Table 2: Events found in the analysis of the full sample of EROS-2 stars (Tisserand 2004). Only event EROS2-SMC-1 is in the Bright-Star Sample and passes the cuts C1-C12 and therefore is used for limits on the optical depth. All fits assume zero blending and no intrinsic variability. The two values of the fitted parameters t0, $t_{\rm E}$ and u0 are for $B_{\rm eros}$ (first line) and $R_{\rm eros}$ (second line). (There are no $R_{\rm eros}$ points during the event for EROS2-LMC-12.) The time of maximum, t0 is given as JD-2450000.

Candidate
EROS-2 star RA (deg) Dec (deg) $R_{\rm eros}$ $(B-R)_{\rm eros}$ t0 $t_{\rm E}$ u0 $\chi^2$/d.o.f.
EROS2-SMC-1 sm005-4m-5761 15.0233 -72.2507 18.14 -0.13 459.0 105.8 0.53 972.4/873
            460.5 101.6 0.52 862.4/748
EROS2-SMC-5 sm006-6k-19475 12.6625 -72.6983 17.83 0.34 1414.8 29.5 0.90 485.1/875
            1432.0 15.1 1.12 560.0/573
EROS2-LMC-8 lm055-7m-23303 76.6396 -71.6624 20.34 1.16 1594.1 15.3 0.01 344.0/572
            1594.1 8.0 0.03 540.9/510
EROS2-LMC-9 lm042-1l-2622 75.3717 -65.0486 20.93 0.23 2204.1 57.8 0.36 640.8/369
            2215.3 52.7 0.30 292.1/228
EROS2-LMC-10 lm045-5n-26323 80.9925 -65.8733 20.55 0.81 1600.3 37.1 0.33 580.0/505
            1602.2 35.9 0.51 649.1/447
EROS2-LMC-11 lm061-4m-15782 88.4392 -71.2536 20.55 0.55 451.9 51.3 0.36 456.5/444
            446.6 46.1 0.37 458.7/394
EROS2-LMC-12 lm085-6l-14234 89.8750 -74.5676 20.19 0.34 2664.0 49.6 0.27 580.4/391


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