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pro vyhledávání: '"Santos, J. S."'
In this work, we investigate the quasinormal modes for a massive scalar field with a nonminimal coupling with gravity in the spacetime of a loop quantum black hole, known as the Self-Dual Black Hole. In this way, we have calculated the characteristic
Externí odkaz:
http://arxiv.org/abs/2103.11212
Akademický článek
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Autor:
SANTOS, J. S.
Publikováno v:
Repositório Institucional da UFESUniversidade Federal do Espírito SantoUFES.
Made available in DSpace on 2016-08-29T11:11:31Z (GMT). No. of bitstreams: 1 tese_4138_JÚLIO SANTOS.pdf: 2026142 bytes, checksum: 259ca4b6ca579442431f23457e52dbcc (MD5) Previous issue date: 2010-05-19
Esse estudo tem como objetivo geral problem
Esse estudo tem como objetivo geral problem
Externí odkaz:
http://repositorio.ufes.br/handle/10/2261
Autor:
SANTOS, J. S.
Publikováno v:
Repositório Institucional da UFESUniversidade Federal do Espírito SantoUFES.
Made available in DSpace on 2016-08-29T11:04:08Z (GMT). No. of bitstreams: 1 tese_9017_TESE__JÚLIO_SANTOS_2015.pdf: 7747404 bytes, checksum: 1c2232c3753423b1a4a5bdb6de733de9 (MD5) Previous issue date: 2015-08-13
O ano de 2015 é um marco histó
O ano de 2015 é um marco histó
Externí odkaz:
http://repositorio.ufes.br/handle/10/2240
Autor:
Oliveira, E. M., Rodrigues, A., Santos, J. S., Trivinho-Strixino, F., Dalla Costa da Rocha, R., Sikora, M. S.
Publikováno v:
Environmental Technology; Nov2024, Vol. 45 Issue 26, p5568-5580, 13p
Autor:
Santos, J. S., Balestra, I., Tozzi, P., Altieri, B., Valtchanov, I., Mercurio, A., Nonino, M., Yu, Heng, Rosati, P., Grillo, C., Medezinski, E., Biviano, A.
We investigate the dust-obscured star formation properties of the massive, X-ray selected galaxy cluster MACS J1931.8-2634 at $z$=0.352. Using far-infrared (FIR) imaging in the range 100-500$\mu$m obtained with the \textit{Herschel} telescope, we ext
Externí odkaz:
http://arxiv.org/abs/1511.03089
Autor:
Tozzi, P., Gastaldello, F., Molendi, S., Ettori, S., Santos, J. S., De Grandi, S., Balestra, I., Rosati, P., Altieri, B., Cresci, G., Menanteau, F., Valtchanov, I.
Publikováno v:
A&A 580, A6 (2015)
(Abridged) We present a spectral analysis of a deep (220 ks) XMM-Newton observation of the Phoenix cluster (SPT-CL J2344-4243), which we also combine with Chandra archival ACIS-I data. We extract CCD and RGS X-ray spectra from the core region to sear
Externí odkaz:
http://arxiv.org/abs/1505.06913
Autor:
Tozzi, P., Santos, J. S., Jee, M. J., Fassbender, R., Rosati, P., Nastasi, A., Forman, W., Sartoris, B., Borgani, S., Boehringer, H., Altieri, B., Pratt, G. W., Nonino, M., Jones, C.
We report the analysis of the Chandra observation of XDCP J0044.0-2033, a massive, distant (z=1.579) galaxy cluster discovered in the XDCP survey. The total exposure time of 380 ks with Chandra ACIS-S provides the deepest X-ray observation currently
Externí odkaz:
http://arxiv.org/abs/1412.5200
Autor:
Dannerbauer, H., Kurk, J. D., De Breuck, C., Wylezalek, D., Santos, J. S., Koyama, Y., Seymour, N., Tanaka, M., Hatch, N., Altieri, B., Coia, D., Galametz, A., Kodama, T., Miley, G., Röttgering, H., Sanchez-Portal, M., Valtchanov, I., Venemans, B., Ziegler, B.
We present APEX LABOCA 870 micron observations of the field around the high-redshift radio galaxy MRC1138-262 at z=2.16. We detect 16 submillimeter galaxies in this ~140 square arcmin bolometer map with flux densities in the range 3-11 mJy. The raw n
Externí odkaz:
http://arxiv.org/abs/1410.3730
Autor:
Fassbender, R., Nastasi, A., Santos, J. S., Lidman, C., Verdugo, M., Koyama, Y., Rosati, P., Pierini, D., Padilla, N., Romeo, A. D., Menci, N., Bongiorno, A., Castellano, M., Cerulo, P., Fontana, A., Galametz, A., Grazian, A., Lamastra, A., Pentericci, L., Sommariva, V., Strazzullo, V., Suhada, R., Tozzi, P.
Publikováno v:
A&A 568, A5 (2014)
We investigate various galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 at z=1.58, which constitutes the most extreme matter density peak at this redshift currently known. We analyze deep VLT/HAWK-I NIR data
Externí odkaz:
http://arxiv.org/abs/1406.3037