J18298+1114

LAMOSTJ182951.20+111441.9  ·  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]43167 ± 1101
log g6.090 ± 0.140
log n(He)/n(H)-1.884 ± 0.178
reduced χ²0.989 over 746 points
radial velocity-74.0 km s−1
resolution (FWHM)2.00 Å
lines fitted15
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:10:14

Observation

source filespec-100473-60109-27021598771503589.fits

Gaia astrometry

Gaia DR3 source4483934243439518720
parallax [mas]0.4315 ± 0.1032
G17.665
μα [mas/yr]-1.228
μδ [mas/yr]-3.864
l, b40.601, 9.846

Published (Culpan et al. 2022)

class (Culpan)sdOB
Teff [K]39240 ± 657
log g5.81 ± 0.09
log y-2.77 ± 0.26
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.20-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.07-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.01-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.98-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.96-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.95-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.94-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.93-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.16-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-1.34-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.12-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.04-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.10-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.99-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.21-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 43167 K · log g 6.090 · E(44−55) 0.076 · χ²r 20.03 over 9 bands

distance 2318 pc · parallax 0.4300 ± 0.1000 mas (23%) · R 0.0616 +0.0222 −0.0137 R☉ · M 0.171 +0.148 −0.069 M☉ — below the 0.47 canonical mass · L 11.9 +10.1 −4.7 L☉

Photometry against the model, with the residual beneath it in units of the error. The horizontal bar on each point is the passband, not an error; a hollow point was not fitted and the tooltip says why. Drag a box to zoom, double-click or Esc to come back out.