10,601 results on '"Calabro A."'
Search Results
202. Management of high and intermediate-high risk pulmonary embolism: A position paper of the Interventional Cardiology Working Group of the Italian Society of Cardiology
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Andò, Giuseppe, Pelliccia, Francesco, Saia, Francesco, Tarantini, Giuseppe, Fraccaro, Chiara, D'Ascenzo, Fabrizio, Zimarino, Marco, Di Marino, Mario, Niccoli, Giampaolo, Porto, Italo, Calabrò, Paolo, Gragnano, Felice, De Rosa, Salvatore, Piccolo, Raffaele, Moscarella, Elisabetta, Fabris, Enrico, Montone, Rocco Antonio, Spaccarotella, Carmen, Indolfi, Ciro, Sinagra, Gianfranco, and Perrone Filardi, Pasquale
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- 2024
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203. A 35-year monitoring of an Italian landfill: Effect of recirculation of reverse osmosis concentrate on leachate characteristics
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Folino, A., Gentili, E., Komilis, D., and Calabrò, P.S.
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- 2024
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204. Preliminary thermal and structural analyses on the parabolic mirror of the Multi-Beam Transmission Line of the DTT ECH system
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Salvitti, A., Bruschi, A., Calabrò, G., Fanale, F., Fanelli, P., Garavaglia, S., Giorgetti, F., Granucci, G., Moro, A., Platania, P., and Romano, A.
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- 2024
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205. Nivolumab plus ipilimumab in melanoma patients with asymptomatic brain metastases: 7-year outcomes and quality of life from the multicenter phase III NIBIT-M2 trial
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Di Giacomo, Anna Maria, Chiarion-Sileni, Vanna, Del Vecchio, Michele, Ferrucci, Pier Francesco, Guida, Michele, Quaglino, Pietro, Guidoboni, Massimo, Marchetti, Paolo, Simonetti, Elena, Santangelo, Federica, Amato, Giovanni, Covre, Alessia, Camerini, Roberto, Valente, Monica, Mandalà, Mario, Giannarelli, Diana, Calabrò, Luana, and Maio, Michele
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- 2024
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206. Extracorporeal cardiopulmonary resuscitation for refractory out-of-hospital cardiac arrest: 10-year experience in a metropolitan cardiac arrest centre in Milan, Italy
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Crivellari, Martina, De Luca, Monica, Fano, Greta, Frau, Giovanna, Oriani, Alessandro, Gerli, Chiara, Mucchetti, Marta, Belletti, Alessandro, Barucco, Gaia, Di Prima, Ambra Licia, Licheri, Margherita, Zarantonello, Sabrina, Turla, Giancarlo Otello, Francescon, Claudia, Scquizzato, Tommaso, Calabrò, Maria Grazia, Franco, Annalisa, Fominskiy, Evgeny, Pieri, Marina, Nardelli, Pasquale, Delrio, Silvia, Altizio, Savino, Ortalda, Alessandro, Melisurgo, Giulio, Ajello, Silvia, Landoni, Giovanni, Zangrillo, Alberto, and Scandroglio, Anna Mara
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- 2024
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207. Tracing the history of past treatments: A multi-analytical study of a 16th-century panel painting copy after Raphael
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Cavaleri, Tiziana, Pelosi, Claudia, Caliri, Claudia, Romano, Paolo Francesco, Colantonio, Claudia, Lanteri, Luca, Calabrò, Giuseppe, Piccirillo, Anna, Ventura, Bernadette, De Blasi, Stefania, Riedo, Chiara, and Scalarone, Dominique
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- 2024
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208. The role of turbulence in the deposition of intrinsically buoyant MPs
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Molazadeh, Marziye, Calabro, Guilherme, Liu, Fan, Tassin, Bruno, Rovelli, Lorenzo, Lorke, Andreas, Dris, Rachid, and Vollertsen, Jes
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- 2024
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209. Remediation of groundwater pollution using photocatalytic membrane reactors
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Bhattacharyya, Saurav, Algieri, Catia, Donato, Laura, Davoli, Mariano, Chakraborty, Sudip, and Calabrò, Vincenza
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- 2024
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210. Real-world Outcome of Patients with Advanced Renal Cell Carcinoma and Intermediate- or Poor-risk International Metastatic Renal Cell Carcinoma Database Consortium Criteria Treated by Immune-oncology Combinations: Differential Effectiveness by Risk Group?
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Santoni, Matteo, Buti, Sebastiano, Myint, Zin W., Maruzzo, Marco, Iacovelli, Roberto, Pichler, Martin, Kopecky, Jindrich, Kucharz, Jakub, Rizzo, Mimma, Galli, Luca, Büttner, Thomas, De Giorgi, Ugo, Kanesvaran, Ravindran, Fiala, Ondřej, Grande, Enrique, Zucali, Paolo Andrea, Kopp, Ray Manneh, Fornarini, Giuseppe, Bourlon, Maria T., Scagliarini, Sarah, Molina-Cerrillo, Javier, Aurilio, Gaetano, Matrana, Marc R., Pichler, Renate, Cattrini, Carlo, Büchler, Tomas, Massari, Francesco, Seront, Emmanuel, Calabrò, Fabio, Pinto, Alvaro, Berardi, Rossana, Zgura, Anca, Mammone, Giulia, Ansari, Jawaher, Atzori, Francesco, Chiari, Rita, Bamias, Aristotelis, Caffo, Orazio, Procopio, Giuseppe, Sunela, Kaisa, Bassanelli, Maria, Ortega, Cinzia, Grillone, Francesco, Landmesser, Johannes, Milella, Michele, Messina, Carlo, Küronya, Zsófia, Mosca, Alessandra, Bhuva, Dipen, Santini, Daniele, Vau, Nuno, Morelli, Franco, Incorvaia, Lorena, Rebuzzi, Sara Elena, Roviello, Giandomenico, Soares, Andrey, Bisonni, Renato, Bimbatti, Davide, Zabalza, Ignacio Ortego, Rizzo, Alessandro, Mollica, Veronica, Sorgentoni, Giulia, Monteiro, Fernando Sabino M., Battelli, Nicola, Bracarda, Sergio, and Porta, Camillo
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- 2024
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211. PAM-6 Coded Modulation for IM/DD Channels with a Peak-Power Constraint
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Prinz, Tobias, Wiegart, Thomas, Plabst, Daniel, Calabrò, Stefano, Böcherer, Georg, Stojanovic, Nebojsa, and Rahman, Talha
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Computer Science - Information Theory - Abstract
Coded modulation with probabilistic amplitude shaping (PAS) is considered for intensity modulation/direct detection channels with a transmitter peak-power constraint. PAS is used to map bits to a uniform PAM-6 distribution and outperforms PAM-8 for rates up to around 2.3 bits per channel use. PAM-6 with PAS also outperforms a cross-shaped QAM-32 constellation by up to 1 dB and 0.65 dB after bit-metric soft- and hard decoding, respectively. An alternative PAM-6 scheme based on a framed cross-shaped QAM-32 constellation is proposed that shows similar gains., Comment: submitted to 11th International Symposium on Topics in Coding
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- 2021
212. The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model
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Fontanot, Fabio, Calabrò, Antonello, Talia, Margherita, Mannucci, Filippo, Castellano, Marco, Cresci, Giovanni, De Lucia, Gabriella, Gallazzi, Anna, Hirschmann, Michaela, Pentericci, Laura, Xie, Lizhi, Amorin, Ricardo, Bolzonella, Micol, Bongiorno, Angela, Cucciati, Olga, Cullen, Fergus, Fynbo, Johan P. U., Hathi, Nimish, Hibon, Pascale, McLure, Ross J., and Pozzetti, Lucia
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In this work, we study the evolution of the mass-metallicity relations (MZRs) as predicted by the GAlaxy Evolution and Assembly (GAEA) semi-analytic model. We contrast these predictions with recent results from the VANDELS survey, that allows us to expand the accessible redshift range for the stellar MZR up to $z\sim3.5$. We complement our study by considering the evolution of the gas-phase MZR in the same redshift range. We show that GAEA is able to reproduce the observed evolution of the $z<3.5$ gas-phase MZR and $z<0.7$ stellar MZR, while it overpredicts the stellar metallicity at $z\sim3.5$. Furthermore, GAEA also reproduces the so-called fundamental metallicity relation (FMR) between gas-phase metallicity, stellar mass and star formation rate (SFR). In particular, the gas-phase FMR in GAEA is already in place at $z\sim5$ and shows almost no evolution at lower redshift. GAEA predicts the existence of a stellar FMR, that is, however, characterized by a relevant redshift evolution, although its shape follows closely the gas-phase FMR. We also report additional unsolved tensions between model and data: the overall normalization of the predicted MZR agrees with observations only within $\sim$0.1 dex; the largest discrepancies are seen at $z\sim3.5$ where models tend to slightly overpredict observed metallicities; the slope of the predicted MZR at fixed SFR is too steep below a few ${\rm M}_\odot\ {\rm yr}^{-1}$. Finally, we provide model predictions for the evolution of the MZRs at higher redshifts, that would be useful in the context of future surveys, like those that will be performed with JWST., Comment: 12 pages, 8 figures, MNRAS accepted, replaced to match the published version
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- 2021
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213. Numerical Solution and Bifurcation Analysis of Nonlinear Partial Differential Equations with Extreme Learning Machines
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Fabiani, Gianluca, Calabrò, Francesco, Russo, Lucia, and Siettos, Constantinos
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Mathematics - Numerical Analysis ,Mathematics - Analysis of PDEs ,Mathematics - Dynamical Systems ,65-XX, 65Nxx, 65-XX, 65P30 - Abstract
We address a new numerical scheme based on a class of machine learning methods, the so-called Extreme Learning Machines with both sigmoidal and radial-basis functions, for the computation of steady-state solutions and the construction of (one dimensional) bifurcation diagrams of nonlinear partial differential equations (PDEs). For our illustrations, we considered two benchmark problems, namely (a) the one-dimensional viscous Burgers with both homogeneous (Dirichlet) and non-homogeneous mixed boundary conditions, and, (b) the one and two-dimensional Liouville-Bratu-Gelfand PDEs with homogeneous Dirichlet boundary conditions. For the one-dimensional Burgers and Bratu PDEs, exact analytical solutions are available and used for comparison purposes against the numerical derived solutions. Furthermore, the numerical efficiency (in terms of accuracy and size of the grid) of the proposed numerical machine learning scheme is compared against central finite differences (FD) and Galerkin weighted-residuals finite-element methods (FEM). We show that the proposed ELM numerical method outperforms both FD and FEM methods for medium to large sized grids, while provides equivalent results with the FEM for low to medium sized grids.
