J11146-0040

SDSSJ111438.57-004024.3  ·  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]53634 ± 1530
log g5.865 ± 0.103
log n(He)/n(H)-0.948 ± 0.086
reduced χ²0.975 over 742 points
radial velocity-187.0 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 19:08:30

Observation

source filespec-3788-55246-0828.fits

Gaia astrometry

Gaia DR3 source3791923099746830848
parallax [mas]0.1516 ± 0.2368
G18.367
μα [mas/yr]-3.907
μδ [mas/yr]-5.865
l, b259.060, 53.743

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO
Teff [K]56722 ± 6000
log g5.56 ± 0.20
log y-0.90 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.03-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.71-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.56-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.48-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.43-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.39-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.37-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.35-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.92-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-3.38-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-2.83-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-2.62-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-2.79-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.51-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.07-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 53634 K · log g 5.865 · E(44−55) 0.074 · χ²r 0.57 over 13 bands

distance 6596 pc · parallax 0.1500 ± 0.2400 mas (160%) · R 0.0832 +0.1600 −0.0390 R☉ · M 0.185 +1.400 −0.133 M☉ · L 51.6 +388.0 −37.0 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.