J23374+0646

SDSSJJ233725.49+064603.0  ·  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]51077 ± 1484
log g5.957 ± 0.161
log n(He)/n(H)0.392 ± 0.149
reduced χ²0.988 over 747 points
radial velocity7.0 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 19:11:06

Observation

source filespec-4407-55884-0904.fits

Gaia astrometry

Gaia DR3 source2756737648135244416
parallax [mas]0.3032 ± 0.1869
G18.391
μα [mas/yr]4.850
μδ [mas/yr]-1.968
l, b92.397, -51.662

Published (Culpan et al. 2022)

class (Culpan)He-sdO
class (SIMBAD)sdOHe

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.11-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.10-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.10-40.0, 31.64.2-43.0, 43.0
Hε3970.070.09-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.09-20.0, 26.24.0-31.8, 32.0
Hη3835.380.09-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.09-16.0, 16.03.9-15.6, 16.7
Hι3770.630.09-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.11-11.9, 11.94.9-15.0, 13.8
He II 54125411.520.13-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.11-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.10-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.10-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.09-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.11-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 51077 K · log g 5.957 · E(44−55) 0.114 · χ²r 1.12 over 13 bands

distance 3298 pc · parallax 0.3000 ± 0.1900 mas (63%) · R 0.0660 +0.0742 −0.0239 R☉ · M 0.144 +0.510 −0.086 M☉ · L 26.7 +93.7 −15.8 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.