J13362-6314

Culpan hotsd

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]43898 ± 828
log g6.256 ± 0.091
log n(He)/n(H)-1.795 ± 0.119
reduced χ²0.998 over 745 points
radial velocity-88.0 km s−1
resolution (FWHM)2.00 Å
lines fitted15
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:09:01

Observation

source filespec-112058-60406-63050396106284458.fits

Gaia astrometry

Gaia DR3 source5865062826743955200
parallax [mas]0.7001 ± 0.0362
G15.947
BP − RP-0.156
Gabs5.173
μα [mas/yr]-8.290
μδ [mas/yr]-1.083
RUWE0.986
l, b307.946, -0.806
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.43-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.27-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.20-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.17-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.14-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.13-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.11-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.11-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.38-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-1.59-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.33-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.23-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.31-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.18-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.44-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 43898 K · log g 6.256 · E(44−55) 0.212 · χ²r 0.36 over 35 bands

distance 1428 pc · parallax 0.7000 ± 0.0400 mas (6%) · R 0.1154 +0.0065 −0.0059 R☉ · M 0.877 +0.150 −0.128 M☉ — above the 0.47 canonical mass · L 44.6 +5.3 −4.5 L☉

Photometry against the model, with the residual beneath it in units of the error. The horizontal bar on each point is the passband, not an error; a hollow point was not fitted and the tooltip says why. Drag a box to zoom, double-click or Esc to come back out.