v1.0.0
API changes:
- The API of
mcmc_lc
has changed significantly (the function was marked
experimental in previous release). - [DEPRECATION] In result of
fit_lc
,res.cov_names
changed to
res.vparam_names
. - [DEPRECATION] In result of
nest_lc
,res.param_names
changed to
res.vparam_names
. This is for compatibility between the results offit_lc
andnest_lc
. [#30] - [DEPRECATION] Deprecate
flatten
keyword argument infit_lc()
in
favor of explicit use offlatten_result()
function.
Enhancements:
- Many new built-in models.
- Many new built-in bandpasses.
- New remote data fetching system. [#73]
- SALT2 model covariance available via
Model.bandfluxcov()
method and
modelcov=True
keyword argument passed tofit_lc
. - New simulation function,
zdist
, generates a distribution of redshifts
given a volumetric rate function and cosmology. - New simulation function,
realize_lcs
, simulates light curve data given a
model, parameters, and observations. - Add color-related keyword arguments to
plot_lc()
. - Add
tighten_ylim
keyword argument toplot_lc()
. - Add
chisq()
function and use internally infit_lc()
. - Add
SFD98Map
class for dealing with SFD (1998) dust maps persistently so
that the underlying FITS files are opened only once. - Update
get_ebv_from_map()
to work with new SkyCoord class in
astropy.coordinates
available in astropy v0.3 onward. Previously, this
function did not work with astropy v0.4.x (where older coordinates classes
had been removed). - Update to new configuration system available in astropy v0.4 onward.
This makes this release incompatible with astropy versions less than
0.4. - Now compatible with Python 3.
- Increased test coverage.
- Numerous minor bugfixes.