J05466+3219

LAMOSTJ054641.31+321942.1 · 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

Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Results and provenance

Fit — Bamberg

T_eff [K]	34238 ± 717
log g	6.037 ± 0.107
log n(He)/n(H)	-1.965 ± 0.148
reduced χ²	1.003 over 638 points
radial velocity	-138.0 km s⁻¹
resolution (FWHM)	2.50 Å
lines fitted	12
grids	HE-0.041.fits HE-0.125.fits HE-0.300.fits HE-0.550.fits +9 more
fitted	04/09/2026 18:27:04

Fit — Lei (TLUSTY)

T_eff [K]	33050 ± 460
log g	5.900 ± 0.130
log n(He)/n(H)	-2.050 ± 0.110
grids	Lei et al. 2019, ApJ 881, 135 SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

source file

spec-56602-GAC085N33M2_sp08-109.fits.gz

Gaia astrometry

Gaia DR3 source	3448218449263806080
parallax [mas]	0.4573 ± 0.0793
G	17.123
G_abs	5.561
μ_α [mas/yr]	-2.309
μ_δ [mas/yr]	0.505
l, b	177.221, 1.960

Published (Culpan et al. 2022)

class (Culpan)	sdB
T_eff [K]	33050 ± 460
log g	5.90 ± 0.13
log y	-2.05 ± 0.11
reference	2019ApJ...881..135L

Fitted lines

line	λ [Å]	shift [Å]	continuum at	±avg	fitted over
H_β	4861.32	-2.24	-40.0, 40.0	5.0	-45.0, 45.0
H_γ	4340.46	-2.00	-40.0, 36.8	4.5	-43.0, 43.0
H_δ	4101.73	-1.89	-40.0, 31.6	4.2	-43.0, 43.0
H_ε	3970.07	-1.83	-28.0, 30.0	4.1	-30.0, 35.0
H_ζ	3889.05	-1.79	-20.0, 26.2	4.0	-31.8, 32.0
H_η	3835.38	-1.77	-20.0, 14.6	4.0	-20.7, 21.8
H_θ	3797.90	-1.75	-16.0, 16.0	3.9	-15.6, 16.7
H_ι	3770.63	-1.74	-13.0, 13.0	3.9	-11.7, 11.6
He II 4686	4685.70	-2.16	-11.9, 11.9	4.9	-15.0, 13.8
He I 4472	4471.60	-2.06	-15.0, 15.0	4.6	-15.0, 15.0
He I 4026	4026.29	-1.85	-24.2, 15.0	4.2	-15.0, 15.0
He I 4922	4921.93	-2.27	-15.0, 15.0	5.1	-15.0, 15.0