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In this paper I will discuss future synergies between the Japanese MAXI X-rayall-sky monitor, to be placed on the International Space Station in 2009, andthe next-generation radio astronomy array LOFAR, currently under constructionin The Netherlands. The wide fields of view and multiple beams of LOFAR willallow, in combination with MAXI, simultaneous all-sky monitoring of the sky inboth the X-ray and radio bands. Focussing on microquasars, X-ray binary jetsystems, I discuss how the combination of MAXI and LOFAR will help us tofurther understand the accretion--outflow coupling in such systems.

MAXI, LOFAR and Microquasars - All-sky monitoring of X-ray binaries in X-rays and radio