Search Results - "Iwert, O."

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    ESPRESSO@VLT -- On-sky performance and first results by Pepe, F, Cristiani, S, Rebolo, R, Santos, N. C, Dekker, H, Cabral, A, Di Marcantonio, P, Figueira, P, Curto, G. Lo, Lovis, C, Mayor, M, Mégevand, D, Molaro, P, Riva, M, Osorio, M. R. Zapatero, Amate, M, Manescau, A, Pasquini, L, Zerbi, F. M, Adibekyan, V, Abreu, M, Affolter, M, Alibert, Y, Aliverti, M, Allart, R, Prieto, C. Allende, Álvarez, D, Alves, D, Avila, G, Baldini, V, Bandy, T, Barros, S. C. C, Benz, W, Bianco, A, Borsa, F, Bourrier, V, Bouchy, F, Broeg, C, Calderone, G, Cirami, R, Coelho, J, Conconi, P, Coretti, I, Cumani, C, Cupani, G, D'Odorico, V, Damasso, M, Deiries, S, Delabre, B, Demangeon, O. D. S, Dumusque, X, Ehrenreich, D, Faria, J. P, Fragoso, A, Genolet, L, Genoni, M, Santos, R. Génova, Hernández, J. I. González, Hughes, I, Iwert, O, Kerber, F, Knudstrup, J, Landoni, M, Lavie, B, Lillo-Box, J, Lizon, J. -L, Maire, C, Martins, C. J . A. P, Mehner, A, Micela, G, Modigliani, A, Monteiro, M. A, Monteiro, M. J. P. F. G, Moschetti, M, Murphy, M. T, Nunes, N, Oggioni, L, Oliveira, A, Oshagh, M, Pallé, E, Pariani, G, Poretti, E, Rasilla, J. L, Rebordão, J, Redaelli, E. M, Tschudi, S. Santana, Santin, P, Santos, P, Ségransan, D, Schmidt, T. M, Segovia, A, Sosnowska, D, Sozzetti, A, Sousa, S. G, Spanò, P, Mascareño, A. Suárez, Tabernero, H, Tenegi, F, Udry, S, Zanutta, A

    Published 01-10-2020
    “…ESPRESSO is the new high-resolution spectrograph of ESO's Very-Large Telescope (VLT). It was designed for ultra-high radial-velocity precision and extreme…”
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    Journal Article
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    Characterization of the K2-38 planetary system. Unraveling one of the densest planets known to date by Toledo-Padrón, B, Lovis, C, Mascareño, A. Suárez, Barros, S. C. C, Hernández, J. I. González, Sozzetti, A, Bouchy, F, Osorio, M. R. Zapatero, Rebolo, R, Cristiani, S, Pepe, F. A, Santos, N. C, Sousa, S. G, Tabernero, H. M, Lillo-Box, J, Bossini, D, Adibekyan, V, Allart, R, Damasso, M, D'Odorico, V, Figueira, P, Lavie, B, Curto, G. Lo, Mehner, A, Micela, G, Modigliani, A, Nunes, N. J, Pallé, E, Abreu, M, Affolter, M, Alibert, Y, Aliverti, M, Prieto, C. Allende, Alves, D, Amate, M, Avila, G, Baldini, V, Bandy, T, Benatti, S, Benz, W, Bianco, A, Broeg, C, Cabral, A, Calderone, G, Cirami, R, Coelho, J, Conconi, P, Coretti, I, Cumani, C, Cupani, G, Deiries, S, Dekker, H, Delabre, B, Demangeon, O, Di Marcantonio, P, Ehrenreich, D, Fragoso, A, Genolet, L, Genoni, M, Santos, R. Génova, Hughes, I, Iwert, O, Knudstrup, J, Landoni, M, Lizon, J. L, Maire, C, Manescau, A, Martins, C. J. A. P, Mégevand, D, Molaro, P, Monteiro, M. J. P. F. G, Monteiro, M. A, Moschetti, M, Mueller, E, Oggioni, L, Oliveira, A, Oshagh, M, Pariani, G, Pasquini, L, Poretti, E, Rasilla, J. L, Redaelli, E, Riva, M, Tschudi, S. Santana, Santin, P, Santos, P, Segovia, A, Sosnowska, D, Spanò, P, Tenegi, F, Udry, S, Zanutta, A, Zerbi, F

