Multi-wavelength photometric variation of PG1605+072

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dc.creatorSchuh, S.
dc.creatorDreizler, S.
dc.creatorHeber, U.
dc.creatorJeffery, C. S.
dc.creatorO'Toole, S. J.
dc.creatorCordes, O.
dc.creatorStahn, T.
dc.creatorLutz, R.
dc.creatorTillich, A.
dc.creatorWET, the
dc.creatorcollaborations, MSST
dc.date2008-12-28
dc.date.accessioned2026-07-07T12:22:59Z
dc.date.available2026-07-07T12:22:59Z
dc.descriptionIn a large coordinated attempt to further our understanding of the $p$-mode pulsating sdB star PG1605+072, the Multi-Site Spectroscopic Telescope (MSST) collaboration has obtained simultaneous time-resolved spectroscopic and photometric observations. The photometry was extended by additional WET data which increased the time base. This contribution outlines the analysis of the MSST photometric light curve, including the four-colour BUSCA data from which chromatic amplitudes have been derived, as well as supplementary FUV spectra and light curves from two different epochs. These results have the potential to complement the interpretation of the published spectroscopic information.
dc.description6 pages, to be published in "Interpretation of asteroseismic data", proceedings of the HELAS NA5 Workshop, eds. W. Dziembowski, M. Breger and M. Thompson, Communications in Asteroseismology, 157
dc.identifierhttps://arxiv.org/abs/0812.4857
dc.identifierhttp://arxiv.org/abs/0812.4857
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213839
dc.subjectAstrophysics
dc.titleMulti-wavelength photometric variation of PG1605+072
dc.typetext

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