Catalog Service: SMC RR Lyrae stars light curve analysis
Description
We present a careful and detailed light curve analysis of RR Lyrae stars in the Small Magellanic Cloud (SMC) discovered by the Optical Gravitational Lensing Experiment (OGLE) project. Out of 536 single-mode RR Lyrae stars selected from the data base, we have investigated the physical properties of 335 'normal-looking' RRab stars and 17 RRc stars that have good quality photometric light curves. We have also been able to estimate the distance modulus of the cloud which is in good agreement with those determined from other independent methods.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2013 Aug 07 15:43:09ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This section describes the data's coverage over the sky, frequency, and time.
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/MNRAS/402/691/table2 (Fourier parameters for 58 overtone mode (RRc) SMC RR Lyr variables in the OGLE data base (I-band data))
VERB=1
VERB=3
Cone search capability for table J/MNRAS/402/691/table1 (Fourier parameters for 478 fundamental mode (RRab) SMC RR Lyr variables in the OGLE data base (I-band data))
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute