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We present a fast methodology to produce mock observations of the thermal and kinetic Sunyaev-Zel'dovich (SZ) effects based on the dark matter only $N$-body simulations coupled with the analytic intra-cluster medium model. The methods…

宇宙学与河外天体物理 · 物理学 2023-01-04 Ken Osato , Daisuke Nagai

The Sunyaev-Zeldovich (SZ) effect is a spectral distortion in the Cosmic Microwave Background (CMB), caused due to up-scattering of CMB photons by high energy electron distributions. The largest SZ distortion in the CMB is caused by the hot…

宇宙学与河外天体物理 · 物理学 2015-12-14 Dhruba Dutta Chowdhury

We introduce the Marenostrum-MultiDark SImulations of galaxy Clusters (MUSIC) Dataset, one of the largest sample of hydrodynamically simulated galaxy clusters with more than 500 clusters and 2000 groups. The objects have been selected from…

宇宙学与河外天体物理 · 物理学 2015-06-05 Federico Sembolini , Gustavo Yepes , Marco De Petris , Stefan Gottloeber , Luca Lamagna , Barbara Comis

The baryon content of high-density regions in the universe is relevant to two critical unanswered questions: the workings of nurture effects on galaxies and the whereabouts of the missing baryons. In this paper, we analyze the distribution…

宇宙学与河外天体物理 · 物理学 2015-05-18 A. Faltenbacher , A. Finoguenov , N. Drory

The kinematic Sunyaev-Zel'dovich (kSZ) effect in the cosmic microwave background (CMB) is a powerful probe of gas physics and large-scale structure (LSS) in our universe. We consider the "projected-field" kSZ estimator, which involves…

宇宙学与河外天体物理 · 物理学 2026-05-21 Michael Jacob Rodriguez , Aleksandra Kusiak , Shivam Pandey , J. Colin Hill

We calculate the CMB temperature distortion due to the energetic electrons and positrons produced by dark matter annihilation (Sunyaev-Zel'dovich effect), in dwarf spheroidal galaxies (dSphs). In the calculation we have included two…

宇宙学与河外天体物理 · 物理学 2015-03-17 Feng Huang , Xuelei Chen , Qiang Yuan , Xiaojun Bi

New generation ground and space-based CMB experiments have ushered in discoveries of massive galaxy clusters via the Sunyaev-Zeldovich (SZ) effect, providing a new window for studying cluster astrophysics and cosmology. Many of the newly…

宇宙学与河外天体物理 · 物理学 2015-06-05 Jens Chluba , Daisuke Nagai , Sergey Sazonov , Kaylea Nelson

We present observations of the Sunyaev-Zel'dovich effect (SZE) in the Bullet cluster (1E 0657--56) using the APEX-SZ instrument at 150 GHz with a resolution of 1 arcmin. The main results are maps of the SZE in this massive, merging galaxy…

The Sunyaev-Zel'dovich (SZ) effect expected to be associated with massive star-formation activity produced during the formation of the most luminous bulges of normal galaxies is discussed. Using 1-D chemohydrodynamical models for spheroidal…

The fraction of ionized gas in the Warm Hot Intergalactic Medium induces temperature anisotropies on the Cosmic Microwave Background similar to those of clusters of galaxies. The Sunyaev-Zel'dovich anisotropies due to these low density,…

宇宙学与河外天体物理 · 物理学 2015-06-15 Ricardo Genova-Santos , Isabel Suarez-Velasquez , Fernando Atrio-Barandela , Jan Muecket

In recent years, observations of the Sunyaev-Zeldovich (SZ) effect have had significant cosmological implications and have begun to serve as a powerful and independent probe of the warm and hot gas that pervades the Universe. As a few…

The cosmic thermal history, quantified by the evolution of the mean thermal energy density in the universe, is driven by the growth of structures as baryons get shock heated in collapsing dark matter halos. This process can be probed by…

宇宙学与河外天体物理 · 物理学 2020-10-21 Yi-Kuan Chiang , Ryu Makiya , Brice Ménard , Eiichiro Komatsu

Measurements of the Sunyaev-Zel'dovich (hereafter SZ) effect distortion of the cosmic microwave background provide us with an independent method to derive the gas temperature of galaxy clusters. In merging galaxy clusters the gas…

宇宙学与河外天体物理 · 物理学 2015-05-20 D. A. Prokhorov , Y. Dubois , S. Nagataki

The energy fed by active galactic nuclei to the surrounding diffuse baryons changes their amount, temperature, and distribution; so in groups and in member galaxies it affects the X-ray luminosity and also the Sunyaev-Zel'dovich effect.…

天体物理学 · 物理学 2009-11-10 A. Lapi , A. Cavaliere , G. De Zotti

The peculiar motions of massive halos probe the distribution of matter in the universe, the gravitational potential, and the history of cosmic structure growth. The kinematic Sunyaev-Zeldovich (kSZ) effect offers a robust observational…

宇宙学与河外天体物理 · 物理学 2025-10-24 Patricio A. Gallardo , Yulin Gong , Boryana Hadzhiyska , Yun-Hsin Hsu

Upcoming observatories will be able to detect the kinetic Sunyaev-Zel'dovitch (kSZ) effect with unprecendented signal-to-noise, and cross-correlations with foreground signals such as galaxy counts are a promising way to extract additional…

天体物理学 · 物理学 2007-05-23 Simon DeDeo , David N. Spergel , Hy Trac

We present gas constraints from Sunyaev-Zel'dovich (SZ) effect measurements in a sample of eleven X-ray and infrared (IR) selected galaxy clusters at z >=1, using data from the Sunyaev-Zel'dovich Array (SZA). The cylindrically integrated…

The hot gas in clusters of galaxies emits thermal bremsstrahlung emission that can be probed directly through measurements in the X-ray band with satellites like ROSAT and ASCA. Another probe of this gas comes from its effect on the cosmic…

天体物理学 · 物理学 2007-05-23 John P. Hughes

We use hydrodynamical simulations to assess the impact of radiative cooling and `pre-heating' on predictions for the Sunyaev--Zel'dovich (SZ) effect. Cooling significantly reduces both the mean SZ signal and its angular power spectrum,…

The recent emergence of detections of the kinetic Sunyaev-Zel'dovich (kSZ) effect through cross-correlation techniques is encouraging for the prospects of future cosmic microwave background (CMB) experiments. Extracting information on the…

宇宙学与河外天体物理 · 物理学 2017-01-20 Nicholas Battaglia