M. Simonte
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View article: ViCTORIA project: The LOFAR-MeerKAT view of active galactic nuclei in Virgo cluster early-type galaxies
ViCTORIA project: The LOFAR-MeerKAT view of active galactic nuclei in Virgo cluster early-type galaxies Open
The evolution of active galactic nuclei (AGNs) is closely connected to their host galaxies and surroundings. Via feedback processes, AGNs can counteract the cooling of the intracluster medium (ICM) and suppress star formation in their host…
View article: ViCTORIA project: The LOFAR-MeerKAT view of AGN in Virgo cluster early-type galaxies
ViCTORIA project: The LOFAR-MeerKAT view of AGN in Virgo cluster early-type galaxies Open
The evolution of Active Galactic Nuclei (AGN) is closely connected to their host galaxies and surroundings. Via feedback processes, AGN can counteract the cooling of the intracluster medium (ICM) and suppress star formation in their host g…
Giant radio galaxies in the LOFAR deep fields Open
Context. The reason why some radio galaxies (RGs) grow to form so-called giant radio galaxies (GRGs) with sizes > 700 kpc, is still unknown. Aims. In this study, we compare the radio, optical and environmental properties of GRGs with those…
Giant radio galaxies in the LOFAR deep fields Open
In this study, we compare the radio, optical and environmental properties of GRGs with those of a control sample of smaller RGs we found in the three LOw-Frequency ARray (LOFAR) deep fields, namely the Bootes, ELAIS-N1, Lockman Hole, for a…
View article: CHEX-MATE: Characterization of the intra-cluster medium temperature distribution
CHEX-MATE: Characterization of the intra-cluster medium temperature distribution Open
Context. Galaxy clusters grow through the accretion of mass over cosmic time. Their observed properties are then shaped by how baryons distribute and energy is diffused. Thus, a better understanding of spatially resolved, projected thermod…
View article: Revisiting the alignment of radio galaxies in the ELAIS-N1 field
Revisiting the alignment of radio galaxies in the ELAIS-N1 field Open
Aims. Previous studies reported an alignment of the major axes of radio galaxies on various angular scales. Here, we study the alignment of radio galaxies in the ELAIS-N1 Low Frequency ARray (LOFAR) deep field, which covers an area of 25 d…
Revisiting the alignment of radio galaxies in the ELAIS-N1 field Open
Aims. Previous studies reported an alignment of the major axes of radio galaxies on various angular scales. Here, we study the alignment of radio galaxies in the ELAIS-N1 Low Frequency ARray (LOFAR) deep field, which covers an area of 25 $…
Giant radio galaxies in the LoTSS Boötes deep field Open
Giant radio galaxies (GRGs) are radio galaxies that have projected linear extents of more than 700 kpc or 1 Mpc, depending on definition. We have carried out a careful visual inspection in search of GRGs of the Bootes LOFAR Deep Field (BLD…
Exploring the relation between turbulent velocity and density fluctuations in the stratified intracluster medium Open
The dynamics of the intracluster medium (ICM) is affected by turbulence driven by several processes, such as mergers, accretion and feedback from active galactic nuclei. X-ray surface brightness fluctuations have been used to constrain tur…
Exploring the relation between turbulent velocity and density fluctuations in the stratified intracluster medium Open
Context. The dynamics of the intracluster medium (ICM) is affected by turbulence driven by several processes, such as mergers, accretion and feedback from active galactic nuclei. Aims. X-ray surface brightness fluctuations have been used t…