J17132+4041

SDSSJ171314.08+404108.9  ·  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]52380 ± 1805
log g5.731 ± 0.158
log n(He)/n(H)-0.529 ± 0.121
reduced χ²0.985 over 748 points
radial velocity102.0 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 19:09:54

Observation

source filespec-4984-55827-0792.fits

Gaia astrometry

Gaia DR3 source1341909823796956672
parallax [mas]0.1242 ± 0.1004
G18.186
μα [mas/yr]-3.880
μδ [mas/yr]-1.419
l, b65.261, 35.287

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdOHe
Teff [K]41926 ± 2000
log g5.42 ± 0.20
log y-0.04 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.321.65-40.0, 40.05.0-45.0, 45.0
Hγ4340.461.48-40.0, 36.84.5-43.0, 43.0
Hδ4101.731.40-40.0, 31.64.2-43.0, 43.0
Hε3970.071.35-28.0, 30.04.1-30.0, 35.0
Hζ3889.051.32-20.0, 26.24.0-31.8, 32.0
Hη3835.381.30-20.0, 14.64.0-20.7, 21.8
Hθ3797.901.29-16.0, 16.03.9-15.6, 16.7
Hι3770.631.28-13.0, 13.03.9-11.7, 11.6
He II 46864685.701.59-11.9, 11.94.9-15.0, 13.8
He II 54125411.521.84-15.0, 15.05.6-15.0, 15.0
He II 45424541.591.55-15.0, 20.04.7-20.0, 20.0
He II 42004199.841.43-23.5, 33.84.3-20.0, 20.0
He I 44724471.601.52-15.0, 15.04.6-15.0, 15.0
He I 40264026.291.37-24.2, 15.04.2-15.0, 15.0
He I 49224921.931.67-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 52380 K · log g 5.731 · E(44−55) 0.062 · χ²r 0.63 over 10 bands

distance 8052 pc · parallax 0.1200 ± 0.1000 mas (83%) · R 0.1515 +0.2179 −0.0614 R☉ · M 0.451 +2.260 −0.293 M☉ · L 156.0 +768.5 −101.0 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.