslib changes relevant to astropy are:
    - The FITS headers returned by ``astropy.wcs.WCS.to_header`` and
      ``astropy.wcs.WCS.to_header_string`` now include values with
      more precision.  This will result in numerical differences in
      your results if you convert ``astropy.wcs.WCS`` objects to FITS
      headers and use the results.
    - ``astropy.wcs.WCS`` now recognises the ``TPV``, ``TPD``,
      ``TPU``, ``DSS``, ``TNX`` and ``ZPX`` polynomial distortions.
    - Added relaxation flags to allow ``PC0i_0ja``, ``PV0j_0ma``, and
      ``PS0j_0ma`` (i.e. with leading zeroes on the index).
    - Tidied up error reporting, particularly relating to translating
      status returns from lower-level functions.
    - Changed output formatting of floating point values in
      ``to_header``.
    - Enhanced text representation of ``WCS`` objects. [#3604]
    - The ``astropy.tests.helper`` module is now part of the public API (and has a
      documentation page).  This module was in previous releases of astropy,
      but was not considered part of the public API until now. [#3890]
    - There is a new function ``astropy.online_help`` to search the
      astropy documentation and display the result in a web
      browser. [#3642]
    + API changes
    - ``astropy.cosmology``
    - ``FLRW._tfunc`` and ``FLRW._xfunc`` are marked as deprecated.  Users
      should use the new public interfaces ``FLRW.lookback_time_integrand``
      and ``FLRW.abs_distance_integrand`` instead. [#3767]
    - ``astropy.io.ascii``
    - The default header line processing was made to be consistent with data line
      processing in that it now ignores blank lines that may have whitespace
      characters.  Any code that explicitly specifies a ``header_start`` value
      for parsing a file with blank lines in the header containing whitespace will
      need to be updated. [#2654]
    - ``astropy.io.fits``
    - The ``uint`` argument to ``fits.open`` is now True by default; that is,
      arrays using the FITS unsigned integer convention will be detected, and
      read as unsigned integers by default.  A new config option for
      ``io.fits``, ``enable_uint``, can be changed to False to revert to the
      original behavior of ignoring the ``uint`` convention unless it is
      explicitly requested with ``uint=True``. [#3916]
    - The ``ImageHDU.NumCode`` and ``ImageHDU.ImgCode`` attributes (and same
      for other classes derived from ``_ImageBaseHDU``) are deprecated.  Instead,
      the ``astropy.io.fits`` module-level constants ``BITPIX2DTYPE`` and
      ``DTYPE2BITPIX`` can be used. [#3916]
    - ``astropy.modeling``
    - Note: Comparisons of model parameters with array-like values now
      yields a Numpy boolean array as one would get with normal Numpy
      array comparison.  Previously this returned a scalar True or False,
      with True only if the comparison was true for all elements compared,
      which could lead to confusing circumstances. [#3912]
    - Using ``model.inverse = None`` to reset a model's inverse to its
      default is deprecated.  In the future this syntax will explicitly make
      a model not have an inverse (even if it has a default).  Instead, use
      ``del model.inverse`` to reset a model's inverse to its default (if it
      has a default, otherwise this just deletes any custom inverse that has
      been assigned to the model and is still equivalent to setting
      ``model.inverse = None``). [#4236]
    - Adds a ``model.has_user_inverse`` attribute which indicates whether or not
      a user has assigned a custom inverse to ``model.inverse``.  This is just
      for informational purposes, for example, for software that introspects
      model objects. [#4236]
    - Renamed the parameters of ``RotateNative2Celestial`` and
      ``RotateCelestial2Native`` from ``phi``, ``theta``, ``psi`` to
      ``lon``, ``lat`` and ``lon_pole``. [#3578]
    - Deprecated the ``Pix2Sky_AZP.check_mu`` and ``Sky2Pix_AZP.check_mu``
      methods (these were obscure "accidentally public" methods that were
      probably not used by anyone). [#3910]
    - Added a phase parameter to the Sine1D model. [#3807]
    - ``astropy.stats``
    - Renamed the ``sigma_clip`` ``sig`` keyword as ``sigma``. [#3595]
    - Changed the ``sigma_clip`` ``varfunc`` keyword to ``stdfunc``. [#3595]
    - Renamed the ``sigma_clipped_stats`` ``mask_val`` keyword to
      ``mask_value``. [#3595]
    - Changed the default ``iters`` keyword value to 5 in both the
      ``sigma_clip`` and ``sigma_clipped_stats`` functions. [#4067]
    - ``astropy.table``
    - ``Table.as_array()`` always returns a structured array with each column in
      the system's native byte order.  The optional ``keep_byteorder=True``
      option will keep each column's data in its original byteorder. [#4080]
    - ``Table.simple_table()`` now creates tables with int64 and float64 types
      instead of int32 and float64. [#4114]
    - ``astropy.time``
    - The ``astropy_time`` attribute and time format has been removed from the
      public interface.  Existing code that instantiates a new time object using
      ``format='astropy_time'`` can simply omit the ``format``
      specification. [#3857]
    - ``astropy.units``
    - Single-item ``Quantity`` instances with record ``dtype`` will now have
      their ``isscalar`` property return ``True``, consistent with behaviour for
      numpy arrays, where ``np.void`` records are considered scalar. [#3899]
    - Three changes relating to the FITS unit format [#3993]:
    - The FITS unit format will no longer parse an arbitrary number as a
      scale value.  It must be a power of 10 of the form ``10^^k``,
      ``10^k``, ``10+k``, ``10-k`` and ``10(k)``. [#3993]
    - Scales that are powers of 10 can be written out.  Previously, any
      non-1.0 scale was rejected.
    - The ``*`` character is accepted as a separator between the scale
      and the units.
    - Unit formatter classes now require the ``parse`` and ``to_string``
      methods are now required to be classmethods (and the formatter
      classes themselves are assumed to be singletons that are not
      instantiated).  As unit formatters are mostly an internal implementation
      detail this is not likely to affect any users. [#4001]
    - CGS E&M units are now defined separately from SI E&M units, and have
      distinct physical types. [#4255]
    - ``astropy.utils``
    - All of the ``get_pkg_data_*`` functions take an optional ``package``
      argument as their second positional argument.  So any code that previously
      passed other arguments to these functions as positional arguments might
      break.  Use keyword argument passing instead to mitigate this. [#4079]
    - ``astropy.utils.iers`` now uses a ``QTable`` internally, which means that
      the numerical columns are stored as ``Quantity``, with full support for
      units.  Furthermore, the ``ut1_utc`` method now returns a ``Quantity``
      instead of a float or an array (as did ``pm_xy`` already). [#3223]
    - ``astropy.utils.iers`` now throws an ``IERSRangeError``, a subclass
      of ``IndexError``, rather than a raw ``IndexError``.  This allows more
      fine-grained catching of situations where a ``Time`` is beyond the range
      of the loaded IERS tables. [#4302]
    - ``astropy.wcs``
    - When compiled with wcslib 5.9 or later, the FITS headers returned
      by ``astropy.wcs.WCS.to_header`` and
      ``astropy.wcs.WCS.to_header_string`` now include values with more
      precision.  This will result in numerical differences in your
      results if you convert ``astropy.wcs.WCS`` objects to FITS headers
      and use the results.
    - If NAXIS1 or NAXIS2 is not passed with the header object to
      WCS.calc_footprint, a ValueError is raised. [#3557]
    + Bug fixes
    - ``astropy.constants``
    - The constants ``Ry`` and ``u`` are now properly used inside the
      corresponding units.  The latter have changed slightly as a result. [#4229]
    - ``astropy.coordinates``
    - Internally, ``coordinates`` now consistently uses the appropriate time
      scales for using ERFA functions. [#4302]
    - ``astropy.io.ascii``
    - Fix a segfault in the fast C parser when one of the column headers
      is empty [#3545].
