J16120+5149

PG1610+519  ·  Culpan knownhsd

χ²/N = 0.90

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]41532 ± 1426
log g5.259 ± 0.107
log n(He)/n(H)-3.292 ± 0.391
reduced χ²0.905 over 639 points
radial velocity-139.0 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 18:32:00

Fit — Lei (TLUSTY)

Teff [K]34620 ± 380
log g5.080 ± 0.050
log n(He)/n(H)-3.000 ± 0.000
gridsLei et al. 2018, ApJ 868, 70
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid
heliumpublished as a limit

Observation

source filespec-56414-HD161547N531412F01_sp05-207.fits.gz

Gaia astrometry

Gaia DR3 source1427678435208512384
parallax [mas]0.9379 ± 0.0370
G13.655
Gabs3.546
μα [mas/yr]2.524
μδ [mas/yr]-17.651
l, b80.506, 45.314

Published (Culpan et al. 2022)

class (Culpan)sdOB+WD
class (SIMBAD)sdO8VIHe1
Teff [K]48506 ± 629
log g5.24 ± 0.08
log y-2.02 ± 0.13
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.25-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.01-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.90-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.84-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.80-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.78-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.76-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.75-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.17-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.07-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.87-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.28-15.0, 15.05.1-15.0, 15.0