Schuh, SLHeber, UDreizler, SO'Toole, SJeffery, CSFalter, SWoolf, VMRiddle, RLHandler, GHurkal, OPakstiene, EKlumpe, EWLaurance, TVuckovic, MZola, SKawaler, SDKanaan, AMonteiro, HGiovannini, OKepler, SOMukadam, AProvencal, JLNitta, AShipman, HMullally, FGrauer, AWood, MABradley, PAKilic, MSekiguchi, KCrowe, RSullivan, DJRosen, RClemens, CXiaojun, JJanulis, RO'Donoghue, DOgloza, WBaran, ASilvotti, RMarinoni, SVauclair, GDolez, NChevreton, MDeetjen, JLNagel, TPerez, JMGSolheim, JEOstensen, RUlla, ABurleigh, MGood, SMetcalfe, TSda Costa, AFMCosta, JESO'Brien, MSKim, SLLee, HSergeev, AAkan, CCakirli, OPaparo, MViraghalmy, G2019-10-272019-10-2720031392-00491392-0049https://hdl.handle.net/11454/379796th Whole Earth Telescope Workshop (WET) -- JUN 20-21, 2002 -- NAPLES, ITALYThe 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.eninfo:eu-repo/semantics/openAccessstars : interiorsstars : individual : PG 1605+072Article1215570WOS:000184698800009N/AN/A