For a list of all services and tables belonging to this service's resource, see Information on resource 'OGLE Time series'
The original OCVS data are provided as a set of tables with stellar parameters, split by variable-star class and sky field. Indeed, different variability classes have different sets of parameters. We preserve the division by variability class, but aggregate stars of a given class from all fields into unified tables with corresponding names, such as cepheids for Classical Cepheids or eclipsing for Eclipsing Binaries and so on. This allows more precise, variability-class–specific queries.
All observed objects, together with their basic parameters, are aggregated in the object_all table, which facilitates generic queries across all classes. This table is served via Cone Search.
The ts_ssa table is the main table for light-curve queries. It is served by TAP and SSA services. The time series themselves, as well as previews of folded and unfolded light curves, can be accessed via DataLink from the ts_ssa and ObsCore tables. Direct links to previews of folded curves are placed in the preview column of both the ts_ssa and ObsCore tables.
Download all RR Lyrae light curves with period in [0.5–0.7 days] range in the I band:
SELECT ssa_targname, accref, o.period FROM ogle.ts_ssa AS t JOIN ogle.rrlyr AS o ON t.ssa_targname = o.object_id WHERE o.period BETWEEN 0.5 AND 0.7 AND t.ssa_bandpass = 'I'
Download all previews of the light curves with epochs (time of maximum brightness) in the future:
SELECT * from ogle.objects_all WHERE epoch > ivo_to_mjd('2027-01-01')
Find all stars with periods longer than the duration of observations in I filter:
SELECT o.* FROM ogle.objects_all o JOIN ogle.ts_ssa t ON o.object_id = t.ssa_targname AND t.ssa_bandpass='I' WHERE o.period > ssa_timeext
Select ten eclipsing binary systems, classified as "Contact" with the longest periods:
SELECT TOP 10 accref, preview, o.* FROM ogle.eclipsing o JOIN ogle.ts_ssa t ON o.object_id = t.ssa_targname WHERE subtype='C' and ssa_length>100 ORDER BY o.period DESC
You can access this service using:
Intervals of messenger energies reflected in this resource: 1.12713 2.55638 eV
Time covered by this resource's data: 1995.77 2024.42
This resource is not (directly) published. This can mean that it was deemed too unimportant, for internal use only, or is just a helper for a published service. Equally likely, however, it is under development, abandoned in development or otherwise unfinished. Exercise some caution.
Other services provided on the underlying data include:
The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| obs_id | Obs. Id | Observation id (a combination of an object id and a passband) to create the preview for. | N/A | N/A |
| bibcode: | 2015AcA....65....1U (OGLE-IV photometry) |
|---|---|
| bibcode: | 2008AcA....58...69U (OGLE-III photometry) |
VOResource XML (that's something exclusively for VO nerds)