A simulation-calibrated limit on the H i power spectrum from the GMRT Epoch of Reionization experiment

被引:271
作者
Paciga, Gregory [1 ]
Albert, Joshua G. [1 ]
Bandura, Kevin [2 ,3 ]
Chang, Tzu-Ching [1 ,4 ]
Gupta, Yashwant [5 ]
Hirata, Christopher [6 ]
Odegova, Julia [1 ]
Pen, Ue-Li [1 ]
Peterson, Jeffrey B. [2 ]
Roy, Jayanta [5 ]
Shaw, J. Richard [1 ]
Sigurdson, Kris [7 ]
Voytek, Tabitha [2 ]
机构
[1] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada
[2] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
[3] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[4] Acad Sinica, IAA, Taipei 10617, Taiwan
[5] Tata Inst Fundamental Res, Natl Ctr Radio Astrophys, Pune 411007, Maharashtra, India
[6] CALTECH, Dept Astrophys, Pasadena, CA 91125 USA
[7] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
基金
加拿大创新基金会; 美国国家科学基金会;
关键词
intergalactic medium; cosmology: observations; diffuse radiation; radio lines: general; 21 CM RADIATION; REDSHIFTED; 21-CM; NEUTRAL HYDROGEN; INTERGALACTIC MEDIUM; COSMIC REIONIZATION; FOREGROUND REMOVAL; HII-REGIONS; DARK-AGES; SUBTRACTION; EMISSION;
D O I
10.1093/mnras/stt753
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Giant Metrewave Radio Telescope Epoch of Reionization experiment is an ongoing effort to measure the power spectrum from neutral hydrogen at high redshift. We have previously reported an upper limit of (70 mK)(2) at wavenumbers of k approximate to 0.65 h Mpc(-1) using a basic piecewise-linear foreground subtraction. In this paper, we explore the use of a singular value decomposition to remove foregrounds with fewer assumptions about the foreground structure. Using this method, we also quantify, for the first time, the signal loss due to the foreground filter and present new power spectra adjusted for this loss, providing a revised measurement of a 2 Sigma upper limit at (248 mK)(2) for k = 0.50 h Mpc(-1). While this revised limit is larger than previously reported, we believe it to be more robust and still represents the best current constraint on reionization at z approximate to 8.6.
引用
收藏
页码:639 / 647
页数:9
相关论文
共 61 条
  • [1] Foregrounds for redshifted 21-cm studies of reionization: Giant meter wave radio telescope 153-MHz observations
    Ali, Sk. Saiyad
    Bharadwaj, Somnath
    Chengalur, Jayaram N.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2008, 385 (04) : 2166 - 2174
  • [2] Ananthakrishnan S., 1995, J ASTROPHYSICS ASTRO, V16, P427
  • [3] The EoR sensitivity of the Murchison Widefield Array
    Beardsley, A. P.
    Hazelton, B. J.
    Morales, M. F.
    Arcus, W.
    Barnes, D.
    Bernardi, G.
    Bowman, J. D.
    Briggs, F. H.
    Bunton, J. D.
    Cappallo, R. J.
    Corey, B. E.
    Deshpande, A.
    deSouza, L.
    Emrich, D.
    Gaensler, B. M.
    Goeke, R.
    Greenhill, L. J.
    Herne, D.
    Hewitt, J. N.
    Johnston-Hollitt, M.
    Kaplan, D. L.
    Kasper, J. C.
    Kincaid, B. B.
    Koenig, R.
    Kratzenberg, E.
    Lonsdale, C. J.
    Lynch, M. J.
    McWhirter, S. R.
    Mitchell, D. A.
    Morgan, E.
    Oberoi, D.
    Ord, S. M.
    Pathikulangara, J.
    Prabu, T.
    Remillard, R. A.
    Rogers, A. E. E.
    Roshi, A.
    Salah, J. E.
    Sault, R. J.
    Shankar, N. Udaya
    Srivani, K. S.
    Stevens, J.
    Subrahmanyan, R.
    Tingay, S. J.
    Wayth, R. B.
    Waterson, M.
    Webster, R. L.
    Whitney, A. R.
    Williams, A.
    Williams, C. L.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 429 (01) : L5 - L9
  • [4] Bebbington D. H. O., 1986, MNRAS, V218, P577
  • [5] Evidence for reionization at z ∼ 6:: Detection of a Gunn-Peterson trough in a z=6.28 quasar
    Becker, RH
    Fan, XH
    White, RL
    Strauss, MA
    Narayanan, VK
    Lupton, RH
    Gunn, JE
    Annis, J
    Bahcall, NA
    Brinkmann, J
    Connolly, AJ
    Csabai, I
    Czarapata, PC
    Doi, M
    Heckman, TM
    Hennessy, GS
    Ivezic, Z
    Knapp, GR
    Lamb, DQ
    McKay, TA
    Munn, JA
    Nash, T
    Nichol, R
    Pier, JR
    Richards, GT
    Schneider, DP
    Stoughton, C
    Szalay, AS
    Thakar, AR
    York, DG
    [J]. ASTRONOMICAL JOURNAL, 2001, 122 (06) : 2850 - 2857
  • [6] Subtraction of point sources from interferometric radio images through an algebraic forward modelling scheme
    Bernardi, G.
    Mitchell, D. A.
    Ord, S. M.
    Greenhill, L. J.
    Pindor, B.
    Wayth, R. B.
    Wyithe, J. S. B.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 413 (01) : 411 - 422
  • [7] On using visibility correlations to probe the HI distribution from the dark ages to the present epoch - I. Formalism and the expected signal
    Bharadwaj, S
    Ali, SS
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 356 (04) : 1519 - 1528
  • [8] Toward empirical constraints on the global redshifted 21 cm brightness temperature during the epoch of reionization
    Bowman, Judd D.
    Rogers, Alan E. E.
    Hewitt, Jacqueline N.
    [J]. ASTROPHYSICAL JOURNAL, 2008, 676 (01) : 1 - 9
  • [9] A lower limit of Δz > 0.06 for the duration of the reionization epoch
    Bowman, Judd D.
    Rogers, Alan E. E.
    [J]. NATURE, 2010, 468 (7325) : 796 - 798
  • [10] Brentjens M., 2011, BAAS, V43