Zobrazeno 1 - 10
of 6 332
pro vyhledávání: '"Llerena P"'
Autor:
Juan Ramos López
Publikováno v:
Entretextos, Vol 18, Iss 34, Pp 344-348 (2024)
La obra de Allen, C. J., & León Llerena, L. M., (TRANS.) (2008). titulada "La coca sabe: coca e identidad cultural en una comunidad andina", realizó su investigación en Sonqo entre los años 1975 y 1985. El objetivo de la etnografía de Catherine
Externí odkaz:
https://doaj.org/article/2dd662dedea54e6f9bb76072fb37e194
Autor:
Isabel Martínez Navas
Publikováno v:
REDUR. Revista Electrónica de Derecho Universidad de La Rioja, Vol 0, Iss 17, Pp 69-136 (2019)
Established in 1485, the Tribunal of the Holy Office of the Inquisition of Llerena was the subject of numerous inspection visits in the 16th and 17th centuries; these inspections determined the accountability of the members of the Court for improper
Externí odkaz:
https://doaj.org/article/d98567fd21b94e148edd2709ee85c0cb
Autor:
Napolitano, Lorenzo, Castellano, Marco, Pentericci, Laura, Vignali, Cristian, Gilli, Roberto, Fontana, Adriano, Santini, Paola, Treu, Tommaso, Calabrò, Antonello, Llerena, Mario, Piconcelli, Enrico, Zappacosta, Luca, Mascia, Sara, Bergamini, Pietro, Bakx, Tom J. L. C., Dickinson, Mark, Glazebrook, Karl, Henry, Alaina, Leethochawalit, Nicha, Mazzolari, Giovanni, Merlin, Emiliano, Morishita, Takahiro, Nanayakkara, Themiya, Paris, Diego, Puccetti, Simonetta, Roberts-Borsani, Guido, Ruiz, Sofia Rojas, Vanzella, Eros, Vito, Fabio, Vulcani, Benedetta, Wang, Xin, Yoon, Ilsang, Zavala, Jorge A.
We present JWST/NIRSpec PRISM spectroscopic characterization of GHZ9 at z= 10.145 $\pm$ 0.010, currently the most distant source detected by the Chandra X-ray Observatory. The spectrum reveals several UV high-ionization lines, including CII, SiIV, [N
Externí odkaz:
http://arxiv.org/abs/2410.18763
Autor:
Napolitano, L., Castellano, M., Pentericci, L., Haro, P. Arrabal, Fontana, A., Treu, T., Bergamini, P., Calabro, A., Mascia, S., Morishita, T., Roberts-Borsani, G., Santini, P., Vanzella, E., Vulcani, B., Zakharova, D., Bakx, T., Dickinson, M., Grillo, C., Leethochawalit, N., Llerena, M., Merlin, E., Paris, D., Rojas-Ruiz, S., Rosati, P., Wang, X., Yoon, I., Zavala, J.
We present JWST/NIRSpec PRISM follow-up of candidate galaxies at z=9-11 selected from deep JWST/NIRCam photometry in GLASS-JWST Early Release Science data. We spectroscopically confirm six sources with secure redshifts at z = 9.52-10.43, each showing
Externí odkaz:
http://arxiv.org/abs/2410.10967
Autor:
Bisigello, L., Gandolfi, G., Feltre, A., Haro, P. Arrabal, Calabrò, A., Cleri, N. J., Costantin, L., Girardi, G., Giulietti, M., Grazian, A., Gruppioni, C., Hathi, N. P., Holwerda, B. W., Llerena, M., Lucas, R. A., Pacucci, F., Prandoni, I., Rodighiero, G., Seillé, L. -M., Wilkins, S. M., Bagley, M., Dickinson., M., Finkelstein, S. L., Kartaltepe, J., Koekemoer, A. M., Papovich, C., Pirzkal, N.
We present the first spectroscopic confirmation of a dust-obscured dwarf galaxy, CEERS-14821. The analysis is performed combining JWST NIRCam broad-band photometry and NIRSpec/PRISM spectroscopic data. From the detection of multiple rest-frame optica
Externí odkaz:
http://arxiv.org/abs/2410.10954
Autor:
Chamorro, Diego, Llerena, David
The micropolar fluid system is a model based on the Navier-Stokes equations which considers two coupled variables: the velocity field $\vec u$ and the microrotation field $\vec\omega$. Assuming an additional condition over the variable $\vec u$ we wi
Externí odkaz:
http://arxiv.org/abs/2406.03291
Autor:
Chávez, Ricardo, Terlevich, Roberto, Terlevich, Elena, González-Morán, Ana, Fernández-Arenas, David, Bresolin, Fabio, Plionis, Manolis, Basilakos, Spyros, Amorín, Ricardo, Llerena, Mario
Over twenty years ago, Type Ia Supernovae (SNIa) [arXiv:astro-ph/9805201, arXiv:astro-ph/9812133] observations revealed an accelerating Universe expansion, suggesting a significant dark energy presence, often modelled as a cosmological constant, $\La
Externí odkaz:
http://arxiv.org/abs/2404.16261
Autor:
Elisa Díaz Álvarez
Publikováno v:
Anuario de la Facultad de Derecho, Universidad de Extremadura, Iss 35, Pp 791-828 (2019)
Crónica
Externí odkaz:
https://doaj.org/article/edbbff10ff6249f997c826935a733ea3
Autor:
Calabro, Antonello, Castellano, Marco, Zavala, Jorge A., Pentericci, Laura, Haro, Pablo Arrabal, Bakx, Tom J. L. C., Burgarella, Denis, Casey, Caitlin M., Dickinson, Mark, Finkelstein, Steven L., Fontana, Adriano, Llerena, Mario, Mascia, Sara, Merlin, Emiliano, Mitsuhashi, Ikki, Napolitano, Lorenzo, Paris, Diego, Perez-Gonzalez, Pablo G., Roberts-Borsani, Guido, Santini, Paola, Treu, Tommaso, Vanzella, Eros
GHZ2/GLASS-z12 has been recently observed by JWST with both NIRSpec and MIRI spectrographs, making it the most distant galaxy ($z_{spec}=12.34$) with complete spectroscopic coverage from rest-frame UV to optical. It is identified as a strong CIV$_{15
Externí odkaz:
http://arxiv.org/abs/2403.12683
Autor:
Castellano, Marco, Napolitano, Lorenzo, Fontana, Adriano, Roberts-Borsani, Guido, Treu, Tommaso, Vanzella, Eros, Zavala, Jorge A., Haro, Pablo Arrabal, Calabrò, Antonello, Llerena, Mario, Mascia, Sara, Merlin, Emiliano, Paris, Diego, Pentericci, Laura, Santini, Paola, Bakx, Tom J. L. C., Bergamini, Pietro, Cupani, Guido, Dickinson, Mark, Filippenko, Alexei V., Glazebrook, Karl, Grillo, Claudio, Kelly, Patrick L., Malkan, Matthew A., Mason, Charlotte A., Morishita, Takahiro, Nanayakkara, Themiya, Rosati, Piero, Sani, Eleonora, Wang, Xin, Yoon, Ilsang
We spectroscopically confirm the $M_{\rm UV} = -20.5$ mag galaxy GHZ2/GLASS-z12 to be at redshift $z=12.34$. The source was selected via NIRCam photometry in GLASS-JWST ERS data, providing the first evidence of a surprising abundance of bright galaxi
Externí odkaz:
http://arxiv.org/abs/2403.10238