We present a study of CHCHCCH, CHCHCN, CHCHCCH, and CHCHCN in TMC-1 using the QUIJOTE line survey. We confirm the presence of CHCHCCH in TMC-1, which was previously reported as tentative by our group. From a detailed study of the ethynyl and cyanide derivatives of CHCH and CHCH in TMC-1, we found that the CHCHCCH/CHCHCN and CHCHCCH/CHCHCN abundance ratios are 1.50.1 and 4.80.5, respectively. The derived CHCHCCH/CHCHCCH abundance ratio is 15.30.8, and that of CHCHCN over CHCHCN is 485. All the single substituted isotopologs of vinyl cyanide have been detected, and we found that the first and second carbon substitutions in CHCHCN provide a C/C ratio in line with that found for other three-carbon bearing species such as HCCNC and HNCCC. However, the third C isotopolog, CHCHCN, presents an increase in its abundance similar to that found for HCCCN. Finally, we observed eight -type transitions of CHCHCN, and we find that their intensity cannot be fitted adopting the dipole moment derived previously. These transitions involve the same rotational levels as those of the -type transitions. From their intensity, we obtain =0.800.03,D, which is found to be in between earlier values derived in the laboratory using intensity measurements or the Stark effect. Our chemical model indicates that the abundances of CHCHCCH, CHCHCN, CHCHCCH, and CHCHCN observed in TMC-1 can be explained in terms of gas-phase reactions.

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