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1. Hemophagocytic Lymphohistiocytosis/Macrophage Activation Syndrome in pediatric Inflammatory Bowel Disease: clinical characteristics and outcomes

Author: Bramuzzo, Matteo, Cananzi, Mara, Alvisi, Patrizia, Cardile, Sabrina, Romano, Claudio, Aloi, Marina, Arrigo, Serena, Felici, Enrico, Lonoce, Luisa, Pieri, Elena Sofia, Scarallo, Luca, Strisciuglio, Caterina, Di Siena, Andrea, and Lega, Sara
Published: 2024
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2. Long−term health outcome and quality of life in children with multisystem inflammatory syndrome: findings from multidisciplinary follow−up at an Italian tertiary−care paediatric hospital

Author: D’Auria, Enza, Bova, Stefania Maria, Dallapiccola, Andrea Riccardo, De Santis, Raffaella, Leone, Alessandro, Calcaterra, Valeria, Mannarino, Savina, Garbin, Massimo, Olivotto, Sara, Zirpoli, Salvatore, Ghezzi, Michele, Munari, Alice Marianna, Verduci, Elvira, Farolfi, Andrea, Bosetti, Alessandra, Perico, Veronica, Capetti, Pietro, Gadda, Arianna, Gianolio, Laura, Lo Monaco, Germana, Lonoce, Luisa, Previtali, Roberto, Serafini, Ludovica, Taranto, Silvia, Veggiotti, Pierangelo, and Zuccotti, Gianvincenzo
Published: 2024
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3. Carbon and nitrogen stable isotopes reveal the human paleodiet evolution during the 8th-12th century in the Venetian Lagoon (Italy)

Author: Battistel, Dario, Viva, Serena, Turetta, Clara, Cadamuro, Silvia, Bonato, Emanuele, Giummolè, Federica, Lonoce, Norma, Barbante, Carlo, and Gelichi, Sauro
Published: 2024
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4. The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster

Author: Lonoce, Ilaria, Freedman, Wendy, and Feldmeier-Krause, Anja
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The Hydra I cluster offers an excellent opportunity to study and compare the relic old stellar populations in the core of its two brightest galaxies. In addition, the differing kinematics of the two galaxies allows a test of the local validity of general scaling relations. In this work we present a direct comparison employing full spectral fitting of new high-quality long-slit optical and NIR spectroscopic data. We retrieve age, metallicity and 19 elemental abundances out to about 12 kpc within each galaxy, as well as the IMF in their central regions. Our results suggest that the inner 5 kpc region of both galaxies, despite their different masses, formed at the same time and evolved with a similar star formation time-scale and chemical enrichment, confirming their early formation in the cluster build up. Only the overall metallicity and IMF radial profiles show differences connected with their different velocity dispersion profiles. The radial trend of the IMF positively correlates with both [Z/H] and velocity dispersion. While the trends of the IMF with metallicity agree with a global trend for both galaxies, the trends with the velocity dispersion exhibit differences. The outer regions show signs of mixed stellar populations with large differences in chemical content compared to the centers, but with similar old ages., Comment: 32 pages, 18 figures. Accepted for publication in ApJ
Published: 2023
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5. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author: Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J. E., Falcón-Barroso, Jesús, Gänsicke, Boris T., Hill, Vanessa, Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Smith, D. J. B., Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S., Antoja, Teresa, Aragón-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Barrena, R., Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J., Domínguez-Palmero, Lilian, Duncan, Kenneth J., Famaey, Benoit, Fariña, Cecilia, Gonzalez, Oscar A., Guest, Steve, Hatch, Nina A., Hess, Kelley M., Hoskin, Matthew J., Irwin, Mike, Knapen, Johan H., Koposov, Sergey E., Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Méndez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguió, Maria, Morrison, Sean, Murphy, David N. A., de Arriba, Luis Peralta, Pérez, Isabel, Pérez-Ràfols, Ignasi, Picó, Sergio, Raddi, Roberto, Romero-Gómez, Mercè, Royer, Frédéric, Siebert, Arnaud, Seabroke, George M., Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C. Clare, Alfaro, Emilio J., Prieto, Carlos Allende, Alonso-Santiago, Javier, Amos, Nicholas J., Ashley, Richard P., Balaguer-Núñez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R., Berlanas, Sara R., Bernard, Edouard J., Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M., Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Domínguez-Gómez, Jesús, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferré-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossat, Matteo, Franciosin, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, García-Benito, Rubén, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T. M., Delgado, Rosa M. González, Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P., Hardcastle, Martin J., Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J., Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, La Barbera, Francesco, Lam, Man I, Larsen, Søren S., Lemasle, Bertrand, Lewis, Ian J., Lhomé, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrin, Laura, Apellániz, Jesús Maíz, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F., Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escudé, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J., Naylor, Tim, Negueruela, Ignacio, Oñorbe, Jose, Pancino, Elena, Peirani, Sébastien, Peletier, Reynier F., Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C., Rossi, Elena Maria, Röttgering, Huub J. A., Rubiño-Martín, Jose Alberto, Montes, Jose Sabater, Juan, José San, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P., Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W., Simón-Díaz, Sergio, Smith, Russell J., Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A., Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J., Vergani, Daniela, Verheijen, Marc A. W., Verro, Kristiina, Vink, Jorick S., Vioque, Miguel, Walcher, C. Jakob, Walton, Nicholas A., Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L., Wilson, Andrew J., Wright, Nicholas J., Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, and Zurita, Cristina
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366$-$959\,nm at $R\sim5000$, or two shorter ranges at $R\sim20\,000$. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for $\sim$3 million stars and detailed abundances for $\sim1.5$ million brighter field and open-cluster stars; (ii) survey $\sim0.4$ million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey $\sim400$ neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in $z<0.5$ cluster galaxies; (vi) survey stellar populations and kinematics in $\sim25\,000$ field galaxies at $0.3\lesssim z \lesssim 0.7$; (vii) study the cosmic evolution of accretion and star formation using $>1$ million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at $z>2$. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator., Comment: 41 pages, 27 figures, accepted for publication by MNRAS; updated version including information on individual grants in a revised Acknowledgements section, corrections to the affiliation list, and an updated references list
Published: 2022
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6. Stellar Population and Elemental Abundance Gradients of Early-type Galaxies

Author: Feldmeier-Krause, A., Lonoce, I., and Freedman, W. L.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The evolution of galaxies is imprinted in their stellar populations. Several stellar population properties in massive early-type galaxies have been shown to correlate with intrinsic galaxy properties like the galaxy's central velocity dispersion, suggesting that stars formed in an initial collapse of gas (z~2). However, stellar populations change as a function of galaxy radius, and it is not clear how local gradients of individual galaxies are influenced by global galaxy properties and galaxy environment. In this paper, we study the stellar populations of eight early-type galaxies as a function of radius. We use optical spectroscopy (~4000-8600 \r{A}) and full-spectral fitting to measure stellar population age, metallicity, IMF slope, and nine elemental abundances (O, Mg, Si, Ca, Ti, C, N, Na, Fe) out to 1 R_e for each galaxy individually. We find a wide range of properties, with ages ranging from 3-13 Gyr. Some galaxies have a radially constant, Salpeter-like IMF, and other galaxies have a super-Salpeter IMF in the center, decreasing to a sub-Salpeter IMF at ~0.5 R_e. We find a global correlation of the central [Z/H] to the central IMF and the radial gradient of the IMF for the eight galaxies, but local correlations of the IMF slope to other stellar population parameters hold only for subsets of the galaxies in our sample. Some elemental abundances also correlate locally with each other within a galaxy, suggesting a common production channel. Those local correlations appear only in subsets of our galaxies indicating variations of the stellar content among different galaxies., Comment: 20 pages, 11 figures, 4 tables (37 pages, 17 figures, 6 tables incl. Appendix). Accepted for publication in ApJ
Published: 2021
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7. The Stellar Initial Mass Function and Population Properties of M89 from Optical and NIR Spectroscopy: Addressing Biases in Spectral Index Analysis

Author: Lonoce, Ilaria, Feldmeier-Krause, Anja, and Freedman, Wendy L.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The complexity of constraining the stellar initial mass function (IMF) in early-type galaxies cannot be overstated, given the necessity of both very high signal-to-noise (S/N) data and the difficulty of breaking the strong degeneracies that occur among several stellar population parameters including age, metallicity and elemental abundances. With this paper, the second in a series, we present a detailed analysis of the biases that can occur when retrieving the IMF shape by exploiting both optical and NIR IMF sensitive spectral indices. As a test case, here we analyze data for the nearby galaxy M89, for which we have high S/N spectroscopic data that cover the 3500-9000{\AA} spectral region and allow us to study the radial variation of the stellar population properties out to 1 R_e. Carrying out parallel simulations that mimic the retrieval of all the explored stellar parameters from a known input model, we quantify the amount of bias at each step of our analysis. From more general simulations we conclude that to accurately retrieve the IMF, it is necessary not only to retrieve accurate estimates of the age and metallicity, but also of all the elemental abundances that the spectral index fits are sensitive to. With our analysis technique applied to M89, we find consistency with a bottom-heavy IMF with a negative gradient from the center to half R_e when using the Conroy et al. 2018 as well as Vazdekis et al. 2016 EMILES stellar population models. We find agreement both with a parallel full spectral fitting of the same data and with literature results., Comment: 35 pages, 21 figures. Accepted for publication in ApJ
Published: 2021
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8. Measuring the stellar population parameters of the early-type galaxy NGC 3923 -- The challenging measurement of the initial mass function

