J21271+0011sdB

GALEXJ21271+0011  ·  21:27:11.50 00:11:45.92  ·  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]28079 ± 125
log g5.568 ± 0.020
log n(He)/n(H)-2.976 ± 0.078
reduced χ²0.980 over 638 points
radial velocity-102.0 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 19:10:41

Fit — uli

Teff [K]28667 ± 146
log g5.481 ± 0.020
log n(He)/n(H)-2.957 ± 0.051
reduced χ²0.982 over 638 points
radial velocity-102.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
fitted04/09/2026 18:37:21

Observation

telescopeSDSS 2.5-M
survey / programmeMWM / mwm_cb
field · MJD104646 · 60605
date2024-10-21
catalogid63050395070733594
exposure4500 s in 5
airmass1.21
seeing (50%)1.67″
E(B−V)0.048
pipelinev6_2_1
S/N (classifier)62.0
source filespec-104646-60605-63050395070733594.fits

Gaia astrometry

Gaia DR3 source2687870218366060416
parallax [mas]0.9076 ± 0.0376
G14.550
BP − RP-0.379
Gabs4.391
μα [mas/yr]-0.254
μδ [mas/yr]-2.904
l, b53.355, -33.902

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB
Teff [K]30082 ± 106
log g5.54 ± 0.02
log y-3.07 ± 0.05
reference2021ApJS..256...28L

Classifier

AGREES

fitted Teff 30082 logg 5.54 logY -3.07 2021ApJS..256...28L

auto: contrast 0.11, within the 0.30 a subdwarf reaches at 28 kK

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.65-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.48-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.40-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.35-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.32-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.30-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.29-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.28-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.59-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.52-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.37-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.67-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 28079 K · log g 5.568 · E(44−55) 0.034 · χ²r 0.18 over 45 bands

distance 1102 pc · parallax 0.9100 ± 0.0400 mas (4%) · R 0.1891 +0.0083 −0.0076 R☉ · M 0.482 +0.074 −0.064 M☉ · L 20.0 +1.9 −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.