    - Fix several bugs that prevented the fast readers from being used
      when guessing the file format.  Also improved the read trace
      information to better understand format guessing. [#4115]
    - Fix an underlying problem that resulted in an uncaught TypeError
      exception when reading a CDS-format file with guessing enabled. [#4120]
    - ``astropy.modeling``
    - ``Simplex`` fitter now correctly passes additional keywords arguments to
      the scipy solver. [#3966]
    - The keyword ``acc`` (for accuracy) is now correctly accepted by
      ``Simplex``. [#3966]
    - ``astropy.units``
    - The units ``Ryd`` and ``u`` are no longer hard-coded numbers, but depend
      on the appropriate values in the ``constants`` module.  As a result, these
      units now imply slightly different conversions.  [#4229]
    + Other Changes and Additions
    - The ``./setup.py test`` command is now implemented in the ``astropy.tests``
      module again (previously its implementation had been moved into
      astropy-helpers).  However, that made it difficult to synchronize changes
      to the Astropy test runner with changes to the ``./setup.py test`` UI.
      astropy-helpers v1.1 and above will detect this implementation of the
      ``test`` command, when present, and use it instead of the old version that
      was included in astropy-helpers (most users will not notice any difference
      as a result of this change). [#4020]
    - The repr for ``Table`` no longer displays ``masked=False`` since tables
      are not masked by default anyway. [#3869]
    - The version of ``PLY`` that ships with astropy has been updated to 3.6.
    - WCSAxes is now required for doc builds. [#4074]
    - Updated ``astropy.tests`` test runner code to work with Coverage v4.0 when
      generating test coverage reports. [#4176]
    - The migration guide from pre-v0.4 coordinates has been removed to avoid
      cluttering the ``astropy.coordinates`` documentation with increasingly
      irrelevant material.  To see the migration guide, we recommend you simply look
      to the archived documentation for previous versions, e.g.
      http://docs.astropy.org/en/v1.0/coordinates/index.html#migrating-from-pre-v0-4-coordinates
      [#4203]
    - In ``astropy.coordinates``, the transformations between GCRS, CIRS,
      and ITRS have been adjusted to more logically reflect the order in
      which they actually apply.  This should not affect most coordinate
      transformations, but may affect code that is especially sensitive to
      machine precision effects that change when the order in which
      transformations occur is changed. [#4255]
  - update to version 1.0.8 (2016-01-08)
    + Bug Fixes
    - ``astropy.io.fits``
    - Fixed an bug where updates to string columns in FITS tables were not saved
      on Python 3. [#4452]
    - ``astropy.units``
    - In-place peak-to-peak calculations now work on ``Quantity``. [#4442]
    - ``astropy.utils``
    - Fixed ``find_api_page`` to work correctly on python 3.x [#4378]
  - update to version 1.0.7:
    * New Features
      + astropy.time
      Fix incorrect value attribute for epoch formats like "unix" when
      scale is different from the class epoch_scale. [#4313]
    * Bug Fixes
      + astropy.coordinates
      Pickling of EarthLocation instances now also works on Python
      2. [#4304]
      + astropy.io.fits
      o Fixed a regression that could cause writes of large FITS files
      to be truncated. [#4307]
      o Astropy v1.0.6 included a fix (#4228) for an obscure case where
      the TDIM of a table column is smaller than the repeat count of
      its data format. This updates that fix in such a way that it
      works with Numpy 1.10 as well. [#4266]
      o Fix fast writer so bytestring column output is not prefixed by
      'b' in Python 3. [#4350]
      + astropy.table
      o Fix a bug when pickling a Table with mixin columns
      (e.g. Time). [#4098]
      + astropy.utils
      o Fixed an issue where if ipython is installed but ipykernel is
      not installed then importing astropy from the ipython console
      gave an IPython.kernel deprecation warning. [#4279]
      o Fixed crash that could occur in ProgressBar when astropy is
      imported in an IPython startup script. [#4274]
  - update to version 1.0.6:
    * astropy.analytic_functions
      + Fixed blackbody analytic functions to properly support arrays of
      temperatures. [#4251]
    * astropy.coordinates
      + Fixed errors in transformations for objects within a few AU of
      the Earth. Included substansive changes to transformation
      machinery that may change distances at levels ~machine precision
      for other objects. [#4254]
    * astropy.io.fits
      + fitsdiff and related functions now do a better job reporting
      differences between values that are different types but have the
      same representation (ex: the string '0' versus the number
      0). [#4122]
      + Miscellaneous fixes for supporting Numpy 1.10. [#4228]
      + Fixed an issue where writing a column of unicode strings to a
      FITS table resulted in a quadrupling of size of the column
      (i.e. the format of the FITS column was 4 characters for every
      one in the original strings). [#4228]
      + Added support for an obscure case (but nonetheless allowed by the
      FITS standard) where a column has some TDIMn keyword, but a
      repeat count in the TFORMn column greater than the number of
      elements implied by the TDIMn. For example TFORMn = 100I, but
      TDIMn = '(5,5)'. In this case the TDIMn implies 5x5 arrays in the
      column, but the TFORMn implies a 100 element 1-D array in the
      column. In this case the TDIM takes precedence, and the remaining
      bytes in the column are ignored. [#4228]
    * astropy.io.votable
      + Fixed crash with Python compiler optimization level = 2. [#4231]
    * astropy.vo
      + Fixed check_conesearch_sites with parallel=True on Python >= 3.3
      and on Windows (it was broken in both those cases for separate
      reasons). [#2970]
    * All tests now pass against Numpy v1.10.x. This implies nominal
      support for Numpy 1.10.x moving forward (but there may still be
      unknown issues). For example, there is already a known performance
      issue with tables containing large multi-dimensional columns--for
      example, tables that contain entire images in one or more of their
      columns. This is a known upstream issue in Numpy. [#4259]
  - Update to 1.0.5
    + Bug Fixes
    * ``astropy.constants``
      > Rename units -> unit and error -> uncertainty in the ``repr`` and ``str``
      of constants to match attribute names. [#4147]
    * ``astropy.coordinates``
      > Fix string representation of ``SkyCoord`` objects transformed into
      the ``AltAz`` frame [#4055]
      > Fix the ``search_around_sky`` function to allow ``storekdtree`` to be
      ``False`` as was intended. [#4082]
    * ``astropy.io.fits``
      > Fix bug when extending one header (without comments) with another
      (with comments). [#3967]
      > Somewhat improved resource usage for FITS data--previously a new ``mmap``
      was opened for each HDU of a FITS file accessed through an ``HDUList``.
      Each ``mmap`` used up a single file descriptor, causing problems with
      system resource limits for some users.  Now only a single ``mmap`` is
      opened, and shared for the data of all HDUs.  Note: The problem still
      persists with using the "convenience" functions.  For example using
      ``fits.getdata`` will create one ``mmap`` per HDU read this way (as
      opposed to opening the file with ``fits.open`` and accessing the HDUs
      through the ``HDUList`` object). [#4097]
      > Fix bug where reading a file without a newline failed with an
      unrelated / unhelpful exception. [#4160]
    * ``astropy.modeling``
      > Cleaned up ``repr`` of models that have no parameters. [#4076]
    * ``astropy.nddata``
      > Initializing ``NDDataArray`` from another instance now sets ``flags`` as
      expected and no longer fails when ``uncertainty`` is set [#4129].