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- 2021
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214. The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
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Saxena, A., Ellis, R. S., Forster, P. U., Calabro, A., Pentericci, L., Carnall, A. C., Castellano, M., Cullen, F., Fontana, A., Franco, M., Fynbo, J. P. U., Gargiulo, A., Garilli, B., Hathi, N. P., McLeod, D. J., Amorin, R., and Zamorani, G.
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Astrophysics - Astrophysics of Galaxies - Abstract
We use VANDELS spectroscopic data overlapping with the $\simeq$7 Ms Chandra Deep Field South survey to extend studies of high-mass X-ray binary systems (XRBs) in 301 normal star-forming galaxies in the redshift range $3 < z < 5.5$. Our analysis evaluates correlations between X-ray luminosities ($L_X$), star formation rates (SFR) and stellar metallicities ($Z_\star$) to higher redshifts and over a wider range in galaxy properties than hitherto. Using a stacking analysis performed in bins of both redshift and SFR for sources with robust spectroscopic redshifts without AGN signatures, we find convincing evolutionary trends in the ratio $L_X$/SFR to the highest redshifts probed, with a stronger trend for galaxies with lower SFRs. Combining our data with published samples at lower redshift, the evolution of $L_X$/SFR to $z\simeq5$ proceeds as $(1 + z)^{1.03 \pm 0.02}$. Using stellar metallicities derived from photospheric absorption features in our spectroscopic data, we confirm indications at lower redshifts that $L_X$/SFR is stronger for metal-poor galaxies. We use semi-analytic models to show that metallicity dependence of $L_X$/SFR alone may not be sufficient to fully explain the observed redshift evolution of X-ray emission from high-mass XRBs, particularly for galaxies with SFR $<30$ $M_\odot$ yr$^{-1}$. We speculate that the discrepancy may arise due to reduced overall stellar ages in the early Universe leading to higher $L_X$/SFR for the same metallicity. We use our data to define the redshift-dependent contribution of XRBs to the integrated X-ray luminosity density and, in comparison with models, find that the contribution of high-mass XRBs to the cosmic X-ray background at $z>6$ may be $\gtrsim 0.25$ dex higher than previously estimated., Comment: 16 pages, 10 figures, Published in MNRAS
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- 2021
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215. The ASTRODEEP-GS43 catalogue: new photometry and redshifts for the CANDELS GOODS-South field
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Merlin, E., Castellano, M., Santini, P., Cipolletta, G., Boutsia, K., Schreiber, C., Buitrago, F., Fontana, A., Elbaz, D., Dunlop, J., Grazian, A., McLure, R., McLeod, D., Nonino, M., Milvang-Jensen, B., Derriere, S., Hathi, N. P., Pentericci, L., Fortuni, F., and Calabrò, A.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
We present ASTRODEEP-GS43, a new multiwavelength photometric catalogue of the GOODS-South field, which builds and improves upon the previously released CANDELS catalogue. We provide photometric fluxes and corresponding uncertainties in 43 optical and infrared bands (25 wide and 18 medium filters), as well as photometric redshifts and physical properties of the 34930 CANDELS $H$-detected objects, plus an additional sample of 178 $H$-dropout sources, of which 173 are $Ks$-detected and 5 IRAC-detected. We keep the CANDELS photometry in 7 bands (CTIO $U$, Hubble Space Telescope WFC3 and ISAAC-$K$), and measure from scratch the fluxes in the other 36 (VIMOS, HST ACS, HAWK-I $Ks$, Spitzer IRAC, and 23 from Subaru SuprimeCAM and Magellan-Baade Fourstar) with state-of-the-art techniques of template-fitting. We then compute new photometric redshifts with three different software tools, and take the median value as best estimate. We finally evaluate new physical parameters from SED fitting, comparing them to previously published ones. Comparing to a sample of 3931 high quality spectroscopic redshifts, for the new photo-$z$'s we obtain a normalized median absolute deviation (NMAD) of 0.015 with 3.01$\%$ of outliers (0.011, 0.22$\%$ on the bright end at $I814$<22.5), similarly to the best available published samples of photometric redshifts, such as the COSMOS UltraVISTA catalogue. The ASTRODEEP-GS43 results are in qualitative agreement with previously published catalogues of the GOODS-South field, improving on them particularly in terms of SED sampling and photometric redshift estimates. The catalogue is available for download from the Astrodeep website., Comment: 15 pages, 14 figures, accepted for publication on A&A
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- 2021
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216. The NIRVANDELS Survey: a robust detection of $\alpha$-enhancement in star-forming galaxies at $z\simeq3.4$
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Cullen, F., Shapley, A. E., McLure, R. J., Dunlop, J. S., Sanders, R. L., Topping, M. W., Reddy, N. A., Amorin, R., Begley, R., Bolzonella, M., Calabro, A., Carnall, A. C., Castellano, M., Cimatti, A., Cirasuolo, M, Cresci, G., Fontana, A., Fontanot, F., Garilli, B., Guaita, L., Hamadouche, M., Hathi, N. P., Mannucci, F., McLeod, D. J., Pentericci, L., Saxena, A., Talia, M., and Zamorani, G.
