The candidates for the U-lines at 1377 and 1394 MHz observed in IRC + 10216 are surveyed by using the RCCSD(T)/aug-cc-pVTZ and/or RCCSD(T)/cc-pVTZ methods. The C6H- anion and the C6H((2)Sigma(+)) radical are proposed as the probable candidates, respectively. The scaling arguments used to improve the predictions of rotational constants are reasonable and represent only a small (within ca. 0.1%) correction to the computed values.