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352 results on '"Fernandes, C. P."'

1. Extremal Problems on Forest Cuts and Acyclic Neighborhoods in Sparse Graphs

Author

Botler, F., Couto, Y. S., Fernandes, C. G., de Figueiredo, E. F., Gómez, R., Santos, V. F. dos, and Sato, C. M.

Subjects
Mathematics - Combinatorics, Computer Science - Discrete Mathematics
Abstract

Chernyshev, Rauch, and Rautenbach proved that every connected graph on $n$ vertices with less than $\frac{11}{5}n-\frac{18}{5}$ edges has a vertex cut that induces a forest, and conjectured that the same remains true if the graph has less than $3n-6$ edges. We improve their result by proving that every connected graph on $n$ vertices with less than $\frac{9}{4}n$ edges has a vertex cut that induces a forest. We also study weaker versions of the problem that might lead to an improvement on the bound obtained.

Published
2024

2. Assessing the detection of floating plastic litter with advanced remote sensing technologies in a hydrodynamic test facility

Author

de Fockert, A., Eleveld, M. A., Bakker, W., Felício, J. M., Costa, T. S., Vala, M., Marques, P., Leonor, N., Moreira, A., Costa, J. R., Caldeirinha, R. F. S., Matos, S. A., Fernandes, C. A., Fonseca, N., Simpson, M.D., Marino, A., Gandini, E., Camps, A., Perez-Portero, A., Gonga, A., Burggraaff, O., Garaba, S. P., Salama, M.S., Xiao, Q., Calvert, R., van den Bremer, T. S., and de Maagt, P.

Published
2024
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5. Accelerating Solutions for the Overdose Crisis: an Effectiveness-Implementation Hybrid Protocol for the HEAL Prevention Cooperative.

Author

Patel, S, Cance, J, Bonar, E, Carter, P, Dickerson, D, Fiellin, L, Fernandes, C, Palimaru, A, Boomer, T, Saldana, L, Singh, R, Tinius, E, Walton, M, Youn, S, Young, S, Philbrick, S, and Lambdin, B

Subjects
Implementation, Opioids, Prevention, Scale-up, Youth, Adolescent, Young Adult, Humans, Drug Overdose, Opioid-Related Disorders, Behavior, Addictive
Abstract

Given increasing opioid overdose mortality rates in the USA over the past 20 years, accelerating the implementation of prevention interventions found to be effective is critical. The Helping End Addiction Long-Term (HEAL) Prevention Cooperative (HPC) is a consortium of research projects funded to implement and test interventions designed to prevent the onset or escalation of opioid misuse among youth and young adults. The HPC offers a unique opportunity to synthesize and share lessons learned from participating research projects varied implementation experiences, which can facilitate quicker integration of effective prevention interventions into practice. This protocol paper describes our hybrid approach to collecting and analyzing information about the implementation experiences of nine of the HPC research projects while they maintain their focus on assessing the effectiveness and cost-effectiveness of prevention interventions. To better understand implementation within this context, we will address five research questions: (1) What were the context and approach for implementing the prevention interventions, and how was the overall implementation experience? (2) How representative of the target population are the participants who were enrolled and retained in the research projects effectiveness trials? (3) For what purposes and how were stakeholders engaged by the research projects? (4) What are the adaptable components of the prevention interventions? And finally, (5) how might implementation of the prevention interventions vary for non-trial implementation? This work will result in intervention-specific and general practical dissemination resources that can help potential adopters and deliverers of opioid misuse prevention make adoption decisions and prepare for successful implementation.

Published
2023

8. Particle-level Simulation of Magnetorheological Fluids: A Fully-Resolved Solver

Author

Fernandes, C. and Faroughi, Salah A.

Subjects
Physics - Fluid Dynamics, Physics - Computational Physics
Abstract

Magnetorheological fluids (MRFs) are smart materials consisting of micro-scale magnetizable particles suspended in a carrier fluid. The rheological properties of a MRF can be changed from a fluid-state to a solid-state upon the application of an external magnetic field. This study reports the development of a particle-level simulation code for magnetic solid spheres moving through an incompressible Newtonian carrier fluid. The numerical algorithm is implemented within an open-source finite-volume solver coupled with an immersed boundary method (FVM-IBM) to perform fully-resolved simulations. The particulate phase of the MRF is modeled using the discrete element method (DEM). The resultant force acting on the particles due to the external magnetic field is computed based on the Clausius-Mossotti relationship. The fixed and mutual dipole magnetic models are then used to account for the magnetic (MAG) interactions between particles. Several benchmark flows were simulated using the newly-developed FVM-IBM-DEM-MAG algorithm to assess the accuracy and robustness of the calculations.

Published
2022

12. Alternatives to $\Lambda$: Torsion, Generalized Couplings, and Scale Invariance

Author

Martins, C. J. A. P., Marques, C. M. J., Fernandes, C. B. D., Oliveira, J. S. J. S., Pinheiro, D. A. R., and Rocha, B. A. R.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology
Abstract

We present a comparative analysis of current observational constraints on three recently discussed alternative models for explaining the low-redshift acceleration of the universe: the so-called steady-state torsion model, the generalized coupling model, and the scale invariant model by Maeder (an example of a broader class which we also briefly study) These are compared to the traditional parameterization of Chevallier, Polarski and Linder. Each of the candidate models is studied under two different assumptions: as genuine alternatives to $\Lambda$CDM (where a new degree of freedom would be expected to explain the recent acceleration of the universe without any cosmological constant) and as parametric extensions of $\Lambda$CDM (where both a cosmological constant and the new mechanism can coexist, and the relative contributions of both are determined by the data). Our comparative analysis suggests that, from a phenomenological point of view, all such models neatly divide into two classes, with different observational consequences., Comment: Summary of a talk given at the Theories of Gravity: Alternatives to the Cosmological and Particle Standard Models parallel session of the Sixteenth Marcel Grossmann Meeting, partially summarizing work previously reported in arXiv:1911.08232 and arXiv:2012.10513. To appear in the proceedings

Published
2021

13. Constraining alternatives to a cosmological constant: generalized couplings and scale invariance

Author

Fernandes, C. B. D., Martins, C. J. A. P., and Rocha, B. A. R.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology
Abstract

We present a comparative analysis of observational low-redshift background constraints on three candidate models for explaining the low-redshift acceleration of the universe. The generalized coupling model by Feng and Carloni and the scale invariant model by Maeder (both of which can be interpreted as bimetric theories) are compared to the traditional parametrization of Chevallier, Polarski and Linder. In principle the generalized coupling model, which in vacuum is equivalent to General Relativity, contains two types of vacuum energy: the usual cosmological constant plus a second contribution due to the matter fields. We show that the former is necessary for the model to agree with low-redshift observations, while there is no statistically significant evidence for the presence of the second. On the other hand the scale invariant model effectively has a time-dependent cosmological constant. In this case we show that a matter density $\Omega_m\sim0.3$ is a relatively poor fit to the data, and the best-fit model would require a fluid with a much smaller density and a significantly positive equation of state parameter., Comment: 15 pages, 6 figures, Physics of the Dark Universe (in press)

