J07010+0941

LAMOSTJ070102.95+094135.6  ·  Culpan knownhsd

χ²/N = 0.96

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]23696 ± 674
log g5.578 ± 0.089
log n(He)/n(H)-3.610 ± 0.272
reduced χ²0.965 over 656 points
radial velocity-185.0 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 18:27:59

Fit — Lei (TLUSTY)

Teff [K]23300 ± 610
log g5.560 ± 0.050
log n(He)/n(H)-3.350 ± 0.300
gridsLei et al. 2019, ApJ 881, 135
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

source filespec-57757-GAC107N09M1_sp14-235.fits.gz

Gaia astrometry

Gaia DR3 source3157919887443293952
parallax [mas]0.5455 ± 0.0788
G17.018
Gabs5.726
μα [mas/yr]-3.204
μδ [mas/yr]-3.761
l, b205.355, 6.520

Published (Culpan et al. 2022)

class (Culpan)sdB
Teff [K]25017 ± 402
log g5.65 ± 0.05
log y-3.70 ± 0.19
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.00-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.68-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.53-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.45-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.40-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.37-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.34-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.33-13.0, 13.03.9-11.7, 11.6
Hκ3750.15-2.31-10.0, 10.03.9-7.4, 8.7
He II 46864685.70-2.89-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.76-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.48-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.04-15.0, 15.05.1-15.0, 15.0