J20551+0252

PG2052+027  ·  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]52509 ± 1445
log g5.866 ± 0.171
log n(He)/n(H)0.406 ± 0.163
reduced χ²0.987 over 750 points
radial velocity248.0 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 19:10:37

Observation

cosmic rays3 pixels cancelled
source filespec-101061-59866-27021598874739386.fits

Gaia astrometry

Gaia DR3 source1730983351999762944
parallax [mas]0.2401 ± 0.0599
G16.121
μα [mas/yr]0.760
μδ [mas/yr]-11.986
l, b50.943, -25.720

Published (Culpan et al. 2022)

class (Culpan)sdOB
class (SIMBAD)sdOHe

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.324.02-40.0, 40.05.0-45.0, 45.0
Hγ4340.463.59-40.0, 36.84.5-43.0, 43.0
Hδ4101.733.39-40.0, 31.64.2-43.0, 43.0
Hε3970.073.28-28.0, 30.04.1-30.0, 35.0
Hζ3889.053.22-20.0, 26.24.0-31.8, 32.0
Hη3835.383.17-20.0, 14.64.0-20.7, 21.8
Hθ3797.903.14-16.0, 16.03.9-15.6, 16.7
Hι3770.633.12-13.0, 13.03.9-11.7, 11.6
He II 46864685.703.88-11.9, 11.94.9-15.0, 13.8
He II 54125411.524.48-15.0, 15.05.6-15.0, 15.0
He II 45424541.593.76-15.0, 20.04.7-20.0, 20.0
He II 42004199.843.47-23.5, 33.84.3-20.0, 20.0
He I 44724471.603.70-15.0, 15.04.6-15.0, 15.0
He I 40264026.293.33-24.2, 15.04.2-15.0, 15.0
He I 49224921.934.07-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 52509 K · log g 5.866 · E(44−55) 0.118 · χ²r 0.10 over 36 bands

distance 4165 pc · parallax 0.2400 ± 0.0600 mas (25%) · R 0.2470 +0.0827 −0.0492 R☉ · M 1.636 +1.321 −0.603 M☉ — above the 0.47 canonical mass · L 418.3 +326.1 −150.6 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.