J14520+4533

SDSSJ145203.94+453329.6  ·  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]46831 ± 659
log g6.111 ± 0.059
log n(He)/n(H)-1.977 ± 0.102
reduced χ²0.994 over 744 points
radial velocity126.0 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 19:09:17

Observation

source filespec-6737-56365-0380.fits

Gaia astrometry

Gaia DR3 source1586890398971315200
parallax [mas]0.2860 ± 0.0701
G17.194
μα [mas/yr]-5.680
μδ [mas/yr]-0.821
l, b78.545, 59.811

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO
Teff [K]49358 ± 5000
log g5.56 ± 0.20
log y-2.01 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.322.04-40.0, 40.05.0-45.0, 45.0
Hγ4340.461.82-40.0, 36.84.5-43.0, 43.0
Hδ4101.731.72-40.0, 31.64.2-43.0, 43.0
Hε3970.071.67-28.0, 30.04.1-30.0, 35.0
Hζ3889.051.63-20.0, 26.24.0-31.8, 32.0
Hη3835.381.61-20.0, 14.64.0-20.7, 21.8
Hθ3797.901.60-16.0, 16.03.9-15.6, 16.7
Hι3770.631.58-13.0, 13.03.9-11.7, 11.6
He II 46864685.701.97-11.9, 11.94.9-15.0, 13.8
He II 54125411.522.27-15.0, 15.05.6-15.0, 15.0
He II 45424541.591.91-15.0, 20.04.7-20.0, 20.0
He II 42004199.841.77-23.5, 33.84.3-20.0, 20.0
He I 44724471.601.88-15.0, 15.04.6-15.0, 15.0
He I 40264026.291.69-24.2, 15.04.2-15.0, 15.0
He I 49224921.932.07-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 46831 K · log g 6.111 · E(44−55) 0.026 · χ²r 0.18 over 26 bands

distance 3496 pc · parallax 0.2900 ± 0.0700 mas (24%) · R 0.1166 +0.0381 −0.0229 R☉ · M 0.642 +0.506 −0.234 M☉ · L 59.0 +44.9 −21.0 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.