1,730 results on '"Hernández N"'
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2. Least action description of dynamic pairing correlations in the fission of Curium and Californium isotopes based on the Gogny energy density functional
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Rodriguez-Guzman, R., Robledo, L. M., Jimenez-Hoyos, C. A., and Hernandez, N. C.
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Nuclear Theory - Abstract
The impact of dynamic pairing correlations and their interplay with Coulomb antipairing effects on the systematic of the spontaneous fission half-lives for the nuclei $^{240-250}$Cm and $^{240-250}$Cf is analyzed, using a hierarchy of approximations based on the parametrization D1M of the Gogny energy density functional (EDF). First, the constrained Hartree-Fock-Bogoliubov (HFB) approximation is used to compute deformed mean-field configurations, zero-point quantum corrections and collective inertias either by using the Slater approximation to Coulomb exchange and neglecting Coulomb antipairing or by fully considering the exchange and pairing channels of the Coulomb interaction. Next, the properties of the {\it{least action}} and {\it{least energy}} fission paths are compared. In the {\it{least action}} case, pairing is identified as the relevant degree of freedom in order to minimize the action entering the Wentzel-Kramers-Brillouin (WKB) approximation to the tunneling probability through the fission barrier. Irrespective of the treatment of Coulomb exchange and antipairing, it is shown that the {\it{least action}} path obtained taking into account the pairing degree of freedom leads to stronger pairing correlations that significantly reduce the spontaneous fission half-lives $t_{SF}$ improving thereby the comparison with the experiment by several orders of magnitude. It is also shown that the Coulomb antipairing effect is, to a large extent, washed out by the {\it{least action}} procedure and therefore the $t_{SF}$ values obtained by the two different treatments of the Coulomb exchange and pairing are of similar quality., Comment: 13 pages, 8 figures
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- 2023
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3. 3-Acetylpyridine-induced ataxic-like motor impairments are associated with plastic changes in the Purkinje cells of the rat cerebellum
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González-Tapia, D., Vázquez-Hernández, N., Urmeneta-Ortiz, F., Navidad-Hernandez, N., Lazo-Yepez, M., Tejeda-Martínez, A., Flores-Soto, M., and González-Burgos, I.
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- 2024
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4. Neutral donors confined in semiconductor coupled quantum dot-rings: Position-dependent properties and optical transparency phenomenon
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Hernández, N., López-Doria, R.A., Suaza, Y.A., and Fulla, M.R.
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- 2025
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5. The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18
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Castro-González, A., Alonso, E. Díez, Blanco, J. Menéndez, Livingston, J., de Leon, J. P., Lillo-Box, J., Korth, J., Menéndez, S. Fernández, Recio, J. M., Izquierdo-Ruiz, F., Lozano, A. Coya, de la Cuesta, F. García, Hernández, N. Gómez, Blanco, J. R. Vidal, Díaz, R. Hevia, Silva, R. Pardo, Acevedo, S. Pérez, Ruiz, J. Polancos, Tijerín, P. Padilla, García, D. Vázquez, Gómez, S. L. Suárez, Riesgo, F. García, Gutiérrez, C. González, Bonavera, L., González-Nuevo, J., Pereira, C. Rodríguez, Lasheras, F. Sánchez, Rodríguez, M. L. Sánchez, Muñiz, R., Rodríguez, J. D. Santos, and Juez, F. J. de Cos
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Astrophysics - Earth and Planetary Astrophysics - Abstract
We present the first results of K2-OjOS, a collaborative project between professional and amateur astronomers primarily aimed to detect, characterize, and validate new extrasolar planets. For this work, 10 amateur astronomers looked for planetary signals by visually inspecting the 20 427 light curves of K2 campaign 18 (C18). They found 42 planet candidates, of which 18 are new detections and 24 had been detected in the overlapping C5 by previous works. We used archival photometric and spectroscopic observations, as well as new high-spatial resolution images in order to carry out a complete analysis of the candidates found, including a homogeneous characterization of the host stars, transit modelling, search for transit timing variations and statistical validation. As a result, we report four new planets (K2-355 b, K2-356 b, K2-357 b, and K2-358 b) and 14 planet candidates. Besides, we refine the transit ephemeris of the previously published planets and candidates by modelling C5, C16 (when available) and C18 photometric data jointly, largely improving the period and mid-transit time precision. Regarding individual systems, we highlight the new planet K2-356 b and candidate EPIC 211537087.02 being near a 2:1 period commensurability, the detection of significant TTVs in the bright star K2-184 (V = 10.35), the location of K2-103 b inside the habitable zone according to optimistic models, the detection of a new single transit in the known system K2-274, and the disposition reassignment of K2-120 b, which we consider as a planet candidate as the origin of the signal cannot be ascertained., Comment: Accepted for publication in MNRAS
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- 2021
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6. Post-stroke sexual dysfunction in males
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Romero-Hernández, C.A., Gómez-Salazar, N., Pradilla-Andrade, I.F., and Hernández, N.
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- 2024
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7. Spectral and optical properties of a [formula omitted] molecular complex confined in InAs/GaAs Quantum Camels: A spatial finite element method treatment
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López-Doria, R.A., Hernández, N., Rivera, I.E., and Fulla, M.R.
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- 2024
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8. Cirugía de la enfermedad inflamatoria intestinal en España: ¿cómo lo estamos haciendo? Resultados iniciales de un registro prospectivo nacional (Registro REIC)
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Enriquez-Navascues, J.M., Elorza-Echaniz, G., Die Trill, J., Ocaña Jimenez, J., Moro-Valdezate, D., Leon-Espinoza, C., Primo-Romaguera, V., Sancho-Muriel, J., Pascual Migueláñez, I., Saavedra, J., Penín de Oliveira, P., Meceira Quintian, F., Carmona Agúndez, M., Gallarín Salamanca, I.M., Lopez de los Reyes, R., Vives Rodriguez, E., Navarro-Sáncheze, A., Soto-Darias, I., Monjero Ares, I., Torres García, M.I., Aldrey Cao, I., Barreiro Dominguez, E.M., Diz Jueguen, S., Bernal Sprekelsen, J.C., Ivorra García-Moncó, P., Vigorita, V., Nogueira Sixto, M., Martín Dieguez, C., López Bañeres, M., Pérez Pérez, T., Añón Iranzo, E., Vázquez-Bouzán, R., Sánchez Espinel, E., Alberdi San Roman, I., Trujillo Barbadillo, A., Martínez-García, R., Menárguez Pina, F.J., Anula Fernández, R., Mayol Martínez, J.A., Romero de Diego, A., de Andres-Asenjo, B., Ibáñez Cánovas, N., Abrisqueta Carrión, J., Estaire Gómez, M., Lorente Poyatos, R.H., Julià-Bergkvist, D., Gómez-Romeu, N., Romero-Simó, M., Mauri-Barberá, F., Arroyo, A., Alcaide-Quiros, M.J., Hernandis Villalba, J.V., Espinosa Soria, J., Parés, D., Corral, J., Jiménez-Gómez, L.M., Zorrilla Ortúzar, J., Abellán Morcillo, I., Bernabé Peñalver, A., Parra Baños, P.A., Muñoz Camarena, J.M., Abellán Garay, L., Milagros Carrasco, M., Rufas Acín, M.P., Ambrona Zafra, D., Padín Álvarez, M.H., Lora Cumplido, P., Fernández-Cepedal, L., García-González, J.M., Pérez Viejo, E., Huerga Álvarez, D., Valle Rubio, A., Jiménez Carneros, V., Arencibia-Pérez, B., Roque-Castellano, C., Ríos Blanco, R., Espina Pérez, B., Caro Tarrago, A., Saeta Campo, R., Illan Riquelme, A., Bermejo Marcos, E., Rodríguez Sánchez, A., Cagigas Fernández, C., Cristóbal Poch, L., Duque Mallen, M.V., Santero Ramírez, M.P., Aguilar Martínez, M.M., Moreno Navas, A., Gallardo Valverde, J.M., Choolani Bhojwani, E., Veleda Belanche, S., Díaz-Maag, C.R., Rodríguez-García, R., Alberca Páramo, A., Pineda Navarro, N., Ferrer Inaebnit, E., Alonso Hernández, N., Ferrer-Márquez, M., Gómez-Carmona, Z., Ramos Fernandez, M., Sanchiz Cardenas, E., Valdes-Hernandez, J., Pérez Sánchez, A., Labalde Martínez, M., García Borda, F.J., Fernández Arias, S., Fernández Hevia, M., Elosua González, T., Jimenez Alvarez, L., Sánchez-Guillén, L., Blanco-Antona, F., Soler-Silva, Á., and Millán, M.
