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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14588
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dc.contributor.authorSarkar, Tapomoy Guha-
dc.date.accessioned2024-04-18T10:17:11Z-
dc.date.available2024-04-18T10:17:11Z-
dc.date.issued2014-
dc.identifier.urihttps://iopscience.iop.org/article/10.1088/1742-6596/484/1/012033/meta-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14588-
dc.description.abstractWe have investigated the cross-correlation of the Lyman-α forest and redshifted 21-cm emission as a new observational probe of the large scale structures in the post-reionization era, with a significant advantage that the problems of continuum subtraction and foreground removal, and other systematics are expected to be considerably less servere in comparison to the respective auto-correlation signals. In this paper, we have explored the possibility of detecting the baryon acoustic oscillation in the cross-correlation signal. We have developed a formalism to calculate the expected cross-correlation signal and its covariance. We have used this to predict the expected signal and noise for a range of observational parameters.en_US
dc.language.isoenen_US
dc.publisherIOPen_US
dc.subjectPhysicsen_US
dc.subjectLyman-αen_US
dc.subjectCosmological Probesen_US
dc.titleThe cross-correlation of redshited 21-cm signal and Lyman-α forest: A cosmological probeen_US
dc.typeImageen_US
Appears in Collections:Department of Physics

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