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# 1.4 (unreleased) | ||
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- No changes yet. | ||
- No changes yet. | ||
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# 1.3 (2019-04-25) | ||
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- 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] | ||
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# 1.2 (2018-06-16) | ||
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- Use install_requires instead of requires. | ||
- Use install_requires instead of requires. | ||
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# 1.1 (2018-06-16) | ||
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- 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] | ||
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# 1.0 (2016-01-09) | ||
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- 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] | ||
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# 0.9.6 (2016-07-31) | ||
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- 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. | ||
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# 0.9.5 (2015-06-07) | ||
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- Fixed calculation of indices for monochromatic \'convolution\'. | ||
- Fixed calculation of indices for monochromatic 'convolution'. | ||
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# 0.9.4 (2015-06-05) | ||
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- Added missing ez_setup.py file. | ||
- Added missing ez_setup.py file. | ||
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# 0.9.3 (2015-06-05) | ||
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- 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] | ||
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# 0.9.2 (2014-12-01) | ||
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- 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. | ||
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# 0.9.1 (2014-03-10) | ||
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- 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`. | ||
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# 0.9.0 (2014-01-30) | ||
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- Initial release | ||
- Initial release | ||
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## v1.4 - 2023-02-06 | ||
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### What's Changed | ||
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- 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 | ||
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**Full Changelog**: https://github.com/astrofrog/sedfitter/compare/v1.3...v1.4 |