J12476+1152sdO

LBQS1245+1208 · 12:47:38.71 11:52:34.10 · 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]	43172 ± 1156
log g	5.739 ± 0.117
log n(He)/n(H)	-2.788 ± 0.374
reduced χ²	1.001 over 746 points
radial velocity	-72.0 km s⁻¹
resolution (FWHM)	2.00 Å
lines fitted	15
grids	HE-0.041.fits HE-0.125.fits HE-0.300.fits HE-0.550.fits +9 more
fitted	04/09/2026 19:08:50

Observation

telescope	SDSS 2.5-M
survey / programme	boss
date	2012-02-24
exposure	5405 s in 12
pipeline	v5_13_2
S/N (classifier)	25.2
source file	spec-5412-55981-0466.fits

Gaia astrometry

Gaia DR3 source	3928015048395839616
parallax [mas]	-0.1180 ± 0.1845
G	18.499
μ_α [mas/yr]	-2.064
μ_δ [mas/yr]	-4.373
l, b	299.408, 74.722

Published (Culpan et al. 2022)

class (Culpan)	sdO
class (SIMBAD)	sdOB

Classifier

AGREES

auto: He II/He I 4.5, EW 0.68, Ca II 8662/8542 = 15.8 -- the star's own Paschen lines, not a companion

Fitted lines

line	λ [Å]	shift [Å]	continuum at	±avg	fitted over
H_β	4861.32	-1.17	-40.0, 40.0	5.0	-45.0, 45.0
H_γ	4340.46	-1.04	-40.0, 36.8	4.5	-43.0, 43.0
H_δ	4101.73	-0.99	-40.0, 31.6	4.2	-43.0, 43.0
H_ε	3970.07	-0.95	-28.0, 30.0	4.1	-30.0, 35.0
H_ζ	3889.05	-0.93	-20.0, 26.2	4.0	-31.8, 32.0
H_η	3835.38	-0.92	-20.0, 14.6	4.0	-20.7, 21.8
H_θ	3797.90	-0.91	-16.0, 16.0	3.9	-15.6, 16.7
H_ι	3770.63	-0.91	-13.0, 13.0	3.9	-11.7, 11.6
He II 4686	4685.70	-1.13	-11.9, 11.9	4.9	-15.0, 13.8
He II 5412	5411.52	-1.30	-15.0, 15.0	5.6	-15.0, 15.0
He II 4542	4541.59	-1.09	-15.0, 20.0	4.7	-20.0, 20.0
He II 4200	4199.84	-1.01	-23.5, 33.8	4.3	-20.0, 20.0
He I 4472	4471.60	-1.07	-15.0, 15.0	4.6	-15.0, 15.0
He I 4026	4026.29	-0.97	-24.2, 15.0	4.2	-15.0, 15.0
He I 4922	4921.93	-1.18	-15.0, 15.0	5.1	-15.0, 15.0