We present continuum observations from the Atacama Large Millimeter/submillimeter Array (ALMA) of 10 high-redshift ($2.2 \le z \le 2.7$) ultraluminous quasars (QSOs) and constrain the presence of hot, ionized, circum-galactic gas in a stacking analysis. We measure a Compton-y parameter profile with a peak value of $(1.7 \pm 1.1) \times 10^{-6}$ at a radius of $\sim50$ kpc. We compare our stacked observations to active galactic nucleus (AGN) feedback wind models and generalized Navarro-Frenk-White (gNFW) pressure profile models to constrain the wind luminosity and halo mass of the stacked QSOs. Our observations constrain the observed stack's halo mass to $<1\times 10^{13}M_{\odot}$ and the stack's feedback wind power $<1\times 10^{12}L_{\odot}$, which is $<1$% of the bolometric luminosity of the quasar.
Search for Galaxy Cluster Candidates in the Cosmic Microwave Background Maps of the Planck Space Mission Using a Convolutional Neural Network Based on the Method of Tracing the Sunyaev-Zeldovich Effect
Forecasts and Simulations for Relativistic Corrections to the Sunyaev-Zeldovich Effect
University of British Columbia（不列颠哥伦比亚大学）；Canadian Institute for Theoretical Astrophysics, University of Toronto（加拿大理论天体物理研究所，多伦多大学）；Berkeley Center for Cosmological Physics, University of California, Berkeley（加州大学伯克利分校宇宙学物理中心）；Kavli Institute for Cosmology Cambridge（卡弗里宇宙学剑桥研究所）；University of Cambridge（剑桥大学）
Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
Princeton University（普林斯顿大学）；Cornell University（康奈尔大学）；Lawrence Berkeley National Laboratory（劳伦斯伯克利国家实验室）；University of California, Berkeley（加州大学伯克利分校）；Stanford University（斯坦福大学）
The kinetic Sunyaev Zeldovich effect as a benchmark for AGN feedback models in hydrodynamical simulations: insights from DESI + ACT
Institute of Astronomy, University of Cambridge（剑桥大学天体物理研究所）；Kavli Institute for Cosmology (KICC), University of Cambridge（剑桥大学卡弗里宇宙学研究所）；Department of Astrophysical Sciences, Princeton University（普林斯顿大学天体物理科学系）；Astrophysics Research Institute, Liverpool John Moores University（利物浦约翰摩尔斯大学天体物理研究所）；Institute for Astronomy, Royal Observatory, Univ. of Edinburgh（爱丁堡大学皇家天文台天体物理研究所）；University of the Western Cape（西开普大学）；South African Astronomical Observatories（南非天文台）；Leiden Observatory, Leiden University（莱顿大学莱顿天文台）；Lorentz Institute for Theoretical Physics, Leiden University（莱顿大学洛伦兹理论物理研究所）
A possible detection of gas rotation in galaxy groups via the kinetic Sunyaev-Zeldovich effect
Astrophysics Research Institute, Liverpool John Moores University（利物浦约翰摩尔斯大学天体物理研究所）；Institute for Astronomy, University of Edinburgh（爱丁堡大学天文研究所）；Universidad Autónoma de Madrid（马德里自治大学）；Centro de Investigación Avanzada en Física Fundamental (CIAFF)（基础物理前沿研究中心）；University of the Western Cape（西开普敦大学）；University of Massachusetts（马萨诸塞大学）；University of Science and Technology of China（中国科学技术大学）；State Key Laboratory of Dark Matter Physics（暗物质物理全国重点实验室）
Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
Institute for Advanced Study（普林斯顿高等研究院）；New York University（纽约大学）；Princeton University（普林斯顿大学）；Flatiron Institute（熨斗研究所）；Columbia University（哥伦比亚大学）；Cornell University（康奈尔大学）
