J17059+3632

SDSSJ170556.15+363221.8  ·  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]48845 ± 1125
log g5.068 ± 0.060
log n(He)/n(H)-1.218 ± 0.046
reduced χ²0.994 over 745 points
radial velocity60.0 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 19:09:50

Observation

source filespec-4988-55825-0831.fits

Gaia astrometry

Gaia DR3 source1339310200352649856
parallax [mas]0.1056 ± 0.0758
G17.482
μα [mas/yr]-2.387
μδ [mas/yr]-0.753
l, b59.955, 36.097

Published (Culpan et al. 2022)

class (Culpan)sdO
class (SIMBAD)sdO

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.320.97-40.0, 40.05.0-45.0, 45.0
Hγ4340.460.87-40.0, 36.84.5-43.0, 43.0
Hδ4101.730.82-40.0, 31.64.2-43.0, 43.0
Hε3970.070.79-28.0, 30.04.1-30.0, 35.0
Hζ3889.050.78-20.0, 26.24.0-31.8, 32.0
Hη3835.380.77-20.0, 14.64.0-20.7, 21.8
Hθ3797.900.76-16.0, 16.03.9-15.6, 16.7
Hι3770.630.75-13.0, 13.03.9-11.7, 11.6
He II 46864685.700.94-11.9, 11.94.9-15.0, 13.8
He II 54125411.521.08-15.0, 15.05.6-15.0, 15.0
He II 45424541.590.91-15.0, 20.04.7-20.0, 20.0
He II 42004199.840.84-23.5, 33.84.3-20.0, 20.0
He I 44724471.600.89-15.0, 15.04.6-15.0, 15.0
He I 40264026.290.81-24.2, 15.04.2-15.0, 15.0
He I 49224921.930.99-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 48845 K · log g 5.068 · E(44−55) 0.034 · χ²r 0.18 over 18 bands

distance 9470 pc · parallax 0.1100 ± 0.0800 mas (73%) · R 0.2528 +0.3298 −0.0981 R☉ · M 0.273 +1.185 −0.172 M☉ · L 328.2 +1413.6 −205.5 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.