J07334+3652sdB

SDSSJ073325.61+365257.6  ·  07:33:25.61 36:52:57.68  ·  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]31760 ± 134
log g6.072 ± 0.018
log n(He)/n(H)-2.477 ± 0.042
reduced χ²0.977 over 637 points
radial velocity-110.0 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 19:07:36

Fit — uli

Teff [K]30528 ± 38
log g6.008 ± 0.019
log n(He)/n(H)-2.486 ± 0.047
reduced χ²0.977 over 637 points
radial velocity-110.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
settledoutside the grid
fitted04/09/2026 18:34:48

Observation

telescopeSDSS 2.5-M
survey / programmeMWM / MWM2
field · MJD015190 · 59248
date2021-02-02
catalogid4553825496
exposure8101 s in 9
airmass1.07
seeing (50%)1.25″
E(B−V)0.031
pipelinev6_2_1
S/N (classifier)91.4
source filespec-015190-59248-4553825496.fits

Gaia astrometry

Gaia DR3 source898625493262383104
parallax [mas]1.1941 ± 0.0402
G15.078
BP − RP-0.415
Gabs5.502
μα [mas/yr]-0.321
μδ [mas/yr]-0.911
l, b182.193, 23.789

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB
Teff [K]32972 ± 106
log g5.92 ± 0.02
log y-2.68 ± 0.05
reference2021ApJS..256...28L

Classifier

AGREES

fitted Teff 32972 logg 5.92 logY -2.68 2021ApJS..256...28L

auto: contrast 0.05, within the 0.28 a subdwarf reaches at 29 kK, Mg I b suggests a companion but Ca II does not (-1.2 sigma)

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.78-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.59-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.51-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.46-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.43-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.41-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.39-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.38-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.72-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.64-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.48-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.81-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 31760 K · log g 6.072 · E(44−55) 0.060 · χ²r 0.20 over 40 bands

distance 837 pc · parallax 1.1900 ± 0.0400 mas (3%) · R 0.1045 +0.0039 −0.0036 R☉ · M 0.470 +0.068 −0.059 M☉ · L 10.0 +0.8 −0.7 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.