J06151+3551

SDSSJ061510.23+355117.2  ·  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]27906 ± 259
log g5.635 ± 0.043
log n(He)/n(H)-2.513 ± 0.083
reduced χ²1.004 over 639 points
radial velocity-108.0 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 18:27:25

Fit — Lei (TLUSTY)

Teff [K]28610 ± 280
log g5.680 ± 0.040
log n(He)/n(H)-2.580 ± 0.060
gridsLei et al. 2019, ApJ 881, 135
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

cosmic rays7 pixels cancelled
source filespec-56628-GAC094N35M1_sp15-228.fits.gz

Gaia astrometry

Gaia DR3 source3452919960980353920
parallax [mas]0.6197 ± 0.0516
G16.425
Gabs5.467
μα [mas/yr]2.265
μδ [mas/yr]-3.649
l, b177.024, 8.825

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sd
Teff [K]29076 ± 184
log g5.51 ± 0.04
log y-2.60 ± 0.06
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.75-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.56-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.48-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.43-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.40-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.38-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.37-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.36-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.69-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-1.61-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.45-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.77-15.0, 15.05.1-15.0, 15.0