J10370-0244

SDSSJ103702.56-024443.2  ·  Culpan knownhsd

χ²/N = 0.99

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]26515 ± 215
log g5.357 ± 0.033
log n(He)/n(H)-2.888 ± 0.111
reduced χ²0.988 over 637 points
radial velocity-81.0 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 19:08:24

Fit — uli

Teff [K]26542 ± 280
log g5.231 ± 0.036
log n(He)/n(H)-2.867 ± 0.085
reduced χ²0.988 over 637 points
radial velocity-81.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh909.grid
h97.grid
h99.grid
h999.grid
fitted04/09/2026 18:35:25

Observation

source filespec-3771-55544-0416.fits

Gaia astrometry

Gaia DR3 source3781404660414879104
parallax [mas]0.3120 ± 0.0640
G16.331
Gabs3.894
μα [mas/yr]-5.676
μδ [mas/yr]-2.791
l, b250.292, 45.940

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.31-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.17-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.11-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.07-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.05-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.04-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.03-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.02-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.27-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.21-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.09-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.33-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Component 1, the subdwarf: Teff 26515 K (held) · log g 5.357 (held) · R 0.2475 R☉ (fitted, with the companion) · χ²r 2.06 over 36 bands

E(44−55) 0.040 (held)

Component 2, the companion: Teff 5000 K (fitted, 3500–8750 K grid) · log g 4.50 (held) · R 0.6306 R☉ (fitted) · χ²r 0.37 for the two components together (Δχ² 248 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 3205 pc · parallax 0.3100 ± 0.0600 mas (19%) · M 0.817 +0.501 −0.266 M☉ — above the 0.47 canonical mass · (from the ONE-star scale -- not corrected for the companion's light) · L 43.8 +25.7 −13.8 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.