Contains the parameters provided in the MACHO Lightcurve Statistical Summary Table for each source in the SMC fields. 
This table contains brief descriptions of the parameters provided for each source in the catalogue of the SMC fields from MACHO. The table contains comprehensive summary statistics that are provided for each star's complete lightcurve, for each MACHO field in the SMC. Required constraints:

Name  Type  Length  Unit  Description  Default Value  Unified Content Descriptor 

id  varchar  24  MACHO star identification (field.tile.seq)  
seqNum  int  4  Sequential number (unique object ID)  
cx  float  8  unit vector of spherical coordinates  pos.distance;pos.cartesian.x  
cy  float  8  unit vector of spherical coordinates  pos.distance;pos.cartesian.y  
cz  float  8  unit vector of spherical coordinates  pos.distance;pos.cartesian.z  
htmID  bigint  8  Hierarchical Triangular Mesh (HTM) index, 20 deep, for equatorial coordinates  pos.eq  
ra  float  8  degrees  J2000 right ascension  pos.eq.ra;meta.main  
dec  float  8  degrees  J2000 declination  pos.eq.dec;meta.main  
npoints  smallint  2  number of observations on the MACHO tile containing this star  
rN  smallint  2  red: number of good points on Lightcurve (LC)  
rmagave  real  4  red: median magnitude of LC in instrumental units  
rerrave  real  4  red: average error of measurements on LC in units of A, where A is the the measured flux divided by the median flux.  
rsig  real  4  red: sqrt of variance of A1 measurements over LC.  
rchi2w  real  4  red: chi^2 per degree of freedom of fit to "constant flux" hypothesis weighted by flux errors  
rqw  real  4  red: probability of getting value as large as rchi2w by chance  
rNr  smallint  2  red: number of points on robustified LC  
rerraver  real  4  red: average error on robustified LC  
rchi2r  real  4  red: chi^2 per degree of freedom for robustified LC (variable star search)  
rqr  real  4  red: probability of getting value as large as rchi2r by chance  
rs5  int  4  red: number of points on LC 5sigma above median  
rs5d  int  4  red: number of points on LC 5sigma below median (eclipsing binary search)  
rmagaveu  real  4  red: median magnitude in instrumental units before removing bad points  
rdskyave  real  4  red: average of red dsky sodophot measure  
rdskysig  real  4  red: sqrt of variance of red dsky sodophot measure  
rpsfave  real  4  red: average over LC of sodophot measure of goodness of psf fit  
rpsfsig  real  4  red: sqrt of variance of red psf sodophot measure  
rcrdave  real  4  red: average of crowding sodophot measure  
rcosmave  real  4  red: average of cosmic ray sodophot measure  
rmissave  real  4  red: average of missing pixel sodophot measure  
bN  smallint  2  blue: number of good points on Lightcurve (LC)  
bmagave  real  4  blue: median magnitude of LC in instrumental units  
berrave  real  4  blue: average error of measurements on LC in units of A, where A is the the measured flux divided by the median flux.  
bsig  real  4  blue: sqrt of variance of A1 measurements over LC.  
bchi2w  real  4  blue: chi^2 per degree of freedom of fit to "constant flux" hypothesis weighted by flux errors  
bqw  real  4  blue: probability of getting value as large as rchi2w by chance  
bNr  int  4  blue: number of points on robustified LC  
berraver  real  4  blue: average error on robustified LC  
bchi2r  real  4  blue: chi^2 per degree of freedom for robustified LC (variable star search)  
bqr  real  4  blue: probability of getting value as large as rchi2r by chance  
bs5  int  4  blue: number of points on LC 5sigma above median  
bs5d  int  4  blue: number of points on LC 5sigma below median (eclipsing binary search)  
bmagaveu  real  4  blue: median magnitude in instrumental units before removing bad points  
bdskyave  real  4  blue: average of blue dsky sodophot measure  
bdskysig  real  4  blue: sqrt of variance of blue dsky sodophot measure  
bpsfave  real  4  blue: average over LC of sodophot measure of goodness of psf fit  
bpsfsig  real  4  blue: sqrt of variance of blue psf sodophot measure  
bcrdave  real  4  blue: average of crowding sodophot measure  
bcosmave  real  4  blue: average of cosmic ray sodophot measure  
bmissave  real  4  blue: average of missing pixel sodophot measure  
bmrN  smallint  2  number of points on the BR LC [aka simultaneous R/B pts]  
bmrsig  real  4  sqrt of variance of BR LC  
bmrchi2w  real  4  chi^2 per degree of freedom for BR LC  
bmrave  real  4  average of BR  
bmrprobspear  real  4  BR ?  
rbcross  real  4  red/blue A1 robustified measurements over LC cross correlation coefficient [WelchStetson; see AJ 105, 1813]  
rauto  real  4  red: A1 robustified measurements over LC autocorrelation (lag=0) coefficient  
bauto  real  4  blue: A1 robustified measurements over LC autocorrelation (lag=0) coefficient  
filterN  smallint  2  number of filters applied; always 3  
filter1_rfilmax  real  4  Filter 1, red: max value of optimum filter for LC  
filter1_rfiltime  real  4  Filter 1, red: LC time at which maximum occurred  
filter1_rNhi  smallint  2  Filter 1, red: number points sigmathreshold high within duration of filter at peak (rfiltime)  
filter1_bfilmax  real  4  Filter 1, blue: max value of optimum filter for LC  
filter1_bfiltime  real  4  Filter 1, blue: LC time at which maximum occurred  
filter1_bNhi  smallint  2  Filter 1, blue: number points sigmathreshold high within duration of filter at peak (bfiltime)  
filter2_rfilmax  real  4  Filter 2, red: max value of optimum filter for LC  
filter2_rfiltime  real  4  Filter 2, red: LC time at which maximum occurred  
filter2_rNhi  smallint  2  Filter 2, red: number points sigmathreshold high within duration of filter at peak (rfiltime)  
filter2_bfilmax  real  4  Filter 2, blue: max value of optimum filter for LC  
filter2_bfiltime  real  4  Filter 2, blue: LC time at which maximum occurred  
filter2_bNhi  smallint  2  Filter 2, blue: number points sigmathreshold high within duration of filter at peak (bfiltime)  
filter3_rfilmax  real  4  Filter 3, red: max value of optimum filter for LC  
filter3_rfiltime  real  4  Filter 3, red: LC time at which maximum occurred  
filter3_rNhi  smallint  2  Filter 3, red: number points sigmathreshold high within duration of filter at peak (rfiltime)  
filter3_bfilmax  real  4  Filter 3, blue: max value of optimum filter for LC  
filter3_bfiltime  real  4  Filter 3, blue: LC time at which maximum occurred  
filter3_bNhi  smallint  2  Filter 3, blue: number points sigmathreshold high within duration of filter at peak (bfiltime)  
Total length  324 