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Astronomy and Astrophysics, ISSN 0004-6361, 08/2017, Volume 604
The hot electrons in the intra-cluster medium produce a spectral distortion of the cosmic microwave background (CMB) black body emission, the thermal... 
Cosmic background radiation | Large-scale structure of Universe | Galaxies: Clusters: General | galaxies: clusters: general | COSMOLOGY | cosmic background radiation | SCALING RELATIONS | GALAXY CLUSTERS | ASTRONOMY & ASTROPHYSICS | large-scale structure of Universe
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 08/2017, Volume 604, p. A94
The hot electrons in the intra-cluster medium produce a spectral distortion of the cosmic microwave background (CMB) black body emission, the thermal... 
Blackbody | Temperature | Red shift | Parameters | Galaxies | Bias | Elastic scattering | Emission | Relativistic velocity | Distortion | Mapping | Spectra | Low level | Contamination | Relativistic effects | Big Bang theory | Emissions | Galactic clusters | Hot electrons | Temperature effects | Cosmic microwave background | Relativism | Air pollution | Electrons
Journal Article
Nature, ISSN 0028-0836, 12/2015, Volume 528, Issue 7580, pp. 105 - 107
Observations of the cosmic microwave background indicate that baryons account for 5 per cent of the Universe's total energy content(1). In the local Universe,... 
CHANDRA VIEW | HUBBLE-FRONTIER-FIELDS | CATALOG | INTERGALACTIC MEDIUM | GALAXY CLUSTERS | MULTIDISCIPLINARY SCIENCES | GAS | DARK-MATTER | LARGE-SCALE FILAMENT | MERGER | ABELL 2744 | Usage | Research | Analysis | Dark matter (Astronomy) | X-rays | Gravity | Space telescopes | Temperature | Stars & galaxies | Cosmology and Extra-Galactic Astrophysics | Physics | Astrophysics
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 06/2018, Volume 614, p. A38
Context. The mass of galaxy clusters is not a direct observable, nonetheless it is commonly used to probe cosmological models. Based on the combination of all... 
Reconstruction | Gravitation | Gravitational lenses | Galaxies | Computer simulation | Emission | X-ray emissions | Satellite observation | Covariance matrix | Galactic clusters | Algorithms | X rays | Covariance | X-ray measurements | Astronomical models | Cosmology | XMM (spacecraft) | Star & galaxy formation | Cosmological models
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 07/2019, Volume 627, p. A143
Context. Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in... 
WEAK | galaxies: clusters: general | ASTRONOMY & ASTROPHYSICS | MASS CALIBRATION | SIMULATIONS | MODEL | methods: numerical | gravitational lensing: weak | INVERSION | X-rays: galaxies: clusters | GALAXY
Journal Article
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 05/2014, Volume 89, Issue 10
We present a self-consistent interpretation of the very high-energy neutrino signal from the direction of the inner Galaxy, which is a part of the astronomical... 
MILKY-WAY | RADIATION | ASTRONOMY & ASTROPHYSICS | ICECUBE | PHYSICS, PARTICLES & FIELDS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 06/2018, Volume 614
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 02/2015, Volume 574
Context Galaxy clusters can be used as Cosmological probes, but to this end they need to be thoroughly understood. Combining all cluster observables in a... 
OUTER REGIONS | galaxies: clusters: general | SUNYAEV-ZELDOVICH | MASS PROFILES | ELLIPSOIDAL GALAXY CLUSTERS | gravitational lensing: weak | A1689 | SCALING RELATIONS | INTRACLUSTER MEDIUM | EMITTING GAS | ASTRONOMY & ASTROPHYSICS | gravitational lensing: strong | X-rays: galaxies: clusters | TRIAXIAL DARK HALOS | ENTROPY
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 2, pp. 1302 - 1307
Radio relics are Mpc-scale diffuse radio sources at the peripheries of galaxy clusters which are thought to trace outgoing merger shocks. We present XMM-Newton... 
Galaxies: clusters: individual: A2744 | X-rays: galaxies: clusters | BOW SHOCK | LARGE-SCALE STRUCTURE | MERGING GALAXY CLUSTER | galaxies: clusters: individual: A2744 | A2744 | PARTICLE-ACCELERATION | WAVES | ASTRONOMY & ASTROPHYSICS | CHANDRA | EMISSION | EFFICIENCY | XMM-NEWTON
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 01/2019, Volume 621, p. A40
Galaxy clusters are the endpoints of structure formation and are continuously growing through the merging and accretion of smaller structures. Numerical... 
galaxies: clusters: general | large-scale structure of Universe | ANALYTICAL-MODEL | galaxies: clusters: intracluster medium | TURBULENT MOTIONS | FRACTIONS | INTRACLUSTER MEDIUM | COSMOLOGICAL PARAMETER CONSTRAINTS | ASTRONOMY & ASTROPHYSICS | GAS | DARK-MATTER | BARYON CONTENT | SIMULATIONS | X-rays: galaxies: clusters | STELLAR MASS
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 12/2013, Volume 560, p. A64
Journal Article
Journal Article
Archives of Biochemistry and Biophysics, ISSN 0003-9861, 12/2008, Volume 480, Issue 1, pp. 27 - 32
Journal Article