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This is the second paper in a series of catalogues of 22-GHz water maserobservations towards the 6.7-GHz methanol masers from the Methanol Multibeam(MMB) Survey. In this paper we present our water maser observations made withthe Australia Telescope Compact Array towards the masers from the MMB surveybetween l = 341$^{\circ}$ through the Galactic centre to l = 6$^{\circ}$. Ofthe 204 6.7-GHz methanol masers in this longitude range we found 101 to haveassociated water maser emission (~ 50 per cent). We found no difference in the6.7-GHz methanol maser luminosities of those with and without water masers. Insources where both maser species are observed, the luminosities of the methanoland water masers are weakly correlated. Studying the mid-infrared colours fromGLIMPSE we found no differences between the colours of those sources associatedwith both methanol and water masers and those associated with just methanol.Comparing the column density and dust mass calculated from the 870-micronthermal dust emission observed by ATLASGAL, we found no differences betweenthose sources associated with both water and methanol masers and those withmethanol only. Since water masers are collisionally pumped and often showemission further away from their accompanying YSO than the radiatively pumped6.7-GHz methanol masers, it is likely water masers are not as tightlycorrelated to the evolution of the parent YSO and so do not trace such a welldefined evolutionary state as 6.7-GHz methanol masers.

A search for water masers associated with class II methanol masers - II. Longitude range 341$^{\circ}$ to 6$^{\circ}$