3C 273 · Lyα Spectroscopic Pipeline
Diagnostic Viewer · IUE SWP · 3C 273

Profile Diagnostic Viewer — Interactive Spectroscopic Pipeline

Power-law continuum · grid-seeded weighted least-squares Gaussian fits · statistical verification · 994–1832 Å (rest frame)
Load Spectrum:

Upload an IUE SWP spectrum (.txt) or load the demo to run the diagnostic fitting pipeline.

Supported format: two-column wavelength · flux text file.

Spectrum: —
—
ACCEPTED
All-lines figure (PNG)
Graph 1 — Rest-frame spectrum observed flux · power-law continuum · shaded: continuum windows
Residual plot — whole spectrum data − continuum − all fitted lines · each line's window shaded in its own colour
Emission-line summary click a row to inspect the line · spectral index and amplitude are shown above (one continuum per spectrum)
LineRest λ (Å)Fitted λ (Å)σ (Å)FWHM (km/s) FluxFlux ErrEW (Å)SNR Window (Å)Min λMax λReduced χ²Status
Graph 2 — Line fit data ± 1σ · Gaussian + local continuum
Graph 3 — Residuals (F − M)/σ
Graph 4 — Residuals vs N(0,1)
Fit parameters (±1σ)
Rest λ—
Centre μ—
Offset Δλ / velocity—
Amplitude A—
σ—
FWHM—
FWHM (km/s)—
Flux √(2π)Aσ—
Equivalent width—
Significance F/σF—
Reduced χ²—
Window W (min–max)—
Verification — statistical checks of the selected line —
Graph 5 — Variability context of this spectrum —
 
LineThis spectrum FYear F̄(F − F̄)/F̄N (year) Fvar (year)± errRegime
Graph 6 and all lines — compare and download selected lines —
Graph 6 — Full-spectrum decomposition each selected line's Gaussian in its own colour
Campaign reference — Fvar per emission line, per year (all dated spectra)
Computed offline by run_variability.py: every spectrum in spectrum/ is fitted with this pipeline, dated from jd.xlsx, and the detected (≥3σ) fluxes of each line are grouped by calendar year. Fvar = √(σ²F − ΔF̄²) / F̄; error √(1/2N)·ΔF̄²/(F̄²Fvar) when σ²F/ΔF̄² < 10, else √(ΔF̄²/N)/F̄ (Vaughan et al. 2003; Sukanya et al. 2018). The fitted spectrum above is placed in this table in Graph 5.
Download campaign workbook (Excel: README, Fvar by year, light curves, line fits, spectra)
LineYearNJDminJD span (d) F̄ΔF̄ (rms err)σ²F/ΔF̄²Fvar± errRegime
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