Zobrazeno 1 - 10
of 58
pro vyhledávání: '"P. J., Amado"'
Autor:
Daniel M. Rojas, Mauricio Gutierrez, Danuil E. Dueñas, Monica A. Martinez, Samuel Valovis, Fernando W. Londoño, Carlos J. Valencia, Andrey F. Salamanca, Juan C. Vargas, Aramis Visbal, Sady S. Salazar, Sergio A. Celis, Diego F. Leon, Cindy N. Isaza, Leidy L. Alvarez, Francisco J. Amado, Rubén H. Castro
Publikováno v:
Revista Fuentes El Reventón Energético, Vol 21, Iss 2, Pp 61-83 (2023)
La canalización generalmente es consecuencia de la heterogeneidad del yacimiento, especialmente por grandes variaciones de permeabilidad, ocasionando reducción en la eficiencia volumétrica como producto de la recirculación del fluido inyectado en
Externí odkaz:
https://doaj.org/article/9fd95d5019a547bc86e846cb59d390dd
Autor:
Dominik Hintz, Sarah Peacock, Travis Barman, Birgit Fuhrmeister, Evangelos Nagel, Andreas Schweitzer, Sandra V. Jeffers, Ignasi Ribas, Ansgar Reiners, Andreas Quirrenbach, Pedro J. Amado, Victor J. S. Béjar, José A. Caballero, Artie P. Hatzes, David Montes
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 1, p 73 (2023)
Ahead of upcoming space missions intending to conduct observations of low-mass stars in the ultraviolet (UV) spectral region it becomes imperative to simultaneously conduct atmospheric modeling from the UV to the visible (VIS) and near-infrared (NIR)
Externí odkaz:
https://doaj.org/article/e76615495d574a12839b148c7693cd27
Autor:
A.P. Lopes, M.A. Mineiro, F. Costa, J. Gomes, C. Santos, C. Antunes, D. Maia, R. Melo, M. Canotilho, E. Magalhães, I. Vicente, C. Valente, B.G. Gonçalves, B. Conde, C. Guimarães, C. Sousa, J. Amado, M.E. Brandão, M. Sucena, M.J. Oliveira, S. Seixas, V. Teixeira, L. Telo
Publikováno v:
Pulmonology, Vol 24, Iss , Pp 1-21 (2018)
Alpha-1-antitrypsin deficiency (AATD) is a genetic autosomal codominant disorder caused by mutations in SERPINA1 gene. It is one of the most prevalent genetic disorders, although it remains underdiagnosed. Whereas at international level there are sev
Externí odkaz:
https://doaj.org/article/3b0c412319364f6ab6501f605d4fd9b6
Autor:
Mary Katherine Gardner, Patricia J. Amado, Muhummad Usman Baig, Sana Mohiuddin, Avis Harden, Linette J. Ewing, Shehla Razvi, Jose A. Cortes, Rodrigo Mejia, Demetrios Petropoulos, Priti Tewari, Ali H. Ahmad
Publikováno v:
Children, Vol 9, Iss 4, p 580 (2022)
Standardized rounding checklists during multidisciplinary rounds (MDR) can reduce medical errors and decrease length of pediatric intensive care unit (PICU) and hospital stay. We added a standardized process for MDR in our oncologic PICU. Our study w
Externí odkaz:
https://doaj.org/article/6e7867df0d31425b89daae34fed0d630
Autor:
M. Perger, G. Anglada-Escudé, D. Baroch, M. Lafarga, I. Ribas, J. C. Morales, E. Herrero, P. J. Amado, J. R. Barnes, J. A. Caballero, S. V. Jeffers, A. Quirrenbach, A. Reiners
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da9b6ca00f33f0232791e4adab3bd337
http://hdl.handle.net/10261/322991
http://hdl.handle.net/10261/322991
Autor:
I. Ribas, A. Reiners, M. Zechmeister, J. A. Caballero, J. C. Morales, S. Sabotta, D. Baroch, P. J. Amado, A. Quirrenbach, M. Abril, J. Aceituno, G. Anglada-Escudé, M. Azzaro, D. Barrado, V. J. S. Béjar, D. Benítez de Haro, G. Bergond, P. Bluhm, R. Calvo Ortega, C. Cardona Guillén, P. Chaturvedi, C. Cifuentes, J. Colomé, D. Cont, M. Cortés-Contreras, S. Czesla, E. Díez-Alonso, S. Dreizler, C. Duque-Arribas, N. Espinoza, M. Fernández, B. Fuhrmeister, D. Galadí-Enríquez, A. García-López, E. González-Álvarez, J. I. González Hernández, E. W. Guenther, E. de Guindos, A. P. Hatzes, Th. Henning, E. Herrero, D. Hintz, Á. L. Huelmo, S. V. Jeffers, E. N. Johnson, E. de Juan, A. Kaminski, J. Kemmer, J. Khaimova, S. Khalafinejad, D. Kossakowski, M. Kürster, F. Labarga, M. Lafarga, S. Lalitha, M. Lampón, J. Lillo-Box, N. Lodieu, M. J. López González, M. López-Puertas, R. Luque, H. Magán, L. Mancini, E. Marfil, E. L. Martín, S. Martín-Ruiz, K. Molaverdikhani, D. Montes, E. Nagel, L. Nortmann, G. Nowak, E. Pallé, V. M. Passegger, A. Pavlov, S. Pedraz, V. Perdelwitz, M. Perger, A. Ramón-Ballesta, S. Reffert, D. Revilla, E. Rodríguez, C. Rodríguez-López, S. Sadegi, M. Á. Sánchez Carrasco, A. Sánchez-López, J. Sanz-Forcada, S. Schäfer, M. Schlecker, J. H. M. M. Schmitt, P. Schöfer, A. Schweitzer, W. Seifert, Y. Shan, S. L. Skrzypinski, E. Solano, O. Stahl, M. Stangret, S. Stock, J. Stürmer, H. M. Tabernero, L. Tal-Or, T. Trifonov, S. Vanaverbeke, F. Yan, M. R. Zapatero Osorio
