J22111+5138

LAMOSTJ221106.31+513832.4  ·  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]37149 ± 1086
log g5.326 ± 0.105
log n(He)/n(H)-2.671 ± 0.336
reduced χ²0.985 over 635 points
radial velocity-10.0 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 18:33:49

Fit — Lei (TLUSTY)

Teff [K]33090 ± 780
log g5.400 ± 0.080
log n(He)/n(H)-2.690 ± 0.240
gridsLei et al. 2019, ApJ 881, 135
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

cosmic rays2 pixels cancelled
source filespec-57675-HD220327N493953B01_sp12-047.fits.gz

Gaia astrometry

Gaia DR3 source2004114070560436736
parallax [mas]0.4539 ± 0.0294
G15.182
Gabs3.528
μα [mas/yr]-6.060
μδ [mas/yr]-4.934
l, b99.327, -3.727

Published (Culpan et al. 2022)

class (Culpan)sdB
Teff [K]33090 ± 780
log g5.40 ± 0.08
log y-2.69 ± 0.24
reference2019ApJ...881..135L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.16-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.14-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.14-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.13-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.13-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.13-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.13-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.13-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.16-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-0.15-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.13-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.16-15.0, 15.05.1-15.0, 15.0