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- 2024
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9. Newman-Janis Ansatz for rotating wormholes
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Gutiérrez-Piñeres, A. C., Hernández, N., and Lopez-Monsalvo, C. S.
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General Relativity and Quantum Cosmology - Abstract
A central problem in General Relativity is obtaining a solution to describe the source's interior counterpart for Kerr black hole. Besides, determining a method to match the interior and exterior solutions through a surface free of predefined coordinates remains an open problem. In this work, we present the ansatz formulated by Newman-Janis to generate solutions to the Einstein field equation inspired by the mentioned problems. We present a collection of independent classes of exact interior solutions of the Einstein equation describing rotating fluids with anisotropic pressures. Furthermore, we will elaborate on some obtained solutions by alluding to rotating wormholes., Comment: Paper prepared for presentation at the XXII International Meeting Physical Interpretations of Relativity Theory - 2021 (Moscow, Russia)
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- 2021
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10. Evolution of octupole deformation and collectivity in neutron-rich lanthanides
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Nomura, K., Rodríguez-Guzmán, R., Robledo, L. M., García-Ramos, J. E., and Hernández, N. C.
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Nuclear Theory ,Nuclear Experiment - Abstract
The onset of octupole deformation and its impact on related spectroscopic properties is studied in even-even neutron-rich lanthanide isotopes Xe, Ba, Ce, and Nd with neutron number $86\leqslant N\leqslant 94$. Microscopic input comes from the Hartree-Fock-Bogoliubov approximation with constrains on the axially symmetric quadrupole and octupole operators using the Gogny-D1M interaction. At the mean-field level, reflection asymmetric ground states are predicted for isotopes with neutron number around $N=88$. Spectroscopic properties are studied by diagonalizing the interacting boson model Hamiltonian, with the parameters obtained via the mapping of the mean-field potential energy surface onto the expectation value of the Hamiltonian in the $s$, $d$, and $f$ boson condensate state. The results obtained for low-energy positive- and negative-parity excitation spectra as well as the electric dipole, quadrupole, and octupole transition probabilities indicate the onset of pronounced octupolarity for $Z\approx 56$ and $N\approx 88$ nuclei., Comment: 15 pages, 13 figures, 2 tables
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- 2021
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11. Rechallenge in idiosyncratic drug-induced liver injury: An analysis of cases in two large prospective registries according to existing definitions
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Pinazo-Bandera, J.M., Niu, H., Alvarez-Alvarez, I., Medina-Cáliz, I., Del Campo-Herrera, E., Ortega-Alonso, A., Robles-Díaz, M., Hernández, N., Paraná, R., Nunes, V., Girala, M., Bessone, F., Lucena, M.I., Andrade, R.J., and García Cortés, M.
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- 2024
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12. Analysis of real-time data gathered using a mobile application from patients treated after code stroke activation in Alicante
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Ros Arlanzón, P., Aledo Sala, C., Hernández Lorido, R., Beltrán Blasco, I., and López Hernández, N.
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- 2024
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13. Magnetic order of tetragonal CuO ultra-thin films
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Hernandez, N. Ortiz, Salman, Z., Prokscha, T., Suter, A., Mardegan, J. R. L., Moser, S., Zakharova, A., Piamonteze, C., and Staub, und U.
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Condensed Matter - Materials Science - Abstract
We present a detailed low-energy muon spin rotation and x-ray magnetic circular dichroism (XMCD) investigation of the magnetic structure in ultra-thin tetragonal (T)-CuO films. The measured muon-spin polarization decay indicates an antiferromagnetic (AFM) order with a transition temperature higher than 200K. The XMCD signal obtained around the Cu $L_{2,3}$ edges indicates the presence of pinned Cu$^{2+}$ moments that are parallel to the sample surface, and additionally, isotropic paramagnetic moments. The pinning of some of the Cu moments is caused by an AFM ordering consisting of moments that lie most likely in the plane of the film. Moreover, pinned moments show a larger orbital magnetic moment contribution with an approximate ratio of $m_{orb}/m_{spin} = 2$, indicating that these spins are located at sites with reduced symmetry. Some fractions of the pinned moments remain pinned from an AFM background even at 360K, indicating that $T_N >$ 360K. A simple model could explain qualitatively these experimental findings; however, it is in contrast to theoretical predictions, showing that the magnetic properties of ultra-thin T-CuO films differ from bulk expectations and is more complex., Comment: 11 Figures
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- 2021
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14. The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy
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Scandariato, G., Borsa, F., Sicilia, D., Malavolta, L., Biazzo, K., Bonomo, A. S., Bruno, G., Claudi, R., Covino, E., Di Marcantonio, P., Esposito, M., Frustagli, G., Lanza, A. F., Maldonado, J., Maggio, A., Mancini, L., Micela, G., Nardiello, D., Rainer, M., Singh, V., Sozzetti, A., Affer, L., Benatti, S., Bignamini, A., Biliotti, V., Capuzzo-Dolcetta, R., Carleo, I., Cosentino, R., Damasso, M., Desidera, S., de Gurtubai, A. Garcia, Ghedina, A., Giacobbe, P., Giani, E., Harutyunyan, A., Hernandez, N., Diaz, M. Hernandez, Knapic, C., Leto, G., Fiorenzano, A. F. Martìnez, Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Poretti, E., and Stoev, H.
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Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
The analysis of exoplanetary atmospheres by means of high-resolution spectroscopy is an expanding research field which provides information on chemical composition, thermal structure, atmospheric dynamics and orbital velocity of exoplanets. In this work, we aim at the detection of the light reflected by the exoplanet 51~Peg~b employing optical high-resolution spectroscopy. To detect the light reflected by the planetary dayside we use optical HARPS and HARPS-N spectra taken near the superior conjunction of the planet, when the flux contrast between the planet and the star is maximum. To search for the weak planetary signal, we cross-correlate the observed spectra with a high S/N stellar spectrum. We homogeneously analyze the available datasets and derive a $10^{-5}$ upper limit on the planet-to-star flux contrast in the optical. The upper limit on the planet-to-star flux contrast of $10^{-5}$ translates into a low albedo of the planetary atmosphere ($\rm A_g\lesssim0.05-0.15$ for an assumed planetary radius in the range $\rm 1.5-0.9~R_{Jup}$, as estimated from the planet's mass).
