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Task to be done to have a model with binary source and their full orbital motion (BSPL_xallarap branch):
make sure .n_sources for xallarap models depends on whether q_source is defined or not
second source trajectory - shift by 180 in xi_u and change xi_semimajor_axis
ModelParameters._update_sources() - update and add calls to it
source mass ratio in ModelParameters
limit source mass ratio to > 0.
ModelParameters.source_2_parameters
make sure q_source cannot be mixed with, e.g., t_0_X
Currently the xallarap parameters of each source are not obtained directly (like, e.g., t_0_1) - do we want that? xi_a_2 is problematic. After discussion with @jenniferyee : No. We should give proper documentation only.
tests for FS case - code changed in commit 053a760
I think q_source.
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Dr. Jennifer C. Yee
(she/her)
Office: P-341
Center for Astrophysics | Harvard & Smithsonian
60 Garden St, MS-15
Cambridge, MA 02138
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Task to be done to have a model with binary source and their full orbital motion (BSPL_xallarap branch):
.n_sources
for xallarap models depends on whetherq_source
is defined or notxi_u
and changexi_semimajor_axis
ModelParameters._update_sources()
- update and add calls to itModelParameters
ModelParameters.source_2_parameters
q_source
cannot be mixed with, e.g.,t_0_X
t_0_1
) - do we want that?xi_a_2
is problematic. After discussion with @jenniferyee : No. We should give proper documentation only.Model.get_trajectory()
(see also issue #94)Trajectory()
ModelParameters.xallarap_reference_position
- define it in a standard way (including docstring)ModelParameters.xallarap_reference_position
- unit testsModelParameters
q_source
Model.plot_trajectory()
mm.ModelParameters({'t_0': 1, 'u_0': 2, 't_E': 3, 'q_source': 1})
rho_2
but withoutq_soruce
parameter_names.pdf
After merge:
_set_default_parameters()
and_check_fixed_parameters()
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