TABLE  u15bua19VarFrameSetInfo

Contains photometric and astrometric noise fitting information for each frameSet.

Strateva et al. 2001, AJ, 122, 1861 fits to the photometric and
astrometric RMS for non-variable stars and expected magnitude limits for
each pointing and filter.

Required constraints:
  • Primary key is (frameSetID)
  • (frameSetID) references u15bua19MergeLog(frameSetID)

NameTypeLengthUnitDescriptionDefault ValueUnified Content Descriptor
frameSetID link to glossarybigint8 frame set ID, unique over the whole WSA via programme ID prefix, assigned by merging procedure ID_FIELD
cuEventIDint4 UID of curation event giving rise to this record REFER_CODE
motionModel link to glossaryvarchar32 Motion model used to produce BestMatch table. Values: static;proper motion;proper motion and parallax.static 
zaStratAst link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zbStratAst link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zcStratAst link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zdStratAst link to glossaryreal4 Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Z band.-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 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zbStratPht link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zcStratPht link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zdStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Z band.-0.9999995e9stat.fit.param;em.opt.I
zchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in Z band-0.9999995e9 
znDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in Z band.-9999 
zisDefPhttinyint1 Use a default model for the photometric noise in Z band.0 
zexpML link to glossaryreal4 Expected magnitude limit of frameSet in this in Z band.-0.9999995e9 
yaStratAst link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ybStratAst link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ycStratAst link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ydStratAst link to glossaryreal4 Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Y band.-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 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ybStratPht link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ycStratPht link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ydStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Y band.-0.9999995e9stat.fit.param;em.IR.NIR
ychiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in Y band-0.9999995e9 
ynDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in Y band.-9999 
yisDefPhttinyint1 Use a default model for the photometric noise in Y band.0 
yexpML link to glossaryreal4 Expected magnitude limit of frameSet in this in Y band.-0.9999995e9 
jaStratAst link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jbStratAst link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jcStratAst link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jdStratAst link to glossaryreal4 Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band.-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 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jbStratPht link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jcStratPht link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jdStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band.-0.9999995e9stat.fit.param;em.IR.J
jchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in J band-0.9999995e9 
jnDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in J band.-9999 
jisDefPhttinyint1 Use a default model for the photometric noise in J band.0 
jexpML link to glossaryreal4 Expected magnitude limit of frameSet in this in J band.-0.9999995e9 
haStratAst link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hbStratAst link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hcStratAst link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hdStratAst link to glossaryreal4 Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band.-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 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hbStratPht link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hcStratPht link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hdStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band.-0.9999995e9stat.fit.param;em.IR.H
hchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in H band-0.9999995e9 
hnDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in H band.-9999 
hisDefPhttinyint1 Use a default model for the photometric noise in H band.0 
hexpML link to glossaryreal4 Expected magnitude limit of frameSet in this in H band.-0.9999995e9 
kaStratAst link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kbStratAst link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kcStratAst link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kdStratAst link to glossaryreal4 Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kchiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in K band-0.9999995e9stat.fit.goodness;em.IR.K
knDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in K band.-9999stat.fit.dof;stat.param;em.IR.K
kisDefAsttinyint1 Use a default model for the astrometric noise in K band.0meta.code;em.IR.K
kaStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kbStratPht link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kcStratPht link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kdStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band.-0.9999995e9stat.fit.param;em.IR.K
kchiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in K band-0.9999995e9 
knDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in K band.-9999 
kisDefPhttinyint1 Use a default model for the photometric noise in K band.0 
kexpML link to glossaryreal4 Expected magnitude limit of frameSet in this in K band.-0.9999995e9 
h2aStratAst link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2bStratAst link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2cStratAst link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2dStratAst link to glossaryreal4 Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2chiSqAst link to glossaryreal4 Goodness of fit of Strateva function to astrometric data in H2 band-0.9999995e9stat.fit.goodness
h2nDofAst link to glossarysmallint2 Number of degrees of freedom of astrometric fit in H2 band.-9999stat.fit.dof;stat.param
h2isDefAsttinyint1 Use a default model for the astrometric noise in H2 band.0meta.code
h2aStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2bStratPht link to glossaryreal4 Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2cStratPht link to glossaryreal4 Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2dStratPht link to glossaryreal4 Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H2 band.-0.9999995e9stat.fit.param
h2chiSqPht link to glossaryreal4 Goodness of fit of Strateva function to photometric data in H2 band-0.9999995e9 
h2nDofPht link to glossarysmallint2 Number of degrees of freedom of photometric fit in H2 band.-9999 
h2isDefPhttinyint1 Use a default model for the photometric noise in H2 band.0 
h2expML link to glossaryreal4 Expected magnitude limit of frameSet in this in H2 band.-0.9999995e9 
Total length344