Published
2020

15. The novel Mechanical Ventilator Milano for the COVID-19 pandemic.

Author

Abba, A, Accorsi, C, Agnes, P, Alessi, E, Amaudruz, P, Annovi, A, Desages, F Ardellier, Back, S, Badia, C, Bagger, J, Basile, V, Batignani, G, Bayo, A, Bell, B, Beschi, M, Biagini, D, Bianchi, G, Bicelli, S, Bishop, D, Boccali, T, Bombarda, A, Bonfanti, S, Bonivento, WM, Bouchard, M, Breviario, M, Brice, S, Brown, R, Calvo-Mozota, JM, Camozzi, L, Camozzi, M, Capra, A, Caravati, M, Carlini, M, Ceccanti, A, Celano, B, Cela Ruiz, JM, Charette, C, Cogliati, G, Constable, M, Crippa, C, Croci, G, Cudmore, S, Dahl, CE, Dal Molin, A, Daley, M, Di Guardo, C, D'Avenio, G, Davignon, O, Del Tutto, M, De Ruiter, J, Devoto, A, Diaz Gomez Maqueo, P, Di Francesco, F, Dossi, M, Druszkiewicz, E, Duma, C, Elliott, E, Farina, D, Fernandes, C, Ferroni, F, Finocchiaro, G, Fiorillo, G, Ford, R, Foti, G, Fournier, RD, Franco, D, Fricbergs, C, Gabriele, F, Galbiati, C, Garcia Abia, P, Gargantini, A, Giacomelli, L, Giacomini, F, Giarratana, LS, Gillespie, S, Giorgi, D, Girma, T, Gobui, R, Goeldi, D, Golf, F, Gorel, P, Gorini, G, Gramellini, E, Grosso, G, Guescini, F, Guetre, E, Hackman, G, Hadden, T, Hawkins, W, Hayashi, K, Heavey, A, Hersak, G, Hessey, N, Hockin, G, Hudson, K, Ianni, A, Ienzi, C, Ippolito, V, and James, CC

Subjects
Mathematical Sciences, Physical Sciences, Engineering, Fluids & Plasmas
Abstract

This paper presents the Mechanical Ventilator Milano (MVM), a novel intensive therapy mechanical ventilator designed for rapid, large-scale, low-cost production for the COVID-19 pandemic. Free of moving mechanical parts and requiring only a source of compressed oxygen and medical air to operate, the MVM is designed to support the long-term invasive ventilation often required for COVID-19 patients and operates in pressure-regulated ventilation modes, which minimize the risk of furthering lung trauma. The MVM was extensively tested against ISO standards in the laboratory using a breathing simulator, with good agreement between input and measured breathing parameters and performing correctly in response to fault conditions and stability tests. The MVM has obtained Emergency Use Authorization by U.S. Food and Drug Administration (FDA) for use in healthcare settings during the COVID-19 pandemic and Health Canada Medical Device Authorization for Importation or Sale, under Interim Order for Use in Relation to COVID-19. Following these certifications, mass production is ongoing and distribution is under way in several countries. The MVM was designed, tested, prepared for certification, and mass produced in the space of a few months by a unique collaboration of respiratory healthcare professionals and experimental physicists, working with industrial partners, and is an excellent ventilator candidate for this pandemic anywhere in the world.

Published
2021

16. The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters

Author

de Oliveira, C. Mendes, Ribeiro, T., Schoenell, W., Kanaan, A., Overzier, R. A., Molino, A., Sampedro, L., Coelho, P., Barbosa, C. E., Cortesi, A., Costa-Duarte, M. V., Herpich, F. R., Hernandez-Jimenez, J. A., Placco, V. M., Xavier, H. S., Abramo, L. R., Saito, R. K., Chies-Santos, A. L., Ederoclite, A., de Oliveira, R. Lopes, Gonçalves, D. R., Akras, S., Almeida, L. A., Almeida-Fernandes, F., Beers, T. C., Bonatto, C., Bonoli, S., Cypriano, E. S., de Lima, Erik V. R., de Souza, R. S., de Souza, G. Fabiano, Ferrari, F., Gonçalves, T. S., Gonzalez, A. H., Gutiérrez-Soto, L. A., Hartmann, E. A., Jaffe, Y., Kerber, L. O., Lima-Dias, C., Lopes, P. A. A., Menendez-Delmestre, K., Nakazono, L. M. I., Novais, P. M., Ortega-Minakata, R. A., Pereira, E. S., Perottoni, H. D., Queiroz, C., Reis, R. R. R., Santos, W. A., Santos-Silva, T., Santucci, R. M., Barbosa, C. L., Siffert, B. B., Sodré Jr., L., Torres-Flores, S., Westera, P., Whitten, D. D., Alcaniz, J. S., Alonso-García, Javier, Alencar, S., Alvarez-Candal, A., Amram, P., Azanha, L., Barbá, R. H., Bernardinelli, P. H., Fernandes, M. Borges, Branco, V., Brito-Silva, D., Buzzo, M. L., Caffer, J., Campillay, A., Cano, Z., Carvano, J. M., Castejon, M., Fernandes, R. Cid, Dantas, M. L. L., Daflon, S., Damke, G., de la Reza, R., de Azevedo, L. J. de Melo, De Paula, D. F., Diem, K. G., Donnerstein, R., Dors, O. L., Dupke, R., Eikenberry, S., Escudero, Carlos G., Faifer, Favio R., Farías, H., Fernandes, B., Fernandes, C., Fontes, S., Galarza, A., Hirata, N. S. T., Katena, L., Gregorio-Hetem, J., Hernández-Fernández, J. D., Izzo, L., Arancibia, M. Jaque, Jatenco-Pereira, V., Jiménez-Teja, Y., Kann, D. A., Krabbe, A. C., Labayru, C., Lazzaro, D., Neto, G. B. Lima, Lopes, Amanda R., Magalhães, R., Makler, M., de Menezes, R., Miralda-Escudé, J., Monteiro-Oliveira, R., Montero-Dorta, A. D., Muñoz-Elgueta, N., Nemmen, R. S., Castellón, J. L. Nilo, Oliveira, A. S., Ortíz, D., Pattaro, E., Pereira, C. B., Quint, B., Riguccini, L., Pinto, H. J. Rocha, Rodrigues, I., Roig, F., Rossi, S., Saha, Kanak, Santos, R., Müller, A. Schnorr, Sesto, Leandro A., Silva, R., Castelli, Analía V. Smith, Teixeira, Ramachrisna, Telles, E., de Souza, R. C. Thom, Thöne, C., Trevisan, M., Postigo, A. de Ugarte, Urrutia-Viscarra, F., Veiga, C. H., Vika, M., Vitorelli, A. Z., Werle, A., Werner, S. V., and Zaritsky, D.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-South, at the Cerro Tololo Inter-American Observatory, Chile. The telescope is equipped with a 9.2k by 9.2k e2v detector with 10 um pixels, resulting in a field-of-view of 2 deg^2 with a plate scale of 0.55"/pixel. The survey consists of four main subfields, which include two non-contiguous fields at high Galactic latitudes (8000 deg^2 at |b| > 30 deg) and two areas of the Galactic plane and bulge (for an additional 1300 deg^2). S-PLUS uses the Javalambre 12-band magnitude system, which includes the 5 u, g, r, i, z broad-band filters and 7 narrow-band filters centered on prominent stellar spectral features: the Balmer jump/[OII], Ca H+K, H-delta, G-band, Mg b triplet, H-alpha, and the Ca triplet. S-PLUS delivers accurate photometric redshifts (delta_z/(1+z) = 0.02 or better) for galaxies with r < 20 AB mag and redshift < 0.5, thus producing a 3D map of the local Universe over a volume of more than 1 (Gpc/h)^3. The final S-PLUS catalogue will also enable the study of star formation and stellar populations in and around the Milky Way and nearby galaxies, as well as searches for quasars, variable sources, and low-metallicity stars. In this paper we introduce the main characteristics of the survey, illustrated with science verification data highlighting the unique capabilities of S-PLUS. We also present the first public data release of ~336 deg^2 of the Stripe-82 area, which is available at http://datalab.noao.edu/splus., Comment: Updated to reflect the published version (MNRAS, 489, 241). For a short introductory video of the S-PLUS project, see https://youtu.be/yc5kHrHU9Jk - The S-PLUS Data Release 1 is available at http://datalab.noao.edu/splus

