J14294+1921

PG1427+195  ·  Culpan knownhsd

χ²/N = 0.97

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]49586 ± 1182
log g5.945 ± 0.171
log n(He)/n(H)0.393 ± 0.129
reduced χ²0.972 over 737 points
radial velocity-11.0 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 19:09:09

Observation

cosmic rays3 pixels cancelled
source filespec-101677-60690-63050394841407786.fits

Gaia astrometry

Gaia DR3 source1239364769480858496
parallax [mas]0.7062 ± 0.0408
G14.072
Gabs3.359
μα [mas/yr]-2.830
μδ [mas/yr]-5.267
l, b19.092, 66.232

Published (Culpan et al. 2022)

class (Culpan)He-sdO
class (SIMBAD)sdOC
Teff [K]54412 ± 503
log g5.68 ± 0.04
log y1.58 ± 0.24
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.18-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.16-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.15-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.15-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.14-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.14-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.14-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.14-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.17-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-0.20-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-0.17-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-0.15-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-0.16-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.15-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.18-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 49586 K · log g 5.945 · E(44−55) 0.018 · χ²r 0.27 over 41 bands

distance 1416 pc · parallax 0.7100 ± 0.0400 mas (6%) · R 0.1920 +0.0120 −0.0106 R☉ · M 1.188 +0.215 −0.180 M☉ — above the 0.47 canonical mass · L 201.0 +26.0 −21.9 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.