Zobrazeno 1 - 10
of 932
pro vyhledávání: '"Gonzalès E"'
Autor:
Sartori José Roberto, Gonzales Elisabeth, Macari Marcos, Dal Pai Vitalino, Oliveira Henrique Nunes de
Publikováno v:
Revista Brasileira de Zootecnia, Vol 32, Iss 4, Pp 918-925 (2003)
O objetivo deste trabalho foi avaliar o efeito da temperatura ambiente sobre as características morfométricas das fibras musculares do músculo flexor longo do hálux de frangos de corte alimentados com a mesma quantidade de ração ("pair-feeding"
Externí odkaz:
https://doaj.org/article/356efebb6228479a8f82c3a7c4237e33
Autor:
Sartori José Roberto, Gonzales Elisabeth, Dal Pai Vitalino, Oliveira Henrique Nunes de, Macari Marcos
Publikováno v:
Revista Brasileira de Zootecnia, Vol 30, Iss 6, Pp 1779-1790 (2001)
O objetivo desta pesquisa foi estudar os efeitos da temperatura ambiente e da restrição alimentar sobre o desempenho e a composição do músculo flexor longo do hálux de frangos de corte. Trezentos e vinte e quatro pintos machos da linhagem Ross,
Externí odkaz:
https://doaj.org/article/1fe94566f6004f0fb80127aacd0215ca
Autor:
Rosenberg Jacob, Ovesen Henrik, Läckberg Zoltan, Jess Per, Heath Jane, Gonzales Elisabeth, Angenete Eva, Thornell Anders, Skullman Stefan, Haglind Eva
Publikováno v:
Trials, Vol 12, Iss 1, p 186 (2011)
Abstract Background Perforated diverticulitis is a condition associated with substantial morbidity. Recently published reports suggest that laparoscopic lavage has fewer complications and shorter hospital stay. So far no randomised study has publishe
Externí odkaz:
https://doaj.org/article/3d4b1dde40d34537a250fbc215ec2963
Publikováno v:
Orphanet Journal of Rare Diseases, Vol 4, Iss 1, p 1 (2009)
Abstract Progressive familial intrahepatic cholestasis (PFIC) refers to heterogeneous group of autosomal recessive disorders of childhood that disrupt bile formation and present with cholestasis of hepatocellular origin. The exact prevalence remains
Externí odkaz:
https://doaj.org/article/a8c63c7ea73e4a1597ac4482cbd40665
Autor:
Peláez-Torres, A., Esparza-Borges, E., Pallé, E., Parviainen, H., Murgas, F., Morello, G., Zapatero-Osorio, M. R., Korth, J., Narita, N., Fukui, A., Carleo, I., Luque, R., García, N. Abreu, Barkaoui, K., Boyle, A., Béjar, V. J. S., Calatayud-Borras, Y., Cheryasov, D. V., Christiansen, J. L., Ciardi, D. R., Enoc, G., Essack, Z., Fukuda, I., Furesz, G., Galán, D., Geraldía-González, S., Giacalone, S., Gill, H., Gonzales, E. J., Hayashi, Y., Ikuta, K., Isogai, K., Kagetani, T., Kawai, Y., Kawauchi, K., Klagyvik, P., Kodama, T., Kusakabe, N., Laza-Ramos, A., de Leon, J. P., Livingston, J. H., Lund, M. B., Madrigal-Aguado, A., Meni, P., Mori, M., Torres, S. Muñoz, Orell-Miquel, J., Puig, M., Ricker, G., Sánchez-Benavente, M., Savel, A. B., Schlieder, J. E., Schwarz, R. P., Sefako, R., Sosa-Guillén, P., Stangret, M., Stockdale, C., Tamura, M., Terada, Y., Twicken, J. D., Watanabe, N., Winn, J., Zheltoukhov, S. G., Ziegler, C., Zou, Y.
