Jesse B. Golden-Marx
YOU?
Author Swipe
View article: A Splashback-like Feature of Central Galaxies in Galaxy Clusters
A Splashback-like Feature of Central Galaxies in Galaxy Clusters Open
We investigate a splashback-like feature in the outer region of central galaxies (CGs) in clusters. This feature is detected as a "dip" in the radial slope of the CG surface brightness, derived through the stacking of Dark Energy Survey da…
View article: Euclid preparation. Methodology for validating the Euclid Catalogue of Galaxy Clusters using external data
Euclid preparation. Methodology for validating the Euclid Catalogue of Galaxy Clusters using external data Open
We present our methodology for identifying known clusters as counterparts to objects in the Euclid Catalogue of Galaxy Clusters (ECGC). Euclid is expected to detect a large number of optically-selected galaxy clusters over the approximatel…
View article: Euclid: Early Release Observations. A combined strong and weak lensing solution for Abell 2390 beyond its virial radius
Euclid: Early Release Observations. A combined strong and weak lensing solution for Abell 2390 beyond its virial radius Open
Euclid is presently mapping the distribution of matter in the Universe in detail via the weak lensing (WL) signature of billions of distant galaxies. The WL signal is most prominent around galaxy clusters, and can extend up to distances we…
View article: <i>Euclid</i>: Early Release Observations
<i>Euclid</i>: Early Release Observations Open
Intracluster light (ICL) provides a record of the dynamical interactions undergone by clusters, giving clues on cluster formation and evolution. Here, we analyse the properties of ICL in the massive cluster Abell 2390 at redshift z = 0.228…
View article: <i>Euclid</i> preparation
<i>Euclid</i> preparation Open
The intracluster light (ICL) permeating galaxy clusters is a tracer of the cluster assembly history and potentially a tracer of their dark matter structure. In this work, we explore the capability of the Euclid Wide Survey to detect ICL us…
View article: <i>Euclid</i>: Early Release Observations – Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions★
<i>Euclid</i>: Early Release Observations – Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions★ Open
The Euclid Early Release Observations (ERO) programme targeted the Perseus cluster of galaxies, gathering deep data in the central region of the cluster over 0.7 deg 2 , including the cluster core up to 0.25 r 200 . The dataset reaches a p…
View article: <i>Euclid</i>: Early Release Observations – Programme overview and pipeline for compact- and diffuse-emission photometry
<i>Euclid</i>: Early Release Observations – Programme overview and pipeline for compact- and diffuse-emission photometry Open
The Euclid Early Release Observations (ERO) showcase Euclid ’s capabilities in advance of its main mission by targeting 17 astronomical objects, including galaxy clusters, nearby galaxies, globular clusters, and star-forming regions. A tot…
View article: <i>Euclid</i>: Early Release Observations – Dwarf galaxies in the Perseus galaxy cluster
<i>Euclid</i>: Early Release Observations – Dwarf galaxies in the Perseus galaxy cluster Open
We make use of the unprecedented depth, spatial resolution, and field of view of the Euclid Early Release Observations (EROs) of the Perseus galaxy cluster to detect and characterise the dwarf galaxy population in this massive system. Usin…
View article: The hierarchical growth of bright central galaxies and intracluster light as traced by the magnitude gap
The hierarchical growth of bright central galaxies and intracluster light as traced by the magnitude gap Open
Using a sample of 2800 galaxy clusters identified in the Dark Energy Survey across the redshift range $0.20 \lt z \lt 0.60$, we characterize the hierarchical assembly of bright central galaxies (BCGs) and the surrounding intracluster light…
View article: <i>Euclid</i>: Early Release Observations – The intracluster light and intracluster globular clusters of the Perseus cluster
<i>Euclid</i>: Early Release Observations – The intracluster light and intracluster globular clusters of the Perseus cluster Open
We study the intracluster light (ICL) and intracluster globular clusters (ICGCs) in the nearby Perseus cluster of galaxies using Euclid ’s Early Release Observations. By modelling the isophotal and iso-density contours, we mapped the distr…