      Initializing an ``NDData`` subclass from a parent instance
      (eg. ``NDDataArray`` from ``NDData``) now sets the attributes other than
      ``data`` as it should [#4137].
    * ``astropy.table``
      > Fix bug when doing outer join on multi-dimensional columns. [#4060]
      > Fix an issue with setting fill value when column dtype is changed. [#4088]
      > Fix bug when unpickling a bare Column where the _parent_table
      attribute was not set.  This impacted the Column representation. [#4099]
      > Fix issue with the web browser opening with an empty page, and ensure that
      the url is correctly formatted for Windows. [#4132]
      > Fix NameError in table stack exception message. [#4213]
    * ``astropy.utils``
      > ``resolve_name`` no longer causes ``sys.modules`` to be cluttered with
      additional copies of modules under a package imported like
      ``resolve_name('numpy')``. [#4084]
      > ``console`` was updated to support IPython 4.x and Jupyter 1.x.
      This should supress a ShimWarning that was appearing at
      import of astropy with IPython 4.0 or later. [#4078]
      > Temporary downloaded files created by ``get_readable_fileobj`` when passed
      a URL are now deleted immediately after the file is closed. [#4198]
    * ``astropy.visualization``
      > The color for axes labels was set to white. Since white labels on white
      background are hard to read, the label color has been changed to black.
      [#4143]
      > ``ImageNormalize`` now automatically determines ``vmin``/``vmax``
      (via the ``autoscale_None`` method) when they have not been set
      explicitly. [#4117]
    * ``astropy.vo``
      > Cone Search validation no longer crashes when the provider gives an
      incomplete test query. It also ensures search radius for a test query
      is not too large to avoid timeout. [#4158, #4159]
    + Other Changes and Additions
    - Astropy now supports Python 3.5. [#4027]
    - Updated bundled version of astropy-helpers to 1.0.5. [#4215]
    - Updated tests to support py.test 2.7, and upgraded the bundled copy of
      py.test to v2.7.3. [#4027]
  - Update to 1.0.4
    + New Features
    * ``astropy.convolution``
      > Modified Cython functions to release the GIL. This enables convolution
      to be parallelized effectively and gives large speedups when used with
      multithreaded task schedulers such as Dask. [#3949]
    + API Changes
    * ``astropy.coordinates``
      > Some transformations for an input coordinate that's a scalar now correctly
      return a scalar.  This was always the intended behavior, but it may break
      code that has been written to work-around this bug, so it may be viewed as
      an unplanned API change [#3920]
    * ``astropy.visualization``
      > The ``astropy_mpl_style`` no longer sets ``interactive`` to ``True``, but
      instead leaves it at the user preference.  This makes using the style
      compatible with building docs with Sphinx, and other non-interactive
      contexts. [#4030]
    + Bug Fixes
    * ``astropy.coordinates``
      > Fix bug where coordinate representation setting gets reset to default value
      when coordinate array is indexed or sliced. [#3824]
      > Fixed confusing warning message shown when using dates outside current IERS
      data. [#3844]
      > ``get_sun`` now yields a scalar when the input time is a scalar (this was a
      regression in v1.0.3 from v1.0.2) [#3998]
      > Fixed bug where some scalar coordinates were incorrectly being changed to
      length-1 array coordinates after transforming through certain frames.
      [#3920]
      > Fixed bug causing the ``separation`` methods of ``SkyCoord`` and frame
      classes to fail due to infinite recursion [#4033]
      > Made it so that passing in a list of ``SkyCoord`` objects that are in
      UnitSphericalRepresentation to the ``SkyCoord`` constructor appropriately
      yields a new object in UnitSphericalRepresentation [#3938]
    * ``astropy.cosmology``
      > Fixed wCDM to not ignore the Ob0 parameter on initialization. [#3934]
    * ``astropy.io.fits``
      > Fixed crash when updating data in a random groups HDU opened in update
      mode. [#3730]
      > Fixed incorrect checksum / datasum being written when re-writing a scaled
      HDU (i.e. non-trivial BSCALE and/or BZERO) with
      ``do_not_scale_image_data=False``. [#3883]
      > Fixed stray deprecation warning in ``BinTableHDU.copy()``. [#3789]
      > Better handling of the ``BLANK`` keyword when auto-scaling scaled image
      data.  The ``BLANK`` keyword is now removed from the header after
      auto-scaling is applied, and it is restored properly (with floating point
      NaNs replaced by the filler value) when updating a file opened with the
      ``scale_back=True`` argument.  Invalid usage of the ``BLANK`` keyword is
      also better warned about during validation. [#3865]
      > Reading memmaped scaled images won't fail when
      ``do_not_scale_image_data=True`` (that is, since we're just reading the raw
      / physical data there is no reason mmap can't be used). [#3766]
      > Fixed a reference cycle that could sometimes cause FITS table-related
      objects (``BinTableHDU``, ``ColDefs``, etc.) to hang around in memory
      longer than expected. [#4012]
    * ``astropy.modeling``
      > Added missing default values for ``Ellipse2D`` parameters. [#3903]
      > Improved support for pickling of compound models, including both compound
      model instances, and new compound model classes. [#3867]
    * ``astropy.table``
      > Added missing default values for ``Ellipse2D`` parameters. [#3903]
    * ``astropy.time``
      > Fixed iteration of scalar ``Time`` objects so that ``iter()`` correctly
      raises a ``TypeError`` on them (while still allowing ``Time`` arrays to be
      iterated). [#4048]
    * ``astropy.units``
      > Added frequency-equivalency check when declaring doppler equivalencies
      [#3728]
      > Define ``floor_divide`` (``//``) for ``Quantity`` to be consistent
      ``divmod``, such that it only works where the quotient is dimensionless.
      This guarantees that ``(q1 // q2) * q2 + (q1 % q2) == q1``. [#3817]
      > Fixed the documentation of supported units to correctly report support for
      SI prefixes.  Previously the table of supported units incorrectly showed
      several derived unit as not supporting prefixes, when in fact they do.
      [#3835]
      > Fix a crash when calling ``astropy.units.cds.enable()``.  This will now
      "set" rather than "add" units to the active set to avoid the namespace
      clash with the default units. [#3873]
      > Ensure in-place operations on ``float32`` quantities work. [#4007]
    * ``astropy.utils``
      > The ``deprecated`` decorator did not correctly wrap classes that have a
      custom metaclass--the metaclass could be dropped from the deprecated
      version of the class. [#3997]
      > The ``wraps`` decorator would copy the wrapped function's name to the
      wrapper function even when ``'__name__'`` is excluded from the ``assigned``
      argument. [#4016]
    * Misc
      > ``fitscheck`` no longer causes scaled image data to be rescaled when
      adding checksums to existing files. [#3884]
      > Fixed an issue where running ``import astropy`` from within the source
      tree did not automatically build the extension modules if the source is
      from a source distribution (as opposed to a git repository). [#3932]
      > Fixed multiple instances of a bug that prevented Astropy from being used
      when compiled with the ``python -OO`` flag, due to it causing all
      docstrings to be stripped out. [#3923]
      > Removed source code template files that were being installed
      accidentally alongside installed Python modules. [#4014]
      > Fixed a bug in the exception logging that caused a crash in the exception
      handler itself on Python 3 when exceptions do not include a message.
      [#4056]
  - update to version 1.0.3:
    * New Features
      + astropy.table
      o Greatly improved the speed of printing a large table to the
      screen when only a few rows are being displayed. [#3796]
      + astropy.time
      o Add support for the 2015-Jun-30 leap second. [#3794]
    * API Changes
      + astropy.io.ascii
      o Note that HTML formatted tables will not always be found with
      guess mode unless it passes certain heuristics that strongly
      suggest the presence of HTML in the input. Code that expects
      to read tables from HTML should specify format='html'
      explicitly. See bug fixes below for more details. [#3693]
    * Bug Fixes
      + astropy.convolution
      o Fix issue with repeated normalizations of Kernels. [#3747]
      + astropy.coordinates
      o Fixed get_sun to yield frames with the obstime set to what's
      passed into the function (previously it incorrectly always had
      J2000). [#3750]
      o Fixed get_sun to account for aberration of light. [#3750]
      o Fixed error in the GCRS->ICRS transformation that gave
      incorrect distances. [#3750]
      + astropy.io.ascii
      o Remove HTML from the list of automatically-guessed formats
      when reading if the file does not appear to be HTML. This was
      necessary to avoid a commonly-encountered segmentation fault
      occurring in the libxml parser on MacOSX. [#3693]
      + astropy.io.fits
      o Fixes to support the upcoming Numpy 1.10. [#3419]
      + astropy.modeling
      o Polynomials are now scaled when used in a compound
      model. [#3702]
      o Fixed the Ellipse2D model to be consistent with Disk2D in how
      pixels are included. [#3736]
      o Fixed crash when evaluating a model that accepts no
      inputs. [#3772]
      + astropy.testing
      o The Astropy py.test plugins that disable unintential internet
      access in tests were also blocking use of local UNIX sockets
      in tests, which prevented testing some multiprocessing
      code--fixed. [#3713]
      + astropy.units
      o Supported full SI prefixes for the barn unit ("picobarn",
      "femtobarn", etc.) [#3753]
      o Fix loss of precision when multiplying non-whole-numbered
      powers of units together. For example, before this change,
      (u.m ** 1.5) ** Fraction(4, 5) resulted in an inaccurate
      floating-point power of 1.2000000000000002. After this change,
      the exact rational number of Fraction(6, 5) is
      maintained. [#3790]
      o Fixed printing of object ndarrays containing multiple Quantity
      objects with differing / incompatible units. Note: Unit
      conversion errors now cause a UnitConversionError exception to
      be raised. However, this is a subclass of the UnitsError
      exception used previously, so existing code that catches
      UnitsError should still work. [#3778]
    * Other Changes and Additions
    - Added a new astropy.__bibtex__ attribute which gives a citation
      for Astropy in bibtex format. [#3697]
    - The bundled version of ERFA was updated to v1.2.0 to address
      leapscond updates. [#3802]
* Mon Jul 27 2015 toddrme2178@gmail.com
  - Fix hdf5 version requirement
* Thu May 21 2015 toddrme2178@gmail.com
  - update to version 1.0.2:
    * New Features
      + "astropy.modeling"
      o Added support for polynomials with degree 0 or degree greater
      than 15.  [#3574, 3589]
    * Bug Fixes
      + "astropy.config"
      o The pre-astropy-0.4 configuration API has been fixed. It was
      inadvertently broken in 1.0.1. [#3627]
      + "astropy.io.fits"
      o Fixed handling of BINTABLE with TDIMn of size 1. [#3580]
      o Fixed a severe memory leak that occurred when reading tile
      compressed images. [#3680]
      o Fixed bug where column data could be unintentionally
      byte-swapped when copying data from an existing FITS file to a
      new FITS table with a TDIMn keyword for that column. [#3561]
      o The "ColDefs.change_attrib", "ColDefs.change_name", and
      "ColDefs.change_unit" methods now work as advertised.  It is
      also possible (and preferable) to update attributes directly
      on "Column" objects (for example setting "column.name"), and
      the change will be accurately reflected in any associated
      table data and its FITS header.  [#3283, #1539, #2618]
      o Fixes an issue with the "FITS_rec" interface to FITS table
      data, where a "FITS_rec" created by copying an existing FITS
      table but adding new rows could not be sliced or masked
      correctly.  [#3641]
      + "astropy.io.votable"
      o Loading a "TABLE" element without any "DATA" now correctly
      creates a 0-row array. [#3636]
      + "astropy.modeling"
      o Added workaround to support inverses on compound models when
      one of the sub-models is itself a compound model with a
      manually-assigned custom inverse. [#3542]
      o Fixed instantiation of polynomial models with constraints for
      parameters (constraints could still be assigned after
      instantiation, but not during).  [#3606]
      o Fixed fitting of 2D polynomial models with the
      "LeVMarLSQFitter". [#3606]
      + "astropy.table"
      o Ensure "QTable" can be pickled [#3590]
      o Some corner cases when instantiating an "astropy.table.Table"
      with a Numpy array are handled [#3637]. Notably:
      o a zero-length array is the same as passing "None"
      o a scalar raises a "ValueError"
      o a one-dimensional array is treated as a single row of a table.
      + "astropy.time"
      o Ensure a "Column" without units is treated as an "array", not
      as an
      o Ensure a "Column" without units is treated as an "array", not
      as an dimensionless "Quantity". [#3648]
      + "astropy.units"
      o Ensure equivalencies that do more than just scale a "Quantity"
      are properly handled also in "ufunc" evaluations. [#2496,
      [#3586]]
      o The LaTeX representation of the Angstrom unit has changed from
      "\overset{\circ}{A}" to "\mathring{A}", which should have
      better support across regular LaTeX, MathJax and matplotlib
      (as of version 1.5) [#3617]
      + "astropy.vo"
      o Using HTTPS/SSL for communication between SAMP hubs now works
      correctly on all supported versions of Python [#3613]
      + "astropy.wcs"
      o When no "relax" argument is passed to "WCS.to_header()" and
      the result omits non-standard WCS keywords, a warning is
      emitted. [#3652]
    * Other Changes and Additions
      + Nothing changed yet.
      + "astropy.units"
      o Clarified imperial mass measurements and added pound force
      (lbf), kilopound (kip), and pound per square inch
      (psi). [#3409]
      + "astropy.vo"
      o The number of retries for connections in "astropy.vo.samp" can
      now be configured by a "n_retries" configuration
      option. [#3612]
      + Testing
      o Running "astropy.test()" from within the IPython prompt has
      been provisionally re-enabled. [#3184]
  - update to version 1.0.1:
    * Bug Fixes
    - astropy.constants
      + Ensure constants can be turned into Quantity safely. [#3537, #3538]
    - astropy.io.ascii
      + Fix a segfault in the fast C parser when one of the column headers is empty [#3545].
      + Fixed support for reading inf and nan values with the fast
      reader in Windows. Also fixed in the case of using
      use_fast_converter=True with the fast reader. [#3525]
      + Fixed use of mmap in the fast reader on Windows. [#3525]
      + Fixed issue where commented header would treat comments
      defining the table (i.e. column headers) as purely information
      comments, leading to problems when trying to round-trip the
      table. [#3562]
    - astropy.modeling
      + Fixed propagation of parameter constraints ('fixed', 'bounds',
      'tied') between compound models and their components. There is
      may still be some difficulty defining 'tied' constraints
      properly for use with compound models, however. [#3481]
    - astropy.nddata
      + Restore several properties to the compatibility class
      NDDataArray that were inadvertently omitted [#3466].
    - astropy.time
      + Time objects now always evalutate to True, except when
      empty. [#3530]
    * Other Changes and Additions
    - Updated bundled astropy-helpers version to v1.0.1 to address
      installation issues with some packages that depend on
      Astropy. [#3541]
    * Miscellaneous
    - astropy._erfa
      + The ERFA wrappers are now written directly in the Python/C API
      rather than using Cython, for greater performance. [#3521]
    - Improve import time of astropy [#3488].
