vr_ratio¶
Violet/Red intensity ratio of a double-peaked emission line.
| Category | Line fitting |
| Backend | scipy - implemented here on top of scipy primitives |
| Version | 1.0.1 |
| Reads | ctx.spectrum (a Spectrum1D) |
| Writes | metrics.vr_ratio, metrics.vr_ratio_minus1, metrics.v_velocity_kms, metrics.r_velocity_kms, metrics.peak_separation_kms, metrics.central_depth, metrics.fwhm_aa, metrics.single_peaked, metrics.v_intensity, metrics.r_intensity, metrics.line_center_aa, extras.vr_result |
Continuum from window-edge medians (mean of the two edge medians, edge = max(3, 0.1 · n)). Detection on the normalised flux with scipy.signal.find_peaks(prominence=min_prominence), restricted to ±0.7 · window around the centre. Returns single_peaked=True with vr_ratio=None when only one side has a peak.
Parameters¶
| Parameter | Default | Required | Description |
|---|---|---|---|
line_center_aa |
6562.82 |
- | Rest wavelength (Å) of the line centre. |
window_half_width_aa |
15.0 |
- | Half-width (Å) of the analysis window around the centre. |
min_prominence |
0.05 |
- | Peak-detection prominence on the normalised flux (find_peaks). |
Use it¶
References¶
- Okazaki 1991, PASJ 43, 75 — long-term V/R variations of Be stars from global one-armed oscillations of the disc.
- Hummel & Vrancken 2000, A&A 359, 1075 — Be-star V/R variability.
- scipy.signal.find_peaks — prominence-thresholded peak detection.
Related algorithms¶
compare_line_fits- Fit one spectral line with every profile in turn and pick the best one.equivalent_width- Measure a line's equivalent width without assuming a profile shape.fit_gaussian_line- Fit a single Gaussian (plus a linear continuum) to one spectral line.fit_lorentzian_line- Fit a single Lorentzian (plus a linear continuum) to one spectral line.fit_voigt_line- Fit a single Voigt profile (plus a linear continuum) to one spectral line.