First Results of the 17th DSN Campaign: Photometry of XX Pyx

We present the first results from multi-site observations of the δ Scuti star XX Pyx (CD–24°7599). The observations were carried out as the 17th run of the Delta Scuti Network. We collected 583 hr of B , V time-series photometry, resulting in a detection level (4 σ ) in the amplitude spectrum of 0.5...

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Veröffentlicht in:International Astronomical Union Colloquium 2000, Vol.176, p.469-470
Hauptverfasser: Arentoft, T., Handle, G., Shobbrook, R. R., Wood, M. A., Crause, L., Crake, P., Podmore, F., Habanyama, A., Oswalt, T., Birch, P. V., Lowe, G., Sterken, C., Meintjes, P., Brink, J., Claver, C. F., Medupe, R., Guzik, J. A., Beach, T. E., Martinez, P., Leibowitz, E. M., Ibbetson, P. A., Smith, T., Ashoka, B. N., Raj, N. E., Kurtz, D. W., Balona, L. A., Costa, J. E. S., Breger, M.
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Sprache:eng
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Zusammenfassung:We present the first results from multi-site observations of the δ Scuti star XX Pyx (CD–24°7599). The observations were carried out as the 17th run of the Delta Scuti Network. We collected 583 hr of B , V time-series photometry, resulting in a detection level (4 σ ) in the amplitude spectrum of 0.5 mmag. We detect 6 new pulsation frequencies, bringing the total number of frequencies known in this star up 19.
ISSN:0252-9211
DOI:10.1017/S0252921100058474