J11047+0925

PG1102+097  ·  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]38387 ± 280
log g5.345 ± 0.028
log n(He)/n(H)-2.343 ± 0.089
reduced χ²0.986 over 744 points
radial velocity-244.0 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 19:08:29

Observation

source filespec-5361-55973-0338.fits

Gaia astrometry

Gaia DR3 source3867259957150344960
parallax [mas]0.0766 ± 0.0672
G16.266
μα [mas/yr]-5.603
μδ [mas/yr]-6.904
l, b242.986, 59.229

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)sdO
Teff [K]37446 ± 2000
log g5.01 ± 0.20
log y-2.10 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.96-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-3.53-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-3.34-40.0, 31.64.2-43.0, 43.0
Hε3970.07-3.23-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-3.17-20.0, 26.24.0-31.8, 32.0
Hη3835.38-3.12-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-3.09-16.0, 16.03.9-15.6, 16.7
Hι3770.63-3.07-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-3.81-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-4.40-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-3.70-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-3.42-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-3.64-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-3.28-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-4.01-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 38387 K · log g 5.345 · E(44−55) 0.034 · χ²r 0.82 over 37 bands

distance 13055 pc · parallax 0.0800 ± 0.0700 mas (88%) · R 0.6726 +1.0256 −0.2800 R☉ · M 3.640 +19.705 −2.403 M☉ — above the 0.47 canonical mass · L 884.8 +4752.4 −583.4 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.