Zobrazeno 1 - 10
of 825
pro vyhledávání: '"Eugênio C"'
Autor:
Pérez-Martínez, J. M., Dannerbauer, H., Emonts, B. H. C., Allison, J. R., Champagne, J. B., Indermuehle, B., Norris, R. P., Serra, P., Seymour, N., Thomson, A. P., Casey, C. M., Chen, Z., Daikuhara, K., De Breuck, C., D'Eugenio, C., Drouart, G., Hatch, N., Jin, S., Kodama, T., Koyama, Y., Lehnert, M. D., Macgregor, P., Miley, G., Naufal, A., Röttgering, H., Sánchez-Portal, M., Shimakawa, R., Zhang, Y., Ziegler, B.
We obtain CO(1-0) molecular gas measurements with ATCA on a sample of 43 spectroscopically confirmed H$\alpha$ emitters in the Spiderweb protocluster at $z=2.16$ and investigate the relation between their star formation and cold gas reservoirs as a f
Externí odkaz:
http://arxiv.org/abs/2411.12138
Autor:
Zhang, Y. H., Dannerbauer, H., Pérez-Martínez, J. M., Koyama, Y., Zheng, X. Z., D'Eugenio, C., Emonts, B. H. C., Calvi, R., Chen, Z., Daikuhara, K., De Breuck, C., Jin, S., Kodama, T., Lehnert, M. D., Naufal, A., Shimakawa, R.
Publikováno v:
A&A 692, A22 (2024)
We report the results of the deep and wide Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm mapping of the Spiderweb protocluster at $z=2.16$. The observations were divided into six contiguous fields covering a survey area of 19.3\,arcmin$^
Externí odkaz:
http://arxiv.org/abs/2410.10169
Autor:
Luiz Guilherme G. Porto, Rosenkranz M. Nogueira, Eugênio C. Nogueira, Guilherme E. Molina, Andrea Farioli, Luiz Fernando Junqueira Jr., Stefanos N. Kales
Publikováno v:
Archives of Endocrinology and Metabolism, Vol 60, Iss 6, Pp 515-525 (2016)
ABSTRACT Objectives Body mass index (BMI) is a widely used proxy of body composition (BC). Concerns exist regarding possible BMI misclassification among active populations. We compared the prevalence of obesity as categorized by BMI or by skinfold es
Externí odkaz:
https://doaj.org/article/b234ab64224e4f15911792e1f587c24f
Publikováno v:
A&A 678, L9 (2023)
Many efforts have been done in recent years to probe the gas fraction evolution of massive quiescent galaxies (QGs); however, a clear picture has not yet been established. Recent spectroscopic confirmations at z>3 offer the chance to measure the resi
Externí odkaz:
http://arxiv.org/abs/2309.12730
Autor:
Melo, Antonio, Costa, Joana, Quintelas, Cristina, Amaral, António L., Ferreira, Eugénio C., Mesquita, Daniela P.
Publikováno v:
In Separation and Purification Technology 3 December 2024 349
Autor:
D'Eugenio, C., Daddi, E., Gobat, R., Strazzullo, V., Lustig, P., Delvecchio, I., Jin, S., Cimatti, A., Onodera, M.
Publikováno v:
A&A 653, A32 (2021)
Tracing the emergence of the massive quiescent galaxy (QG) population requires the build-up of reliable quenched samples. We present Hubble Space Telescope WFC3/G141 grism spectra of 10 quiescent galaxy candidates selected at $2.5
Externí odkaz:
http://arxiv.org/abs/2012.02767
Autor:
Delvecchio, I., Daddi, E., Sargent, M. T., Jarvis, M. J., Elbaz, D., Jin, S., Liu, D., Whittam, I. H., Algera, H., Carraro, R., D'Eugenio, C., Delhaize, J., Kalita, B. S., Leslie, S., Molnar, D. Cs., Novak, M., Prandoni, I., Smolcic, V., Ao, Y., Aravena, M., Bournaud, F., Collier, J. D., Randriamampandry, S. M., Randriamanakoto, Z., Rodighiero, G., Schober, J., White, S. V., Zamorani, G.
Publikováno v:
A&A 647, A123 (2021)
Several works in the past decade have used the ratio between total (rest 8-1000$\mu$m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q$_{IR}$), often referred to as the "infrared-radio correlation" (IRRC), to calibrate radio
Externí odkaz:
http://arxiv.org/abs/2010.05510
Autor:
Daddi, E., Valentino, F., Rich, R. M., Neill, J. D., Gronke, M., O'Sullivan, D., Elbaz, D., Bournaud, F., Finoguenov, A., Marchal, A., Delvecchio, I., Jin, S., Liu, D., Calabro, A., Coogan, R., D'Eugenio, C., Gobat, R., Kalita, B. S., Laursen, P., Martin, D. C., Puglisi, A., Schinnerer, E., Strazzullo, V., Wang, T.
We have discovered a 300kpc-wide giant Lya nebula centered on the massive galaxy group RO-1001 at z=2.91 in the COSMOS field. Keck Cosmic Web Imager observations reveal three cold gas filaments converging into the center of the potential well of its
Externí odkaz:
http://arxiv.org/abs/2006.11089
Autor:
D'Eugenio, C., Daddi, E., Gobat, R., Strazzullo, V., Lustig, P., Delvecchio, I., Jin, S., Puglisi, A., Calabró, A., Mancini, C., Dickinson, M., Cimatti, A., Onodera, M.
We have obtained spectroscopic confirmation with Hubble Space Telescope WFC3/G141 of a first sizeable sample of nine quiescent galaxies at 2.4
Externí odkaz:
http://arxiv.org/abs/2003.04342
Autor:
Braga, Adelaide, Mesquita, Daniela P., Cordeiro, Ana, Belo, Isabel, Ferreira, Eugénio C., Amaral, A. Luís
Publikováno v:
In Process Biochemistry June 2023 129:221-229