H i as a probe of the large-scale structure in the post-reionization universe

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 1, 2010, Pages 567-580

  Bagla, J S ^a   Khandai, Nishikanta ^a,b   Datta, Kanan K ^a,c,d  

^a HARISH CHANDRA RESEARCH INSTITUTE   (India)

^b CARNEGIE MELLON UNIVERSITY   (United States)

^c INDIAN INSTITUTE OF TECHNOLOGY   (India)

^d STOCKHOLM UNIVERSITY   (Sweden)

Author keywords

Galaxies: evolution; Galaxies: ISM; Large scale structure of Universe; Methods: numerical; Radio lines: galaxies

Indexed keywords

DISTRIBUTION FUNCTIONS; GALAXIES; GRAVITATION; NUMERICAL METHODS;

DIRECT-DETECTION; GALAXIES: ISM; GALAXY EVOLUTION; GIANT METERWAVE RADIO TELESCOPES; LARGE SCALE STRUCTURE OF UNIVERSE; METHOD: NUMERICAL; RADIO LINES:GALAXIES; RED SHIFT; REIONIZATION; STATISTICAL DETECTION;

VISIBILITY;

EID: 77956398550     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16933.x     Document Type: Article

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