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The EoR sensitivity of the Murchison Widefield Array
journal contribution
posted on 2023-05-17, 21:54 authored by Beardsley, AP, Hazelton, BJ, Morales, MF, Arcus, W, Barnes, D, Bernardi, G, Bowman, JD, Briggs, FH, Bunton, JD, Cappallo, RJ, Corey, BE, Deshpande, A, deSouza, L, Emrich, D, Gaensler, BM, Goeke, R, Greenhill, LJ, Herne, D, Hewitt, JN, Johnston-Hollitt, M, Kaplan, DL, Kasper, JC, Kincaid, BB, Koenig, R, Kratzenberg, E, Lonsdale, CJ, Lynch, MJ, McWhirter, SR, Mitchell, DA, Morgan, E, Oberoi, D, Ord, SM, Pathikulangara, J, Prabu, T, Remillard, RA, Rogers, AEE, Roshi, A, Salah, JE, Sault, RJ, Udaya Shankar, N, Srivani, KS, Stevens, J, Subrahmanyan, R, Tingay, SJ, Wayth, RB, Waterson, M, Webster, RL, Whitney, AR, Williams, A, Williams, CL, Wyithe, JSBUsing the final 128 antenna locations of the MurchisonWidefield Array (MWA), we calculate its sensitivity to the epoch of reionization (EoR) power spectrum of redshifted 21 cm emission for a fiducial model and provide the tools to calculate the sensitivity for any model. Our calculation takes into account synthesis rotation, chromatic and asymmetrical baseline effects, and excludes modes that will be contaminated by foreground subtraction. For the fiducial model, the MWA will be capable of a 14σ detection of the EoR signal with one full season of observation on two fields (900 and 700 h).
History
Publication title
Monthly Notices of the Royal Astronomical Society: LettersVolume
429Pagination
L5-L9ISSN
1745-3933Department/School
School of Natural SciencesPublisher
Oxford University PressPlace of publication
United KingdomRights statement
Copyright 2012 the authorsRepository Status
- Restricted