Author: Feldmeier-Krause, A., Lonoce, I., and Freedman, W. L.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Recent studies of early-type galaxies have suggested that the initial mass function (IMF) slope is bottom-heavy, i.e. they contain a larger fraction of low-mass stars than the Milky Way. However, measurements of the IMF remain challenging in unresolved galaxies because features in their observed spectra are sensitive to a number of factors including the stellar age, metallicity, and elemental abundances, in addition to the IMF. In this paper, we use new high signal-to-noise IMACS (Magellan) spectra to study the elliptical shell galaxy NGC 3923 at optical (3700-6600 Angstrom), and near-infrared (7900-8500 Angstrom) wavelengths, as a function of radius. We have undertaken a number of independent approaches to better understand the uncertainties in our results. 1) We compare two different stellar population model libraries; 2) we undertake spectral index fitting as well as full spectral fitting; 3) we have performed simulations for which we a priori know the input IMF, and which closely match our data; 4) we also investigate the effects of including a two-component, rather than a single stellar population. We show that our results are sensitive to the assumptions we make and to the methods we use. In addition, we evaluate the accuracy and precision of our results based on simulated mock data. We find some indication (although assumption-dependent) for a bottom-heavy IMF in the mass-range 0.5-1.0 M_sun, while the IMF in the mass-range 0.08-0.5 M_sun appears to be Milky-Way like and constant. Including near-infrared data to our analysis gives consistent results, and improves the precision., Comment: 24 pages (37 pages incl. Appendix), 12 Figures (21), 6 Tables (7) Accepted for publication in ApJ
Published: 2020
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9. Bone marrow ectopic expression of a non-coding RNA in childhood T-cell acute lymphoblastic leukemia with a novel t(2;11)(q11.2;p15.1) translocation

Author: Leszl Anna, Panagopoulos Ioannis, Vasta Isabella, Caruso Sebastiano, D'Addabbo Pietro, Albano Francesco, Impera Luciana, Lonoce Angelo, Guastadisegni Maria, Basso Giuseppe, Rocchi Mariano, and Storlazzi Clelia
Subjects: Neoplasms. Tumors. Oncology. Including cancer and carcinogens, RC254-282
Abstract: Abstract Chromosomal translocations play a crucial role in tumorigenesis, often resulting in the formation of chimeric genes or in gene deregulation through position effects. T-cell acute lymphoblastic leukemia (T-ALL) is associated with a large number of such rearrangements. We report the ectopic expression of the 3' portion of EST DA926692 in the bone marrow of a childhood T-ALL case showing a t(2;11)(q11.2;p15.1) translocation as the sole chromosome abnormality. The breakpoints, defined at the sequence level, mapped within HPS5 (Hermansky Pudlak syndrome 5) intron 1 at 11p15.1, and DA926692 exon 2 at 2q11.2. The translocation was accompanied by a submicroscopic inversion that brought the two genes into the same transcriptional orientation. No chimeric trancript was detected. Interestingly, Real-Time Quantitative (RQ)-PCR detected, in the patient's bone marrow, expression of a 173 bp product corresponding to the 3' portion of DA926692. Samples from four T-ALL cases with a normal karyotype and normal bone marrow used as controls were negative. It might be speculated that the juxtaposition of this genomic segment to the CpG island located upstream HPS5 activated DA92669 expression. RQ-PCR analysis showed expression positivity in 6 of 23 human tissues examined. Bioinformatic analysis excluded that this small non-coding RNA is a precursor of micro-RNA, although it is conceivable that it has a different, yet unknown, functional role. To the best of our knowledge, this is the first report, in cancer, of the activation of a small non-coding RNA as a result of a chromosomal translocation.
Published: 2008
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10. Dual biological therapy and small molecules in pediatric inflammatory bowel disease

Author: Francesca Penagini, Luisa Lonoce, Luisa Abbattista, Valentina Silvera, Giulia Rendo, Lucia Cococcioni, Dario Dilillo, Valeria Calcaterra, and Gian Vincenzo Zuccotti
Subjects: Inflammatory Bowel Disease, Pediatric, Dual biological Therapy, Small molecules, Therapeutics. Pharmacology, RM1-950
Abstract: Inflammatory bowel diseases (IBDs) including Crohn’s disease (CD), ulcerative colitis (UC) and inflammatory bowel disease unclassified (IBD-U) are chronic inflammatory disorders which can affect the gastrointestinal tract. Anti-tumor necrosis factors antibodies (anti-TNFα) such as infliximab (IFX) and adalimumab (ADA) are the first line biological therapy for severe or complicated IBDs in pediatric age. Second line therapeutic options as vedolizumab (VDZ) and ustekinumab (UST) are currently used off-label in pediatric age. Furthermore, despite optimization of biologics, a great proportion of patients may fail to respond to biologic agents (up to 30%) or lose response over the time (around 50%) hence these patients may be left without another valid therapeutic option. Consequently, several efforts have been made in the last years in order to develop new drugs and to contrive new therapeutic strategies. Small molecule drugs (SMDs) and combination therapy with either two biologic agents or with a SMD and a biological agent have recently been proposed. Data on safety and efficacy of these new therapeutic options are limited. The objective of the present review is to summarize the most up-to-date available literature in pediatric IBD.
Published: 2023
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11. Stellar population properties of individual massive early-type galaxies at 1.4 < z < 2

Author: Lonoce, I., Maraston, C., Thomas, D., Longhetti, M., Parikh, T., Guarnieri, P., and Comparat, J.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We analyse publicly available, individual spectra of four, massive ($M>10^{11}M_{\odot}$) early-type galaxies with redshifts in the range 1.4 < z < 2 to determine their stellar content, extending our previous work up to z~2. The wide wavelength range of the VLT/X-Shooter spectroscopic data in the UV-Optical-NIR arms along with the availability of spectro-photometry allows us to explore different techniques to obtain the stellar population properties, namely through age/metallicity sensitive spectral indices, full spectral fitting and broad-band photometric fitting. Moreover, together with the widely used optical Lick indices we consider further indices in the UV rest-frame, and demonstrate that UV indices significantly help the accuracy of the resulting population parameters. We find galaxy ages ranging from 0.2 to 4 Gyr, where the oldest galaxy is found at the lowest redshift, with an excellent agreement between ages determined via indices, full spectral fitting or broad-band colours. These ages are in perfect agreement with ages of local galaxies at the same velocity dispersion when we assume pure passive evolution. Total metallicities derived from indices show some scatter (between less than half-solar to very high values, ([Z/H]~0.6]). We speculate on possible mechanisms explaining these values, but given the sample size and low S/N of the spectra no conclusion can be made. Indices in the UV-rest frame generally lead to similar conclusions as optical indices. For the oldest galaxy (4 Gyr) we show that its UV-indices can only be explained by stellar population models including a UV contribution from old stellar populations, suggesting that old, UV bright populations start to inhabit mature galaxies of a few Gyr of age. This is the highest redshift (z~1.4) detection of the UV-upturn up to date., Comment: 23 pages, Accepted for publication in MNRAS
Published: 2019
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12. A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE

Author: Costantin, L., Iovino, A., Zibetti, S., Longhetti, M., Gallazzi, A., Mercurio, A., Lonoce, I., Balcells, M., Bolzonella, M., Busarello, G., Dalton, G., Ferré-Mateu, A., García-Benito, R., Gargiulo, A., Haines, C., Jin, S., La Barbera, F., McGee, S., Merluzzi, P., Morelli, L., Murphy, D. N. A., de Arriba, L. Peralta, Pizzella, A., Poggianti, B. M., Pozzetti, L., Sánchez-Blázquez, P., Talia, M., Tortora, C., Trager, S. C., Vazdekis, A., Vergani, D., and Vulcani, B.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide invaluable information for reconstructing the history of star formation in individual galaxies up to redshifts of about 0.7. We aim at defining simple but robust and meaningful physical parameters that can be used to trace the coexistence of widely diverse stellar components: younger stellar populations superimposed on the bulk of older ones. We produce spectra of galaxies closely mimicking data from the forthcoming Stellar Populations at intermediate redshifts Survey (StePS), a survey that uses the WEAVE spectrograph on the William Herschel Telescope. First, we assess our ability to reliably measure both ultraviolet and optical spectral indices in galaxies of different spectral types for typically expected signal-to-noise levels. Then, we analyze such mock spectra with a Bayesian approach, deriving the probability density function of r- and u-band light-weighted ages as well as of their difference. We find that the ultraviolet indices significantly narrow the uncertainties in estimating the r- and u-band light-weighted ages and their difference in individual galaxies. These diagnostics, robustly retrievable for large galaxy samples even when observed at moderate signal-to-noise ratios, allow us to identify secondary episodes of star formation up to an age of ~0.1 Gyr for stellar populations older than ~1.5 Gyr, pushing up to an age of ~1 Gyr for stellar populations older than ~5 Gyr. The difference between r-band and u-band light-weighted ages is shown to be a powerful diagnostic to characterize and constrain extended star-formation histories and the presence of young stellar populations on top of older ones. This parameter can be used to explore the interplay between different galaxy star-formation histories and physical parameters such as galaxy mass, size, morphology, and environment., Comment: 18 pages, 20 figures, accepted for publication in A&A
Published: 2019
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13. An unexpected demographic regime: The western necropolis of the Greek colony of Himera (Sicily, Italy) (550-409 BCE)

