J17030+1508

LAMOSTJ170303.98+150818.3  ·  Culpan knownhsd

χ²/N = 1.00

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.

Results and provenance

Fit — Bamberg

Teff [K]26809 ± 393
log g5.367 ± 0.064
log n(He)/n(H)-1.795 ± 0.057
reduced χ²1.003 over 647 points
radial velocity-75.0 km s−1
resolution (FWHM)2.50 Å
lines fitted13
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 18:32:22

Fit — Lei (TLUSTY)

Teff [K]27460 ± 400
log g5.340 ± 0.040
log n(He)/n(H)-1.880 ± 0.770
gridsLei et al. 2020, ApJ 889, 117
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

cosmic rays3 pixels cancelled
source filespec-58632-GACII257N14B1_sp14-113.fits.gz

Gaia astrometry

Gaia DR3 source4545907052398514432
parallax [mas]0.3634 ± 0.0688
G17.096
Gabs4.886
μα [mas/yr]-7.491
μδ [mas/yr]-3.526
l, b35.062, 30.687

Published (Culpan et al. 2022)

class (Culpan)sdB
Teff [K]30659 ± 307
log g5.64 ± 0.05
log y-1.72 ± 0.03
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.22-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.09-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.03-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.99-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.97-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.96-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.95-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.94-13.0, 13.03.9-11.7, 11.6
Hκ3750.15-0.94-10.0, 10.03.9-7.4, 8.7
He II 46864685.70-1.17-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.12-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.01-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.23-15.0, 15.05.1-15.0, 15.0