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Astrophysics - Astrophysics of Galaxies - Abstract
We present results from the NIRVANDELS survey investigating the gas-phase metallicity ($\mathrm{Z}_{\mathrm{gas}}$, tracing O/H) and stellar metallicity ($Z_{\star}$, tracing Fe/H) of 33 star-forming galaxies at redshifts $2.95 < z < 3.80$. Based on a combined analysis of deep optical and near-IR spectra, tracing the rest-frame far ultraviolet and rest-frame optical respectively, we present the first simultaneous determination of the stellar and gas-phase mass-metallicity relationships (MZRs) at $z\simeq3.4$. In both cases, we find that metallicity increases with increasing stellar mass ($M_{\star}$), and that the power-law slope at $M_{\star} \lesssim 10^{10} \mathrm{M}_{\odot}$ of both MZRs scales as $Z \propto M_{\star}^{0.3}$. Comparing the stellar and gas-phase MZRs, we present direct evidence for super-solar O/Fe ratios (i.e., $\alpha$-enhancement) at $z>3$, finding $\mathrm{(O/Fe)}\simeq (2.54 \pm 0.38) \times \mathrm{(O/Fe)}_{\odot}$, with no clear dependence on $M_{\star}$., Comment: 18 pages, 11 figures, MNRAS accepted
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- 2021
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217. The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements
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Garilli, B., McLure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., Cucciati, O., Iovino, A., Amorin, R., Bolzonella, M., Bongiorno, A., Castellano, M., Cimatti, A., Cirasuolo, M., Cullen, F., Dunlop, J., Elbaz, D., Finkelstein, S., Fontana, A., Fontanot, F., Fumana, M., Guaita, L., Hartley, W., Jarvis, M., Juneau, S., Maccagni, D., McLeod, D., Nandra, K., Pompei, E., Pozzetti, L., Scodeggio, M., Talia, M., Calabro', A., Cresci, G., Fynbo, J. P. U., Hathi, N. P., Hibon, P., Koekemoer, A. M., Magliocchetti, M., Salvato, M., Vietri, G., Zamorani, G., Almaini, O., Balestra, I., Bardelli, S., Begley, R., Brammer, G., Bell, E. F., Bowler, R. A. A., Brusa, M., Buitrago, F., Caputi, C., Cassata, P., Charlot, S., Citro, A., Cristiani, S., Curtis-Lake, E., Dickinson, M., Fazio, G., Ferguson, H. C., Fiore, F., Franco, M., Georgakakis, A., Giavalisco, M., Grazian, A., Hamadouche, M., Jung, I., Kim, S., Khusanova, Y., Fevre, O. Le, Longhetti, M., Lotz, J., Mannucci, F., Maltby, D., Matsuoka, K., Mendez-Hernandez, H., Mendez-Abreu, J., Mignoli, M., Moresco, M., Nonino, M., Pannella, M., Papovich, C., Popesso, P., Roberts-Borsani, G., Rosario, D. J., Saldana-Lopez, A., Santini, P., Saxena, A., Schaerer, D., Schreiber, C., Stark, D., Tasca, L. A. M., Thomas, R., Vanzella, E., Wild, V., Williams, C., and Zucca, E.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We give a detailed description of sample selection, observations and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at iAB = 25. The high Signal to Noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5{\AA} allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-IR photometry and physical parameters derived through SED fitting. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range 8.3< Log(M*/Msolar)<11.7. All catalogues and spectra are accessible through the survey database (http://vandels.inaf.it) where all information can be queried interactively, and via the ESO Archive (https://www.eso.org/qi/)., Comment: 16 pages, 13 figures, accepted for publication in Astronomy & Astrophysics
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- 2021
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218. A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4
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Puglisi, Annagrazia, Daddi, Emanuele, Brusa, Marcella, Bournaud, Frederic, Fensch, Jeremy, Liu, Daizhong, Delvecchio, Ivan, Calabrò, Antonello, Circosta, Chiara, Valentino, Francesco, Perna, Michele, Jin, Shuowen, Enia, Andrea, Mancini, Chiara, and Rodighiero, Giulia
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Astrophysics - Astrophysics of Galaxies - Abstract
Feedback-driven winds from star formation or active galactic nuclei might be a relevant channel for the abrupt quenching star formation in massive galaxies. However, both observations and simulations support the idea that these processes are non-conflictingly co-evolving and self-regulating. Furthermore, evidence of disruptive events that are capable of fast quenching is rare, and constraints on their statistical prevalence are lacking. Here we present a massive starburst galaxy at z=1.4 which is ejecting $46 \pm 13$\% of its molecular gas mass at a startling rate of $\gtrsim 10,000$ M$_{\odot}{\rm yr}^{-1}$. A broad component that is red-shifted from the galaxy emission is detected in four (low- and high-J) CO and [CI] transitions and in the ionized phase, which ensures a robust estimate of the expelled gas mass. The implied statistics suggest that similar events are potentially a major star-formation quenching channel. However, our observations provide compelling evidence that this is not a feedback-driven wind, but rather material from a merger that has been probably tidally ejected. This finding challenges some literature studies in which the role of feedback-driven winds might be overstated., Comment: Published in Nature Astronomy as an Article on 11 January 2021. The published version is available at https://www.nature.com/articles/s41550-020-01268-x (DOI 10.1038/s41550-020-01268-x)
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- 2021
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219. Gallium Nitride (GaN) based High-Power Multilevel H-Bridge Inverter for Wireless Power Transfer of Electric Vehicles.
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Javad Chevinly, Shervin Salehi Rad, Elias Nadi, Bogdan Proca, John Wolgemuth, Anthony Calabro, Hua Zhang, and Fei Lu
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- 2024
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220. Ketone Bodies after Cardiac Arrest: A Narrative Review and the Rationale for Use
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Filippo Annoni, Elisa Gouvea Bogossian, Lorenzo Peluso, Fuhong Su, Anthony Moreau, Leda Nobile, Stefano Giuseppe Casu, Elda Diletta Sterchele, Lorenzo Calabro, Michele Salvagno, Mauro Oddo, and Fabio Silvio Taccone
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ketone bodies ,ischemia–reperfusion ,cerebral metabolism ,anoxic brain injury ,heart arrest ,Cytology ,QH573-671 - Abstract
Cardiac arrest survivors suffer the repercussions of anoxic brain injury, a critical factor influencing long-term prognosis. This injury is characterised by profound and enduring metabolic impairment. Ketone bodies, an alternative energetic resource in physiological states such as exercise, fasting, and extended starvation, are avidly taken up and used by the brain. Both the ketogenic diet and exogenous ketone supplementation have been associated with neuroprotective effects across a spectrum of conditions. These include refractory epilepsy, neurodegenerative disorders, cognitive impairment, focal cerebral ischemia, and traumatic brain injuries. Beyond this, ketone bodies possess a plethora of attributes that appear to be particularly favourable after cardiac arrest. These encompass anti-inflammatory effects, the attenuation of oxidative stress, the improvement of mitochondrial function, a glucose-sparing effect, and the enhancement of cardiac function. The aim of this manuscript is to appraise pertinent scientific literature on the topic through a narrative review. We aim to encapsulate the existing evidence and underscore the potential therapeutic value of ketone bodies in the context of cardiac arrest to provide a rationale for their use in forthcoming translational research efforts.
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- 2024
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221. Extreme learning machine collocation for the numerical solution of elliptic PDEs with sharp gradients
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Calabrò, Francesco, Fabiani, Gianluca, and Siettos, Constantinos
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Mathematics - Numerical Analysis - Abstract
We introduce a new numerical method based on machine learning to approximate the solution of elliptic partial differential equations with collocation using a set of sigmoidal functions. We show that a feedforward neural network with a single hidden layer with sigmoidal functions and fixed, random, internal weights and biases can be used to compute accurately a collocation solution. The choice to fix internal weights and bias leads to the so-called Extreme Learning Machine network. We discuss how to determine the range for both internal weights and biases in order to obtain a good underlining approximating space, and we explore the required number of collocation points. We demonstrate the efficiency of the proposed method with several one-dimensional diffusion-advection-reaction problems that exhibit steep behaviors, such as boundary layers. The boundary conditions are imposed directly as collocation equations. We point out that there is no need of training the network, as the proposed numerical approach results to a linear problem that can be easily solved using least-squares. Numerical results show that the proposed method achieves a good accuracy. Finally, we compare the proposed method with finite differences and point out the significant improvements in terms of computational cost, thus avoiding the time-consuming training phase.
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- 2020
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222. The emergence of passive galaxies in the early Universe
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Santini, P., Castellano, M., Merlin, E., Fontana, A., Fortuni, F., Kodra, D., Magnelli, B., Menci, N., Calabrò, A., Lovell, C. C., Pentericci, L., Testa, V., and Wilkins, S. M.
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Astrophysics - Astrophysics of Galaxies - Abstract
The emergence of passive galaxies in the early Universe results from the interplay among the processes responsible for their rapid assembly and for the abrupt shut-down of their SF. Investigating the individual properties and demographics of early passive galaxies will improve our understanding of these mechanisms. In this work we present a follow-up analysis of the z>3 passive galaxy candidates selected by Merlin et al. (2019) in the CANDELS fields. We begin by first confirming the accuracy of their passive classification by exploiting their sub-mm emission to demonstrate the lack of ongoing SF. Using archival ALMA observations we are able to confirm at least 61% of the observed candidates as passive. While the remainder lack sufficiently deep data for confirmation, we are able to validate the entire sample in a statistical sense. We then estimate the Stellar Mass Function (SMF) of all 101 passive candidates in three redshift bins from z=5 to z=3. We adopt a stepwise approach that has the advantage of taking into account photometric errors, observational incompleteness, and the Eddington bias without any a-posteriori correction. We observe a pronounced evolution in the SMF around z~4, indicating that we are witnessing the emergence of the passive population at this epoch. Massive (M>10^11Msun) passive galaxies, only accounting for a small (<10%) fraction of galaxies at z>4, become dominant at later epochs. Thanks to a combination of photometric quality, sample selection and methodology, we overall find a higher density of passive galaxies than previous works. The comparison with theoretical predictions, despite a qualitative agreement, denotes a still incomplete understanding of the physical processes responsible for the formation of these galaxies. Finally, we extrapolate our results to predict the number of early passive galaxies expected in surveys carried out with future facilities., Comment: A&A in press, version updated to match the accepted version
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- 2020
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223. The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3
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Calabrò, A., Castellano, M., Pentericci, L., Fontanot, F., Menci, N., Cullen, F., McLure, R., Bolzonella, M., Cimatti, A., Marchi, F., Talia, M., Amorín, R., Cresci, G., De Lucia, G., Fynbo, J., Fontana, A., Franco, M., Hathi, N. P., Hibon, P., Hirschmann, M., Mannucci, F., Santini, P., Saxena, A., Schaerer, D., Xie, L., and Zamorani, G.