  - specfile: added fits2bitmap binary
  - update to version 1.0:
    * General
    - Astropy now requires a Numpy 1.6.0 or later.
    * New Features
    - astropy.analytic_functions
      + The astropy.analytic_functions was added to contain analytic
      functions useful for astronomy [#3077].
    - astropy.coordinates
      + astropy.coordinates now has a full stack of frames allowing
      transformations from ICRS or other celestial systems down to
      Alt/Az coordinates. [#3217]
      + astropy.coordinates now has a get_sun function that gives the
      coordinates of the Sun at a specified time. [#3217]
      + SkyCoord now has to_pixel and from_pixel methods that convert
      between celestial coordinates as SkyCoord objects and pixel
      coordinates given an astropy.wcs.WCS object. [#3002]
      + SkyCoord now has search_around_sky and search_around_3d
      convenience methods that allow searching for all coordinates
      within a certain distance of another SkyCoord. [#2953]
      + SkyCoord can now accept a frame instance for the frame= keyword
      argument. [#3063]
      + SkyCoord now has a guess_from_table method that can be used to
      quickly create SkyCoord objects from an astropy.table.Table
      object. [#2951]
      + astropy.coordinates now has a Galactocentric frame, a coordinate
      frame centered on a (user specified) center of the Milky
      Way. [#2761, #3286]
      + SkyCoord now accepts more formats of the coordinate string when
      the representation has ra and dec attributes. [#2920]
      + SkyCoord can now accept lists of SkyCoord objects, frame
      objects, or representation objects and will combine them into a
      single object.  [#3285]
      + Frames and SkyCoord instances now have a method
      is_equivalent_frame that can be used to check that two frames
      are equivalent (ignoring the data).  [#3330]
      + The __repr__ of coordinate objects now shows scalar coordinates
      in the same format as vector coordinates. [#3350, 3448]
    - astropy.cosmology
      + Added lookback_distance, which is c * lookback_time. [#3145]
      + Add baryonic matter density and dark matter only density
      parameters to cosmology objects [#2757].
      + Add a clone method to cosmology objects to allow copies of
      cosmological objects to be created with the specified variables
      modified [#2592].
      + Increase default numerical precision of z_at_value following the
      accurate by default, fast by explicit request model [#3074].
      + Cosmology functions that take a single (redshift) input now
      broadcast like numpy ufuncs.  So, passing an arbitrarily shaped
      array of inputs will produce an output of the same
      shape. [#3178, #3194]
    - astropy.io.ascii
      + Simplify the way new Reader classes are defined, allowing custom
      behavior entirely by overriding inherited class attributes
      instead of setting instance attributes in the Reader __init__
      method. [#2812]
      + There is now a faster C/Cython engine available for reading and
      writing simple ASCII formats like CSV. Both are enabled by
      default, and fast reading will fall back on an ordinary reader
      in case of a parsing failure. Their behavior can be altered with
      the parameter fast_reader in read and fast_writer in
      write. [#2716]
      + Make Latex/AASTex tables use unit attribute of Column for
      output. [#3064]
      + Store comment lines encountered during reading in metadata of
      the output table via meta['comment_lines']. [#3222]
      + Write comment lines in Table metadata during output for all
      basic formats, IPAC, and fast writers. This functionality can be
      disabled with comment=False. [#3255]
      + Add reader / writer for the Enhanced CSV format which stores
      table and column meta data, in particular data type and
      unit. [#2319]
      + Automatically use guess=False when reading if the file format is
      provided and the format parameters are uniquely specified.  This
      update also removes duplicate format guesses to improve
      performance. [#3418]
    - astropy.io.fits
      + The fitsdiff script ignores some things by default when
      comparing fits files (e.g. empty header lines). This adds a
    - -exact option where nothing is ignored. [#2782, #3110]
      + The fitsheader script now takes a --keyword option to extract a
      specific keyword from the header of a FITS file, and a --table
      option to export headers into any of the data formats supported
      by astropy.table. [#2555, #2588]
      + Section now supports all advanced indexing features ndarray does
      (slices with any steps, integer arrays, boolean arrays, None,
      Ellipsis).  It also properly returns scalars when this is
      appropriate. [#3148]
    - astropy.io.votable
      + astropy.io.votable.parse now takes a datatype_mapping keyword
      argument to map invalid datatype names to valid ones in order to
      support non-compliant files. [#2675]
    - astropy.modeling
      + Added the capability of creating new "compound" models by
      combining existing models using arithmetic operators.  See the
      "What's New in 1.0" page in the Astropy documentation for more
      details. [#3231]
      + A new custom_model decorator/factory function has been added for
      converting normal functions to Model classes that can work
      within the Astropy modeling framework.  This replaces the old
      custom_model_1d function which is now deprecated.  The new
      function works the same as the old one but is less limited in
      the types of models it can be used to created.  [#1763]
      + The Model and Fitter classes have .registry attributes which
      provide sets of all loaded Model and Fitter classes (this is
      useful for building UIs for models and fitting). [#2725]
      + A dict-like meta member was added to Model. it is to be used to
      store any optional information which is relevant to a project
      and is not in the standard Model class. [#2189]
      + Added Ellipse2D model. [#3124]
    - astropy.nddata
      + New array-related utility functions in astropy.nddata.utils for
      adding and removing arrays from other arrays with different
      sizes/shapes. [#3201]
      + New metaclass NDDataBase for enforcing the nddata interface in
      subclasses without restricting implementation of the data
      storage. [#2905]
      + New mixin classes NDSlicingMixin for slicing, NDArithmeticMixin
      for arithmetic operations, and NDIOMixin for input/ouput in
      NDData. [#2905]
      + Added a decorator support_nddata that can be used to write
      functions that can either take separate arguments or NDData
      objects. [#2855]
    - astropy.stats
      + Added mad_std() function. [#3208]
      + Added gaussian_fwhm_to_sigma and gaussian_sigma_to_fwhm
      constants. [#3208]
      + New function sigma_clipped_stats which can be used to quickly
      get common statistics for an array, using sigma clipping at the
      same time.  [#3201]
    - astropy.table
      + Changed the internal implementation of the Table class changed
      so that it no longer uses numpy structured arrays as the core
      table data container.  [#2790, #3179]
      + Tables can now be written to an html file that includes
      interactive browsing capabilities. To write out to this format,
      use Table.write('filename.html', format='jsviewer'). [#2875]
      + A quantity property and to method were added to Table columns
      that allow the column values to be easily converted to
      astropy.units.Quantity objects. [#2950]
      + Add unique convenience method to table. [#3185]
    - astropy.tests
      + Added a new Quantity-aware assert_quantity_allclose. [#3273]
    - astropy.time
      + Time can now handle arbitrary array dimensions, with operations
      following standard numpy broadcasting rules. [#3138]
    - astropy.units
      + Support for VOUnit has been updated to be compliant with version
      1.0 of the standard. [#2901]
      + Added an insert method to insert values into a Quantity object.
      This is similar to the numpy.insert function. [#3049]
      + When viewed in IPython, Quantity objects with array values now
      render using LaTeX and scientific notation. [#2271]
      + Added units.quantity_input decorator to validate quantity inputs
      to a function for unit compatibility. [#3072]
      + Added units.astronomical_unit as a long form for
      units.au. [#3303]
    - astropy.utils
      + Added a new decorator astropy.utils.wraps which acts as a
      replacement for the standard library's functools.wraps, the only
      difference being that the decorated function also preserves the
      wrapped function's call signature. [#2849]
      + astropy.utils.compat.numpy has been revised such that it can
      include patched versions of routines from newer numpy versions.
