J08449-0558

Culpan hotsd

χ²/N = 0.98

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]53475 ± 2237
log g6.155 ± 0.128
log n(He)/n(H)-2.076 ± 0.133
reduced χ²0.983 over 745 points
radial velocity-195.0 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 19:08:03

Observation

source filespec-111386-60351-63050396004585863.fits

Gaia astrometry

Gaia DR3 source5760469888980571648
parallax [mas]0.4501 ± 0.0841
G16.983
BP − RP-0.290
Gabs5.250
μα [mas/yr]-2.629
μδ [mas/yr]-5.425
RUWE1.006
l, b232.331, 21.922
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.16-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.82-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.67-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.58-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.53-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.49-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.47-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.45-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-3.05-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-3.52-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-2.95-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-2.73-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-2.91-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.62-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.20-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Component 1, the subdwarf: Teff 53475 K (held) · log g 6.155 (held) · R 0.0704 R☉ (fitted, with the companion) · χ²r 1.63 over 35 bands

E(44−55) 0.017 (held)

Component 2, the companion: Teff 4500 K (fitted, 3500–8750 K grid) · log g 4.50 (held) · R 0.4624 R☉ (fitted) · χ²r 0.09 for the two components together (Δχ² 180 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 2222 pc · parallax 0.4500 ± 0.0800 mas (18%) · M 0.466 +0.253 −0.143 M☉ · (from the ONE-star scale -- not corrected for the companion's light) · L 65.9 +33.9 −19.3 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.