Published
2019
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17. Absorption of single-layer hexagonal boron nitride in the ultraviolet

Author

Henriques, J. C. G., Ventura, G. B., Fernandes, C. D. M., and Peres, N. M. R.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

In this paper we theoretically describe the absorption of hexagonal boron nitride (hBN) single layer. We develop the necessary formalism and present an efficient method for solving the Wannier equation for excitons. We give predictions for the absorption of hBN on quartz and on graphite. We compare our predictions with recently published results [Elias {\it et al.}, Nat. Comm. {\bf 10}, 2639 (2019)] for a monolayer of hBN on graphite. The spontaneous radiative lifetime of excitons in hBN is also computed. We argue that the optical properties of hBN in the ultraviolet are very useful for the study of peptides and other biomolecules., Comment: 14 pages

Published
2019
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19. Bulgeless galaxies in the COSMOS field: environment and star formation evolution at $z < 1$

Author

Grossi, M., Fernandes, C. A. C., Sobral, D., Afonso, J., Telles, E., Bizzocchi, L., Paulino-Afonso, A., and Matute, I.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

Combining the catalogue of galaxy morphologies in the COSMOS field and the sample of H$\alpha$ emitters at redshifts $z=0.4$ and $z=0.84$ of the HiZELS survey, we selected $\sim$ 220 star-forming bulgeless systems (S\'ersic index $n \leq 1.5$) at both epochs. We present their star formation properties and we investigate their contribution to the star formation rate function (SFRF) and global star formation rate density (SFRD) at $z < 1$. For comparison, we also analyse H$\alpha$ emitters with more structurally evolved morphologies that we split into two classes according to their S\'ersic index $n$: intermediate ($ 1.5 < n \leq 3 $) and bulge-dominated ($n > 3$). At both redshifts the SFRF is dominated by the contribution of bulgeless galaxies and we show that they account for more than 60% of the cosmic SFRD at $z < 1$. The decrease of the SFRD with redshift is common to the three morphological types but it is stronger for bulge-dominated systems. Star-forming bulgeless systems are mostly located in regions of low to intermediate galaxy densities ($\Sigma \sim 1 - 4$ Mpc$^{-2}$) typical of field-like and filament-like environments and their specific star formation rates (sSFRs) do not appear to vary strongly with local galaxy density. Only few bulgeless galaxies in our sample have high (sSFR $>$ 10$^{-9}$ yr$^{-1}$) and these are mainly low-mass systems. Above $M_* \sim 10^{10}$ M$_{\odot}$ bulgeless are evolving at a "normal" rate (10$^{-9}$ yr$^{-1} <$ sSFR $<$10$^{-10}$ yr$^{-1}$) and in the absence of an external trigger (i.e. mergers/strong interactions) they might not be able to develop a central classical bulge., Comment: 14 page, 9 figures, accepted for publication in MNRAS

Published
2017
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20. Analytical solutions for the Schr\'odinger equation subjected to a deformable hyperbolic potential

Author

Fernandes, C. J. M. and Cunha, M. S.

Subjects
Quantum Physics
Abstract

In this work we discuss in detail the known solutions of the stationary Schr\"odinger equation subject to a deformable hyperbolic tangent potential exactly soluble $ V(x) = \frac {V_0} {2} (1+ \tanh (\delta x)) $. We find the analytical solutions in terms of Gauss hypergeometric functions for the scattering states with energy greater than the maximum value of the potential. We also discussed the case for the energy lower than the maximum and the similarities and differences with the abrupt step potential in both cases. We graphically illustrate the relevant physical situations to the problem., Comment: 16 pages, 19 figures. In Portuguese

Published
2016

21. Ionization and feedback in Ly$\alpha$ halos around two radio galaxies at z$\sim$2.5

Author

Morais, S. G., Humphrey, A., Villar-Martín, M., Lagos, P., Moyano, M., Overzier, R., Alighieri, S. di Serego, Vernet, J., and Fernandes, C. A. C.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We present new spectroscopic observations of two high redshift radio galaxies, TXS 0211-122 (z=2.34) and TXS 0828+193 (z=2.57), known to be associated with large Ly$\alpha$ halos. The observations were taken with the slits placed perpendicularly to the radio axis. With access to pre-existing Keck II observations taken with the slit placed along the radio axis we are able to compare the properties of the gas in different regions of the galaxies. In both objects we detect spatially extended Ly$\alpha$ emission perpendicularly to the radio axis. In TXS 0211-122, the flux and velocity profiles of Ly$\alpha$ are strongly affected by HI absorption/scattering. In line with previous studies, we find evidence for outflowing gas along the radio axis which may be the result of jet-gas interactions. In the slit oriented perpendicularly to the radio axis we find less perturbed gas kinematics, suggesting outflows of ionized gas in this object are focused along the radio jet axis. Additionally, we find evidence for a giant, UV-emitting arc or shell-like structure surrounding the radio galaxy Ly$\alpha$ halo, possibly resulting from feedback activity. In TXS 0828+193 a large Ly$\alpha$ halo ($\sim$56 kpc) is detected perpendicularly to the radio axis. Along both slit position angles we find evidence for outflowing gas, which we argue is part of an approximately spherical, expanding shell or bubble of gas powered by feedback activity in the central regions of the galaxy. Our results suggest a diversity in the spatial distribution of ionized outflows in powerful radio galaxies at z$\sim$2.5.

Published
2016
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22. Accurate PSF-matched photometry and photometric redshifts for the Extreme Deep Field with the Chebyshev-Fourier functions

Author

Jiménez-Teja, Y., Benítez, N., Molino, A., and Fernandes, C. A. C.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

Photometric redshifts, which have become the cornerstone of several of the largest astronomical surveys like PanStarrs, DES, J-PAS or the LSST, require precise measurements of galaxy photometry in different bands using a consistent physical aperture. This is not trivial, due to the variation in the shape and width of the Point Spread Function (PSF) introduced by wavelength differences, instrument positions and atmospheric conditions. Current methods to correct for this effect rely on a detailed knowledge of the PSF characteristics as a function of the survey coordinates, which can be difficult due to the relative paucity of stars tracking the PSF behaviour. Here we show that it is possible to measure accurate, consistent multicolour photometry without knowing the shape of PSF. The Chebyshev-Fourier Functions (CHEFs) can fit the observed profile of each object and produce high signal-to-noise integrated flux measurements unaffected by the PSF. These total fluxes, which encompass all the galaxy populations, are much more useful for Galaxy Evolution studies than aperture photometry. We compare the total magnitudes and colours obtained using our software to traditional photometry with SExtractor, using real data from the COSMOS survey and the Hubble Ultra Deep Field. We also apply the CHEFs technique to the recently published Extreme Deep Field and compare the results to those from ColorPro on the HUDF. We produce a photometric catalogue with 35732 sources (10823 with S/N>5), reaching a photometric redshift precision of 2% due to the extraordinary depth and wavelength coverage of the XDF images., Comment: 12 pages, 12 figures, submitted to MNRAS 2014 July 10, accepted 2015 July 15

