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Instrument Selected Data All Data

Observations Summary

Instrument
 		 #Meas
 		 T*min
[day]		 T*max
[day]		 ΔT
[day]		 RV
[m/s]		 RVerr
[m/s]		 FeH
 		 Vsini
[km/s]

T* = bjd - 2,400,000

Instruments

No data

Periodogram settings

Periodogram Sampling
Periodogram oversampling
Periodogram ΔP/P
Periodogram autoload

Selection criteria

Radial Velocity Filter (max error) [m/s]

Binning

Data binning

Units

Companion mass unit
Apply data selection Reload deleted points

Instruments

Select

Data Binning

Selection Criteria

Pre-binning Post-binning
Parameter From To From To
RJD (ex: 54000.0)
RV [m/s]
RV Error [m/s]
FWHM [m/s]
BIS [m/s]
Contrast [m/s]
S-Index x 1000[-]
Hα-Index [-]
Na-Index [-]
Log(R'/HK) [-]
Berv [m/s]
DRS quality control:

Correlations


X: 
Y: 

Z: 
Residuals




Correlations:

R : 0.0
Weighted R : 0.0







  • Options

    Model Sampling:
      Display Model

    From [BJD -2,450,000.0]:
    To [BJD -2,450,000.0]:
Data Binning:     




No data to display



auto

  • False Alarm Probability

    Method/Precision:
    Compute Hide

  • Periodogram configuration

    Oversamp:
    Pmin:
    Pmax:

    Sampling:
    OK




No data to display



Compute

  • Periodogram configuration

    Nb prominent peaks:
    Max iter:

    Period min [d]:
    Oversampling:

    N phi:




No data to display



  • Options

    Units:
    Orbit Sampling:
      Display orbit
Star barycentric orbit

  • Options

    Unit:
    Orbits:
Relative orbits
Acknowledgements Keplerian model initial conditions are computed using the formalism described in Delisle et al. 2016. Activity cycles are modeled following Delisle et al. 2018. Analytical FAP values are estimated following Baluev 2008, and numerical FAP values are computed by permutation of the calendar. The MCMC algorithm is described in Díaz et al. 2014, 2016. References