J11372+1208sdOB

SDSSJ113715.31+120810.0  ·  11:37:15.31 12:08:09.85  ·  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.

Line-profile fit — uli

profile fit on the uli grid
Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Results and provenance

Fit — Bamberg

Teff [K]33980 ± 224
log g5.940 ± 0.027
log n(He)/n(H)-1.240 ± 0.037
reduced χ²0.973 over 636 points
radial velocity-186.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:08:37

Fit — uli

Teff [K]34026 ± 149
log g5.926 ± 0.027
log n(He)/n(H)-1.275 ± 0.041
reduced χ²0.972 over 636 points
radial velocity-186.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
fitted04/09/2026 18:35:35

Observation

telescopeSDSS 2.5-M
survey / programmeboss
date2012-02-29
exposure3603 s in 8
pipelinev5_13_2
S/N (classifier)52.7
source filespec-5379-55986-0522.fits

Gaia astrometry

Gaia DR3 source3917573295704299904
parallax [mas]0.4364 ± 0.0650
G16.128
Gabs4.356
μα [mas/yr]2.873
μδ [mas/yr]4.944
l, b250.075, 67.040

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)DA4

Classifier

DISPUTED

auto: He II 0.57 (4.4 sigma), Mg I b suggests a companion but Ca II does not (-0.1 sigma)

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.02-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.69-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.54-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.46-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.41-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.38-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.36-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.34-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.91-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.77-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.50-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.05-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 33980 K · log g 5.940 · E(44−55) 0.016 · χ²r 0.32 over 36 bands

distance 2291 pc · parallax 0.4400 ± 0.0700 mas (16%) · R 0.1554 +0.0274 −0.0201 R☉ · M 0.770 +0.316 −0.202 M☉ — above the 0.47 canonical mass · L 29.1 +11.1 −7.1 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.