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- 2020
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15. Analysis of magnetic polarities in active regions for the prediction of solar flares
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Hernández, N. Granados and Domínguez, S. Vargas
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Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
Solar active regions and the processes that occur in them have been extensively studied and analyzed and many types of models and characterizations have been proposed for the occurrence of different eruptive events that take place in the solar atmosphere. The most characteristic of these regions are those that have opposite magnetic polarity, which, in their majority, generate explosive events such as the so-called solar flares. The flares are intense explosions occurring in the solar atmosphere with adverse effects on the Earth and the technology developed by humans, and they are also determining factors in the so-called space weather. For this reason, attempts have been made to predict the occurrence of these events. In the present study, we developed a predictive model of solar flares higher than M5 based on the articles proposed by Korsos, et al. (2014, 2015) using the relationship between the flares and the bipolar active regions. The analysis took into account the areas of the umbrae of opposite polarity, their average magnetic field, and the magnetic barycenter from each sunspot in the region for a sample of three active regions to find the temporal variation due to the evolution of the sunspots, thus confirming previous results reported in the literature. We made a statistical analysis to determine whether after a flare occurs, another can arise in the subsequent hours., Comment: 12 pages, 7 figures, 7 tables (in spanish)
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- 2020
16. Magnetic field dependent cycloidal rotation in pristine and Ge doped CoCr$_2$O$_4$
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Hernandez, N Ortiz, Parchenko, S, Mardegan, J R L, Porer, M, Schierle, E, Weschke, E, Ramakrishnan, M, Radovic, M, Heuver, J A, Noheda, B, Daffe, N, Dreiser, J, Ueda, H., and Staub, U
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Condensed Matter - Strongly Correlated Electrons - Abstract
We report a soft x-ray resonant magnetic scattering study of the spin configuration in multiferroic thin films of Co$_{0.975}$Ge$_{0.025}$Cr$_2$O$_4$ (Ge-CCO) and CoCr$_2$O$_4$ (CCO), under low- and high-magnetic fields, from 0.2 T up to 6.5 T. A characterization of Ge-CCO at a low magnetic field is performed and the results are compared to those of pure CCO. The ferrimagnetic phase transition temperature $T_C \approx 95$ K and the multiferroic transition temperature $T_S \approx 27$ K in Ge-CCO are comparable to those observed in CCO. In Ge-CCO, the ordering wave vector $\textit{(qq0)}$ observed below $T_S$ is slightly larger compared to that of CCO, and, unlike CCO, the diffraction intensity consists of two contributions that show a dissimilar x-ray polarization dependence. In Ge-CCO, the coercive field observed at low temperatures was larger than the one reported for CCO. In both compounds, an unexpected reversal of the spiral helicity and therefore the electric polarization was observed on simply magnetic field cooling. In addition, we find a change in the helicity as a function of momentum transfer in the magnetic diffraction peak of Ge-CCO, indicative of the presence of multiple magnetic spirals., Comment: 20 pages, 12 figures
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- 2020
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17. The GAPS programme at TNG XXII. The GIARPS view of the extended helium atmosphere of HD189733 b accounting for stellar activity
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Guilluy, G., Andretta, V., Borsa, F., Giacobbe, P., Sozzetti, A., Covino, E., Bourrier, V., Fossati, L., Bonomo, A. S., Esposito, M., Giampapa, M. S., Harutyunyan, A., Rainer, M., Brogi, M., Bruno, G., Claudi, R., Frustagli, G., Lanza, A. F., Mancini, L., Pino, L., Poretti, E., Scandariato, G., Affer, L., Baffa, C., Baruffolo, A., Benatti, S., Biazzo, K., Bignamini, A., Boschin, W., Carleo, I., Cecconi, M., Cosentino, R., Damasso, M., Desidera, M., Falcini, G., Fiorenzano, A. F. Martinez, Ghedina, A., González-Álvarez, E., Guerra, J., Hernandez, N., Leto, G., Maggio, A., Malavolta, L., Maldonado, J., Micela, G., Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., and Reiners, A.
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Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Exoplanets orbiting very close to their host star are strongly irradiated. This can lead the upper atmospheric layers to expand and evaporate into space. The metastable helium (HeI) triplet at 1083.3nm has recently been shown to be a powerful diagnostic to probe extended and escaping exoplanetary atmosphere. We perform high-resolution transmission spectroscopy of the transiting hot Jupiter HD189733b with the GIARPS (GIANO-B + HARPS-N) observing mode of the Telescopio Nazionale Galileo, taking advantage of the simultaneous optical+near infrared spectral coverage to detect HeI in the planet's extended atmosphere and to gauge the impact of stellar magnetic activity on the planetary absorption signal. Observations were performed during five transit events of HD189733b. By comparison of the in- and out-of-transit GIANO-B observations we compute high-resolution transmission spectra, on which we perform equivalent width measurements and light-curves analyses to gauge the excess in-transit absorption in the HeI triplet. We detect an absorption signal during all five transits. The mean in-transit absorption depth amounts to 0.75+/-0.03%. We detect night-to-night variations in the HeI absorption signal likely due to the transit events occurring in presence of stellar surface inhomogeneities. We evaluate the impact of stellar-activity pseudo-signals on the true planetary absorption using a comparative analysis of the HeI and the H$\alpha$ lines. We interpret the time-series of the HeI absorption lines in the three nights not affected by stellar contamination -exhibiting a mean in-transit absorption depth of 0.77+/-0.04%- using a 3-d atmospheric code. Our simulations suggest that the helium layers only fill part of the Roche lobe. Observations can be explained with a thermosphere heated to $\sim$12000 K, expanding up to $\sim$1.2 planetary radii, and losing $\sim$1 g/s of metastable helium., Comment: 17 pages, 17 figures, accepted for publication in A&A
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- 2020
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18. Linear energy transfer (LET) distribution outside small radiotherapy field edges produced by 6 MV X-rays
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Huerta-Juan, Y., Xicohténcatl-Hernández, N., and Massillon-JL, G.
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- 2023
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19. Liver injury due to COVID-19 in critically ill adult patients. A retrospective study
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Alva, N.V., Méndez, O.R., Gasca, J.C., Salvador, I., Hernández, N., and Valdez, M.
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- 2024
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20. Evaluation of the incorporation of an IOTA-ADNEX model in the discrimination of adnexal masses in our third-level hospital centre, taking into account the menopausal status of patients. Five years of experience
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Elsner Hernández, N., De Luis Escudero, J.F., Pérez Méndez, L.I., Báez Quintana, D.R., Bruno Santana, E., Pérez Álvarez, J.A., Sierra Medina, N.R., Chulilla Pérez, C., and Quesada López-Fe, A.
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- 2024
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21. Magnetic order of tetragonal CuO ultrathin films
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Ortiz Hernández, N, Salman, Z, Prokscha, T, Suter, A, Mardegan, JRL, Moser, S, Zakharova, A, Piamonteze, C, and Staub, U
- Published
- 2021
22. Magnetic order of tetragonal CuO ultrathin films
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Hernández, N Ortiz, Salman, Z, Prokscha, T, Suter, A, Mardegan, JRL, Moser, S, Zakharova, A, Piamonteze, C, and Staub, U
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Physical Sciences ,Chemical Sciences ,Engineering ,Fluids & Plasmas - Published
- 2021
23. The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: confirmation of HD 285507 b and refutation of AD Leo b
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Carleo, I., Malavolta, L., Lanza, A. F., Damasso, M., Desidera, S., Borsa, F., Mallonn, M., Pinamonti, M., Gratton, R., Alei, E., Benatti, S., Mancini, L., Maldonado, J., Biazzo, K., Esposito, M., Frustagli, G., González-Álvarez, E., Micela, G., Scandariato, G., Sozzetti, A., Affer, L., Bignamini, A., Bonomo, A. S., Claudi, R., Cosentino, R., Covino, E., Fiorenzano, A. F. M., Giacobbe, P., Harutyunyan, A., Leto, G., Maggio, A., Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Poretti, E., Rainer, M., Redfield, S., Baffa, C., Baruffolo, A., Buchschacher, N., Billotti, V., Cecconi, M., Falcini, G., Fantinel, D., Fini, L., Galli, A., Ghedina, A., Ghinassi, F., Giani, E., Gonzalez, C., Gonzalez, M., Guerra, J., Diaz, M. Hernandez, Hernandez, N., Iuzzolino, M., Lodi, M., Oliva, E., Origlia, L., Ventura, H. Perez, Puglisi, A., Riverol, C., Riverol, L., Juan, J. San, Sanna, N., Scuderi, S., Seemann, U., Sozzi, M., and Tozzi, A.
