Detecting neutral hydrogen in emission at redshift z ≃ 1

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 3, 2011, Pages 2580-2593

  Khandai, Nishikanta ^a   Sethi, Shiv K ^a,b   Di Matteo, Tiziana ^a   Croft, Rupert A C ^a   Springel, Volker ^c,d   Jana, Anirban ^e   Gardner, Jeffrey P ^f  

^a CARNEGIE MELLON UNIVERSITY   (United States)

^b RAMAN RESEARCH INSTITUTE   (India)

^c HEIDELBERG INSTITUTE FOR THEORETICAL STUDIES   (Germany)

^d UNIVERSITY OF HEIDELBERG   (Germany)

^e PITTSBURGH SUPERCOMPUTING CENTER   (United States)

^f UNIVERSITY OF WASHINGTON   (United States)

Author keywords

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

Indexed keywords

COSMOLOGY; FUNCTIONS; HYDROGEN; INTERFEROMETERS;

'CURRENT; DETECTABILITY; GALAXY EVOLUTION; LARGE N; LARGE SCALE STRUCTURE OF UNIVERSE; MASS FUNCTIONS; N-BODY SIMULATION; NEUTRAL HYDROGEN; RADIO LINES:GALAXIES; RED SHIFT;

GALAXIES;

EID: 79961020783     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18881.x     Document Type: Article

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