We perform a multiparameter likelihood analysis to compare measurements of the cosmic microwave background (CMB) power spectra with predictions from models involving cosmic strings. Adding strings to the standard case of a primordial spectrum with power-law tilt
ns, we find a 2

detection of strings:
f10=0.11±0.05, where
f10 is the fractional contribution made by strings in the temperature power spectrum (at
![[script-l]](http://scitation.aip.org/stockgif3/ell.gif)
=10). CMB data give moderate preference to the model
ns=1 with cosmic strings over the standard zero-strings model with variable tilt. When additional non-CMB data are incorporated, the two models become on a par. With variable
ns and these extra data, we find that
f10<0.11, which corresponds to
Gµ<0.7×10
-6 (where
µ is the string tension and
G is the gravitational constant).