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Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the proto-planetary disk or the circularization of an initial high eccentric orbit by tidal dissipation leading to a strong decrease of the semimajor axis. Different formation scenarios result in different observable effects, such as orbital parameters (obliquity/eccentricity), or frequency of planets at different stellar ages. In the context of the GAPS Young-Objects project, we are carrying out a radial velocity survey with the aim to search and characterize young hot-Jupiter planets. Our purpose is to put constraints on evolutionary models and establish statistical properties, such as the frequency of these planets from a homogeneous sample. Since young stars are in general magnetically very active, we performed multi-band (visible and near-infrared) spectroscopy with simultaneous GIANO-B + HARPS-N (GIARPS) observing mode at TNG. This helps to deal with stellar activity and distinguish the nature of radial velocity variations: stellar activity will introduce a wavelength-dependent radial velocity amplitude, whereas a Keplerian signal is achromatic. As a pilot study, we present here the cases of two already claimed hot Jupiters orbiting young stars: HD285507 b and AD Leo b. Our analysis of simultaneous high-precision GIARPS spectroscopic data confirms the Keplerian nature of HD285507's radial velocities variation and refines the orbital parameters of the hot Jupiter, obtaining an eccentricity consistent with a circular orbit. On the other hand, our analysis does not confirm the signal previously attributed to a planet orbiting AD Leo. This demonstrates the power of the multi-band spectroscopic technique when observing active stars.
- Published
- 2020
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24. Temporal evolution and correlations of optical activity indicators measured in Sun-as-a-star observations
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Maldonado, J., Phillips, D. F., Dumusque, X., Cameron, A. Collier, Haywood, R. D., Lanza, A. F., Micela, G., Mortier, A., Saar, S. H., Sozzetti, A., Rice, K., Milbourne, T., Cecconi, M., Cegla, H. M., Cosentino, R., Costes, J., Ghedina, A., Gonzalez, M., Guerra, J., Hernández, N., Li, C. -H., Lodi, M., Malavolta, L., Molinari, E., Pepe, F., Piotto, G., Poretti, E., Sasselov, D., Juan, J. San, Thompson, S., Udry, S., and Watson, C.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
(Abridged) We perform a detailed study of the main optical activity indicators (Ca II H & K, Balmer lines, Na I D$_{\rm 1}$ D$_{\rm 2}$, and He I D$_{\rm 3}$) measured for the Sun using the data provided by the HARPS-N solar-telescope feed at the Telescopio Nazionale Galileo. The value of the solar rotation period is found in all the activity indicators, with the only exception being H$\delta$. The derived values vary from 26.29 days (H$\gamma$ line) to 31.23 days (He I). From an analysis of sliding periodograms we find that in most of the activity indicators the spectral power is split into several "bands" of periods around 26 and 30 days, that might be explained by the migration of active regions between the equator and a latitude of $\sim$ 30$^{\circ}$, spot evolution or a combination of both effects. In agreement with previous works a typical lifetime of active regions of $\sim$ ten rotation periods is inferred from the pooled variance diagrams. We find that H$\alpha$, H$\beta$, H$\gamma$, H$\epsilon$, and He I show a significant correlation with the S index. Significant correlations between the contrast, bisector span, and the heliocentric radial velocity with the activity indexes are also found. We show that the full width at half maximum, the bisector, and the disc-integrated magnetic field correlate with the radial velocity variations. The correlation of the S index and H$\alpha$ changes with time, increasing with larger sun spot numbers and solar irradiance. A similar tendency with the S index - radial velocity correlation is also present in the data. Our results are consistent with a scenario in which higher activity favours the correlation between the S index and the H$\alpha$ activity indicators and between the S index and radial velocity variations., Comment: Accepted by Astronomy & Astrophysics
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- 2019
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25. Optical and electronic properties of a singly ionized double donor confined in coupled quantum dot-rings
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Hernández, N., López-Doria, R.A., and Fulla, M.R.
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- 2023
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26. [Artículo traducido] Sonidegib para el tratamiento del carcinoma basocelular avanzado en práctica clínica real: estudio nacional multicéntrico
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Moreno-Arrones, O.M., Béa-Ardebol, S., Mayo-Martinez, F., Pérez-Pastor, G., Torres-Navarro, I., Bonfill-Ortí, M., Deza, G., Ruiz-Salas, V., Masferrer, E., Feal, C., Turrión-Merino, L., Toll, A., Yébenes, M., Galiano-Mejías, S., Jaka, A., Ferrandiz-Pulido, C., Florez, A., Hernández-Hernández, N., Fernández-de-Misa, R., Rios-Buceta, L., and Sanmartin, O.
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- 2023
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27. Sonidegib as a Locally Advanced Basal Cell Carcinoma Therapy in Real-life Clinical Setting: A National Multicentre Study
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Moreno-Arrones, O.M., Béa-Ardebol, S., Mayo-Martinez, F., Pérez-Pastor, G., Torres-Navarro, I., Bonfill-Ortí, M., Deza, G., Ruiz-Salas, V., Masferrer, E., Feal, C., Turrión-Merino, L., Toll, A., Yébenes, M., Galiano-Mejías, S., Jaka, A., Ferrandiz-Pulido, C., Florez, A., Hernández-Hernández, N., Fernández-de-Misa, R., Rios-Buceta, L., and Sanmartin, O.
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- 2023
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28. Magnetic and electronic properties at the gamma-Al2O3/SrTiO3 interface
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Mardegan, J. R. L., Christensen, D. V., Chen, Y. Z., Parchenko, S., Avula, S. R. V., Ortiz-Hernandez, N., Decker, M., Piamonteze, C., Pryds, N., and Staub, U.
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Condensed Matter - Strongly Correlated Electrons - Abstract
The magnetic and electronic nature of the gamma-Al2O3/SrTiO3 spinel/perovskite interface is explored by means of x-ray absorption spectroscopy. Polarized x-ray techniques combined with atomic multiplet calculations reveal localized magnetic moments assigned to Ti3+ at the interface with equivalent size for in- and out-of-plane magnetic field directions. Although magnetic fingerprints are revealed, the Ti3+ magnetism can be explained by a paramagnetic response at low temperature under applied magnetic fields. Modeling the x-ray linear dichroism results in a delta0 = 1.9 eV splitting between the t2g and eg states for the Ti4+ 3d0 orbitals. In addition these results indicate that the lowest energy states have the out-of-plane dxz/dyz symmetry. The isotropic magnetic moment behavior and the lowest energy dxz/dyz states are in contrast to the observations for the two-dimensional electron gas at the perovskite/perovskite interface of LaAlO3/SrTiO3, that exhibits an anisotropic magnetic dxy ground state., Comment: 6 pages, 5 figures
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- 2019
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29. Intelligent Fuzzy Clinical Decision Support System to Predict the Coimbra Breast Cancer Dataset
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Hernández-Julio, Y. F., Muñoz-Hernández, H., Díaz-Pertuz, L. A., Prieto-Guevara, M., Arrieta-Hernández, N. S., Figueroa-Mendoza, N. A., Aviles-Román, M., Nieto-Bernal, W., Kacprzyk, Janusz, Series Editor, Gomide, Fernando, Advisory Editor, Kaynak, Okyay, Advisory Editor, Liu, Derong, Advisory Editor, Pedrycz, Witold, Advisory Editor, Polycarpou, Marios M., Advisory Editor, Rudas, Imre J., Advisory Editor, Wang, Jun, Advisory Editor, Kahraman, Cengiz, editor, Tolga, A. Cagri, editor, Cevik Onar, Sezi, editor, Cebi, Selcuk, editor, Oztaysi, Basar, editor, and Sari, Irem Ucal, editor
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- 2022
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30. Métodos anticonceptivos de larga duración (LARC): características de las usuarias, tasa de continuidad y efectividad
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Martínez Pérez, A., Terrón Barroso, J., Alayón Hernández, N., and Ariza Chana, N.E.
