Anthony H. Gonzalez
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View article: A Deep Dive down the Broad-line Region: Permitted O <scp>I</scp> , Ca <scp>II,</scp> and Fe <scp>II</scp> Emission in an Active Galactic Nucleus Little Red Dot at <i>z</i> = 5.3
A Deep Dive down the Broad-line Region: Permitted O <span>I</span> , Ca <span>II,</span> and Fe <span>II</span> Emission in an Active Galactic Nucleus Little Red Dot at <i>z</i> = 5.3 Open
We present a spectroscopic analysis of a broad-line active galactic nucleus (AGN) selected as a little red dot (LRD) at z = 5.3 behind the Bullet cluster (Bz5.3) based on JWST/NIRCam and NIRSpec data. The detection of strong Fe ii , O i , …
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: Intra-cluster light as a dynamical clock for galaxy clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea, and Horizon-AGN simulations
Intra-cluster light as a dynamical clock for galaxy clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea, and Horizon-AGN simulations Open
Context. As the most massive nodes of the cosmic web, galaxy clusters represent the best probes of structure formation. Over time, they grow by accreting and disrupting satellite galaxies, adding those stars to the brightest cluster galaxy…
View article: Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs Open
Context. The South Pole Telescope third-generation camera (SPT-3G) has observed over 10,000 square degrees of sky at 95, 150, and 220 GHz (3.3, 2.0, 1.4 mm, respectively) overlapping the ongoing 14,000 square-degree Euclid Wide Survey. The…
View article: Evidence for Environmental Effects in the <i>z</i> = 4.3 Protocluster Core SPT2349–56
Evidence for Environmental Effects in the <i>z</i> = 4.3 Protocluster Core SPT2349–56 Open
We present Atacama Large Millimeter/submillimeter Array observations of the [C I ] 492 and 806 GHz fine-structure lines in 25 dusty star-forming galaxies (DSFGs) at z = 4.3 in the core of the SPT2349–56 protocluster. The protocluster galax…
View article: The Massive and Distant Clusters of WISE Survey. XII. Exploring X-Ray Active Galactic Nuclei in Dynamically Active Massive Galaxy Clusters at <i>z</i> ∼ 1
The Massive and Distant Clusters of WISE Survey. XII. Exploring X-Ray Active Galactic Nuclei in Dynamically Active Massive Galaxy Clusters at <i>z</i> ∼ 1 Open
We present an analysis of the cluster X-ray morphology and active galactic nucleus (AGN) activity in nine z ∼ 1 galaxy clusters from the Massive and Distant Clusters of WISE Survey observed with Chandra. Using photon asymmetry ( A phot ) t…
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: JWST Early Release Science Program TEMPLATES: Targeting Extremely Magnified Panchromatic Lensed Arcs and Their Extended Star Formation
JWST Early Release Science Program TEMPLATES: Targeting Extremely Magnified Panchromatic Lensed Arcs and Their Extended Star Formation Open
This paper gives an overview of Targeting Extremely Magnified Panchromatic Lensed Arcs and Their Extended Star formation (TEMPLATES), a JWST Early Release Science program that targeted four extremely bright, gravitationally lensed galaxies…
View article: LEUCEMIA MIELOIDE CRÔNICA: AVANÇOS EM DIAGNÓSTICO, TRATAMENTO E PROGNÓSTICO
LEUCEMIA MIELOIDE CRÔNICA: AVANÇOS EM DIAGNÓSTICO, TRATAMENTO E PROGNÓSTICO Open
A leucemia mieloide crônica (LMC) é uma neoplasia hematológica caracterizada pela proliferação descontrolada de células mieloides, frequentemente associada ao cromossomo Philadelphia e à fusão do gene BCR-ABL. O tratamento com inibidores d…
View article: Evidence for environmental effects in the $z\,{=}\,4.3$ protocluster core SPT2349$-$56
Evidence for environmental effects in the $z\,{=}\,4.3$ protocluster core SPT2349$-$56 Open
We present ALMA observations of the [CI] 492 and 806$\,$GHz fine-structure lines in 25 dusty star-forming galaxies (DSFGs) at $z\,{=}\,4.3$ in the core of the SPT2349$-$56 protocluster. The protocluster galaxies exhibit a median $L^\prime_…
View article: Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at <i>z</i> = 2.363 and CARLA-Ser J0950+2743 at <i>z</i> = 2.243
Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at <i>z</i> = 2.363 and CARLA-Ser J0950+2743 at <i>z</i> = 2.243 Open
Galaxy clusters are the largest gravitationally bound structures in the Universe and therefore are a powerful tool for studying mass assembly at different epochs. At z > 2, they provide the unique opportunity to place solid constraints not…
View article: Kinematic Analysis of z = 4.3 Galaxies in the SPT2349–56 Protocluster Core
Kinematic Analysis of z = 4.3 Galaxies in the SPT2349–56 Protocluster Core Open
SPT2349−56 is a protocluster discovered in the 2500 deg 2 South Pole Telescope (SPT) survey. In this paper, we study the kinematics of the galaxies found in the core of SPT2349−56 using high-resolution (1.55 kpc spatial resolution at z = 4…
View article: The Massive and Distant Clusters of WISE Survey 2: Second Data Release
The Massive and Distant Clusters of WISE Survey 2: Second Data Release Open
We present the second data release of the Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2). We expand from the equatorial first data release to most of the Dark Energy Camera Legacy Survey area, covering a total area of 6498 deg 2 …
View article: Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays: mission overview
Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays: mission overview Open
View article: The Massive and Distant Clusters of WISE Survey 2: Second Data Release
The Massive and Distant Clusters of WISE Survey 2: Second Data Release Open
We present the second data release of the Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2). We expand from the equatorial first data release to most of the Dark Energy Camera Legacy Survey area, covering a total area of 6498 deg^2.…
View article: Revisão sistemática dos avanços no diagnóstico e tratamento do acidente vascular cerebral: perspectivas neurocientíficas e atualizações clínicas
