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astrofrog authored and github-actions[bot] committed Feb 6, 2023
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# 1.4 (unreleased)

- No changes yet.
- No changes yet.

# 1.3 (2019-04-25)

- Fixed an issue that occurred during the convolution if not all SEDs
had the same number of wavelengths. \[#66\]
- Fixed an issue that occurred during the convolution if not all SEDs
- had the same number of wavelengths. [#66]

# 1.2 (2018-06-16)

- Use install_requires instead of requires.
- Use install_requires instead of requires.

# 1.1 (2018-06-16)

- Fix color of lines in SED plots. \[#52\]
- Fix Windows compatibility. \[#53\]
- Fix compatibility with Astropy 2.x and above. \[#60\]
- Fix color of lines in SED plots. [#52]
- Fix Windows compatibility. [#53]
- Fix compatibility with Astropy 2.x and above. [#60]

# 1.0 (2016-01-09)

- Fixed a bug in the calculation of the reduced chi\^2: this should
have used the number of valid data points (valid flag 1 or 4) but
instead was using the total number of valid and invalid points.
\[#49\]
- Fixed compatibility with Python 3.6. \[#49\]
- Fixed a bug in the calculation of the reduced chi^2: this should
- have used the number of valid data points (valid flag 1 or 4) but
- instead was using the total number of valid and invalid points.
- [#49]
- Fixed compatibility with Python 3.6. [#49]

# 0.9.6 (2016-07-31)

- A valid flag of \'9\' can now be used to denote a flux that should
be plotted but not fit. \[#32\]
- Fix issues that occurred if no valid fits were present for a given
source. \[#38\]
- Switch the order of the dimensions in SED flux cubes to optimize
performance. This means that this version of the SED fitter will be
incompatible with flux cubes generated with earlier versions, but
will result in significant performance improvements when plotting
SEDs. \[#44\]
- Add a `memmap` option to `convolve_model_dir` that controls whether
memory mapping is used to read the flux cubes (in the case where
SEDs are stored in cubes rather than individual files). If the cubes
can fit in memory, the convolution is much faster if the memory
mapping is explicitly turned off.
- A valid flag of '9' can now be used to denote a flux that should
- be plotted but not fit. [#32]
- Fix issues that occurred if no valid fits were present for a given
- source. [#38]
- Switch the order of the dimensions in SED flux cubes to optimize
- performance. This means that this version of the SED fitter will be
- incompatible with flux cubes generated with earlier versions, but
- will result in significant performance improvements when plotting
- SEDs. [#44]
- Add a `memmap` option to `convolve_model_dir` that controls whether
- memory mapping is used to read the flux cubes (in the case where
- SEDs are stored in cubes rather than individual files). If the cubes
- can fit in memory, the convolution is much faster if the memory
- mapping is explicitly turned off.

# 0.9.5 (2015-06-07)

- Fixed calculation of indices for monochromatic \'convolution\'.
- Fixed calculation of indices for monochromatic 'convolution'.

# 0.9.4 (2015-06-05)

- Added missing ez_setup.py file.
- Added missing ez_setup.py file.

# 0.9.3 (2015-06-05)

- Fixed a bug with filter normalization if filter was given in
increasing wavelength. \[#26\]
- Fixed plotting of source names when using Latex. \[#25\]
- Fixed a bug with filter normalization if filter was given in
- increasing wavelength. [#26]
- Fixed plotting of source names when using Latex. [#25]

# 0.9.2 (2014-12-01)

- Added support for a new model directory format that stores all SEDs
in a single file. \[#16\]
- Added a new Fitter class that provides an OO interface to the
fitter. This makes it easier to fit sources one by one without
reloading models. \[#12\]
- Various bug fixes.
- Added support for a new model directory format that stores all SEDs
- in a single file. [#16]
- Added a new Fitter class that provides an OO interface to the
- fitter. This makes it easier to fit sources one by one without
- reloading models. [#12]
- Various bug fixes.

# 0.9.1 (2014-03-10)

- Added documentation on convolution.
- Added page about accessing model packages.
- Renamed `wavelength` attribute on `Filter` and `ConvolvedFluxes` to
`central_wavelength`, renamed `r` attribute on `Filter` to
`response`, and removed `wav` attribute for `Filter` since it was
reduntant with `nu`.
- Added documentation on convolution.
- Added page about accessing model packages.
- Renamed `wavelength` attribute on `Filter` and `ConvolvedFluxes` to
- `central_wavelength`, renamed `r` attribute on `Filter` to
- `response`, and removed `wav` attribute for `Filter` since it was
- reduntant with `nu`.

# 0.9.0 (2014-01-30)

- Initial release
- Initial release

## v1.4 - 2023-02-06

### What's Changed

- Small astropy 4.0 compatibility refactor by @keflavich in https://github.com/astrofrog/sedfitter/pull/67
- Update package infrastructure and fix compatibility with latest astropy versions by @astrofrog in https://github.com/astrofrog/sedfitter/pull/79
- ndistances can't be a float in recent versions of numpy by @keflavich in https://github.com/astrofrog/sedfitter/pull/73
- Use memmap when reading in model grids by @keflavich in https://github.com/astrofrog/sedfitter/pull/78
- More infrastructure improvements by @astrofrog in https://github.com/astrofrog/sedfitter/pull/80

**Full Changelog**: https://github.com/astrofrog/sedfitter/compare/v1.3...v1.4

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