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@Article{Braga:2020:CoApIm,
               author = "Braga, Jo{\~a}o",
          affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Coded aperture imaging in high-energy astrophysics",
              journal = "Publications of the Astronomical Society of the Pacific",
                 year = "2020",
               volume = "132",
               number = "1007",
                pages = "e012001",
             keywords = ": instrumentation: detectors  methods: observational  methods: 
                         statistical  space vehicles: instruments  techniques: image 
                         processing  telescopes.",
             abstract = "Hard X-ray and low-energy gamma-ray coded-aperture imaging (CAI) 
                         instruments have been highly successful as high-energy surveyors 
                         and transient-source discoverers and trackers over the past 
                         decades. Albeit having relatively low sensitivity as compared with 
                         focusing instruments, coded-aperture telescopes still represent a 
                         very good choice for simultaneous, high cadence spectral 
                         measurements of individual point sources in large source fields. 
                         Here, I present a review of the fundamentals of CAI instruments in 
                         high-energy astrophysics, with an emphasis on the fundamental 
                         aspects of the technique, coded-mask instrument characteristics, 
                         and properties of the reconstructed images.",
                  doi = "10.1088/1538-3873/ab450a",
                  url = "http://dx.doi.org/10.1088/1538-3873/ab450a",
                 issn = "0004-6280",
             language = "en",
           targetfile = "braga_coded.pdf",
        urlaccessdate = "22 abr. 2021"
}


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