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- 2023
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31. GIARPS: commissioning and first scientific results
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Claudi, R., Benatti, S., Carleo, I., Ghedina, A., Guerra, J., Ghinassi, F., Harutyunyan, A., Micela, G., Molinari, E., Oliva, E., Rainer, M., Tozzi, A., Baffa, C., Baruffolo, A., Biliotti, V., Buchschacher, N., Cecconi, M., Cosentino, R., Falcini, G., Fantinel, D., Fini, L., Giani, E., Gonzalez--Alvarez, E., Gonzalez, M., Gonzalez, C., Gratton, R., Hernandez, N., Iuzzolino, M., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Puglisi, A., Sanna, N., Juan, J. San, Scuderi, S., Seemann, U., Sozzetti, A., Sozzi, M., Ventura, H. Perez, Diaz, M. Hernandez, Galli, A., Riverol, L., and Riverol, C.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
GIARPS (GIAno \& haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both high resolution spectrographs, HARPS-N (VIS) and GIANO-B (NIR), working simultaneously. This could be considered the first and unique worldwide instrument providing cross-dispersed echelle spectroscopy at a resolution of 50,000 in the NIR range and 115,000 in the VIS and over in a wide spectral range ($0.383 - 2.45\ \mu$m) in a single exposure. The science case is very broad, given the versatility of such an instrument and its large wavelength range. A number of outstanding science cases encompassing mainly extra-solar planet science starting from rocky planets search and hot Jupiters to atmosphere characterization can be considered. Furthermore both instruments can measure high precision radial velocities by means the simultaneous thorium technique (HARPS-N) and absorbing cell technique (GIANO-B) in a single exposure. Other science cases are also possible. GIARPS, as a brand new observing mode of the TNG started after the moving of GIANO-A (fiber fed spectrograph) from Nasmyth-A to Nasmyth-B where it was re-born as GIANO-B (no more fiber feed spectrograph). The official Commissioning finished on March 2017 and then it was offered to the community. Despite the work is not finished yet. In this paper we describe the preliminary scientific results obtained with GIANO-B and GIARPS observing mode with data taken during commissioning and first open time observations., Comment: 10 pages, 11 figures, Telescopes and Astronomical instrumentation, SPIE Conf. 2018
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- 2018
32. Multi-band high resolution spectroscopy rules out the hot Jupiter BD+20 1790b - First data from the GIARPS Commissioning
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Carleo, I., Benatti, S., Lanza, A. F., Gratton, R., Claudi, R., Desidera, S., Mace, G. N., Messina, S., Sanna, N., Sissa, E., Ghedina, A., Ghinassi, F., Guerra, J., Harutyunyan, A., Micela, G., Molinari, E., Oliva, E., Tozzi, A., Baffa, C., Baruffolo, A., Bignamini, A., Buchschacher, N., Cecconi, M., Cosentino, R., Endl, M., Falcini, G., Fantinel, D., Fini, L., Fugazza, D., Galli, A., Giani, E., González, C., González-Álvarez, E., González, M., Hernandez, N., Diaz, M. Hernandez, Iuzzolino, M., Kaplan, K. F., Kidder, B. T., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Ventura, H. Perez, Puglisi, A., Rainer, M., Riverol, L., Riverol, C., Juan, J. San, Scuderi, S., Seemann, U., Sokal, K. R., Sozzetti, A., and Sozzi, M.
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Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature of the RV variations for the young active K5 star BD+20 1790, for which visible (VIS) RV measurements show divergent results on the existence of a substellar companion. Methods. We compare VIS data with high precision RVs in the near infrared (NIR) range by using the GIANO - B and IGRINS spectrographs. In addition, we present for the first time simultaneous VIS-NIR observations obtained with GIARPS (GIANO - B and HARPS - N) at Telescopio Nazionale Galileo (TNG). Orbital RVs are achromatic, so the RV amplitude does not change at different wavelengths, while stellar activity induces wavelength-dependent RV variations, which are significantly reduced in the NIR range with respect to the VIS. Results. The NIR radial velocity measurements from GIANO - B and IGRINS show an average amplitude of about one quarter with respect to previously published VIS data, as expected when the RV jitter is due to stellar activity. Coeval multi-band photometry surprisingly shows larger amplitudes in the NIR range, explainable with a mixture of cool and hot spots in the same active region. Conclusions. In this work, the claimed massive planet around BD+20 1790 is ruled out by our data. We exploited the crucial role of multi- wavelength spectroscopy when observing young active stars: thanks to facilities like GIARPS that provide simultaneous observations, this method can reach its maximum potential., Comment: 12 pages, 7 figures
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- 2018
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33. GIARPS@TNG GIANO-B & HARPS-N together for a wider wavelength range spectroscopy
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Claudi, R., Benatti, S., Carleo, I., Ghedina, A., Guerra, J., Micela, G., Molinari, E., Oliva, E., Rainer, M., Tozzi, A., Baffa, C., Baruffolo, A., Buchschacher, N., Cecconi, M., Cosentino, R., Fantinel, D., Fini, L., Ghinassi, F., Giani, E., Gonzalez, E., Gonzalez, M., Gratton, R., Harutyunyan, A., Hernandez, N., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Sanna, N., Sanjuan, J., Scuderi, S., Seemann, U., Sozzetti, A., Ventura, H. Perez, Diaz, M. Hernandez, Galli, A., Gonzalez, C., Riverol, L., and Riverol, C.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
Since 2012, thanks to the installation of the high resolution echelle spectrograph in the optical range HARPS-N, the Italian telescope TNG (La Palma) became one of the key facilities for the study of the extrasolar planets. In 2014 TNG also offered GIANO to the scientific community, providing a near-infrared (NIR) cross-dispersed echelle spectroscopy covering 0.97 - 2.45 micron at a resolution of 50,000. GIANO, although designed for direct light-feed from the telescope at the Nasmyth-B focus, was provisionally mounted on the rotating building and connected via fibers to only available interface at the Nasmyth-A focal plane. The synergy between these two instruments is particularly appealing for a wide range of science cases, especially for the search for exoplanets around young and active stars and the characterisation of their atmosphere. Through the funding scheme "WOW" (a Way to Others Worlds), the Italian National Institute for Astrophysics (INAF) proposed to position GIANO at the focal station for which it was originally designed and the simultaneous use of these spectrographs with the aim to achieve high-resolution spectroscopy in a wide wavelength range (0.383-2.45 micron) obtained in a single exposure, giving rise to the project called GIARPS (GIANO-B & HARPS-N). Because of its characteristics GIARPS can be considered the first and unique worldwide instrument providing not only high resolution in a large wavelength band, but also a high precision radial velocity measurement both in the visible and in the NIR arm, since in the next future GIANO-B will be equipped with gas absorption cells., Comment: EPJP - Focus Point on Highlights on Planetary Sciences in Italy
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- 2017
34. Refractive index change of a D2+ complex in GaAs/AlxGa1−xAs quantum ring
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Hernández, N., López-Doria, R. A., Rivera, I. E., and Fulla, M. R.
