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Home All issues Volume 707 (March 2026) A&A, 707 (2026) A225 Full HTML
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Table B.1

SED fitting results.

# Teff E(B-V) R
K mag R⊙
16 <17100.0 >0.0 15.0−2.8+1.4Mathematical equation: $15.0_{ - 2.8}^{ + 1.4}$
18 <16200.0 >0.0 40.0−9.2+1.6Mathematical equation: $40.0_{ - 9.2}^{ + 1.6}$
28 18000−2600+6900Mathematical equation: $18000_{ - 2600}^{ + 6900}$ >0.0 15.0−4.0+5.3Mathematical equation: $15.0_{ - 4.0}^{ + 5.3}$
29 >15300.0 – 5.0−0.9+8.7Mathematical equation: $5.0_{ - 0.9}^{ + 8.7}$
30 15000−9700+14000Mathematical equation: $15000_{ - 9700}^{ + 14000}$ – 12.0−5.8+3.2Mathematical equation: $12.0_{ - 5.8}^{ + 3.2}$
31 20000−17800+24500Mathematical equation: $20000_{ - 17800}^{ + 24500}$ – <12.2
32 <17300.0 >0.0 15.0−3.1+1.7Mathematical equation: $15.0_{ - 3.1}^{ + 1.7}$
33 <23400.0 – 5.0−0.9+2.7Mathematical equation: $5.0_{ - 0.9}^{ + 2.7}$
34 15000−1900+14600Mathematical equation: $15000_{ - 1900}^{ + 14600}$ – 8.0−3.6+0.3Mathematical equation: $8.0_{ - 3.6}^{ + 0.3}$
35 20000−4100+9400Mathematical equation: $20000_{ - 4100}^{ + 9400}$ – 20.0−6.0+8.1Mathematical equation: $20.0_{ - 6.0}^{ + 8.1}$
36 <17400.0 >0.0 15.0−2.8+2.6Mathematical equation: $15.0_{ - 2.8}^{ + 2.6}$
37 <17400.0 – 15.0−2.5+2.6Mathematical equation: $15.0_{ - 2.5}^{ + 2.6}$
38 <18900.0 >0.0 5.0−0.6+1.2Mathematical equation: $5.0_{ - 0.6}^{ + 1.2}$
39 19000−4600+21100Mathematical equation: $19000_{ - 4600}^{ + 21100}$ – 8.0−3.6+3.0Mathematical equation: $8.0_{ - 3.6}^{ + 3.0}$
40 21000−5900+2200Mathematical equation: $21000_{ - 5900}^{ + 2200}$ – 5.0−0.6+2.4Mathematical equation: $5.0_{ - 0.6}^{ + 2.4}$
41 21000−4700+2800Mathematical equation: $21000_{ - 4700}^{ + 2800}$ – 5.0−0.6+2.7Mathematical equation: $5.0_{ - 0.6}^{ + 2.7}$
42 <17800.0 >0.0 40.0−7.1+3.4Mathematical equation: $40.0_{ - 7.1}^{ + 3.4}$
43 <16200.0 >0.0 15.0−2.8+1.1Mathematical equation: $15.0_{ - 2.8}^{ + 1.1}$
44 15000−3500+22100Mathematical equation: $15000_{ - 3500}^{ + 22100}$ 0.127−0.136+0.228Mathematical equation: $0.127_{ - 0.136}^{ + 0.228}$ 8.0−3.3+0.6Mathematical equation: $8.0_{ - 3.3}^{ + 0.6}$
45 20000−3900+7600Mathematical equation: $20000_{ - 3900}^{ + 7600}$ >0.0 15.0−3.7+4.7Mathematical equation: $15.0_{ - 3.7}^{ + 4.7}$
46 <15900.0 >0.0 20.0−3.9+0.9Mathematical equation: $20.0_{ - 3.9}^{ + 0.9}$
47 25000−1300+1600Mathematical equation: $25000_{ - 1300}^{ + 1600}$ >0.0 20.0−7.2+9.6Mathematical equation: $20.0_{ - 7.2}^{ + 9.6}$
48 16000−2700+17400Mathematical equation: $16000_{ - 2700}^{ + 17400}$ >0.0 5.0−3.0+0.9Mathematical equation: $5.0_{ - 3.0}^{ + 0.9}$
49 <21600.0 – 5.0−0.6+2.1Mathematical equation: $5.0_{ - 0.6}^{ + 2.1}$
50 <19100.0 – 10.0−3.2+3.4Mathematical equation: $10.0_{ - 3.2}^{ + 3.4}$
51 <15500.0 >0.0 8.0−1.5+0.3Mathematical equation: $8.0_{ - 1.5}^{ + 0.3}$
52 <24400.0 – 15.0−4.9+5.9Mathematical equation: $15.0_{ - 4.9}^{ + 5.9}$
53 <16800.0 >0.0 8.0−2.7+0.6Mathematical equation: $8.0_{ - 2.7}^{ + 0.6}$

Notes. SED fitting results for the effective temperature of the optical counterpart, the absorption and the stellar radius. Upper limits denote parameters for which no lower uncertainty could be determined, and lower limits denote those with no upper uncertainty. Parameters for which neither uncertainty could be determined are indicated with ‘−’.

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