      The first addition is a version of broadcast_arrays that can be
      used with Quantity and other ndarray subclasses (using the
      subok=True flag). [#2327]
      + Added astropy.utils.resolve_name which returns a member of a
      module or class given the fully qualified dotted name of that
      object as a string. [#3389]
      + Added astropy.utils.minversion which can be used to check
      minimum version requirements of Python modules (to test for
      specific features and/ or bugs and the like). [#3389]
    - astropy.visualization
      + Created astropy.visualization module and added functionality
      relating to image normalization (i.e. stretching and scaling) as
      well as a new script fits2bitmap that can produce a bitmap image
      from a FITS file.  [#3201]
      + Added dictionary
      astropy.visualization.mpl_style.astropy_mpl_style which can be
      used to set a uniform plotstyle specifically for tutorials that
      is improved compared to matplotlib defaults. [#2719, #2787,
      [#3200]]
    - astropy.wcs
      + wcslib has been upgraded to version 4.25.  This brings a single
      new feature:
      + equinox and radesys will now be given default values conforming
      with the WCS specification if EQUINOXa and RADESYa,
      respectively, are not present in the header.
      + The minimum required version of wcslib is now 4.24. [#2503]
      + Added a new function wcs_to_celestial_frame that can be used to
      find the astropy.coordinates celestial frame corresponding to a
      particular WCS.  [#2730]
      + astropy.wcs.WCS.compare now supports a tolerance keyword
      argument to allow for approximate comparison of floating-point
      values. [#2503]
      + added pixel_scale_matrix, celestial, is_celestial, and
      has_celestial convenience attributes. Added
      proj_plane_pixel_scales, proj_plane_pixel_area, and
      non_celestial_pixel_scales utility functions for retrieving WCS
      pixel scale and area information [#2832, #3304]
      + Added two functions pixel_to_skycoord and skycoord_to_pixel that
      make it easy to convert between SkyCoord objects and pixel
      coordinates. [#2885]
      + all_world2pix now uses a much more sophisticated and complete
      algorithm to iteratively compute the inverse WCS
      transform. [#2816]
      + Add ability to use WCS object to define projections in
      Matplotlib, using the WCSAxes package. [#3183]
      + Added is_proj_plane_distorted for testing if pixels are
      distorted. [#3329]
    - Misc
      + astropy._erfa was added as a new subpackage wrapping the
      functionality of the ERFA library in python.  This is primarily
      of use for other astropy subpackages, but the API may be made
      more public in the future. [#2992]
    * API Changes
    - astropy.coordinates
      + Subclasses of BaseCoordinateFrame which define a custom repr
      should be aware of the format expected in SkyCoord.__repr__(),
      which changed in this release. [#2704, #2882]
      + The CartesianPoints class (deprecated in v0.4) has now been
      removed.  [#2990]
      + The previous astropy.coordinates.builtin_frames module is now a
      subpackage.  Everything that was in the
      astropy.coordinates.builtin_frames module is still accessible
      from the new package, but the classes are now in separate
      modules.  This should have no direct impact at the user
      level. [#3120]
      + Support for passing a frame as a positional argument in the
      SkyCoord class has now been deprecated, except in the case where
      a frame with data is passed as the sole positional
      argument. [#3152]
      + Improved __repr__ of coordinate objects representing a single
      coordinate point for the sake of easier copy/pasting. [#3350]
    - astropy.cosmology
      + The functional interface to the cosmological routines as well as
      set_current and get_current (deprecated in v0.4) have now been
      removed. [#2990]
    - astropy.io.ascii
      + Added a new argument to htmldict in the HTML reader named
      parser, which allows the user to specify which parser
      BeautifulSoup should use as a backend. [#2815]
      + Add FixedWidthTwoLine reader to guessing. This will allows to
      read tables that a copied from screen output like print my_table
      to be read automatically. Discussed in #3025 and #3099 [#3109]
    - astropy.io.fits
      + A new optional argument cache has been added to
      astropy.io.fits.open().  When opening a FITS file from a URL,
      cache is a boolean value specifying whether or not to save the
      file locally in Astropy's download cache (True by
      default). [#3041]
    - astropy.modeling
      + Model classes should now specify inputs and outputs class
      attributes instead of the old n_inputs and n_outputs.  These
      should be tuples providing human-readable *labels* for all
      inputs and outputs of the model.  The length of the tuple
      indicates the numbers of inputs and outputs.  See "What's New in
      Astropy 1.0" for more details. [#2835]
      + It is no longer necessary to include __init__ or __call__
      definitions in Model subclasses if all they do is wrap the
      super-method in order to provide a nice call signature to the
      docs.  The inputs class attribute is now used to generate a nice
      call signature, so these methods should only be overridden by
      Model subclasses in order to provide new functionality. [#2835]
      + Most models included in Astropy now have sensible default values
      for most or all of their parameters.  Call help(ModelClass) on
      any model to check what those defaults are.  Most of them time
      they should be overridden, but some of them are useful (for
      example spatial offsets are always set at the origin by
      default). Another rule of thumb is that, where possible, default
      parameters are set so that the model is a no-op, or close to it,
      by default. [#2932]
      + The Model.inverse method has been changed to a *property*, so
      that now accessing model.inverse on a model returns a new model
      that implements that model's inverse, and *calling*
      model.inverse(...)` on some independent variable computes the
      value of the inverse (similar to what the old Model.invert()
      method was meant to do).  [#3024]
      + The Model.invert() method has been removed entirely (it was
      never implemented and there should not be any existing code that
      relies on it).  [#3024]
      + custom_model_1d is deprecated in favor of the new custom_model
      (see "New Features" above).  [#1763]
      + The Model.param_dim property (deprecated in v0.4) has now been
      removed.  [#2990]
      + The Beta1D and Beta2D models have been renamed to Moffat1D and
      Moffat2D. [#3029]
    - astropy.nddata
      + flags, shape, size, dtype and ndim properties removed from
      astropy.nddata.NDData. [#2905]
      + Arithmetic operations, uncertainty propagation, slicing and
      automatic conversion to a numpy array removed from
      astropy.nddata.NDData. The class astropy.nddata.NDDataArray is
      functionally equivalent to the old NDData.  [#2905]
    - astropy.table
      + The Column.units property (deprecated in v0.3) has now been
      removed.  [#2990]
      + The Row.data and Table._data attributes have been deprecated
      related to the change in Table implementation.  They are
      replaced by Row.as_void() and Table.as_array() methods,
      respectively. [#2790]
      + The Table.create_mask method has been removed.  This
      undocumented method was a development orphan and would cause
      corruption of the table if called. [#2790]
      + The return type for integer item access to a Column
      (e.g. col[12] or t['a'][12]) is now always a numpy scalar, numpy
      ndarray, or numpy MaskedArray.  Previously if the column was
      multidimensional then a Column object would be returned. [#3095]
      + The representation of Table and Column objects has been changed
      to be formatted similar to the print output. [#3239]
    - astropy.time
      + The Time.val and Time.vals properties (deprecated in v0.3) and
      the Time.lon, and Time.lat properties (deprecated in v0.4) have
      now been removed. [#2990]
      + Add decimalyear format that represents time as a decimal
      year. [#3265]
    - astropy.units
      + Support for VOUnit has been updated to be compliant with version
      1.0 of the standard. This means that some VOUnit strings that
      were rejected before are now acceptable. [#2901] Notably:
    - SI prefixes are supported on most units
    - Binary prefixes are supported on "bits" and "bytes"
    - Custom units can be defined "inline" by placing them between single
      quotes.
      + Unit.get_converter has been deprecated.  It is not strictly
      necessary for end users, and it was confusing due to lack of
      support for Quantity objects. [#3456]
    - astropy.utils
      + Some members of astropy.utils.misc were moved into new
      submodules.  Specifically:
    - deprecated, deprecated_attribute, and lazyproperty ->
      astropy.utils.decorators
    - find_current_module, find_mod_objs ->
      astropy.utils.introspection
      All of these functions can be imported directly from
      astropy.utils which should be preferred over referencing
      individual submodules of astropy.utils.  [#2857]
      + The ProgressBar.iterate class method (deprecated in v0.3) has
      now been removed. [#2990]
      + Updated astropy/utils/console.py ProgressBar() module to display
      output to IPython notebook with the addition of an interactive
      kwarg. [#2658] [#2789]
    - astropy.wcs
      + The WCS.calcFootprint method (deprecated in v0.4) has now been
      removed.  [#2990]
      + An invalid unit in a CUNITn keyword now displays a warning and
      returns a UnrecognizedUnit instance rather than raising an
      exception [#3190]
    * Bug Fixes
    - astropy.convolution
      + astropy.convolution.discretize_model now handles arbitrary
      callables correctly [#2274].
    - astropy.coordinates
      + Angle.to_string now outputs unicode arrays instead of object
      arrays.  [#2981]
      + SkyCoord.to_string no longer gives an error when used with an
      array coordinate with more than one dimension. [#3340]
      + Fixed support for subclasses of UnitSphericalRepresentation and
      SphericalRepresentation [#3354, #3366]
      + Fixed latex display of array angles in IPython notebook. [#3480]
    - astropy.io.ascii
      + In the CommentedHeader the data_start parameter now defaults to
      0, which is the first uncommented line. Discussed in
      [#2692]. [#3054]
      + Position lines in FixedWidthTwoLine reader could consist of many
      characters.  Now, only one character in addition to the
      delimiter is allowed. This bug was discovered as part of [#3109]
      + The IPAC table writer now consistently uses the fill_values
      keyword to specify the output null values.  Previously the
      behavior was inconsistent or incorrect. [#3259]
      + The IPAC table reader now correctly interprets abbreviated
      column types.  [#3279]
      + Tables that look almost, but not quite like DAOPhot tables could
      cause guessing to fail. [#3342]
    - astropy.io.fits
      + Fixed the problem in fits.open of some filenames with colon (:)
      in the name being recognized as URLs instead of file
      names. [#3122]
      + Setting memmap=True in fits.open and related functions now
      raises a ValueError if opening a file in memory-mapped mode is
      impossible. [#2298]
      + CONTINUE cards no longer end the value of the final card in the
      series with an ampersand, per the specification of the CONTINUE
      card convention. [#3282]
      + Fixed a crash that occurred when reading an ASCII table
      containing zero-precision floating point fields. [#3422]
      + When a float field for an ASCII table has zero-precision a
      decimal point (with no digits following it) is still written to
      the field as long as there is space for it, as recommended by
      the FITS standard.  This makes it less ambiguous that these
      columns should be interpreted as floats. [#3422]
    - astropy.logger
      + Fix a bug that occurred when displaying warnings that produced
      an error message dictionary changed size during
      iteration. [#3353]
    - astropy.modeling
      + Fixed a bug in SLSQPLSQFitter where the maxiter argument was not
      passed correctly to the optimizer. [#3339]
    - astropy.table
      + Fix a problem where table.hstack fails to stack multiple
      references to the same table, e.g. table.hstack([t, t]). [#2995]
      + Fixed a problem where table.vstack and table.hstack failed to
      stack a single table, e.g. table.vstack([t]). [#3313]
      + Fix a problem when doing nested iterators on a single
      table. [#3358]
      + Fix an error when an empty list, tuple, or ndarray is used for
      item access within a table.  This now returns the table with no
      rows. [#3442]
    - astropy.time
      + When creating a Time object from a datetime object the time zone
      info is now correctly used. [#3160]
      + For Time objects, it is now checked that numerical input is
      finite. [#3396]
    - astropy.units
      + Added a latex_inline unit format that returns the units in LaTeX
      math notation with negative exponents instead of fractions
      [#2622].
      + When using a unit that is deprecated in a given unit format,
      non-deprecated alternatives will be suggested. [#2806] For
      example::
      >>> import astropy.units as u
      >>> u.Unit('Angstrom', format='fits')
      WARNING: UnitsWarning: The unit 'Angstrom' has been deprecated
      in the FITS standard. Suggested: nm (with data multiplied by
      0.1).  [astropy.units.format.utils]
    - astropy.utils
      + treat_deprecations_as_exceptions has been fixed to recognize
      Astropy deprecation warnings. [#3015]
    - astropy.wcs
      + astropy.wcs.WCS.sub now accepts unicode strings as input on
      Python 2.x [#3356]
    - Misc
      + Some modules and tests that would crash upon import when using a
      non-final release of Numpy (e.g. 1.9.0rc1). [#3471]
    * Other Changes and Additions
    - The bundled copy of astropy-helpers has been updated to
      v1.0. [#3515]
    - The bundled copy of astropy-helpers has been updated to
      v1.0. [#3513]
    - Updated astropy.extern.configobj to Version 5. Version 5 uses
      six and the same code covers both Python 2 and Python 3. [#3149]
    - astropy.coordinates
      + The repr of SkyCoord and coordinate frame classes now separate
      frame attributes and coordinate information.  [#2704, #2882]
    - astropy.io.fits
      + Overwriting an existing file using the clobber=True option no
      longer displays a warning message. [#1963]
      + fits.open no longer catches OSError exceptions on missing or
      unreadable files-- instead it raises the standard Python
      exceptions in such cases. [#2756, #2785]
    - astropy.table
      + Sped up setting of Column slices by an order of
      magnitude. [#2994, #3020]
    - Updated the bundled six module to version 1.7.3 and made 1.7.3
      the minimum acceptable version of six. [#2814]
    - The version of ERFA included with Astropy is now v1.1.1 [#2971]
    - The code base is now fully Python 2 and 3 compatible and no
      longer requires 2to3. [#2033]
    - `funcsigs <https://pypi.python.org/pypi/funcsigs>`_ is included
      in utils.compat, but defaults to the inspect module components
      where available (3.3+) [#3151].
    - The list of modules displayed in the pytest header can now be
      customized.  [#3157]
    - `jinja2 <http://jinja.pocoo.org/docs/dev/>`_>=2.7 is now
      required to build the source code from the git repository, in
      order to allow the ERFA wrappers to be generated. [#3166]
  - update to version 0.4.4:
    * astropy.vo.samp
      + astropy.vo.samp is now usable on Python builds that do not
      support the SSLv3 protocol (which depends both on the version of
      Python and the version of OpenSSL or LibreSSL that it is built
      against.) [#3308]
      + The default SSL protocol used is now determined from the default
      used in the Python ssl standard library. This default may be
      different depending on the exact version of Python you are
      using. [#3308]
    * astropy.wcs
      + WCS allows slices of the form slice(None, x, y), which
      previously resulted in an unsliced copy being returned (note:
      this was previously incorrectly reported as fixed in v0.4.3)
      [#2909]
  - changes from version 0.4.3:
    * astropy.coordinates
      + The Distance class has been fixed to no longer rely on the
      deprecated cosmology functions. [#2991]
      + Ensure float32 values can be used in coordinate
      representations. [#2983]
      + Fix frame attribute inheritance in SkyCoord.transform_to()
      method so that the default attribute value (e.g. equinox) for
      the destination frame gets used if no corresponding value was
      explicitly specified. [#3106]
      + Angle accepts hours:mins or deg:mins initializers (without
      seconds). In these cases float minutes are also accepted.
