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21 cm tomography is expected to be difficult in part because of serious foreground contamination.
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2002
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Bowman J. D., Morales M. F., Hewitt J. N., 2007, ApJ, 661, 1
2007
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Wyithe S., Loeb A., Geil P., 2007, ArXiv e-prints: 0709.2955 (astro-ph)
2007
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Gleser L., Nusser A., Benson A. J., 2008, MNRAS, 391, 383
2008
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Jelić V., Zaroubi S., Labropoulos P., Thomas R. M., Bernardi G., Brentjens M. A., de Bruyn A. G., Ciardi B., Harker G., Koopmans L. V. E., Pandey V. N., Schaye J., Yatawatta S., 2008, MNRAS, 389, 1319
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Mao Y., Tegmark M., McQuinn M., Zaldarriaga M., Zahn O., 2008, PRD, 78, 023529
2008
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Benton Metcalf R., 2009, ArXiv e-prints: 0901.0245
2009
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Bowman J. D., Morales M. F., Hewitt J. N., 2009, ApJ, 695, 183
2009
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Harker G., Zaroubi S., Bernardi G., Brentjens M. A., de Bruyn A. G., Ciardi B., Jelic V., Koopmans L. V. E., Labropoulos P., Mellema G., Offringa A., Pandey V. N., Schaye J., Thomas R. M., Yatawatta S., 2009, ArXiv e-prints: 0903.2760 (astro-ph)
2009
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Liu A., Tegmark M., Zaldarriaga M., 2009, MNRAS, 394, 1575
2009
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Metcalf R. B., White S. D. M., 2009, MNRAS, 394, 704
2009
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