Self-lensing binaries as probes of supernova physics

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Volume 706 (February 2026)

A&A, 706 (2026) A232

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Table 3.

Properties of SL sources.

Group	⟨τ_eff⟩	⟨M_lens⟩	⟨M_source⟩	⟨P_orb⟩	⟨n_cov⟩	⟨n_rec⟩	⟨v_cm⟩	⟨n_tot⟩	μ_sl, max
𝒢_BH, short	$0 . 16_{- 0.11}^{+ 0.26}$ $0.16_{-0.11}^{+0.26}$	$4 . 21_{- 2.09}^{+ 9.46}$ $4.21_{-2.09}^{+9.46}$	$1 . 52_{- 0.77}^{+ 3.16}$ $1.52_{-0.77}^{+3.16}$	$2 . 31_{- 1.21}^{+ 11.72}$ $2.31_{-1.21}^{+11.72}$	$1 . 00_{- 0.00}^{+ 67.09}$ $1.00_{-0.00}^{+67.09}$	$59 . 70_{- 55.62}^{+ 174.90}$ $59.70_{-55.62}^{+174.90}$	$114 . 90_{- 108.79}^{+ 90.66}$ $114.90_{-108.79}^{+90.66}$	$99 . 40_{- 93.90}^{+ 420.68}$ $99.40_{-93.90}^{+420.68}$	13.589040
𝒢_BH, long	$1 . 86_{- 0.71}^{+ 3.84}$ $1.86_{-0.71}^{+3.84}$	$3 . 25_{- 0.99}^{+ 8.22}$ $3.25_{-0.99}^{+8.22}$	$0 . 52_{- 0.22}^{+ 1.62}$ $0.52_{-0.22}^{+1.62}$	$25 . 85_{- 15.15}^{+ 260.38}$ $25.85_{-15.15}^{+260.38}$	$1 . 00_{- 0.00}^{+ 3.53}$ $1.00_{-0.00}^{+3.53}$	$73 . 70_{- 68.30}^{+ 64.83}$ $73.70_{-68.30}^{+64.83}$	$98 . 86_{- 91.79}^{+ 102.96}$ $98.86_{-91.79}^{+102.96}$	$85 . 00_{- 64.60}^{+ 115.33}$ $85.00_{-64.60}^{+115.33}$	200.920301
𝒢_NS	$0 . 24_{- 0.13}^{+ 1.42}$ $0.24_{-0.13}^{+1.42}$	$1 . 28_{- 0.10}^{+ 0.33}$ $1.28_{-0.10}^{+0.33}$	$2 . 18_{- 1.43}^{+ 2.73}$ $2.18_{-1.43}^{+2.73}$	$6 . 03_{- 4.91}^{+ 36.47}$ $6.03_{-4.91}^{+36.47}$	$1 . 00_{- 0.00}^{+ 38.39}$ $1.00_{-0.00}^{+38.39}$	$44 . 06_{- 40.32}^{+ 157.14}$ $44.06_{-40.32}^{+157.14}$	$27 . 18_{- 24.10}^{+ 116.83}$ $27.18_{-24.10}^{+116.83}$	$75 . 30_{- 64.70}^{+ 206.10}$ $75.30_{-64.70}^{+206.10}$	350.909716

Notes. Median properties (except μ_sl, max) of the SL sources in different groups visible in Fig. A.5 for each survey and Galactic component. All values are medians weighted by detection probability across all models. The errors represent tenth and 90th percentiles for lower- and upper-script, respectively. See text for group definitions. Properties include effective Einstein crossing time (τ_eff [day]), lens mass (M_lens[M_⊙]), source mass (M_source[M_⊙]), orbital period (P_orb [day]), coverage (n_cov), recurrence (n_rec), centre-of-mass velocity (v_cm[km/s]), total coverage (n_tot), and highest magnification (μ_sl, max).

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