J14258-0133

PG1423-013  ·  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]50560 ± 947
log g6.034 ± 0.061
log n(He)/n(H)-1.744 ± 0.060
reduced χ²0.981 over 746 points
radial velocity-38.0 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 19:09:07

Observation

source filespec-4032-55333-0926.fits

Gaia astrometry

Gaia DR3 source3652544715138169216
parallax [mas]0.3195 ± 0.0741
G16.570
μα [mas/yr]-2.862
μδ [mas/yr]1.067
l, b345.107, 53.403

Published (Culpan et al. 2022)

class (Culpan)sdO+WD?
class (SIMBAD)sdO
Teff [K]52662 ± 1000
log g5.50 ± 0.10
log y-1.61 ± 0.10
reference2007A&A...462..269S

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.62-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.55-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.52-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.50-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.49-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.49-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.48-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.48-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.59-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-0.69-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-0.58-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-0.53-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-0.57-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.51-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.62-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 50560 K · log g 6.034 · E(44−55) 0.042 · χ²r 0.16 over 35 bands

distance 3130 pc · parallax 0.3200 ± 0.0700 mas (22%) · R 0.1362 +0.0414 −0.0256 R☉ · M 0.734 +0.532 −0.258 M☉ — above the 0.47 canonical mass · L 109.4 +76.5 −37.3 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.