J11375+4600

PG1134+463  ·  Culpan knownhsd

χ²/N = 0.96

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]50016 ± 924
log g6.189 ± 0.126
log n(He)/n(H)0.304 ± 0.089
reduced χ²0.957 over 744 points
radial velocity59.0 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 19:08:39

Observation

cosmic rays11 pixels cancelled
source filespec-100423-60065-27021597919315064.fits

Gaia astrometry

Gaia DR3 source785980977968930560
parallax [mas]0.5154 ± 0.0486
G15.148
Gabs3.747
μα [mas/yr]-11.799
μδ [mas/yr]-7.907
l, b155.874, 66.114

Published (Culpan et al. 2022)

class (Culpan)He-sdO
class (SIMBAD)sdO
Teff [K]48889 ± 5000
log g5.69 ± 0.20
log y1.09 ± 0.40
reference2009PhDT.......273H

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.96-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.85-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.81-40.0, 31.64.2-43.0, 43.0
Hε3970.070.78-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.77-20.0, 26.24.0-31.8, 32.0
Hη3835.380.75-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.75-16.0, 16.03.9-15.6, 16.7
Hι3770.630.74-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.92-11.9, 11.94.9-15.0, 13.8
He II 54125411.521.07-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.89-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.83-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.88-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.79-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.97-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 50016 K · log g 6.189 · E(44−55) 0.036 · χ²r 0.46 over 39 bands

distance 1940 pc · parallax 0.5200 ± 0.0500 mas (10%) · R 0.1638 +0.0172 −0.0142 R☉ · M 1.515 +0.396 −0.296 M☉ — above the 0.47 canonical mass · L 151.5 +33.4 −25.4 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.