Tootfinder

The miniJPAS Survey: The radial distribution of star formation rates in faint X-ray active galactic nuclei
Nischal Acharya, Silvia Bonoli, Mara Salvato, Ariana Cortesi, M. Rosa Gonz\'alez Delgado, Ivan Ezequiel Lopez, Isabel Marquez, Gin\'es Mart\'inez-Solaeche, Abdurro'uf, David Alexander, Marcella Brusa, Jon\'as Chaves-Montero, Juan Antonio Fern\'andez Ontiveros, Brivael Laloux, Andrea Lapi, George Mountrichas, Cristina Ramos Almeida, Julio Esteban Rodr\'…

Controlled Fabrication of Native Ultra-Thin Amorphous Gallium Oxide from 2D Gallium Sulfide for Emerging Electronic Applications
AbdulAziz AlMutairi, Aferdita Xhameni, Xuyun Guo, Irina Chirc\u{a}, Valeria Nicolosi, Stephan Hofmann, Antonio Lombardo
https://arxiv.org/abs/2405.05632

Controlled Fabrication of Native Ultra-Thin Amorphous Gallium Oxide from 2D Gallium Sulfide for Emerging Electronic Applications
Oxidation of two-dimensional (2D) layered materials has proven advantageous in creating oxide/2D material heterostructures, opening the door for a new paradigm of low-power electronic devices. Gallium (II) sulfide ($β$-GaS), a hexagonal phase group III monochalcogenide, is a wide bandgap semiconductor with a bandgap exceeding 3 eV in single and few layer form. Its oxide, gallium oxide (Ga$_2$O$_3$), combines large bandgap (4.4-5.3 eV) with high dielectric constant (~10). Despite the technologi…

The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
Ana M. Conrado, Rosa M. Gonz\'alez Delgado, Rub\'en Garc\'ia-Benito, Isabel P\'erez, Simon Verley, Tom\'as Ruiz-Lara, Laura S\'anchez-Menguiano, Salvador Duarte Puertas, Andoni Jim\'enez, Jes\'us Dom\'inguez-G\'omez, Daniel Espada, Mar\'ia Argudo-Fern\'andez, Manuel Alc\'azar-Laynez, Guillermo Bl\'azquez-Calero, Bahar Bidaran, Almudena Zu…

The CAVITY project. The spatially resolved stellar population properties of galaxies in voids
The Universe is shaped as a web-like structure, formed by clusters, filaments, and walls that leave large volumes in between named voids. Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution than galaxies in denser environments (filaments and walls). However, the effect of the void environment on their stellar population properties is still unclear. We aim to address this question using 118 optical integral field unit datacubes from the Ca…