J06475+1350

LAMOSTJ064734.86+135011.3  ·  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]32158 ± 500
log g5.896 ± 0.070
log n(He)/n(H)-2.116 ± 0.125
reduced χ²0.986 over 638 points
radial velocity-137.0 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 18:27:48

Fit — Lei (TLUSTY)

Teff [K]31770 ± 220
log g6.060 ± 0.040
log n(He)/n(H)-2.460 ± 0.180
gridsLei et al. 2019, ApJ 881, 135
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

cosmic rays11 pixels cancelled
source filespec-57367-GAC100N13M1_sp09-030.fits.gz

Gaia astrometry

Gaia DR3 source3352835983053282304
parallax [mas]0.5479 ± 0.0666
G16.796
Gabs5.521
μα [mas/yr]1.949
μδ [mas/yr]-3.672
l, b200.148, 5.423

Published (Culpan et al. 2022)

class (Culpan)sdB
Teff [K]33246 ± 169
log g6.03 ± 0.03
log y-2.37 ± 0.06
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.22-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.98-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.87-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.81-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.78-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.75-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.74-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.72-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.14-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.04-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.84-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.25-15.0, 15.05.1-15.0, 15.0