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Astrophysics - Astrophysics of Galaxies - Abstract
The estimate of stellar metallicities (Z*) of high-z galaxies are of paramount importance in order to understand the complexity of dust effects and the reciprocal interrelations among stellar mass, dust attenuation, stellar age, and metallicity. Benefiting from uniquely deep FUV spectra of >500 star-forming galaxies at redshifts 2
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- 2020
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224. Aggression in Healthcare Work Environments and Its Related Psycho Health Consequences
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Vitale, Elsa, Lupo, Roberto, Calabrò, Antonino, Conte, Luana, Martin, Colin R., editor, Preedy, Victor R., editor, and Patel, Vinood B., editor
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- 2023
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225. Optimization of Capillary-Based Western Blotting for MYO7A
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Calabro, Kaitlyn R., Boye, Sanford L., Boye, Shannon E., Crusio, Wim E., Series Editor, Dong, Haidong, Series Editor, Radeke, Heinfried H., Series Editor, Rezaei, Nima, Series Editor, Steinlein, Ortrud, Series Editor, Xiao, Junjie, Series Editor, Ash, John D., editor, Pierce, Eric, editor, Anderson, Robert E., editor, Bowes Rickman, Catherine, editor, Hollyfield, Joe G., editor, and Grimm, Christian, editor
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- 2023
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226. Evaluation Aspects in the Strategic Planning of a Reticular DMO for the Promotion of Inner Areas of Calabria
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Calabrò, Francesco, Lorè, Immacolata, Goos, Gerhard, Founding Editor, Hartmanis, Juris, Founding Editor, Bertino, Elisa, Editorial Board Member, Gao, Wen, Editorial Board Member, Steffen, Bernhard, Editorial Board Member, Yung, Moti, Editorial Board Member, Gervasi, Osvaldo, editor, Murgante, Beniamino, editor, Rocha, Ana Maria A. C., editor, Garau, Chiara, editor, Scorza, Francesco, editor, Karaca, Yeliz, editor, and Torre, Carmelo M., editor
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- 2023
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227. The Strategic Planning for the Promotion of Cultural Tourism in a Wide Area of Calabria: The Armeni Valley
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Calabrò, Francesco, Lorè, Immacolata, Viglianisi, Angela, Goos, Gerhard, Founding Editor, Hartmanis, Juris, Founding Editor, Bertino, Elisa, Editorial Board Member, Gao, Wen, Editorial Board Member, Steffen, Bernhard, Editorial Board Member, Yung, Moti, Editorial Board Member, Gervasi, Osvaldo, editor, Murgante, Beniamino, editor, Rocha, Ana Maria A. C., editor, Garau, Chiara, editor, Scorza, Francesco, editor, Karaca, Yeliz, editor, and Torre, Carmelo M., editor
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- 2023
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228. Maternal Mind-Mindedness and Communicative Functions in Free-Play and Mealtime Contexts: Stability, Continuity and Relations with Child Language at 16 Months
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Longobardi, Emiddia, Spataro, Pietro, and Calabro, Martina
- Abstract
The present study aimed at investigating the contextual stability, the contextual continuity and the concurrent associations between maternal measures (general language, communicative functions and mind-mindedness) and child measures (total number of word types and tokens) in two different contexts, free-play and mealtime. To this purpose, the interactions occurring between 25 mothers and their 16-month-old children in each context were video-recorded, transcribed and later coded for the selected measures. Significant contextual stability was observed in the mothers' production of general language measures (total number of utterances, total number of words and MLU), in the children's production of word types and tokens, and in some communicative functions (Tutorial, Control and Asynchronous). No contextual stability was found for the mothers' production of attuned mind-related comments. For continuity, both mothers and children produced more utterances and words in the free-play than in the mealtime context; the production of attuned mind-related comments and the use of the Control function were also more frequent in the free-play context. Lastly, the analysis of the concurrent correlations indicated that, especially in the mealtime context, the number of words produced by children was positively associated with the number of words produced by mothers and by their use of the Tutorial and Didactic functions, but negatively associated with their use of the Control function. The mothers' production of attuned mind-related comments bore no relation with children's expressive language. Similarities and differences with previous findings are discussed.
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- 2022
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229. Baseline brain function in the preadolescents of the ABCD Study
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Chaarani, B, Hahn, S, Allgaier, N, Adise, S, Owens, MM, Juliano, AC, Yuan, DK, Loso, H, Ivanciu, A, Albaugh, MD, Dumas, J, Mackey, S, Laurent, J, Ivanova, M, Hagler, DJ, Cornejo, MD, Hatton, S, Agrawal, A, Aguinaldo, L, Ahonen, L, Aklin, W, Anokhin, AP, Arroyo, J, Avenevoli, S, Babcock, D, Bagot, K, Baker, FC, Banich, MT, Barch, DM, Bartsch, H, Baskin-Sommers, A, Bjork, JM, Blachman-Demner, D, Bloch, M, Bogdan, R, Bookheimer, SY, Breslin, F, Brown, S, Calabro, FJ, Calhoun, V, Casey, BJ, Chang, L, Clark, DB, Cloak, C, Constable, RT, Constable, K, Corley, R, Cottler, LB, Coxe, S, Dagher, RK, Dale, AM, Dapretto, M, Delcarmen-Wiggins, R, Dick, AS, Do, EK, Dosenbach, NUF, Dowling, GJ, Edwards, S, Ernst, TM, Fair, DA, Fan, CC, Feczko, E, Feldstein-Ewing, SW, Florsheim, P, Foxe, JJ, Freedman, EG, Friedman, NP, Friedman-Hill, S, Fuemmeler, BF, Galvan, A, Gee, DG, Giedd, J, Glantz, M, Glaser, P, Godino, J, Gonzalez, M, Gonzalez, R, Grant, S, Gray, KM, Haist, F, Harms, MP, Hawes, S, Heath, AC, Heeringa, S, Heitzeg, MM, Hermosillo, R, Herting, MM, Hettema, JM, Hewitt, JK, Heyser, C, Hoffman, E, Howlett, K, Huber, RS, Huestis, MA, Hyde, LW, Iacono, WG, Infante, MA, Irfanoglu, O, Isaiah, A, and Iyengar, S
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Biological Psychology ,Cognitive and Computational Psychology ,Psychology ,Mind and Body ,Substance Misuse ,Behavioral and Social Science ,Clinical Research ,Mental Health ,Basic Behavioral and Social Science ,Neurosciences ,Drug Abuse (NIDA only) ,1.2 Psychological and socioeconomic processes ,Underpinning research ,Neurological ,Mental health ,Adolescent ,Adolescent Development ,Brain ,Child ,Female ,Humans ,Magnetic Resonance Imaging ,Male ,Reference Values ,ABCD Consortium ,Cognitive Sciences ,Neurology & Neurosurgery ,Biological psychology - Abstract
The Adolescent Brain Cognitive Development (ABCD) Study® is a 10-year longitudinal study of children recruited at ages 9 and 10. A battery of neuroimaging tasks are administered biennially to track neurodevelopment and identify individual differences in brain function. This study reports activation patterns from functional MRI (fMRI) tasks completed at baseline, which were designed to measure cognitive impulse control with a stop signal task (SST; N = 5,547), reward anticipation and receipt with a monetary incentive delay (MID) task (N = 6,657) and working memory and emotion reactivity with an emotional N-back (EN-back) task (N = 6,009). Further, we report the spatial reproducibility of activation patterns by assessing between-group vertex/voxelwise correlations of blood oxygen level-dependent (BOLD) activation. Analyses reveal robust brain activations that are consistent with the published literature, vary across fMRI tasks/contrasts and slightly correlate with individual behavioral performance on the tasks. These results establish the preadolescent brain function baseline, guide interpretation of cross-sectional analyses and will enable the investigation of longitudinal changes during adolescent development.
