J09535+1145

χ²/N = 0.99

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]35889 ± 437
log g5.883 ± 0.067
log n(He)/n(H)-1.457 ± 0.067
reduced χ²0.994 over 639 points
radial velocity-72.0 km s−1
resolution (FWHM)2.50 Å
lines fitted12
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 18:30:02

Fit — Lei (TLUSTY)

Teff [K]34780 ± 510
log g5.830 ± 0.110
log n(He)/n(H)-1.490 ± 0.100
gridsLei et al. 2019, ApJ 881, 135
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

source filespec-57400-HD095839N105737B02_sp14-080.fits.gz

Gaia astrometry

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.17-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.04-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.99-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.95-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.93-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.92-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.91-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.91-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.13-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.07-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.97-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.18-15.0, 15.05.1-15.0, 15.0