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Table 1:

Summary $^{\dagger }$of the, so far, 15 dwarf star microlensing events in the Bulge that have been observed with high-resolution spectrographs. They have been sorted according to their metallicities (as given in Table 2).
Object RAJ2000 DEJ2000 l b $T_{\rm E}$ $T_{\rm max}$ $A_{\rm max}$ $T_{\rm obs}$ Exp. S/N Spec. R Ref.
  [hh:mm:ss] [dd:mm:ss] [deg] [deg] [days] [HJD]   [MJD] [s]        
OGLE-2009-BLG-076S $\phantom{^{b}}$ 17:58:31.9 -29:12:17.8 +1.21 -2.56 36.9 4916.46 70 4916.291 7200 30 UVES 45 000 B09a
MOA-2009-BLG-493S $\phantom{^{b}}$ 17:55:46.0 -28:48:25.8 +1.25 -1.84 13.2 5094.61 150 5093.980 7200 40 UVES 45 000 TW
MOA-2009-BLG-133S $\phantom{^{b}}$ 18:06:32.8 -31:30:10.7 +0.05 -5.19 26.6 4932.10 70 4932.233 7200 35 UVES 45 000 TW
MOA-2009-BLG-475S $\phantom{^{b}}$ 18:02:27.3 -27:26:49.9 +3.16 -2.45 34.0 5084.92 62 5084.980 7200 20 UVES 45 000 TW
MACHO-1999-BLG-022S$^{\ddag }$ 18:05:05.8 -28:34:39.5 +2.46 -3.51 265.0 1365.50 28 1366.315 12600 80 HIRES 29 000 C03
OGLE-2008-BLG-209S $\phantom{^{b}}$ 18:04:50.0 -29:42:35.3 +1.44 -4.01 19.5 4606.09 30 4606.833 5400 30 MIKE 47 000 B09b
MOA-2009-BLG-489S $\phantom{^{b}}$ 17:57:46.5 -28:38:57.8 +1.61 -2.14 58.9 5095.52 103 5094.982 7200 65 UVES 45 000 TW
MOA-2009-BLG-456S $\phantom{^{b}}$ 17:48:56.3 -34:13:32.3 -4.16 -3.34 36.2 5090.94 77 5090.982 7200 45 UVES 45 000 TW
OGLE-2007-BLG-514S $\phantom{^{b}}$ 17:58:03.0 -27:31:08.2 +2.62 -1.63 76.0 4386.28 1200 4385.985 4800 30 MIKE 25 000 E10
MOA-2009-BLG-259S $\phantom{^{b}}$ 17:57:57.6 -29:11:39.1 +1.15 -2.45 69.1 5016.77 220 5016.227 7920 50 UVES 45 000 TW
MOA-2008-BLG-311S $\phantom{^{b}}$ 17:56:53.7 -31:23:40.3 -0.87 -3.35 15.7 4655.40 400 4654.952 7200 85 MIKE 29 000 C09
MOA-2008-BLG-310S $\phantom{^{b}}$ 17:54:14.4 -34:46:37.7 -4.09 -4.56 7.1 4656.39 280 4655.957 7200 90 MIKE 41 000 C09
OGLE-2007-BLG-349S $\phantom{^{b}}$ 18:05:23.0 -26:25:27.1 +4.38 -2.52 109.4 4348.56 400 4348.237 3050 90 HIRES 48 000 C08
MOA-2006-BLG-099S $\phantom{^{b}}$ 17:54:10.2 -35:13:34.9 -4.48 -4.78 30.1 3940.35 380 3940.090 2400 30 MIKE 19 000 J08
OGLE-2006-BLG-265S $\phantom{^{b}}$ 18:07:18.9 -27:47:44.0 +3.38 -3.55 28.6 3893.24 212 3892.581 900 45 HIRES 45 000 J07

Notes.  $^{(\dagger)}$ Given for each microlensing event is: RA and DE coordinates (J2000) read from the fits headers of the spectra (the direction where the telescope pointed during observation); galactic coordinates (l and b); duration of the event in days ($T_{\rm E}$); time when maximum magnification occured ( $T_{\rm max}$); maximum magnification ( $A_{\rm max}$); time when event was observed with high-resolution spectrograph ( $T_{\rm obs}$); magnification at the time of observation ( $A_{\rm obs}$); the exposure time (Exp.), the measured signal-to-noise ration per pixel at $\sim$6400 Å; the spectrograph that was used; the spectral resolution; and the reference where the star first appeared: TW = This Work, B09a = Bensby et al. (2009a), B09b = Bensby et al. (2009b), J07 = Johnson et al. (2007), J08 = Johnson et al. (2008), C08 = Cohen et al. (2008), C09 = Cohen et al. (2009), C03 = Cavallo et al. (2003), E10 = Epstein et al. (2010). $^{(\ddag )}$ MACHO ID: 109.20893.3423.


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