TY  -  
T1  - Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection 
SN  -  /  
UR  - http://hdl.handle.net/10138/304643 
T3  -  
A1  - Euclid Collaboration; Adam, R.; Kurki-Suonio, H. 
A2  -  
PB  -  
Y1  - 2019 
LA  - eng 
AB  - Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clusters from surveys with a well-known selection function and robust mass estimates, which is particularly challenging at high redshift. The Euclid wide survey will cover 15 000 deg(2) of the sky, avoiding contamination by light from our Galaxy and our solar system in the optical and near-infrared bands, down to magnitude ... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - methods: numerical; galaxies: clusters: general; cosmology: observations; large-scale structure of Universe; DIGITAL SKY SURVEY; INFRARED LUMINOSITY FUNCTION; K-BAND PROPERTIES; VLT DEEP SURVEY; RADIAL-DISTRIBUTION; CANDIDATE CATALOG; STAR-FORMATION; RED-SEQUENCE; DARK ENERGY; APPLES A(2); 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -