J08434+0824sdB

SDSSJ084328.87+082438.2  ·  08:43:28.87 08:24:38.38  ·  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.

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]23982 ± 190
log g5.630 ± 0.023
log n(He)/n(H)-3.970 ± 0.331
reduced χ²0.983 over 659 points
radial velocity-59.0 km s−1
resolution (FWHM)2.00 Å
lines fitted13
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:08:00

Fit — uli

Teff [K]23851 ± 217
log g5.532 ± 0.025
log n(He)/n(H)-3.317 ± 0.060 upper limit
reduced χ²0.984 over 659 points
radial velocity-59.0 km s−1
resolution (FWHM)2.00 Å
lines fitted13
gridsh909.grid
h97.grid
h99.grid
h999.grid
settledoutside the grid
fitted04/09/2026 18:35:03

Observation

telescopeSDSS 2.5-M
survey / programmeboss
date2011-11-28
exposure7207 s in 16
pipelinev5_13_2
S/N (classifier)69.1
source filespec-5289-55893-0570.fits

Gaia astrometry

Gaia DR3 source597102541222525056
parallax [mas]0.5130 ± 0.0612
G16.422
Gabs5.008
μα [mas/yr]4.866
μδ [mas/yr]-9.668
l, b218.274, 28.697

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)DAZ
Teff [K]26928 ± 350
log g5.77 ± 0.04
log y-3.70 ± 0.15
reference2021ApJS..256...28L

Classifier

AGREES

fitted Teff 26928 logg 5.77 logY -3.7 2021ApJS..256...28L

auto: contrast 0.15, within the 0.35 a subdwarf reaches at 24 kK, Ca II 8662/8542 = 6.7 -- the star's own Paschen lines, not a companion

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.96-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.85-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.81-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.78-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.77-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.75-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.75-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.74-13.0, 13.03.9-11.7, 11.6
Hκ3750.15-0.74-10.0, 10.03.9-7.4, 8.7
He II 46864685.70-0.92-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-0.88-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.79-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.97-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 23982 K · log g 5.630 · E(44−55) 0.038 · χ²r 0.15 over 41 bands

distance 1949 pc · parallax 0.5100 ± 0.0600 mas (12%) · R 0.1666 +0.0227 −0.0177 R☉ · M 0.432 +0.141 −0.098 M☉ · L 8.3 +2.4 −1.7 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.