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41by Deeg, H. J., Alonso, R., Belmonte, J. A., Horne, Keith, Alsubai, K., Cameron, A. C., Doyle, L. R.“... objectives are the detection of all giant-planet transits (with periods up to some weeks) across stars up...”
Published 2004
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42“... objectives are the detection of all giant-planet tran sits (with periods up to some weeks) across stars up...”
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43by Deeg, H. J., Alonso, R., Belmonte, J. A., Horne, K., Alsubai, K., Cameron, A., Doyle, L. R.“... objectives are the detection of all giant‐planet transits (with periods up to some weeks) across stars up...”
Published in Astronomische Nachrichten (2004)
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44by Porco, C.C., West, R.A., McEwen, A.S., Del Genio, A.D., Ingersoll, A.P., Thomas, P.C., Squyres, S.W., Dones, L., Murray, C.D., Johnson, T.V., Burns, J.A., Brahic, A., Neukum, G., Veverka, J., Barbara, J.M., Denk, T., Evans, M., Ferrier, J.J., Geissler, P., Helfenstein, P., Roatsch, T., Throop, H., Tiscareno, M., Vasavada A.“... as the spacecraft encountered the giant planet en route to Saturn. We report findings on Jupiter's zonal winds...”
Published 2003
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45by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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46by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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47by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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48by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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49by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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50by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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51by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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52by Donati, J.-F., Moutou, C., Farès, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... (at intermediate latitudes) is synchronized with the orbital motion of its giant planet (period 3.3 d). Assuming...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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53by Baldwin, E.C.“... produced by the hypervelocity impact of cosmic dust observed on lunar return samples, to the giant planet...”
Published 2008
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54by Fares, R., Donati, J. -F., Moutou, C., Jardine, M. M., Griessmeier, J. -M., Zarka, P., Shkolnik, E. L., Bohlender, D., Catala, C., Cameron, A. C.“...HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study...”
Published 2010
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55by Fares, R., Donati, J.-F., Moutou, C., Jardine, M. M., Grießmeier, J.-M., Zarka, P., Shkolnik, E. L., Bohlender, D., Catala, C., Cameron, A. C.“...HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study...”
Published in Monthly Notices of the Royal Astronomical Society (2010)
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56“... in astrophysical bodies, such as in giant planet interiors. In this talk, we show that such periodically stratified...”
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57by Porco, Carolyn C., West, Robert A., McEwen, Alfred, Del Genio, Anthony D., Ingersoll, Andrew P., Thomas, Peter, Squyres, Steve, Dones, Luke, Murray, Carl D., Johnson, Torrence V., Burns, Joseph A., Brahic, Andre, Neukum, Gerhard, Veverka, Joseph, Barbara, John M., Denk, Tilmann, Evans, Michael, Ferrier, Joseph J., Geissler, Paul, Helfenstein, Paul, Roatsch, Thomas, Throop, Henry, Tiscareno, Matthew, Vasavada, Ashwin R.“... as the spacecraft encountered the giant planet en route to Saturn. We report findings on Jupiter's zonal winds...”
Published in Science (2003)
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58by Deeg, H J, Alonso, R, Belmonte, J A, Horne, K, Alsubai, K, Cameron, A, Doyle, L R“... objectives are the detection of all giant-planet transits (with periods up to some weeks) across stars up...”
Published in Astronomische Nachrichten (2004)
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59by Porco, Carolyn C., West, Robert A., McEwen, Alfred, Del Genio, Anthony D., Ingersoll, Andrew P., Thomas, Peter, Squyres, Steve, Dones, Luke, Murray, Carl D., Johnson, Torrence V., Burns, Joseph A., Brahic, Andre, Neukum, Gerhard, Veverka, Joseph, Barbara, John M., Denk, Tilmann, Evans, Michael, Ferrier, Joseph J., Geissler, Paul, Helfenstein, Paul, Roatsch, Thomas, Throop, Henry, Tiscareno, Matthew, Vasavada, Ashwin R.“... as the spacecraft encountered the giant planet en route to Saturn. We report findings on Jupiter's zonal winds...”
Published in Science (2003)
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60by Lainey, V., Karatekin, Ö., Desmars, J., Charnoz, S., Arlot, J-E., Emelyanov, N., Poncin-Lafitte, C. Le, Mathis, S., Remus, F., Tobie, G., Zahn, J-P.“... ratio can be determined at different frequencies, it may also be possible to constrain the giant planet...”
Published in The Astrophysical Journal (2012)
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