Publikováno v:
Astronomy and Astrophysics
The CARMENES instrument was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The broad wavelength coverage was designed to provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b8cfde360b03faee5da32e1d3b118d3
https://hdl.handle.net/21.11116/0000-000C-B462-A
https://hdl.handle.net/21.11116/0000-000C-B462-A
Autor:
J. Blanco-Pozo, M. Perger, M. Damasso, G. Anglada Escudé, I. Ribas, D. Baroch, J. A. Caballero, C. Cifuentes, S. V. Jeffers, M. Lafarga, A. Kaminski, S. Kaur, E. Nagel, V. Perdelwitz, M. Pérez-Torres, A. Sozzetti, D. Viganò, P. J. Amado, G. Andreuzzi, V. J. S. Béjar, E. L. Brown, F. Del Sordo, S. Dreizler, D. Galadí-Enríquez, A. P. Hatzes, M. Kürster, A. F. Lanza, A. Melis, E. Molinari, D. Montes, M. Murgia, E. Pallé, L. Peña-Moñino, D. Perrodin, M. Pilia, E. Poretti, A. Quirrenbach, A. Reiners, A. Schweitzer, M. R. Zapatero Osorio, M. Zechmeister
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf77027919a5f79d8528d286d3a46de1
Autor:
D. Kossakowski, M. Kürster, T. Trifonov, Th. Henning, J. Kemmer, J. A. Caballero, R. Burn, S. Sabotta, J. S. Crouse, T. J. Fauchez, E. Nagel, A. Kaminski, E. Herrero, E. Rodríguez, E. González-Álvarez, A. Quirrenbach, P. J. Amado, I. Ribas, A. Reiners, J. Aceituno, V. J. S. Béjar, D. Baroch, S. T. Bastelberger, P. Chaturvedi, C. Cifuentes, S. Dreizler, S. V. Jeffers, R. Kopparapu, M. Lafarga, M. J. López-González, S. Martín-Ruiz, D. Montes, J. C. Morales, E. Pallé, A. Pavlov, S. Pedraz, V. Perdelwitz, M. Pérez-Torres, M. Perger, S. Reffert, C. Rodríguez López, M. Schlecker, P. Schöfer, A. Schweitzer, Y. Shan, A. Shields, S. Stock, E. Wolf, M. R. Zapatero Osorio, M. Zechmeister
Publikováno v:
Astronomy and Astrophysics
We present the discovery of an Earth-mass planet ($M_b\sin i = 1.26\pm0.21M_\oplus$) on a 15.6d orbit of a relatively nearby ($d\sim$9.6pc) and low-mass ($0.167\pm0.011 M_\odot$) M5.0V star, Wolf 1069. Sitting at a separation of $0.0672\pm0.0014$au a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d0f6c669db9fb87600abf790cc0e855
https://hdl.handle.net/21.11116/0000-000C-AB8F-3
https://hdl.handle.net/21.11116/0000-000C-AB8F-3
Autor:
A. Suárez Mascareño, M. Damasso, N. Lodieu, A. Sozzetti, V. J. S. Béjar, S. Benatti, M. R. Zapatero Osorio, G. Micela, R. Rebolo, S. Desidera, F. Murgas, R. Claudi, J. I. González Hernández, L. Malavolta, C. del Burgo, V. D’Orazi, P. J. Amado, D. Locci, H. M. Tabernero, F. Marzari, D. S. Aguado, D. Turrini, C. Cardona Guillén, B. Toledo-Padrón, A. Maggio, J. Aceituno, F. F. Bauer, J. A. Caballero, P. Chinchilla, E. Esparza-Borges, E. González-Álvarez, T. Granzer, R. Luque, E. L. Martín, G. Nowak, M. Oshagh, E. Pallé, H. Parviainen, A. Quirrenbach, A. Reiners, I. Ribas, K. G. Strassmeier, M. Weber, M. Mallonn
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years1,2. These theoretical expectations remai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e3e7e7ccf0ffdcc878d3580171eb7d5
https://doi.org/10.1038/s41550-021-01533-7
https://doi.org/10.1038/s41550-021-01533-7
Autor:
A. Suárez Mascareño, E. González-Álvarez, M. R. Zapatero Osorio, J. Lillo-Box, J. P. Faria, V. M. Passegger, J. I. González Hernández, P. Figueira, A. Sozzetti, R. Rebolo, F. Pepe, N. C. Santos, S. Cristiani, C. Lovis, A. M. Silva, I. Ribas, P. J. Amado, J. A. Caballero, A. Quirrenbach, A. Reiners, M. Zechmeister, V. Adibekyan, Y. Alibert, V. J. S. Béjar, S. Benatti, V. D’Odorico, M. Damasso, J.-B. Delisle, P. Di Marcantonio, S. Dreizler, D. Ehrenreich, A. P. Hatzes, N. C. Hara, Th. Henning, A. Kaminski, M. J. López-González, C. J. A. P. Martins, G. Micela, D. Montes, E. Pallé, S. Pedraz, E. Rodríguez, C. Rodríguez-López, L. Tal-Or, S. Sousa, S. Udry
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1584dc6c075fb22abc8242da3c89c47f
http://arxiv.org/abs/2212.07332
http://arxiv.org/abs/2212.07332