J11428+1115

SDSSJ114251.76+111507.9  ·  Culpan knownhsd

χ²/N = 1.02

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]54378 ± 2890
log g6.135 ± 0.163
log n(He)/n(H)-1.629 ± 0.208
reduced χ²1.019 over 744 points
radial velocity-180.0 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 19:08:40

Observation

cosmic rays6 pixels cancelled
source filespec-5379-55986-0141.fits

Gaia astrometry

Gaia DR3 source3916474436911989120
parallax [mas]0.1637 ± 0.2723
G18.731
μα [mas/yr]-3.666
μδ [mas/yr]-5.534
l, b254.199, 67.379

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.92-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.61-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.46-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.38-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.34-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.30-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.28-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.26-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.81-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-3.25-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-2.73-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-2.52-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-2.68-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.42-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.96-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 54378 K · log g 6.135 · E(44−55) 0.032 · χ²r 1.46 over 10 bands

distance 6109 pc · parallax 0.1600 ± 0.2700 mas (169%) · R 0.0583 +0.1144 −0.0275 R☉ · M 0.170 +1.320 −0.123 M☉ · L 26.7 +208.6 −19.3 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.