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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2519
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dc.contributor.authorSwarup, G-
dc.date.accessioned2008-06-27T09:12:46Z-
dc.date.available2008-06-27T09:12:46Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 451 - 452en
dc.identifier.urihttp://hdl.handle.net/2248/2519-
dc.description.abstractOne of the most challenging problems in astronomy today is to search for reionization of the neutral hydrogen (HI), which is expected to occur somewhere between redshifts of about 6 to 20. The reionization is likely to result in spatial and spectral fluctuations in emission and absorption in the redshifted 21cm radiation of several milli-Kelvin (mK) in the frequency range of about 100 to 200 MHz. Also there is expected to occur a gradual step of few mK in the global 21cm radiation. Here we discuss various search strategies.en
dc.format.extent56604 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..451Sen
dc.subjectGMRTen
dc.subjectCMBen
dc.subjectReionizationen
dc.subjectRFIen
dc.subjectHIen
dc.subjectEarly universeen
dc.titleSearch for HI Reionization Epoch in the Early Universeen
dc.typeArticleen
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