J17126+5625

PG1711+565  ·  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]51863 ± 1657
log g5.830 ± 0.081
log n(He)/n(H)-2.782 ± 0.379
reduced χ²0.991 over 745 points
radial velocity13.0 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 19:09:53

Observation

cosmic rays7 pixels cancelled
source filespec-101143-60063-27021597904639878.fits

Gaia astrometry

Gaia DR3 source1432782883580373504
parallax [mas]0.3208 ± 0.0426
G16.010
Gabs3.532
μα [mas/yr]-0.727
μδ [mas/yr]-1.215
l, b84.622, 35.847

Published (Culpan et al. 2022)

class (Culpan)sdB
class (SIMBAD)sdB

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.21-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.19-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.18-40.0, 31.64.2-43.0, 43.0
Hε3970.070.17-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.17-20.0, 26.24.0-31.8, 32.0
Hη3835.380.17-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.16-16.0, 16.03.9-15.6, 16.7
Hι3770.630.16-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.20-11.9, 11.94.9-15.0, 13.8
He II 54125411.520.23-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.20-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.18-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.19-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.17-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.21-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Component 1, the subdwarf: Teff 51863 K (held) · log g 5.830 (held) · R 0.1550 R☉ (fitted, with the companion) · χ²r 0.58 over 35 bands

E(44−55) 0.018 (held)

Component 2, the companion: Teff 5125 K (fitted, 3500–8750 K grid) · log g 4.50 (held) · R 0.8249 R☉ (fitted) · χ²r 0.12 for the two components together (Δχ² 324 over one star, same bands)

The dashed curves beneath the model are the two components of this fit: the subdwarf alone and the cool companion.

distance 3117 pc · parallax 0.3200 ± 0.0400 mas (12%) · M 1.047 +0.383 −0.255 M☉ — above the 0.47 canonical mass · (from the ONE-star scale -- not corrected for the companion's light) · L 276.6 +91.6 −61.8 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.