Author: Lonoce, Norma, Dalla-Zuanna, Gianpiero, Fabbri, Pier Francesco, Vassallo, Stefano, and Barbiera, Irene
Published: 2023
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14. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author: Jin, S, Trager, S, Dalton, G, Aguerri, J, Drew, J, Falcón-Barroso, J, Gänsicke, B, Hill, V, Iovino, A, Pieri, M, Poggianti, B, Smith, D, Vallenari, A, Abrams, D, Aguado, D, Antoja, T, Aragón-Salamanca, A, Ascasibar, Y, Babusiaux, C, Balcells, M, Barrena, R, Battaglia, G, Belokurov, V, Bensby, T, Bonifacio, P, Bragaglia, A, Carrasco, E, Carrera, R, Cornwell, D, Domínguez-Palmero, L, Duncan, K, Famaey, B, Fari na, C, Gonzalez, O, Guest, S, Hatch, N, Hess, K, Hoskin, M, Irwin, M, Knapen, J, Koposov, S, Kuchner, U, Laigle, C, Lewis, J, Longhetti, M, Lucatello, S, Méndez-Abreu, J, Mercurio, A, Molaeinezhad, A, Monguió, M, Morrison, S, Murphy, D, de Arriba, L, Pérez, I, Pérez-Ràfols, I, Picó, S, Raddi, R, Romero-Gómez, M, Royer, F, Siebert, A, Seabroke, G, Som, D, Terrett, D, Thomas, G, Wesson, R, Worley, C, Alfaro, E, Prieto, C, Alonso-Santiago, J, Amos, N, Ashley, R, Balaguer-Nú nez, L, Balbinot, E, Bellazzini, M, Benn, C, Berlanas, S, Bernard, E, Best, P, Bettoni, D, Bianco, A, Bishop, G, Blomqvist, M, Boeche, C, Bolzonella, M, Bonoli, S, Bosma, A, Britavskiy, N, Busarello, G, Caffau, E, Cantat-Gaudin, T, Castro-Ginard, A, Couto, G, Carbajo-Hijarrubia, J, Carter, D, Casamiquela, L, Conrado, A, Corcho-Caballero, P, Costantin, L, Deason, A, de Burgos, A, De Grandi, S, Di Matteo, P, Domínguez-Gómez, J, Dorda, R, Drake, A, Dutta, R, Erkal, D, Feltzing, S, Ferré-Mateu, A, Feuillet, D, Figueras, F, Fossati, M, Franciosini, E, Frasca, A, Fumagalli, M, Gallazzi, A, García-Benito, R, Fusillo, N, Gebran, M, Gilbert, J, Gledhill, T, Delgado, R, Greimel, R, Guarcello, M, Guerra, J, Gullieuszik, M, Haines, C, Hardcastle, M, Harris, A, Haywood, M, Helmi, A, Hernandez, N, Herrero, A, Hughes, S, Irsic, V, Jablonka, P, Jarvis, M, Jordi, C, Kondapally, R, Kordopatis, G, Krogager, J, Barbera, F, Lam, M, Larsen, S, Lemasle, B, Lewis, I, Lhomé, E, Lind, K, Lodi, M, Longobardi, A, Lonoce, I, Magrini, L, Apellániz, J, Marchal, O, Marco, A, Martin, N, Matsuno, T, Maurogordato, S, Merluzzi, P, Miralda-Escudé, J, Molinari, E, Monari, G, Morelli, L, Mottram, C, Naylor, T, Negueruela, I, Onorbe, J, Pancino, E, Peirani, S, Peletier, R, Pozzetti, L, Rainer, M, Ramos, P, Read, S, Rossi, E, Röttgering, H, Rubi no-Martín, J, Montes, J, Juan, J, Sanna, N, Schallig, E, Schiavon, R, Schultheis, M, Serra, P, Shimwell, T, Simón-Díaz, S, Smith, R, Sordo, R, Sorini, D, Soubiran, C, Starkenburg, E, Steele, I, Stott, J, Stuik, R, Tolstoy, E, Tortora, C, Tsantaki, M, Van der Swaelmen, M, van Weeren, R, Vergani, D, Verheijen, M, Verro, K, Vink, J, Vioque, M, Walcher, C, Walton, N, Wegg, C, Weijmans, A, Williams, W, Wilson, A, Wright, N, Xylakis-Dornbusch, T, Youakim, K, Zibetti, S, Zurita, C, Jin, Shoko, Trager, Scott C, Dalton, Gavin B, Aguerri, J Alfonso L, Drew, J E, Falcón-Barroso, Jesús, Gänsicke, Boris T, Hill, Vanessa, Iovino, Angela, Pieri, Matthew M, Poggianti, Bianca M, Smith, D J B, Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S, Antoja, Teresa, Aragón-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J, Domínguez-Palmero, Lilian, Duncan, Kenneth J, Famaey, Benoit, Fari na, Cecilia, Gonzalez, Oscar A, Guest, Steve, Hatch, Nina A, Hess, Kelley M, Hoskin, Matthew J, Irwin, Mike, Knapen, Johan H, Koposov, Sergey E, Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Méndez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguió, Maria, Morrison, Sean, Murphy, David N A, de Arriba, Luis Peralta, Pérez, Isabel, Pérez-Ràfols, Ignasi, Picó, Sergio, Raddi, Roberto, Romero-Gómez, Mercè, Royer, Frédéric, Siebert, Arnaud, Seabroke, George M, Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C Clare, Alfaro, Emilio J, Prieto, Carlos Allende, Alonso-Santiago, Javier, Amos, Nicholas J, Ashley, Richard P, Balaguer-Nú nez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R, Berlanas, Sara R, Bernard, Edouard J, Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M, Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Domínguez-Gómez, Jesús, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferré-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossati, Matteo, Franciosini, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, García-Benito, Rubén, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T M, Delgado, Rosa M González, Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P, Hardcastle, Martin J, Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J, Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, Barbera, Francesco La, Lam, Man I, Larsen, Søren S, Lemasle, Bertrand, Lewis, Ian J, Lhomé, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrini, Laura, Apellániz, Jesús Maíz, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F, Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escudé, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J, Naylor, Tim, Negueruela, Ignacio, Onorbe, Jose, Pancino, Elena, Peirani, Sébastien, Peletier, Reynier F, Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C, Rossi, Elena Maria, Röttgering, Huub J A, Rubi no-Martín, Jose Alberto, Montes, Jose Sabater, Juan, José San, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P, Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W, Simón-Díaz, Sergio, Smith, Russell J, Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A, Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J, Vergani, Daniela, Verheijen, Marc A W, Verro, Kristiina, Vink, Jorick S, Vioque, Miguel, Walcher, C Jakob, Walton, Nicholas A, Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L, Wilson, Andrew J, Wright, Nicholas J, Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, Zurita, Cristina, Jin, S, Trager, S, Dalton, G, Aguerri, J, Drew, J, Falcón-Barroso, J, Gänsicke, B, Hill, V, Iovino, A, Pieri, M, Poggianti, B, Smith, D, Vallenari, A, Abrams, D, Aguado, D, Antoja, T, Aragón-Salamanca, A, Ascasibar, Y, Babusiaux, C, Balcells, M, Barrena, R, Battaglia, G, Belokurov, V, Bensby, T, Bonifacio, P, Bragaglia, A, Carrasco, E, Carrera, R, Cornwell, D, Domínguez-Palmero, L, Duncan, K, Famaey, B, Fari na, C, Gonzalez, O, Guest, S, Hatch, N, Hess, K, Hoskin, M, Irwin, M, Knapen, J, Koposov, S, Kuchner, U, Laigle, C, Lewis, J, Longhetti, M, Lucatello, S, Méndez-Abreu, J, Mercurio, A, Molaeinezhad, A, Monguió, M, Morrison, S, Murphy, D, de Arriba, L, Pérez, I, Pérez-Ràfols, I, Picó, S, Raddi, R, Romero-Gómez, M, Royer, F, Siebert, A, Seabroke, G, Som, D, Terrett, D, Thomas, G, Wesson, R, Worley, C, Alfaro, E, Prieto, C, Alonso-Santiago, J, Amos, N, Ashley, R, Balaguer-Nú nez, L, Balbinot, E, Bellazzini, M, Benn, C, Berlanas, S, Bernard, E, Best, P, Bettoni, D, Bianco, A, Bishop, G, Blomqvist, M, Boeche, C, Bolzonella, M, Bonoli, S, Bosma, A, Britavskiy, N, Busarello, G, Caffau, E, Cantat-Gaudin, T, Castro-Ginard, A, Couto, G, Carbajo-Hijarrubia, J, Carter, D, Casamiquela, L, Conrado, A, Corcho-Caballero, P, Costantin, L, Deason, A, de Burgos, A, De Grandi, S, Di Matteo, P, Domínguez-Gómez, J, Dorda, R, Drake, A, Dutta, R, Erkal, D, Feltzing, S, Ferré-Mateu, A, Feuillet, D, Figueras, F, Fossati, M, Franciosini, E, Frasca, A, Fumagalli, M, Gallazzi, A, García-Benito, R, Fusillo, N, Gebran, M, Gilbert, J, Gledhill, T, Delgado, R, Greimel, R, Guarcello, M, Guerra, J, Gullieuszik, M, Haines, C, Hardcastle, M, Harris, A, Haywood, M, Helmi, A, Hernandez, N, Herrero, A, Hughes, S, Irsic, V, Jablonka, P, Jarvis, M, Jordi, C, Kondapally, R, Kordopatis, G, Krogager, J, Barbera, F, Lam, M, Larsen, S, Lemasle, B, Lewis, I, Lhomé, E, Lind, K, Lodi, M, Longobardi, A, Lonoce, I, Magrini, L, Apellániz, J, Marchal, O, Marco, A, Martin, N, Matsuno, T, Maurogordato, S, Merluzzi, P, Miralda-Escudé, J, Molinari, E, Monari, G, Morelli, L, Mottram, C, Naylor, T, Negueruela, I, Onorbe, J, Pancino, E, Peirani, S, Peletier, R, Pozzetti, L, Rainer, M, Ramos, P, Read, S, Rossi, E, Röttgering, H, Rubi no-Martín, J, Montes, J, Juan, J, Sanna, N, Schallig, E, Schiavon, R, Schultheis, M, Serra, P, Shimwell, T, Simón-Díaz, S, Smith, R, Sordo, R, Sorini, D, Soubiran, C, Starkenburg, E, Steele, I, Stott, J, Stuik, R, Tolstoy, E, Tortora, C, Tsantaki, M, Van der Swaelmen, M, van Weeren, R, Vergani, D, Verheijen, M, Verro, K, Vink, J, Vioque, M, Walcher, C, Walton, N, Wegg, C, Weijmans, A, Williams, W, Wilson, A, Wright, N, Xylakis-Dornbusch, T, Youakim, K, Zibetti, S, Zurita, C, Jin, Shoko, Trager, Scott C, Dalton, Gavin B, Aguerri, J Alfonso L, Drew, J E, Falcón-Barroso, Jesús, Gänsicke, Boris T, Hill, Vanessa, Iovino, Angela, Pieri, Matthew M, Poggianti, Bianca M, Smith, D J B, Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S, Antoja, Teresa, Aragón-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J, Domínguez-Palmero, Lilian, Duncan, Kenneth J, Famaey, Benoit, Fari na, Cecilia, Gonzalez, Oscar A, Guest, Steve, Hatch, Nina A, Hess, Kelley M, Hoskin, Matthew J, Irwin, Mike, Knapen, Johan H, Koposov, Sergey E, Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Méndez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguió, Maria, Morrison, Sean, Murphy, David N A, de Arriba, Luis Peralta, Pérez, Isabel, Pérez-Ràfols, Ignasi, Picó, Sergio, Raddi, Roberto, Romero-Gómez, Mercè, Royer, Frédéric, Siebert, Arnaud, Seabroke, George M, Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C Clare, Alfaro, Emilio J, Prieto, Carlos Allende, Alonso-Santiago, Javier, Amos, Nicholas J, Ashley, Richard P, Balaguer-Nú nez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R, Berlanas, Sara R, Bernard, Edouard J, Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M, Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Domínguez-Gómez, Jesús, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferré-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossati, Matteo, Franciosini, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, García-Benito, Rubén, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T M, Delgado, Rosa M González, Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P, Hardcastle, Martin J, Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J, Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, Barbera, Francesco La, Lam, Man I, Larsen, Søren S, Lemasle, Bertrand, Lewis, Ian J, Lhomé, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrini, Laura, Apellániz, Jesús Maíz, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F, Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escudé, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J, Naylor, Tim, Negueruela, Ignacio, Onorbe, Jose, Pancino, Elena, Peirani, Sébastien, Peletier, Reynier F, Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C, Rossi, Elena Maria, Röttgering, Huub J A, Rubi no-Martín, Jose Alberto, Montes, Jose Sabater, Juan, José San, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P, Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W, Simón-Díaz, Sergio, Smith, Russell J, Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A, Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J, Vergani, Daniela, Verheijen, Marc A W, Verro, Kristiina, Vink, Jorick S, Vioque, Miguel, Walcher, C Jakob, Walton, Nicholas A, Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L, Wilson, Andrew J, Wright, Nicholas J, Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, and Zurita, Cristina
Abstract: WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2-deg field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable ‘mini’ integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366–959 nm at R ∼ 5000, or two shorter ranges at R ∼ 20 000. After summarizing the design and implementation of WEAVE and its data systems, we present the organization, science drivers, and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy’s origins by completing Gaia’s phase-space information, providing metallicities to its limiting magnitude for ∼3 million stars and detailed abundances for ∼1.5 million brighter field and open-cluster stars; (ii) survey ∼0.4 million Galactic-plane OBA stars, young stellar objects, and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey ∼400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionized gas in z < 0.5 cluster galaxies; (vi) survey stellar populations and kinematics in ∼25 000 field galaxies at 0.3 ≲ z ≲ 0.7; (vii) study the cosmic evolution of accretion and star formation using >1 million spectra of LOFAR-selected radio sources; and (viii) trace structures using intergalactic/circumgalactic gas at z > 2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.
Published: 2024

