J12418+1731

Feige67  ·  Culpan knownhsd

outside the grid χ²/N = 0.98

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]56212 ± 1735
log g6.064 ± 0.097
log n(He)/n(H)-1.590 ± 0.104
reduced χ²0.978 over 742 points
radial velocity-120.0 km s−1
resolution (FWHM)2.50 Å
lines fitted15
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
settledoutside the grid
fitted04/09/2026 18:30:42

Observation

source filespec-59200-HD124029N161645V01_sp09-108.fits.gz

Gaia astrometry

Gaia DR3 source3935488605023787392
parallax [mas]2.9149 ± 0.0735
G11.755
Gabs4.128
μα [mas/yr]-7.170
μδ [mas/yr]-37.278
l, b289.479, 80.143

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdOpec
Teff [K]61114 ± 318
log g5.92 ± 0.01
log y-1.59 ± 0.04
reference2018A&A...609A..89L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.95-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.74-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.64-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.59-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.56-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.54-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.52-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.51-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.88-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-2.17-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.82-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.68-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.79-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.61-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.97-15.0, 15.05.1-15.0, 15.0