J11509+1631

SDSSJ115059.67+163139.4  ·  Culpan knownhsd

χ²/N = 0.99

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]46416 ± 754
log g6.042 ± 0.105
log n(He)/n(H)-0.541 ± 0.081
reduced χ²0.995 over 745 points
radial velocity-263.0 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 19:08:41

Observation

cosmic rays3 pixels cancelled
source filespec-5892-56035-0008.fits

Gaia astrometry

Gaia DR3 source3926312214122239360
parallax [mas]0.5862 ± 0.1362
G17.588
μα [mas/yr]-9.071
μδ [mas/yr]-18.964
l, b246.976, 72.446

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdOHe
Teff [K]46141 ± 2588
log g5.75 ± 0.17
log y-0.28 ± 0.22
reference2019MNRAS.486.2169K

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-4.26-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-3.81-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-3.60-40.0, 31.64.2-43.0, 43.0
Hε3970.07-3.48-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-3.41-20.0, 26.24.0-31.8, 32.0
Hη3835.38-3.36-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-3.33-16.0, 16.03.9-15.6, 16.7
Hι3770.63-3.31-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-4.11-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-4.75-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-3.98-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-3.68-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-3.92-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-3.53-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-4.32-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 46416 K · log g 6.042 · E(44−55) 0.034 · χ²r 0.13 over 9 bands

distance 1706 pc · parallax 0.5900 ± 0.1400 mas (24%) · R 0.0479 +0.0146 −0.0090 R☉ · M 0.092 +0.068 −0.033 M☉ — below the 0.47 canonical mass · L 9.6 +6.8 −3.3 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.