15. Dual Biological Therapy and Small Molecules in pediatric Inflammatory Bowel Disease

Author: Penagini, Francesca, Lonoce, Luisa, Abbattista, Luisa, Silvera, Valentina, Rendo, Giulia, Cococcioni, Lucia, Dilillo, Dario, Calcaterra, Valeria, and Zuccotti, Gian Vincenzo
Published: 2023
Full Text: View/download PDF

16. Ultramassive dense early-type galaxies: velocity dispersions and number density evolution since z=1.6

Author: Gargiulo, A., Saracco, P., Tamburri, S., Lonoce, I., and Ciocca, F.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: In this paper we investigate the mass assembly history of ultramassive (Mstar > 10^11Msun) dense (Sigma = Mstar/(2*pi*Re^2) > 2500 Msun/pc^2) early-type galaxies (ETGs) over the last 9 Gyr. We have traced the evolution of the number density rho of ultramassive dense ETGs and have compared their structural (effective radius Re and stellar mass Mstar) and dynamical (velocity dispersion sigma_e) parameters over the redshift range 0 < z < 1.6. We have derived the number density at 1.6 < z < 1 from the MUNICS and GOODS-South surveys, while we have used the COSMOS and SDSS spectroscopic surveys to probe the intermediate and local redshift range. For the comparison of the dynamical and structural parameters, we have collected the ultramassive dense ETGs at 1.2 < z < 1.6 for which velocity dispersion measurements are available (11 ETGs). For 4 of them we present unpublished estimates of sigma_e. We probe the intermediate redshift range, and the local universe using the samples of ETGs by Saglia et al. (2010), Zahid et al. (2015), and by Thomas et al. (2010). We find that the number density of ultramassive dense ETGs evolves as rho(z) = K*(1 + z)^(0.3\pm0.8) implying a decrease of ~ 25% of the population since z = 1.6. By comparing the values of Re, Mstar, and sigma_e of ultramassive dense ETGs over the range 0 < z < 1.6 we find that all the high-z ETGs have a counterpart in the local universe. This implies either that the majority (~70%) of ultramassive dense ETGs has already completed its assembly and its shaping at = 1.4, or that, if a significant fraction of them evolves in size, new ultramassive dense ETGs must form at z < 1.5 to maintain their number density almost constant. The difficulty into identify good progenitors for these new dense ETGs at z < 1.5, and the stellar populations properties of local ultramassive dense ETGs point toward the first hypothesis., Comment: 22 pages, 16 figures, accepted for publication in A&A
Published: 2016
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17. The wide-field, multiplexed, spectroscopic facility WEAVE : Survey design, overview, and simulated implementation

Author: Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J. E., Falcon-Barroso, Jesus, Gaensicke, Boris T., Hill, Vanessa, Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Smith, D. J. B., Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S., Antoja, Teresa, Aragon-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Barrena, R., Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J., Dominguez-Palmero, Lilian, Duncan, Kenneth J., Famaey, Benoit, Farina, Cecilia, Gonzalez, Oscar A., Guest, Steve, Hatch, Nina A., Hess, Kelley M., Hoskin, Matthew J., Irwin, Mike, Knapen, Johan H., Koposov, Sergey E., Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Mendez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguio, Maria, Morrison, Sean, Murphy, David N. A., de Arriba, Luis Peralta, Perez, Isabel, Perez-Rafols, Ignasi, Pico, Sergio, Raddi, Roberto, Romero-Gomez, Merce, Royer, Frederic, Siebert, Arnaud, Seabroke, George M., Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C. Clare, Alfaro, Emilio J., Allende Prieto, Carlos, Alonso-Santiago, Javier, Amos, Nicholas J., Ashley, Richard P., Balaguer-Nunez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R., Berlanas, Sara R., Bernard, Edouard J., Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M., Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Dominguez-Gomez, Jesus, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferre-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossati, Matteo, Franciosini, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, Garcia-Benito, Ruben, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T. M., Gonzalez Delgado, Rosa M., Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P., Hardcastle, Martin J., Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J., Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, La Barbera, Francesco, Lam, Man I., Larsen, Sren S., Lemasle, Bertrand, Lewis, Ian J., Lhome, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrini, Laura, Maiz Apellaniz, Jesus, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F., Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escude, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J., Naylor, Tim, Negueruela, Ignacio, Onorbe, Jose, Pancino, Elena, Peirani, Sebastien, Peletier, Reynier F., Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C., Rossi, Elena Maria, Roettgering, Huub J. A., Rubino-Martin, Jose Alberto, Sabater, Jose, San Juan, Jose, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P., Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W., Simon-Diaz, Sergio, Smith, Russell J., Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A., Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J., Vergani, Daniela, Verheijen, Marc A. W., Verro, Kristiina, Vink, Jorick S., Vioque, Miguel, Walcher, C. Jakob, Walton, Nicholas A., Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L., Wilson, Andrew J., Wright, Nicholas J., Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, Zurita, Cristina, Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J. E., Falcon-Barroso, Jesus, Gaensicke, Boris T., Hill, Vanessa, Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Smith, D. J. B., Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S., Antoja, Teresa, Aragon-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Barrena, R., Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J., Dominguez-Palmero, Lilian, Duncan, Kenneth J., Famaey, Benoit, Farina, Cecilia, Gonzalez, Oscar A., Guest, Steve, Hatch, Nina A., Hess, Kelley M., Hoskin, Matthew J., Irwin, Mike, Knapen, Johan H., Koposov, Sergey E., Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Mendez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguio, Maria, Morrison, Sean, Murphy, David N. A., de Arriba, Luis Peralta, Perez, Isabel, Perez-Rafols, Ignasi, Pico, Sergio, Raddi, Roberto, Romero-Gomez, Merce, Royer, Frederic, Siebert, Arnaud, Seabroke, George M., Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C. Clare, Alfaro, Emilio J., Allende Prieto, Carlos, Alonso-Santiago, Javier, Amos, Nicholas J., Ashley, Richard P., Balaguer-Nunez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R., Berlanas, Sara R., Bernard, Edouard J., Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M., Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Dominguez-Gomez, Jesus, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferre-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossati, Matteo, Franciosini, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, Garcia-Benito, Ruben, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T. M., Gonzalez Delgado, Rosa M., Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P., Hardcastle, Martin J., Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J., Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, La Barbera, Francesco, Lam, Man I., Larsen, Sren S., Lemasle, Bertrand, Lewis, Ian J., Lhome, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrini, Laura, Maiz Apellaniz, Jesus, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F., Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escude, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J., Naylor, Tim, Negueruela, Ignacio, Onorbe, Jose, Pancino, Elena, Peirani, Sebastien, Peletier, Reynier F., Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C., Rossi, Elena Maria, Roettgering, Huub J. A., Rubino-Martin, Jose Alberto, Sabater, Jose, San Juan, Jose, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P., Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W., Simon-Diaz, Sergio, Smith, Russell J., Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A., Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J., Vergani, Daniela, Verheijen, Marc A. W., Verro, Kristiina, Vink, Jorick S., Vioque, Miguel, Walcher, C. Jakob, Walton, Nicholas A., Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L., Wilson, Andrew J., Wright, Nicholas J., Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, and Zurita, Cristina
Abstract: WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2-deg field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366-959nm at R similar to 5000, or two shorter ranges at . After summarizing the design and implementation of WEAVE and its data systems, we present the organization, science drivers, and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for similar to 3 million stars and detailed abundances for similar to 1.5 million brighter field and open-cluster stars; (ii) survey similar to 0.4 million Galactic-plane OBA stars, young stellar objects, and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey similar to 400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionized gas in z < 0.5 cluster galaxies; (vi) survey stellar populations and kinematics in field galaxies at 0.3 less than or similar to z less than or similar to 0.7; (vii) study the cosmic evolution of accretion and star formation using >1 million spectra of LOFAR-selected radio sources; and (viii) trace structures using intergalactic/circumgalactic gas at z > 2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.
Published: 2024
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18. Old age and super-solar metallicity in a massive z~1.4 early-type galaxy from VLT/X-Shooter spectroscopy

