J16342+1631

SDSSJ163413.09+163109.4  ·  Culpan knownhsd

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]38608 ± 787
log g5.088 ± 0.092
log n(He)/n(H)-2.188 ± 0.120
reduced χ²0.985 over 745 points
radial velocity94.0 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 19:09:44

Observation

source filespec-4064-55366-0104.fits

Gaia astrometry

Gaia DR3 source4465985437664273536
parallax [mas]0.1552 ± 0.1518
G18.285
μα [mas/yr]-2.017
μδ [mas/yr]-3.295
l, b33.415, 37.629

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)DAO
Teff [K]34600 ± 900
log g4.73 ± 0.12
log y-2.00 ± 0.50
reference2015A&A...577A..26G

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.321.52-40.0, 40.05.0-45.0, 45.0
Hγ4340.461.36-40.0, 36.84.5-43.0, 43.0
Hδ4101.731.29-40.0, 31.64.2-43.0, 43.0
Hε3970.071.24-28.0, 30.04.1-30.0, 35.0
Hζ3889.051.22-20.0, 26.24.0-31.8, 32.0
Hη3835.381.20-20.0, 14.64.0-20.7, 21.8
Hθ3797.901.19-16.0, 16.03.9-15.6, 16.7
Hι3770.631.18-13.0, 13.03.9-11.7, 11.6
He II 46864685.701.47-11.9, 11.94.9-15.0, 13.8
He II 54125411.521.70-15.0, 15.05.6-15.0, 15.0
He II 45424541.591.42-15.0, 20.04.7-20.0, 20.0
He II 42004199.841.32-23.5, 33.84.3-20.0, 20.0
He I 44724471.601.40-15.0, 15.04.6-15.0, 15.0
He I 40264026.291.26-24.2, 15.04.2-15.0, 15.0
He I 49224921.931.54-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 38608 K · log g 5.088 · E(44−55) 0.138 · χ²r 0.47 over 10 bands

distance 6443 pc · parallax 0.1600 ± 0.1500 mas (94%) · R 0.1449 +0.2318 −0.0623 R☉ · M 0.093 +0.537 −0.063 M☉ · L 41.9 +242.4 −28.3 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.