S. Pandey, J. C. Hill, A. Alarcon, O. Alves, A. Amon, D. Anbajagane, F. Andrade-Oliveira, N. Battaglia, E. Baxter, K. Bechtol, M. R. Becker, G. M. Bernstein, J. Blazek, S. L. Bridle, E. Calabrese, H. Camacho, A. Campos, A. Carnero Rosell, M. Carrasco Kind, R. Cawthon, C. Chang, R. Chen, P. Chintalapati, A. Choi, J. Cordero, W. Coulton, M. Crocce, C. Davis, J. DeRose, M. Devlin, H. T. Diehl, S. Dodelson, C. Doux, A. Drlica-Wagner, K. Eckert, T. F. Eifler, J. Elvin-Poole, S. Everett, X. Fang, A. Ferté, P. Fosalba, O. Friedrich, M. Gatti, E. Gaztanaga, G. Giannini, V. Gluscevic, D. Gruen, R. A. Gruendl, B. Ried Guachalla, I. Harrison, W. G. Hartley, K. Herner, H. Huang, E. M. Huff, D. Huterer, B. Jain, M. Jarvis, E. Krause, N. Kuropatkin, A. Kusiak, P. Leget, P. Lemos, A. R. Liddle, M. Lokken, N. MacCrann, J. McCullough, K. Moodley, J. Muir, J. Myles, A. Navarro-Alsina, Y. Omori, Y. Park, B. Partridge, A. Porredon, J. Prat, M. Raveri, A. Refregier, R. P. Rollins, A. Roodman, R. Rosenfeld, A. J. Ross, E. S. Rykoff, S. Samuroff, J. Sanchez, C. Sánchez, L. F. Secco, I. Sevilla-Noarbe, S. Shaikh, E. Sheldon, T. Shin, Cristóbal Sifón, C. To, A. Troja, M. A. Troxel, I. Tutusaus, T. N. Varga, N. Weaverdyck, R. H. Wechsler, E. J. Wollack, B. Yanny, B. Yin, Y. Zhang, J. Zuntz, S. S. Allam, D. Bacon, S. Bocquet, D. Brooks, D. L. Burke, J. Carretero, R. Cawthon, M. Costanzi, L. N. da Costa, M. E. da Silva Pereira, T. M. Davis, S. Desai, J. Frieman, J. García-Bellido, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, N. Jeffrey, S. Lee, J. L. Marshall, J. Mena-Fernández, R. Miquel, J. J. Mohr, R. L. C. Ogando, A. A. Plazas Malag'on, A. K. Romer, E. Sanchez, B. Santiago, M. Smith, E. Suchyta, M. E. C. Swanson, D. Thomas, V. Vikram, A. R. Walker, J. Weller, P. Wiseman

We present a joint analysis of weak gravitational lensing (shear) data obtained from the first three years of observations by the Dark Energy Survey and thermal Sunyaev-Zel'dovich (tSZ) effect measurements from a combination of Atacama Cosmology Telescope (ACT) and Planck data. A combined analysis of shear (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) can jointly probe both the distribution of matter and the thermodynamic state of the gas, accounting for the correlated effects of baryonic feedback on both observables. We detect the shear$~\times~$tSZ cross-correlation at a 21$\sigma$ significance, the highest to date, after minimizing the bias from cosmic infrared background leakage in the tSZ map. By jointly modeling the small-scale shear auto-correlation and the shear$~\times~$tSZ cross-correlation, we obtain $S_8 = 0.811^{+0.015}_{-0.012}$ and $\Omega_{\rm m} = 0.263^{+0.023}_{-0.030}$, results consistent with primary CMB analyses from Planck and P-ACT. We find evidence for reduced thermal gas pressure in dark matter halos with masses $M < 10^{14} \, M_{\odot}/h$, supporting predictions of enhanced feedback from active galactic nuclei on gas thermodynamics. A comparison of the inferred matter power suppression reveals a $2-4\sigma$ tension with hydrodynamical simulations that implement mild baryonic feedback, as our constraints prefer a stronger suppression. Finally, we investigate biases from cosmic infrared background leakage in the tSZ-shear cross-correlation measurements, employing mitigation techniques to ensure a robust inference. Our code is publicly available on GitHub.