J15261+0016

SDSSJ152607.88+001640.7  ·  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]52880 ± 805
log g5.814 ± 0.063
log n(He)/n(H)-0.686 ± 0.051
reduced χ²0.975 over 745 points
radial velocity-130.0 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 19:09:23

Observation

source filespec-4012-55327-0892.fits

Gaia astrometry

Gaia DR3 source4417304530279961088
parallax [mas]0.1903 ± 0.0682
G16.819
μα [mas/yr]-8.670
μδ [mas/yr]-9.524
l, b3.561, 44.190

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO
Teff [K]62093 ± 6000
log g5.51 ± 0.20
log y-0.45 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.11-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.88-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.78-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.72-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.69-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.66-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.65-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.64-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.03-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-2.35-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.97-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.82-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.94-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.75-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.13-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 52880 K · log g 5.814 · E(44−55) 0.046 · χ²r 0.20 over 31 bands

distance 5255 pc · parallax 0.1900 ± 0.0700 mas (37%) · R 0.2004 +0.1113 −0.0526 R☉ · M 0.957 +1.381 −0.443 M☉ — above the 0.47 canonical mass · L 283.2 +401.2 −129.4 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.