An ultradeep submillimetre map: Beneath the SCUBA confusion limit with lensing and robust source extraction

Monthly Notices of the Royal Astronomical Society

Volumn 368, Issue 1, 2006, Pages 487-496

  Knudsen, K K ^a,b   Barnard, V E ^c   Van Der Werf, P P ^a   Vielva, P ^d   Kneib, J P ^e,f,g   Blain, A W ^f   Barreiro, R B ^d   Ivison, R J ^h   Smail, I ⁱ   Peacock, J A ^h  

^a LEIDEN UNIVERSITY   (Netherlands)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF HAWAII   (United States)

^d INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^e OBSERVATOIRE MIDI PYRÉNÉES   (France)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g OBSERVATOIRE DE MARSEILLE   (France)

^h UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

ⁱ DURHAM UNIVERSITY   (United Kingdom)

Author keywords

Galaxies: high redshift; Methods: data analysis; Submillimetre

Indexed keywords

COSMOLOGY; EXTRACTION; GALAXIES;

BOLOMETER ARRAY; GALAXIES:HIGH-REDSHIFT; LOW SIGNAL-TO-NOISE RATIO; METHODS. DATA ANALYSIS; MEXICAN HAT WAVELET; NON-TRIVIAL TASKS; SOURCE EXTRACTION; STRUCTURED BACKGROUND; SUBMILLIMETRE; ULTRA DEEPS;

SIGNAL TO NOISE RATIO;

EID: 33645814844     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10138.x     Document Type: Article

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