Table 4: The 11 events of the EROS collaboration used in the past to set upper limits on the microlensing optical depth toward the LMC and to measure the depth toward the SMC. Candidates marked "B-S'' in Col. 2 occur on stars in the EROS-2 Bright-Star Sample. All candidates except EROS2-SMC-1 have been eliminated as variable stars or as supernovae.
Candidate EROS-2 star $R_{\rm eros}$ $(B-R)_{\rm eros}$ Original ref. Status

EROS1-LMC-1 lm058-2k-21915 18.75 0.34 Aubourg et al. (1993) 2nd variation (Tisserand 2004) (Figure 9)

EROS1-LMC-2 lm043-6m- 9377 B-S 19.32 -0.04 Aubourg et al. (1993) 2nd variation (Lasserre et al. 2000)

EROS2-LMC-3 lm034-6l-20493 20.90 0.61 Lasserre et al. (2000) 2nd variation (Tisserand 2004)

EROS2-LMC-4 lm018-6n-23236 19.10 1.87 Lasserre et al. (2000) 2nd variation (Milsztajn et al. 2001)

EROS2-LMC-5 lm015-3n-22431 B-S 19.17 0.14 Milsztajn et al. (2001) Supernova (Tisserand 2004)

EROS2-LMC-6 lm067-5m-14700 21.01 0.63 Milsztajn et al. (2001) Supernova (Tisserand 2004)

EROS2-LMC-7 lm070-3n-23389 21.00 0.76 Milsztajn et al. (2001) Supernova (Tisserand 2004)

EROS2-SMC-1 sm005-4m-5761 B-S 18.13 -0.13 Palanque-D. et al. (1998) Fig. 7

EROS2-SMC-2 sm001-6l-13221 B-S 19.56 0.44 Afonso et al. (2003a) long period variable (Tisserand 2004)

EROS2-SMC-3 sm001-6n-16904 B-S 19.31 0.59 Afonso et al. (2003a) long period variable (Tisserand 2004)

EROS2-SMC-4 sm002-7m-21331 B-S 19.48 0.32 Afonso et al. (2003a) long period variable (Tisserand 2004)

**Table 4:** The 11 events of the EROS collaboration used in the past to set upper limits on the microlensing optical depth toward the LMC and to measure the depth toward the SMC. Candidates marked "B-S'' in Col. 2 occur on stars in the EROS-2 Bright-Star Sample. All candidates except EROS2-SMC-1 have been eliminated as variable stars or as supernovae.
Candidate	EROS-2 star	$R_{\rm eros}$	$(B-R)_{\rm eros}$	Original ref.	Status
EROS1-LMC-1	lm058-2k-21915	18.75	0.34	Aubourg et al. (1993)	2nd variation (Tisserand 2004) (Figure 9)
EROS1-LMC-2	lm043-6m- 9377 B-S	19.32	-0.04	Aubourg et al. (1993)	2nd variation (Lasserre et al. 2000)
EROS2-LMC-3	lm034-6l-20493	20.90	0.61	Lasserre et al. (2000)	2nd variation (Tisserand 2004)
EROS2-LMC-4	lm018-6n-23236	19.10	1.87	Lasserre et al. (2000)	2nd variation (Milsztajn et al. 2001)
EROS2-LMC-5	lm015-3n-22431 B-S	19.17	0.14	Milsztajn et al. (2001)	Supernova (Tisserand 2004)
EROS2-LMC-6	lm067-5m-14700	21.01	0.63	Milsztajn et al. (2001)	Supernova (Tisserand 2004)
EROS2-LMC-7	lm070-3n-23389	21.00	0.76	Milsztajn et al. (2001)	Supernova (Tisserand 2004)
EROS2-SMC-1	sm005-4m-5761 B-S	18.13	-0.13	Palanque-D. et al. (1998)	Fig. 7
EROS2-SMC-2	sm001-6l-13221 B-S	19.56	0.44	Afonso et al. (2003a)	long period variable (Tisserand 2004)
EROS2-SMC-3	sm001-6n-16904 B-S	19.31	0.59	Afonso et al. (2003a)	long period variable (Tisserand 2004)
EROS2-SMC-4	sm002-7m-21331 B-S	19.48	0.32	Afonso et al. (2003a)	long period variable (Tisserand 2004)