J07079+3551

LAMOSTJ070758.35+355127.6  ·  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]54977 ± 1966
log g6.024 ± 0.134
log n(He)/n(H)-0.897 ± 0.124
reduced χ²0.983 over 745 points
radial velocity15.0 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 19:07:34

Observation

cosmic rays3 pixels cancelled
source filespec-100839-60674-63050394829181528.fits

Gaia astrometry

Gaia DR3 source945758945404830464
parallax [mas]0.1574 ± 0.0780
G16.898
μα [mas/yr]0.443
μδ [mas/yr]-0.449
l, b181.467, 18.608

Published (Culpan et al. 2022)

class (Culpan)sdO
Teff [K]56397 ± 674
log g6.11 ± 0.06
log y-1.34 ± 0.07
reference2021ApJS..256...28L

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.24-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.22-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.21-40.0, 31.64.2-43.0, 43.0
Hε3970.070.20-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.19-20.0, 26.24.0-31.8, 32.0
Hη3835.380.19-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.19-16.0, 16.03.9-15.6, 16.7
Hι3770.630.19-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.23-11.9, 11.94.9-15.0, 13.8
He II 54125411.520.27-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.23-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.21-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.22-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.20-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.25-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 54977 K · log g 6.024 · E(44−55) 0.078 · χ²r 0.87 over 23 bands

distance 6353 pc · parallax 0.1600 ± 0.0800 mas (50%) · R 0.2351 +0.2064 −0.0761 R☉ · M 2.134 +5.411 −1.169 M☉ — above the 0.47 canonical mass · L 455.2 +1149.6 −247.1 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.