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- 2022
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35. Design of multilayer hybrid sol-gel coatings with bifunctional barrier-bioactive response on the Elektron 21 magnesium alloy for biomedical applications
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Durán, K.S., Hernández, N., Rueda, L.M., Hernández-Barrios, C.A., Coy, A.E., and Viejo, F.
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- 2021
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36. Optical absorption computation of a [formula omitted] artificial molecule in GaAs/Ga[formula omitted]Al[formula omitted]As nanometer-scale rings
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Hernández, N., López, R., Álvarez, J.A., Marín, J.H., Fulla, M.R., and Tobón, H.
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- 2021
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37. One-year prognosis of non-traumatic cortical subarachnoid haemorrhage: a prospective series of 34 patients
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Galiano Blancart, R.F., Fortea, G., Pampliega Pérez, A., Martí, S., Parkhutik, V., Sánchez Cruz, A.V., Soriano, C., Geffner Sclarsky, D., Pérez Saldaña, M.T., López Hernández, N., Beltrán, I., and Lago Martín, A.
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- 2021
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38. Pronóstico al año de la hemorragia subaracnoidea cortical no traumática: Serie prospectiva de 34 pacientes
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Galiano Blancart, R.F., Fortea, G., Pampliega Pérez, A., Martí, S., Parkhutik, V., Sánchez Cruz, A.V., Soriano, C., Geffner Sclarsky, D., Pérez Saldaña, M.T., López Hernández, N., Beltrán, I., and Lago Martín, A.
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- 2021
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39. Spinogenesis in spinal cord motor neurons following pharmacological lesions to the rat motor cortex
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Martínez-Torres, N.I., González-Tapia, D., Flores-Soto, M., Vázquez-Hernández, N., Salgado-Ceballos, H., and González-Burgos, I.
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- 2021
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40. Espinogénesis en motoneuronas de la médula espinal tras la lesión farmacológica de la corteza motora de ratas
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Martínez-Torres, N.I., González-Tapia, D., Flores-Soto, M., Vázquez-Hernández, N., Salgado-Ceballos, H., and González-Burgos, I.
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- 2021
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41. Plastic changes to dendritic spines in the cerebellar and prefrontal cortices underlie the decline in motor coordination and working memory during successful aging
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Vázquez-Hernández, N., Martínez-Torres, N.I., and González-Burgos, I.
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- 2021
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42. Risk profiles and one-year outcomes of patients with newly diagnosed atrial fibrillation in India: Insights from the GARFIELD-AF Registry
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Kakkar, Ajay K., Bassand, Jean-Pierre, John Camm, A., Fitzmaurice, David A., Goldhaber, Samuel Z., Goto, Shinya, Haas, Sylvia, Hacke, Werner, Mantovani, Lorenzo G., Misselwitz, Frank, Pieper, Karen S., Turpie, Alexander G.G., van Eickels, Martin, Verheugt, Freek W.A., Kayani, Gloria, Fox, Keith A.A., Gersh, Bernard J., Luciardi, Hector Lucas, Gibbs, Harry, Brodmann, Marianne, Cools, Frank, Barretto, Antonio Carlos Pereira, Connolly, Stuart J., Spyropoulos, Alex, Eikelboom, John, Corbalan, Ramon, Hu, Dayi, Jansky, Petr, Nielsen, Jørn Dalsgaard, Ragy, Hany, Raatikainen, Pekka, Le Heuzey, Jean-Yves, Darius, Harald, Keltai, Matyas, Kakkar, Sanjay, Sawhney, Jitendra Pal Singh, Agnelli, Giancarlo, Ambrosio, Giuseppe, Koretsune, Yukihiro, Sánchez Díaz, Carlos Jerjes, Ten Cate, Hugo, Atar, Dan, Stepinska, Janina, Panchenko, Elizaveta, Lim, Toon Wei, Jacobson, Barry, Oh, Seil, Viñolas, Xavier, Rosenqvist, Marten, Steffel, Jan, Angchaisuksiri, Pantep, Oto, Ali, Parkhomenko, Alex, Al Mahmeed, Wael, Fitzmaurice, David, Hu, D.Y., Chen, K.N., Zhao, Y.S., Zhang, H.Q., Chen, J.Z., Cao, S.P., Wang, D.W., Yang, Y.J., Li, W.H., Yin, Y.H., Tao, G.Z., Yang, P., Chen, Y.M., He, S.H., Wang, Ying, Wang, Yong, Fu, G.S., Li, X., Wu, T.G., Cheng, X.S., Yan, X.W., Zhao, R.P., Chen, M.S., Xiong, L.G., Chen, P., Jiao, Y., Guo, Y., Xue, L., Wang, F.Z., Li, H., Yang, Z.M., Bai, C.L., Chen, J., Chen, J.Y., Chen, X., Feng, S., Fu, Q.H., Gao, X.J., Guo, W.N., He, R.H., He, X.A., Hu, X.S., Huang, X.F., Li, B., Li, J., Li, L., Li, Y.H., Liu, T.T., Liu, W.L., Liu, Y.Y., Lu, Z.C., Luo, X.L., Ma, T.Y., Peng, J.Q., Sheng, X., Shi, X.J., Sun, Y.H., Tian, G., Wang, K., Wang, L., Wu, R.N., Xie, Q., Xu, R.Y., Yang, J.S., Yang, L.L., Yang, Q., Ye, Y., Yu, H.Y., Yu, J.H., Yu, T., Zhai, H., Zhan, Q., Zhang, G.S., Zhang, Q., Zhang, R., Zhang, Y., Zheng, W.Y., Zhou, B., Zhou, Z.H., Zhu, X.Y., Kakkar, S., Sawhney, J.P.S., Jadhav, P., Durgaprasad, R., Ravi Shankar, A.G., Rajput, R.K., Bhargava, K., Sarma, R., Srinivas, A., Roy, D., Nagamalesh, U.M., Chopda, M., Kishore, R., Kulkarni, G., Chandwani, P., Pothiwala, R.A., Padinhare Purayil, M., Shah, S., Chawla, K., Kothiwale, V.A., Raghuraman, B., Vijayaraghavan, G., Vijan, V.M., Bantwal, G., Bisne, V., Khan, A., Gupta, J.B., Kumar, S., Jain, D., Abraham, S., Adak, D., Barai, A., Begum, H., Bhattacharjee, P., Dargude, M., Davies, D., Deshpande, B., Dhakrao, P., Dhyani, V., Duhan, S., Earath, M., Ganatra, A., Giradkar, S., Jain, V., Karthikeyan, R., Kasala, L., Kaur, S., Krishnappa, S., Lawande, A., Lokesh, B., Madarkar, N., Meena, R., More, P., Naik, D., Prashanth, K., Rao, M., Rao, N.M., Sadhu, N., Shah, D., Sharma, M., Shiva, P., Singhal, S., Suresh, S., Vanajakshamma, V., Panse, S.G., Koretsune, Y., Kanamori, S., Yamamoto, K., Kumagai, K., Katsuda, Y., Sadamatsu, K., Toyota, F., Mizuno, Y., Misumi, I., Noguchi, H., Ando, S., Suetsugu, T., Minamoto, M., Oda, Hiroshi, Shiraishi, K., Adachi, S., Chiba, K., Norita, H., Tsuruta, M., Koyanagi, T., Ando, H., Higashi, T., Okada, K., Azakami, S., Komaki, S., Kumeda, K., Murayama, T., Matsumura, J., Oba, Y., Sonoda, R., Goto, K., Minoda, K., Haraguchi, Y., Suefuji, H., Miyagi, H., Kato, H., Nakamura, Tadashi, Nakamura, Tsugihiro, Nandate, H., Zaitsu, R., Fujiura, Yoshihisa, Yoshimura, A., Numata, H., Ogawa, J., Tatematsu, H., Kamogawa, Y., Murakami, K., Wakasa, Y., Yamasawa, M., Maekawa, H., Abe, S., Kihara, H., Tsunoda, S., Saito, Katsumi, Saito, Kazuyuki, Fudo, T., Obunai, K., Tachibana, H., Oba, I., Kuwahata, T., Higa, S., Gushiken, M., Eto, T., Yoshida, H., Ikeda, D., Fujiura, Yoshitake, Ishizawa, M., Nakatsuka, M., Murata, K., Ogurusu, C., Shimoyama, M., Akutsu, M., Takamura, I., Hoshino, F., Yokota, N., Iwao, T., Tsuchida, K., Takeuchi, M., Hatori, Y., Kitami, Y., Nakamura, Yoichi, Oyama, R., Ageta, M., Oda, Hiroyuki, Go, Y., Mishima, K., Unoki, T., Morii, S., Shiga, Yuhei, Sumi, H., Nagatomo, T., Sanno, K., Fujisawa, K., Atsuchi, Y., Nagoshi, T., Seto, T., Tabuchi, T., Kameko, M., Nii, K., Oshiro, K., Takezawa, H., Nagano, S., Miyamoto, N., Iwaki, M., Nakamura, Yuichiro, Fujii, M., Okawa, M., Abe, Masahiko, Abe, Masatake, Abe, Mitsunori, Saito, T., Mito, T., Nagao, K., Minami, J., Mita, T., Sakuma, I., Taguchi, T., Marusaki, S., Doi, H., Tanaka, M., Fujito, T., Matsuta, M., Kusumoto, T., Kakinoki, S., Ashida, K., Yoshizawa, N., Agata, J., Arasaki, O., Manita, M., Ikemura, M., Fukuoka, S., Murakami, H., Matsukawa, S., Hata, Y., Taniguchi, T., Ko, T., Kubo, H., Imamaki, M., Akiyama, M., Inagaki, M., Odakura, H., Ueda, T., Katsube, Y., Nakata, A., Watanabe, H., Techigawara, M., Igarashi, M., Taga, K., Kimura, T., Tomimoto, S., Shibuya, M., Nakano, M., Ito, K., Seo, T., Hiramitsu, S., Hosokawa, H., Hoshiai, M., Hibino, M., Miyagawa, K., Horie, Hajime, Sugishita, N., Shiga, Yukio, Soma, A., Neya, K., Yoshida, Tetsuro, Yoshida, Tomoki, Mizuguchi, M., Ishiguro, M., Minagawa, T., Wada, M., Mukawa, H., Okuda, F., Nagasaka, S., Abe, Y., Adachi, Sen, Adachi, Susumu, Adachi, T., Akahane, K., Amano, T., Aoki, K., Aoyama, T., Arai, H., Arima, S., Arino, T., Asano, H., Asano, T., Azuma, J., Baba, T., Betsuyaku, T., Chibana, H., Date, H., Doiuchi, J., Emura, Y., Endo, M., Fujii, Y., Fujiki, R., Fujisawa, A., Fujisawa, Y., Fukuda, T., Fukui, T., Furukawa, N., Furukawa, T., Furumoto, W., Goto, T., Hamaoka, M., Hanazono, N., Hasegawa, K., Hatsuno, T., Hayashi, Y., Higuchi, K., Hirasawa, K., Hirayama, H., Hirose, M., Hirota, S., Honda, M., Horie, Hideki, Ido, T., Iiji, O., Ikeda, H., Ikeda, K., Ikeoka, K., Imaizumi, M., Inaba, H., Inoue, T., Iseki, F., Ishihara, A., Ishioka, N., Ito, N., Iwase, T., Kakuda, H., Kamata, J., Kanai, H., Kanda, H., Kaneko, M., Kano, H., Kasai, T., Kato, T., Kato, Y., Kawada, Y., Kawai, K., Kawakami, K., Kawakami, S., Kawamoto, T., Kawano, S., Kim, J., Kira, T., Kitazawa, H., Kitazumi, H., Kito, T., Kobayashi, T., Koeda, T., Kojima, J., Komatsu, H., Komatsu, I., Koshibu, Y., Kotani, T., Kozuka, T., Kumai, Y., Kumazaki, T., Maeda, I., Maeda, K., Maruyama, Y., Matsui, S., Matsushita, K., Matsuura, Y., Mineoi, K., Mitsuhashi, H., Miura, N., Miyaguchi, S., Miyajima, S., Miyamoto, H., Miyashita, A., Miyata, S., Mizuguchi, I., Mizuno, A., Mori, T., Moriai, O., Morishita, K., Murai, O., Nagai, Sho, Nagai, Shunichi, Nagata, E., Nagata, H., Nakagomi, A., Nakahara, S., Nakamura, M., Nakamura, R., Nakanishi, N., Nakayama, T., Nakazato, R., Nanke, T., Nariyama, J., Niijima, Y., Niinuma, H., Nishida, Y., Nishihata, Y., Nishino, K., Nishioka, H., Nishizawa, K., Niwa, I., Nomura, K., Nomura, S., Nozoe, M., Ogawa, T., Ohara, N., Okada, M., Okamoto, K., Okita, H., Okuyama, M., Ono, H., Ono, T., Onuki Pearce, Y., Oriso, S., Ota, A., Otaki, E., Saito, Y., Sakai, H., Sakamoto, N., Sakamoto, Y., Samejima, Y., Sasagawa, Y., Sasaguri, H., Sasaki, A., Sasaki, T., Sato, Kazuki, Sato, Kiyoharu, Sawano, M., Seki, S., Sekine, Y., Seta, Y., Sezaki, K., Shibata, N., Shiina, Y., Shimono, H., Shimoyama, Y., Shindo, T., Shinohara, 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K., Hines, C., Hines, K., Jackson, A.M., Jean, C., Jethoo, G., Kahlon, R., Kelly, S., Kim, R., Korley, V., Kornder, J., Kwan, L., Largy, J., Lewis, C., Lewis, S., Mangat, I., Moor, R., Navratil, J., Neas, I., Otis, J., Otis, R., Pandey, M., Petrie, F., Pinter, A., Raines, M., Roberts, P., Robinson, M., Sas, G., Schulman, S., Snell, L., Spearson, S., Stevenson, J., Trahey, T., Wong, S., Wright, D., Ragy, H., Abd El-Aziz, A., Abou Seif, S.K., El Din, M.G., El Etriby, S., Elbahry, A., El-Etreby, A., Elkhadem, M., Katta, A., Khairy, T., Mowafy, A., Nawar, M., Ohanissian, A., Reda, A., Reda, M., Salem, H., Sami, N., Samir, S., Setiha, M., Sobhy, M., Soliman, A., Taha, N., Tawfik, M., Zaatout, E., Kettles, D., Bayat, J., Siebert, H., Horak, A., Kelfkens, Y., Garda, R., Pillay, T., Guerra, M., van Zyl, L., Theron, H., Murray, A., Louw, R., Greyling, D., Mntla, P., Ueckermann, V., Loghdey, R., Ismail, S., Ahmed, F., Engelbrecht, J., Ramdass, A., Maharajh, S., Oosthuysen, W., Angel, G., Bester, C., Booysen, M., Boshoff, C., Cannon, C., Cassimjee, S., Chami, C., Conway, G., Davids, A., de Meyer, L., Du Plessis, G., Ellis, T., Henley, L., Karsten, M., Loyd, E., Marks, J., Mavhusa, L., Mostert, M., Page, A., Rikhotso, L., Salie, M., Sasto, J., Shaik, F., Skein, A., Smith, L., Tarr, G., Tau, T., van Zyl, F., Al Mahmeed, W., Yousef, G., Agrawal, A., Nathani, M., Ibrahim, M., Esheiba, E.M., Singh, R., Naguib, A., Abu-Mahfouz, M., Al Omairi, M., Al Naeemi, A., Maruthanayagam, R., Bazargani, N., Wassef, A., Gupta, R., Khan, M., Subbaraman, B., Abdul, A., Al Mulla, A., El Bardisy, S., Haridas, P., Jadhav, S., Magdaluyo, K., Makdad, M., Maqsood, I., Mohamed, R., Sharma, N., Sharma, R., Thanzeel, M., Goldhaber, S.Z., Canosa, R., Rama, P., Blumberg, E., Garcia, J., Mullen, P., Wilson, V., Quick, A., Ferrick, K., Kutayli, W.M., Cox, M., Franco, M., Falkowski, S., Mendelson, R., Williams, M., Miller, S., Beach, S., Alfieri, A., Gutowski, T., Haque, I., Reddy, R., Ahmed, W., Delafontaine, P., Diercks, D., Theodoro, D., Remmel, K., Alberts, M., Ison, R., Noveck, H., Duffy, P., Pitta, S., Nishijima, D., Treasure, C., Asafu-Adjaye, N., Ball, K., Bartlett, M., Bentley, M., Bowers, S., Brown, A., Browne, A., Cameron-Watts, J., Canova, M., Cassidy, D., Cervellione, K., Congal, S., DePauw, J., Dickerson, A., Eley, M., Evans, L., Felpel, S., Ferdinand, K., Fielder, D., Gentry, P., Haideri, A., Hakimi, F., Harbour, T., Hartranft, E., Hawkins, B., Headlee, M., Henson, L., Herrick, C., Hicks, T., Jasinski, S., Jones, A., Jones, L., Jones, P., Karl, S., Keeling, M., Kerr, J., Knowles, P., Langdon, J., Lay, M., Lee, J.A., Lincoln, T., Malone, E., Merliss, A., Merritt, D., Minardo, J., Mooso, B., Orosco, C., Palumbo, V., Parker, M., Parrott, T., Paserchia, S., Pearl, G., Peterson, J., Pickelsimer, N., Purcell, T., Raynor, J., Raziano, S., Richard, C., Richardson, T., Robertson, C., Sage, A., Sanghera, T., Shaw, P., Shoemaker, J., Smith, K., Stephanie, B., Thatcher, A., Theobald, H., Thompson, N., Treasure, L., Tripti, T., Verdi, C., Worthy, V., Sawhney, Jitendra PS., Kothiwale, Veerappa A., Bisne, Vikas, Durgaprasad, Rajashekhar, Jadhav, Praveen, Chopda, Manoj, Vanajakshamma, Velam, Meena, Ramdhan, Vijayaraghavan, Govindan, Chawla, Kamaldeep, and Allu, Jagan
