| /dports/math/armadillo/armadillo-10.7.1/include/armadillo_bits/ |
| H A D | gmm_full_bones.hpp | 83 …template<typename T1> inline Row<eT> norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_…
|
| H A D | gmm_diag_bones.hpp | 83 …template<typename T1> inline Row<eT> norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_…
|
| H A D | gmm_diag_meat.hpp | 625 gmm_diag<eT>::norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_mode) const in norm_hist() function in gmm_priv::gmm_diag
|
| H A D | gmm_full_meat.hpp | 664 gmm_full<eT>::norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_mode) const in norm_hist() function in gmm_priv::gmm_full
|
| /dports/math/R-cran-RcppArmadillo/RcppArmadillo/inst/include/armadillo_bits/ |
| H A D | gmm_diag_bones.hpp | 83 …template<typename T1> inline Row<eT> norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_…
|
| H A D | gmm_full_bones.hpp | 83 …template<typename T1> inline Row<eT> norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_…
|
| H A D | gmm_full_meat.hpp | 664 gmm_full<eT>::norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_mode) const in norm_hist() function in gmm_priv::gmm_full
|
| H A D | gmm_diag_meat.hpp | 625 gmm_diag<eT>::norm_hist(const Base<eT,T1>& expr, const gmm_dist_mode& dist_mode) const in norm_hist() function in gmm_priv::gmm_diag
|
| /dports/math/py-seaborn/seaborn-0.11.0/seaborn/ |
| H A D | distributions.py | 2402 color=None, vertical=False, norm_hist=False, axlabel=None, argument
2576 norm_hist = norm_hist or kde or (fit is not None)
2608 hist_kws.setdefault("density", norm_hist)
|
| /dports/math/octave-forge-image/image-2.12.0/inst/ |
| H A D | graythresh.m | 269 norm_hist = ihist / total; variable
270 total_mean = sum (bins .* norm_hist);
271 total_variance = sum (((bins - total_mean).^2) .* norm_hist);
|
| /dports/math/py-Pyomo/Pyomo-6.1.2/pyomo/contrib/parmest/ |
| H A D | graphics.py | 299 g.map_diag(sns.distplot, kde=False, hist=True, norm_hist=False)
|
| /dports/astro/py-pykep/pykep-2.6/doc/sphinx/examples/ |
| H A D | conjunctions.ipynb | 1845 …"sns.distplot(np.array(mins) * pykep.EARTH_RADIUS / 1000, hist=True, kde=False, norm_hist=True, bi…
1850 …"sns.distplot(np.array(mins) * pykep.EARTH_RADIUS / 1000, hist=True, kde=False, norm_hist=True, bi…
|
| /dports/astro/pykep/pykep-2.6/doc/sphinx/examples/ |
| H A D | conjunctions.ipynb | 1845 …"sns.distplot(np.array(mins) * pykep.EARTH_RADIUS / 1000, hist=True, kde=False, norm_hist=True, bi…
1850 …"sns.distplot(np.array(mins) * pykep.EARTH_RADIUS / 1000, hist=True, kde=False, norm_hist=True, bi…
|