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- 2021
230. Prediction of incident atrial fibrillation in hypertrophic cardiomyopathy
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Losi, Maria Angela, Monda, Emanuele, Lombardi, Raffaella, Lioncino, Michele, Canciello, Grazia, Rubino, Marta, Todde, Gaetano, Caiazza, Martina, Borrelli, Felice, Fusco, Adelaide, Cirillo, Annapaola, Perillo, Errico Federico, Sepe, Joseph, Pacella, Daniela, de Simone, Giovanni, Calabro, Paolo, Esposito, Giovanni, and Limongelli, Giuseppe
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- 2024
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231. Physics-Informed Neural Networks for 2nd order ODEs with sharp gradients
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De Florio, Mario, Schiassi, Enrico, Calabrò, Francesco, and Furfaro, Roberto
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- 2024
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232. Familial hypercholesterolaemia in children and adolescents from 48 countries: a cross-sectional study
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Dharmayat, Kanika Inamdar, Vallejo-Vaz, Antonio J., Stevens, Christophe A.T., Brandts, Julia M., Lyons, Alexander R.M., Groselj, Urh, Abifadel, Marianne, Aguilar-Salinas, Carlos A., Alhabib, Khalid, Alkhnifsawi, Mutaz, Almahmeed, Wael, Alnouri, Fahad, Alonso, Rodrigo, Al-Rasadi, Khalid, Ashavaid, Tester F., Banach, Maciej, Béliard, Sophie, Binder, Christoph, Bourbon, Mafalda, Chlebus, Krzysztof, Corral, Pablo, Cruz, Diogo, Descamps, Olivier S., Drogari, Euridiki, Durst, Ronen, Ezhov, Marat V., Genest, Jacques, Harada-Shiba, Mariko, Holven, Kirsten B., Humphries, Steve E., Khovidhunkit, Weerapan, Lalic, Katarina, Laufs, Ulrich, Liberopoulos, Evangelos, Roeters van Lennep, Jeanine, Lima-Martinez, Marcos Miguel, Lin, Jie, Maher, Vincent, März, Winfried, Miserez, André R., Mitchenko, Olena, Nawawi, Hapizah, Panayiotou, Andrie G., Paragh, György, Postadzhiyan, Arman, Reda, Ashraf, Reiner, Željko, Reyes, Ximena, Sadiq, Fouzia, Sahebkar, Amirhossein, Schunkert, Heribert, Shek, Aleksandr B., Stroes, Eric, Su, Ta-Chen, Subramaniam, Tavintharan, Susekov, Andrey, Vázquez Cárdenas, Alejandra, Huong Truong, Thanh, Tselepis, Alexandros D., Vohnout, Branislav, Wang, Luya, Yamashita, Shizuya, Al-Sarraf, Ahmad, Al-Sayed, Nasreen, Davletov, Kairat, Dwiputra, Bambang, Gaita, Dan, Kayikcioglu, Meral, Latkovskis, Gustavs, Marais, A. David, Thushara Matthias, Anne, Mirrakhimov, Erkin, Nordestgaard, Børge G., Petrulioniene, Zaneta, Pojskic, Belma, Sadoh, Wilson, Tilney, Myra, Tomlinson, Brian, Tybjærg-Hansen, Anne, Viigimaa, Margus, Catapano, Alberico L., Freiberger, Tomas, Hovingh, G. Kees, Mata, Pedro, Soran, Handrean, Raal, Frederick, Watts, Gerald F., Schreier, Laura, Bañares, Virginia, Greber-Platzer, Susanne, Baumgartner-Kaut, Margot, de Gier, Charlotte, Dieplinger, Hans, Höllerl, Florian, Innerhofer, Reinhold, Karall, Daniela, Lischka, Julia, Ludvik, Bernhard, Mäser, Martin, Scholl-Bürgi, Sabine, Thajer, Alexandra, Toplak, Hermann, Demeure, Fabian, Mertens, Ann, Balligand, Jean-Luc, Stephenne, Xavier, Sokal, Etienne, Petrov, Ivo, Goudev, Assen, Nikolov, Fedya, Tisheva, Snejana, Yotov, Yoto, Tzvetkov, Ivajlo, Hegele, Robert A, Gaudet, Daniel, Brunham, Liam, Ruel, Isabelle, McCrindle, Brian, Cuevas, Ada, Perica, Dražen, Symeonides, Phivos, Trogkanis, Efstratios, Kostis, Andreas, Ioannou, Andreas, Mouzarou, Angeliki, Georgiou, Anthoula, Stylianou, Andreas, Miltiadous, George, Iacovides, Paris, Deltas, Constantinos, Vrablik, Michal, Urbanova, Zuzana, Jesina, Pavel, Tichy, Lukas, Hyanek, Josef, Dvorakova, Jana, Cepova, Jana, Sykora, Josef, Buresova, Kristyna, Pipek, Michal, Pistkova, Eva, Bartkova, Ivana, S|ulakova, Astrid, Toukalkova, Lenka, Spenerova, Michaela, Maly, Jan, Benn, Marianne, Bendary, Ahmed, Elbahry, Atef, Ferrières, Jean, Ferrieres, Dorota, Peretti, Noel, Bruckert, Eric, Gallo, Antonio, Valero, René, Mourre, Florian, Aouchiche, Karine, Reynaud, Rachel, Tounian, Patrick, Lemale, Julie, Boccara, Franck, Moulin, Philippe, Charrières, Sybil, Di Filippo, Mathilde, Cariou, Bertrand, Paillard, François, Dourmap, Caroline, Pradignac, Alain, Verges, Bruno, Simoneau, Isabelle, Farnier, Michel, Cottin, Yves, Yelnik, Cecile, Hankard, Regis, Schiele, François, Durlach, Vincent, Sultan, Ariane, Carrié, Alain, Rabès, Jean-Pierre, Sanin, Veronika, Schmieder, Raphael S., Ates, Sara, Rizos, Christos V., Skoumas, Ioannis, Tziomalos, Konstantinos, Rallidis, Loukianos, Kotsis, Vasileios, Doumas, Michalis, Skalidis, Emmanouil, Kolovou, Genovefa, Kolovou, Vana, Garoufi, Anastasia, Koutagiar, Iosif, Polychronopoulos, Georgios, Kiouri, Estela, Antza, Christina, Zacharis, Evangelos, Attilakos, Achilleas, Sfikas, George, Koumaras, Charalambos, Anagnostis, Panagiotis, Anastasiou, Georgia, Liamis, George, Adamidis, Petros-Spyridon, Milionis, Haralambos, Lambadiari, Vaia, Stabouli, Stella, Filippatos, Theodosios, Mollaki, Vicky, Tsaroumi, Anastasia, Lamari, Frida, Proyias, Pavlos, Harangi, Mariann, Reddy, Lakshmi Lavanya, Shah, Swarup A. V, Ponde, Chandrashekhar K., Dalal, Jamshed J., Sawhney, Jitendra P.S., Verma, Ishwar C., Hosseini, Susan, Jamialahmadi, Tannaz, Alareedh, Mohammed, Shaghee, Foaad, Rhadi, Sabah Hasan, Abduljalal, Maryam, Alfil, Sarmad, Kareem, Huda, Cohen, Hofit, Leitersdorf, Eran, Schurr, Daniel, Shpitzen, Shoshi, Arca, Marcello, Averna, Maurizio, Bertolini, Stefano, Calandra, Sebastiano, Tarugi, Patrizia, Casula, Manuela, Galimberti, Federica, Gazzotti, Marta, Olmastroni, Elena, Sarzani, Riccardo, Ferri, Claudio, Repetti, Elena, Giorgino, Francesco, Suppressa, Patrizia, Bossi, Antonio Carlo, Borghi, Claudio, Muntoni, Sandro, Cipollone, Francesco, Scicali, Roberto, Pujia, Arturo, Passaro, Angelina, Berteotti, Martina, Pecchioli, Valerio, Pisciotta, Livia, Mandraffino, Giuseppe, Pellegatta, Fabio, Mombelli, Giuliana, Branchi, Adriana, Fiorenza, Anna Maria, Pederiva, Cristina, Werba, José Pablo, Parati, Gianfranco, Nascimbeni, Fabio, Iughetti, Lorenzo, Fortunato, Giuliana, Cavallaro, Raimondo, Iannuzzo, Gabriella, Calabrò, Paolo, Cefalù, Angelo Baldassare, Capra, Maria Elena, Zambon, Alberto, Pirro, Matteo, Sbrana, Francesco, Trenti, Chiara, Minicocci, Ilenia, Federici, Massimo, Del Ben, Maria, Buonuomo, Paola Sabrina, Moffa, Simona, Pipolo, Antonio, Citroni, Nadia, Guardamagna, Ornella, Lia, Salvatore, Benso, Andrea, Biolo, Gianni Biolo, Maroni, Lorenzo, Lupi, Alessandro, Bonanni, Luca, Rinaldi, Elisabetta, Zenti, Maria Grazia, Masuda, Daisaku, Mahfouz, Linda, Jambart, Selim, Ayoub, Carine, Ghaleb, Youmna, Kasim, Noor Alicezah Mohd, Nor, Noor Shafina Mohd, Al-Khateeb, Alyaa, Kadir, Siti Hamimah Sheikh Abdul, Chua, Yung-An, Razman, Aimi Zafira, Nazli, Sukma Azureen, Ranai, Norashikin Mohd, Latif, Ahmad Zubaidi Abd, Torres, María Teresa Magaña, Mehta, Roopa, Martagon, Alexandro J., Ramirez, Gabriela A. Galan, Antonio-Villa, Neftali Eduardo, Vargas-Vazquez, Arsenio, Elias-Lopez, Daniel, Retana, Gustavo Gonzalez, Encinas, Bethsabel Rodrıguez, Macıas, Jose J. Ceballos, Zazueta, Alejandro Romero, Alvarado, Rocio Martinez, Portano, Julieta D. Morales, Lopez, Humberto Alvares, Sauque-Reyna, Leobardo, Gomez Herrera, Laura G., Simental Mendia, Luis E., Aguilar, Humberto Garcia, Cooremans, Elizabeth Ramirez, Aparicio, Berenice Pe~na, Zubieta, Victoria Mendoza, Gonzalez, Perla A. Carrillo, Ferreira-Hermosillo, Aldo, Portilla, Nacu Caracas, Dominguez, Guadalupe Jimenez, Garcia, Alinna Y. Ruiz, Arriaga Cazares, Hector E., Gonzalez Gonzalez, Jesus R., Mendez Valencia, Carla V., Padilla Padilla, Francisco G., Prado, Ramon Madriz, De los Rios Ibarra, Manuel O., Arjona Villica~na, Ruy D., Acevedo Rivera, Karina J., Carrera, Ricardo Allende, Alvarez, Jose A., Amezcua Martinez, Jose C., Barrera Bustillo, Manuel de los Reyes, Vargas, Gonzalo Carazo, Chacon, Roberto Contreras, Figueroa Andrade, Mario H., Ortega, Ashanty Flores, Alcala, Hector Garcia, Garcia de Leon, Laura E., Guzman, Berenice Garcia, Gardu~no Garcia, Jose J., Garnica Cuellar, Juan C., Gomez Cruz, Jose R., Garcia, Anell Hernandez, Holguin Almada, Jesus R., Herrera, Ursulo Juarez, Sobrevilla, Fabiola Lugo, Rodriguez, Eduardo Marquez, Sibaja, Cristina Martinez, Medrano Rodriguez, Alma B., Morales Oyervides, Jose C., Perez Vazquez, Daniel I., Reyes Rodriguez, Eduardo A., Osorio, Ma. Ludivina Robles, Saucedo, Juan