J06451+2118

LAMOSTJ064508.27+211815.0  ·  Culpan knownhsd

χ²/N = 1.00

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]26258 ± 426
log g5.373 ± 0.067
log n(He)/n(H)-2.450 ± 0.114
reduced χ²1.000 over 660 points
radial velocity-63.0 km s−1
resolution (FWHM)2.50 Å
lines fitted13
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 18:27:46

Fit — Lei (TLUSTY)

Teff [K]27260 ± 260
log g5.300 ± 0.070
log n(He)/n(H)-2.520 ± 0.240
gridsLei et al. 2019, ApJ 881, 135
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

cosmic rays31 pixels cancelled
source filespec-57068-GAC101N22M1_sp05-070.fits.gz

Gaia astrometry

Gaia DR3 source3378155777335873664
parallax [mas]0.4195 ± 0.0502
G16.128
Gabs4.337
μα [mas/yr]5.021
μδ [mas/yr]-4.583
l, b193.146, 8.214

Published (Culpan et al. 2022)

class (Culpan)sdB
Teff [K]26840 ± 606
log g5.15 ± 0.06
log y-2.69 ± 0.07
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.02-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.91-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.86-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.83-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.82-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.81-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.80-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.79-13.0, 13.03.9-11.7, 11.6
Hκ3750.15-0.79-10.0, 10.03.9-7.4, 8.7
He II 46864685.70-0.98-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-0.94-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.85-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.03-15.0, 15.05.1-15.0, 15.0