OGLE Variables in Magellanic Clouds (Ita+, 2004)

Details OGLE Variables in Magellanic Clouds (Ita+, 2004) OGLE Variables in Magellanic Clouds (Ita+, 2004)

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..73530705i&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/353/705. Originally published in: 2004MNRAS.353..705I

Physics

Magellanic Clouds, Stars: Variable, Photometry: Infrared

Scientific paper

We cross-identified OGLE variables in the Magellanic Clouds (Zebrun et al., 2001AcA....51..317Z) with the SIRIUS NIR sources that have been detected in at least two of the three (JHKs) wavebands, and then determined their pulsation periods by using the phase dispersion minimization (PDM) technique (Stellingwerf, 1978ApJ...224..953S). Details of the cross-identifications and period findings are described in Paper I (Ita et al., 2004MNRAS.347..720I).
(2 data files).

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