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Öğe PG 1605+072 in WET XCoV22: Support for the multi site spectroscopic telescope(Inst Theoretical Physics Astronomy, 2003) Schuh, SL; Heber, U; Dreizler, S; O'Toole, S; Jeffery, CS; Falter, S; Woolf, VM; Riddle, RL; Handler, G; Hurkal, O; Pakstiene, E; Klumpe, EW; Laurance, T; Vuckovic, M; Zola, S; Kawaler, SD; Kanaan, A; Monteiro, H; Giovannini, O; Kepler, SO; Mukadam, A; Provencal, JL; Nitta, A; Shipman, H; Mullally, F; Grauer, A; Wood, MA; Bradley, PA; Kilic, M; Sekiguchi, K; Crowe, R; Sullivan, DJ; Rosen, R; Clemens, C; Xiaojun, J; Janulis, R; O'Donoghue, D; Ogloza, W; Baran, A; Silvotti, R; Marinoni, S; Vauclair, G; Dolez, N; Chevreton, M; Deetjen, JL; Nagel, T; Perez, JMG; Solheim, JE; Ostensen, R; Ulla, A; Burleigh, M; Good, S; Metcalfe, TS; da Costa, AFM; Costa, JES; O'Brien, MS; Kim, SL; Lee, H; Sergeev, A; Akan, C; Cakirli, O; Paparo, M; Viraghalmy, GThe Multi-site spectroscopic telescope is a virtual instrument and the name of a collaboration that opens up a new observational window by combining continuous observations of spectroscopic variations and simultaneous photometric monitoring. This constitutes an enormous observational effort, but in return promises to finally provide access to a mode identification for and an asteroseismological analysis of the pulsating sdB star PG 1605+072. Multi-Site Spectroscopic Telescope observations for this object have been secured during a large coordinated campaign in May and June of the year 2002. The frequency resolution and coverage of the photometric time series has been noticeably enhanced by a significant contribution from the Whole Earth Telescope, which was used to observe PG 1605+072 as an alternate target during the WET XCov22 campaign, also conducted in May 2002. This paper briefly outlines the motivation for the MSST project and tries to give a first assessment of the overall quality of the data obtained, with a focus on the Whole Earth Telescope observations.Öğe PG 1605+072 in WET XCoV22: Support for the multi site spectroscopic telescope(Inst Theoretical Physics Astronomy, 2003) Schuh, SL; Heber, U; Dreizler, S; O'Toole, S; Jeffery, CS; Falter, S; Woolf, VM; Riddle, RL; Handler, G; Hurkal, O; Pakstiene, E; Klumpe, EW; Laurance, T; Vuckovic, M; Zola, S; Kawaler, SD; Kanaan, A; Monteiro, H; Giovannini, O; Kepler, SO; Mukadam, A; Provencal, JL; Nitta, A; Shipman, H; Mullally, F; Grauer, A; Wood, MA; Bradley, PA; Kilic, M; Sekiguchi, K; Crowe, R; Sullivan, DJ; Rosen, R; Clemens, C; Xiaojun, J; Janulis, R; O'Donoghue, D; Ogloza, W; Baran, A; Silvotti, R; Marinoni, S; Vauclair, G; Dolez, N; Chevreton, M; Deetjen, JL; Nagel, T; Perez, JMG; Solheim, JE; Ostensen, R; Ulla, A; Burleigh, M; Good, S; Metcalfe, TS; da Costa, AFM; Costa, JES; O'Brien, MS; Kim, SL; Lee, H; Sergeev, A; Akan, C; Cakirli, O; Paparo, M; Viraghalmy, GThe Multi-site spectroscopic telescope is a virtual instrument and the name of a collaboration that opens up a new observational window by combining continuous observations of spectroscopic variations and simultaneous photometric monitoring. This constitutes an enormous observational effort, but in return promises to finally provide access to a mode identification for and an asteroseismological analysis of the pulsating sdB star PG 1605+072. Multi-Site Spectroscopic Telescope observations for this object have been secured during a large coordinated campaign in May and June of the year 2002. The frequency resolution and coverage of the photometric time series has been noticeably enhanced by a significant contribution from the Whole Earth Telescope, which was used to observe PG 1605+072 as an alternate target during the WET XCov22 campaign, also conducted in May 2002. This paper briefly outlines the motivation for the MSST project and tries to give a first assessment of the overall quality of the data obtained, with a focus on the Whole Earth Telescope observations.