View article: Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies Open
The number density and redshift evolution of optically selected galaxy clusters offer an independent measurement of the amplitude of matter fluctuations, $S_8$. However, recent results have shown that clusters chosen by the redMaPPer algor…
View article: The Hierarchical Growth of Bright Central Galaxies and Intracluster Light as Traced by the Magnitude Gap
The Hierarchical Growth of Bright Central Galaxies and Intracluster Light as Traced by the Magnitude Gap Open
Using a sample of 2800 galaxy clusters identified in the Dark Energy Survey across the redshift range $0.20 < z < 0.60$, we characterize the hierarchical assembly of Bright Central Galaxies (BCGs) and the surrounding intracluster light (IC…
View article: <i>Euclid</i>: Early Release Observations – A preview of the Euclid era through a galaxy cluster magnifying lens
<i>Euclid</i>: Early Release Observations – A preview of the Euclid era through a galaxy cluster magnifying lens Open
We present the first analysis of the Euclid Early Release Observations (ERO) program that targets fields around two lensing clusters, Abell 2390 and Abell 2764. We use imaging data from the Visible instrument (VIS) and the Near-Infrared Sp…
View article: Euclid: Early Release Observations -- A preview of the Euclid era through a galaxy cluster magnifying lens
Euclid: Early Release Observations -- A preview of the Euclid era through a galaxy cluster magnifying lens Open
We present the first analysis of the Euclid Early Release Observations (ERO) program that targets fields around two lensing clusters, Abell 2390 and Abell 2764. We use VIS and NISP imaging to produce photometric catalogs for a total of $\s…
View article: Euclid: Early Release Observations -- The intracluster light and intracluster globular clusters of the Perseus cluster
Euclid: Early Release Observations -- The intracluster light and intracluster globular clusters of the Perseus cluster Open
We study the intracluster light (ICL) and intracluster globular clusters (ICGCs) in the nearby Perseus galaxy cluster using Euclid's EROs. By modelling the isophotal and iso-density contours, we mapped the distributions and properties of t…
View article: Dark Energy Survey Year 6 results: Intra-cluster light from redshift 0.2 to 0.5
Dark Energy Survey Year 6 results: Intra-cluster light from redshift 0.2 to 0.5 Open
Using the full 6 years of imaging data from the Dark Energy Survey, we study the surface brightness profiles of galaxy cluster central galaxies and intra-cluster light. We apply a ‘stacking’ method to over 4000 galaxy clusters identified b…
View article: The CluMPR galaxy cluster-finding algorithm and DESI legacy survey galaxy cluster catalogue
The CluMPR galaxy cluster-finding algorithm and DESI legacy survey galaxy cluster catalogue Open
Galaxy clusters enable unique opportunities to study cosmology, dark matter, galaxy evolution, and strongly lensed transients. We here present a new cluster-finding algorithm, CluMPR (Clusters from Masses and Photometric Redshifts), that e…
View article: Candidate cluster-scale gravitationally lensed quasars from CluMPR and DESI Legacy Survey
Candidate cluster-scale gravitationally lensed quasars from CluMPR and DESI Legacy Survey Open
Candidate cluster-scale strongly-lensed quasars from DESI Legacy Survey (DESI QSO targets) and CluMPR DESI Legacy Survey galaxy cluster catalog. Paper decribing the CluMPR galaxy cluster catalogs and candidate lensed quasar catalogs: The C…
View article: The CluMPR Galaxy Cluster Catalogue for DESI Legacy Survey DR9
The CluMPR Galaxy Cluster Catalogue for DESI Legacy Survey DR9 Open
Galaxy cluster catalog and cluster member galaxy catalogs compiled using the CluMPR cluster-finding algorithm. Paper decribing the CluMPR algorithms and cluster catalogs: The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey G…
View article: Euclid: Early Release Observations – Dwarf galaxies in the Perseus galaxy cluster
Euclid: Early Release Observations – Dwarf galaxies in the Perseus galaxy cluster Open
We make use of the unprecedented depth, spatial resolution, and field of view of the Euclid Early Release Observations of the Perseus galaxy cluster to detect and characterise the dwarf galaxy population in this massive system. The Euclid …
