Zobrazeno 1 - 10
of 272
pro vyhledávání: '"Battistini C"'
Autor:
Bensby, T., Bergemann, M., Rybizki, J., Lemasle, B., Howes, L., Kovalev, M., Agertz, O., Asplund, M., Barklem, P., Battistini, C., Casagrande, L., Chiappini, C., Church, R., Feltzing, S., Ford, D., Gerhard, O., Kushniruk, I., Kordopatis, G., Lind, K., Minchev, I., McMillan, P., Rix, H. -W., Ryde, N., Traven, G.
Publikováno v:
The Messenger, 2019, 175, 35
The signatures of the formation and evolution of a galaxy are imprinted in its stars. Their velocities, ages, and chemical compositions present major constraints on models of galaxy formation, and on various processes such as the gas inflows and outf
Externí odkaz:
http://arxiv.org/abs/1903.02470
Autor:
de Jong, R. S., Agertz, O., Berbel, A. Agudo, Aird, J., Alexander, D. A., Amarsi, A., Anders, F., Andrae, R., Ansarinejad, B., Ansorge, W., Antilogus, P., Anwand-Heerwart, H., Arentsen, A., Arnadottir, A., Asplund, M., Auger, M., Azais, N., Baade, D., Baker, G., Baker, S., Balbinot, E., Baldry, I. K., Banerji, M., Barden, S., Barklem, P., Barthélémy-Mazot, E., Battistini, C., Bauer, S., Bell, C. P. M., Bellido-Tirado, O., Bellstedt, S., Belokurov, V., Bensby, T., Bergemann, M., Bestenlehner, J. M., Bielby, R., Bilicki, M., Blake, C., Bland-Hawthorn, J., Boeche, C., Boland, W., Boller, T., Bongard, S., Bongiorno, A., Bonifacio, P., Boudon, D., Brooks, D., Brown, M. J. I., Brown, R., Brüggen, M., Brynnel, J., Brzeski, J., Buchert, T., Buschkamp, P., Caffau, E., Caillier, P., Carrick, J., Casagrande, L., Case, S., Casey, A., Cesarini, I., Cescutti, G., Chapuis, D., Chiappini, C., Childress, M., Christlieb, N., Church, R., Cioni, M. -R. L., Cluver, M., Colless, M., Collett, T., Comparat, J., Cooper, A., Couch, W., Courbin, F., Croom, S., Croton, D., Daguisé, E., Dalton, G., Davies, L. J. M., Davis, T., de Laverny, P., Deason, A., Dionies, F., Disseau, K., Doel, P., Döscher, D., Driver, S. P., Dwelly, T., Eckert, D., Edge, A., Edvardsson, B., Youssoufi, D. El, Elhaddad, A., Enke, H., Erfanianfar, G., Farrell, T., Fechner, T., Feiz, C., Feltzing, S., Ferreras, I., Feuerstein, D., Feuillet, D., Finoguenov, A., Ford, D., Fotopoulou, S., Fouesneau, M., Frenk, C., Frey, S., Gaessler, W., Geier, S., Fusillo, N. Gentile, Gerhard, O., Giannantonio, T., Giannone, D., Gibson, B., Gillingham, P., González-Fernández, C., Gonzalez-Solares, E., Gottloeber, S., Gould, A., Grebel, E. K., Gueguen, A., Guiglion, G., Haehnelt, M., Hahn, T., Hansen, C. J., Hartman, H., Hauptner, K., Hawkins, K., Haynes, D., Haynes, R., Heiter, U., Helmi, A., Aguayo, C. Hernandez, Hewett, P., Hinton, S., Hobbs, D., Hoenig, S., Hofman, D., Hook, I., Hopgood, J., Hopkins, A., Hourihane, A., Howes, L., Howlett, C., Huet, T., Irwin, M., Iwert, O., Jablonka, P., Jahn, T., Jahnke, K., Jarno, A., Jin, S., Jofre, P., Johl, D., Jones, D., Jönsson, H., Jordan, C., Karovicova, I., Khalatyan, A., Kelz, A., Kennicutt, R., King, D., Kitaura, F., Klar, J., Klauser, U., Kneib, J., Koch, A., Koposov, S., Kordopatis, G., Korn, A., Kosmalski, J., Kotak, R., Kovalev, M., Kreckel, K., Kripak, Y., Krumpe, M., Kuijken, K., Kunder, A., Kushniruk, I., Lam, M. I, Lamer, G., Laurent, F., Lawrence, J., Lehmitz, M., Lemasle, B., Lewis, J., Li, B., Lidman, C., Lind, K., Liske, J., Lizon, J. -L., Loveday, J., Ludwig, H. -G., McDermid, R. M., Maguire, K., Mainieri, V., Mali, S., Mandel, H., Mandel, K., Mannering, L., Martell, S., Delgado, D. Martinez, Matijevic, G., McGregor, H., McMahon, R., McMillan, P., Mena, O., Merloni, A., Meyer, M. J., Michel, C., Micheva, G., Migniau, J. -E., Minchev, I., Monari, G., Muller, R., Murphy, D., Muthukrishna, D., Nandra, K., Navarro, R., Ness, M., Nichani, V., Nichol, R., Nicklas, H., Niederhofer, F., Norberg, P., Obreschkow, D., Oliver, S., Owers, M., Pai, N., Pankratow, S., Parkinson, D., Parry, I., Paschke, J., Paterson, R., Pecontal, A., Phillips, D., Pillepich, A., Pinard, L., Pirard, J., Piskunov, N., Plank, V., Plüschke, D., Pons, E., Popesso, P., Power, C., Pragt, J., Pramskiy, A., Pryer, D., Quattri, M., Queiroz, A. B. de Andrade, Quirrenbach, A., Rahurkar, S., Raichoor, A., Ramstedt, S., Rau, A., Recio-Blanco, A., Reiss, R., Renaud, F., Revaz, Y., Rhode, P., Richard, J., Richter, A. D., Rix, H. -W., Robotham, A. S. G., Roelfsema, R., Romaniello, M., Rosario, D., Rothmaier, F., Roukema, B., Ruchti, G., Rupprecht, G., Rybizki, J., Ryde, N., Saar, A., Sadler, E., Sahlén, M., Salvato, M., Sassolas, B., Saunders, W., Saviauk, A., Sbordone, L., Schmidt, T., Schnurr, O., Scholz, R. -D., Schwope, A., Seifert, W., Shanks, T., Sheinis, A., Sivov, T., Skúladóttir, Á., Smartt, S., Smedley, S., Smith, G., Smith, R., Sorce, J., Spitler, L., Starkenburg, E., Steinmetz, M., Stilz, I., Storm, J., Sullivan, M., Sutherland, W., Swann, E., Tamone, A., Taylor, E. N., Teillon, J., Tempel, E., ter Horst, R., Thi, W. -F., Tolstoy, E., Trager, S., Traven, G., Tremblay, P. -E., Tresse, L., Valentini, M., van de Weygaert, R., Ancker, M. van den, Veljanoski, J., Venkatesan, S., Wagner, L., Wagner, K., Walcher, C. J., Waller, L., Walton, N., Wang, L., Winkler, R., Wisotzki, L., Worley, C. C., Worseck, G., Xiang, M., Xu, W., Yong, D., Zhao, C., Zheng, J., Zscheyge, F., Zucker, D.
Publikováno v:
The Messenger, 2019, 175, 3
We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey facility under development for the four-metre-class Visible and Infrared Survey Telescope for Astronomy (VISTA) at Paranal. I
Externí odkaz:
http://arxiv.org/abs/1903.02464
Autor:
Guiglion, G., Battistini, C., Bell, C. P. M., Bensby, T., Boller, T., Chiappini, C., Comparat, J., Christlieb, N., Church, R., Cioni, M. -R. L., Davies, L., Dwelly, T., de Jong, R. S., Feltzing, S., Gueguen, A., Howes, L., Irwin, M., Kushniruk, I., Lam, M. I, Liske, J., McMahon, R., Merloni, A., Norberg, P., Robotham, A. S. G., Schnurr, O., Sorce, J. G., Starkenburg, E., Storm, J., Swann, E., Tempel, E., Thi, W. -F., Worley, C. C., Walcher, C. J.
Publikováno v:
The Messenger, 2019, 175, 17
The current status of and motivation for the 4MOST Survey Strategy, as developed by the Consortium science team, are presented here. Key elements of the strategy are described, such as sky coverage, number of visits and total exposure times in differ
Externí odkaz:
http://arxiv.org/abs/1903.02466
Autor:
Walcher, C. J., Banerji, M., Battistini, C., Bell, C. P. M., Bellido-Tirado, O., Bensby, T., Bestenlehner, J. M., Boller, T., Brynnel, J., Casey, A., Chiappini, C., Christlieb, N., Church, R., Cioni, M. -R. L., Croom, S., Comparat, J., Davies, L. J. M., de Jong, R. S., Dwelly, T., Enke, H., Feltzing, S., Feuillet, D., Fouesneau, M., Ford, D., Frey, S., Gonzalez-Solares, E., Gueguen, A., Howes, L., Irwin, M., Klar, J., Kordopatis, G., Korn, A., Krumpe, M., Kushniruk, I., Lam, M. I, Lewis, J., Lind, K., Liske, J., Loveday, J., Mainieri, V., Martell, S., Matijevic, G., McMahon, R., Merloni, A., Murphy, D., Niederhofer, F., Norberg, P., Pramskiy, A., Romaniello, M., Robotham, A. S. G., Rothmaier, F., Ruchti, G., Schnurr, O., Schwope, A., Smedley, S., Sorce, J., Starkenburg, E., Stilz, I., Storm, J., Tempel, E., Thi, W. -F., Traven, G., Valentini, M., Ancker, M. van den, Walton, N., Winkler, R., Worley, C. C., Worseck, G.