    Published 01-10-2020
    “…A&A 641, A92 (2020) We characterized the transiting planetary system orbiting the G2V star K2-38 using the new-generation echelle spectrograph ESPRESSO. We…”
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    Journal Article
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    A precise architecture characterization of the $\pi$ Men planetary system by Damasso, M, Sozzetti, A, Lovis, C, Barros, S. C. C, Sousa, S. G, Demangeon, O. D. S, Faria, J. P, Lillo-Box, J, Cristiani, S, Pepe, F, Rebolo, R, Santos, N. C, Osorio, M. R. Zapatero, Hernández, J. I. González, Amate, M, Pasquini, L, Zerbi, F. M, Adibekyan, V, Abreu, M, Affolter, M, Alibert, Y, Aliverti, M, Allart, R, Prieto, C. Allende, Álvarez, D, Alves, D, Avila, G, Baldini, V, Bandy, T, Benz, W, Bianco, A, Borsa, F, Bossini, D, Bourrier, V, Bouchy, F, Broeg, C, Cabral, A, Calderone, G, Cirami, R, Coelho, J, Conconi, P, Coretti, I, Cumani, C, Cupani, G, D'Odorico, V, Deiries, S, Dekker, H, Delabre, B, Di Marcantonio, P, Dumusque, X, Ehrenreich, D, Figueira, P, Fragoso, A, Genolet, L, Genoni, M, Santos, R. Génova, Hughes, I, Iwert, O, Kerber, F, Knudstrup, J, Landoni, M, Lavie, B, Lizon, J. -L, Curto, G. Lo, Maire, C, Martins, C. J . A. P, Mégevand, D, Mehner, A, Micela, G, Modigliani, A, Molaro, P, Monteiro, M. A, Monteiro, M. J. P. F. G, Moschetti, M, Mueller, E, Murphy, M. T, Nunes, N, Oggioni, L, Oliveira, A, Oshagh, M, Pallé, E, Pariani, G, Poretti, E, Rasilla, J. L, Rebordão, J, Redaelli, E. M, Riva, M, Tschudi, S. Santana, Santin, P, Santos, P, Ségransan, D, Schmidt, T. M, Segovia, A, Sosnowska, D, Spanò, P, Mascareño, A. Suárez, Tabernero, H, Tenegi, F, Udry, S, Zanutta, A

    Published 13-07-2020
    “…A&A 642, A31 (2020) The bright star $\pi$ Men was chosen as the first target for a radial velocity follow-up to test the performance of ESPRESSO, the new…”
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    Journal Article
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    4MOST: Project overview and information for the First Call for Proposals by Agertz, O, Aird, J, Andrae, R, Anwand-Heerwart, H, Baker, S, Barklem, P, Bellido-Tirado, O, Bergemann, M, Bongiorno, A, Brown, R, Brüggen, M, Brzeski, J, Cesarini, I, Chiappini, C, Christlieb, N, Cioni, M. -R. L, Comparat, J, Cooper, A, Croton, D, Davies, L. J. M, de Laverny, P, Disseau, K, Elhaddad, A, Farrell, T, Fechner, T, Feiz, C, Ferreras, I, Finoguenov, A, Fotopoulou, S, Fouesneau, M, Frenk, C, Fusillo, N. Gentile, Gerhard, O, Giannantonio, T, Gonzalez-Solares, E, Guiglion, G, Haehnelt, M, Hahn, T, Hartman, H, Hawkins, K, Hobbs, D, Hoenig, S, Howlett, C, Huet, T, Jablonka, P, Jofre, P, Khalatyan, A, King, D, Koposov, S, Korn, A, Kovalev, M, Lam, M. I, Lawrence, J, Lemasle, B, Lind, K, Liske, J, Lizon, J. -L, Loveday, J, McDermid, R. M, Mainieri, V, Mandel, K, Matijevic, G, McGregor, H, McMillan, P, Navarro, R, Ness, M, Nicklas, H, Norberg, P, Owers, M, Paterson, R, Pecontal, A, Pirard, J, Power, C, Queiroz, A. B. de Andrade, Ramstedt, S, Recio-Blanco, A, Richter, A. D, Rybizki, J, Ryde, N, Salvato, M, Sbordone, L, Schnurr, O, Scholz, R. -D, Schwope, A, Seifert, W, Shanks, T, Sivov, T, Smartt, S, Smith, R, Sullivan, M, Swann, E, Tamone, A, Teillon, J, Thi, W. -F, Tresse, L, Valentini, M, Ancker, M. van den, Venkatesan, S, Wagner, L, Walcher, C. J

    Published 01-04-2019
    “…The Messenger, 2019, 175, 3 We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey…”
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    Journal Article
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