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    • CHIPS: The Cosmological HI Power Spectrum Estimator 

      Trott, Cathryn; Pindor, Bart; Procopio, Pietro; Wayth, Randall; Mitchell, Daniel; McKinley, Benjamin; Tingay, Steven; Barry, N.; Beardsley, A.; Bernardi, G.; Bowman, Judd; Briggs, F.; Cappallo, R.; Carroll, P.; de Oliveira-Costa, A.; Dillon, Joshua; Ewall-Wice, A.; Feng, L.; Greenhill, Lincoln Jared; Hazelton, B.; Hewitt, J.; Hurley-Walker, N.; Johnston-Hollitt, M.; Jacobs, Daniel; Kaplan, D.; Kim, HS; Lenc, E.; Line, J.; Loeb, Abraham; Lonsdale, C.; Morales, M.; Morgan, E.; Neben, A.; Thyagarajan, Nithyanandan; Oberoi, D.; Offringa, A.; Ord, S; Paul, S.; Pober, J.; Prabu, T.; Riding, J.; Shankar, N.; Sethi, Shiv; Srivani, K.; Subrahmanyan, R.; Sullivan, I.; Tegmark, M.; Webster, R.; Williams, A.; Williams, C.; Wu, C.; Wyithe, J. (American Astronomical Society, 2016)
      Detection of the cosmological neutral hydrogen signal from the Epoch of Reionization, and estimation of its basic physical parameters, is the principal scientific aim of many current low-frequency radio telescopes. Here ...