J08080+1208sdB

SDSSJ080801.40+120826.9  ·  08:08:01.42 12:08:27.10  ·  Culpan knownhsd

χ²/N = 1.00

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]36068 ± 254
log g5.996 ± 0.031
log n(He)/n(H)-1.859 ± 0.057
reduced χ²0.998 over 639 points
radial velocity-176.0 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 19:07:48

Fit — uli

Teff [K]33640 ± 327
log g5.975 ± 0.029
log n(He)/n(H)-1.861 ± 0.040
reduced χ²1.002 over 639 points
radial velocity-176.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
fitted04/09/2026 18:34:55

Observation

telescopeSDSS 2.5-M
survey / programmeboss
date2011-02-11
exposure7207 s in 16
pipelinev5_13_2
S/N (classifier)72.9
source filespec-4505-55603-0168.fits

Gaia astrometry

Gaia DR3 source649989153600135680
parallax [mas]0.5030 ± 0.0680
G16.288
Gabs4.819
μα [mas/yr]-0.332
μδ [mas/yr]-5.745
l, b210.392, 22.413

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)DAO/sdO

Classifier

DISPUTED

auto: contrast 0.04, within the 0.25 a subdwarf reaches at 32 kK

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.85-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.55-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.41-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.33-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.28-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.25-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.23-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.21-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.75-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.63-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.36-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.89-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 36068 K · log g 5.996 · E(44−55) 0.038 · χ²r 0.12 over 34 bands

distance 1988 pc · parallax 0.5000 ± 0.0700 mas (14%) · R 0.1228 +0.0193 −0.0147 R☉ · M 0.546 +0.203 −0.135 M☉ · L 23.0 +7.8 −5.2 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.