J17323+7021

HS1732+7023  ·  Culpan knownhsd

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]53660 ± 1388
log g5.337 ± 0.075
log n(He)/n(H)-0.960 ± 0.065
reduced χ²1.002 over 746 points
radial velocity133.0 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 19:10:02

Observation

cosmic rays3 pixels cancelled
source filespec-101180-59658-27021597906153355.fits

Gaia astrometry

Gaia DR3 source1638672002159650176
parallax [mas]0.1537 ± 0.0420
G15.859
μα [mas/yr]-0.873
μδ [mas/yr]0.378
l, b101.019, 32.052

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.322.16-40.0, 40.05.0-45.0, 45.0
Hγ4340.461.93-40.0, 36.84.5-43.0, 43.0
Hδ4101.731.82-40.0, 31.64.2-43.0, 43.0
Hε3970.071.76-28.0, 30.04.1-30.0, 35.0
Hζ3889.051.73-20.0, 26.24.0-31.8, 32.0
Hη3835.381.70-20.0, 14.64.0-20.7, 21.8
Hθ3797.901.68-16.0, 16.03.9-15.6, 16.7
Hι3770.631.67-13.0, 13.03.9-11.7, 11.6
He II 46864685.702.08-11.9, 11.94.9-15.0, 13.8
He II 54125411.522.40-15.0, 15.05.6-15.0, 15.0
He II 45424541.592.01-15.0, 20.04.7-20.0, 20.0
He II 42004199.841.86-23.5, 33.84.3-20.0, 20.0
He I 44724471.601.98-15.0, 15.04.6-15.0, 15.0
He I 40264026.291.79-24.2, 15.04.2-15.0, 15.0
He I 49224921.932.18-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 53660 K · log g 5.337 · E(44−55) 0.050 · χ²r 0.10 over 35 bands

distance 6506 pc · parallax 0.1500 ± 0.0400 mas (27%) · R 0.3829 +0.1451 −0.0819 R☉ · M 1.164 +1.074 −0.455 M☉ — above the 0.47 canonical mass · L 1096.3 +985.4 −420.2 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.