Subtraction of point sources from interferometric radio images through an algebraic forward modelling scheme

Monthly Notices of the Royal Astronomical Society

Volumn 413, Issue 1, 2011, Pages 411-422

  Bernardi, G ^a   Mitchell, D A ^a   Ord, S M ^a   Greenhill, L J ^a   Pindor, B ^b   Wayth, R B ^c   Wyithe, J S B ^b  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY OF MELBOURNE   (Australia)

^c ICRAR/Curtin Institute of Radioastronomy   (Australia)

Author keywords

Cosmology: observations; Dark ages; Diffuse radiation; First stars; Methods: data analysis; Methods: numerical; Reionization; Techniques: interferometric

Indexed keywords

ANGULAR DISTRIBUTION; ERRORS; INTERFEROMETRY; NUMERICAL METHODS; SIGNAL TO NOISE RATIO; THERMAL NOISE;

COSMOLOGY OBSERVATIONS; DARK AGE; DIFFUSE RADIATION; FIRST STAR; INTERFEROMETRICS; METHOD: NUMERICAL; METHODS. DATA ANALYSIS; POINT-SOURCES; REIONIZATION; TECHNIQUE: INTERFEROMETRIC;

ALGEBRA;

EID: 79960816080     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.18145.x     Document Type: Article

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