Now showing items 2231-2240 of 70736

    • Greig, B.; Trott, Cathryn ; Barry, Nichole ; Mutch, S.J.; Pindor, B.; Webster, R.L.; Wyithe, J.S.B. (2021)
      We use the latest multiredshift (z = 6.5-8.7) upper limits on the 21-cm signal from the Murchison Widefield Array (MWA) to explore astrophysical models which are inconsistent with the data. We explore these limits in the ...
    • Line, Jack ; Mitchell, D.A.; Pindor, B.; Riding, J.L.; McKinley, Ben ; Webster, R.L.; Trott, Cathryn ; Hurley-Walker, Natasha ; Offringa, A.R. (2020)
      To make a power spectrum (PS) detection of the 21-cm signal from the Epoch of Reionisation (EoR), one must avoid/subtract bright foreground sources. Sources such as Fornax A present a modelling challenge due to spatial ...
    • Watkinson, C.A.; Trott, Cathryn ; Hothi, I. (2021)
      Numerous studies have established the theoretical potential of the 21-cm bispectrum to boost our understanding of the Epoch of Reionization (EoR). We take a first look at the impact of foregrounds (FGs) and instrumental ...
    • Joseph, R.C.; Trott, Cathryn ; Wayth, Randall ; Nasirudin, A. (2020)
      Detecting a signal from the Epoch of Reionization (EoR) requires an exquisite understanding of Galactic and extragalactic foregrounds, low-frequency radio instruments, instrumental calibration, and data analysis pipelines. ...
    • Li, W.; Pober, J.C.; Barry, N.; Hazelton, B.J.; Morales, M.F.; Trott, Cathryn ; Lanman, A.; Wilensky, M.; Sullivan, I.; Beardsley, A.P.; Booler, Tom ; Bowman, J.D.; Byrne, R.; Crosse, B.; Emrich, David ; Franzen, Thomas ; Hasegawa, K.; Horsley, L.; Johnston-Hollitt, Melanie ; Jacobs, D.C.; Jordan, Chris ; Joseph, R.C.; Kaneuji, T.; Kaplan, D.L.; Kenney, David ; Kubota, K.; Line, Jack ; Lynch, Christene ; McKinley, Ben ; Mitchell, D.A.; Murray, Steven ; Pallot, D.; Pindor, B.; Rahimi, M.; Riding, J.; Sleap, G.; Steele, K.; Takahashi, K.; Tingay, Steven ; Walker, Mia ; Wayth, Randall ; Webster, R.L.; Williams, Andrew ; Wu, C.; Wyithe, J.S.B.; Yoshiura, S.; Zheng, Q. (2019)
      The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to perform sky-model and redundant interferometric ...
    • Yoshiura, S.; Ichiki, K.; Pindor, B.; Takahashi, K.; Tashiro, H.; Trott, Cathryn (2019)
      Observation of the 21 cm line signal from neutral hydrogen during the epoch of reionization is challenging due to extremely bright Galactic and extragalactic foregrounds and complicated instrumental calibration. A reasonable ...
    • Allison, J.R.; Sadler, E.M.; Amaral, A.D.; An, T.; Curran, S.J.; Darling, J.; Edge, A.C.; Ellison, S.L.; Emig, K.L.; Gaensler, B.M.; Garratt-Smithson, L.; Glowacki, Marcin ; Grasha, K.; Koribalski, B.S.; Lagos, C.D.P.; Lah, P.; Mahony, E.K.; Mao, S.A.; Morganti, R.; Moss, V.A.; Pettini, M.; Pimbblet, K.A.; Power, C.; Salas, P.; Staveley-Smith, L.; Whiting, M.T.; Wong, O.I.; Yoon, H.; Zheng, Z.; Zwaan, M.A. (2022)
      We describe the scientific goals and survey design of the First Large Absorption Survey in H i (FLASH), a wide field survey for 21-cm line absorption in neutral atomic hydrogen (H i) at intermediate cosmological redshifts. ...
    • Arcus, W.R.; James, Clancy ; Ekers, Ronald ; Wayth, Randall (2022)
      We model the fast radio burst (FRB) dispersion measure (DM) distribution for the Five-hundred-meter Aperture Spherical Telescope (FAST) and compare this with the four FRBs published in the literature to date. We compare ...
    • James, Clancy ; Prochaska, J.X.; Macquart, Jean-Pierre ; North-Hickey, F.O.; Bannister, K.W.; Dunning, A. (2022)
      We develop a sophisticated model of fast radio burst (FRB) observations, accounting for the intrinsic cosmological gas distribution and host galaxy contributions, and give the most detailed account yet of observational ...
    • James, Clancy ; Anderson, Gemma ; Wen, L.; Bosveld, J.; Chu, Q.; Kovalam, M.; Slaven-Blair, T.J.; Williams, Andrew (2019)
      We examine how fast radio burst (FRB)-like signals predicted to be generated during the merger of a binary neutron star (BNS) may be detected in low-frequency radio observations triggered by the aLIGO/Virgo gravitational-wave ...