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CHANG-ES XXXI—A Decade of CHANG-ES: What We Have Learned from Radio Observations of Edge-on Galaxies
DOI: 10.3390/galaxies12030022 Bibcode: 2024Galax..12...22I

Murphy, Eric; Beck, Rainer; Walterbos, Rene +21 more

CHANG-ES (Continuum Halos in Nearby Galaxies—an EVLA Survey) is an ambitious project to target 35 nearby disk galaxies that are edge-on to the line of sight. The orientation permits both the disk and halo regions to be studied. The observations were initially at 1.5 GHz (L-band) and 6.0 GHz (C-band) in a variety of VLA array configurations, and in…

2024 Galaxies
XMM-Newton 10
The Scavenger Hunt for Quasar Samples to Be Used as Cosmological Tools
DOI: 10.3390/galaxies12010004 Bibcode: 2024Galax..12....4D

Bargiacchi, Giada; Dainotti, Maria Giovanna; Lenart, Aleksander Łukasz +1 more

Although the Λ Cold Dark Matter model is the most accredited cosmological model, information at high redshifts (z) between type Ia supernovae (z=2.26) and the Cosmic Microwave Background (z=1100) is crucial to validate this model further. To this end, we have discovered a sample of 1132 quasars up to z=7.54 exhibiting a reduced intrinsic dispersio…

2024 Galaxies
XMM-Newton 10
Galaxy Groups as the Ultimate Probe of AGN Feedback
DOI: 10.3390/galaxies12030024 Bibcode: 2024Galax..12...24E

Finoguenov, Alexis; Gastaldello, Fabio; O'Sullivan, Ewan +3 more

The co-evolution between supermassive black holes and their environment is most directly traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere supplies the central regions with fresh gas, igniting active galactic nuclei (AGN) with long duty cycles. The outflows from the central engine tightly couple with the surroun…

2024 Galaxies
XMM-Newton 6
A Study of Interstellar Medium in the Line of Sight of Transient Neutron Star Low-Mass X-ray Binary, MXB 1659-298, by Timing and Spectral Analysis
DOI: 10.3390/galaxies12040041 Bibcode: 2024Galax..12...41M

Mahato, Rabindra; Baruah, Monmoyuri; Bhattacharya, Parag

This work is dedicated to the study of interstellar medium (ISM) along the line of sight (LOS) of the transient low-mass X-ray binary, MXB 1659-298, capitalizing the high resolving power of XMM-Newton in the soft energy range. We emphasized the analysis of reflection grating spectrometer (RGS) data in the energy range 0.5–2.15 keV, suitable for th…

2024 Galaxies
XMM-Newton 0