Published
2015
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23. The COVID-19 Pandemic in Brazil: Some Aspects and Tools

Author

Pedro Rafael D. Marinho, Gauss M. Cordeiro, Hemilio Fernandes C. Coelho, and Poliana C. Cabral

Subjects
Brazil, COVID-19, GAMLSS models, statistics, tools, web application, Internal medicine, RC31-1245
Abstract

The article presents some aspects related to the COVID-19 pandemic in Brazil including public health, challenges facing healthcare workers and adverse impacts on the country’s economy. Its main contribution is the availability of two web applications for online monitoring of the evolution of the pandemic in Brazil and South America. The applications provide the possibility to download data in different formats, view interactive maps and graphs of the cumulative confirmed cases, deaths and lethality rates, in addition to presenting plots of moving averages for states and municipalities. The predictions about new cases and new deaths caused by COVID-19, in states and regions of Brazil, are also reported using GAMLSS models. The forecasts can be easily used by public managers for effective decision-making.

Published
2021
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25. J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey

Author

Benitez, N., Dupke, R., Moles, M., Sodre, L., Cenarro, J., Marin-Franch, A., Taylor, K., Cristobal, D., Fernandez-Soto, A., de Oliveira, C. Mendes, Cepa-Nogue, J., Abramo, L. R., Alcaniz, J. S., Overzier, R., Hernandez-Monteagudo, C., Alfaro, E. J., Kanaan, A., Carvano, J. M., Reis, R. R. R., Gonzalez, E. Martinez, Ascaso, B., Ballesteros, F., Xavier, H. S., Varela, J., Ederoclite, A., Ramio, H. Vazquez, Broadhurst, T., Cypriano, E., Angulo, R., Diego, J. M., Zandivarez, A., Diaz, E., Melchior, P., Umetsu, K., Spinelli, P. F., Zitrin, A., Coe, D., Yepes, G., Vielva, P., Sahni, V., Marcos-Caballero, A., Kitaura, F. Shu, Maroto, A. L., Masip, M., Tsujikawa, S., Carneiro, S., Nuevo, J. Gonzalez, Carvalho, G. C., Reboucas, M. J., Carvalho, J. C., Abdalla, E., Bernui, A., Pigozzo, C., Ferreira, E. G. M., Devi, N. Chandrachani, Bengaly Jr., C. A. P., Campista, M., Amorim, A., Asari, N. V., Bongiovanni, A., Bonoli, S., Bruzual, G., Cardiel, N., Cava, A., Fernandes, R. Cid, Coelho, P., Cortesi, A., Delgado, R. G., Garcia, L. Diaz, Espinosa, J. M. R., Galliano, E., Gonzalez-Serrano, J. I., Falcon-Barroso, J., Fritz, J., Fernandes, C., Gorgas, J., Hoyos, C., Jimenez-Teja, Y., Lopez-Aguerri, J. A., Juan, C. Lopez-San, Mateus, A., Molino, A., Novais, P., OMill, A., Oteo, I., Perez-Gonzalez, P. G., Poggianti, B., Proctor, R., Ricciardelli, E., Sanchez-Blazquez, P., Storchi-Bergmann, T., Telles, E., Schoennell, W., Trujillo, N., Vazdekis, A., Viironen, K., Daflon, S., Aparicio-Villegas, T., Rocha, D., Ribeiro, T., Borges, M., Martins, S. L., Marcolino, W., Martinez-Delgado, D., Perez-Torres, M. A., Siffert, B. B., Calvao, M. O., Sako, M., Kessler, R., Alvarez-Candal, A., De Pra, M., Roig, F., Lazzaro, D., Gorosabel, J., de Oliveira, R. Lopes, Lima-Neto, G. B., Irwin, J., Liu, J. F., Alvarez, E., Balmes, I., Chueca, S., Costa-Duarte, M. V., da Costa, A. A., Dantas, M. L. L., Diaz, A. Y., Fabregat, J., Ferrari, F., Gavela, B., Gracia, S. G., Gruel, N., Gutierrez, J. L. L., Guzman, R., Hernandez-Fernandez, J. D., Herranz, D., Hurtado-Gil, L., Jablonsky, F., Laporte, R., Tiran, L. L. Le, Licandro, J, Lima, M., Martin, E., Martinez, V., Montero, J. J. C., Penteado, P., Pereira, C. B., Peris, V., Quilis, V., Sanchez-Portal, M., Soja, A. C., Solano, E., Torra, J., and Valdivielso, L.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

The Javalambre-Physics of the Accelerated Universe Astrophysical Survey (J-PAS) is a narrow band, very wide field Cosmological Survey to be carried out from the Javalambre Observatory in Spain with a purpose-built, dedicated 2.5m telescope and a 4.7 sq.deg. camera with 1.2Gpix. Starting in late 2015, J-PAS will observe 8500sq.deg. of Northern Sky and measure $0.003(1+z)$ photo-z for $9\times10^7$ LRG and ELG galaxies plus several million QSOs, sampling an effective volume of $\sim 14$ Gpc$^3$ up to $z=1.3$ and becoming the first radial BAO experiment to reach Stage IV. J-PAS will detect $7\times 10^5$ galaxy clusters and groups, setting constrains on Dark Energy which rival those obtained from its BAO measurements. Thanks to the superb characteristics of the site (seeing ~0.7 arcsec), J-PAS is expected to obtain a deep, sub-arcsec image of the Northern sky, which combined with its unique photo-z precision will produce one of the most powerful cosmological lensing surveys before the arrival of Euclid. J-PAS unprecedented spectral time domain information will enable a self-contained SN survey that, without the need for external spectroscopic follow-up, will detect, classify and measure $\sigma_z\sim 0.5\%$ redshifts for $\sim 4000$ SNeIa and $\sim 900$ core-collapse SNe. The key to the J-PAS potential is its innovative approach: a contiguous system of 54 filters with $145\AA$ width, placed $100\AA$ apart over a multi-degree FoV is a powerful "redshift machine", with the survey speed of a 4000 multiplexing low resolution spectrograph, but many times cheaper and much faster to build. The J-PAS camera is equivalent to a 4.7 sq.deg. "IFU" and it will produce a time-resolved, 3D image of the Northern Sky with a very wide range of Astrophysical applications in Galaxy Evolution, the nearby Universe and the study of resolved stellar populations., Comment: 215 pages, 70 figures. J-PAS "Red Book", containing a description of the technical aspects of the Survey and its main scientific goals

Published
2014

26. Unravelling the effect of SrTiO3 antiferrodistortive phase transition on the magnetic properties of La0.7Sr0.3MnO3 thin films

Author

Mota, D. A., Barcelay, Y. Romaguera, Senos, A. M. R., Fernandes, C. M., Tavares, P. B., Gomes, I. T., Sá, P., Fernandes, L., Almeida, B. G., Figueiras, F., Vaghefi, P. Mirzadeh, Amaral, V. S., Almeida, A., de la Cruz, J. Pérez, and Moreira, J. Agostinho

