J21424-6019

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]54660 ± 2788
log g6.048 ± 0.214
log n(He)/n(H)-0.800 ± 0.197
reduced χ²1.004 over 746 points
radial velocity-105.0 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 19:10:46

Observation

source filespec-106279-60226-63050396469325441.fits

Gaia astrometry

Gaia DR3 source6410092557312874112
parallax [mas]0.3849 ± 0.0607
G16.942
BP − RP-0.523
Gabs4.869
μα [mas/yr]-1.736
μδ [mas/yr]-7.742
RUWE0.999
l, b333.313, -44.044
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.70-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.52-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.44-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.39-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.36-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.34-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.33-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.32-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.64-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-1.90-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.59-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.47-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.57-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.41-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.72-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 54660 K · log g 6.048 · E(44−55) 0.008 · χ²r 0.25 over 33 bands

distance 2598 pc · parallax 0.3800 ± 0.0600 mas (16%) · R 0.0864 +0.0163 −0.0117 R☉ · M 0.305 +0.134 −0.083 M☉ — below the 0.47 canonical mass · L 60.0 +24.8 −15.3 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.