J20496+3004

Feige114  ·  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.

Results and provenance

Fit — Bamberg

Teff [K]40320 ± 267
log g5.665 ± 0.031
log n(He)/n(H)-2.735 ± 0.085
reduced χ²0.984 over 637 points
radial velocity-45.0 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 18:33:17

Fit — Lei (TLUSTY)

Teff [K]37330 ± 170
log g5.540 ± 0.060
log n(He)/n(H)-2.580 ± 0.120
gridsLei et al. 2018, ApJ 868, 70
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

cosmic rays17 pixels cancelled
source filespec-57695-HD205307N293856V01_sp03-139.fits.gz

Gaia astrometry

Gaia DR3 source1858674589447492608
parallax [mas]1.2181 ± 0.0317
G13.488
Gabs3.947
μα [mas/yr]-4.194
μδ [mas/yr]0.190
l, b73.336, -8.702

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)B
Teff [K]37689 ± 189
log g5.56 ± 0.02
log y-2.83 ± 0.08
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.73-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.65-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.62-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.60-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.58-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.58-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.57-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.57-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.70-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-0.67-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.60-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.74-15.0, 15.05.1-15.0, 15.0