Bryan, G. L. & Norman, M. L. Statistical properties of X-ray clusters: analytic and numerical comparisons. Astrophys. J. 495, 80–99 (1998).
Chiang, Y.-K., Makiya, R., Ménard, B. & Komatsu, E. The cosmic thermal history probed by Sunyaev–Zeldovich effect tomography. Astrophys. J. 902, 56 (2020).
Li, Q. et al. THE THREE HUNDRED Project: the evolution of physical baryon profiles. Mon. Not. R. Astron. Soc. 523, 1228–1246 (2023).
Rohr, E. et al. The cooler past of the intracluster medium in TNG-cluster. Mon. Not. R. Astron. Soc. 536, 1226–1250 (2025).
Mantz, A. B. et al. The XXL Survey. XVII. X-ray and Sunyaev–Zel’dovich properties of the redshift 2.0 galaxy cluster XLSSC 122. Astron. Astrophys. 620, 2 (2018).
Gobat, R. et al. Sunyaev-Zel’dovich detection of the galaxy cluster Cl J1449+0856 at z = 1.99: the pressure profile in uv space. Astron. Astrophys. 629, 104 (2019).
Di Mascolo, L. et al. Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. Nature 615, 809–812 (2023).
Miller, T. B. et al. A massive core for a cluster of galaxies at a redshift of 4.3. Nature 556, 469–472 (2018).
Chapman, S. C. et al. Brightest cluster galaxy formation in the z = 4.3 protocluster SPT 2349-56: discovery of a radio-loud active galactic nucleus. Astrophys. J. 961, 120 (2024).
Zhou, D. et al. A large molecular gas reservoir in the protocluster SPT2349-56 at z = 4.3. Astrophys. J. Lett. 982, 17 (2025).
Chapman, S. C. et al. An overabundance of radio-AGN in the SPT2349-56 protocluster: preheating the intra-cluster medium. Preprint at https://arxiv.org/abs/2511.17814 (2025).
Sunyaev, R. A. & Zeldovich, Y. B. Formation of clusters of galaxies; protocluster fragmentation and intergalactic gas heating. Astron. Astrophys. 20, 189 (1972).
Sunyaev, R. A. & Zeldovich, I. B. Microwave background radiation as a probe of the contemporary structure and history of the universe. Annu. Rev. Astron. Astrophys. 18, 537–560 (1980).
Voit, G. M. Tracing cosmic evolution with clusters of galaxies. Rev. Mod. Phys. 77, 207–258 (2005).
Wang, G. C. P. et al. Overdensities of submillimetre-bright sources around candidate protocluster cores selected from the South Pole Telescope survey. Mon. Not. R. Astron. Soc. 508, 3754–3770 (2021).
Hill, R. et al. Megaparsec-scale structure around the protocluster core SPT2349-56 at z = 4.3. Mon. Not. R. Astron. Soc. 495, 3124–3159 (2020).
McCarthy, I. G., Babul, A., Bower, R. G. & Balogh, M. L. Towards a holistic view of the heating and cooling of the intracluster medium. Mon. Not. R. Astron. Soc. 386, 1309–1331 (2008).
Henden, N. A., Puchwein, E. & Sijacki, D. The redshift evolution of X-ray and Sunyaev-Zel’dovich scaling relations in the FABLE simulations. Mon. Not. R. Astron. Soc. 489, 2439–2470 (2019).
Bennett, J. S., Sijacki, D., Costa, T., Laporte, N. & Witten, C. The growth of the gargantuan black holes powering high-redshift quasars and their impact on the formation of early galaxies and protoclusters. Mon. Not. R. Astron. Soc. 527, 1033–1054 (2024).
Carlstrom, J. E., Holder, G. P. & Reese, E. D. Cosmology with the Sunyaev-Zel’dovich effect. Annu. Rev. Astron. Astrophys. 40, 643–680 (2002).
Mroczkowski, T. et al. Astrophysics with the spatially and spectrally resolved Sunyaev-Zeldovich effects. A millimetre/submillimetre probe of the warm and hot universe. Space Sci. Rev. 215, 17 (2019).
