Zobrazeno 1 - 10
of 70 261
pro vyhledávání: '"Celeste Are"'
Autor:
Singh, Akriti, Guaita, Lucia, Hibon, Pascale, Häussler, Boris, Lee, Kyoung-Soo, Ramakrishnan, Vandana, Kumar, Ankit, Padilla, Nelson, Firestone, Nicole M., Song, Hyunmi, Artale, Maria Celeste, Hwang, Ho Seong, Iribarren, Paulina Troncoso, Gronwall, Caryl, Gawiser, Eric, Nantais, Julie, Valdes, Francisco, Park, Changbom, Yang, Yujin
The aim of this study is to identify quiescent galaxies in the 2-deg$^2$ COSMOS field at $z \sim 3.1$ and analyze their environment. Using data from the ODIN survey and COSMOS2020 catalog, we identify 24 massive quiescent galaxies (MQGs) with stellar
Externí odkaz:
http://arxiv.org/abs/2411.12722
Autor:
Paz, Ivan Lopez, Fleta, Celeste, Rafí, Joan Marc, Rius, Gemma, Godignon, Philippe, Pellegrini, Giulio, Mena, Silvia, Jimenez, Marcio, Henao, Angela, Bravo, Javier, Boer, Roeland, Molas, Bernat, Guardiola, Consuelo
To cope with environments with high levels of radiation, non-silicon semiconductors such as silicon carbide detectors are being proposed for instrumentation. 4H-SiC diodes for radiation detection have been fabricated in the IMB-CNM Clean Room, for wh
Externí odkaz:
http://arxiv.org/abs/2411.12320
Autor:
Ortiz, M. Espinoza, Guaita, L., Demarco, R., Calabró, A., Pentericci, L., Castellano, M., Artale, M. Celeste, Hathi, N. P., Koekemoer, Anton M., Mannucci, F., Hibon, P., McLeod, D. J., Gargiulo, A., Pompei, E.
Context: Understanding galaxy evolution in dense environments, particularly proto-clusters, is crucial for studying mechanisms driving star formation and quenching. Aims: This study examines how two proto-cluster over-densities at 3 < z < 4 impact st
Externí odkaz:
http://arxiv.org/abs/2411.08155
Autor:
Sgalletta, Cecilia, Mapelli, Michela, Boco, Lumen, Santoliquido, Filippo, Artale, M. Celeste, Iorio, Giuliano, Lapi, Andrea, Spera, Mario
As the number of gravitational-wave detections grows, the merger rate of binary black holes (BBHs) can help us to constrain their formation, the properties of their progenitors, and their birth environment. Here, we aim to address the impact of the m
Externí odkaz:
http://arxiv.org/abs/2410.21401
Autor:
Ramakrishnan, Vandana, Lee, Kyoung-Soo, Firestone, Nicole, Gawiser, Eric, Artale, Maria Celeste, Gronwall, Caryl, Guaita, Lucia, Im, Sang Hyeok, Jeong, Woong-Seob, Kim, Seongjae, Kumar, Ankit, Lee, Jaehyun, Moon, Byeongha, Padilla, Nelson, Park, Changbom, Song, Hyunmi, Troncoso, Paulina, Yang, Yujin
The One-hundred-deg$^2$ DECam Imaging in Narrowbands (ODIN) survey is carrying out a systematic search for protoclusters during Cosmic Noon, using Ly$\alpha$-emitting galaxies (LAEs) as tracers. Once completed, ODIN aims to identify hundreds of proto
Externí odkaz:
http://arxiv.org/abs/2410.18341
Autor:
Montero-Dorta, Antonio D., Contreras, Sergio, Artale, M. Celeste, Rodriguez, Facundo, Favole, Ginevra
The large-scale linear halo bias encodes the relation between the clustering of dark-matter (DM) halos and that of the underlying matter density field. Although the primary dependence of bias on halo mass is well understood in the context of structur
Externí odkaz:
http://arxiv.org/abs/2410.18319
Autor:
Ribeiro, Danilo Monteiro, Melo, Felipe Vasconcelos, Negromonte, Vitor, Matias, Gabriel Walisson, Farias, Adna, Azul, Celeste, Chaves, Ana Paula, Gama, Kiev
Autism Spectrum Disorder (ASD) is a neurodivergent condition with a wide range of characteristics and support levels. Individuals with ASD can exhibit various combinations of traits such as difficulties in social interaction, communication, and langu
Externí odkaz:
http://arxiv.org/abs/2410.14033
Autor:
Andrews, Moira, Artale, M. Celeste, Kumar, Ankit, Lee, Kyoung-Soo, Florek, Tess, Anand, Kaustub, Cerdosino, Candela, Ciardullo, Robin, Firestone, Nicole, Gawiser, Eric, Gronwall, Caryl, Guaita, Lucia, Hong, Sungryong, Hwang, Ho Seong, Lee, Jaehyun, Lee, Seong-Kook, Padilla, Nelson, Park, Jaehong, Popescu, Roxana, Ramakrishnan, Vandana, Song, Hyunmi, Cádiz, F. Vivanco, Vogelsberger, Mark
We investigate the physical properties and redshift evolution of simulated galaxies residing in protoclusters at cosmic noon, to understand the influence of the environment on galaxy formation. This work is to build clear expectations for the ongoing
Externí odkaz:
http://arxiv.org/abs/2410.08412
While many astrophysical plasmas can be modelled successfully assuming ionisation and thermal equilibrium, in some cases this is not appropriate and a non-equilibrium approach is required. In nebulae around evolved stars the local elemental abundance
Externí odkaz:
http://arxiv.org/abs/2409.18904
Publikováno v:
Phys. Rev. E 110, 044133 (2024). (14 pages.) OPEN ACCESS
We perform a numerical study of the kinetic Blume-Capel (BC) model to find if it exhibits the metamagnetic anomalies previously observed in the kinetic Ising model for supercritical periods. We employ a heat-bath Monte Carlo (MC) algorithm on a squar
Externí odkaz:
http://arxiv.org/abs/2408.17199