Results 51 to 60 of about 2,402,391 (371)
Single-Cell Hi-C Technologies and Computational Data Analysis. [PDF]
Adv Sci (Weinh)This review provides a detailed examination of scHi‐C technologies, offering quantitative evaluations of 13 protocols. It addresses computational challenges arising from data sparsity and presents systematic insights into data analysis methods, including clustering, TAD calling and 3D reconstruction.
Dautle MA, Chen Y.
europepmc +2 more sources
Outskirts of Galaxy Clusters [PDF]
Space Science Reviews, 2013 52 pages. Review paper. Accepted for publication in Space Science Reviews (eds: S. Ettori, M. Meneghetti). This is a product of the work done by an international team at the International Space Science Institute (ISSI) in Bern on "Astrophysics and Cosmology with Galaxy Clusters: the X-ray and Lensing View"
T. H. Reiprich +7 more
openaire +4 more sources
Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey [PDF]
, 2015 We study the characteristics of the galaxy cluster samples expected from the European Space Agency's Euclid satellite and forecast constraints on parameters describing a variety of cosmological models.
B. Sartoris +15 more
semanticscholar +1 more source
THE DETERMINATION OF THE MORPHOLOGICAL TYPES OF GALAXY CLUSTERS USING CLUSTER CARTOGRAPHY
Odessa Astronomical Publications, 2016 We discuss the possibility of using the Cluster Cartography set for the determined the morphological types of galaxy clusters. The applied morphological scheme was proposed by Panko (2013).
E. A. Panko, S. I. Emelyanov
doaj +1 more source
The Hubble constant from galaxy cluster scaling-relation and SNe Ia observations: a consistency test
European Physical Journal C: Particles and Fields, 2023 In this paper, we propose a self-consistent test for a Hubble constant estimate using galaxy cluster and type Ia supernovae (SNe Ia) observations. The approach consists, in a first step, of obtaining the observational value of the galaxy cluster scaling ...
Kamal Bora, R. F. L. Holanda
doaj +1 more source
ILLUMINATING A DARK LENS: A TYPE Ia SUPERNOVA MAGNIFIED BY THE FRONTIER FIELDS GALAXY CLUSTER ABELL 2744 [PDF]
, 2015 SN HFF14Tom is a Type Ia SN discovered at z = 1.3457 ± 0.0001 ?> behind the galaxy cluster Abell 2744 (z = 0.308). In a cosmology-independent analysis, we find that HFF14Tom is 0.77 ± 0.15 mag brighter than unlensed Type Ia SNe at similar redshift ...
S. Rodney +29 more
semanticscholar +1 more source
Do cluster properties affect the quenching rate? [PDF]
, 2014 The quenching rate is known to depend on galaxy stellar mass and environment, however, possible dependences on the hosting halo properties, such as mass, richness, and dynamical status, are still debated.
Andreon, S., Raichoor, A.
core +2 more sources
Supernovae in Galaxy Clusters [PDF]
International Astronomical Union Colloquium, 2005 SummaryWe present the results of several surveys for supernovae (SNe) in galaxy clusters. SNe discovered in deep, archival HST images were used to measure the cluster SN Ia rate to z = 1. A search for SNe in nearby (0.06 ≤ z ≤ 0.2) Abell galaxy clusters yielded 15 SNe, 12 of which were spectroscopically confirmed.
Alexei V. Filippenko +5 more
openaire +4 more sources
Quenched Galaxies in Clusters of Galaxies and Their Outskirts [PDF]
Astrophysical Bulletin, 2020 Based on the SDSS data, the properties of galaxies with quenched star formation (QGs) within the "splashback"-radius of galaxy clusters $R_{\rm sp}$ and beyond it have been studied.
F. G. Kopylova, Alexander I. Kopylov
openaire +3 more sources
SEARCH FOR EXTENDED GAMMA-RAY EMISSION FROM THE VIRGO GALAXY CLUSTER WITH FERMI-LAT [PDF]
, 2015 Galaxy clusters are one of the prime sites to search for dark matter (DM) annihilation signals. Depending on the substructure of the DM halo of a galaxy cluster and the cross sections for DM annihilation channels, these signals might be detectable by the
M. Ackermann +152 more
semanticscholar +1 more source