J02585+0310

PG0255+029  ·  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]47201 ± 1034
log g6.223 ± 0.099
log n(He)/n(H)-2.046 ± 0.144
reduced χ²0.990 over 745 points
radial velocity-103.0 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 19:07:25

Observation

source filespec-101840-60578-63050396551256494.fits

Gaia astrometry

Gaia DR3 source1792620565667968
parallax [mas]0.6300 ± 0.0474
G15.969
Gabs5.030
μα [mas/yr]4.402
μδ [mas/yr]-6.137
l, b173.248, -46.890

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-1.67-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-1.49-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-1.41-40.0, 31.64.2-43.0, 43.0
Hε3970.07-1.36-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-1.34-20.0, 26.24.0-31.8, 32.0
Hη3835.38-1.32-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-1.30-16.0, 16.03.9-15.6, 16.7
Hι3770.63-1.30-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-1.61-11.9, 11.94.9-15.0, 13.8
He II 54125411.52-1.86-15.0, 15.05.6-15.0, 15.0
He II 45424541.59-1.56-15.0, 20.04.7-20.0, 20.0
He II 42004199.84-1.44-23.5, 33.84.3-20.0, 20.0
He I 44724471.60-1.54-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-1.38-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-1.69-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 47201 K · log g 6.223 · E(44−55) 0.088 · χ²r 0.26 over 33 bands

distance 1587 pc · parallax 0.6300 ± 0.0500 mas (8%) · R 0.1014 +0.0084 −0.0072 R☉ · M 0.629 +0.137 −0.109 M☉ — above the 0.47 canonical mass · L 46.0 +8.0 −6.4 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.