Rosas, Tamayo, Margarita Torres, Valdez Talavera, Luis A., Vera Arroyo, Luis E., Zepeda Carrillo, Eloy A., Galema-Boers, Annette, Weigman, Albert, Bogsrud, Martin P., Malik, Munir, Shah, Saeedullah, Khan, Sabeen Abid, Rana, Muhammad Asim, Batool, Hijab, Starostecka, Ewa, Konopka, Agnieszka, Lewek, Joanna, Bielecka-Dąbrowa, Agata, Gach, Agnieszka, Jóźwiak, Jacek, Pajkowski, Marcin, Romanowska-Kocejko, Marzena, Żarczyńska-Buchowiecka, Marta, Hellmann, Marcin, Chmara, Magdalena, Wasąg, Bartosz, Parczewska, Aleksandra, Gilis-Malinowska, Natasza, Borowiec-Wolna, Justyna, Stróżyk, Aneta, Michalska-Grzonkowska, Aleksandra, Chlebus, Izabela, Kleinschmidt, Mariola, Wojtecka, Agnieszka, Zdrojewski, Tomasz, Myśliwiec, Małgorzata, Hennig, Matylda, Medeiros, Ana Margarida, Alves, Ana Catarina, Almeida, Ana Filipa, Lopes, Andreia, Guerra, António, Bilhoto, Carla, Simões, Fernando, Silva, Francisco, Lobarinhas, Goreti, Gama, Guida, Palma, Isabel, Salgado, José Miguel, Matos, Luísa Diogo, Moura, Márcio de, Virtuoso, Maria João, Tavares, Mónica, Ferreira, Patrícia, Pais, Patrícia, Garcia, Paula, Coelho, Raquel, Ribeiro, Raquel, Correia, Susana, Sadykova, Dinara, Slastnikova, Evgenia, Alammari, Dalal, Mawlawi, Horia Ahmed, Alsahari, Atif, Khudary, Alia Abdullah, Alrowaily, Nawal Lafi, Rajkovic, Natasa, Popovic, Ljiljana, Singh, Sandra, Rasulic, Iva, Petakov, Ana, Lalic, Nebojsa M., Peng, Fabian Kok, Vasanwala, Rashida Farhan, Venkatesh, Sreedharan Aravind, Raslova, Katarina, Fabryova, Lubomira, Nociar, Jan, Šaligova, Jana, Potočňáková, Ludmila, Kozárová, Miriam, Varga, Tibor, Kadurova, Michaela, Debreova, Marianna, Novodvorsky, Peter, Gonova, Katarina, Klabnik, Alexander, Buganova, Ingrid, Battelino, Tadej, Bizjan, Barbara Jenko, Debeljak, Marusa, Kovac, Jernej, Mlinaric, Matej, Molk, Neza, Sikonja, Jaka, Sustar, Ursa, Podkrajsek, Katarina Trebusak, Muñiz-Grijalvo, Ovidio, Díaz-Díaz, Jose Luis, de Andrés, Raimundo, Fuentes-Jiménez, Francisco, Blom, Dirk, Miserez, Eleonore B., Shipton, Janine L., Ganokroj, Poranee, Futema, Marta, Ramaswami, Uma, Alieva, Rano B., Fozilov, Khurshid G., Khoshimov, Shavkat U., Nizamov, Ulugbek I., Abdullaeva, Guzal J., Kan, Liliya E., Abdullaev, Alisher A., Zakirova, Daria V., Do, Doan-Loi, Nguyen, Mai-Ngoc-Thi, Kim, Ngoc-Thanh, Le, Thanh-Tung, Le, Hong-An, Santos, Raul, and Ray, Kausik K.
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- 2024
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233. Efficacy and Safety of Pembrolizumab plus Axitinib combination for Metastatic Renal Cell Carcinoma in a Real-World Scenario: Data From the Prospective ProPAXI Study
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Guida, Annalisa, Gili, Alessio, Mosillo, Claudia, Maruzzo, Marco, Lai, Eleonora, Pierantoni, Francesco, Bimbatti, Davide, Basso, Umberto, Fornarini, Giuseppe, Rebuzzi, Sara Elena, Calabrò, Fabio, Cerbone, Linda, Caserta, Claudia, Sirgiovanni, Grazia, Serafin, Debora, Caffo, Orazio, Scagliarini, Sarah, and Bracarda, Sergio
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- 2024
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234. The Effects of Corticosteroids on Survival in Pediatric and Nonelderly Adult Patients Undergoing Cardiac Surgery: A Meta-analysis of Randomized Studies
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Oriani, Alessandro, Prima, Ambra Licia Di, Mucchetti, Marta, Ortalda, Alessandro, Calabrò, Maria Grazia, Zangrillo, Alberto, Losiggio, Rosario, Lomivorotov, Vladimir, D'Andria Ursoleo, Jacopo, Kotani, Yuki, Monaco, Fabrizio, Milojevic, Milan, Yavorovskiy, Andrey, Lee, Todd C., and Landoni, Giovanni
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- 2024
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235. Secondary prevention and extreme cardiovascular risk evaluation (SEVERE-0): Prevalence of extreme cardiovascular risk in cardiological rehabilitation patients and its impact on functional improvement
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Tognola, Chiara, Myriam Intravaia, Rita Cristina, Senini, Eleonora, Pezzoli, Stefano, Riccio, Alfonso, Gualini, Elena, Fabbri, Saverio, Bellantonio, Valentina, Politi, Francesco, Campana, Marta, Fucile, Ilaria, Mancusi, Costantino, Golia, Enrica, Cesaro, Arturo, De Luca, Nicola, Calabrò, Paolo, Giannattasio, Cristina, and Maloberti, Alessandro
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- 2024
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236. Active help-seeking and metacognition interact in supporting children’s retention of science facts
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Shields, Michelle, Calabro, Grai, and Selmeczy, Diana
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- 2024
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237. Reproducibility of an artificial intelligence optical coherence tomography software for tissue characterization: Implications for the design of longitudinal studies
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Garg, Mohil, Garcia-Garcia, Hector M., Calderón, Andrea Teira, Gupta, Jaytin, Sortur, Shrayus, Levine, Molly B., Singla, Puneet, Picchi, Andrea, Sardella, Gennaro, Adamo, Marianna, Frigoli, Enrico, Limbruno, Ugo, Rigattieri, Stefano, Diletti, Roberto, Boccuzzi, Giacomo, Zimarino, Marco, Contarini, Marco, Russo, Filippo, Calabro, Paolo, Andò, Giuseppe, Varbella, Ferdinando, Garducci, Stefano, Palmieri, Cataldo, Briguori, Carlo, Sánchez, Jorge Sanz, and Valgimigli, Marco
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- 2024
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238. Suicide attempts in French Polynesia during the era of COVID-19: a prospective analysis over three years
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Sebti, Johan, Serres, Marguerite, Calabro, Valérie, and Tsai, Guochuan Emil
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- 2024
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239. PDE models for vegetation biomass and autotoxicity
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Abbas, Mudassar, Giannino, Francesco, Iuorio, Annalisa, Ahmad, Zubair, and Calabró, Francesco
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- 2025
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240. Sustainability concerns influence studies reported at the 2022 MRS Fall Meeting & Exhibit: mrs.org/fall2022
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Meiksin, Judy, Afful, Henry Quansah, Atwa, Mohamed, Calabro, Rosemary, Mahmood, Yasir, Mistry, Aashutosh, and Tamakloe, Senam
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- 2023
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241. The pediatric leukemia oncoprotein NUP98-KDM5A induces genomic instability that may facilitate malignant transformation
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Joan Domingo-Reinés, Rosa Montes, Adrián Garcia-Moreno, Amador Gallardo, Jose Manuel Sanchez-Manas, Iván Ellson, Mar Lamolda, Chiara Calabro, Jose Antonio López-Escamez, Purificación Catalina, Pedro Carmona-Sáez, Pedro J. Real, David Landeira, and Verónica Ramos-Mejia
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Cytology ,QH573-671 - Abstract
Abstract Pediatric Acute Myeloid Leukemia (AML) is a rare and heterogeneous disease characterized by a high prevalence of gene fusions as driver mutations. Despite the improvement of survival in the last years, about 50% of patients still experience a relapse. It is not possible to improve prognosis only with further intensification of chemotherapy, as come with a severe cost to the health of patients, often resulting in treatment-related death or long-term sequels. To design more effective and less toxic therapies we need a better understanding of pediatric AML biology. The NUP98-KDM5A chimeric protein is exclusively found in a particular subgroup of young pediatric AML patients with complex karyotypes and poor prognosis. In this study, we investigated the impact of NUP98-KDM5A expression on cellular processes in human Pluripotent Stem Cell models and a patient-derived cell line. We found that NUP98-KDM5A generates genomic instability through two complementary mechanisms that involve accumulation of DNA damage and direct interference of RAE1 activity during mitosis. Overall, our data support that NUP98-KDM5A promotes genomic instability and likely contributes to malignant transformation.
