J14159-0227

SDSSJ141558.19-022714.3  ·  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]37478 ± 620
log g5.867 ± 0.074
log n(He)/n(H)-2.473 ± 0.130
reduced χ²0.983 over 745 points
radial velocity-130.0 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 19:09:06

Observation

source filespec-4035-55383-0112.fits

Gaia astrometry

Gaia DR3 source3646597074491788800
parallax [mas]0.3963 ± 0.1977
G18.458
μα [mas/yr]-5.691
μδ [mas/yr]-6.126
l, b340.812, 54.081

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-2.11-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.88-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.78-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.72-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.69-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.66-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.65-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.64-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-2.03-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-2.35-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.97-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.82-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.94-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.75-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-2.13-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 37478 K · log g 5.867 · E(44−55) 0.076 · χ²r 0.30 over 12 bands

distance 2523 pc · parallax 0.4000 ± 0.2000 mas (50%) · R 0.0583 +0.0517 −0.0190 R☉ · M 0.092 +0.235 −0.050 M☉ — below the 0.47 canonical mass · L 6.0 +15.5 −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.