The TESS mission searches for transiting exoplanets by monitoring the brightness of hundreds of thousands of stars across the entire sky. M-type planet hosts are ideal targets for this mission due to their smaller size and cooler temperatures, which
Externí odkaz:
http://arxiv.org/abs/2409.07400
Autor:
Hori, Y., Fukui, A., Hirano, T., Narita, N., de Leon, J. P., Ishikawa, H. T., Hartman, J. D., Morello, G., García, N. Abreu, Hernández, L. Álvarez, Béjar, V. J. S., Calatayud-Borras, Y., Carleo, I., Enoc, G., Esparza-Borges, E., Fukuda, I., Galán, D., Geraldía-González, S., Hayashi, Y., Ikoma, M., Ikuta, K., Isogai, K., Kagetani, T., Kawai, Y., Kawauchi, K., Kimura, T., Kodama, T., Korth, J., Kusakabe, N., Laza-Ramos, A., Livingston, J. H., Luque, R., Miyakawa, K., Mori, M., Torres, S. Muñoz, Murgas, F., Orell-Miquel, J., Palle, E., Parviainen, H., Peláez-Torres, A., Puig-Subirá, M., Sánchez-Benavente, M., Sosa-Guillén, P., Stangret, M., Terada, Y., Watanabe, N., Bakos, G. Á., Barkaoui, K., Beichman, C., Benkhaldoun, Z., Boyle, A. W., Ciardi, D. R., Clark, C. A., Collins, K. A., Collins, K. I., Conti, D. M., Crossfield, I. J. M., Everett, M. E., Furlan, E., Ghachoui, M., Gillon, M., Gonzales, E. J., Higuera, J., Horne, K., Howell, S. B., Jehin, E., Lester, K. V., Lund, M. B., Matson, R., Matthews, E. C., Pozuelos, F. J., Safonov, B. S., Schlieder, J. E., Schwarz, R. P., Sefako, R., Srdoc, G., Strakhov, I. A., Waalkes, W. C., Ziegler, C., Charbonneau, D., Essack, Z., Timmermans, M., Guerrero, N. M., Harakawa, H., Hedges, C., Ishizuka, M., Jenkins, J. M., Konishi, M., Kotani, T., Kudo, T., Kurokawa, T., Kuzuhara, M., Nishikawa, J., Omiya, M., Ricker, G. R., Seager, S., Serizawa, T., Striegel, S., Tamura, M., Ueda, A., Vanderspek, R., Vievard, S., Winn, J. N.
Sub-Neptunes with $2-3R_\oplus$ are intermediate in size between rocky planets and Neptune-sized planets. The orbital properties and bulk compositions of transiting sub-Neptunes provide clues to the formation and evolution of close-in small planets.
Externí odkaz:
http://arxiv.org/abs/2405.12637
Autor:
Mallorquín, M., Goffo, E., Pallé, E., Lodieu, N., Béjar, V. J. S., Isaacson, H., Osorio, M. R. Zapatero, Dreizler, S., Stock, S., Luque, R., Murgas, F., Peña, L., Sanz-Forcada, J., Morello, G., Ciardi, D. R., Furlan, E., Collins, K. A., Herrero, E., Vanaverbeke, S., Plavchan, P., Narita, N., Schweitzer, A., Pérez-Torres, M., Quirrenbach, A., Kemmer, J., Hatzes, A. P., Howard, A., Schlecker, M., Reffert, S., Nagel, E., Morales, J. C., Orell-Miquel, J., Duque-Arribas, C., Carleo, I., Cifuentes, C., Nowak, G., Ribas, I., Reiners, A., Amado, P. J., Caballero, J. A., Henning, Th., Pinter, V., Murphy, J. M. Akana, Beard, C., Blunt, S., Brinkman, C. L., Cale, B., Chontos, A., Collins, K. I., Crossfield, I. J. M., Dai, F., Dalba, P. A., Dufoer, S., Mufti, M. El, Espinoza, N., Fetherolf, T., Fukui, A., Giacalone, S., Gnilka, C., Gonzales, E., Grunblatt, S. K., Howell, S., Huber, D., Kane, S. R., de León, J. P., Lubin, J., MacDougall, M. G., Massey, B., Montes, D., Mori, M., Parviainen, H., Passegger, V. M., Polanski, A. S., Robertson, P., Schwarz, R. P., Srdoc, G., Tabernero, H. M., Tanner, A., Turtelboom, E., Van Zandt, J., Weiss, L., Zechmeister, M.