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- 2023
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242. Effects of traffic light labelling and increased healthy range on beverage choices from vending machines
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Ryan Calabro, Eva Kemps, Ivanka Prichard, and Marika Tiggemann
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Soft drink ,Beverage choice ,Vending machine ,Traffic light system ,Healthy range ,Nudging ,Public aspects of medicine ,RA1-1270 ,Nutritional diseases. Deficiency diseases ,RC620-627 - Abstract
Abstract Objective: To test whether traffic light labels and an increased range of healthy beverages, individually and in combination, can increase healthy beverage choices from vending machines. Design: Two studies (n 558, 420) tested whether the provision of traffic light labels (green, amber and red) and an increased range of healthy beverages (from 20 % to 50 % green options), individually and in combination, could increase healthy beverage choices from a digital vending machine display. The studies used a between-subjects experimental design, and a hypothetical beverage choice, a limitation when considering real-world applicability. Setting: Both studies utilised an online Qualtrics survey that featured a digital vending machine display. Participants: Both studies (n 558, 420) consisted of university students from Flinders University and individuals from a survey recruitment service. Results: Featuring traffic lights did not significantly influence beverage choices (P = 0·074), while increasing the healthy range (P = 0·003, OR = 3·27), and the combination of both, did significantly increase healthier beverage choices (P < 0·001, OR = 4·83). Conclusions: The results suggest that the traffic light system and increased healthy range are not maximally effective when used on their own, and benefit greatly when combined, to increase healthy beverage choices. It was suggested that the provision of traffic light labels supplied the necessary nutritional information, and the increased healthy range offered greater opportunity to act in accordance with that information. In so doing, the present findings offer a promising pathway for reducing unhealthy beverage consumption.
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- 2024
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243. Cooling and Timing tests of the ATLAS Fast Tracker VME boards
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Sottocornola, S., Annovi, A., Biesuz, N. V., Brost, E., Calvetti, M., Gentsos, C., Holmes, T., Horyn, L., Iizawa, T., Lanza, A., Long, J. D., Mastrandrea, P., Maznas, I., Negri, A., Calabro, D., Piendibene, M., Roda, C., Romano, E., and Seiss, T.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment ,I.5.4 ,I.5.5 ,B.8.1 ,B.4.4 - Abstract
The Fast Tracker (FTK) is an ATLAS trigger upgrade built for full event, low-latency, high-rate tracking. The FTK core, made of 9U VME boards, performs the most demanding computational task. The Associative Memory Board Serial Link Processor (AMB) and the Auxiliary card (AUX), plugged on the front and back sides of the same VME slot, constitute the Processing Unit (PU), which finds tracks using hits from 8 layers of the inner detector. The PU works in pipeline with the Second Stage Board (SSB), which finds 12-layer tracks by adding extra hits to the identified tracks. In the designed configuration, 16 PUs and 4 SSBs are installed in a VME crate. The high power-consumption of the AMB, AUX and SSB (respectively of about 250 W, 70 W and 160 W per board) required the development of a custom cooling system. Even though the expected power consumption for each VME crate of the FTK system is high compared to a common VME setup, the 8 FTK core crates will use $\approx$ 60 kW, which is just a fraction of the power and the space needed for a CPU farm performing the same task. We report on the integration of 32 PUs and 8 SSBs inside the FTK system, on the infrastructures needed to run and cool them, and on the tests performed to verify the system processing rate and the temperature stability at a safe value., Comment: Real Time 2020 conference, 8 pages
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- 2020
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244. Investigating the Effect of Galaxy Interactions on AGN Enhancement at $0.5<z<3.0$
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Shah, Ekta A., Kartaltepe, Jeyhan S., Magagnoli, Christina T., Cox, Isabella G., Wetherell, Caleb T., Vanderhoof, Brittany N., Calabro, Antonello, Chartab, Nima, Conselice, Christopher J., Croton, Darren J., Donley, Jennifer, de Groot, Laura, de la Vega, Alexander, Hathi, Nimish P., Ilbert, Olivier, Inami, Hanae, Kocevski, Dale D., Koekemoer, Anton M., Lemaux, Brian C., Mantha, Kameswara Bharadwaj, Marchesi, Stefano, Martig, Marie, Masters, Daniel C., McGrath, Elizabeth J., McIntosh, Daniel H., Moreno, Jorge, Nayyeri, Hooshang, Pampliega, Belen Alcalde, Salvato, Mara, Snyder, Gregory F., Straughn, Amber N., Treister, Ezequiel, and Weston, Madalyn E.
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Astrophysics - Astrophysics of Galaxies - Abstract
Galaxy interactions and mergers are thought to play an important role in the evolution of galaxies. Studies in the nearby universe show a higher AGN fraction in interacting and merging galaxies than their isolated counterparts, indicating that such interactions are important contributors to black hole growth. To investigate the evolution of this role at higher redshifts, we have compiled the largest known sample of major spectroscopic galaxy pairs (2381 with $\Delta V <5000$ km s$^{-1}$) at $0.5
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- 2020
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245. Three Lyman-alpha emitting filaments converging to a massive galaxy group at z=2.91: discussing the case for cold gas infall
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Daddi, E., Valentino, F., Rich, R. M., Neill, J. D., Gronke, M., O'Sullivan, D., Elbaz, D., Bournaud, F., Finoguenov, A., Marchal, A., Delvecchio, I., Jin, S., Liu, D., Calabro, A., Coogan, R., D'Eugenio, C., Gobat, R., Kalita, B. S., Laursen, P., Martin, D. C., Puglisi, A., Schinnerer, E., Strazzullo, V., and Wang, T.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We have discovered a 300kpc-wide giant Lya nebula centered on the massive galaxy group RO-1001 at z=2.91 in the COSMOS field. Keck Cosmic Web Imager observations reveal three cold gas filaments converging into the center of the potential well of its ~4x10^13Msun dark matter halo, hosting 1200Msun/yr of star formation as probed by ALMA and NOEMA observations. The nebula morphological and kinematics properties and the prevalence of blueshifted components in the Lya spectra are consistent with a scenario of gas accretion. The upper limits on AGN activity and overall energetics favor gravity as the primary Lya powering source and infall as the main source of gas flows to the system. Although interpretational difficulties remain, with outflows and likely also photoionization with ensuing recombination still playing a role, this finding provides arguably an ideal environment to quantitatively test models of cold gas accretion and galaxy feeding inside an actively star-forming massive halo at high redshift., Comment: 20 pages, 12 figures, 3 tables. Accepted for publication in A&A
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- 2020
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246. Complexity Reduction of Volterra Nonlinear Equalization for Optical Short-Reach IM/DD Systems
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Wettlin, Tom, Rahman, Talha, Wei, Jinlong, Calabrò, Stefano, Stojanovic, Nebojsa, and Pachnicke, Stephan
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Electrical Engineering and Systems Science - Signal Processing - Abstract
We investigate approaches to reduce the computational complexity of Volterra nonlinear equalizers (VNLEs) for short-reach optical transmission systems using intensity modulation and direct detection (IM/DD). In this contribution we focus on a structural reduction of the number of kernels, i.e. we define rules to decide which terms need to be implemented and which can be neglected before the kernels are calculated. This static complexity reduction is to be distinguished from other approaches like pruning or L1 regularization, that are applied after the adaptation of the full Volterra equalizer e.g. by thresholding. We investigate the impact of the complexity reduction on 90 GBd PAM6 IM/DD experimental data acquired in a back-to-back setup as well as in case of transmission over 1 km SSMF. First, we show, that the third-order VNLE terms have a significant impact on the overall performance of the system and that a high number of coefficients is necessary for optimal performance. Afterwards, we show that restrictions, for example on the tap spacing among samples participating in the same kernel, can lead to an improved tradeoff between performance and complexity compared to a full third-order VNLE. We show an example, in which the number of third-order kernels is halved without any appreciable performance degradation.
