J00031+2412sdB

SDSSJ000307.06+241211.6  ·  00:03:07.06 24:12:11.63  ·  Culpan knownhsd

χ²/N = 0.99

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]27537 ± 225
log g5.574 ± 0.037
log n(He)/n(H)-2.677 ± 0.076
reduced χ²0.989 over 639 points
radial velocity-92.0 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 19:07:08

Fit — uli

Teff [K]27994 ± 303
log g5.477 ± 0.039
log n(He)/n(H)-2.695 ± 0.073
reduced χ²0.994 over 639 points
radial velocity-92.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
fitted04/09/2026 18:34:25

Observation

telescopeSDSS 2.5-M
survey / programmeboss
date2013-09-04
exposure6301 s in 14
pipelinev5_13_2
S/N (classifier)63.2
source filespec-6879-56539-0704.fits

Gaia astrometry

Gaia DR3 source2849938472818734720
parallax [mas]0.4415 ± 0.0627
G16.356
Gabs4.632
μα [mas/yr]3.843
μδ [mas/yr]2.689
l, b109.036, -37.361

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB

Classifier

AGREES

auto: contrast 0.15, within the 0.30 a subdwarf reaches at 28 kK, Mg I b suggests a companion but Ca II does not (0.4 sigma)

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.49-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.33-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.26-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.22-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.19-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.18-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.17-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.16-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.44-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.37-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.24-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.51-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 27537 K · log g 5.574 · E(44−55) 0.132 · χ²r 0.37 over 36 bands

distance 2265 pc · parallax 0.4400 ± 0.0600 mas (14%) · R 0.1993 +0.0332 −0.0248 R☉ · M 0.544 +0.213 −0.139 M☉ · L 20.6 +7.4 −4.9 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.