BRIGHT SOURCE SUBTRACTION REQUIREMENTS FOR REDSHIFTED 21 cm MEASUREMENTS
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Abhirup Datta | Judd D. Bowman | Chris L. Carilli | C. Carilli | J. Bowman | A. Datta | C. Carilli | A. Datta
[1] Chris Blake,et al. Measurement of the angular correlation function of radio galaxies from the NRAO VLA Sky Survey , 2002 .
[2] Roger J. Cappallo,et al. Real-Time Calibration of the Murchison Widefield Array , 2008, IEEE Journal of Selected Topics in Signal Processing.
[3] Ue-Li Pen,et al. The GMRT EoR Experiment: Limits on Polarized Sky Brightness at 150 MHz , 2008, 0807.1056.
[4] Mervyn J. Lynch,et al. THE PRECISION ARRAY FOR PROBING THE EPOCH OF RE-IONIZATION: EIGHT STATION RESULTS , 2009, 0904.2334.
[5] Judd D. Bowman,et al. FOREGROUND CONTAMINATION IN INTERFEROMETRIC MEASUREMENTS OF THE REDSHIFTED 21 cm POWER SPECTRUM , 2008, 0807.3956.
[6] Matias Zaldarriaga,et al. Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization , 2005, astro-ph/0512263.
[7] Saleem Zaroubi,et al. Non-parametric foreground subtraction for 21-cm epoch of reionization experiments , 2009 .
[8] S. Bhatnagar,et al. DETECTION OF SIGNALS FROM COSMIC REIONIZATION USING RADIO INTERFEROMETRIC SIGNAL PROCESSING , 2009, 0908.2639.
[9] Alan E. E. Rogers,et al. The Murchison Widefield Array: Design Overview , 2009, Proceedings of the IEEE.
[10] S. Bharadwaj,et al. The multifrequency angular power spectrum of the epoch of reionization 21-cm signal , 2006, astro-ph/0605546.
[11] Matias Zaldarriaga,et al. Will point sources spoil 21-cm tomography? , 2008, 0807.3952.
[12] Andrew J. Benson,et al. Decontamination of cosmological 21-cm maps , 2007, 0712.0497.
[13] Berkeley,et al. Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array , 2007, 0711.4373.
[14] Judd D. Bowman,et al. The Sensitivity of First-Generation Epoch of Reionization Observatories and Their Potential for Differentiating Theoretical Power Spectra , 2005, astro-ph/0507357.
[15] Steven Furlanetto,et al. Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe , 2006 .
[16] S. Zaroubi,et al. Foreground simulations for the LOFAR-epoch of reionization experiment , 2008, 0804.1130.
[17] Klaus Maisinger,et al. Maximum-likelihood estimation of the cosmic microwave background power spectrum from interferometer observations , 2002 .
[18] B. Keating,et al. Observational Constraints on Cosmic Reionization , 2006 .
[19] A Fast Gridded Method for the Estimation of the Power Spectrum of the Cosmic Microwave Background from Interferometer Data with Application to the Cosmic Background Imager , 2002, astro-ph/0205385.
[20] 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 .
[21] Abraham Loeb,et al. In the Beginning: The First Sources of Light and the Reionization of the Universe , 2000 .
[22] S. Zaroubi,et al. Fast Large-Scale Reionization Simulations , 2008, 0809.1326.
[23] P. Peebles. Principles of Physical Cosmology , 1993 .
[24] Garching,et al. Detection and extraction of signals from the epoch of reionization using higher-order one-point statistics , 2008, 0809.2428.
[25] Benedetta Ciardi,et al. The 21-cm emission from the reionization epoch: extended and point source foregrounds , 2004 .
[26] IoA,et al. Radio Foregrounds for the 21 Centimeter Tomography of the Neutral Intergalactic Medium at High Redshifts , 2001, astro-ph/0109241.
[27] Mark Dragovan,et al. Interferometric observation of cosmic microwave background anisotropies , 1999 .
[28] Miguel F. Morales,et al. Toward Epoch of Reionization Measurements with Wide-Field Radio Observations , 2003 .
[29] C. Contaldi,et al. A Fast Gridded Method for the Estimation of the Power Spectrum of the CMB from Interferometer Data with Application to the Cosmic Background Imager , 2022 .
[30] Judd D. Bowman,et al. IMPROVING FOREGROUND SUBTRACTION IN STATISTICAL OBSERVATIONS OF 21 cm EMISSION FROM THE EPOCH OF REIONIZATION , 2006 .
[31] M. Zaldarriaga,et al. 21 Centimeter Fluctuations from Cosmic Gas at High Redshifts , 2003, astro-ph/0311514.
[32] J. Hewitt,et al. Statistical EOR detection and the Mileura Widefield Array , 2006 .