J08280+4040

SDSSJ082802.03+404008.9  ·  Culpan knownhsd

χ²/N = 1.00

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]46086 ± 886
log g5.771 ± 0.073
log n(He)/n(H)-2.095 ± 0.106
reduced χ²1.003 over 744 points
radial velocity91.0 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 19:07:55

Observation

source filespec-3808-55513-0338.fits

Gaia astrometry

Gaia DR3 source914500864915422848
parallax [mas]0.1681 ± 0.1416
G17.915
μα [mas/yr]0.846
μδ [mas/yr]-4.770
l, b180.575, 34.983

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO
Teff [K]49800 ± 1700
log g5.36 ± 0.08
log y-1.30 ± 0.40
referenceGeierprep

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.321.48-40.0, 40.05.0-45.0, 45.0
Hγ4340.461.32-40.0, 36.84.5-43.0, 43.0
Hδ4101.731.25-40.0, 31.64.2-43.0, 43.0
Hε3970.071.21-28.0, 30.04.1-30.0, 35.0
Hζ3889.051.18-20.0, 26.24.0-31.8, 32.0
Hη3835.381.16-20.0, 14.64.0-20.7, 21.8
Hθ3797.901.15-16.0, 16.03.9-15.6, 16.7
Hι3770.631.14-13.0, 13.03.9-11.7, 11.6
He II 46864685.701.42-11.9, 11.94.9-15.0, 13.8
He II 54125411.521.64-15.0, 15.05.6-15.0, 15.0
He II 45424541.591.38-15.0, 20.04.7-20.0, 20.0
He II 42004199.841.27-23.5, 33.84.3-20.0, 20.0
He I 44724471.601.36-15.0, 15.04.6-15.0, 15.0
He I 40264026.291.22-24.2, 15.04.2-15.0, 15.0
He I 49224921.931.49-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 46086 K · log g 5.771 · E(44−55) 0.018 · χ²r 0.60 over 9 bands

distance 5949 pc · parallax 0.1700 ± 0.1400 mas (82%) · R 0.1261 +0.1862 −0.0518 R☉ · M 0.342 +1.784 −0.224 M☉ · L 64.7 +332.0 −42.3 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.