J07388+0328

Culpan hotsd

χ²/N = 1.01

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]50665 ± 1531
log g5.958 ± 0.100
log n(He)/n(H)-2.070 ± 0.131
reduced χ²1.006 over 745 points
radial velocity-127.0 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 19:07:38

Observation

source filespec-103396-60037-27021598090183122.fits

Gaia astrometry

Gaia DR3 source3137069096828338944
parallax [mas]0.4546 ± 0.0489
G15.814
BP − RP-0.450
Gabs4.102
μα [mas/yr]-2.131
μδ [mas/yr]-3.501
RUWE1.129
l, b215.247, 12.141
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.06-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.84-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.74-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.68-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.65-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.62-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.61-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.60-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.99-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-2.29-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.92-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.78-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.89-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.71-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.09-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 50665 K · log g 5.958 · E(44−55) 0.046 · χ²r 0.26 over 35 bands

distance 2200 pc · parallax 0.4500 ± 0.0500 mas (11%) · R 0.1357 +0.0165 −0.0132 R☉ · M 0.611 +0.181 −0.129 M☉ — above the 0.47 canonical mass · L 109.4 +28.1 −20.5 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.