Publikováno v:
The Messenger, 2019, 175, 12
The 4MOST instrument is a multi-object spectrograph that will address Galactic and extragalactic science cases simultaneously by observing targets from a large number of different surveys within each science exposure. This parallel mode of operation
Externí odkaz:
http://arxiv.org/abs/1903.02465
Autor:
Christlieb, N., Battistini, C., Bonifacio, P., Caffau, E., Ludwig, H. -G., Asplund, M., Barklem, P., Bergemann, M., Church, R., Feltzing, S., Ford, D., Grebel, E. K., Hansen, C. J., Helmi, A., Kordopatis, G., Kovalev, M., Korn, A., Lind, K., Quirrenbach, A., Rybizki, J., Skúladóttir, Á., Starkenburg, E.
Publikováno v:
The Messenger, 2019, 175, 26
We will study the formation history of the Milky Way, and the earliest phases of its chemical enrichment, with a sample of more than 1.5 million stars at high galactic latitude. Elemental abundances of up to 20 elements with a precision of better tha
Externí odkaz:
http://arxiv.org/abs/1903.02468
Autor:
Lind, K., Koposov, S. E., Battistini, C., Marino, A. F., Ruchti, G., Serenelli, A., Worley, C. C., Alves-Brito, A., Asplund, M., Barklem, P. S., Bensby, T., Bergemann, M., Blanco-Cuaresma, S., Bragaglia, A., Edvardsson, B., Feltzing, S., Gruyters, P., Heiter, U., Jofre, P., Korn, A. J., Nordlander, T., Ryde, N., Soubiran, C., Gilmore, G., Randich, S., Ferguson, A. M. N., Jeffries, R. D., Vallenari, A., Prieto, C. Allende, Pancino, E., Recio-Blanco, A., Romano, D., Smiljanic, R., Bellazzini, M., Damiani, F., Hill, V., de Laverny, P., Jackson, R. J., Lardo, C., Zaggia, S.
Publikováno v:
A&A 575, L12 (2015)
A small fraction of the halo field is made up of stars that share the light element (Z<=13) anomalies characteristic of second generation globular cluster (GC) stars. The ejected stars shed light on the formation of the Galactic halo by tracing the d
Externí odkaz:
http://arxiv.org/abs/1502.03934
Akademický článek
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Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Walcher, C., Banerji, M., Battistini, C., Bell, C., Bellido-Tirado, O., Bensby, T., Bestenlehner, J., Boller, T., Brynnel, J., Casey, A., Chiappini, C., Christlieb, N., Church, R., Cioni, M., Croom, S., Comparat, J., Davies, L., de Jong, R., Dwelly, T., Enke, H., Feltzing, S., Feuillet, D., Fouesneau, M., Ford, D., Frey, S., Gonzalez-Solares, E., Gueguen, A., Howes, L., Irwin, M., Klar, J., Kordopatis, G., Korn, A., Krumpe, M., Kushniruk, I., Lam, M., Lewis, J., Lind, K., Liske, J., Loveday, J., Mainieri, V., Martell, S., Matijevic, G., McMahon, R., Merloni, A., Murphy, D., Niederhofer, F., Norberg, P., Pramskiy, A., Romaniello, M., Robotham, A., Rothmaier, F., Ruchti, G., Schnurr, O., Schwope, A., Smedley, S., Sorce, J., Starkenburg, E., Stilz, I., Storm, J., Tempel, E., Thi, W., Traven, G., Valentini, M., van den Ancker, M., Walton, N., Winkler, R., Worley, C.
Publikováno v:
The Messenger
The 4MOST instrument is a multi-object spectrograph that will address Galactic and extragalactic science cases simultaneously by observing targets from a large number of different surveys within each science exposure. This parallel mode of operation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::663544f25b552a79e34a6799c3a87e6b
https://doi.org/10.18727/0722-6691/5118
https://doi.org/10.18727/0722-6691/5118
Autor:
Amelio, S, Battistini, C
The aim of this paper is to analyze the level of acceptance of social responsibility practices in Italy and in particular to evaluate the degree of social responsibility arising from the websites of Italian listed companies. CSR communication contrib
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::9b83296122e8cfb9b5ef0e8a80baa8ad
http://hdl.handle.net/10281/228395
http://hdl.handle.net/10281/228395