J17077-6722

Culpan hotsd

χ²/N = 0.96

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]44839 ± 942
log g6.178 ± 0.106
log n(He)/n(H)-1.604 ± 0.121
reduced χ²0.957 over 744 points
radial velocity-46.0 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 19:09:51

Observation

source filespec-030412-60063-27021599280348982.fits

Gaia astrometry

Gaia DR3 source5814742165191289984
parallax [mas]0.3619 ± 0.0502
G16.496
BP − RP-0.436
Gabs4.289
μα [mas/yr]0.129
μδ [mas/yr]-5.826
RUWE0.944
l, b324.005, -15.735
selectionf_plx

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.75-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.67-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.63-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.61-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.60-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.59-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.58-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.58-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.72-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-0.83-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-0.70-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-0.64-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-0.69-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.62-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.76-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 44839 K · log g 6.178 · E(44−55) 0.054 · χ²r 0.25 over 36 bands

distance 2763 pc · parallax 0.3600 ± 0.0500 mas (14%) · R 0.1359 +0.0221 −0.0166 R☉ · M 1.018 +0.390 −0.256 M☉ — above the 0.47 canonical mass · L 67.3 +23.6 −15.6 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.