Systematics Uncertainties#
NMMA currently uses --error-budget to specify the constant systematic uncertainties to be added to the likelihood quadrature.
However, it is now possible to use systematic error (\(\sigma_{sys}\)) prior in form of a freely sampled parameter, time dependent and/or filter dependent systematic error. This can done by specifying the file path using the --systematics-file in lightcurve-analysis command.
For more information on systematics error, please refer to the paper.
The following are the examples of the systematics file:
Example 1: Freely sampled (time independent) systematic error#
In this case the systematic error is freely sampled and is not dependent on time or filter.
config:
withTime:
value: false
filters:
- null
time_nodes: 4
type: Uniform
minimum: 0
maximum: 2
withoutTime:
value: true
type: Uniform
minimum: 0
maximum: 2
Example 2: Time dependent systematic error#
In this configuration, a single systematic error is applied across all filters.
config:
withTime:
value: true
filters:
- null
time_nodes: 4
type: Uniform
minimum: 0
maximum: 2
withoutTime:
value: false
type: Uniform
minimum: 0
maximum: 2
Example 3: Time and filter dependent systematic error#
In this configuration, the sdssu and ztfr filters are sampled together for systematic errors, while the 2massks filter is sampled independently. All other filters are grouped and sampled together
config:
withTime:
value: true
filters:
- [sdssu, ztfr]
- [2massks]
- null
time_nodes: 4
type: Uniform
minimum: 0
maximum: 2
withoutTime:
value: false
type: Uniform
minimum: 0
maximum: 2
Distribution types#
Distribution can be of any of the analytical prior from bilby.
Please refer to bilby documentation for more information on the available distribution type and their usage. Only positional arguments are required for any of the distrbutions.