Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Odorico, P. D."'
Autor:
Genoni, Matteo, Dekker, Hans, Covino, Stefano, Cirami, Roberto, Scalera, Marcello Agostino, Bissel, Lawrence, Seifert, Walter, Calcines, Ariadna, Avila, Gerardo, Stuermer, Julian, Ritz, Christopher, Lunney, David, Miller, Chris, Watson, Stephen, Waring, Chris, Castilho, Bruno Vaz, De Arruda, Marcio, Verducci, Orlando, Coretti, Igor, Oggioni, Luca, Pariani, Giorgio, Redaelli, Edoardo Alberto Maria, D'Ambrogio, Matteo, Calderone, Giorgio, Porru, Matteo, Stilz, Ingo, Smiljanic, Rodolfo, Cupani, Guido, Franchini, Mariagrazia, Scaudo, Andrea, Geers, Vincent, De Caprio, Vincenzo, Auria, Domenico D', Sibalic, Mina, Opitom, Cyrielle, Cescutti, Gabriele, Odorico, Valentina D', Janssen, Ruben Sanchez, Quirrenbach, Andreas, Barbuy, Beatriz, Cristiani, Stefano, Di Marcantonio, Paolo
Publikováno v:
Proceedings Volume 13096, Ground-based and Airborne Instrumentation for Astronomy X; 130967T (2024)
In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at ground-UV wavelengths for the foreseeable future. The Cassegrain U-Band Efficient Spectrograph (CUBES) has been designed to provi
Externí odkaz:
http://arxiv.org/abs/2412.03460
Autor:
Casasayas-Barris, N., Palle, E., Stangret, M., Bourrier, V, Tabernero, H. M., Yan, F., Borsa, F., Allart, R., Osorio, M. R. Zapatero, Lovis, C., Sousa, S. G., Chen, G., Oshagh, M., Santos, N. C., Pepe, F., Rebolo, R., Molaro, P., Cristiani, S., Adibekyan, V., Alibert, Y., Prieto, C. Allende, Bouchy, F., Demangeon, O. D. S., Di Marcantonio, P., Odorico, V. D, Ehrenreich, D., Figueira, P., Santos, R. Génova, Hernández, J. I. González, Lavie, B., Lillo-Box, J., Curto, G. Lo, Martins, C. J. A. P., Mehner, A., Micela, G., Nunes, N. J., Poretti, E., Sozzetti, A., Mascareño, A. Suárez, Udry, S.
We observed two transits of the iconic gas giant HD 209458b between 380 and 780 nm, using the high-resolution ESPRESSO spectrograph. The derived planetary transmission spectrum exhibits features at all wavelengths where the parent star shows strong a
Externí odkaz:
http://arxiv.org/abs/2101.04094
Autor:
Carniani, S., Marconi, A., Biggs, A., Cresci, G., Cupani, G., Odorico, V. D', Humphreys, E., Maiolino, R., Mannucci, F., Molaro, P., Nagao, T., Testi, L., Zwaan, M. A.
We performed a kinematical analysis of the [CII] line emission of the BR 1202-0725 system at z~4,7 using ALMA observations. The most prominent sources of this system are a quasar and a submillimeter galaxy, separated by a projected distance of about
Externí odkaz:
http://arxiv.org/abs/1308.5113
The galaxy Luminosity Function (LF) has been estimated in the rest frame B luminosity at 0
Externí odkaz:
http://arxiv.org/abs/astro-ph/0103113
Autor:
Ratajczak, Z., Odorico, P. D., Bestelmeyer, B., Collins, Scott L., Forest Isbell, Nippert, J. B.
Publikováno v:
Ecological Monographs, vol 87, iss 2
Ratajczak, Z; D'Odorico, P; Collins, SL; Bestelmeyer, BT; Isbell, FI; & Nippert, JB. (2017). The interactive effects of press/pulse intensity and duration on regime shifts at multiple scales. Ecological Monographs, 87(2), 198-218. doi: 10.1002/ecm.1249. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/34g6v6ms
Experts@Minnesota
Ratajczak, Z; D'Odorico, P; Collins, SL; Bestelmeyer, BT; Isbell, FI; & Nippert, JB. (2017). The interactive effects of press/pulse intensity and duration on regime shifts at multiple scales. Ecological Monographs, 87(2), 198-218. doi: 10.1002/ecm.1249. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/34g6v6ms
Experts@Minnesota
© 2017 by the Ecological Society of America Regime shifts are difficult-to-reverse transitions that occur when an ecosystem reorganizes around a new set of self-reinforcing feedbacks. Regime shifts are predicted to occur when the intensity of some e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3fc2e7df7f512b50262b1cc2e718af72
https://escholarship.org/uc/item/34g6v6ms
https://escholarship.org/uc/item/34g6v6ms
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.