Zobrazeno 21 - 30
of 552
pro vyhledávání: '"D'Odorico, V."'
Autor:
Cristiani, S., Alcalá, J. M., Alencar, S. H. P., Balashev, S. A., Bastian, N., Barbuy, B., Battino, U., Calcines, A., Calderone, G., Cambianica, P., Carini, R., Carter, B., Cassisi, S., Castilho, B. V., Cescutti, G., Christlieb, N., Cirami, R., Coretti, I., Cooke, R., Covino, S., Cremonese, G., Cunha, K., Cupani, G., da Silva, A. R., De Caprio, V., De Cia, A., Dekker, H., D'Elia, V., De Silva, G., Diaz, M., Di Marcantonio, P., D'Auria, D., D'Odorico, V., Fitzsimmons, A., Ernandes, H., Evans, C., Franchini, M., Genoni, M., Gänsicke, B., Giribaldi, R. E., Gneiding, C., Grazian, A., Hansen, C. J., La Forgia, F., Landoni, M., Lazzarin, M., Lunney, D., Maciel, W., Marcolino, W., Marconi, M., Migliorini, A., Miller, C., Noterdaeme, P., Opitom, C., Pariani, G., Pilecki, B., Piranomonte, S., Quirrenbach, A., Redaelli, E. M. A., Pereira, C. B., Randich, S., Rossi, S., Sanchez-Janssen, R., Seifert, W., Smiljanic, R., Snodgrass, C., Stilz, I., Stürmer, J., Vanzella, E., Ventura, P., Verducci, O., Waring, C., Watson, S., Wells, M., Wright, D., Zafar, T., Zanutta, A.
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/2208.01672
Autor:
Tripodi, R., Feruglio, C., Fiore, F., Bischetti, M., D'Odorico, V., Carniani, S., Cristiani, S., Gallerani, S., Maiolino, R., Marconi, A., Pallottini, A., Piconcelli, E., Vallini, L., Zana, T.
Publikováno v:
A&A 665, A107 (2022)
The outstanding mass growth of supermassive black holes (SMBHs) at the Reionisation Epoch and how it is related to the concurrent growth of their host galaxies, poses challenges to theoretical models aimed at explaining how these systems formed in sh
Externí odkaz:
http://arxiv.org/abs/2207.03314
Autor:
Martins, C. J. A. P., Cristiani, S., Cupani, G., D'Odorico, V., Santos, R. Génova, Leite, A. C. O., Marques, C. M. J., Milaković, D., Molaro, P., Murphy, Michael T., Nunes, N. J., Schmidt, Tobias M., Adibekyan, V., Alibert, Y., Di Marcantonio, Paolo, Hernández, J. I. González, Mégevand, D., Palle, E., Pepe, F. A., Santos, N. C., Sousa, S. G., Sozzetti, A., Mascareño, A. Suárez, Osorio, M. R. Zapatero
Dynamical scalar fields in an effective four-dimensional field theory are naturally expected to couple to the rest of the theory's degrees of freedom, unless some new symmetry is postulated to suppress these couplings. In particular, a coupling to th
Externí odkaz:
http://arxiv.org/abs/2205.13848
Autor:
Bischetti, M., Feruglio, C., D'Odorico, V., Arav, N., Bañados, E., Becker, G., Bosman, S. E. I., Carniani, S., Cristiani, S., Cupani, G., Davies, R., Eilers, A. C., Farina, E. P., Ferrara, A., Maiolino, R., Mazzucchelli, C., Mesinger, A., Meyer, R., Onoue, M., Piconcelli, E., Ryan-Weber, E., Schindler, J-T., Wang, F., Yang, J., Zhu, Y., Fiore, F.
Publikováno v:
Nature, 605, 244-247 (2022)
Luminous quasars powered by accretion onto billion solar mass black holes already exist at the epoch of Reionisation, when the Universe was 0.5-1 Gyr old. These objects likely reside in over-dense regions of the Universe, and will grow to form today'
Externí odkaz:
http://arxiv.org/abs/2205.00021
Autor:
D'Odorico, V., Finlator, K., Cristiani, S., Cupani, G., Perrotta, S., Calura, F., Cènturion, M., Becker, G., Berg, T. A. M., Lopez, S., Ellison, S., Pomante, E.
