TABLE  userv1802VarFrameSetInfo

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 userv1802MergeLog(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 
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 length94