Correcting window size for mass averages. #73
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elenagonzalez870
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May 8, 2026
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- Currently, the local squared mass averages are calculated within a window that is either AVEKERNEL or 1.0e-4 * ((double) clus.N_STAR) / 2.0. For clusters with a large number of stars, this means that mass averages are computed over a window containing thousands of neighbors. This is inconsitent with the fact that other averaged local quantities (like calc_n_local) are always calculated in a fixed window, and it is likely just legacy code that was never changed.
…window that is either AVEKERNEL or 1.0e-4 * ((double) clus.N_STAR) / 2.0. For clusters with a large number of stars, this means that mass averages are computed over a window containing thousands of neighbors. This is inconsitent with the fact that other averaged local quantities (like calc_n_local) are always calculated in a fixed window, and it is likely just legacy code that was never changed.
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Pull request overview
This PR updates the neighbor-window selection used when computing the local average of mass², making it consistently use the fixed AVEKERNEL window size instead of scaling with clus.N_STAR.
Changes:
- Set the averaging half-window
pincalc_average_mass_sqr()to always beAVEKERNEL(removing theMAX(1e-4*N_STAR/2, AVEKERNEL)scaling).
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looks good to me! |
carlrodriguez
self-requested a review
May 25, 2026 17:44
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