We investigate the abundance and distribution of metals in the high-redshift intergalactic medium and circum-galactic medium through the analysis of a sample of almost 600 SiIV absorption lines detected in high and intermediate resolution spectra of
Externí odkaz:
http://arxiv.org/abs/2202.12206
Autor:
Faria, J. P., Mascareño, A. Suárez, Figueira, P., Silva, A. M., Damasso, M., Demangeon, O., Pepe, F., Santos, N. C., Rebolo, R., Cristiani, S., Adibekyan, V., Alibert, Y., Allart, R., Barros, S. C. C., Cabral, A., D'Odorico, V., Di Marcantonio, P., Dumusque, X., Ehrenreich, D., Hernández, J. I. González, Hara, N., Lillo-Box, J., Curto, G. Lo, Lovis, C., Martins, C. J. A. P., Mégevand, D., Mehner, A., Micela, G., Molaro, P., Nunes, N. J., Pallé, E., Poretti, E., Sousa, S. G., Sozzetti, A., Tabernero, H., Udry, S., Osorio, M. R. Zapatero
Proxima Centauri is the closest star to the Sun. This small, low-mass, mid M dwarf is known to host an Earth-mass exoplanet with an orbital period of 11.2 days within the habitable zone, as well as a long-period planet candidate with an orbital perio
Externí odkaz:
http://arxiv.org/abs/2202.05188
Autor:
Pallottini, A., Ferrara, A., Gallerani, S., Behrens, C., Kohandel, M., Carniani, S., Vallini, L., Salvadori, S., Gelli, V., Sommovigo, L., D'Odorico, V., Di Mascia, F., Pizzati, E.
We introduce SERRA, a suite of zoom-in high-resolution ($\sim 10\,\rm pc$) cosmological simulations including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post-processed to derive galaxy UV+FIR continuum and emission l
Externí odkaz:
http://arxiv.org/abs/2201.02636
Autor:
Molaro, P., Izzo, L., D'Odorico, V., Aydi, E., Bonifacio, P., Cescutti, G., Harvey, E. J., Hernanz, M., Selvelli, P., della Valle, M.
We report the search for 7Be isotope in the outbursts of the classical nova V6595 Sgr by means of high resolution UVES observations taken at the ESO VLT in April 2021, about two weeks after discovery and under difficult circumstances due to the pande
Externí odkaz:
http://arxiv.org/abs/2111.01469
Autor:
Demangeon, Olivier D. S., Osorio, M. R. Zapatero, Alibert, Y., Barros, S. C. C., Adibekyan, V., Tabernero, H. M., Antoniadis-Karnavas, A., Camacho, J. D., Mascareño, A. Suárez, Oshagh, M., Micela, G., Sousa, S. G., Lovis, C., Pepe, F. A., Rebolo, R., Cristiani, S., Santos, N. C., Allart, R., Prieto, C. Allende, Bossini, D., Bouchy, F., Cabral, A., Damasso, M., Di Marcantonio, P., D'Odorico, V., Ehrenreich, D., Faria, J., Figueira, P., Santos, R. Génova, Haldemann, J., Hara, N., Hernández, J. I. González, Lavie, B., Lillo-Box, J., Curto, G. Lo, Martins, C. J. A. P., Mégevand, D., Mehner, A., Molaro, P., Nunes, N. J., Pallé, E., Pasquini, L., Poretti, E., Sozzetti, A., Udry, S.
Publikováno v:
A&A 653, A41 (2021)
The advent of a new generation of radial velocity instruments has allowed us to break the one Earth-mass barrier. We report a new milestone in this context with the detection of the lowest-mass planet measured so far using radial velocities: L 98-59
Externí odkaz:
http://arxiv.org/abs/2108.03323
Autor:
Di Mascia, F., Gallerani, S., Ferrara, A., Pallottini, A., Maiolino, R., Carniani, S., D'Odorico, V.
We investigate the attenuation law in $z\sim 6$ quasars by combining cosmological zoom-in hydrodynamical simulations of quasar host galaxies, with multi-frequency radiative transfer calculations. We consider several dust models differing in terms of
Externí odkaz:
http://arxiv.org/abs/2106.15625