TABLE  videoVarFrameSetInfo

Contains fitting information for each frameSet.

Strateva et al. fits and expected magnitude limit for each filter

Required constraints:
  • Primary key is (frameSetID)
  • (frameSetID) references videoMergeLog(frameSetID)

NameTypeLengthUnitDescriptionDefault ValueUnified Content Descriptor
frameSetID link to glossarybigint8 frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure meta.id;obs.field
cuEventIDint4 UID of curation event giving rise to this record meta.bib
motionModel link to glossaryvarchar32 Motion model used to produce BestMatch table. Values: static;proper motion;proper motion and parallax.staticmeta.code.class
zaStratAst link to glossaryreal4 Strateva parameter, a, in fit to astrometric rms vs magnitude in Z band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.opt.I
zbStratAst link to glossaryreal4 Strateva parameter, b, in fit to astrometric rms vs magnitude in Z band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.opt.I
zcStratAst link to glossaryreal4 Strateva parameter, c, in fit to astrometric rms vs magnitude in Z band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.opt.I
zchiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in Z band-0.9999995e9stat.fit.goodness;em.opt.I
znDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in Z band.-9999stat.fit.dof;stat.param;em.opt.I
zisDefAsttinyint1 Use a default model for the astrometric noise in Z band.0meta.code;em.opt.I
zaStratPht link to glossaryreal4 Strateva parameter, a, in fit to photometric rms vs magnitude in Z band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.opt.I
zbStratPht link to glossaryreal4 Strateva parameter, b, in fit to photometric rms vs magnitude in Z band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.opt.I
zcStratPht link to glossaryreal4 Strateva parameter, c, in fit to photometric rms vs magnitude in Z band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.opt.I
zchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in Z band-0.9999995e9stat.fit.goodness;em.opt.I
znDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in Z band.-9999stat.fit.dof;stat.param;em.opt.I
zisDefPhttinyint1 Use a default model for the photometric noise in Z band.0meta.code;em.opt.I
zexpMLreal4magExpected magnitude limit of frameSet in this in Z band.-0.9999995e9phot.mag;em.opt.I;stat.max
yaStratAst link to glossaryreal4 Strateva parameter, a, in fit to astrometric rms vs magnitude in Y band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.NIR
ybStratAst link to glossaryreal4 Strateva parameter, b, in fit to astrometric rms vs magnitude in Y band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.NIR
ycStratAst link to glossaryreal4 Strateva parameter, c, in fit to astrometric rms vs magnitude in Y band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.NIR
ychiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in Y band-0.9999995e9stat.fit.goodness;em.IR.NIR
ynDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in Y band.-9999stat.fit.dof;stat.param;em.IR.NIR
yisDefAsttinyint1 Use a default model for the astrometric noise in Y band.0meta.code;em.IR.NIR
yaStratPht link to glossaryreal4 Strateva parameter, a, in fit to photometric rms vs magnitude in Y band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.NIR
ybStratPht link to glossaryreal4 Strateva parameter, b, in fit to photometric rms vs magnitude in Y band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.NIR
ycStratPht link to glossaryreal4 Strateva parameter, c, in fit to photometric rms vs magnitude in Y band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.NIR
ychiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in Y band-0.9999995e9stat.fit.goodness;em.IR.NIR
ynDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in Y band.-9999stat.fit.dof;stat.param;em.IR.NIR
yisDefPhttinyint1 Use a default model for the photometric noise in Y band.0meta.code;em.IR.NIR
yexpMLreal4magExpected magnitude limit of frameSet in this in Y band.-0.9999995e9phot.mag;em.IR.NIR;stat.max
jaStratAst link to glossaryreal4 Strateva parameter, a, in fit to astrometric rms vs magnitude in J band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.J
jbStratAst link to glossaryreal4 Strateva parameter, b, in fit to astrometric rms vs magnitude in J band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.J
jcStratAst link to glossaryreal4 Strateva parameter, c, in fit to astrometric rms vs magnitude in J band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.J
jchiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in J band-0.9999995e9stat.fit.goodness;em.IR.J
jnDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in J band.-9999stat.fit.dof;stat.param;em.IR.J
jisDefAsttinyint1 Use a default model for the astrometric noise in J band.0meta.code;em.IR.J
jaStratPht link to glossaryreal4 Strateva parameter, a, in fit to photometric rms vs magnitude in J band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.J
jbStratPht link to glossaryreal4 Strateva parameter, b, in fit to photometric rms vs magnitude in J band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.J
jcStratPht link to glossaryreal4 Strateva parameter, c, in fit to photometric rms vs magnitude in J band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.J
jchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in J band-0.9999995e9stat.fit.goodness;em.IR.J
jnDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in J band.-9999stat.fit.dof;stat.param;em.IR.J
jisDefPhttinyint1 Use a default model for the photometric noise in J band.0meta.code;em.IR.J
jexpMLreal4magExpected magnitude limit of frameSet in this in J band.-0.9999995e9phot.mag;em.IR.J;stat.max
haStratAst link to glossaryreal4 Strateva parameter, a, in fit to astrometric rms vs magnitude in H band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.H
hbStratAst link to glossaryreal4 Strateva parameter, b, in fit to astrometric rms vs magnitude in H band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.H
hcStratAst link to glossaryreal4 Strateva parameter, c, in fit to astrometric rms vs magnitude in H band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.H
hchiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in H band-0.9999995e9stat.fit.goodness;em.IR.H
hnDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in H band.-9999stat.fit.dof;stat.param;em.IR.H
hisDefAsttinyint1 Use a default model for the astrometric noise in H band.0meta.code;em.IR.H
haStratPht link to glossaryreal4 Strateva parameter, a, in fit to photometric rms vs magnitude in H band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.H
hbStratPht link to glossaryreal4 Strateva parameter, b, in fit to photometric rms vs magnitude in H band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.H
hcStratPht link to glossaryreal4 Strateva parameter, c, in fit to photometric rms vs magnitude in H band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.H
hchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in H band-0.9999995e9stat.fit.goodness;em.IR.H
hnDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in H band.-9999stat.fit.dof;stat.param;em.IR.H
hisDefPhttinyint1 Use a default model for the photometric noise in H band.0meta.code;em.IR.H
hexpMLreal4magExpected magnitude limit of frameSet in this in H band.-0.9999995e9phot.mag;em.IR.H;stat.max
ksaStratAst link to glossaryreal4 Strateva parameter, a, in fit to astrometric rms vs magnitude in Ks band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.K
ksbStratAst link to glossaryreal4 Strateva parameter, b, in fit to astrometric rms vs magnitude in Ks band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.K
kscStratAst link to glossaryreal4 Strateva parameter, c, in fit to astrometric rms vs magnitude in Ks band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.K
kschiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in Ks band-0.9999995e9stat.fit.goodness;em.IR.K
ksnDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in Ks band.-9999stat.fit.dof;stat.param;em.IR.K
ksisDefAsttinyint1 Use a default model for the astrometric noise in Ks band.0meta.code;em.IR.K
ksaStratPht link to glossaryreal4 Strateva parameter, a, in fit to photometric rms vs magnitude in Ks band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.K
ksbStratPht link to glossaryreal4 Strateva parameter, b, in fit to photometric rms vs magnitude in Ks band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.K
kscStratPht link to glossaryreal4 Strateva parameter, c, in fit to photometric rms vs magnitude in Ks band, see Sesar et al. 2007.-0.9999995e9stat.fit.param;em.IR.K
kschiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in Ks band-0.9999995e9stat.fit.goodness;em.IR.K
ksnDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in Ks band.-9999stat.fit.dof;stat.param;em.IR.K
ksisDefPhttinyint1 Use a default model for the photometric noise in Ks band.0meta.code;em.IR.K
ksexpMLreal4magExpected magnitude limit of frameSet in this in Ks band.-0.9999995e9phot.mag;em.IR.K;stat.max
Total length254