Subjects
Condensed Matter - Materials Science, Condensed Matter - Strongly Correlated Electrons
Abstract

Epitaxial La0.7Sr0.3MnO3 (LSMO) thin films, with different thickness ranging from 20 nm up to 330 nm, were deposited on (100)-oriented strontium titanate (STO) substrates by pulsed laser deposition, and their structure and morphology characterized at room temperature. Magnetic and electric transport properties of the as-processed thin films reveal an abnormal behavior in the temperature dependent magnetization M(T) below the antiferrodistortive STO phase transition (TSTO) and also an anomaly in the magnetoresistance and electrical resistivity close to the same temperature. Up to 100 nm LSMO thin films, an in-excess magnetization and pronounced changes in the coercivity are evidenced, achieved through the interface-mediated magnetoelastic coupling with antiferrodistortive domain wall movement occurring below TSTO. Contrarily, for thicker LSMO thin films, above 100 nm, an in-defect magnetization is observed. This reversed behavior can be understood within the emergence in the upper layer of the film, observed by high resolution transmission electron microscopy, of a branched structure needed to relax elastic energy stored in the film which leads to randomly oriented magnetic domain reconstructions. For enough high-applied magnetic fields, as thermodynamic equilibrium is reached, a fully suppression of the anomalous magnetization occurs, wherein the temperature dependence of the magnetization starts to follow the expected Brillouin behavior., Comment: 15 pages, 9 figures

Published
2014
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30. High coercivity induced by mechanical milling in cobalt ferrite powders

Author

Ponce, A. S., Chagas, E. F., Prado, R. J., Fernandes, C. H. M., Terezo, A. J., and Baggio-Saitovitch, E.

Subjects
Condensed Matter - Materials Science
Abstract

In this work we report a study of the magnetic behavior of ferrimagnetic oxide CoFe2O4 treated by mechanical milling with different grinding balls. The cobalt ferrite nanoparticles were prepared using a simple hydrothermal method and annealed at 500oC. The non-milled sample presented coercivity of about 1.9 kOe, saturation magnetization of 69.5 emu/g, and a remanence ratio of 0.42. After milling, two samples attained coercivity of 4.2 and 4.1 kOe, and saturation magnetization of 67.0 and 71.4 emu/g respectively. The remanence ratio MR/MS for these samples increase to 0.49 and 0.51, respectively. To investigate the influence of the microstructure on the magnetic behavior of these samples, we used X-ray powder diffraction (XPD), transmission electron microscopy (TEM), and vibrating sample magnetometry (VSM). The XPD analysis by the Williamson-Hall plot was used to estimate the average crystallite size and strain induced by mechanical milling in the samples.

Published
2013

33. Metallicity of M dwarfs II. A comparative study of photometric metallicity scales

Author

Neves, V., Bonfils, X., Santos, N. C., Delfosse, X., Forveille, T., Allard, F., Natário, C., Fernandes, C. S., and Udry, S.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

Stellar parameters are not easily derived from M dwarf spectra, which are dominated by complex bands of diatomic and triatomic molecules and not well described at the line by line level by atmospheric models. M dwarf metallicities are therefore most commonly derived through less direct techniques. Several recent publications propose calibrations that provide the metallicity of an M dwarf from its Ks band absolute magnitude and its V-Ks color, but disagree at the \pm0.1 dex level. We compare these calibrations on a sample of 23 M dwarfs, which we select as wide (> 5 arcsec) companions of F-, G- or K- dwarfs with metallicities measured on a homogeneous scale, and which we require to have V band photometry measured to better than \sim0.03 magnitude. We find that the Schlaufman & Laughlin (2010) calibration has lowest offsets and residuals against our sample, and use our improved statistics to marginally refine that calibration. With more strictly selected photometry than in previous studies, the dispersion around the calibration is well in excess of the [Fe/H] and photometric uncertainties. This suggests that the origin of the remaining dispersion is astrophysical rather than observational., Comment: paper accepted in A&A, 12 pages, 3 figures; A&A REF: AA/2011/18115

Published
2011
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34. Ultra Steep Spectrum radio sources in the Lockman Hole: SERVS identifications and redshift distribution at the faintest radio fluxes

Author

Afonso, J., Bizzocchi, L., Ibar, E., Grossi, M., Simpson, C., Chapman, S., Jarvis, M. J., Rottgering, H., Norris, R. P., Dunlop, J., Ivison, R. J., Messias, H., Pforr, J., Vaccari, M., Seymour, N., Best, P., González-Solares, E., Farrah, D., Fernandes, C. A. C., Huang, J. -S., Lacy, M., Maraston, C., Marchetti, L., Mauduit, J. -C., Oliver, S., Rigopoulou, D., Stanford, S. A., Surace, J., and Zeimann, G.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

Ultra Steep Spectrum (USS) radio sources have been successfully used to select powerful radio sources at high redshifts (z>~2). Typically restricted to large-sky surveys and relatively bright radio flux densities, it has gradually become possible to extend the USS search to sub-mJy levels, thanks to the recent appearance of sensitive low-frequency radio facilities. Here a first detailed analysis of the nature of the faintest USS sources is presented. By using Giant Metrewave Radio Telescope and Very Large Array radio observations of the Lockman Hole at 610 MHz and 1.4 GHz, a sample of 58 USS sources, with 610 MHz integrated fluxes above 100 microJy, is assembled. Deep infrared data at 3.6 and 4.5 micron from the Spitzer Extragalactic Representative Volume Survey (SERVS) is used to reliably identify counterparts for 48 (83%) of these sources, showing an average total magnitude of [3.6](AB)=19.8 mag. Spectroscopic redshifts for 14 USS sources, together with photometric redshift estimates, improved by the use of the deep SERVS data, for a further 19 objects, show redshifts ranging from z=0.1 to z=2.8, peaking at z~0.6 and tailing off at high redshifts. The remaining 25 USS sources, with no redshift estimate, include the faintest [3.6] magnitudes, with 10 sources undetected at 3.6 and 4.5 micron (typically [3.6]>22-23 mag, from local measurements), which suggests the likely existence of higher redshifts among the sub-mJy USS population. The comparison with the Square Kilometre Array Design Studies Simulated Skies models indicate that Fanaroff-Riley type I radio sources and radio-quiet Active Galactic Nuclei may constitute the bulk of the faintest USS population, and raises the possibility that the high efficiency of the USS technique for the selection of high redshift sources remains even at the sub-mJy level., Comment: Accepted for publication in the Astrophysical Journal. 33 pages, 8 figures, 3 tables. v2: Corrected typos

Published
2011
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35. Using Dissortative Mating Genetic Algorithms to Track the Extrema of Dynamic Deceptive Functions

Author

Fernandes, C. M., Merelo, J. J., and Rosa, A. C.

Subjects
Computer Science - Neural and Evolutionary Computing
Abstract

Traditional Genetic Algorithms (GAs) mating schemes select individuals for crossover independently of their genotypic or phenotypic similarities. In Nature, this behaviour is known as random mating. However, non-random schemes - in which individuals mate according to their kinship or likeness - are more common in natural systems. Previous studies indicate that, when applied to GAs, negative assortative mating (a specific type of non-random mating, also known as dissortative mating) may improve their performance (on both speed and reliability) in a wide range of problems. Dissortative mating maintains the genetic diversity at a higher level during the run, and that fact is frequently observed as an explanation for dissortative GAs ability to escape local optima traps. Dynamic problems, due to their specificities, demand special care when tuning a GA, because diversity plays an even more crucial role than it does when tackling static ones. This paper investigates the behaviour of dissortative mating GAs, namely the recently proposed Adaptive Dissortative Mating GA (ADMGA), on dynamic trap functions. ADMGA selects parents according to their Hamming distance, via a self-adjustable threshold value. The method, by keeping population diversity during the run, provides an effective means to deal with dynamic problems. Tests conducted with deceptive and nearly deceptive trap functions indicate that ADMGA is able to outperform other GAs, some specifically designed for tracking moving extrema, on a wide range of tests, being particularly effective when speed of change is not very fast. When comparing the algorithm to a previously proposed dissortative GA, results show that performance is equivalent on the majority of the experiments, but ADMGA performs better when solving the hardest instances of the test set., Comment: Technical report complementing Carlos Fernandes' PhD

Published
2009

37. Superlens made of a metamaterial with extreme effective parameters

Author

Silveirinha, M. G., Fernandes, C. A., and Costa, J. R.

Subjects
Condensed Matter - Materials Science
Abstract

We propose a superlens formed by an ultra-dense array of crossed metallic wires. It is demonstrated that due to the anomalous interaction between crossed wires, the structured substrate is characterized by an anomalously high index of refraction and supports strongly confined guided modes with very short propagation wavelengths. It is theoretically proven that a planar slab of such structured material makes a superlens that may compensate for the attenuation introduced by free-space propagation and restore the subwavelength details of the source. The bandwidth of the proposed device can be quite significant since the response of the structured substrate is non-resonant. The theoretical results are fully supported by numerical simulations., Comment: Accepted for publication in Phys. Rev. B (in press)

Published
2008
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38. Experimental Demonstration of a Structured Material with Extreme Effective Parameters at Microwaves

Author

Silveirinha, M. G., Fernandes, C. A., Costa, J. R., and Medeiros, C. R.

Subjects
Condensed Matter - Materials Science
Abstract

Following our recent theoretical studies [M. G. Silveirinha, C. A. Fernandes, Phys. Rev. B, 78, 033108, 2008], it is experimentally verified that an array of crossed metallic wires may behave as a nonresonant material with extremely large index of refraction at microwaves, and may enable the realization of ultra-subwavelength waveguides., Comment: accepted for publication in Applied Physics Letters (in press). Applied Physics Letters (in press) (2008)

Published
2008
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39. The extreme, red afterglow of GRB 060923A: Distance or dust?

Author

Tanvir, N. R., Levan, A. J., Rol, E., Starling, R. L. C., Gorosabel, J., Priddey, R. S., Malesani, D., Jakobsson, P., O'Brien, P. T., Jaunsen, A. O., Hjorth, J., Fynbo, J. P. U., Melandri, A., Gomboc, A., Milvang-Jensen, B., Fruchter, A. S., Jarvis, M., Fernandes, C. A. C., and Wold, T.

Subjects
Astrophysics
Abstract

Gamma-ray bursts are powerful probes of the early universe, but locating and identifying very distant GRBs remains challenging. We report here the discovery of the K-band afterglow of Swift GRB 060923A, imaged within the first hour post-burst, and the faintest so far found. It was not detected in any bluer bands to deep limits, making it a candidate very high redshift burst (z>11). However, our later-time optical imaging and spectroscopy reveal a faint galaxy coincident with the GRB position which, if it is the host, implies a more moderate redshift (most likely z<2.8) and therefore that dust is the likely cause of the very red afterglow colour. This being the case, it is one of the few instances so far found of a GRB afterglow with high dust extinction., Comment: Submitted to MNRAS (revised in light of referee's comments)

Published
2008
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40. KohonAnts: A Self-Organizing Ant Algorithm for Clustering and Pattern Classification

Author

Fernandes, C., Mora, A. M., Merelo, J. J., Ramos, V., and Laredo, J. L. J.

Subjects
Computer Science - Neural and Evolutionary Computing, Computer Science - Computer Vision and Pattern Recognition
Abstract

In this paper we introduce a new ant-based method that takes advantage of the cooperative self-organization of Ant Colony Systems to create a naturally inspired clustering and pattern recognition method. The approach considers each data item as an ant, which moves inside a grid changing the cells it goes through, in a fashion similar to Kohonen's Self-Organizing Maps. The resulting algorithm is conceptually more simple, takes less free parameters than other ant-based clustering algorithms, and, after some parameter tuning, yields very good results on some benchmark problems., Comment: Submitted to ALIFE XI

Published
2008

41. The log-periodic-AR(1)-GARCH(1,1) model for financial crashes

Author

Gazola, L., Fernandes, C., Pizzinga, A., and Riera, R.

Subjects
Quantitative Finance - Statistical Finance, Physics - Data Analysis, Statistics and Probability, Physics - Physics and Society
Abstract

This paper intends to meet recent claims for the attainment of more rigorous statistical methodology within the econophysics literature. To this end, we consider an econometric approach to investigate the outcomes of the log-periodic model of price movements, which has been largely used to forecast financial crashes. In order to accomplish reliable statistical inference for unknown parameters, we incorporate an autoregressive dynamic and a conditional heteroskedasticity structure in the error term of the original model, yielding the log-periodic-AR(1)-GARCH(1,1) model. Both the original and the extended models are fitted to financial indices of U. S. market, namely S&P500 and NASDAQ. Our analysis reveal two main points: (i) the log-periodic-AR(1)-GARCH(1,1) model has residuals with better statistical properties and (ii) the estimation of the parameter concerning the time of the financial crash has been improved., Comment: 17 pages, 4 figures, 12 tables, to appear in Europen Physical Journal B

Published
2008
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43. Computational Chemotaxis in Ants and Bacteria over Dynamic Environments

Author

Ramos, Vitorino, Fernandes, C. M., Rosa, A. C., and Abraham, A.

Subjects
Computer Science - Multiagent Systems, Computer Science - Artificial Intelligence, Quantitative Biology - Populations and Evolution, Quantitative Biology - Quantitative Methods, I.2, I.2.11, G.1.6
Abstract

Chemotaxis can be defined as an innate behavioural response by an organism to a directional stimulus, in which bacteria, and other single-cell or multicellular organisms direct their movements according to certain chemicals in their environment. This is important for bacteria to find food (e.g., glucose) by swimming towards the highest concentration of food molecules, or to flee from poisons. Based on self-organized computational approaches and similar stigmergic concepts we derive a novel swarm intelligent algorithm. What strikes from these observations is that both eusocial insects as ant colonies and bacteria have similar natural mechanisms based on stigmergy in order to emerge coherent and sophisticated patterns of global collective behaviour. Keeping in mind the above characteristics we will present a simple model to tackle the collective adaptation of a social swarm based on real ant colony behaviors (SSA algorithm) for tracking extrema in dynamic environments and highly multimodal complex functions described in the well-know De Jong test suite. Later, for the purpose of comparison, a recent model of artificial bacterial foraging (BFOA algorithm) based on similar stigmergic features is described and analyzed. Final results indicate that the SSA collective intelligence is able to cope and quickly adapt to unforeseen situations even when over the same cooperative foraging period, the community is requested to deal with two different and contradictory purposes, while outperforming BFOA in adaptive speed. Results indicate that the present approach deals well in severe Dynamic Optimization problems., Comment: 8 pages, 6 figures, in CEC 07 - IEEE Congress on Evolutionary Computation, ISBN 1-4244-1340-0, pp. 1009-1017, Sep. 2007

Published
2007
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45. Physical, chemical and mechanical properties of Pinus sylvestris wood at five sites in Portugal

Author

Fernandes C, Gaspar MJ, Pires J, Alves A, Simões R, Rodrigues JC, Silva Maria E, Carvalho A, Brito José E, and Lousada José L

Subjects
Bending Tests, Correlations, Mechanical Traits, NIR Spectrometry, Scots Pine, Wood-Density Components, Wood Quality, X-ray Microdensitometry, Forestry, SD1-669.5
Abstract

The reduction of resinous species in Portuguese forest areas has caused constraints to wood industry supplies. Portugal represents the extreme southwest of Scots pine (Pinus sylvestris) natural distribution and large gaps exist in the knowledge of its wood-quality characteristics. Understanding the relationship between these traits is important for recognizing which combination of wood properties is the most suitable for specific uses. To address these questions, we assessed wood-quality traits, namely, wood-density components (microdensitometric analysis), chemical composition (NIR spectrometry) and mechanical properties (bending tests) of wood samples collected at five representative forest sites in Portugal. Our results showed that Portuguese Pinus sylvestris has good radial growth and denser wood, higher extractive content and higher stiffness and strength than northern European provenances. The lignin content was within the range attributed to softwoods. Among the Portuguese stands, trees growing at lower-altitude sites exhibited denser wood and higher mechanical properties, while trees from high-elevations showed higher amounts of lignin. Ring density was more strongly correlated with earlywood than latewood density. A negative, non-significant correlation was found between ring density and width, supporting the assumption that the higher radial growth (ring width) does not negatively affect wood quality (density). In general, chemical properties had a weak relationship with physical and mechanical properties (MOE and MOR). Both mechanical traits were positively correlated with density and growth components, supporting the assumption that trees with high radial growth do not exhibit poorer mechanical performances.

Published
2017
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46. A importância da abordagem familiar no tratamento dos transtornos alimentares

Author

Adriana Fernandes C. Dáquer, Monica Duchesne, and Cristiane Simão

Subjects
Transtornos alimentares, terapia de família, FBT, terapia familiar sistêmica, Psychiatry, RC435-571
Abstract

Os transtornos alimentares (TA) se caracterizam por comportamentos alimentares inadequados, que prejudicam a saúde física, interferem nas relações psicossociais do indivíduo e causam impacto negativo nas relações familiares e sobre os cuidadores. Uma vez que a faixa etária mais comum de início dos sintomas corresponde à adolescência e ao início da vida adulta, o sistema familiar possui potencial terapêutico e pode contribuir para a manutenção dos ganhos obtidos. Por isso, vários estudos se concentram em intervenções com a participação da família. Inicialmente, as terapias familiares para TA focaram a atenção na anorexia nervosa (AN), em virtude de sua maior gravidade. Com o tempo, as abordagens exitosas têm sido adaptadas ao tratamento de outros TA, tais como a bulimia nervosa (BN) e o transtorno alimentar restritivo evitativo (TARE). Atualmente, o family-based treatment (FBT) é considerado padrão-ouro em inclusão familiar no contexto do tratamento dos TA, com amplas evidências indicando os seus resultados. Neste artigo, além do FBT, abordaremos a terapia familiar sistêmica, focando nas mudanças da dinâmica familiar.

Published
2019
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47. Erratum to: Insight into particle production mechanisms via angular correlations of identified particles in pp collisions at s=7 TeV

