J07107+6655sdB

HS0705+6700  ·  07:10:42.05 66:55:43.54  ·  Culpan knownhsd

χ²/N = 1.01

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.

Line-profile fit — uli

profile fit on the uli grid
Observed spectrum in black, model in red, offset by line. Balmer series left, helium right.

Results and provenance

Fit — Bamberg

Teff [K]28009 ± 584
log g5.570 ± 0.101
log n(He)/n(H)-2.427 ± 0.113
reduced χ²1.011 over 639 points
radial velocity-59.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsHE-0.041.fits
HE-0.125.fits
HE-0.300.fits
HE-0.550.fits
+9 more
fitted04/09/2026 19:07:34

Fit — uli

Teff [K]28575 ± 686
log g5.473 ± 0.103
log n(He)/n(H)-2.425 ± 0.121
reduced χ²1.010 over 639 points
radial velocity-59.0 km s−1
resolution (FWHM)2.00 Å
lines fitted12
gridsh667.grid
h909.grid
h97.grid
h99.grid
+1 more
fitted04/09/2026 18:34:46

Observation

telescopeSDSS 2.5-M
survey / programmeMWM / mwm_cb
field · MJD102983 · 59952
date2023-01-08
catalogid27021597913228689
exposure900 s in 1
airmass1.23
seeing (50%)1.10″
E(B−V)0.052
pipelinev6_2_1
S/N (classifier)22.8
source filespec-102983-59952-27021597913228689.fits

Gaia astrometry

Gaia DR3 source1102107819544067456
parallax [mas]0.7895 ± 0.0321
G14.616
BP − RP-0.344
Gabs4.143
μα [mas/yr]-0.454
μδ [mas/yr]-7.705
l, b148.843, 26.666

Published (Culpan et al. 2022)

class (Culpan)sdB+dM
class (SIMBAD)sdB+dM
Teff [K]30200 ± 1000
log g5.70 ± 0.20
log y-2.60 ± 0.30
reference2003A&A...400..939E

Classifier

AGREES

fitted Teff 30200 logg 5.7 logY -2.6 2003A&A...400..939E

auto: contrast 0.17, within the 0.34 a subdwarf reaches at 25 kK, Ca II 8662/8542 = 6.2 -- the star's own Paschen lines, not a companion; CONTINUUM WAVY (0.030, typical 0.008) -- Balmer jump and continuum shape unreliable

Fitted lines

lineλ [Å]shift [Å]continuum at±avgfitted over
Hβ4861.32-0.96-40.0, 40.05.0-45.0, 45.0
Hγ4340.46-0.85-40.0, 36.84.5-43.0, 43.0
Hδ4101.73-0.81-40.0, 31.64.2-43.0, 43.0
Hε3970.07-0.78-28.0, 30.04.1-30.0, 35.0
Hζ3889.05-0.77-20.0, 26.24.0-31.8, 32.0
Hη3835.38-0.75-20.0, 14.64.0-20.7, 21.8
Hθ3797.90-0.75-16.0, 16.03.9-15.6, 16.7
Hι3770.63-0.74-13.0, 13.03.9-11.7, 11.6
He II 46864685.70-0.92-11.9, 11.94.9-15.0, 13.8
He I 44724471.60-0.88-15.0, 15.04.6-15.0, 15.0
He I 40264026.29-0.79-24.2, 15.04.2-15.0, 15.0
He I 49224921.93-0.97-15.0, 15.05.1-15.0, 15.0

Spectral energy distribution

Teff 28009 K · log g 5.570 · E(44−55) 0.090 · χ²r 0.28 over 37 bands

distance 1267 pc · parallax 0.7900 ± 0.0300 mas (4%) · R 0.2319 +0.0103 −0.0095 R☉ · M 0.729 +0.113 −0.098 M☉ — above the 0.47 canonical mass · L 29.8 +2.9 −2.5 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.