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View article: Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample
Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample Open
In this work, we derive and calibrate the redshift distribution of the MagLim++ lens galaxy sample used in the Dark Energy Survey Year 6 (DES Y6) 3x2pt cosmology analysis. The 3x2pt analysis combines galaxy clustering from the lens galaxy …
View article: Intelligence in the Mesh: How AI and FEA are Revolutionising Failure Analysis in Automotive Engineering
Intelligence in the Mesh: How AI and FEA are Revolutionising Failure Analysis in Automotive Engineering Open
View article: Genomic epidemiology of Mycobacterium tuberculosis in Wales
Genomic epidemiology of Mycobacterium tuberculosis in Wales Open
Identification of factors contributing to tuberculosis (TB) transmission can guide targeted measures to reduce morbidity. Varying findings for factors associated with TB genomic clustering exist. We describe Mycobacterium tuberculosis stra…
View article: Constraining Star Formation in M87 Using Deep Hubble Space Telescope UV Data
Constraining Star Formation in M87 Using Deep Hubble Space Telescope UV Data Open
We analyzed the deepest Hubble Space Telescope F275W ultraviolet (UV) imaging of M87 to obtain the most robust constraints on its star formation rate (SFR) and star formation history (SFH). After removing the galaxy continuum and globular …
View article: Dark Energy Survey Year 3 Results: Cosmological constraints from second and third-order shear statistics
Dark Energy Survey Year 3 Results: Cosmological constraints from second and third-order shear statistics Open
We present a cosmological analysis of the third-order aperture mass statistic using Dark Energy Survey Year 3 (DES Y3) data. We perform a complete tomographic measurement of the three-point correlation function of the Y3 weak lensing shape…
View article: Euclid preparation. Constraining parameterised models of modifications of gravity with the spectroscopic and photometric primary probes
Euclid preparation. Constraining parameterised models of modifications of gravity with the spectroscopic and photometric primary probes Open
The Euclid mission has the potential to understand the fundamental physical nature of late-time cosmic acceleration and, as such, of deviations from the standard cosmological model, LCDM. In this paper, we focus on model-independent method…
View article: Stellar population modelling of neutron stars and black holes: spatially resolved graveyards in MaNGA/SDSS-IV galaxies
Stellar population modelling of neutron stars and black holes: spatially resolved graveyards in MaNGA/SDSS-IV galaxies Open
We update our stellar population models for the time evolution of the number and mass of massive remnants – neutron stars and black holes – with a new initial mass–remnant mass relation for core collapse supernovae. The calculations are ba…
View article: Improving the Reliability of Satellite Components Using Finite Element Analysis and 3D Printing as a Vital Tool for Modern Space Missions
Improving the Reliability of Satellite Components Using Finite Element Analysis and 3D Printing as a Vital Tool for Modern Space Missions Open
View article: Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering
Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering Open
Galaxy clusters provide a unique probe of the late-time cosmic structure and serve as a powerful independent test of the $\Lambda$CDM model. This work presents the first set of cosmological constraints derived with ~16,000 optically select…
View article: A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE)
A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) Open
We reconstructed the star formation histories of seven massive ( M ⋆ ≳ 10 10 M ⊙ ) early-type galaxies (ETGs) in the Virgo cluster by analysing their spatially resolved stellar population (SP) properties including their ultraviolet (UV) an…
View article: Sloan Digital Sky Survey IV MaStar: Quantification and Abatement of Interstellar Absorption in the Largest Empirical Stellar Spectral Library
Sloan Digital Sky Survey IV MaStar: Quantification and Abatement of Interstellar Absorption in the Largest Empirical Stellar Spectral Library Open
We assess the impact of Ca ii λ λ 3934, 3969 and Na i λ λ 5891, 5897 absorption arising in the interstellar medium (ISM) on the Sloan Digital Sky Survey-IV MaNGA Stellar Library (MaStar) and produce corrected spectroscopy for 80% of the 24…
View article: SDSS-IV MaStar: Quantification and Abatement of Interstellar Absorption in the Largest Empirical Stellar Spectral Library
SDSS-IV MaStar: Quantification and Abatement of Interstellar Absorption in the Largest Empirical Stellar Spectral Library Open
We assess the impact of CaII 3934,3969 and NaI 5891,5897 absorption arising in the interstellar medium (ISM) on the SDSS-IV MaNGA Stellar Library (MaStar) and produce corrected spectroscopy for 80% of the 24,162-star catalog. We model the …
View article: Les modes de gestion dans les groupes féministes et leur offre en rétributions : le point de vue des militantes en Abitibi-Témiscamingue
Les modes de gestion dans les groupes féministes et leur offre en rétributions : le point de vue des militantes en Abitibi-Témiscamingue Open
La relation entre la gestion féministe et le militantisme a peu été explorée dans les études scientifiques depuis l’arrivée des groupes féministes au Québec. Les résultats d’une recherche qualitative ayant abordé cette relation sous l’angl…
View article: Dark energy survey year 3 results: cosmology from galaxy clustering and galaxy–galaxy lensing in harmonic space
Dark energy survey year 3 results: cosmology from galaxy clustering and galaxy–galaxy lensing in harmonic space Open
We present the joint tomographic analysis of galaxy-galaxy lensing and galaxy clustering in harmonic space (HS), using galaxy catalogues from the first three years of observations by the Dark Energy Survey (DES Y3). We utilize the redMaGiC…
View article: Azimuthal variations of stellar populations in barred galaxies
Azimuthal variations of stellar populations in barred galaxies Open
Bars are expected to impact the distribution of stellar populations both during bar formation, as they rearrange stars into new orbits, and afterwards, due to the redistribution of star-formation-fuelling gas and transfer of angular moment…
View article: Azimuthal Variations of Stellar Populations in Barred Galaxies
Azimuthal Variations of Stellar Populations in Barred Galaxies Open
Bars are expected to impact the distribution of stellar populations both during bar formation, as they rearrange stars into new orbits, and afterwards, due to the redistribution of star-formation-fuelling gas and transfer of angular moment…
View article: Dark Energy Survey: Galaxy sample for the baryonic acoustic oscillation measurement from the final dataset
Dark Energy Survey: Galaxy sample for the baryonic acoustic oscillation measurement from the final dataset Open
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
View article: Unveiling Wind Turbine Failures Causes, Detection, and Prevention for Enhanced Reliability
Unveiling Wind Turbine Failures Causes, Detection, and Prevention for Enhanced Reliability Open
View article: Carbon- and Oxygen-rich stars in MaStar: identification and classification
Carbon- and Oxygen-rich stars in MaStar: identification and classification Open
Carbon- and Oxygen-rich stars populating the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase of stellar evolution are relevant contributors to the spectra of ∼1 Gyr old populations. Atmosphere models for these types are uncertain,…
View article: Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset Open
In this paper we present and validate the galaxy sample used for the analysis of the baryon acoustic oscillation (BAO) signal in the Dark Energy Survey (DES) Y6 data. The definition is based on a color and redshift-dependent magnitude cut …
View article: Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\rm eff}$=0.85 from the final dataset
Dark Energy Survey: A 2.1% measurement of the angular Baryonic Acoustic Oscillation scale at redshift $z_{\rm eff}$=0.85 from the final dataset Open
We present the angular diameter distance measurement obtained with the Baryonic Acoustic Oscillation feature from galaxy clustering in the completed Dark Energy Survey, consisting of six years (Y6) of observations. We use the Y6 BAO galaxy…
View article: $\\mathrm{SDSS}$-$\\mathrm{IV}$ $\\mathrm{MaNGA}$: a catalogue of spectroscopically detected strong galaxy–galaxy lens candidates
$\\mathrm{SDSS}$-$\\mathrm{IV}$ $\\mathrm{MaNGA}$: a catalogue of spectroscopically detected strong galaxy–galaxy lens candidates Open
We spectroscopically detected candidate emission-lines of 8 likely, 17 probable, and 69 possible strong galaxy–galaxy gravitational lens candidates found within the spectra of ≈10000 galaxy targets contained within the completed Mapping of…
View article: iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. - III. Stellar metallicity drivers in MaNGA and TNG50
iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. - III. Stellar metallicity drivers in MaNGA and TNG50 Open
The iMaNGA project uses a forward-modelling approach to compare the predictions of cosmological simulations with observations from SDSS-IV/MaNGA. We investigate the dependency of age and metallicity radial gradients on galaxy morphology, s…
View article: iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50 Open
The iMaNGA project uses a forward-modelling approach to compare the predictions of cosmological simulations with observations from SDSS-IV/MaNGA. We investigate the dependency of age and metallicity radial gradients on galaxy morphology, s…
View article: The Dark Energy Survey Year 3 high-redshift sample: selection, characterization, and analysis of galaxy clustering
The Dark Energy Survey Year 3 high-redshift sample: selection, characterization, and analysis of galaxy clustering Open
The fiducial cosmological analyses of imaging surveys like DES typically probe the Universe at redshifts z < 1. We present the selection and characterization of high-redshift galaxy samples using DES Year 3 data, and the analysis of the…
View article: The PSZ-MCMF catalogue of <i>Planck</i> clusters over the DES region
The PSZ-MCMF catalogue of <i>Planck</i> clusters over the DES region Open
We present the first systematic follow-up of Planck Sunyaev–Zeldovich effect (SZE) selected candidates down to signal-to-noise (S/N) of 3 over the 5000 deg2 covered by the Dark Energy Survey. Using the MCMF cluster confirmation algorithm, …
View article: Continuous Gravitational Waves from Galactic Neutron Stars: Demography, Detectability, and Prospects
Continuous Gravitational Waves from Galactic Neutron Stars: Demography, Detectability, and Prospects Open
We study the prospects for the detection of continuous gravitational signals from normal Galactic neutron stars, i.e., nonrecycled stars. We use a synthetic population generated by evolving stellar remnants in time, according to several mo…
View article: DeepZipper. II. Searching for lensed supernovae in dark energy survey data with deep learning
DeepZipper. II. Searching for lensed supernovae in dark energy survey data with deep learning Open
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
View article: iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs – II. The catalogue
iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs – II. The catalogue Open
Strengthening the synergy between simulations and observations is essential to test galaxy formation and evolution theories. To achieve this goal, in the first paper of this series, we presented a method to generate mock SDSS-IV/Mapping Ne…
View article: Supplementary Figure 1 from Essential Requirement for PP2A Inhibition by the Oncogenic Receptor c-KIT Suggests PP2A Reactivation as a Strategy to Treat c-KIT<sup>+</sup> Cancers
Supplementary Figure 1 from Essential Requirement for PP2A Inhibition by the Oncogenic Receptor c-KIT Suggests PP2A Reactivation as a Strategy to Treat c-KIT<sup>+</sup> Cancers Open
Supplementary Figure 1 from Essential Requirement for PP2A Inhibition by the Oncogenic Receptor c-KIT Suggests PP2A Reactivation as a Strategy to Treat c-KIT+ Cancers