J03383-5758

Culpan hotsd

χ²/N = 1.01

Spectrum

shaded: the intervals the fit used ·  │ a cancelled pixeldrag on either panel to zoom · dbl-click or Esc to reset · arrows to pan

The whole reduced spectrum above, the region marked on it below. Shaded bands are the intervals the fit used; a tick under the axis marks a pixel the rejection mask cancelled.

Line-profile fit — Bamberg

profile fit on the Bamberg grid
Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Results and provenance

Fit — Bamberg

Teff [K]50429 ± 2131
log g6.126 ± 0.144
log n(He)/n(H)-2.140 ± 0.196
reduced χ²1.009 over 745 points
radial velocity-198.0 km s−1
resolution (FWHM)2.00 Å
lines fitted15
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:07:28

Observation

source filespec-110095-60285-63050395801109703.fits

Gaia astrometry

Gaia DR3 source4729626958543290368
parallax [mas]0.3950 ± 0.0375
G16.335
BP − RP-0.351
Gabs4.317
μα [mas/yr]15.304
μδ [mas/yr]5.600
RUWE1.004
l, b271.342, -47.625
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.21-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.87-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.71-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.62-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.57-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.53-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.51-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.49-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-3.09-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-3.57-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-3.00-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-2.77-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-2.95-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.66-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.25-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Component 1, the subdwarf: Teff 50429 K (held) · log g 6.126 (held) · R 0.1193 R☉ (fitted, with the companion) · χ²r 0.99 over 37 bands

E(44−55) 0.039 (held)

Component 2, the companion: Teff 4625 K (fitted, 3500–8750 K grid) · log g 4.50 (held) · R 0.4615 R☉ (fitted) · χ²r 0.13 for the two components together (Δχ² 127 over one star, same bands)

The dashed curves beneath the model are the two components of this fit: the subdwarf alone and the cool companion.

distance 2532 pc · parallax 0.4000 ± 0.0400 mas (10%) · M 0.918 +0.242 −0.181 M☉ — above the 0.47 canonical mass · (from the ONE-star scale -- not corrected for the companion's light) · L 109.7 +24.5 −18.5 L☉

Photometry against the model, with the residual beneath it in units of the error. The horizontal bar on each point is the passband, not an error; a hollow point was not fitted and the tooltip says why. Drag a box to zoom, double-click or Esc to come back out.