Cosmic strings have been on the ropes [my bad] since the late 90's. The original concept predicted the CMB would be non-guassian. COBE dealt the first blow and WMAP applied the coup-de-grace. As noted in the referenced paper:
"...the CMB anisotropieswere consistent with a Gaussian signature, while numerical simulations of all topological defects show that they would leave distinct non-Gaussian signatures in the CMB."
The cosmic string scenario predicted they would arise from GUT phase transitions, and be abundant. Again from the paper:
"If we expect GUT scale strings to form, one defect would be created per causal horizon. This leads to a possibility of ~13000 cosmic strings in CMB.The gravitational signatures of these strings will persist in the CMB even if the strings themselves have dissipated."
From another recent paper:
http://www.arxiv.org/abs/astro-ph/0410073
Cosmic Strings Reborn?
"Cosmic strings were very popular in the eighties, and much of the nineties,
because they seemed to offer a neat alternative to inflation as a means of generating the primordial density perturbations from which galaxies and clusters eventually grew. In particular, for GUT-scale strings, the predicted string tension was about right to explain their magnitude. But towards the millennium their popularity waned, swept away by the avalanche of data, especially the microwave background measurements from COBE, BOOMERanG, and, more recently, WMAP. This eventually showed beyond doubt that cosmic strings or other topological defects could not provide an adequate explanation for the bulk of the density perturbations."
The 2 sigma result [which is not very significant as noted by SpaceTiger] for CSL-1 reported by Wright & Lo is rather optimistic when you look at the overall data. For instance:
"We have also investigated claims of a possible cosmic string detection of the object CSL-1, and found little evidence of a string at this position. For the proposed string mass... CMB temperatures at the location of CSL-1 would require the string to have been moving very relativistically, with v~0 96c. We conclude that this is unlikely,"
While the evidence is not damning, it's a bear market for cosmic strings.