Results 81 to 90 of about 12,901,041 (346)
Galaxy groups in the 2dF galaxy redshift survey: Large Scale Structure with Groups
We use the 2dF Galaxy Group Catalogue constructed by Merch\'an & Zandivarez to study the large scale structure of the Universe traced by galaxy groups. We concentrate on the computation of the power spectrum and the two point correlation function.
Abadi +45 more
core +2 more sources
The DEEP2 galaxy redshift survey: the evolution of the blue fraction in groups and the field [PDF]
We explore the behavior of the blue galaxy fraction over the redshift range 0.75
Coil, Alison L. +11 more
core +1 more source
Chandra view of Abell 407: the central compact group of galaxies and the interaction between the radio AGN and the ICM [PDF]
Chao Qiang Geng +10 more
openalex +1 more source
Galaxy groups can be characterized by the radius of decoupling from cosmic expansion, the radius of the caustic of second turnaround, and the velocity dispersion of galaxies within this latter radius.
R. Brent Tully
semanticscholar +1 more source
Solid Harmonic Wavelet Bispectrum for Image Analysis
The Solid Harmonic Wavelet Bispectrum (SHWB), a rotation‐ and translation‐invariant descriptor that captures higher‐order (phase) correlations in signals, is introduced. Combining wavelet scattering, bispectral analysis, and group theory, SHWB achieves interpretable, data‐efficient representations and demonstrates competitive performance across texture,
Alex Brown +3 more
wiley +1 more source
Metallicity structure in X-ray bright galaxy groups
Using Chandra X-ray data of a sample of 15 X-ray bright galaxy groups, we present preliminary results of a coherent study of the radial distribution of metal abundances in the hot gas in groups.
A. Finoguenov +6 more
core +1 more source
The GEEC2 spectroscopic survey of Galaxy groups at 0.8 < z < 1 [PDF]
We present the data release of the Gemini-South GMOS spectroscopy in the fields of 11 galaxy groups at $0.8 50$ per cent complete for galaxies within the virial radius, and with stellar mass $M_{\rm star}>10^{10.3}M_\odot$.
M. Balogh +15 more
semanticscholar +1 more source
This article proposes a lightweight YOLOv4‐based detection model using MobileNetV3 or CSPDarknet53_tiny, achieving 30+ FPS and higher mAP. It also presents a ShuffleNet‐based classification model with transfer learning and GAN‐augmented images, improving generalization and accuracy.
Qingyang Liu, Yanrong Hu, Hongjiu Liu
wiley +1 more source
Groups and Protocluster Candidates in the CLAUDS and HSC-SSP Joint Deep Surveys
Using the extended halo-based group finder developed by Yang et al., which is able to deal with galaxies via spectroscopic and photometric redshifts simultaneously, we construct galaxy group and candidate protocluster catalogs in a wide redshift range (0
Qingyang Li +18 more
doaj +1 more source
X-ray bright groups and their galaxies [PDF]
Combining X-ray data from the ROSAT PSPC and optical data drawn from the literature, we examine in detail the relationship between the X-ray and optical properties of X-ray bright galaxy groups. We find a relationship between optical luminosity and X-ray
Helsdon, Stephen F., Ponman, Trevor J.
core +3 more sources

