J15410+3638

SDSSJ154100.52+363840.9  ·  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]40994 ± 670
log g5.395 ± 0.068
log n(He)/n(H)-2.405 ± 0.138
reduced χ²0.991 over 744 points
radial velocity165.0 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 19:09:29

Observation

source filespec-4974-56038-0870.fits

Gaia astrometry

Gaia DR3 source1374648744586858624
parallax [mas]0.0736 ± 0.0808
G17.700
μα [mas/yr]1.765
μδ [mas/yr]-0.919
l, b58.687, 53.086

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)sdO

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.322.68-40.0, 40.05.0-45.0, 45.0
Hγ4340.462.39-40.0, 36.84.5-43.0, 43.0
Hδ4101.732.26-40.0, 31.64.2-43.0, 43.0
Hε3970.072.19-28.0, 30.04.1-30.0, 35.0
Hζ3889.052.14-20.0, 26.24.0-31.8, 32.0
Hη3835.382.11-20.0, 14.64.0-20.7, 21.8
Hθ3797.902.09-16.0, 16.03.9-15.6, 16.7
Hι3770.632.08-13.0, 13.03.9-11.7, 11.6
He II 46864685.702.58-11.9, 11.94.9-15.0, 13.8
He II 54125411.522.98-15.0, 15.05.6-15.0, 15.0
He II 45424541.592.50-15.0, 20.04.7-20.0, 20.0
He II 42004199.842.31-23.5, 33.84.3-20.0, 20.0
He I 44724471.602.46-15.0, 15.04.6-15.0, 15.0
He I 40264026.292.22-24.2, 15.04.2-15.0, 15.0
He I 49224921.932.71-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 40994 K · log g 5.395 · E(44−55) 0.042 · χ²r 0.17 over 9 bands

distance 13587 pc · parallax 0.0700 ± 0.0800 mas (114%) · R 0.3171 +0.5420 −0.1397 R☉ · M 0.913 +5.781 −0.629 M☉ · L 256.2 +1623.7 −175.9 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.