You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
I am exploring the possibility of adding Scalpels to juliet (for who's not familiar with it, check Cameron+2020), and I am wondering how should it be done. From what I understand, juliet should first read the base Scalpels vector (U0) from a file, and then simply calculate the residuals during the fit as:
res = (RV_values - matrix_N@matrix_C) * (RV_values - matrix_N@matrix_C)
rv_drive is the planetary signal model evaluated with Radvel for planet 1 (and so on, if there are others), and p1 are the parameters of the first planet. Of course, for each planet there should be a new rv_drive in matrix_N and "1" in matric_C. Finally, "offset" and "alpha" are the new priors related to the Scalpels vector (if U0 is mono-dimensional, otherwise there should be an "alpha" for each dimension of the vector). For example, if we have N radial-velocity points, one planet and a mono-dimensional U0, then:
where matrix_N dimensions are Nx3 and matrix_C 3x1. So, I guess the main change should be the addition of a correction factor to K during the sampling. @nespinoza, what do you think?
The text was updated successfully, but these errors were encountered:
Hi everyone,
I am exploring the possibility of adding Scalpels to juliet (for who's not familiar with it, check Cameron+2020), and I am wondering how should it be done. From what I understand, juliet should first read the base Scalpels vector (U0) from a file, and then simply calculate the residuals during the fit as:
res = (RV_values - matrix_N@matrix_C) * (RV_values - matrix_N@matrix_C)
where
rv_drive is the planetary signal model evaluated with Radvel for planet 1 (and so on, if there are others), and p1 are the parameters of the first planet. Of course, for each planet there should be a new rv_drive in matrix_N and "1" in matric_C. Finally, "offset" and "alpha" are the new priors related to the Scalpels vector (if U0 is mono-dimensional, otherwise there should be an "alpha" for each dimension of the vector). For example, if we have N radial-velocity points, one planet and a mono-dimensional U0, then:
matrix_N@matrix_C = 1*offset + K*1 + U0*alpha = offset + K + U0*alpha.
where matrix_N dimensions are Nx3 and matrix_C 3x1. So, I guess the main change should be the addition of a correction factor to K during the sampling. @nespinoza, what do you think?
The text was updated successfully, but these errors were encountered: