Zobrazeno 1 - 10
of 20 832
pro vyhledávání: '"P. Pino"'
Publikováno v:
ESPOCH Congresses, Vol 1, Iss 5, Pp 1347-1356 (2021)
Abstract The objective of this research was to determine the quality of the protein present in sausages fortified with quinoa as a substitute for animal protein, through the identification and quantification of amino acids, using gas chromatography a
Externí odkaz:
https://doaj.org/article/6d5b81a891034c4098d3eff12e21fe82
Publikováno v:
ESPOCH Congresses, Vol 1, Iss 5, Pp 1357-1369 (2021)
Abstract The present study aimed to assess the bromatological composition when soy protein was added in the preparation of cooked ham. An experimental approach was used. There were three treatments in which 2.50% (T1), 5.00% (T2) and 7.50% (T3) soy p
Externí odkaz:
https://doaj.org/article/c82d9210ac434a7aaff07b3bd5ba3036
Measurements from astroparticle experiments, such as the 2017 flare associated with the source TXS 0506+056, indicate that blazars act as multi-messenger (MM; radiation and neutrinos) factories. Theoretically, the particle acceleration mechanisms res
Externí odkaz:
http://arxiv.org/abs/2411.10210
Autor:
Marconcini, C., D'Eugenio, F., Maiolino, R., Arribas, S., Bunker, A., Carniani, S., Charlot, S., Perna, M., Del Pino, B. Rodríguez, Übler, H., Pérez-González, P. G., Willott, C. J., Böker, T., Cresci, G., Curti, M., Lamperti, I., Scholtz, J., Parlanti, E., Venturi, G.
We present JWST/NIRSpec integral field spectroscopic (IFS) observations of the \Lyalpha emitter CR7 at z ~ 6.6, observed as part of the GA-NIFS program. Using low-resolution PRISM (R ~ 100) data, we confirm a bright \Lyalpha emitter, and a diffuse \L
Externí odkaz:
http://arxiv.org/abs/2411.08627
Autor:
Scholtz, J., Curti, M., D'Eugenio, F., Übler, H., Maiolino, R., Marconcini, C., Smit, R., Perna, M., Witstok, J., Arribas, S., Böker, T., Bunker, A. J., Carniani, S., Charlot, S., Cresci, G., Pérez-González, P. G., Lamperti, I., Del Pino, B. Rodríguez, Parlanti, E., Venturi, G.
We present deep JWST/NIRSpec integral-field spectroscopy (IFS) and ALMA [CII]$\lambda$158$\mu$m observations of COS-3018, a star-forming galaxy at z$\sim$6.85, as part of the GA-NIFS programme. Both G395H (R$\sim$ 2700) and PRISM (R$\sim$ 100) NIRSpe
Externí odkaz:
http://arxiv.org/abs/2411.07695
Recent advancements in ultra-stable ground-based high-resolution spectrographs have propelled ground-based astronomy to the forefront of exoplanet detection and characterisation. Retrieving accurate atmospheric parameters depends on accurate modellin
Externí odkaz:
http://arxiv.org/abs/2410.19588
This paper addresses the long-time dynamics of solutions to the 2D incompressible Euler equations. We construct solutions with continuous vorticity $\omega_{\varepsilon}(x,t)$ concentrated around points $\xi_{j}(t)$ that converge to a sum of Dirac de
Externí odkaz:
http://arxiv.org/abs/2410.18220
Autor:
Smith, Peter C. B., Sanchez, Jorge A., Line, Michael R., Rauscher, Emily, Mansfield, Megan Weiner, Kempton, Eliza M. -R., Savel, Arjun, Wardenier, Joost P., Pino, Lorenzo, Bean, Jacob L., Beltz, Hayley, Panwar, Vatsal, Brogi, Matteo, Malsky, Isaac, Fortney, Jonathan, Desert, Jean-Michel, Pelletier, Stefan, Parmentier, Vivien, Kanumalla, Krishna, Welbanks, Luis, Meyer, Michael, Monnier, John
A primary goal of exoplanet science is to measure the atmospheric composition of gas giants in order to infer their formation and migration histories. Common diagnostics for planet formation are the atmospheric metallicity ([M/H]) and the carbon-to-o
Externí odkaz:
http://arxiv.org/abs/2410.19017
We numerically investigate a crucial parameter for understanding particle acceleration theory via turbulence-induced magnetic reconnection: the particle acceleration time. We examine particles accelerated either during the jet's dynamic evolution or
Externí odkaz:
http://arxiv.org/abs/2410.13071
We consider the Ginzburg-Landau equation in the plane linearized around the standard degree-one vortex solution $W(x)=w(r)e^{i\theta}$. Using explicit representation formulae for the Fourier modes in $\theta$, we obtain sharp estimates for the invers
Externí odkaz:
http://arxiv.org/abs/2410.12646