J16147+0821

SDSSJ161442.26+082145.2  ·  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]51202 ± 1082
log g6.073 ± 0.070
log n(He)/n(H)-2.178 ± 0.107
reduced χ²1.003 over 747 points
radial velocity-28.0 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 19:09:38

Observation

source filespec-4896-55712-0628.fits

Gaia astrometry

Gaia DR3 source4452174369027959168
parallax [mas]0.1538 ± 0.0751
G17.042
μα [mas/yr]-2.830
μδ [mas/yr]-1.252
l, b21.463, 38.509

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)DAO/sdO
Teff [K]53470 ± 5000
log g5.37 ± 0.20
log y-1.72 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.45-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.41-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.38-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.37-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.36-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.36-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.35-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.35-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.44-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-0.51-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-0.42-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-0.39-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-0.42-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.38-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.46-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 51202 K · log g 6.073 · E(44−55) 0.170 · χ²r 1.59 over 25 bands

distance 6502 pc · parallax 0.1500 ± 0.0800 mas (53%) · R 0.2675 +0.2311 −0.0859 R☉ · M 3.087 +7.665 −1.676 M☉ — above the 0.47 canonical mass · L 443.1 +1093.6 −239.0 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.