activity
20152026
most citedJ-PLUS: The Javalambre Photometric Local Universe Survey

248 citations · 1.1k across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2026

Euclid: Scaled-up little red dots and other sources with v-shaped spectral energy distributions at z>4

Euclid Collaboration, A. A. Tumborang, K. I. Caputi +169

Little Red Dots (LRDs) are some the most intriguing galaxy populations recently identified at z>~4 with JWST. They constitute the most extreme class of a more abundant population o…

astro-ph.EP2026

Exoplanet Search and Characterization with the Proposed POET Canadian Space Mission

S. Metchev, J. Rowe, P. Miles-Páez +20

The Photometric Observations of Exoplanet Transits (POET) is a proposed micro-satellite mission dedicated to the characterization and discovery of transiting exoplanets. POET has b…

quant-ph2026

Polariton-polariton coherent coupling in a molecular spin-superconductor chip

Carolina del Río, Marcos Rubín-Osanz, David Rodriguez +12

The ability to establish coherent communication channels is key for scaling up quantum devices. Here, we engineer interactions between distant polaritons, hybrid spin-photon excita…

astro-ph.GA2026★ 5 cited

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometric Catalog

Brant E. Robertson, Benjamin D. Johnson, Sandro Tacchella +34

JADES Data Release 5 (DR5) photometric catalogs and describes the methodologies used for source detection, deblending, photometry, uncertainty estimation, and catalog curation. The…

astro-ph.IM2025

Sailing to the next safe harbour in our trip to the early Universe: The massive star population of metal-poor galaxies

N. Castro, M. Garcia, A. Herrero +5

Very metal-poor massive stars in the Local Group are our best proxies for the Universe's first stars, making them essential for modeling reionization and early galactic chemical ev…

quant-ph2025

Optimizing magnetic coupling in lumped element superconducting resonators for molecular spin qubits

Marcos Rubín-Osanz, David Rodriguez, Ignacio Gimeno +18

We engineer lumped-element superconducting resonators that maximize magnetic coupling to molecular spin qubits, achieving record single-spin couplings up to kHz and collectiv…

astro-ph.GA2025

CO Depletion in Infrared Dark Clouds

G. Cosentino, J. C. Tan, C. Gainey +10

Infrared Dark Clouds (IRDCs) are cold, dense structures representative of the initial conditions of star formation. Many studies of IRDCs employ CO to investigate cloud dynamics. H…

astro-ph.EP2025

Blind search for activity-sensitive lines in the near-infrared using HARPS and NIRPS observations of Proxima and Gl 581

João Gomes da Silva, Elisa Delgado-Mena, Nuno C. Santos +145

Stellar activity variability is one of the main obstacles to the detection of Earth-like planets using the RV method. The aim of this work is to measure the effect of activity in t…

astro-ph.GA2025★ 1 cited

CHemical Evolution in MassIve star-forming COres (CHEMICO). I. Evolution of the temperature structure

F. Fontani, V. M. Rivilla, E. Roueff +8

Increasing evidence shows that most stars in the Milky Way, including the Sun, are born in star-forming regions containing also high-mass stars, but due to both observational and t…

astro-ph.SR2025

Euclid: Quick Data Release (Q1) -- Ultracool dwarfs in the Euclid Deep Fields

A. Mohandasan, R. L. Smart, C. Reylé +180

Ultracool dwarfs (UCDs) encompass the lowest-mass stars and brown dwarfs at the substellar boundary. These intrinsically faint objects are challenging to detect, but the wide cover…

astro-ph.GA2024

CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. IV. ALMA observations of organic species at Galactocentric radius ~23 kpc

F. Fontani, G. Vermariën, S. Viti +7

Single-dish observations suggest that the abundances of organic species in star-forming regions of the outer Galaxy, characterised by sub-Solar metallicities, are comparable to tho…

astro-ph.EP2024★ 17 cited

Euclid: Early Release Observations -- A glance at free-floating new-born planets in the sigma Orionis cluster