Revisão sistemática dos avanços no diagnóstico e tratamento do acidente vascular cerebral: perspectivas neurocientíficas e atualizações clínicas Open
O Acidente Vascular Cerebral (AVC) é uma condição médica crítica caracterizada pela interrupção súbita do fluxo sanguíneo para uma parte do cérebro, resultando em danos neurológicos que podem variar em severidade. A definição moderna do AV…
View article: STROBE-X Mission Overview
STROBE-X Mission Overview Open
We give an overview of the science objectives and mission design of the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) observatory, which has been proposed as a NASA probe-class (~$1.5B) mission in response…
View article: <i>Euclid</i>: Early Release Observations – Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field
<i>Euclid</i>: Early Release Observations – Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field Open
We present an analysis of Euclid observations of a 0.6 deg 2 field in the central region of the Fornax galaxy cluster that were acquired during the performance verification phase. With these data, we investigated the potential of Euclid to…
View article: The Massive and Distant Clusters of WISE Survey 2: A Stacking Analysis Investigating the Evolution of Star Formation Rates and Stellar Masses in Groups and Clusters
The Massive and Distant Clusters of WISE Survey 2: A Stacking Analysis Investigating the Evolution of Star Formation Rates and Stellar Masses in Groups and Clusters Open
The evolution of galaxies depends on their masses and local environments; understanding when and how environmental quenching starts to operate remains a challenge. Furthermore, studies of the high-redshift regime have been limited to massi…
View article: SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region Open
We present an extension to a Sunyaev–Zel’dovich Effect (SZE) selected cluster catalogue based on observations from the South Pole Telescope (SPT); this catalogue extends to lower signal to noise than the previous SPT–SZ catalogue and there…
View article: The Massive and Distant Clusters of WISE Survey 2: A Stacking Analysis Investigating the Evolution of Star Formation Rates and Stellar Masses in Groups and Clusters
The Massive and Distant Clusters of WISE Survey 2: A Stacking Analysis Investigating the Evolution of Star Formation Rates and Stellar Masses in Groups and Clusters Open
The evolution of galaxies depends on their masses and local environments; understanding when and how environmental quenching starts to operate remains a challenge. Furthermore, studies of the high-redshift regime have been limited to massi…
View article: The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release
The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release Open
The Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2) is a new survey designed as the successor of the original MaDCoWS survey. MaDCoWS2 improves upon its predecessor by using deeper optical and infrared data and a more powerful det…
View article: Euclid: Early Release Observations -- Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field
Euclid: Early Release Observations -- Globular clusters in the Fornax galaxy cluster, from dwarf galaxies to the intracluster field Open
We present an analysis of Euclid observations of a 0.5 deg$^2$ field in the central region of the Fornax galaxy cluster that were acquired during the performance verification phase. With these data, we investigate the potential of Euclid f…
View article: TEMPLATES: Characterization of a Merger in the Dusty Lensing SPT0418–47 System
TEMPLATES: Characterization of a Merger in the Dusty Lensing SPT0418–47 System Open
We present JWST and Atacama Large Millimeter/submillimeter Array (ALMA) imaging for the lensing system SPT0418−47, which includes a strongly lensed, dusty, star-forming galaxy at redshift z = 4.225 and an associated multiply imaged compani…
View article: The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release
The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release Open
The Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2) is a new survey designed as the successor of the original MaDCoWS survey. MaDCoWS2 improves upon its predecessor by using deeper optical and infrared data and a more powerful det…
View article: The miniJPAS survey
The miniJPAS survey Open
Context. Galaxy clusters are an essential tool to understand and constrain the cosmological parameters of our universe. Thanks to its multi-band design, J-PAS offers a unique group and cluster detection window using precise photometric red…
View article: Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus
Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus Open
We have observed the z = 4.3 protocluster SPT2349−56 with the Australia Telescope Compact Array (ATCA) with the aim of detecting radio-loud active galactic nuclei (AGNs) among the ∼30 submillimeter (submm) galaxies (SMGs) identified in the…
View article: Experiences and perceptions of healthcare professionals with long-acting injectable antipsychotic use in schizophrenia: survey results from the multinational ADVANCE study
Experiences and perceptions of healthcare professionals with long-acting injectable antipsychotic use in schizophrenia: survey results from the multinational ADVANCE study Open
View article: Extended Lyman-<i>α</i> emission towards the SPT2349-56 protocluster at <i>z</i> = 4.3
Extended Lyman-<i>α</i> emission towards the SPT2349-56 protocluster at <i>z</i> = 4.3 Open
Context. Deep spectroscopic surveys with the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed that some of the brightest infrared sources in the sky correspond to concentrations of submillimeter galaxies (SMGs) at high red…
View article: The miniJPAS survey: Optical detection of galaxy clusters with PZWav
The miniJPAS survey: Optical detection of galaxy clusters with PZWav Open
Galaxy clusters are an essential tool to understand and constrain the cosmological parameters of our Universe. Thanks to its multi-band design, J-PAS offers a unique group and cluster detection window using precise photometric redshifts an…