J23183+5625

Culpan hotsd

χ²/N = 0.98

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]47817 ± 1158
log g5.692 ± 0.077
log n(He)/n(H)-2.303 ± 0.145
reduced χ²0.977 over 744 points
radial velocity-116.0 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 19:11:03

Observation

cosmic rays4 pixels cancelled
source filespec-100594-60647-63050394940897352.fits

Gaia astrometry

Gaia DR3 source1997202467436858496
parallax [mas]0.8731 ± 0.0250
G15.181
BP − RP0.146
Gabs4.886
μα [mas/yr]-3.909
μδ [mas/yr]1.643
RUWE1.025
l, b110.277, -4.138
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.88-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.68-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.59-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.54-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.50-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.48-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.47-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.46-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.81-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-2.09-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.76-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.63-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.73-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.56-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.90-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 47817 K · log g 5.692 · E(44−55) 0.408 · χ²r 0.59 over 43 bands

distance 1145 pc · parallax 0.8700 ± 0.0300 mas (3%) · R 0.1628 +0.0051 −0.0048 R☉ · M 0.476 +0.066 −0.058 M☉ · L 124.9 +8.3 −7.6 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.