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- 2018
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43. CNNs for Fine-Grained Car Model Classification
- Author
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Corrales, H., Llorca, D. F., Parra, I., Vigre, S., Quintanar, A., Lorenzo, J., Hernández, N., Goos, Gerhard, Founding Editor, Hartmanis, Juris, Founding Editor, Bertino, Elisa, Editorial Board Member, Gao, Wen, Editorial Board Member, Steffen, Bernhard, Editorial Board Member, Woeginger, Gerhard, Editorial Board Member, Yung, Moti, Editorial Board Member, Moreno-Díaz, Roberto, editor, Pichler, Franz, editor, and Quesada-Arencibia, Alexis, editor
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- 2020
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44. Pasting and viscoelastic properties of starches isolated from tropical fruits.
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Martínez-Ortiz, M. A., Balois-Morales, R., Bello-Lara, J. E., Chavarría-Hernández, N., and Rodríguez-Hernández, A. I.
- Subjects
TROPICAL fruit ,RHEOLOGY ,BIOTECHNOLOGY ,AMYLOSE ,STARCH ,MANGO ,CORNSTARCH ,WHEAT starch - Abstract
The exploration of new starch sources has increased due to the demand to develop green materials. In this sense, diverse polysaccharides, including starch, can be isolated from fruits due to their significant postharvest loss in many countries with vast fruit biodiversity. The present work examined the chemical composition, morphology, and rheological properties of starches isolated from tropical fruits in Mexico, namely: (1) stenospermocarpic mango (Mangifera indica L.) 'Ataulfo', which is considered a postharvest loss due to its small size and no commercial value; (2) 'Pera' banana (Musa ABB), a low commercial value fruit; and (3) soursop (Annona muricata L.), a highly perishable fruit. The research concerning the morphological and rheological properties of those starches is scarce to date. The starches presented amylose contents ranging between 24.7 and 29.4% (w/w), congruent with the amylose content in most normal native starches. During pasting, the viscosities of the 7% fruit starch suspensions were higher than those of the normal corn starch (reference). Mango and soursop starches are rapid-swelling starches; their pasting temperatures were 66.3 and 69.5°C, respectively. Banana starch showed the highest peak viscosity value (0.89 Pa s), and soursop starch pastes exhibited the lowest retrogradation tendency (setback viscosity = 0.168 Pa s). After cooling, the starch pastes exhibited soft gel-like viscoelastic behaviour. Accordingly, the rheological characterisation of the pastes and gels of the isolated starches allows us to propose them as new starches for diverse food and biotechnological applications. [ABSTRACT FROM AUTHOR]
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- 2024
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45. Motor learning induces plastic changes in Purkinje cell dendritic spines in the rat cerebellum
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González-Tapia, D., González-Ramírez, M.M., Vázquez-Hernández, N., and González-Burgos, I.
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- 2020
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46. El aprendizaje motor induce cambios plásticos en las espinas dendríticas de las células de Purkinje del cerebelo de ratas
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González-Tapia, D., González-Ramírez, M.M., Vázquez-Hernández, N., and González-Burgos, I.
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- 2020
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47. Clinical significance of epithelial–mesenchymal transition-related markers expression in the micrometastatic sentinel lymph node of NSCLC
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Lafuente-Sanchis, A., Olmo, A., Carretero, J., Alcacer Fernandez-Coronado, J., Estors-Guerrero, M., Martínez-Hernández, N. J., Cremades, A., Zúñiga, A., Alcacer, J., Farras, R., Cuenca, M., and Galbis-Caravajal, J. M.
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- 2020
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48. The flashfm approach for fine-mapping multiple quantitative traits
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Hernández, N., Soenksen, J., Newcombe, P., Sandhu, M., Barroso, I., Wallace, C., and Asimit, J. L.
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- 2021
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49. Review of the scientific evidence and technical opinion on noncaloric sweetener consumption in gastrointestinal diseases
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Bueno-Hernández, N., Vázquez-Frías, R., Abreu y Abreu, A.T., Almeda-Valdés, P., Barajas-Nava, L.A., Carmona-Sánchez, R.I., Chávez-Sáenz, J., Consuelo-Sánchez, A., Espinosa-Flores, A.J., Hernández-Rosiles, V., Hernández-Vez, G., Icaza-Chávez, M.E., Noble-Lugo, A., Romo-Romo, A., Ruiz-Margaín, A., Valdovinos-Díaz, M.A., and Zárate-Mondragón, F.E.
- Published
- 2019
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50. Production and characterization of biodegradable films of a novel polyhydroxyalkanoate (PHA) synthesized from peanut oil
- Author
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Pérez-Arauz, A.O., Aguilar-Rabiela, A.E., Vargas-Torres, A., Rodríguez-Hernández, A.-I., Chavarría-Hernández, N., Vergara-Porras, B., and López-Cuellar, M.R.
- Published
- 2019
- Full Text
- View/download PDF
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