Context : The earliest evolutionary stages of low-mass protostars are characterised by the so-called hot-corino stage , when the newly born star heats the surrounding material and enrich the gas chemically . Studying this evolutionary phase of solar protostars may help understand the evolution of prebiotic complex molecules in the development of planetary systems . Aims : In this paper we focus on the occurrence of glycolaldehyde ( HCOCH _ { 2 } OH ) in young solar analogs by performing the first homogeneous and unbiased study of this molecule in the Class 0 protostars of the nearby Perseus star forming region . Methods : We obtained sub-arcsec angular resolution maps at 1.3mm and 1.4mm of glycolaldehyde emission lines using the IRAM Plateau de Bure ( PdB ) interferometer in the framework of the CALYPSO IRAM large program . Results : Glycolaldehyde has been detected towards 3 Class 0 and 1 Class I protostars out of the 13 continuum sources targeted in Perseus : NGC1333-IRAS2A1 , NGC1333-IRAS4A2 , NGC1333-IRAS4B1 , and SVS13-A . The NGC1333 star forming region looks particularly glycolaldehyde rich , with a rate of occurrence up to 60 % . The glycolaldehyde spatial distribution overlaps with the continuum one , tracing the inner 100 au around the protostar . A large number of lines ( up to 18 ) , with upper-level energies E _ { u } from 37 K up to 375 K has been detected . We derived column densities \geq 10 ^ { 15 } cm ^ { -2 } and rotational temperatures T _ { rot } between 115 K and 236 K , imaging for the first time hot-corinos around NGC1333-IRAS4B1 and SVS13-A . Conclusions : In multiple systems glycolaldehyde emission is detected only in one component . The case of the SVS13-A+B and IRAS4-A1+A2 systems support that the detection of glycolaldehyde ( at least in the present Perseus sample ) indicates older protostars ( i.e . SVS13-A and IRAS4-A2 ) , evolved enough to develop the hot-corino region ( i.e . 100 K in the inner 100 au ) . However , only two systems do not allow us to firmly conclude whether the primary factor leading to the detection of glycolaldehyde emission is the environments hosting the protostars , evolution ( e.g . low value of L _ { submm } / L _ { int } ) , or accretion luminosity ( high L _ { int } ) .