E. L. Martín, M. {Ž}erjal, H. Bouy +175

We provide an early assessment of the imaging capabilities of the Euclid space mission to probe deeply into nearby star-forming regions and associated very young open clusters, and…

astro-ph.IM2024★ 45 cited

Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometry

J. -C. Cuillandre, E. Bertin, M. Bolzonella +260

The Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-f…

astro-ph.GA2023

The GUAPOS project: G31.41+0.31 Unbiased ALMA sPectral Observational Survey. IV. Phosphorus-bearing molecules and their relation with shock tracers

F. Fontani, C. Mininni, M. T. Beltrán +6

The astrochemistry of the important biogenic element phosphorus (P) is still poorly understood, but observational evidence indicates that P-bearing molecules are likely associated…

astro-ph.EP2022★ 55 cited

Detection of barium in the atmospheres of the ultra-hot gas giants WASP-76b and WASP-121b

T. Azevedo Silva, O. D. S. Demangeon, N. C. Santos +33

High-resolution spectroscopy studies of ultra-hot Jupiters have been key in our understanding of exoplanet atmospheres. Observing into the atmospheres of these giant planets allows…

astro-ph.GA2022★ 35 cited

Torus and polar dust dependence on AGN properties

I. García-Bernete, O. González-Martín, C. Ramos Almeida +8

We present a statistical analysis of the properties of the obscuring material around active galactic nuclei (AGN). This study represents the first of its kind for an ultra-hard X-r…

astro-ph.EP2021★ 77 cited

The all-sky PLATO input catalogue

M. Montalto, G. Piotto, P. M. Marrese +29

Context. The ESA PLAnetary Transits and Oscillations of stars (PLATO) mission will search for terrestrial planets in the habitable zone of solar-type stars. Because of telemetry li…

astro-ph.EP2021★ 158 cited

The CARMENES search for exoplanets around M dwarfs -- Planet occurrence rates from a subsample of 71 stars

S. Sabotta, M. Schlecker, P. Chaturvedi +25

The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 nearby M dwarfs over the past five years as part of its guaranteed time observations (GTO) pr…

astro-ph.GA2020★ 19 cited

MUSE reveals extended circumnuclear outflows in the Seyfert 1 NGC 7469

A. C. Robleto-Orús, J. P. Torres-Papaqui, A. L. Longinotti +9

NGC 7469 is a well known Luminous IR Galaxy, with a circumnuclear star formation ring ( pc radius) surrounding a Seyfert 1 AGN. Nuclear unresolved winds were previously d…

astro-ph.GA2020★ 52 cited

Polycyclic Aromatic Hydrocarbons in Seyfert and star-forming galaxies

I. García-Bernete, D. Rigopoulou, A. Alonso-Herrero +3

Polycyclic Aromatic Hydrocarbons (PAHs) are carbon-based molecules resulting from the union of aromatic rings and related species, which are likely responsible for strong infrared…

astro-ph.GA2020★ 68 cited

Multi-phase feedback processes in the Sy2 galaxy NGC 5643

I. García-Bernete, A. Alonso-Herrero, S. García-Burillo +11

We study the multi-phase feedback processes in the central ~3 kpc of the barred Sy 2 galaxy NGC 5643. We use observations of the cold molecular gas (ALMA CO(2-1)) and ionized gas (…

astro-ph.IM2020★ 43 cited

The nature of point source fringes in mid-infrared spectra acquired with the James Webb Space Telescope

Ioannis Argyriou, Martyn Wells, Alistair Glasse +10

The constructive and destructive interference in different layers of the James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) detector arrays modulate the detected sign…

astro-ph.SR2020★ 16 cited

The lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1)

J. Arancibia-Silva, J. Bouvier, A. Bayo +4

Context. As a fragile element, lithium is a sensitive probe of physical processes occurring in stellar interiors. Aims. We aim at investigating the relationship between lithium abu…

astro-ph.SR2019★ 69 cited

The extended halo of NGC 2682 (M 67) from Gaia DR2

R. Carrera, M. Pasquato, A. Vallenari +8

Context: NGC 2682 is a nearby open cluster, approximately 3.5 Gyr old. Dynamically, most open clusters should dissolve on shorter timescales, of ~ 1 Gyr. Having survived until now,…