Zobrazeno 1 - 3
of 3
pro vyhledávání: '"D'Odorico, V."'
Autor:
Valentina D'Odorico, Fabrizio Fiore, Roberto Maiolino, Andrea Ferrara, Stefano Carniani, Chiara Feruglio, Enrico Piconcelli, Stefano Cristiani, Andrea Pallottini, Simona Gallerani, Alessandro Marconi
Publikováno v:
The Astrophysical Journal
We report the discovery of Serenity-18, a galaxy at z=5.939 for which we could measure the content of molecular gas, M(H_2)~ 5 x10^9 M_sun, traced by the CO(6-5) emission, together with the metal-poor ([Fe/H]=-3.08 +- 0.12, [Si/H]=-2.86 +- 0.14) gas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f89b389b18c95bf3a433d51ae5f8196
http://arxiv.org/abs/1808.01146
http://arxiv.org/abs/1808.01146
Autor:
Lajos G. Balázs, E. Le Floc'h, René Hudec, Ehud Behar, Giancarlo Ghirlanda, Valentina D'Odorico, Silvia Zane, J. P. Osborne, P. T. O'Brien, Stéphane Paltani, Dorottya Szécsi, A. Gomboc, B. Ciardi, Lise Christensen, U. Maio, Yuji Urata, Sandro Mereghetti, Ruben Salvaterra, F. Frontera, E. Piedipalumbo, Sergio Campana, Joseph Caruana, Olga Sergijenko, Pasquier Noterdaeme, A. De Cia, Lorenzo Amati, Diego Götz, Elizabeth R. Stanway, L. V. Toth, S. D. Vergani, M. de Pasquale, Nial R. Tanvir, Z. Bagoly, L. Graziani, M. Della Valle, S. Basa, Piero Rosati, István T. Horváth
Publikováno v:
Exper.Astron.
Exper.Astron., 2021, 52 (3), pp.219-244. ⟨10.1007/s10686-021-09778-w⟩
Tanvir, N R, Le Floc'h, E, Christensen, L, Caruana, J, Salvaterra, R, Ghirlanda, G, Ciardi, B, Maio, U, D'Odorico, V, Piedipalumbo, E, Campana, S, Noterdaeme, P, Graziani, L, Amati, L, Bagoly, Z, Balazs, L G, Basa, S, Behar, E, De Cia, A, Valle, M D, De Pasquale, M, Frontera, F, Gomboc, A, Gotz, D, Horvath, I, Hudec, R, Mereghetti, S, O'Brien, P T, Osborne, J P, Paltani, S, Rosati, P, Sergijenko, O, Stanway, E R, Szecsi, D, Toth, L V, Urata, Y, Vergani, S & Zane, S 2021, ' Exploration of the high-redshift universe enabled by THESEUS ', Experimental Astronomy, vol. 52, no. 3, pp. 219-244 . https://doi.org/10.1007/s10686-021-09778-w
Exper.Astron., 2021, 52 (3), pp.219-244. ⟨10.1007/s10686-021-09778-w⟩
Tanvir, N R, Le Floc'h, E, Christensen, L, Caruana, J, Salvaterra, R, Ghirlanda, G, Ciardi, B, Maio, U, D'Odorico, V, Piedipalumbo, E, Campana, S, Noterdaeme, P, Graziani, L, Amati, L, Bagoly, Z, Balazs, L G, Basa, S, Behar, E, De Cia, A, Valle, M D, De Pasquale, M, Frontera, F, Gomboc, A, Gotz, D, Horvath, I, Hudec, R, Mereghetti, S, O'Brien, P T, Osborne, J P, Paltani, S, Rosati, P, Sergijenko, O, Stanway, E R, Szecsi, D, Toth, L V, Urata, Y, Vergani, S & Zane, S 2021, ' Exploration of the high-redshift universe enabled by THESEUS ', Experimental Astronomy, vol. 52, no. 3, pp. 219-244 . https://doi.org/10.1007/s10686-021-09778-w
At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over the whole of cosmic history. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::df3e642f049af15e3b6338e42703aca6
https://hal.science/hal-03224684
https://hal.science/hal-03224684
Autor:
Paolo Molaro, Alessandro Marconi, A. D. Biggs, Tohru Nagao, Guido Cupani, Elizabeth Humphreys, Stefano Carniani, Leonardo Testi, Valentina D'Odorico, Giovanni Cresci, F. Mannucci, Martin Zwaan, Roberto Maiolino
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1b5b69e32c2e20c4a413e742edafa5b
https://hdl.handle.net/11384/89582
https://hdl.handle.net/11384/89582