J21107+0001

SDSSJ211045.16+000142.0  ·  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]40081 ± 410
log g5.699 ± 0.041
log n(He)/n(H)-2.503 ± 0.085
reduced χ²0.988 over 745 points
radial velocity11.0 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 19:10:38

Observation

cosmic rays3 pixels cancelled
source filespec-4191-55444-0700.fits

Gaia astrometry

Gaia DR3 source2689963413627537792
parallax [mas]0.1792 ± 0.0727
G17.013
μα [mas/yr]1.658
μδ [mas/yr]-7.569
l, b50.562, -30.535

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)sdO
Teff [K]36268 ± 1037
log g5.35 ± 0.15
log y-2.10 ± 0.20
reference2017OAst...26..164G

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.18-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.16-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.15-40.0, 31.64.2-43.0, 43.0
Hε3970.070.15-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.14-20.0, 26.24.0-31.8, 32.0
Hη3835.380.14-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.14-16.0, 16.03.9-15.6, 16.7
Hι3770.630.14-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.17-11.9, 11.94.9-15.0, 13.8
He II 54125411.520.20-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.17-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.15-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.16-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.15-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.18-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 40081 K · log g 5.699 · E(44−55) 0.094 · χ²r 0.15 over 31 bands

distance 5580 pc · parallax 0.1800 ± 0.0700 mas (39%) · R 0.2445 +0.1631 −0.0698 R☉ · M 1.093 +1.970 −0.542 M☉ — above the 0.47 canonical mass · L 139.3 +246.8 −68.4 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.