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:
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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 co-ordinates | pos.distance;pos.cartesian.x | ||
cy | float | 8 | unit vector of spherical co-ordinates | pos.distance;pos.cartesian.y | ||
cz | float | 8 | unit vector of spherical co-ordinates | pos.distance;pos.cartesian.z | ||
htmID | bigint | 8 | Hierarchical Triangular Mesh (HTM) index, 20 deep, for equatorial co-ordinates | 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 A-1 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 5-sigma above median | |||
rs5d | int | 4 | red: number of points on LC 5-sigma 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 A-1 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 5-sigma above median | |||
bs5d | int | 4 | blue: number of points on LC 5-sigma 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 B-R LC [aka simultaneous R/B pts] | |||
bmrsig | real | 4 | sqrt of variance of B-R LC | |||
bmrchi2w | real | 4 | chi^2 per degree of freedom for B-R LC | |||
bmrave | real | 4 | average of B-R | |||
bmrprobspear | real | 4 | B-R ? | |||
rbcross | real | 4 | red/blue A-1 robustified measurements over LC cross correlation coefficient [Welch-Stetson; see AJ 105, 1813] | |||
rauto | real | 4 | red: A-1 robustified measurements over LC autocorrelation (lag=0) coefficient | |||
bauto | real | 4 | blue: A-1 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 |