Author

Adam, J., Adamová, D., Aggarwal, M. M., Rinella, G. Aglieri, Agnello, M., Agrawal, N., Ahammed, Z., Ahmad, S., Ahn, S. U., Aiola, S., Akindinov, A., Alam, S. N., Albuquerque, D. S. D., Aleksandrov, D., Alessandro, B., Alexandre, D., Molina, R. Alfaro, Alici, A., Alkin, A., Alme, J., Alt, T., Altinpinar, S., Altsybeev, I., Prado, C. Alves Garcia, An, M., Andrei, C., Andrews, H. A., Andronic, A., Anguelov, V., Anson, C., Antičić, T., Antinori, F., Antonioli, P., Anwar, R., Aphecetche, L., Appelshäuser, H., Arcelli, S., Arnaldi, R., Arnold, O. W., Arsene, I. C., Arslandok, M., Audurier, B., Augustinus, A., Averbeck, R., Azmi, M. D., Badalà, A., Baek, Y. W., Bagnasco, S., Bailhache, R., Bala, R., Baldisseri, A., Baral, R. C., Barbano, A. M., Barbera, R., Barile, F., Barioglio, L., Barnaföldi, G. G., Barnby, L. S., Barret, V., Bartalini, P., Barth, K., Bartke, J., Bartsch, E., Basile, M., Bastid, N., Basu, S., Bathen, B., Batigne, G., Camejo, A. Batista, Batyunya, B., Batzing, P. C., Bearden, I. G., Beck, H., Bedda, C., Behera, N. K., Belikov, I., Bellini, F., Martinez, H. Bello, Bellwied, R., Beltran, L. G. E., Belyaev, V., Bencedi, G., Beole, S., Bercuci, A., Berdnikov, Y., Berenyi, D., Bertens, R. A., Berzano, D., Betev, L., Bhasin, A., Bhat, I. R., Bhati, A. K., Bhattacharjee, B., Bhom, J., Bianchi, L., Bianchi, N., Bianchin, C., Bielčík, J., Bielčíková, J., Bilandzic, A., Biro, G., Biswas, R., Biswas, S., Blair, J. T., Blau, D., Blume, C., Bock, F., Bogdanov, A., Boldizsár, L., Bombara, M., Bonora, M., Book, J., Borel, H., Borissov, A., Borri, M., Botta, E., Bourjau, C., Braun-Munzinger, P., Bregant, M., Broker, T. A., Browning, T. A., Broz, M., Brucken, E. J., Bruna, E., Bruno, G. E., Budnikov, D., Buesching, H., Bufalino, S., Buhler, P., Buitron, S. A. I., Buncic, P., Busch, O., Buthelezi, Z., Butt, J. B., Buxton, J. T., Cabala, J., Caffarri, D., Caines, H., Caliva, A., Villar, E. Calvo, Camerini, P., Capon, A. A., Carena, F., Carena, W., Carnesecchi, F., Castellanos, J. Castillo, Castro, A. J., Casula, E. A. R., Sanchez, C. Ceballos, Cerello, P., Cerkala, J., Chang, B., Chapeland, S., Chartier, M., Charvet, J. L., Chattopadhyay, S., Chattopadhyay, S., Chauvin, A., Cherney, M., Cheshkov, C., Cheynis, B., Barroso, V. Chibante, Chinellato, D. D., Cho, S., Chochula, P., Choi, K., Chojnacki, M., Choudhury, S., Christakoglou, P., Christensen, C. H., Christiansen, P., Chujo, T., Chung, S. U., Cicalo, C., Cifarelli, L., Cindolo, F., Cleymans, J., Colamaria, F., Colella, D., Collu, A., Colocci, M., Balbastre, G. Conesa, Valle, Z. Conesa del, Connors, M. E., Contreras, J. G., Cormier, T. M., Morales, Y. Corrales, Maldonado, I. Cortés, Cortese, P., Cosentino, M. R., Costa, F., Crkovská, J., Crochet, P., Albino, R. Cruz, Cuautle, E., Cunqueiro, L., Dahms, T., Dainese, A., Danisch, M. C., Danu, A., Das, D., Das, I., Das, S., Dash, A., Dash, S., De, S., De Caro, A., de Cataldo, G., de Conti, C., de Cuveland, J., De Falco, A., De Gruttola, D., De Marco, N., De Pasquale, S., De Souza, R. D., Degenhardt, H. F., Deisting, A., Deloff, A., Deplano, C., Dhankher, P., Di Bari, D., Di Mauro, A., Di Nezza, P., Di Ruzza, B., Corchero, M. A. Diaz, Dietel, T., Dillenseger, P., Divià, R., Djuvsland, Ø., Dobrin, A., Gimenez, D. Domenicis, Dönigus, B., Dordic, O., Drozhzhova, T., Dubey, A. K., Dubla, A., Ducroux, L., Duggal, A. K., Dupieux, P., Ehlers, R. J., Elia, D., Endress, E., Engel, H., Epple, E., Erazmus, B., Erhardt, F., Espagnon, B., Esumi, S., Eulisse, G., Eum, J., Evans, D., Evdokimov, S., Fabbietti, L., Fabris, D., Faivre, J., Fantoni, A., Fasel, M., Feldkamp, L., Feliciello, A., Feofilov, G., Ferencei, J., Téllez, A. Fernández, Ferreiro, E. G., Ferretti, A., Festanti, A., Feuillard, V. J. G., Figiel, J., Figueredo, M. A. S., Filchagin, S., Finogeev, D., Fionda, F. M., Fiore, E. M., Floris, M., Foertsch, S., Foka, P., Fokin, S., Fragiacomo, E., Francescon, A., Francisco, A., Frankenfeld, U., Fronze, G. G., Fuchs, U., Furget, C., Furs, A., Girard, M. Fusco, Gaardhøje, J. J., Gagliardi, M., Gago, A. M., Gajdosova, K., Gallio, M., Galvan, C. D., Gangadharan, D. R., Ganoti, P., Gao, C., Garabatos, C., Garcia-Solis, E., Garg, K., Garg, P., Gargiulo, C., Gasik, P., Gauger, E. F., Ducati, M. B. Gay, Germain, M., Ghosh, P., Ghosh, S. K., Gianotti, P., Giubellino, P., Giubilato, P., Gladysz-Dziadus, E., Glässel, P., Coral, D. M. Goméz, Ramirez, A. Gomez, Gonzalez, A. S., Gonzalez, V., González-Zamora, P., Gorbunov, S., Görlich, L., Gotovac, S., Grabski, V., Graczykowski, L. K., Graham, K. L., Greiner, L., Grelli, A., Grigoras, C., Grigoriev, V., Grigoryan, A., Grigoryan, S., Grion, N., Gronefeld, J. M., Grosa, F., Grosse-Oetringhaus, J. F., Grosso, R., Gruber, L., Grull, F. R., Guber, F., Guernane, R., Guerzoni, B., Gulbrandsen, K., Gunji, T., Gupta, A., Gupta, R., Guzman, I. B., Haake, R., Hadjidakis, C., Hamagaki, H., Hamar, G., Hamon, J. C., Harris, J. W., Harton, A., Hatzifotiadou, D., Hayashi, S., Heckel, S. T., Hellbär, E., Helstrup, H., Herghelegiu, A., Corral, G. Herrera, Herrmann, F., Hess, B. A., Hetland, K. F., Hillemanns, H., Hippolyte, B., Hladky, J., Horak, D., Hosokawa, R., Hristov, P., Hughes, C., Humanic, T. J., Hussain, N., Hussain, T., Hutter, D., Hwang, D. S., Ilkaev, R., Inaba, M., Ippolitov, M., Irfan, M., Isakov, V., Islam, M. S., Ivanov, M., Ivanov, V., Izucheev, V., Jacak, B., Jacazio, N., Jacobs, P. M., Jadhav, M. B., Jadlovska, S., Jadlovsky, J., Jahnke, C., Jakubowska, M. J., Janik, M. A., Jayarathna, P. H. S. Y., Jena, C., Jena, S., Jercic, M., Bustamante, R. T. Jimenez, Jones, P. G., Jusko, A., Kalinak, P., Kalweit, A., Kang, J. H., Kaplin, V., Kar, S., Uysal, A. 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2019
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49. Relative particle yield fluctuations in Pb--PbsNN=2.76TeV collisions at Pb--PbsNN=2.76TeV

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Acharya, S., Adamová, D., Adolfsson, J., Aggarwal, M. M., Aglieri Rinella, G., Agnello, M., Agrawal, N., Ahammed, Z., Ahn, S. U., Aiola, S., Akindinov, A., Al-Turany, M., Alam, S. N., Albuquerque, D. S. D., Aleksandrov, D., Alessandro, B., Molina, R. Alfaro, Ali, Y., Alici, A., Alkin, A., Alme, J., Alt, T., Altenkamper, L., Altsybeev, I., Prado, C. Alves Garcia, Andrei, C., Andreou, D., Andrews, H. A., Andronic, A., Anguelov, V., Anson, C., Antičić, T., Antinori, F., Antonioli, P., Aphecetche, L., Appelshäuser, H., Arcelli, S., Arnaldi, R., Arnold, O. W., Arsene, I. C., Arslandok, M., Audurier, B., Augustinus, A., Averbeck, R., Azmi, M. D., Badalà, A., Baek, Y. W., Bagnasco, S., Bailhache, R., Bala, R., Baldisseri, A., Ball, M., Baral, R. C., Barbano, A. M., Barbera, R., Barile, F., Barioglio, L., Barnaföldi, G. G., Barnby, L. S., Barret, V., Bartalini, P., Barth, K., Bartsch, E., Bastid, N., Basu, S., Batigne, G., Batyunya, B., Batzing, P. C., BazoAlba, J. L., Bearden, I. G., Beck, H., Bedda, C., Behera, N. K., Belikov, I., Bellini, F., Bello Martinez, H., Bellwied, R., Beltran, L. G. E., Belyaev, V., Bencedi, G., Beole, S., Bercuci, A., Berdnikov, Y., Berenyi, D., Bertens, R. A., Berzano, D., Betev, L., Bhasin, A., Bhat, I. R., Bhattacharjee, B., Bhom, J., Bianchi, A., Bianchi, L., Bianchi, N., Bianchin, C., Bielčík, J., Bielčíková, J., Bilandzic, A., Biro, G., Biswas, R., Biswas, S., Blair, J. T., Blau, D., Blume, C., Boca, G., Bock, F., Bogdanov, A., Boldizsár, L., Bombara, M., Bonomi, G., Bonora, M., Book, J., Borel, H., Borissov, A., Borri, M., Botta, E., Bourjau, C., Bratrud, L., Braun-Munzinger, P., Bregant, M., Broker, T. A., Broz, M., Brucken, E. J., Bruna, E., Bruno, G. E., Budnikov, D., Buesching, H., Bufalino, S., Buhler, P., Buncic, P., Busch, O., Buthelezi, Z., Butt, J. B., Buxton, J. T., Cabala, J., Caffarri, D., Caines, H., Caliva, A., Villar, E. Calvo, Camerini, P., Capon, A. 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2019
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