      + astropy.coordinates.SkyCoord objects are now copyable. [#2888 ]
      + astropy.coordinates.SkyCoord object attributes are now
      immutable. It is still technically possible to change the
      internal data for an array-valued coordinate object but this
      leads to inconsistencies [#2889] and should not be done. [#2888]
    * astropy.cosmology
      + The ztol keyword argument to z_at_value now works correctly
      [#2993].
    * astropy.io.ascii
      + Fix a bug in Python 3 when guessing file format using a file
      object as input. Also improve performance in same situation for
      Python 2. [#3132]
      + Fix a problem where URL was being downloaded for each
      guess. [#2001]
    * astropy.io.fits
      + The in operator now works correctly for checking if an extension
      is in an HDUList (as given via EXTNAME, (EXTNAME, EXTVER)
      tuples, etc.) [#3060]
      + Added workaround for bug in MacOS X <= 10.8 that caused
      np.fromfile to fail. [#3078]
      + Added support for the RICE_ONE compression type synonym. [#3115]
    * astropy.modeling
      + Fixed a test failure on Debian/PowerPC and Debian/s390x. [#2708]
      + Fixed crash in evaluating models that have more outputs than
      inputs--this case may not be handled as desired for all
      conceivable models of this format (some may have to implement
      custom prepare_inputs and prepare_outputs methods). But as long
      as all outputs can be assumed to have a shape determined from
      the broadcast of all inputs with all parameters then this can be
      used safely. [#3250]
    * astropy.table
      + Fix a bug that caused join to fail for multi-dimensional
      columns. [#2984]
      + Fix a bug where MaskedColumn attributes which had been changed
      since the object was created were not being carried through when
      slicing. [#3023]
      + Fix a bug that prevented initializing a table from a structured
      array with multi-dimensional columns with copy=True. [#3034]
      + Fixed unnecessarily large unicode columns when instantiating a
      table from row data on Python 3. [#3052]
      + Improved the warning message when unable to aggregate
      non-numeric columns. [#2700]
    * astropy.units
      + Operations on quantities with incompatible types now raises a
      much more informative TypeError. [#2934]
      + Quantity.tolist now overrides the ndarray method to give a
      NotImplementedError (by renaming the previous list
      method). [#3050]
      + Quantity.round now always returns a Quantity (previously it
      returned an ndarray for decimals>0). [#3062]
      + Ensured np.squeeze always returns a Quantity (it only worked if
      no dimensions were removed). [#3045]
      + Input to Quantity with a unit attribute no longer can get
      mangled with copy=False. [#3051]
      + Remove trailing space in __format__ calls for dimensionless
      quantities. [#3097]
      + Comparisons between units and non-unit-like objects now works
      correctly. [#3108]
      + Units with fractional powers are now correctly multiplied
      together by using rational arithmetic. [#3121]
      + Removed a few entries from spectral density equivalencies which
      did not make sense. [#3153]
    * astropy.utils
      + Fixed an issue with the deprecated decorator on classes that
      invoke super() in their __init__ method. [#3004]
      + Fixed a bug which caused the metadata_conflicts parameter to be
      ignored in the astropy.utils.metadata.merge function. [#3294]
    * astropy.vo
      + Fixed an issue with reconnecting to a SAMP Hub. [#2674 ]
    * astropy.wcs
      + Invalid or out of range values passed to wcs_world2pix will now
      be correctly identified and returned as nan values. [#2965]
      + Fixed an issue which meant that Python thought WCS objects were
      iterable. [#3066]
    * Misc
      + Astropy will now work if your Python interpreter does not have
      the bz2 module installed. [#3104]
      + Fixed ResourceWarning for astropy/extern/bundled/six.py that
      could occur sometimes after using Astropy in Python 3.4. [#3156]
    * astropy.coordinates
      + Improved the agreement of the FK5 <-> Galactic conversion with
      other codes, and with the FK5 <-> FK4 <-> Galactic
      route. [#3107]
  - specfile:
    * update copyright year
    * added libhdf5 requirement
  - update to version 0.4.2:
    * astropy.coordinates
    - Angle accepts hours:mins or deg:mins initializers (without
      seconds). In these cases float minutes are also accepted.
    - The repr for coordinate frames now displays the frame
      attributes (ex: ra, dec) in a consistent order. It should be
      noted that as part of this fix, the
      BaseCoordinateFrame.get_frame_attr_names() method now returns
      an OrderedDict instead of just a dict. [#2845]
    * astropy.io.fits
    - Fixed a crash when reading scaled float data out of a FITS file
      that was loaded from a string (using HDUList.fromfile) rather
      than from a file. [#2710]
    - Fixed a crash when reading data from an HDU whose header
      contained in invalid value for the BLANK keyword (e.g., a string
      value instead of an integer as required by the FITS
      Standard). Invalid BLANK keywords are now warned about, but are
      otherwise ignored. [#2711]
    - Fixed a crash when reading the header of a tile-compressed HDU
      if that header contained invalid duplicate keywords resulting in
      a KeyError [#2750]
    - Fixed crash when reading gzip-compressed FITS tables through the
      Astropy Table interface. [#2783]
    - Fixed corruption when writing new FITS files through to gzipped
      files. [#2794]
    - Fixed crash when writing HDUs made with non-contiguous data
      arrays to file-like objects. [#2794]
    - It is now possible to create astropy.io.fits.BinTableHDU objects
      with a table with zero rows. [#2916]
    * astropy.io.misc
    - Fixed a bug that prevented h5py Dataset objects from being
      automatically recognized by Table.read. [#2831]
    * astropy.modeling
    - Make LevMarLSQFitter work with weights keyword. [#2900]
    * astropy.table
    - Fixed reference cycle in tables that could prevent Table objects
      from being freed from memory. [#2879]
    - Fixed an issue where Table.pprint() did not print the header to
      stdout when stdout is redirected (say, to a file). [#2878]
    - Fixed printing of masked values when a format is
      specified. [#1026]
    - Ensured that numpy ufuncs that return booleans return plain
      ndarray instances, just like the comparison operators. [#2963]
    * astropy.time
    - Ensure bigendian input to Time works on a little-endian machine
      (and vice versa). [#2942]
    * astropy.units
    - Ensure unit is kept when adding 0 to quantities. [#2968]
    * astropy.utils
    - Fixed color printing on Windows with IPython 2.0. [#2878]
    * astropy.vo
    - Improved error message on Cone Search time out. [#2687]
    * Fixed a couple issues with files being inappropriately included
      and/or excluded from the source archive distributions of
      Astropy. [#2843, #2854]
    * As part of fixing the fact that masked elements of table columns
      could not be printed when a format was specified, the column
      format string options were expanded to allow simple specifiers
      such as '5.2f'. [#2898]
    * Ensure numpy 1.9 is supported. [#2917]
    * Ensure numpy master is supported, by making np.cbrt work with
      quantities. [#2937]

Files

/etc/alternatives/fits2bitmap
/etc/alternatives/fitscheck
/etc/alternatives/fitsdiff
/etc/alternatives/fitsheader
/etc/alternatives/fitsinfo
/etc/alternatives/samp_hub
/etc/alternatives/volint
/etc/alternatives/wcslint
/usr/bin/fits2bitmap
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/usr/bin/fitsdiff
/usr/bin/fitsdiff-2.7
/usr/bin/fitsheader
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/usr/bin/wcslint-2.7
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/usr/lib64/python2.7/site-packages/astropy-2.0.3-py2.7.egg-info/SOURCES.txt
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/usr/lib64/python2.7/site-packages/astropy-2.0.3-py2.7.egg-info/requires.txt
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Fabrice Bellet, Thu Nov 7 23:07:43 2019