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- 2020
247. X-ray properties of He II 1640 emitting galaxies in VANDELS
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Saxena, A., Pentericci, L., Schaerer, D., Schneider, R., Amorin, R., Bongiorno, A., Calabrò, A., Castellano, M., Cimatti, A., Cullen, F., Fontana, A., Fynbo, J. P. U., Hathi, N., McLeod, D. J., Talia, M., and Zamorani, G.
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Astrophysics - Astrophysics of Galaxies - Abstract
We explore X-ray emission from a sample of 18 He II 1640 emitting star-forming galaxies at z ~ 2.3-3.6 from the VANDELS survey in the Chandra Deep Field South, to set constraints on the role of X-ray sources in powering the He II emission. We find that 4 He II emitters have tentative detections with S/N ~ 2 and have X-ray luminosities, L_X = 1.5-4.9 x 10^41 erg/s. The stacked luminosity of all 18 He II emitters is 2.6 x 10^41 erg/s, and that of a subset of 13 narrow He II emitters (FHWM(He II) < 1000 km/s) is 3.1 x 10^41 erg/s. We also measure stacked L_X for non-He II emitters through bootstrapping of matched samples, and find L_X = 2.5 x 10^41 erg/s, which is not significantly different from L_X measured for He II emitters. The L_X per star-formation rate for He II emitters (log (L_X/SFR) ~ 40.0) and non-emitters (log (L_X/SFR) ~ 39.9) are also comparable and in line with the redshift evolution and metallicity dependence predicted by models. Due to the non-significant difference between the X-ray emission from galaxies with and without He II, we conclude that X-ray binaries or weak or obscured AGNs are unlikely to be the dominant producers of He II ionising photons in VANDELS star-forming galaxies at z ~ 3. Given the comparable physical properties of both He II emitters and non-emitters reported previously, alternative He II ionising mechanisms such as localised low-metallicity stellar populations, Pop-III stars, etc. may need to be explored., Comment: 12 pages, 5 figures, accepted for publication in MNRAS
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- 2020
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248. The Typical Massive Quiescent Galaxy at z$\sim$3 is a Post-starburst
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D'Eugenio, C., Daddi, E., Gobat, R., Strazzullo, V., Lustig, P., Delvecchio, I., Jin, S., Puglisi, A., Calabró, A., Mancini, C., Dickinson, M., Cimatti, A., and Onodera, M.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We have obtained spectroscopic confirmation with Hubble Space Telescope WFC3/G141 of a first sizeable sample of nine quiescent galaxies at 2.4
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- 2020
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249. Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
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Carnall, A. C., Walker, S., McLure, R. J., Dunlop, J. S., McLeod, D. J., Cullen, F., Wild, V., Amorin, R., Bolzonella, M., Castellano, M., Cimatti, A., Cucciati, O., Fontana, A., Gargiulo, A., Garilli, B., Jarvis, M. J., Pentericci, L., Pozzetti, L., Zamorani, G., Calabro, A., Hathi, N. P., and Koekemoer, A. M.
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Astrophysics - Astrophysics of Galaxies - Abstract
We present a sample of 151 massive ($M_* > 10^{10}\mathrm{M_\odot}$) quiescent galaxies at $2 < z < 5$, based on a sophisticated Bayesian spectral energy distribution fitting analysis of the CANDELS UDS and GOODS-South fields. Our sample includes a robust sub-sample of 61 objects for which we confidently exclude low-redshift and star-forming solutions. We identify 10 robust objects at $z>3$, of which 2 are at $z>4$. We report formation redshifts, demonstrating that the oldest objects formed at $z > 6$, however individual ages from our photometric data have significant uncertainties, typically $\sim0.5$ Gyr. We demonstrate that the UVJ colours of the quiescent population evolve with redshift at $z>3$, becoming bluer and more similar to post-starburst galaxies at lower redshift. Based upon this we construct a model for the time-evolution of quiescent galaxy UVJ colours, concluding that the oldest objects are consistent with forming the bulk of their stellar mass at $z\sim6-7$ and quenching at $z\sim5$. We report spectroscopic redshifts for two of our objects at $z=3.440$ and $3.396$, which exhibit extremely weak Ly$\alpha$ emission in ultra-deep VANDELS spectra. We calculate star-formation rates based on these line fluxes, finding that these galaxies are consistent with our quiescent selection criteria, provided their Ly$\alpha$ escape fractions are $>3$ and $>10$ per cent respectively. We finally report that our highest-redshift robust object exhibits a continuum break at $\lambda\sim7000$A in a spectrum from VUDS, consistent with our photometric redshift of $z_\mathrm{phot}=4.72^{+0.06}_{-0.04}$. If confirmed as quiescent this object would be the highest-redshift known quiescent galaxy. To obtain stronger constraints on the times of the earliest quenching events, high-SNR spectroscopy must be extended to $z\gtrsim3$ quiescent objects., Comment: 14 pages, 8 figures, MNRAS accepted
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- 2020
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250. The VANDELS survey: A strong correlation between Ly$\alpha$ equivalent width and stellar metallicity at $\mathbf{3\leq z \leq 5}$
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Cullen, F., McLure, R. J., Dunlop, J. S., Carnall, A. C., McLeod, D. J., Shapley, A. E., Amorín, R., Bolzonella, M., Castellano, M., Cimatti, A., Cirasuolo, M., Cucciati, O., Fontana, A., Fontanot, F., Garilli, B., Guaita, L., Jarvis, M. J., Pentericci, L., Pozzetti, L., Talia, M., Zamorani, G., Calabrò, A., Cresci, G., Fynbo, J. P. U., Hathi, N. P., Giavalisco, M., Koekemoer, A., Mannucci, F., and Saxena, A.
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Astrophysics - Astrophysics of Galaxies - Abstract
We present the results of a new study investigating the relationship between observed Ly$\alpha$ equivalent width ($W_{\lambda}$(Ly$\alpha$)) and the metallicity of the ionizing stellar population ($Z_{\star}$) for a sample of $768$ star-forming galaxies at $3 \leq z \leq 5$ drawn from the VANDELS survey. Dividing our sample into quartiles of rest-frame $W_{\lambda}$(Ly$\alpha$) across the range $-58 \unicode{xC5} \lesssim$ $W_{\lambda}$(Ly$\alpha$) $\lesssim 110 \unicode{xC5}$ we determine $Z_{\star}$ from full spectral fitting of composite far-ultraviolet (FUV) spectra and find a clear anti-correlation between $W_{\lambda}$(Ly$\alpha$) and $Z_{\star}$. Our results indicate that $Z_{\star}$ decreases by a factor $\gtrsim 3$ between the lowest $W_{\lambda}$(Ly$\alpha$) quartile ($\langle$$W_{\lambda}$(Ly$\alpha$)$\rangle=-18\unicode{xC5}$) and the highest $W_{\lambda}$(Ly$\alpha$) quartile ($\langle$$W_{\lambda}$(Ly$\alpha$)$\rangle=24\unicode{xC5}$). Similarly, galaxies typically defined as Lyman Alpha Emitters (LAEs; $W_{\lambda}$(Ly$\alpha$) $>20\unicode{xC5}$) are, on average, metal poor with respect to the non-LAE galaxy population ($W_{\lambda}$(Ly$\alpha$) $\leq20\unicode{xC5}$) with $Z_{\star}$$_{\rm{non-LAE}}\gtrsim 2 \times$ $Z_{\star}$$_{\rm{LAE}}$. Finally, based on the best-fitting stellar models, we estimate that the increasing strength of the stellar ionizing spectrum towards lower $Z_{\star}$ is responsible for $\simeq 15-25\%$ of the observed variation in $W_{\lambda}$(Ly$\alpha$) across our sample, with the remaining contribution ($\simeq 75-85\%$) being due to a decrease in the HI/dust covering fractions in low $Z_{\star}$ galaxies., Comment: 10 pages, 6 figures, MNRAS accepted
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- 2020
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