J13259-0323

SDSSJ132556.93-032329.6  ·  Culpan knownhsd

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]51084 ± 2116
log g6.032 ± 0.130
log n(He)/n(H)-2.617 ± 0.314
reduced χ²0.980 over 743 points
radial velocity-190.0 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 19:08:59

Observation

source filespec-108356-60469-27021598146751731.fits

Gaia astrometry

Gaia DR3 source3637042077927661056
parallax [mas]0.4347 ± 0.1447
G17.967
μα [mas/yr]-4.391
μδ [mas/yr]-8.290
l, b319.521, 58.364

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO
Teff [K]53272 ± 5000
log g5.77 ± 0.20
log y-2.23 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.08-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.75-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.60-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.52-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.46-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.43-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.41-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.39-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.97-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-3.43-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-2.88-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-2.66-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-2.83-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.55-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.12-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 51084 K · log g 6.032 · E(44−55) 0.036 · χ²r 0.32 over 10 bands

distance 2300 pc · parallax 0.4300 ± 0.1400 mas (33%) · R 0.0515 +0.0258 −0.0128 R☉ · M 0.105 +0.133 −0.046 M☉ — below the 0.47 canonical mass · L 16.3 +20.3 −7.1 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.