J18144+4543

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]43264 ± 565
log g6.226 ± 0.062
log n(He)/n(H)-2.378 ± 0.177
reduced χ²0.981 over 746 points
radial velocity-142.0 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 19:10:13

Observation

cosmic rays3 pixels cancelled
source filespec-104494-60466-63050395022727090.fits

Gaia astrometry

Gaia DR3 source2115508887792039936
parallax [mas]0.6397 ± 0.0331
G15.677
BP − RP-0.501
Gabs4.707
μα [mas/yr]-2.454
μδ [mas/yr]-6.104
RUWE1.081
l, b73.308, 25.236
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.30-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-2.06-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.94-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.88-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.84-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.82-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.80-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.79-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.22-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-2.56-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-2.15-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.99-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-2.12-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.91-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.33-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 43264 K · log g 6.226 · E(44−55) 0.014 · χ²r 0.39 over 38 bands

distance 1563 pc · parallax 0.6400 ± 0.0300 mas (5%) · R 0.1086 +0.0061 −0.0054 R☉ · M 0.725 +0.124 −0.105 M☉ — above the 0.47 canonical mass · L 37.3 +4.3 −3.7 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.