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Along with/in place of migrating ztfperiodic to scope (#189), we should consider using cesium for ZTF light curve feature generation going forward. It will be important to ensure a reasonable level of consistency between new and old scope feature sets.
Below are my initial findings for ztfperiodic features that appear to be missing (or different) in cesium after searching through descriptions here. This list may be updated if suitably similar features are identified in cesium.
Missing features from cesium
Anderson-Darling (ad)
Shapiro-Wilk (sw)
welch_i
f1_bic
f1_a
f1_b
f1_phi0
f1_power
von Neumann statistic (inv_vonneumannratio)
norm_excess_var
roms
significance
smallkurt
wstd
Different in cesium
chi2red: the only chi2 features in cesium are qso_log_chi2_qsonu and qso_log_chi2nuNULL_chi2nu
norm_peak_to_peak_amp: has some similar features; percent_amplitude and percent_difference_flux_percentile
slight differences in percentile flux ratios (e.g. i60r is closest to flux_percentile_ratio_mid65)
The text was updated successfully, but these errors were encountered:
Along with/in place of migrating
ztfperiodic
to scope (#189), we should consider using cesium for ZTF light curve feature generation going forward. It will be important to ensure a reasonable level of consistency between new and old scope feature sets.Below are my initial findings for
ztfperiodic
features that appear to be missing (or different) incesium
after searching through descriptions here. This list may be updated if suitably similar features are identified incesium
.Missing features from cesium
ad
)sw
)welch_i
f1_bic
f1_a
f1_b
f1_phi0
f1_power
inv_vonneumannratio
)norm_excess_var
roms
significance
smallkurt
wstd
Different in cesium
chi2red
: the only chi2 features incesium
areqso_log_chi2_qsonu
andqso_log_chi2nuNULL_chi2nu
norm_peak_to_peak_amp
: has some similar features;percent_amplitude
andpercent_difference_flux_percentile
i60r
is closest toflux_percentile_ratio_mid65
)The text was updated successfully, but these errors were encountered: