J/AcA/68/183/table2Characteristics of 2509 microlensing eventsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintEventEvent Namemeta.id;meta.maincharLensSpTypeLens Spectral Typesrc.spTypecharLensSourceLens GDR2 IDmeta.idRALdegLens Right ascension (ICRS, Ep=J2015.5)degpos.eq.rae_RALdegError on Lens RA (mas)masstat.errorfloatDELdegLens Declination (ICRS, Ep=J2015.5)degpos.eq.dece_DELdegError on Lens DE (mas)masstat.errorfloatLenspmRALens Proper Motion along RA, pmRA*cosDEmas/yrpos.pmdoublee_LenspmRAError on Lens Proper Motion RAmas/yrstat.errorfloatLenspmDELens Proper Motion along DEmas/yrpos.pmdoublee_LenspmDEError on Lens Proper Motion DEmas/yrstat.errorfloatLensplxLens Parallaxmaspos.parallax.trigfloate_LensplxError on Lens Parallaxmasstat.errorfloatLensGmagLens G Mean Magnitudemagphot.mag;em.optfloate_LensGmagError on Lens G Mean Magnitudemagstat.error;phot.magfloatLensBPmagLens G_BP Mean Magnitudemagphot.mag;em.opt.Bfloate_LensBPmagError on Lens G_BP Mean Magnitudemagstat.error;phot.magfloatLensRPmagLens G_RP Mean Magnitudemagphot.mag;em.opt.Rfloate_LensRPmagError on Lens G_RP Mean Magnitudemagstat.error;phot.magfloatLensMassLens MasssolMassphys.massfloatSourceSource Gaia DR2 IDmeta.id.parentRAICRSSource Right ascension (ICRS, Ep=J2015.5)degpos.eq.ra;meta.maine_RAICRSError on Source RAmasstat.error;pos.eq.rafloatDEICRSSource Declination (ICRS, Ep=2015.5)degpos.eq.dec;meta.maine_DEICRSError on Source DEmasstat.error;pos.eq.decfloatpmRA? Source Proper Motion along RAmas/yrpos.pm;pos.eq.rafloatnullablee_pmRA? Error on Source Proper Motion RAmas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmDE? Source Proper Motion along DEmas/yrpos.pm;pos.eq.decdoublenullablee_pmDE? Error on Source Proper Motion DEmas/yrstat.error;pos.pm;pos.eq.decfloatnullableplx? Source Parallaxmaspos.parallax.trigfloatnullablee_plx? Error On Source Parallaxmasstat.error;pos.parallaxfloatnullableGmagSource G Mean Magnitudemagphot.mag;em.optfloate_GmagError On Source G Mean Magnitudemagstat.error;phot.magfloatBPmag? Source G_BP Mean Magnitudemagphot.mag;em.opt.Bfloatnullablee_BPmag? Error On Source G_BP Mean Magnitudemagstat.error;phot.magfloatnullableRPmag? Source G_RP Mean Magnitudemagphot.mag;em.opt.Rfloatnullablee_RPmag? Error On Source G_RP Mean Magnitudemagstat.error;phot.magfloatnullablee1_thetaE2.3 Percentile theta_Emasstat.errorfloate2_thetaE15.9 Percentile theta_Emasstat.errorfloatthetaEMedian theta_Emasstat.fit.paramfloate3_thetaE84.1 Percentile theta_Emasstat.errorfloate4_thetaE97.7 Percentile theta_Emasstat.errorfloate1_u0t2.3 Percentile u_0 (u_0_t)stat.errorfloate2_u0t15.9 Percentile u_0 (u_0_t)stat.errorfloatu0tMedian angular distance on the sky u_0 (u_0_t)pos.distance;stat.minfloate3_u0t84.1 Percentile u_0 (u_0_t)stat.errorfloate4_u0t97.7 Percentile u_0 (u_0_t)stat.errorfloatP(u0<1)Probability that the event will have u_0_<1stat.fit.goodnessfloatP(u0<2)Probability that the event will have u_0_<2stat.fit.goodnessfloatP(u0<5)Probability that the event will have u_0_<5stat.fit.goodnessfloatP(u0<10)Probability that the event will have u_0_<10stat.fit.goodnessfloate1_thetaE*u02.3 Percentile theta_E*u_0masstat.errorfloate2_thetaE*u015.9 Percentile theta_E*u_0masstat.errorfloatthetaE*u0Median theta_E*u_0masstat.fit.paramfloate3_thetaE*u084.1 Percentile theta_E*u_0masstat.errorfloate4_thetaE*u097.7 Percentile theta_E*u_0masstat.errorfloatP(thetaE*u0<100)Probability that the event will have theta_E_*u_0_<100masstat.fit.goodnessfloatP(thetaE*u0<200)Probability that the event will have theta_E_*u_0_<200masstat.fit.goodnessfloatP(thetaE*u0<500)Probability that the event will have theta_E_*u_0_<500masstat.fit.goodnessfloatP(thetaE*u0<1000)Probability that the event will have theta_E_*u_0_<1000masstat.fit.goodnessfloate1_t02.3 Percentile t_0_ (Julian year)yrstat.errordoublee2_t015.9 Percentile t_0_ (Julian year)yrstat.errordoublee3_t084.1 Percentile t_0_ (Julian year)yrstat.errordoublee4_t097.7 Percentile t_0_ (Julian year)yrstat.errordoublee1_dAA12.3 Percentile {DELTA}(A,A_1_)magstat.errorfloate2_dAA115.9 Percentile {DELTA}(A,A_1_)magstat.errorfloatdAA1Median difference between the minimum and maximum magnifications of an event over the time period adopted in this paper {DELTA}(A,A_1_)magphot.mag;arith.difffloate3_dAA184.1 Percentile {DELTA}(A,A_1_)]magstat.errorfloate4_dAA197.7 Percentile {DELTA}(A,A_1_)]magstat.errorfloate1_TdAA12.3 Percentile T[{DELTA}(A,A_1_)]dstat.errorfloate2_TdAA115.9 Percentile T[{DELTA}(A,A_1_)]dstat.errorfloatTdAA1Median amount of time that an event spends with its magnification above min{A,A1}+{DELTA}(A,A_1_)/2, T[{DELTA}(A,A_1)]dtime;arith.difffloate3_TdAA184.1 Percentile T[{DELTA}(A,A_1_)]dstat.errorfloate4_TdAA197.7 Percentile T[{DELTA}(A,A_1_)]dstat.errorfloatP(dAA1>0.4)Probability that the event will have {DELTA}(A,A_1_)>0.4mmagstat.fit.goodnessfloate1_dALI22.3 Percentile {DELTA}A_LI2_magstat.errorfloate2_dALI215.9 Percentile {DELTA}A_LI2_magstat.errorfloatdALI2Median {DELTA}A_LI2_magphot.mag;arith.difffloate3_dALI284.1 Percentile {DELTA}A_LI2_magstat.errorfloate4_dALI297.7 Percentile {DELTA}A_LI2_magstat.errorfloatP(dALI2>0.4)Probability that the event will have {DELTA}A_LI2_>0.4mmagstat.fit.goodnessfloate1_dmth22.3 Percentile {DELTA}({delta}_mic_,{theta}_2_)masstat.errorfloate2_dmth215.9 Percentile {DELTA}({delta}_mic_,{theta}_2_)masstat.errorfloatdmth2Median difference between the minimum and maximum astrometric shifts of an event over the time period adopted in this paper {DELTA}({delta}_mic_,{theta}_2_)masstat.fit.paramfloate3_dmth284.1 Percentile {DELTA}({delta}_mic_,{theta}_2_)masstat.errorfloate4_dmth297.7 Percentile {DELTA}({delta}_mic_,{theta}_2_)masstat.errorfloate1_Tdmth22.3 Percentile T[{DELTA}({delta}_mic_,{theta}_2_)]dstat.errordoublee2_Tdmth215.9 Percentile T[{DELTA}({delta}_mic_,{theta}_2_)]dstat.errordoubleTdmth2Median amount of time that an event spends with its astrometric shift above min({delta}_mic_,{theta}_2_)+ {DELTA}({delta}_mic_,{theta}_2_)/2, T[{DELTA}({delta}_mic_,{theta}_2_)]dtime;arith.diffdoublee3_Tdmth284.1 Percentile T[{DELTA}({delta}_mic_,{theta}_2_)]dstat.errordoublee4_Tdmth297.7 Percentile T[{DELTA}({delta}_mic_,{theta}_2_)]dstat.errordoubleP(dmth2>0.131)Probability that the event will have {DELTA}({delta}_mic_,{theta}_2_) >0.131masstat.fit.goodnessfloate1_dthLI22.3 Percentile {DELTA}theta_LI2_masstat.errorfloate2_dthLI215.9 Percentile {DELTA}theta_LI2_masstat.errorfloatdthLI2Median {DELTA}theta_LI2_masstat.fit.paramfloate3_dthLI284.1 Percentile {DELTA}theta_LI2_masstat.errorfloate4_dthLI297.7 Percentile {DELTA}theta_LI2_masstat.errorfloatP(dthLI2>0.131)Probability that the event will have {DELTA}theta_LI2_>0.131masstat.fit.goodnessfloat_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.ranullableindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decnullableindexedt0Median t_0_ (Julian year)yrtime.epochdouble