We present new photometric observations of 15 symbiotic stars covering their last orbital cycle ( s ) from 2003.9 to 2007.2 .
We obtained our data by both classical photoelectric and CCD photometry .
Main results are : EG And brightened by \sim 0.3 mag in U from 2003 .
A \sim 0.5 mag deep primary minimum developed in the U light curve ( LC ) at the end of 2006 .
Z And continues its recent activity that began during the 2000 autumn .
A new small outburst started in summer of 2004 with the peak U -magnitude of \sim 9.2 .
During the spring of 2006 the star entered a massive outburst .
It reached its historical maximum at U \sim 8.0 in 2006 July .
AE Ara erupted in 2006 February with \Delta m _ { vis } \sim 1.2 mag .
BF Cyg entered a new active stage in 2006 August .
A brightness maximum ( U \sim 9.4 ) was measured during 2006 September .
CH Cyg persists in a quiescent phase .
During 2006 June – December a \sim 2 mag decline in all colours was measured .
CI Cyg started a new active phase during 2006 May – June .
After 31 years it erupted by about 2 mag in U .
TX CVn maintains a bright stage with U \sim 10.5 from 2003 .
AG Dra entered a new major outburst in 2006 June .
It reached its maximum at U \sim 8.0 in 2006 September .
AR Pav persists at a low level of the activity .
AG Peg ’ s LC profile varies markedly during different orbital cycles .
AX Per continues its quiescent phase .