View article: The High-redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Investigating the Role of Environment on Bent Radio AGNs Using LOFAR
The High-redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Investigating the Role of Environment on Bent Radio AGNs Using LOFAR Open
Bent radio active galactic nucleus (AGN) morphology depends on the density of the surrounding gas. However, bent sources are found inside and outside clusters, raising the question of how environment impacts bent AGN morphology. We analyze…
View article: Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5 Open
Using the full six years of imaging data from the Dark Energy Survey, we study the surface brightness profiles of galaxy cluster central galaxies and intra-cluster light. We apply a ``stacking'' method to over four thousand galaxy clusters…
View article: The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Investigating the Role of Environment on Bent Radio AGNs using LOFAR
The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Investigating the Role of Environment on Bent Radio AGNs using LOFAR Open
Bent radio AGN morphology depends on the density of the surrounding gas. However, bent sources are found inside and outside clusters, raising the question of how environment impacts bent AGN morphology. We analyze new LOw-Frequency Array T…
View article: Candidate cluster-scale gravitationally lensed quasars from CluMPR and DESI Legacy Survey
Candidate cluster-scale gravitationally lensed quasars from CluMPR and DESI Legacy Survey Open
Candidate cluster-scale strongly-lensed quasars from DESI Legacy Survey (DESI QSO targets) and CluMPR DESI Legacy Survey galaxy cluster catalog. Paper decribing the CluMPR galaxy cluster catalogs and candidate lensed quasar catalogs: The C…
View article: The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue
The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue Open
Galaxy clusters enable unique opportunities to study cosmology, dark matter, galaxy evolution, and strongly-lensed transients. We here present a new cluster-finding algorithm, CluMPR (Clusters from Masses and Photometric Redshifts), that e…
View article: The CluMPR Galaxy Cluster Catalogue for DESI Legacy Survey DR9
The CluMPR Galaxy Cluster Catalogue for DESI Legacy Survey DR9 Open
Galaxy cluster catalog and cluster member galaxy catalogs compiled using the CluMPR cluster-finding algorithm. Paper decribing the CluMPR algorithms and cluster catalogs: The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey G…
View article: Characterizing the intracluster light over the redshift range 0.2 &lt; <i>z</i> &lt; 0.8 in the DES-ACT overlap
Characterizing the intracluster light over the redshift range 0.2 < <i>z</i> < 0.8 in the DES-ACT overlap Open
We characterize the properties and evolution of bright central galaxies (BCGs) and the surrounding intracluster light (ICL) in galaxy clusters identified in the Dark Energy Survey and Atacama Cosmology Telescope Survey (DES-ACT) overlappin…
View article: Satellite Content and Halo Mass of Galaxy Clusters: Comparison between Red-Sequence and Halo-based Optical Cluster Finders
Satellite Content and Halo Mass of Galaxy Clusters: Comparison between Red-Sequence and Halo-based Optical Cluster Finders Open
Cluster cosmology depends critically on how optical clusters are selected from imaging surveys. We compare the conditional luminosity function (CLF) and weak lensing halo masses between two different cluster samples at fixed richness, dete…
View article: Characterising the Intracluster Light over the Redshift Range $0.2 < z < 0.8$ in the DES-ACT Overlap
Characterising the Intracluster Light over the Redshift Range $0.2 < z < 0.8$ in the DES-ACT Overlap Open
We characterise the properties and evolution of Bright Central Galaxies (BCGs) and the surrounding intracluster light (ICL) in galaxy clusters identified in overlapping regions of the Dark Energy Survey and Atacama Cosmology Telescope Surv…
View article: The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies
The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies Open
We quantify evolution in the cluster-scale stellar mass–halo mass (SMHM) relation’s parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range 0.03 ≤ z ≤ 0.60. The precision on the inferred SMHM parameters…