@Article{TusnskiVali:2014:DeExIn,
               author = "Tusnski, Luis Ricardo Moretto and Valio, Adriana",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and CRAAM, 
                         Mackenzie University",
                title = "Detection of exomoons inside the habitable zone",
              journal = "Proceedings of the International Astronomical Union",
                 year = "2014",
               volume = "8",
               number = "S293",
                pages = "168--170",
             keywords = "planets, satellites: general, photometric techniques.",
             abstract = "Since the discovery of the first exoplanets, those most adequate 
                         for life to begin and evolve have been sought. Due to 
                         observational bias, however, most of the discovered planets so far 
                         are gas giants, precluding their habitability. However, if these 
                         hot Jupiters are located in the habitable zones of their host 
                         stars, and if rocky moons orbit them, then these moons may be 
                         habitable. In this work, we present a model for planetary transit 
                         simulation considering the presence of moons around a planet. The 
                         moon orbit is considered to be circular and coplanar with the 
                         planetary orbit. The other physical and orbital parameters of the 
                         star, planet, and moon, can be adjusted in each simulation. It is 
                         possible to simulate as many successive transits as desired. Since 
                         the presence of spots on the surface of the star may produce a 
                         signal similar to that of the presence of a moon, our model also 
                         allows for the inclusion of starspots. The goal is to determine 
                         the criteria for detectability of moons using photometry with the 
                         CoRoT and Kepler telescopes taking into account the stellar 
                         activity.",
                  doi = "10.1017/S1743921313012751",
                  url = "http://dx.doi.org/10.1017/S1743921313012751",
                 issn = "1743-9213 and 1743-9221",
                label = "scopus 2014-05 TusnskiVali:2014:DeExIn",
             language = "en",
           targetfile = "S1743921313012751a.pdf",
        urlaccessdate = "27 abr. 2024"
}