author = "Amati, L. and O'Brien, P. and G{\"o}tz, D. and Bozzo, E. and 
                         Tenzer, C. and Frontera, F. and Ghirlanda, G. and Labanti, C. and 
                         Osborne, J. P. and Stratta, G. and Tanvir, N. and Willingale, R. 
                         and Attina, P. and Campana, R. and Castro-Tirado, A. J. and 
                         Contini, C. and Fuschino, F. and Gomboc, A. and Hudec, R. and 
                         Orleanski, P. and Renotte, E. and Rodic, T. and Bagoly, Z. and 
                         Blain, A. and Callanan, P. and Covino, S. and Ferrara, A. and Le 
                         Floch, E. and Marisaldi, M. and Mereghetti, S. and Rosati, P. and 
                         Vacchi, A. and D'Avanzo, P. and Giommi, P. and Piranomonte, S. and 
                         Piro, L. and Reglero, V. and Rossi, A. and Santangelo, A. and 
                         Salvaterra, R. and Tagliaferri, G. and Vergani, S. and 
                         Vinciguerra, S. and Briggs, M. and Campolongo, E. and Ciolfi, R. 
                         and Connaughton, V. and Cordier, B. and Morelli, B. and Orlandini, 
                         M. and Adami, C. and Argan, A. and Atteia, J. -L. and Auricchio, 
                         N. and Balazs, L. and Baldazzi, G. and Basa, S. and Basak, R. and 
                         Bellutti, P. and Bernardini, M. G. and Bertuccio, G. and Braga, 
                         Jo{\~a}o and Branchesi, M. and Brandt, S. and Brocato, E. and 
                         Budtz-Jorgensen, C. and Bulgarelli, A. and Burderi, L. and Camp, 
                         J. and Capozziello, S. and Caruana, J. and Casella, P. and Cenko, 
                         B. and Chardonnet, P. and Ciardi, B. and Colafrancesco, S. and 
                         Dainotti, M. G. and D'Elia, V. and De Martino, D. and De Pasquale, 
                         M. and Del Monte, E. and Della Valle, M. and Drago, A. and 
                         Evangelista, Y. and Feroci, M. and Finelli, F. and Fiorini, M. and 
                         Fynbo, J. and Gal-Yam, A. and Gendre, B. and Ghisellini, G. and 
                         Grado, A. and Guidorzi, C. and Hafizi, M. and Hanlon, L. and 
                         Hjorth, J. and Izzo, L. and Kiss, L. and Kumar, P. and Kuvvetli, 
                         I. and Lavagna, M. and Li, T. and Longo, F. and Lyutikov, M. and 
                         Maio, U. and Maiorano, E. and Malcovati, P. and Malesani, D. and 
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                         Nargaard-Nielsen, H. U. and Nicastro, L. and Palazzi, E. and 
                         Paltani, S. and Panessa, F. and Pareschi, G. and Pe'er, A. and 
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                         and Rauw, G. and Razzano, M. and Read, A. and Rezzolla, L. and 
                         Romano, P. and Ruffini, R. and Savaglio, S. and Sguera, V. and 
                         Schady, P. and Skidmore, W. and Song, L. and Stanway, E. and 
                         Starling, R. and Topinka, M. and Troja, E. and van Putten, M. and 
                         Vanzella, E. and Vercellone, S. and Wilson-Hodge, C. and Yonetoku, 
                         D. and Zampa, G. and Zampa, N. and Zhang, B. and Zhang, B. B. and 
                         Zhang, S. and Zhang, S. -N. and Antonelli, A. and Bianco, F. and 
                         Boci, S. and Boer, M. and Botticella, M. T. and Boulade, O. and 
                         Butler, C. and Campana, S. and Capitanio, F. and Celotti, A. and 
                         Chen, Y. and Colpi, M. and Comastri, A. and Cuby, J. -G. and 
                         Dadina, M. and De Luca, A. and Dong, Y. -W. and Ettori, S. and 
                         Gandhi, P. and Geza, E. and Greiner, J. and Guiriec, S. and Harms, 
                         J. and Hernanz, M. and Hornstrup, A. and Hutchinson, I. and 
                         Israel, G. and Jonker, P. and Kaneko, Y. and Kawai, N. and 
                         Wiersema, K. and Korpela, S. and Lebrun, V. and Lu, F. and 
                         MacFadyen, A. and Malaguti, G. and Maraschi, L. and Melandri, A. 
                         and Modjaz, M. and Morris, D. and Omodei, N. and Paizis, A. and 
                         P{\'a}ta, P. and Petrosian, V. and Rachevski, A. and Rhoads, J. 
                         and Ryde, F. and Sabau-Graziati, L. and Shigehiro, N. and Sims, M. 
                         and Soomin, J. and Sz{\'e}csi, D. and Urata, Y. and Uslenghi, M. 
                         and Valenziano, L. and Vianello, G. and Vojtech, S. and Watson, D. 
                         and Zicha, J.",
          affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
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                         and {} and {} and {} and {} and {} and {} and {} and {} and {} and 
                         {} and {} and {} and {} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)}",
                title = "The THESEUS space mission concept: science case, design and 
                         expected performances",
              journal = "Advances in Space Research",
                 year = "2018",
               volume = "62",
               number = "1",
                pages = "191--244",
                 note = "{cited By 0}",
             keywords = "Astrophysics, Ionization, Stars, Telescopes, X rays, Cosmology: 
                         observation, Dark ages, Gamma-ray: bursts, Gravitational 
                         radiation, High sensitivity, Luminosity functions, 
                         Multi-wavelengths, Star formation rates, Gamma rays.",
             abstract = "THESEUS is a space mission concept aimed at exploiting Gamma-Ray 
                         Bursts for investigating the early Universe and at providing a 
                         substantial advancement of multi-messenger and time-domain 
                         astrophysics. These goals will be achieved through a unique 
                         combination of instruments allowing GRB and X-ray transient 
                         detection over a broad field of view (more than 1sr) with 
                         0.5{\^a}1 arcmin localization, an energy band extending from 
                         several MeV down to 0.3 keV and high sensitivity to transient 
                         sources in the soft X-ray domain, as well as on-board prompt (few 
                         minutes) follow-up with a 0.7 m class IR telescope with both 
                         imaging and spectroscopic capabilities. THESEUS will be perfectly 
                         suited for addressing the main open issues in cosmology such as, 
                         e.g., star formation rate and metallicity evolution of the 
                         inter-stellar and intra-galactic medium up to redshift {\^a}10, 
                         signatures of Pop III stars, sources and physics of re-ionization, 
                         and the faint end of the galaxy luminosity function. In addition, 
                         it will provide unprecedented capability to monitor the X-ray 
                         variable sky, thus detecting, localizing, and identifying the 
                         electromagnetic counterparts to sources of gravitational 
                         radiation, which may be routinely detected in the late 
                         {\^a}20s/early {\^a}30s by next generation facilities like 
                         aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will 
                         also provide powerful synergies with the next generation of 
                         multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, 
                         ATHENA).  2018 COSPAR.",
                  doi = "10.1016/j.asr.2018.03.010",
                  url = "http://dx.doi.org/10.1016/j.asr.2018.03.010",
                 issn = "0273-1177 and 1879-1948",
                label = "iso2018-07-05",
             language = "en",
           targetfile = "amati_theseu.pdf",
                  url = "https://www.scopus.com/inward/record.uri?eid=2-s2.0-85046789580\&doi=10.1016%2fj.asr.2018.03.010\&partnerID=40\&md5=7890c008c634b99df4562ff5c234b337",
        urlaccessdate = "04 dez. 2020"