J10233+4620

SDSSJ102320.36+462026.8  ·  Culpan knownhsd

χ²/N = 1.01

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]49405 ± 1020
log g5.961 ± 0.146
log n(He)/n(H)0.448 ± 0.156
reduced χ²1.006 over 744 points
radial velocity-48.0 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 19:08:22

Observation

source filespec-6659-56607-0438.fits

Gaia astrometry

Gaia DR3 source833475855904134400
parallax [mas]0.0564 ± 0.1193
G18.108
μα [mas/yr]-1.911
μδ [mas/yr]-5.342
l, b169.574, 55.127

Published (Culpan et al. 2022)

class (Culpan)He-sdO
class (SIMBAD)sdO
Teff [K]52458 ± 5000
log g5.82 ± 0.20
log y1.71 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.78-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.69-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.66-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.64-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.62-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.61-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.61-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.60-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.75-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-0.87-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-0.73-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-0.67-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-0.72-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.64-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.79-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 49405 K · log g 5.961 · E(44−55) 0.020 · χ²r 0.18 over 9 bands

distance 17730 pc · parallax 0.0600 ± 0.1200 mas (200%) · R 0.2017 +0.4167 −0.0978 R☉ · M 1.357 +11.544 −0.997 M☉ · L 218.4 +1835.1 −160.4 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.