We have made new observations of water lines towards the very distant
galaxy IRAS 10214+4724. When combined to our previous observations, th
e new data give further support to the detection of the 2(11) --> 2(02
) para line. We also report more stringent upper limits on the 1(10) -
-> 1(01) and 4(14) --> 3(21) transitions of ortho water.