Mira variables om ROTSE-IIId

We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TUBITAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. In these variables, 17 periods are identified for the first time

Cone search capability for table J/other/NewA/17.504/table1 (Mira variables with new periods from ROTSE-IIId)

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/other/NewA/17.504
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/NewA/17.504
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/NewA/17.504
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/other/NewA/17.504
Provenance
Creator Yesilyaprak C.; Yerli S.K.; Gucsav B.B.; Aksaker N.; Dikicioglu E.,Helvaci M.; Coker D.; Aydin M.E.; Dincel B.; Uzun N.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy