signal op• Datenarten: signal × indices → signal
• Aufruf: import fullseye as fs; fs.ledger.peak_subbin(x, idx=None, mode='parabola') (die Implementierung direkt: import dsp; dsp.peak_subbin(x, idx=None, mode='parabola'); aus dem Register: ops1d.get("peak_subbin"))
> Für diesen Operator gibt es noch keine Übersetzung. Es folgt der Originaltext unverändert.
Peak position between samples — the vertex of a fit through 3 points.
find_peaks returns integer indices, so the position of a spectral line or a correlation peak is quantised to the bin grid no matter how finely the peak itself is resolved. This refines each index to a float by fitting the sample and its two neighbours.
*mode* picks what is fitted:
"parabola"
a x^2 + b x + c through the three raw values. The classic estimator;
exact for a genuinely parabolic top and cheap.
"gauss"
the same parabola through log of the three values, which is exact for
a Gaussian peak. Requires all three values positive — a magnitude
spectrum qualifies, a signed correlation does not. Non-positive
neighbourhoods raise ValueError rather than silently returning the
integer index, because "the refinement quietly did nothing" is the
failure this operator exists to remove.
Measured on a Gaussian of width 1.7 bins centred at 40.37: the integer argmax gives 40 (error 0.37 bins), parabola gives 40.3553 (error 0.0147) and gauss gives 40.3700 (error 0, to machine precision). The parabola is biased on a Gaussian, and the bias grows as the peak gets narrower — the same measurement at widths 6.0 / 3.0 / 1.7 / 1.0 bins errs by 0.0012 / 0.0047 / 0.0147 / 0.0434. That is the whole reason gauss
exists: for a spectral line the log-parabola is not an approximation, it is the exact model.
The refinement is still an assumption about shape, not a measurement of it. On a triangular peak, whose top is not smooth, parabola errs by 0.0857 bins where the integer index errs by 0.30 — better, but three times worse than on the Gaussian it was designed for.
The shift is not clamped. A vertex more than half a sample away from the index means the index was not a local maximum in the first place, and that is
information: clamping it to +/-0.5 would return a plausible number for a bin that has no peak in it. Run find_peaks first, or clamp deliberately at the call site when evaluating bins that are not maxima (a harmonic comb, for instance).
A peak sitting on the first or last sample has no neighbour on one side and keeps its integer position (there is nothing to interpolate against); the returned array says so by being exactly equal to the input index there.
x : array_like
The 1-D signal the peaks were found in.
idx : int, sequence of int, or None
Peak indices. None means "the argmax", so peak_subbin(mag) is the
one-liner for a single line.
mode : {"parabola", "gauss"}
float or ndarray
Refined position(s) in samples. Scalar in, scalar out.
find_peaks : which indices to refine.
• Katalog der Beispieldaten (Download-URLs / Lizenzen) — 2-D nutzt skimage.data (BSD/Public Domain) plus synthetische Bilder, 3-D nennt Download-URLs echter Datenquellen (Stanford, PDS, …).
• Herkunft und Literatur der Operatoren — die Quellen der Forschung/Verfahren, auf denen diese Operatorfamilie beruht.
• Der kanonische Algorithmus (Autor, Jahr) und seine Anwendungen stehen im Familienleitfaden oben.
• poc_multibeam_bathymetry — py -3.11 examples/poc_multibeam_bathymetry.py
• poc_print_registration — py -3.11 examples/poc_print_registration.py
• poc_web_roll_periodicity — py -3.11 examples/poc_web_roll_periodicity.py
signal als Eingabe)create_funct_1d_array · create_funct_1d_pairs · smooth_funct_1d_gauss · smooth_funct_1d_mean · derivate_funct_1d · integrate_funct_1d · zero_crossings_funct_1d · local_min_max_funct_1d
signal)lowpass · highpass · bandpass · envelope · rms · local_std · quantize · companding_mu_law
*Provenance: dsp.py — ONED Operator-Registry. Diese Notiz wird von tools/opdocs.py md erzeugt (nicht von Hand bearbeiten).*
© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.