Now showing items 1-3 of 3

    • 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 ...
    • Enabling a High Throughput Real Time Data Pipeline for a Large Radio Telescope Array with GPUs 

      Pfister, Hanspeter; Edgar, Richard G; Mitchell, Daniel A; Ord, Stephen M; Greenhill, Lincoln J.; Clark, Michael A.; Dale, Kevin; Wayth, Randall B. (Elsevier, 2010)
      The Murchison Widefield Array (MWA) is a next-generation radio telescope currently under construction in the remote Western Australia Outback. Raw data will be generated continuously at 5 GiB s\(^{−1}\), grouped into 8 s ...
    • Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole 

      Lenc, E.; Gaensler, B; Sun, X. H.; Sadler, E. M.; Willis, A. G.; Barry, N.; Beardsley, A. P.; Bell, M. E.; Bernardi, G.; Bowman, J. D.; Briggs, F.; Callingham, J. R.; Cappallo, R. J.; Carroll, P.; Corey, B. E.; Oliveira-Costa, A. de; Deshpande, A. A.; Dillon, J. S.; Dwarkanath, K. S.; Emrich, D.; Ewall-Wice, A.; Feng, L.; For, B.-Q.; Goeke, R.; Greenhill, Lincoln Jared; Hancock, P.; Hazelton, B. J.; Hewitt, J. N.; Hindson, L.; Hurley-Walker, N.; Johnston-Hollitt, M.; Jacobs, D. C.; Kapińska, A. D.; Kaplan, D. L.; Kasper, Justin C.; Kim, H.-S.; Kratzenberg, E.; Line, J.; Loeb, Abraham; Lonsdale, C. J.; Lynch, M. J.; McKinley, B.; McWhirter, S. R.; Mitchell, D. A.; Morales, M. F.; Morgan, E.; Morgan, J.; Murphy, T.; Neben, A. R.; Oberoi, D.; Offringa, A. R.; Ord, S; Paul, S.; Pindor, B.; Pober, J. C.; Prabu, T.; Procopio, P.; Riding, J.; Rogers, A. E. E.; Roshi, A. (American Astronomical Society, 2016)
      We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), covering 625 deg^2 centered on RA=0 h, Dec=-27 deg. The sensitivity available in our deep observations allows an in-band, ...