J22408+5437

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.

Line-profile fit — uli

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

Results and provenance

Fit — Bamberg

Teff [K]38808 ± 509
log g5.535 ± 0.069
log n(He)/n(H)-1.309 ± 0.075
reduced χ²0.977 over 638 points
radial velocity-247.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:10:56

Fit — uli

Teff [K]36290 ± 331
log g5.349 ± 0.070
log n(He)/n(H)-1.267 ± 0.070
reduced χ²0.990 over 638 points
radial velocity-247.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
fitted04/09/2026 18:37:32

Observation

source filespec-100601-60310-63050394943960848.fits

Gaia astrometry

Gaia DR3 source2003241230122936064
parallax [mas]0.7010 ± 0.0229
G14.980
BP − RP0.011
Gabs4.208
μα [mas/yr]-1.087
μδ [mas/yr]2.028
RUWE0.950
l, b104.700, -3.552
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-4.01-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-3.58-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-3.38-40.0, 31.64.2-43.0, 43.0
Hε3970.07-3.27-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-3.20-20.0, 26.24.0-31.8, 32.0
Hη3835.38-3.16-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-3.13-16.0, 16.03.9-15.6, 16.7
Hι3770.63-3.11-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-3.86-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-3.68-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-3.32-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-4.06-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Component 1, the subdwarf: Teff 38808 K (held) · log g 5.535 (held) · R 0.2185 R☉ (fitted, with the companion) · χ²r 1.80 over 32 bands

E(44−55) 0.302 (held)

Component 2, the companion: Teff 4250 K (fitted, 3500–8750 K grid) · log g 4.50 (held) · R 0.5454 R☉ (fitted) · χ²r 0.65 for the two components together (Δχ² 69 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 1427 pc · parallax 0.7000 ± 0.0200 mas (3%) · M 0.756 +0.113 −0.098 M☉ — above the 0.47 canonical mass · (from the ONE-star scale -- not corrected for the companion's light) · L 123.6 +10.6 −9.6 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.