Author: Lonoce, Ilaria, Longhetti, Marcella, Maraston, Claudia, Thomas, Daniel, Mancini, Chiara, Cimatti, Andrea, Ciocca, Federica, Citro, Annalisa, Daddi, Emanuele, Alighieri, Sperello di Serego, Gargiulo, Adriana, Maiolino, Roberto, Mannucci, Filippo, Moresco, Michele, Pozzetti, Lucia, Quai, Salvatore, and Saracco, Paolo
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the first estimate of age, stellar metallicity and chemical abundance ratios, for an individual early-type galaxy at high-redshift (z = 1.426) in the COSMOS field. Our analysis is based on observations obtained with the X-Shooter instrument at the VLT, which cover the visual and near infrared spectrum at high (R >5000) spectral resolution. We measure the values of several spectral absorptions tracing chemical species, in particular Magnesium and Iron, besides determining the age-sensitive D4000 break. We compare the measured indices to stellar population models, finding good agreement. We find that our target is an old (t > 3 Gyr), high-metallicity ([Z/H] > 0.5) galaxy which formed its stars at z_{form} > 5 within a short time scale ~0.1 Gyr, as testified by the strong [\alpha/Fe] ratio ( > 0.4), and has passively evolved in the first > 3-4 Gyr of its life. We have verified that this result is robust against the choice and number of fitted spectral features, and stellar population model. The result of an old age and high-metallicity has important implications for galaxy formation and evolution confirming an early and rapid formation of the most massive galaxies in the Universe., Comment: 8 pages, 7 figures, accepted for publication in MNRAS
Published: 2015
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19. Carbon and nitrogen stable isotopes reveal the human paleodiet evolution during the 8th-12th century in the Venetian Lagoon (Italy)

Author: Battistel, Dario, Viva, Serena, Turetta, Clara, Cadamuro, Silvia, Bonato, Emanuele, Giummolè, Federica, Lonoce, Norma, Barbante, Carlo, and Gelichi, Sauro
Abstract: The paleodiet evolution in a human community of Venetian Lagoon between the eighth and twelfth centuries has been reconstructed by the stable isotopes analysis of δ13C and δ15N found in collagen of teeth and bones from St. Mauro archaeological site (Jesolo, Venice). A total of 52 individuals of various ages, sex, chronologies, and pathological condition were included in this study. Our findings revealed the presence of two distinct dietary patterns influenced only by chronology. We observed that a more fish-based diet (30–60% of the overall diet) prevailed between the eighth and tenth centuries. However, between the tenth and twelfth centuries, fish consumption decreased (10–30% of the overall diet), and there was a shift towards a diet rich in terrestrial protein sources. We link this change in dietary habits to economic development also evidenced by the transformations of the site and increased trade with the hinterland. Furthermore, it was observed significantly higher δ15N values in individuals from 8th-10th compared to those from tenth-twelfth centuries. We proposed two potential explanations: a shift in child-rearing practices, such as delayed weaning during early middle age compared to late middle age, or a change in diet of breast feeders. [ABSTRACT FROM AUTHOR]
Published: 2024
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20. A novel method for the isolation of single cells mimicking circulating tumour cells adhered on Smart Bio Surface slides by Laser Capture Microdissection

Author: Visci, Grazia, primary, Tolomeo, Doron, additional, Lonoce, Angelo, additional, Arshadi, Aram, additional, Bascetta, Lorenzo, additional, Trotta, Gianluca, additional, van Riel, Margot, additional, Vermeesch, Joris Robert, additional, Carbone, Roberta, additional, and Storlazzi, Clelia Tiziana, additional
Published: 2024
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21. Long-Term Health Outcome and Quality of Life in Children with Multisystem Inflammatory Syndrome: Findings from Multidisciplinary Follow Up at an Italian Tertiary-Care Paediatric Hospital

Author: D'Auria, Enza, primary, Bova, Stefania Maria, additional, Dallapiccola, Andrea Riccardo, additional, De Santis, Raffaella, additional, Leone, Alessandro, additional, Calcaterra, Valeria, additional, Mannarino, Savina, additional, Garbin, Massimo, additional, Olivotto, Sara, additional, Zirpoli, Salvatore, additional, Ghezzi, Michele, additional, Munari, Alice Marianna, additional, Verduci, Elvira, additional, Farolfi, Andrea, additional, Bosetti, Alessandra, additional, Perico, Veronica, additional, Capetti, Pietro, additional, Gadda, Arianna, additional, Gianolio, Laura, additional, Lo Monaco, Germana, additional, Lonoce, Luisa, additional, Previtali, Roberto, additional, Serafini, Ludovica, additional, Taranto, Silvia, additional, Veggiotti, Pierangelo, additional, and Zuccotti, Gian Vincenzo, additional
Published: 2024
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22. Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ~ 1.4

Author: Gargiulo, A., Saracco, P., Longhetti, M., Tamburri, S., Lonoce, I., and Ciocca, F.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: This paper aims at understanding if the normalization of the stellar initial mass function (IMF) of massive early-type galaxies (ETGs) varies with cosmic time and/or with mean stellar mass density Sigma (M*/2\pi Re^2). For this purpose we collected a sample of 18 dense (Sigma>2500 M_sun/pc^2) ETGs at 1.2 = 1.4 follow the same IMF-sigma_e trend of typical local ETGs, but with a lower mass-normalization. Nonetheless, once the IMF-sigma_e trend we have found for high-z dense ETGs is compared with that of local ETGs with similar Sigma and sigma_e, they turn out to be consistent. The similarity between the IMF-sigma_e trends of dense high-z and low-z ETGs over 9 Gyr of evolution and their lower mass-normalization with respect to the mean value of local ETGs suggest that, independently on formation redshift, the physical conditions characterizing the formation of a dense spheroid lead to a mass spectrum of new formed stars with an higher ratio of high- to low-mass stars with respect to the IMF of normal local ETGs., Comment: 9 pages, 4 figures, accepted for pubblication in A&A, updated to match final journal version
Published: 2014
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23. Spectral detection of multiple stellar populations in z~1 early-type galaxies

Author: Lonoce, I., Longhetti, M., Saracco, P., Gargiulo, A., and Tamburri, S.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a spectroscopic analysis based on measurements of two mainly age-dependent spectrophotometric indices in the 4000A rest frame region, i.e. H+K(CaII) and Delta4000, for a sample of 15 early-type galaxies (ETGs) at 0.7 < z_{spec} < 1.1, morphologically selected in the GOODS-South field. Ages derived from the two different indices by means of the comparison with stellar population synthesis models, are not consistent with each other for at least nine galaxies (60 per cent of the sample), while for the remaining six galaxies, the ages derived from their global spectral energy distribution (SED) fitting are not consistent with those derived from the two indices. We then hypothesized that the stellar content of many galaxies is made of two stellar components with different ages. The double-component analysis, performed by taking into account both the index values and the observed SED, fully explains the observational data and improves the results of the standard one-component SED fitting in 9 out of the 15 objects, i.e. those for which the two indices point towards two different ages. In all of them, the bulk of the mass belongs to rather evolved stars, while a small mass fraction is many Gyr younger. In some cases, thanks to the sensitivity of the H+K(CaII) index, we find that the minor younger component reveals signs of recent star formation. The distribution of the ages of the younger stellar components appears uniformly in time and this suggests that small amounts of star formation could be common during the evolution of high-z ETGs. We argue the possibility that these new star formation episodes could be frequently triggered by internal causes due to the presence of small gas reservoir., Comment: 18 pages, 12 figures. Accepted for publication in MNRAS
Published: 2014
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24. The population of early-type galaxies: how it evolves with time and how it differs from passive and late-type galaxies

Author: Tamburri, S., Saracco, P., Longhetti, M., Gargiulo, A., Lonoce, I., and Ciocca, F.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The aim of our analysis is twofold. On the one hand we are interested in addressing whether a sample of ETGs morphologically selected differs from a sample of passive galaxies in terms of galaxy statistics. On the other hand we study how the relative abundance of galaxies, the number density and the stellar mass density for different morphological types change over the redshift range 0.6=10^(11) M_sol) galaxies, with the fraction of massive ETGs rising up to 40% and the fraction of massive LTGs decreasing down to 60%. Moreover, we find that the number density and the stellar mass density of the whole population of massive galaxies increase almost by a factor of ~10 between 0.63-4x10^(11) M_sol) both ETGs and LTGs do not increase since z~2.5, contrary to the lower mass galaxies. This suggests that the population of the most massive galaxies formed at z>2.5-3 and that the assembly of such high-mass galaxies is not effective at lower redshift., Comment: 15 pages, 14 figures. Published in A&A
Published: 2014
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25. LBT-LUCIFER spectroscopy: kinematics of a compact early type galaxy at z\simeq1.4

