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:
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Name | Type | Length | Unit | Description | Default Value | Unified Content Descriptor |
---|---|---|---|---|---|---|
frameSetID ![]() | bigint | 8 | frame set ID, unique over the whole WSA via programme ID prefix, assigned by merging procedure | ID_FIELD | ||
cuEventID | int | 4 | UID of curation event giving rise to this record | REFER_CODE | ||
motionModel ![]() | varchar | 32 | Motion model used to produce BestMatch table. Values: static;proper motion;proper motion and parallax. | static | ||
jaStratAst ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jbStratAst ![]() | real | 4 | Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jcStratAst ![]() | real | 4 | Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jdStratAst ![]() | real | 4 | Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jchiSqAst ![]() | real | 4 | Goodness of fit of Strateva function to astrometric data in J band | -0.9999995e9 | stat.fit.goodness;em.IR.J | |
jnDofAst ![]() | smallint | 2 | Number of degrees of freedom of astrometric fit in J band. | -9999 | stat.fit.dof;stat.param;em.IR.J | |
jisDefAst | tinyint | 1 | Use a default model for the astrometric noise in J band. | 0 | meta.code;em.IR.J | |
jaStratPht ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jbStratPht ![]() | real | 4 | Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jcStratPht ![]() | real | 4 | Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jdStratPht ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in J band. | -0.9999995e9 | stat.fit.param;em.IR.J | |
jchiSqPht ![]() | real | 4 | Goodness of fit of Strateva function to photometric data in J band | -0.9999995e9 | ||
jnDofPht ![]() | smallint | 2 | Number of degrees of freedom of photometric fit in J band. | -9999 | ||
jisDefPht | tinyint | 1 | Use a default model for the photometric noise in J band. | 0 | ||
jexpML ![]() | real | 4 | Expected magnitude limit of frameSet in this in J band. | -0.9999995e9 | ||
haStratAst ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hbStratAst ![]() | real | 4 | Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hcStratAst ![]() | real | 4 | Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hdStratAst ![]() | real | 4 | Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hchiSqAst ![]() | real | 4 | Goodness of fit of Strateva function to astrometric data in H band | -0.9999995e9 | stat.fit.goodness;em.IR.H | |
hnDofAst ![]() | smallint | 2 | Number of degrees of freedom of astrometric fit in H band. | -9999 | stat.fit.dof;stat.param;em.IR.H | |
hisDefAst | tinyint | 1 | Use a default model for the astrometric noise in H band. | 0 | meta.code;em.IR.H | |
haStratPht ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hbStratPht ![]() | real | 4 | Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hcStratPht ![]() | real | 4 | Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hdStratPht ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in H band. | -0.9999995e9 | stat.fit.param;em.IR.H | |
hchiSqPht ![]() | real | 4 | Goodness of fit of Strateva function to photometric data in H band | -0.9999995e9 | ||
hnDofPht ![]() | smallint | 2 | Number of degrees of freedom of photometric fit in H band. | -9999 | ||
hisDefPht | tinyint | 1 | Use a default model for the photometric noise in H band. | 0 | ||
hexpML ![]() | real | 4 | Expected magnitude limit of frameSet in this in H band. | -0.9999995e9 | ||
kaStratAst ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kbStratAst ![]() | real | 4 | Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kcStratAst ![]() | real | 4 | Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kdStratAst ![]() | real | 4 | Parameter, c3 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kchiSqAst ![]() | real | 4 | Goodness of fit of Strateva function to astrometric data in K band | -0.9999995e9 | stat.fit.goodness;em.IR.K | |
knDofAst ![]() | smallint | 2 | Number of degrees of freedom of astrometric fit in K band. | -9999 | stat.fit.dof;stat.param;em.IR.K | |
kisDefAst | tinyint | 1 | Use a default model for the astrometric noise in K band. | 0 | meta.code;em.IR.K | |
kaStratPht ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kbStratPht ![]() | real | 4 | Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kcStratPht ![]() | real | 4 | Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kdStratPht ![]() | real | 4 | Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in K band. | -0.9999995e9 | stat.fit.param;em.IR.K | |
kchiSqPht ![]() | real | 4 | Goodness of fit of Strateva function to photometric data in K band | -0.9999995e9 | ||
knDofPht ![]() | smallint | 2 | Number of degrees of freedom of photometric fit in K band. | -9999 | ||
kisDefPht | tinyint | 1 | Use a default model for the photometric noise in K band. | 0 | ||
kexpML ![]() | real | 4 | Expected magnitude limit of frameSet in this in K band. | -0.9999995e9 | ||
Total length | 194 |