Original three-dataset framework#
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The current multidimensional GP models support an arbitrary number of datasets and heterogeneous cadences. PyORBIT also keeps the older Rajpaul-style framework, where the model is built from exactly three synchronous datasets: radial velocities, one chromospheric activity indicator, and BIS.
This model is mainly retained for reproducibility of older analyses. For new analyses, the multidimensional models described in the quasi-periodic kernel page are usually more flexible.
Model definition and requirements#
model name: gp_framework_quasiperiodic
required common object:
activityexpects three datasets with the same times and length
supported dataset roles: RV, one of
H-alpha,S_index, orCa_HK, andBIS
model name: gp_pyaneti_quasiperiodic
required common object:
activitymultidimensional quasi-periodic model using the
pyanetibackendsupports the same dataset coefficient notation as the newer multidimensional models
Keywords#
Model-wide keywords, with the default value in boldface.
hyperparameters_condition
accepted values:
True|Falseactivates the quasi-periodic hyperparameter condition described in the quasi-periodic kernel.
rotation_decay_condition
accepted values:
True|Falseif activated, requires
Pdec > 2 Prot.
use_stellar_rotation_period
accepted values:
True|Falsereplaces
Protwithrotation_periodfromstar_parameters.
use_stellar_activity_decay
accepted values:
True|Falsereplaces
Pdecwithactivity_decayfromstar_parameters.
derivative
accepted values: mapping of dataset names to booleans
available for
gp_pyaneti_quasiperiodic. IfFalse, the derivative coefficientrot_ampis fixed to zero for that dataset.
Examples#
Original fixed framework:
1inputs:
2 RVdata:
3 file: datasets/RV_PyORBIT.dat
4 kind: RV
5 models:
6 - gp_framework
7 Sdata:
8 file: datasets/Sindex_PyORBIT.dat
9 kind: S_index
10 models:
11 - gp_framework
12 BISdata:
13 file: datasets/BIS_PyORBIT.dat
14 kind: BIS
15 models:
16 - gp_framework
17common:
18 activity:
19 boundaries:
20 Prot: [10.0, 20.0]
21 Pdec: [20.0, 1000.0]
22 Oamp: [0.001, 1.0]
23 Vc: [-100.0, 100.0]
24 Vr: [-100.0, 100.0]
25 Lc: [-10.0, 10.0]
26 Bc: [-100.0, 100.0]
27 Br: [-100.0, 100.0]
28models:
29 gp_framework:
30 model: gp_framework_quasiperiodic
31 common: activity
32 hyperparameters_condition: True
pyaneti multidimensional backend:
1models:
2 gp_pyaneti:
3 model: gp_pyaneti_quasiperiodic
4 common: activity
5 hyperparameters_condition: True
6 RVdata:
7 boundaries:
8 rot_amp: [0.0, 20.0]
9 con_amp: [-20.0, 20.0]
10 derivative: True
11 Sdata:
12 boundaries:
13 con_amp: [-1.0, 1.0]
14 derivative: False
Model parameters#
gp_framework_quasiperiodic#
Name |
Parameter |
Common? |
Definition |
Notes |
|---|---|---|---|---|
|
Rotational period of the star |
common |
|
|
|
Decay timescale of active regions |
common |
|
|
|
Coherence scale |
common |
|
|
|
Coefficient of |
common |
|
|
|
Coefficient of |
common |
|
|
|
Coefficient of |
common |
|
|
|
Coefficient of |
common |
|
|
|
Coefficient of |
common |
|
gp_pyaneti_quasiperiodic#
Name |
Parameter |
Common? |
Definition |
Notes |
|---|---|---|---|---|
|
Rotational period of the star |
common |
|
|
|
Decay timescale of active regions |
common |
|
|
|
Coherence scale |
common |
|
|
|
Coefficient of the latent GP |
dataset |
|
|
|
Coefficient of the first derivative of the latent GP |
dataset |
|
Fixed to zero when |