Author: Longhetti, Marcella, Saracco, Paolo, Gargiulo, Adriana, Tamburri, Sonia, and Lonoce, Ilaria
Subjects: Astrophysics - Galaxy Astrophysics, Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract: We present a high signal to noise (S/N$>$10) medium resolution (R=2000) LBT-LUCIFER spectrum of the early-type galaxy (ETG) S2F1-142 at $z\simeq1.4$. By means of the CaT line at $8662$ \AA, we measured its redshift $z=1.386\pm 0.001$ and we estimated its velocity dispersion $\sigma_{v}=340 ^{-60}_{+120}$ km/s. Its corresponding virial mass is 3.9$\times10^{11}$ M$_\odot$, compatible with the stellar mass estimates obtained assuming Initial Mass Functions (IMFs) less dwarf rich than the Salpeter one. S2F1-142 is a compact galaxy with $R_{e}$=3.1$\pm$0.2 kpc, i.e., an effective radius more than three times smaller than the average $R_{e}$ of early-type galaxies with the same mass in the local universe. At the same time, we found local and high redshift galaxies with a similar mass content and similar effective radius confirming that it is fully consistent with the already available measures of $R_{e}$ and $\sigma_{v}$ both in the local and in the distant universe. Considering the distribution of $R_{e}$ and $\sigma_{v}$ as a function of the stellar mass content of ETGs, both in the local and in the distant universe, we noticed that the measured velocity dispersions of the more compact galaxies are on average slightly lower than expected on the basis of their compactness and the virial theorem, suggesting that {\it i)} their dark matter content is lower than in the more diffuse galaxies and/or {\it ii)} their luminosity profiles are steeper than in the more diffuse galaxies and/or {\it iii)} their larger compactness is an apparent effect caused by the overestimate of their stellar mass content (due to bottom lighter IMF and/or systematic affecting the stellar mass estimates)., Comment: 8 pages, 8 figures, accepted for publication in MNRAS
Published: 2014

26. Scaling relations of cluster elliptical galaxies at z~1.3. Distinguishing luminosity and structural evolution

Author: Saracco, P., Casati, A., Gargiulo, A., Longhetti, M., Lonoce, I., Tamburri, S., Bettoni, D., D'Onofrio, M., Fasano, G., Poggianti, B. M., Boutsia, K., Fumana, M., and Sani, E.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: [Abridged] We studied the size-surface brightness and the size-mass relations of a sample of 16 cluster elliptical galaxies in the mass range 10^{10}-2x10^{11} M_sun which were morphologically selected in the cluster RDCS J0848+4453 at z=1.27. Our aim is to assess whether they have completed their mass growth at their redshift or significant mass and/or size growth can or must take place until z=0 in order to understand whether elliptical galaxies of clusters follow the observed size evolution of passive galaxies. To compare our data with the local universe we considered the Kormendy relation derived from the early-type galaxies of a local Coma Cluster reference sample and the WINGS survey sample. The comparison with the local Kormendy relation shows that the luminosity evolution due to the aging of the stellar content already assembled at z=1.27 brings them on the local relation. Moreover, this stellar content places them on the size-mass relation of the local cluster ellipticals. These results imply that for a given mass, the stellar mass at z~1.3 is distributed within these ellipticals according to the same stellar mass profile of local ellipticals. We find that a pure size evolution, even mild, is ruled out for our galaxies since it would lead them away from both the Kormendy and the size-mass relation. If an evolution of the effective radius takes place, this must be compensated by an increase in the luminosity, hence of the stellar mass of the galaxies, to keep them on the local relations. We show that to follow the Kormendy relation, the stellar mass must increase as the effective radius. However, this mass growth is not sufficient to keep the galaxies on the size-mass relation for the same variation in effective radius. Thus, if we want to preserve the Kormendy relation, we fail to satisfy the size-mass relation and vice versa., Comment: Accepted for publication in A&A, updated to match final journal version
Published: 2014
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27. The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster

Author: Ilaria Lonoce, W. L. Freedman, and A. Feldmeier-Krause
Subjects: Early-type galaxies, Initial mass function, Astrophysics, QB460-466
Abstract: The Hydra I cluster offers an excellent opportunity to study and compare the relic old stellar populations in the core of its two brightest galaxies. In addition, the differing kinematics of the two galaxies allows a test of the local validity of general scaling relations. In this work, we present a direct comparison employing full spectral fitting of new high-quality long-slit optical and near-infrared spectroscopic data. We retrieve age, metallicity, and 19 elemental abundances out to ∼12 kpc within each galaxy, as well as the Initial Mass Function (IMF) in their central regions. Our results suggest that the inner ∼5 kpc regions of both galaxies, despite their different masses, formed at the same time and evolved with a similar star formation timescale and chemical enrichment, confirming their early formation in the cluster buildup. Only the overall metallicity and IMF radial profiles show differences connected with their different velocity dispersion profiles. The radial trends of the IMF positively correlate with both [Z/H] and σ . While the trends of the IMF slope values with metallicity agree with a global trend for both galaxies, the trends with the velocity dispersion exhibit differences. The outer regions show signs of mixed stellar populations with large differences in chemical content compared to the centers, but with similarly old ages.
Published: 2023
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28. 1q23.1 homozygous deletion and downregulation of Fc receptor-like family genes confer poor prognosis in chronic lymphocytic leukemia

Author: Daniele, Giulia, L’Abbate, Alberto, Turchiano, Antonella, Palumbo, Orazio, Carella, Massimo, Lo Cunsolo, Crocifissa, Iuzzolino, Paolo, Lonoce, Angelo, Hernández-Sánchez, María, Minoia, Carla, Leone, Patrizia, Hernandez-Rivas, Jesus Maria, and Storlazzi, Clelia Tiziana
Published: 2019
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29. Subcellular localization and interactions among rubber particle proteins from Hevea brasiliensis

Author: Brown, Daniel, Feeney, Mistianne, Ahmadi, Mathin, Lonoce, Chiara, Sajari, Roslinda, Di Cola, Alessandra, and Frigerio, Lorenzo
Published: 2017

30. Barrier Impairment and Type 2 Inflammation in Allergic Diseases: The Pediatric Perspective

Author: Michele Ghezzi, Elena Pozzi, Luisa Abbattista, Luisa Lonoce, Gian Vincenzo Zuccotti, and Enza D’Auria
Subjects: children, inflammation, biologics, severe asthma, allergic rhinitis, atopic dermatitis, Pediatrics, RJ1-570
Abstract: Allergic diseases represent a global burden. Although the patho-physiological mechanisms are still poorly understood, epithelial barrier dysfunction and Th2 inflammatory response play a pivotal role. Barrier dysfunction, characterized by a loss of differentiation, reduced junctional integrity, and altered innate defence, underpins the pathogenesis of allergic diseases. Epithelial barrier impairment may be a potential therapeutic target for new treatment strategies Up now, monoclonal antibodies and new molecules targeting specific pathways of the immune response have been developed, and others are under investigation, both for adult and paediatric populations, which are affected by atopic dermatitis (AD), asthma, allergic rhinitis (AR), chronic rhinosinusitis with nasal polyps (CRSwNP), or eosinophilic esophagitis (EoE). In children affected by severe asthma biologics targeting IgE, IL-5 and against IL-4 and IL-13 receptors are already available, and they have also been applied in CRSwNP. In severe AD Dupilumab, a biologic which inhibits both IL-4 and IL-13, the most important cytokines involved in inflammation response, has been approved for treatment of patients over 12 years. While a biological approach has already shown great efficacy on the treatment of severe atopic conditions, early intervention to restore epithelial barrier integrity, and function may prevent the inflammatory response and the development of the atopic march.
Published: 2021
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31. MYC-containing amplicons in acute myeloid leukemia: genomic structures, evolution, and transcriptional consequences

Author: L′Abbate, Alberto, Tolomeo, Doron, Cifola, Ingrid, Severgnini, Marco, Turchiano, Antonella, Augello, Bartolomeo, Squeo, Gabriella, D′Addabbo, Pietro, Traversa, Debora, Daniele, Giulia, Lonoce, Angelo, Pafundi, Mariella, Carella, Massimo, Palumbo, Orazio, Dolnik, Anna, Muehlematter, Dominique, Schoumans, Jacqueline, Van Roy, Nadine, De Bellis, Gianluca, Martinelli, Giovanni, Merla, Giuseppe, Bullinger, Lars, Haferlach, Claudia, and Storlazzi, Clelia Tiziana
Published: 2018
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32. The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster*

Author: Lonoce, Ilaria, primary, Freedman, W. L., additional, and Feldmeier-Krause, A., additional
Published: 2023
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33. Self-reported vs measured body mass index in the italian adults within cuore project 2018-19

