J11242+1413

SDSSJ112415.16+141346.1  ·  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]47470 ± 724
log g6.044 ± 0.060
log n(He)/n(H)-2.204 ± 0.121
reduced χ²0.978 over 745 points
radial velocity-102.0 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 19:08:33

Observation

source filespec-5370-56003-0716.fits

Gaia astrometry

Gaia DR3 source3966702125228627200
parallax [mas]0.1833 ± 0.0933
G16.637
μα [mas/yr]2.888
μδ [mas/yr]-3.793
l, b240.964, 65.936

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdB

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.65-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.48-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.40-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.35-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.32-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.30-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.29-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.28-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.59-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-1.84-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.55-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.43-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.52-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.37-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.67-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 47470 K · log g 6.044 · E(44−55) 0.012 · χ²r 0.51 over 14 bands

distance 5456 pc · parallax 0.1800 ± 0.0900 mas (50%) · R 0.2251 +0.2048 −0.0739 R☉ · M 2.054 +5.433 −1.140 M☉ — above the 0.47 canonical mass · L 231.7 +612.1 −127.3 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.