J07489+3042

GALEXJ07489+3042  ·  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]29986 ± 280
log g5.753 ± 0.042
log n(He)/n(H)-1.981 ± 0.043
reduced χ²0.997 over 639 points
radial velocity-194.0 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 18:28:49

Fit — Lei (TLUSTY)

Teff [K]31080 ± 90
log g5.650 ± 0.020
log n(He)/n(H)-1.980 ± 0.040
gridsLei et al. 2018, ApJ 868, 70
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

source filespec-56338-GAC114N32B1_sp07-139.fits.gz

Gaia astrometry

Gaia DR3 source879237740307303040
parallax [mas]1.3338 ± 0.0322
G14.046
Gabs4.715
μα [mas/yr]-18.330
μδ [mas/yr]-6.022
l, b189.715, 25.013

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB
Teff [K]30760 ± 830
log g5.71 ± 0.17
log y-1.85 ± 0.13
reference2012MNRAS.427.2180N

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-3.15-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.81-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-2.65-40.0, 31.64.2-43.0, 43.0
Hε3970.07-2.57-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-2.52-20.0, 26.24.0-31.8, 32.0
Hη3835.38-2.48-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-2.46-16.0, 16.03.9-15.6, 16.7
Hι3770.63-2.44-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-3.03-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-2.89-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-2.61-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-3.19-15.0, 15.05.1-15.0, 15.0