Arşiv logosu
  • Türkçe
  • English
  • Giriş
    Yeni kullanıcı mısınız? Kayıt için tıklayın. Şifrenizi mi unuttunuz?
Arşiv logosu
  • Koleksiyonlar
  • Sistem İçeriği
  • Analiz
  • Talep/Soru
  • Türkçe
  • English
  • Giriş
    Yeni kullanıcı mısınız? Kayıt için tıklayın. Şifrenizi mi unuttunuz?
  1. Ana Sayfa
  2. Yazara Göre Listele

Yazar "O'Toole, S" seçeneğine göre listele

Listeleniyor 1 - 2 / 2
Sayfa Başına Sonuç
Sıralama seçenekleri
  • Küçük Resim Yok
    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, G
    The 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.
  • Küçük Resim Yok
    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, G
    The 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.

| Ege Üniversitesi | Kütüphane | Açık Erişim Politikası | Rehber | OAI-PMH |

Bu site Creative Commons Alıntı-Gayri Ticari-Türetilemez 4.0 Uluslararası Lisansı ile korunmaktadır.


Ege Üniversitesi Rektörlüğü Gençlik Caddesi No : 12 35040 Bornova - İZMİR, TÜRKİYE
İçerikte herhangi bir hata görürseniz lütfen bize bildirin

DSpace 7.6.1, Powered by İdeal DSpace

DSpace yazılımı telif hakkı © 2002-2025 LYRASIS

  • Çerez Ayarları
  • Gizlilik Politikası
  • Son Kullanıcı Sözleşmesi
  • Geri Bildirim