Spacek, A., Scannapieco, E., Cohen, S., Joshi, B. & Mauskopf, P. Constraining AGN feedback in massive ellipticals with South Pole telescope measurements of the thermal Sunyaev-Zel’dovich effect. Astrophys. J. 819, 128 (2016).
Arnaud, M. et al. The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the YSZ–M500 relation. Astron. Astrophys. 517, 92 (2010).
Maughan, B. J., Giles, P. A., Randall, S. W., Jones, C. & Forman, W. R. Self-similar scaling and evolution in the galaxy cluster X-ray luminosity-temperature relation. Mon. Not. R. Astron. Soc. 421, 1583–1602 (2012).
Planck Collaboration. Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts. Astron. Astrophys. 571, 20 (2014).
McDonald, M. et al. The remarkable similarity of massive galaxy clusters from z ~ 0 to z ~ 1.9. Astrophys. J. 843, 28 (2017).
Mostoghiu, R. et al. The Three Hundred Project: the evolution of galaxy cluster density profiles. Mon. Not. R. Astron. Soc. 483, 3390–3403 (2019).
Marrone, D. P. et al. LoCuSS: the Sunyaev-Zel’dovich effect and weak-lensing mass scaling relation. Astrophys. J. 754, 119 (2012).
Bocquet, S. et al. Cluster cosmology constraints from the 2500 deg2 SPT-SZ survey: inclusion of weak gravitational lensing data from Magellan and the Hubble Space Telescope. Astrophys. J. 878, 55 (2019).
Bigwood, L., Bourne, M. A., Iršič, V., Amon, A. & Sijacki, D. The case for large-scale AGN feedback in galaxy formation simulations: insights from XFABLE. Mon. Not. R. Astron. Soc. 542, 3206–3230 (2025).
Lucie-Smith, L. et al. Cosmological feedback from a halo assembly perspective. Phys. Rev. D. 112, 063541 (2025).
Nagarajan, A. et al. Weak-lensing mass calibration of the Sunyaev-Zel’dovich effect using APEX-SZ galaxy clusters. Mon. Not. R. Astron. Soc. 488, 1728–1759 (2019).
Andreon, S. et al. Witnessing the intracluster medium assembly at the cosmic noon in JKCS 041. Mon. Not. R. Astron. Soc. 522, 4301–4309 (2023).
van Marrewijk, J. et al. XLSSC 122 caught in the act of growing up: spatially resolved SZ observations of a z = 1.98 galaxy cluster. Astron. Astrophys. 689, 41 (2024).
Remus, R.-S., Dolag, K. & Dannerbauer, H. The young and the wild: what happens to protoclusters forming at redshift z ≈ 4? Astrophys. J. 950, 191 (2023).
Aljamal, E. et al. Mass proxy quality of massive halo properties in the IllustrisTNG and FLAMINGO simulations: I. Hot gas. Mon. Not. R. Astron. Soc. 544, 67–94 (2025).
Bassini, L. et al. The DIANOGA simulations of galaxy clusters: characterising star formation in protoclusters. Astron. Astrophys. 642, 37 (2020).
Lim, S. et al. Is there enough star formation in simulated protoclusters? Mon. Not. R. Astron. Soc. 501, 1803–1822 (2021).
Hlavacek-Larrondo, J. et al. X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: tracing the evolution of AGN feedback in clusters of galaxies out to z = 1.2. Astrophys. J. 805, 35 (2015).
Valentino, F. et al. A giant Lyα nebula in the core of an X-ray cluster at z = 1.99: implications for early energy injection. Astrophys. J. 829, 53 (2016).
Cielo, S., Babul, A., Antonuccio-Delogu, V., Silk, J. & Volonteri, M. Feedback from reorienting AGN jets. I. Jet-ICM coupling, cavity properties and global energetics. Astron. Astrophys. 617, 58 (2018).
Heckman, T. M. & Best, P. N. A global inventory of feedback. Galaxies 11, 21 (2023).
