J14276+0142sdB

PG1425+019 · 14:27:41.02 01:42:55.01 · Culpan knownhsd

χ²/N = 0.97

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

Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Line-profile fit — uli

Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Results and provenance

Fit — Bamberg

T_eff [K]	29326 ± 155
log g	5.669 ± 0.024
log n(He)/n(H)	-3.704 ± 0.336
reduced χ²	0.974 over 640 points
radial velocity	-66.0 km s⁻¹
resolution (FWHM)	2.00 Å
lines fitted	12
grids	HE-0.041.fits HE-0.125.fits HE-0.300.fits HE-0.550.fits +9 more
fitted	04/09/2026 19:09:08

Fit — uli

T_eff [K]	29919 ± 139
log g	5.587 ± 0.026
log n(He)/n(H)	-3.226 ± 0.078 upper limit
reduced χ²	0.977 over 640 points
radial velocity	-66.0 km s⁻¹
resolution (FWHM)	2.00 Å
lines fitted	12
grids	h667.grid h909.grid h97.grid h99.grid +1 more
settled	outside the grid
fitted	04/09/2026 18:36:02

Observation

telescope	SDSS 2.5-M
survey / programme	boss
date	2011-03-09
exposure	5405 s in 12
pipeline	v5_13_2
S/N (classifier)	65.5
source file	spec-4027-55629-0036.fits

Gaia astrometry

Gaia DR3 source	3654573039213596672
parallax [mas]	0.4569 ± 0.0630
G	16.119
G_abs	4.444
μ_α [mas/yr]	-0.169
μ_δ [mas/yr]	-3.914
l, b	349.225, 55.684

Published (Culpan et al. 2022)

class (Culpan)	sdB
class (SIMBAD)	DA
T_eff [K]	33417 ± 556
log g	5.76 ± 0.11
log y	-3.02 ± 0.41
reference	2021ApJS..256...28L

Classifier

AGREES

fitted Teff 33417 logg 5.76 logY -3.02 2021ApJS..256...28L

auto: contrast 0.09, within the 0.29 a subdwarf reaches at 29 kK, Mg I b suggests a companion but Ca II does not (-0.0 sigma)

Fitted lines

line	λ [Å]	shift [Å]	continuum at	±avg	fitted over
H_β	4861.32	-1.07	-40.0, 40.0	5.0	-45.0, 45.0
H_γ	4340.46	-0.96	-40.0, 36.8	4.5	-43.0, 43.0
H_δ	4101.73	-0.90	-40.0, 31.6	4.2	-43.0, 43.0
H_ε	3970.07	-0.87	-28.0, 30.0	4.1	-30.0, 35.0
H_ζ	3889.05	-0.86	-20.0, 26.2	4.0	-31.8, 32.0
H_η	3835.38	-0.84	-20.0, 14.6	4.0	-20.7, 21.8
H_θ	3797.90	-0.84	-16.0, 16.0	3.9	-15.6, 16.7
H_ι	3770.63	-0.83	-13.0, 13.0	3.9	-11.7, 11.6
He II 4686	4685.70	-1.03	-11.9, 11.9	4.9	-15.0, 13.8
He I 4472	4471.60	-0.98	-15.0, 15.0	4.6	-15.0, 15.0
He I 4026	4026.29	-0.89	-24.2, 15.0	4.2	-15.0, 15.0
He I 4922	4921.93	-1.08	-15.0, 15.0	5.1	-15.0, 15.0

Spectral energy distribution

T_eff 29326 K · log g 5.669 · E(44−55) 0.028 · χ²_r 0.17 over 37 bands

distance 2189 pc · parallax 0.4600 ± 0.0600 mas (13%) · R 0.1730 +0.0278 −0.0209 R☉ · M 0.511 +0.193 −0.128 M☉ · L 20.0 +7.0 −4.6 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.