J14455+1727

Culpan hotsd

outside the grid 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]62949 ± 748
log g7.279 ± 0.076
log n(He)/n(H)-2.809 ± 0.123
reduced χ²0.990 over 744 points
radial velocity19.0 km s−1
resolution (FWHM)2.50 Å
lines fitted15
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
settledoutside the grid
fitted04/09/2026 18:31:28

Fit — Lei (TLUSTY)

Teff [K]71170 ± 6170
log g6.900 ± 0.070
log n(He)/n(H)-2.080 ± 0.240
gridsLei et al. 2020, ApJ 889, 117
SYNSPEC 49 spectra from NLTE TLUSTY 204 model atmospheres, through XTgrid

Observation

source filespec-57870-HD145323N181407M01_sp10-031.fits.gz

Gaia astrometry

Gaia DR3 source1234828283288291840
parallax [mas]1.4175 ± 0.0648
G16.209
BP − RP-0.553
Gabs6.967
μα [mas/yr]-3.808
μδ [mas/yr]-21.680
RUWE0.958
l, b18.748, 61.984
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.31-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.28-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.26-40.0, 31.64.2-43.0, 43.0
Hε3970.070.25-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.25-20.0, 26.24.0-31.8, 32.0
Hη3835.380.24-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.24-16.0, 16.03.9-15.6, 16.7
Hι3770.630.24-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.30-11.9, 11.94.9-15.0, 13.8
He II 54125411.520.34-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.29-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.27-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.28-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.26-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.31-15.0, 15.05.1-15.0, 15.0