Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Marcelo V. dos Santos"'
Autor:
Eduardo J. de Mericia, Larissa C. O. Santos, Carlos Alexandre Wuensche, Vincenzo Liccardo, Camila P. Novaes, Jacques Delabrouille, Mathieu Remazeilles, Filipe B. Abdalla, Chang Feng, Luciano Barosi, Amilcar Queiroz, Thyrso Villela, Bin Wang, Jiajun Zhang, Alessandro Marins, Andre A. Costa, Elisa G. M. Ferreira, Ricardo G. Landim, Marcelo V. dos Santos
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2023, 671, pp.A58. ⟨10.1051/0004-6361/202243804⟩
Astronomy and Astrophysics-A&A, 2023, 671, pp.A58. ⟨10.1051/0004-6361/202243804⟩
To recover the 21 cm hydrogen line, it is essential to separate the cosmological signal from the much stronger foreground contributions at radio frequencies. The BINGO radio telescope is designed to measure the 21 cm line and detect BAOs using the in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5fcad9191b342163f97cac91df29b0b
Autor:
José Ítalo S. Mota, Rui M Patrício Silva-Júnior, Clarissa Silva Martins, Ana Carolina Bueno, Luiz Eduardo Luiz Eduardo Wildemberg, Ximene L da Silva Antunes, Jorge G Okanobo Ozaki, Fernanda B Coeli-Lacchin, Carlos Garcia-Peral, Antonio Edson R Oliveira, Antonio Carlos dos Santos, Ayrton C Moreira, Helio Rubens Machado, Marcelo V dos Santos, Leandro M Colli, Mônica R Gadelha, Sonir R Antonini, Margaret de Castro
Publikováno v:
Journal of the Endocrine Society. 6:A511-A511
Objectives To evaluate how telomeres length behaves in adamantinomtous craniopharyngioma (aCP) and if it contributes to the pathogenesis of aCPs with and without CTNNB1 mutations. Design: Retrospective cross-sectional study enrolling 42 aCPpatients f
Autor:
Camila P. Novaes, Jiajun Zhang, Eduardo J. de Mericia, Filipe B. Abdalla, Vincenzo Liccardo, Carlos A. Wuensche, Jacques Delabrouille, Mathieu Remazeilles, Larissa Santos, Ricardo G. Landim, Elcio Abdalla, Luciano Barosi, Amilcar Queiroz, Thyrso Villela, Bin Wang, André A. Costa, Elisa G. M. Ferreira, Alessandro Marins, Marcelo V. dos Santos
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
[Context] A new and promising technique for observing the Universe and study the dark sector is the intensity mapping of the redshifted 21 cm line of neutral hydrogen (H I). The Baryon Acoustic Oscillations [BAO] from Integrated Neutral Gas Observati
Autor:
Filipe B. Abdalla, Alessandro Marins, Pablo Motta, Elcio Abdalla, Rafael M. Ribeiro, Carlos A. Wuensche, Jacques Delabrouille, Karin S. F. Fornazier, Vincenzo Liccardo, Bruno Maffei, Eduardo J. de Mericia, Carlos H. N. Otobone, Juliana F. R. dos Santos, Gustavo B. Silva, Jordany Vieira, João A. M. Barretos, Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz, Thyrso Villela, Bin Wang, Andre A. Costa, Elisa G. M. Ferreira, Ricardo G. Landim, Camila Paiva Novaes, Michael W. Peel, Larissa Santos, Marcelo V. dos Santos, Jiajun Zhang
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664, pp.A16. ⟨10.1051/0004-6361/202141382⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Astronomy and Astrophysics-A&A, 2022, 664, pp.A16. ⟨10.1051/0004-6361/202141382⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
The BINGO telescope was designed to measure the fluctuations of the 21-cm radiation arising from the hyperfine transition of neutral hydrogen and aims to measure the Baryon Acoustic Oscillations (BAO) from such fluctuations, therefore serving as a pa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::17340114ab3daf11a9081736e8af848c
https://hal.archives-ouvertes.fr/hal-03287268
https://hal.archives-ouvertes.fr/hal-03287268
Autor:
Carlos A. Wuensche, Thyrso Villela, Elcio Abdalla, Vincenzo Liccardo, Frederico Vieira, Ian Browne, Michael W. Peel, Christopher Radcliffe, Filipe B. Abdalla, Alessandro Marins, Luciano Barosi, Francisco A. Brito, Amilcar R. Queiroz, Bin Wang, Andre A. Costa, Elisa G. M. Ferreira, Karin S.F. Fornazier, Ricardo G. Landim, Camila P. Novaes, Larissa Santos, Marcelo V. dos Santos, Jiajun Zhang, Tianyue Chen, Jacques Delabrouille, Clive Dickinson, Giancarlo de Gasperis, Edmar C. Gurjão, Stuart Harper, Yin-Zhe Ma, Telmo Machado, Bruno Maffei, Eduardo J. de Mericia, Christian Monstein, Pablo Motta, Carlos H. N. Otobone, Luiz A. Reitano, Mathieu Remazeilles, Sambit Roychowdhury, João R. L. Santos, Alexandre J. R. Serres, Andreia P. Souza, Cesar Strauss, Jordany Vieira, Haiguang Xu
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664, pp.A15. ⟨10.1051/0004-6361/202039962⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Astronomy and Astrophysics-A&A, 2022, 664, pp.A15. ⟨10.1051/0004-6361/202039962⟩
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
The measurement of diffuse 21-cm radiation from the hyperfine transition of neutral hydrogen (HI signal) in different redshifts is an important tool for modern cosmology. However, detecting this faint signal with non-cryogenic receivers in single-dis