Heckman, T. M., Roy, N., Best, P. N. & Kondapally, R. Mergers, radio jets, and quenching star formation in massive galaxies: quantifying their synchronized cosmic evolution and assessing the energetics. Astrophys. J. 977, 125 (2024).
Rennehan, D., Babul, A., Moa, B. & Davé, R. The OBSIDIAN model: three regimes of black hole feedback. Mon. Not. R. Astron. Soc. 532, 4793–4809 (2024).
Huško, F. et al. A hybrid active galactic nucleus feedback model with spinning black holes, winds and jets. Preprint at arxiv.org/abs/2509.05179 (2025)
Begelman, M. C. & Cioffi, D. F. Overpressured cocoons in extragalactic radio sources. Astrophys. J. Lett. 345, 21 (1989).
Nesvadba, N. P. H., Lehnert, M. D., De Breuck, C., Gilbert, A. M. & van Breugel, W. Evidence for powerful AGN winds at high redshift: dynamics of galactic outflows in radio galaxies during the “Quasar Era”. Astron. Astrophys. 491, 407–424 (2008).
Fabian, A. C. Observational evidence of active galactic nuclei feedback. Annu. Rev. Astron. Astrophys. 50, 455–489 (2012).
Chadayammuri, U., Tremmel, M., Nagai, D., Babul, A. & Quinn, T. Fountains and storms: the effects of AGN feedback and mergers on the evolution of the intracluster medium in the ROMULUSC simulation. Mon. Not. R. Astron. Soc. 504, 3922–3937 (2021).
Grayson, S., Scannapieco, E. & Davé, R. Distinguishing active galactic nuclei feedback models with the thermal Sunyaev–Zel’dovich effect. Astrophys. J. 957, 17 (2023).
Altamura, E. et al. EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies. Mon. Not. R. Astron. Soc. 520, 3164–3186 (2023).
Gardner, A., Baxter, E., Raghunathan, S., Cui, W. & Ceverino, D. Prospects for studying the mass and gas in protoclusters with future CMB observations. Open J. Astrophys. 7, 2 (2024).
Vogelsberger, M. et al. The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations. Mon. Not. R. Astron. Soc. 474, 2073–2093 (2018).
Huško, F., Lacey, C. G., Schaye, J., Nobels, F. S. J. & Schaller, M. Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters. Mon. Not. R. Astron. Soc. 527, 5988–6020 (2024).
Mantz, A. B. et al. The XXL Survey. V. Detection of the Sunyaev-Zel’dovich effect of the redshift 1.9 galaxy cluster XLSSU J021744.1-034536 with CARMA. Astrophys. J. 794, 157 (2014).
Planck Collaboration. Planck 2015 results. XIII. Cosmological parameters. Astron. Astrophys. 594, 13 (2016).
Bushouse, H. et al. JWST calibration pipeline. Zenodo https://doi.org/10.5281/zenodo.6984365 (2025).
Bradley, L. et al. Astropy/photutils: 2.0.2. Zenodo https://doi.org/10.5281/zenodo.13989456 (2024).
Fujimoto, S. et al. ALMA census of faint 1.2 mm sources down to ~0.02 mJy: extragalactic background light and dust-poor, high-z galaxies. Astrophys. J. Suppl. Ser. 222, 1 (2016).
Fujimoto, S. et al. ALMA Lensing Cluster Survey: deep 1.2 mm number counts and infrared luminosity functions at z = 1–8. Astrophys. J. Suppl. Ser. 275, 36 (2024).
Tazzari, M. Mtazzari/uvplot (v0.1.1). Zenodo https://doi.org/10.5281/zenodo.1003113 (2017).
Wang, T. et al. Discovery of a galaxy cluster with a violently starbursting core at z = 2.506. Astrophys. J. 828, 56 (2016).
Grishin, K. A. et al. Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at z = 2.363 and CARLA-Ser J0950+2743 at z = 2.243. Astron. Astrophys. 693, 1 (2025).