Publikováno v:
A&A 680, A76 (2023)
We report the discovery, mass, and radius determination of TOI-1801 b, a temperate mini-Neptune around a young M dwarf. TOI-1801 b was observed in TESS sectors 22 and 49, and the alert that this was a TESS planet candidate with a period of 21.3 days
Externí odkaz:
http://arxiv.org/abs/2310.10244
Autor:
Naponiello, L., Mancini, L., Sozzetti, A., Bonomo, A. S., Morbidelli, A., Dou, J., Zeng, L., Leinhardt, Z. M., Biazzo, K., Cubillos, P., Pinamonti, M., Locci, D., Maggio, A., Damasso, M., Lanza, A. F., Lissauer, J. J., Bignamini, A., Boschin, W., Bouma, L. G., Carter, P. J., Ciardi, D. R., Collins, K. A., Cosentino, R., Crossfield, I., Desidera, S., Dumusque, X., Fiorenzano, A. F. M., Fukui, A., Giacobbe, P., Gnilka, C. L., Ghedina, A., Gonzales, E., Guilluy, G., Harutyunyan, A., Howell, S. B., Jenkins, J. M., Lund, M. B., Jensen, E. L. N., Kielkopf, J. F., Lester, K. V., Malavolta, L., Mann, A. W., Matson, R. A., Matthews, E. C., Nardiello, D., Narita, N., Pace, E., Pagano, I., Palle, E., Pedani, M., Seager, S., Schlieder, J. E., Schwarz, R. P., Shporer, A., Twicken, J. D., Winn, J. N., Ziegler, C., Zingales, T.
Publikováno v:
Nature, published online on the 30th of August 2023 and printed the 12th of October 2023
Neptune-sized planets exhibit a wide range of compositions and densities, depending onf cators related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relativel
Externí odkaz:
http://arxiv.org/abs/2309.01464
Autor:
Damasso, M., Rodrigues, J., Castro-González, A., Lavie, B., Davoult, J., Osorio, M. R. Zapatero, Dou, J., Sousa, S. G., Owen, J. E., Sossi, P., Adibekyan, V., Osborn, H., Leinhardt, Z., Alibert, Y., Lovis, C., Mena, E. Delgado, Sozzetti, A., Barros, S. C. C., Bossini, D., Ziegler, C., Ciardi, D. R., Matthews, E. C., Carter, P. J., Lillo-Box, J., Mascareño, A. Suárez, Cristiani, S., Pepe, F., Rebolo, R., Santos, N. C., Prieto, C. Allende, Benatti, S., Bouchy, F., Briceño, C., Di Marcantonio, P., D'Odorico, V., Dumusque, X., Egger, J. A., Ehrenreich, D., Faria, J., Figueira, P., Santos, R. Génova, Gonzales, E. J., Hernández, J. I. González, Law, N., Curto, G. Lo, Mann, A. W., Martins, C. J. A. P., Mehner, A., Micela, G., Molaro, P., Nunes, N. J., Palle, E., Poretti, E., Schlieder, J. E., Udry, S.
We followed-up with ESPRESSO the K0V star HIP 29442 (TOI-469), already known to host a validated sub-Neptune companion TOI-469.01. We aim to verify the planetary nature of TOI-469.01. We modelled radial velocity and photometric time series to measure
Externí odkaz:
http://arxiv.org/abs/2308.13310
Autor:
Hartman, J. D., Bakos, G. Á., Csubry, Z., Howard, A. W., Isaacson, H., Giacalone, S., Chontos, A., Narita, N., Fukui, A., de Leon, J. P., Watanabe, N., Mori, M., Kagetani, T., Fukuda, I., Kawai, Y., Ikoma, M., Palle, E., Murgas, F., Esparza-Borges, E., Parviainen, H., Bouma, L. G., Cointepas, M., Bonfils, X., Almenara, J. M., Collins, Karen A., Collins, Kevin I., Relles, Howard M., Barkaoui, Khalid, Schwarz, Richard P., Mourad, Ghachoui, Timmermans, Mathilde, Dransfield, Georgina, Burdanov, Artem, de Wit, Julien, Jehin, Emmanuël, Triaud, Amaury H. M. J., Gillon, Michaël, Benkhaldoun, Zouhair, Horne, Keith, Sefako, Ramotholo, Jordán, A., Brahm, R., Suc, V., Howell, Steve B., Furlan, E., Schlieder, J. E., Ciardi, D., Barclay, T., Gonzales, E. J., Crossfield, I., Dressing, C. D., Goliguzova, M., Tatarnikov, A., Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Striegel, Stephanie, Shporer, Avi, Vanderburg, Andrew, Levine, Alan M., Kostov, Veselin B., Watanabe, David
We present the discovery from the TESS mission of two giant planets transiting M dwarf stars: TOI 4201 b and TOI 5344 b. We also provide precise radial velocity measurements and updated system parameters for three other M dwarfs with transiting giant
Externí odkaz:
http://arxiv.org/abs/2307.06809