J09214+0246

PG0918+029  ·  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.

Results and provenance

Fit — Bamberg

Teff [K]31121 ± 300
log g5.793 ± 0.046
log n(He)/n(H)-2.364 ± 0.065
reduced χ²0.993 over 640 points
radial velocity-134.0 km s−1
resolution (FWHM)2.50 Å
lines fitted12
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 18:29:37

Fit — Lei (TLUSTY)

Teff [K]31610 ± 240
log g5.840 ± 0.040
log n(He)/n(H)-2.460 ± 0.100
gridsLei et al. 2018, ApJ 868, 70
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

source filespec-56296-VB140N02V2_sp04-108.fits.gz

Gaia astrometry

Gaia DR3 source3845583703883921920
parallax [mas]2.1042 ± 0.0484
G13.284
Gabs4.928
μα [mas/yr]-25.209
μδ [mas/yr]-20.608
l, b229.408, 34.282

Published (Culpan et al. 2022)

class (Culpan)sdB+WD
class (SIMBAD)sdB1VIIHe6
Teff [K]32369 ± 173
log g5.81 ± 0.03
log y-2.49 ± 0.03
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.17-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.94-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.83-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.77-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.74-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.71-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.70-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.69-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.09-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.00-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.80-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.20-15.0, 15.05.1-15.0, 15.0