DETECTION OF SIGNALS FROM COSMIC REIONIZATION USING RADIO INTERFEROMETRIC SIGNAL PROCESSING
暂无分享,去创建一个
[1] H I 21 Centimeter Absorption beyond the Epoch of Reionization , 2002, astro-ph/0205169.
[2] C. Carilli,et al. Synthesis Imaging in Radio Astronomy II , 1999 .
[3] Judd D. Bowman,et al. FOREGROUND CONTAMINATION IN INTERFEROMETRIC MEASUREMENTS OF THE REDSHIFTED 21 cm POWER SPECTRUM , 2008, 0807.3956.
[4] Saleem Zaroubi,et al. Non-parametric foreground subtraction for 21-cm epoch of reionization experiments , 2009 .
[5] Andrew J. Benson,et al. Decontamination of cosmological 21-cm maps , 2007, 0712.0497.
[6] Matias Zaldarriaga,et al. Will point sources spoil 21-cm tomography? , 2008, 0807.3952.
[7] J. Hewitt,et al. Statistical EOR detection and the Mileura Widefield Array , 2006 .
[8] S. Zaroubi,et al. Foreground simulations for the LOFAR-epoch of reionization experiment , 2008, 0804.1130.
[9] Steven Furlanetto,et al. Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe , 2006 .
[10] S. Zaroubi,et al. Fast Large-Scale Reionization Simulations , 2008, 0809.1326.
[11] IoA,et al. Radio Foregrounds for the 21 Centimeter Tomography of the Neutral Intergalactic Medium at High Redshifts , 2001, astro-ph/0109241.
[12] Matias Zaldarriaga,et al. Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization , 2005, astro-ph/0512263.
[13] W. D. Cotton,et al. Pixelization and dynamic range in radio interferometry , 2008, 0809.1447.
[14] J. Baldwin,et al. The 6C survey of radio sources – II. The zone $30^\circ \lt \delta \lt 51^\circ, 08^\text h30^\text m\lt\alpha\lt17^\text h30^\text m$ , 1988 .
[15] Robert H. Becker,et al. Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z ∼ 6 Quasars. II. A Sample of 19 Quasars , 2005, astro-ph/0512082.
[16] S. Zaroubi,et al. Foregrounds for observations of the cosmological 21 cm line - I. First Westerbork measurements of Galactic emission at 150 MHz in a low latitude field , 2009, 0904.0404.
[17] D. Barnes,et al. Prospects for Redshifted 21 cm Observations of Quasar H II Regions , 2005, astro-ph/0506045.
[18] M. A. Voronkov,et al. The Cotton-Schwab Clean At Ultra-High Dynamic Range , 2004 .
[19] Roger J. Cappallo,et al. Real-Time Calibration of the Murchison Widefield Array , 2008, IEEE Journal of Selected Topics in Signal Processing.
[20] Judd D. Bowman,et al. IMPROVING FOREGROUND SUBTRACTION IN STATISTICAL OBSERVATIONS OF 21 cm EMISSION FROM THE EPOCH OF REIONIZATION , 2006 .
[21] S. Bhatnagar,et al. Scale sensitive deconvolution of interferometric images - I. Adaptive Scale Pixel (Asp) decomposition , 2004 .
[22] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE * OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[23] R. Davies,et al. Astronomical Society of the Pacific Conference Series , 2010 .
[24] B. Skiff,et al. VizieR Online Data Catalog , 2009 .