@Article{TintoAraś:2016:CoObGr,
               author = "Tinto, Massimo and Ara{\'u}jo, Jos{\'e} Carlos Neves de",
          affiliation = "{California Institute of Technology} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Coherent observations of gravitational radiation with LISA and 
                         gLISA",
              journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",
                 year = "2016",
               volume = "94",
               number = "8",
                month = "Oct.",
             abstract = "The geosynchronous Laser Interferometer Space Antenna (gLISA) is a 
                         space-based gravitational wave (GW) mission that, for the past 5 
                         years, has been under joint study at the Jet Propulsion 
                         Laboratory; Stanford University; the National Institute for Space 
                         Research (I.N.P.E., Brazil); and Space Systems Loral. If flown at 
                         the same time as the LISA mission, the two arrays will deliver a 
                         joint sensitivity that accounts for the best performance of both 
                         missions in their respective parts of the millihertz band. This 
                         simultaneous operation will result in an optimally combined 
                         sensitivity curve that is {"}white{"} from about 3×10-3 Hz to 1 
                         Hz, making the two antennas capable of detecting, with high 
                         signal-to-noise ratios (SNRs), coalescing black-hole binaries 
                         (BHBs) with masses in the range (10-108)M. Their ability of 
                         jointly tracking, with enhanced SNR, signals similar to that 
                         observed by the Advanced Laser Interferometer Gravitational Wave 
                         Observatory (aLIGO) on September 14, 2015 (the GW150914 event) 
                         will result in a larger number of observable small-mass binary 
                         black holes and an improved precision of the parameters 
                         characterizing these sources. Together, LISA, gLISA and aLIGO will 
                         cover, with good sensitivity, the (10-4-103) Hz frequency band.",
                  doi = "10.1103/PhysRevD.94.081101",
                  url = "http://dx.doi.org/10.1103/PhysRevD.94.081101",
                 issn = "1550-7998",
             language = "en",
           targetfile = "tinto_coherent.pdf",
        urlaccessdate = "27 abr. 2024"
}