Travascio, A. et al. X-ray view of a massive node of the cosmic web at z = 3 II. Discovery of extended X-ray emission around a hyperluminous QSO. Preprint at arxiv.org/abs/2508.20074 (2025).
Diemer, B. COLOSSUS: a Python toolkit for cosmology, large-scale structure, and dark matter halos. Astrophys. J. Suppl. Ser. 239, 35 (2018).
Diemer, B. & Joyce, M. An accurate physical model for halo concentrations. Astrophys. J. 871, 168 (2019).
Hill, R. et al. Rapid build-up of the stellar content in the protocluster core SPT2349-56 at z = 4.3. Mon. Not. R. Astron. Soc. 512, 4352–4377 (2022).
Vito, F. et al. Fast supermassive black hole growth in the SPT2349–56 protocluster at z = 4.3. Astron. Astrophys. 689, A130 (2024).
Heckman, T. M. & Best, P. N. The coevolution of galaxies and supermassive black holes: insights from surveys of the contemporary Universe. Annu. Rev. Astron. Astrophys. 52, 589–660 (2014).
Nusser, A., Silk, J. & Babul, A. Suppressing cluster cooling flows by self-regulated heating from a spatially distributed population of active galactic nuclei. Mon. Not. R. Astron. Soc. 373, 739–746 (2006).
Jennings, F. J., Babul, A., Davé, R., Cui, W. & Rennehan, D. HYENAS: X-ray bubbles and cavities in the intragroup medium. Mon. Not. R. Astron. Soc. 536, 145–165 (2025).
Kondapally, R. et al. Cosmic evolution of radio-AGN feedback: confronting models with data. Mon. Not. R. Astron. Soc. 523, 5292–5305 (2023).
Venkateshwaran, A. et al. Kinematic analysis of z = 4.3 galaxies in the SPT2349–56 protocluster core. Astrophys. J. 977, 161 (2024).
Spilker, J. S. et al. Ubiquitous molecular outflows in z > 4 massive, dusty galaxies. II. Momentum-driven winds powered by star formation in the early Universe. Astrophys. J. 905, 86 (2020).
Duan, X. & Guo, F. On the energy coupling efficiency of AGN outbursts in galaxy clusters. Astrophys. J. 896, 114 (2020).
O’Dea, C. P. The compact steep-spectrum and gigahertz peaked-spectrum radio sources. Publ. Astron. Soc. Pac. 110, 493–532 (1998).
Yamada, M., Sugiyama, N. & Silk, J. The Sunyaev-Zeldovich effect by cocoons of radio galaxies. Astrophys. J. 522, 66–73 (1999).
Bromberg, O., Nakar, E., Piran, T. & Sari, R. The propagation of relativistic jets in external media. Astrophys. J. 740, 100 (2011).
Cen, R. Global preventive feedback of powerful radio jets on galaxy formation. Proc. Natl Acad. Sci. USA 121, 2402435121 (2024).
Boselli, A., Fossati, M. & Sun, M. Ram pressure stripping in high-density environments. Astron. Astrophys. Rev. 30, 3 (2022).
Astropy Collaboration. The Astropy Project: sustaining and growing a community-oriented open-source project and the latest major release (v5.0) of the core package. Astrophys. J. 935, 167 (2022).
Ginsburg, A. et al. astroquery: an astronomical web-querying package in Python. Astron. J. 157, 98 (2019).
CASA Team. CASA, the common astronomy software applications for radio astronomy. Publ. Astron. Soc. Pac. 134, 114501 (2022).
Hunter, J. D. Matplotlib: a 2D graphics environment. Comput. Sci. Eng. 9, 90–95 (2007).
Harris, C. R. et al. Array programming with NumPy. Nature 585, 357–362 (2020).
The pandas development team. pandas-dev/pandas: Pandas. Zenodo https://doi.org/10.5281/zenodo.3509134 (2025).
Ginsburg, A. et al. radio-astro-tools/spectral-cube: v.0.4.4. Zenodo https://doi.org/10.5281/zenodo.2573901 (2019).