Author: Donfrancesco, Chiara, primary, Iannucci, Laura, additional, Bologna, Emanuela, additional, Profumo, Elisabetta, additional, Lonoce, Cinzia, additional, Buttari, Brigitta, additional, Lonardo, Anna, additional, Vannucchi, Serena, additional, and Palmieri, Luigi, additional
Published: 2023
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34. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author: Universidad de Alicante. Departamento de Física Aplicada, Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J.E., Falcón-Barroso, Jesús, Gänsicke, B.T., Hill, V., Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Fumagalli, Michele, Boeche, Corrado, Fariña, Cecilia, Gonzalez, Oscar A., Guest, Steve, Bellazzini, M., Drake, Alyssa, Longhetti, Marcella, Herrero, Artemio, Monari, Giacomo, Carrasco, Esperanza, Dutta, Rajeshwari, Deason, Alis, Irwin, M., Sordo, R., Serra, Paolo, Lucatello, Sara, Bolzonella, Micol, Gallazzi, Anna, Peralta de Arriba, Luis, García-Benito, Rubén, Van der Swaelmen, M., Stuik, Remko, Peletier, Reynier F., Hughes, Sarah, de Burgos, Abel, Magrini, L., Ferré-Mateu, Anna, Pérez, Isabel, Carter, David, Haines, Christopher P., Som, Debopam, Lind, K., Hardcastle, Martin J., Raddi, Roberto, Weijmans, Anne-Marie, Vioque, Miguel, Schiavon, Ricardo P., Figueras, Francesca, Irsic, Vid, Bernard, Edouard J., Jablonka, Pascale, Amos, Nicholas J., Lodi, Marcello, Ascasibar, Yago, Abrams, Don Carlos, Best, Philip, Gebran, M., Lam, Man I., Bonoli, Silvia, Larsen, Søren S., Domínguez-Palmero, Lilian, Bragaglia, A., Verro, Kristiina, Longobardi, Alessia, Morelli, Lorenzo, Jarvis, Matt J., Schultheis, Mathias, Feuillet, D.K., Bosma, Albert, Haywood, Misha, Marco, Amparo, Casamiquela, L., Sabater Montes, Jose, Martin, Nicolas F., Sorini, Daniele, Cantat-Gaudin, T., Kuchner, Ulrike, Hoskin, Matthew J., Smith, D.J.B., Jordi, C., Mottram, Christopher J., Fossati, Matteo, Naylor, Tim, Dorda Laforet, Ricardo, San Juan, José, Antoja, Teresa, Vink, Jorick S., Merluzzi, Paola, Franciosini, E., Lewis, Ian J., Ramos, Pau, Gilbert, James, Read, Shaun C., Siebert, Arnaud, Picó, Sergio, Hatch, Nina A., Miralda-Escudé, Jordi, Sanna, N., Tolstoy, Eline, Negueruela, Ignacio, Vallenari, A., Gledhill, T.M., González Delgado, Rosa M., Maurogordato, Sophie, Simón Díaz, Sergio, Helmi, Amina, Wright, N., Méndez-Abreu, Jairo, Smith, Russell J., Babusiaux, Carine, Gullieuszik, Marco, Balbinot, Eduardo, Alonso-Santiago, Javier, Hernandez, Nauzet, Onorbe, Jose, Tortora, Crescenzo, Kondapally, Rohit, Tsantaki, M., Bettoni, Daniela, Pérez-Ràfols, Ignasi, Xylakis-Dornbusch, Theodora, Schallig, Ellen, Hess, Kelley M., Soubiran, C., Kordopatis, G., Röttgering, Huub J.A., Walton, N., Lhomé, Emilie, Wegg, Christopher, La Barbera, Francesco, Carbajo-Hijarrubia, Juan, Caffau, Elisabetta, Alfaro, Emilio J., Starkenburg, Else, Youakim, Kris, Aragón-Salamanca, Alfonso, Zibetti, Stefano, Marchal, Olivier, Erkal, Denis, Domínguez-Gómez, Jesús, Molinari, Emilio, van Weeren, Reinout J., Carrera, Ricardo, Pancino, E., Cornwell, Daniel J., Gentile Fusillo, Nicola, Frasca, A., Britavskiy, Nikolay, Mercurio, Amata, Zurita, Cristina, Allende Prieto, C., Balcells, Marc, Peirani, Sébastien, Williams, Wendy L., Knapen, Johan H., Rubiño-Martín, J.A., Terrett, David, Koposov, S., Rainer, Monica, Harris, Amy, Guerra, Jose, De Grandi, Sabrina, Belokurov, Vasily, Molaeinezhad, Alireza, Steele, Iain A., Monguió, María, Shimwell, Timothy W., Thomas, Guillaume, Busarello, Gianni, Lewis, J., Stott, John, Duncan, Kenneth J., Romero-Gómez, Mercè, Vergani, Daniela, Royer, Frédéric, Lemasle, Bertrand, Krogager, Jens-Kristian, Greimel, Robert, Wesson, Roger, Bianco, Andrea, Morrison, Sean, Di Matteo, Paola, Barrena, R., Verheijen, Marc A.W., Laigle, Clotilde, Ashley, Richard P., Wilson, Andrew J., Conrado, Ana M., Balaguer-Nunez, L., Feltzing, S., Walcher, C. Jakob, Matsuno, Tadafumi, Maíz Apellániz, Jesús, Battaglia, Giuseppina, Murphy, D.N.A., Bishop, Georgia, Bensby, T., Blomqvist, Michael, Aguado, David S., Corcho-Caballero, Pablo, Worley, C.C., Guarcello, Mario Giuseppe, Benn, Chris R., Bonifacio, P., Seabroke, G.M., Castro-Ginard, Alfred, Famaey, Benoit, Couto, Guilherme, Rossi, Elena Maria, Pozzetti, Lucia, Lonoce, Ilaria, Berlanas, Sara R., Costantin, Luca, Universidad de Alicante. Departamento de Física Aplicada, Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J.E., Falcón-Barroso, Jesús, Gänsicke, B.T., Hill, V., Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Fumagalli, Michele, Boeche, Corrado, Fariña, Cecilia, Gonzalez, Oscar A., Guest, Steve, Bellazzini, M., Drake, Alyssa, Longhetti, Marcella, Herrero, Artemio, Monari, Giacomo, Carrasco, Esperanza, Dutta, Rajeshwari, Deason, Alis, Irwin, M., Sordo, R., Serra, Paolo, Lucatello, Sara, Bolzonella, Micol, Gallazzi, Anna, Peralta de Arriba, Luis, García-Benito, Rubén, Van der Swaelmen, M., Stuik, Remko, Peletier, Reynier F., Hughes, Sarah, de Burgos, Abel, Magrini, L., Ferré-Mateu, Anna, Pérez, Isabel, Carter, David, Haines, Christopher P., Som, Debopam, Lind, K., Hardcastle, Martin J., Raddi, Roberto, Weijmans, Anne-Marie, Vioque, Miguel, Schiavon, Ricardo P., Figueras, Francesca, Irsic, Vid, Bernard, Edouard J., Jablonka, Pascale, Amos, Nicholas J., Lodi, Marcello, Ascasibar, Yago, Abrams, Don Carlos, Best, Philip, Gebran, M., Lam, Man I., Bonoli, Silvia, Larsen, Søren S., Domínguez-Palmero, Lilian, Bragaglia, A., Verro, Kristiina, Longobardi, Alessia, Morelli, Lorenzo, Jarvis, Matt J., Schultheis, Mathias, Feuillet, D.K., Bosma, Albert, Haywood, Misha, Marco, Amparo, Casamiquela, L., Sabater Montes, Jose, Martin, Nicolas F., Sorini, Daniele, Cantat-Gaudin, T., Kuchner, Ulrike, Hoskin, Matthew J., Smith, D.J.B., Jordi, C., Mottram, Christopher J., Fossati, Matteo, Naylor, Tim, Dorda Laforet, Ricardo, San Juan, José, Antoja, Teresa, Vink, Jorick S., Merluzzi, Paola, Franciosini, E., Lewis, Ian J., Ramos, Pau, Gilbert, James, Read, Shaun C., Siebert, Arnaud, Picó, Sergio, Hatch, Nina A., Miralda-Escudé, Jordi, Sanna, N., Tolstoy, Eline, Negueruela, Ignacio, Vallenari, A., Gledhill, T.M., González Delgado, Rosa M., Maurogordato, Sophie, Simón Díaz, Sergio, Helmi, Amina, Wright, N., Méndez-Abreu, Jairo, Smith, Russell J., Babusiaux, Carine, Gullieuszik, Marco, Balbinot, Eduardo, Alonso-Santiago, Javier, Hernandez, Nauzet, Onorbe, Jose, Tortora, Crescenzo, Kondapally, Rohit, Tsantaki, M., Bettoni, Daniela, Pérez-Ràfols, Ignasi, Xylakis-Dornbusch, Theodora, Schallig, Ellen, Hess, Kelley M., Soubiran, C., Kordopatis, G., Röttgering, Huub J.A., Walton, N., Lhomé, Emilie, Wegg, Christopher, La Barbera, Francesco, Carbajo-Hijarrubia, Juan, Caffau, Elisabetta, Alfaro, Emilio J., Starkenburg, Else, Youakim, Kris, Aragón-Salamanca, Alfonso, Zibetti, Stefano, Marchal, Olivier, Erkal, Denis, Domínguez-Gómez, Jesús, Molinari, Emilio, van Weeren, Reinout J., Carrera, Ricardo, Pancino, E., Cornwell, Daniel J., Gentile Fusillo, Nicola, Frasca, A., Britavskiy, Nikolay, Mercurio, Amata, Zurita, Cristina, Allende Prieto, C., Balcells, Marc, Peirani, Sébastien, Williams, Wendy L., Knapen, Johan H., Rubiño-Martín, J.A., Terrett, David, Koposov, S., Rainer, Monica, Harris, Amy, Guerra, Jose, De Grandi, Sabrina, Belokurov, Vasily, Molaeinezhad, Alireza, Steele, Iain A., Monguió, María, Shimwell, Timothy W., Thomas, Guillaume, Busarello, Gianni, Lewis, J., Stott, John, Duncan, Kenneth J., Romero-Gómez, Mercè, Vergani, Daniela, Royer, Frédéric, Lemasle, Bertrand, Krogager, Jens-Kristian, Greimel, Robert, Wesson, Roger, Bianco, Andrea, Morrison, Sean, Di Matteo, Paola, Barrena, R., Verheijen, Marc A.W., Laigle, Clotilde, Ashley, Richard P., Wilson, Andrew J., Conrado, Ana M., Balaguer-Nunez, L., Feltzing, S., Walcher, C. Jakob, Matsuno, Tadafumi, Maíz Apellániz, Jesús, Battaglia, Giuseppina, Murphy, D.N.A., Bishop, Georgia, Bensby, T., Blomqvist, Michael, Aguado, David S., Corcho-Caballero, Pablo, Worley, C.C., Guarcello, Mario Giuseppe, Benn, Chris R., Bonifacio, P., Seabroke, G.M., Castro-Ginard, Alfred, Famaey, Benoit, Couto, Guilherme, Rossi, Elena Maria, Pozzetti, Lucia, Lonoce, Ilaria, Berlanas, Sara R., and Costantin, Luca
Abstract: WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable ‘mini’ integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366−959 nm at R ∼ 5000, or two shorter ranges at R ∼ 20 000. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy’s origins by completing Gaia’s phase-space information, providing metallicities to its limiting magnitude for ∼3 million stars and detailed abundances for ∼1.5 million brighter field and open-cluster stars; (ii) survey ∼0.4 million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey ∼400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in z < 0.5 cluster galaxies; (vi) survey stellar populations and kinematics in ∼25 000 field galaxies at 0.3 ≲ z ≲ 0.7; (vii) study the cosmic evolution of accretion and star formation using >1 million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at z > 2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.
Published: 2023

35. Self-reported vs measured body mass index in the italian adults within cuore project 2018-19

Author: Chiara Donfrancesco, Laura Iannucci, Emanuela Bologna, Elisabetta Profumo, Cinzia Lonoce, Brigitta Buttari, Anna Lonardo, Serena Vannucchi, and Luigi Palmieri
Subjects: Health (social science), Epidemiology, Health Policy, Public Health, Environmental and Occupational Health, Medicine (miscellaneous), Health Informatics
Published: 2023
Full Text: View/download PDF

36. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author: Jin, Shoko, primary, Trager, Scott C, additional, Dalton, Gavin B, additional, Aguerri, J Alfonso L, additional, Drew, J E, additional, Falcón-Barroso, Jesús, additional, Gänsicke, Boris T, additional, Hill, Vanessa, additional, Iovino, Angela, additional, Pieri, Matthew M, additional, Poggianti, Bianca M, additional, Smith, D J B, additional, Vallenari, Antonella, additional, Abrams, Don Carlos, additional, Aguado, David S, additional, Antoja, Teresa, additional, Aragón-Salamanca, Alfonso, additional, Ascasibar, Yago, additional, Babusiaux, Carine, additional, Balcells, Marc, additional, Barrena, R, additional, Battaglia, Giuseppina, additional, Belokurov, Vasily, additional, Bensby, Thomas, additional, Bonifacio, Piercarlo, additional, Bragaglia, Angela, additional, Carrasco, Esperanza, additional, Carrera, Ricardo, additional, Cornwell, Daniel J, additional, Domínguez-Palmero, Lilian, additional, Duncan, Kenneth J, additional, Famaey, Benoit, additional, Fari na, Cecilia, additional, Gonzalez, Oscar A, additional, Guest, Steve, additional, Hatch, Nina A, additional, Hess, Kelley M, additional, Hoskin, Matthew J, additional, Irwin, Mike, additional, Knapen, Johan H, additional, Koposov, Sergey E, additional, Kuchner, Ulrike, additional, Laigle, Clotilde, additional, Lewis, Jim, additional, Longhetti, Marcella, additional, Lucatello, Sara, additional, Méndez-Abreu, Jairo, additional, Mercurio, Amata, additional, Molaeinezhad, Alireza, additional, Monguió, Maria, additional, Morrison, Sean, additional, Murphy, David N A, additional, de Arriba, Luis Peralta, additional, Pérez, Isabel, additional, Pérez-Ràfols, Ignasi, additional, Picó, Sergio, additional, Raddi, Roberto, additional, Romero-Gómez, Mercè, additional, Royer, Frédéric, additional, Siebert, Arnaud, additional, Seabroke, George M, additional, Som, Debopam, additional, Terrett, David, additional, Thomas, Guillaume, additional, Wesson, Roger, additional, Worley, C Clare, additional, Alfaro, Emilio J, additional, Prieto, Carlos Allende, additional, Alonso-Santiago, Javier, additional, Amos, Nicholas J, additional, Ashley, Richard P, additional, Balaguer-Nú nez, Lola, additional, Balbinot, Eduardo, additional, Bellazzini, Michele, additional, Benn, Chris R, additional, Berlanas, Sara R, additional, Bernard, Edouard J, additional, Best, Philip, additional, Bettoni, Daniela, additional, Bianco, Andrea, additional, Bishop, Georgia, additional, Blomqvist, Michael, additional, Boeche, Corrado, additional, Bolzonella, Micol, additional, Bonoli, Silvia, additional, Bosma, Albert, additional, Britavskiy, Nikolay, additional, Busarello, Gianni, additional, Caffau, Elisabetta, additional, Cantat-Gaudin, Tristan, additional, Castro-Ginard, Alfred, additional, Couto, Guilherme, additional, Carbajo-Hijarrubia, Juan, additional, Carter, David, additional, Casamiquela, Laia, additional, Conrado, Ana M, additional, Corcho-Caballero, Pablo, additional, Costantin, Luca, additional, Deason, Alis, additional, de Burgos, Abel, additional, De Grandi, Sabrina, additional, Di Matteo, Paola, additional, Domínguez-Gómez, Jesús, additional, Dorda, Ricardo, additional, Drake, Alyssa, additional, Dutta, Rajeshwari, additional, Erkal, Denis, additional, Feltzing, Sofia, additional, Ferré-Mateu, Anna, additional, Feuillet, Diane, additional, Figueras, Francesca, additional, Fossati, Matteo, additional, Franciosini, Elena, additional, Frasca, Antonio, additional, Fumagalli, Michele, additional, Gallazzi, Anna, additional, García-Benito, Rubén, additional, Fusillo, Nicola Gentile, additional, Gebran, Marwan, additional, Gilbert, James, additional, Gledhill, T M, additional, Delgado, Rosa M González, additional, Greimel, Robert, additional, Guarcello, Mario Giuseppe, additional, Guerra, Jose, additional, Gullieuszik, Marco, additional, Haines, Christopher P, additional, Hardcastle, Martin J, additional, Harris, Amy, additional, Haywood, Misha, additional, Helmi, Amina, additional, Hernandez, Nauzet, additional, Herrero, Artemio, additional, Hughes, Sarah, additional, Irsic, Vid, additional, Jablonka, Pascale, additional, Jarvis, Matt J, additional, Jordi, Carme, additional, Kondapally, Rohit, additional, Kordopatis, Georges, additional, Krogager, Jens-Kristian, additional, Barbera, Francesco La, additional, Lam, Man I, additional, Larsen, Søren S, additional, Lemasle, Bertrand, additional, Lewis, Ian J, additional, Lhomé, Emilie, additional, Lind, Karin, additional, Lodi, Marcello, additional, Longobardi, Alessia, additional, Lonoce, Ilaria, additional, Magrini, Laura, additional, Apellániz, Jesús Maíz, additional, Marchal, Olivier, additional, Marco, Amparo, additional, Martin, Nicolas F, additional, Matsuno, Tadafumi, additional, Maurogordato, Sophie, additional, Merluzzi, Paola, additional, Miralda-Escudé, Jordi, additional, Molinari, Emilio, additional, Monari, Giacomo, additional, Morelli, Lorenzo, additional, Mottram, Christopher J, additional, Naylor, Tim, additional, Negueruela, Ignacio, additional, Onorbe, Jose, additional, Pancino, Elena, additional, Peirani, Sébastien, additional, Peletier, Reynier F, additional, Pozzetti, Lucia, additional, Rainer, Monica, additional, Ramos, Pau, additional, Read, Shaun C, additional, Rossi, Elena Maria, additional, Röttgering, Huub J A, additional, Rubi no-Martín, Jose Alberto, additional, Montes, Jose Sabater, additional, Juan, José San, additional, Sanna, Nicoletta, additional, Schallig, Ellen, additional, Schiavon, Ricardo P, additional, Schultheis, Mathias, additional, Serra, Paolo, additional, Shimwell, Timothy W, additional, Simón-Díaz, Sergio, additional, Smith, Russell J, additional, Sordo, Rosanna, additional, Sorini, Daniele, additional, Soubiran, Caroline, additional, Starkenburg, Else, additional, Steele, Iain A, additional, Stott, John, additional, Stuik, Remko, additional, Tolstoy, Eline, additional, Tortora, Crescenzo, additional, Tsantaki, Maria, additional, Van der Swaelmen, Mathieu, additional, van Weeren, Reinout J, additional, Vergani, Daniela, additional, Verheijen, Marc A W, additional, Verro, Kristiina, additional, Vink, Jorick S, additional, Vioque, Miguel, additional, Walcher, C Jakob, additional, Walton, Nicholas A, additional, Wegg, Christopher, additional, Weijmans, Anne-Marie, additional, Williams, Wendy L, additional, Wilson, Andrew J, additional, Wright, Nicholas J, additional, Xylakis-Dornbusch, Theodora, additional, Youakim, Kris, additional, Zibetti, Stefano, additional, and Zurita, Cristina, additional
Published: 2023
Full Text: View/download PDF

37. The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Author: Shoko Jin, Scott C Trager, Gavin B Dalton, J Alfonso L Aguerri, J E Drew, Jesús Falcón-Barroso, Boris T Gänsicke, Vanessa Hill, Angela Iovino, Matthew M Pieri, Bianca M Poggianti, D J B Smith, Antonella Vallenari, Don Carlos Abrams, David S Aguado, Teresa Antoja, Alfonso Aragón-Salamanca, Yago Ascasibar, Carine Babusiaux, Marc Balcells, R Barrena, Giuseppina Battaglia, Vasily Belokurov, Thomas Bensby, Piercarlo Bonifacio, Angela Bragaglia, Esperanza Carrasco, Ricardo Carrera, Daniel J Cornwell, Lilian Domínguez-Palmero, Kenneth J Duncan, Benoit Famaey, Cecilia Fari na, Oscar A Gonzalez, Steve Guest, Nina A Hatch, Kelley M Hess, Matthew J Hoskin, Mike Irwin, Johan H Knapen, Sergey E Koposov, Ulrike Kuchner, Clotilde Laigle, Jim Lewis, Marcella Longhetti, Sara Lucatello, Jairo Méndez-Abreu, Amata Mercurio, Alireza Molaeinezhad, Maria Monguió, Sean Morrison, David N A Murphy, Luis Peralta de Arriba, Isabel Pérez, Ignasi Pérez-Ràfols, Sergio Picó, Roberto Raddi, Mercè Romero-Gómez, Frédéric Royer, Arnaud Siebert, George M Seabroke, Debopam Som, David Terrett, Guillaume Thomas, Roger Wesson, C Clare Worley, Emilio J Alfaro, Carlos Allende Prieto, Javier Alonso-Santiago, Nicholas J Amos, Richard P Ashley, Lola Balaguer-Nú nez, Eduardo Balbinot, Michele Bellazzini, Chris R Benn, Sara R Berlanas, Edouard J Bernard, Philip Best, Daniela Bettoni, Andrea Bianco, Georgia Bishop, Michael Blomqvist, Corrado Boeche, Micol Bolzonella, Silvia Bonoli, Albert Bosma, Nikolay Britavskiy, Gianni Busarello, Elisabetta Caffau, Tristan Cantat-Gaudin, Alfred Castro-Ginard, Guilherme Couto, Juan Carbajo-Hijarrubia, David Carter, Laia Casamiquela, Ana M Conrado, Pablo Corcho-Caballero, Luca Costantin, Alis Deason, Abel de Burgos, Sabrina De Grandi, Paola Di Matteo, Jesús Domínguez-Gómez, Ricardo Dorda, Alyssa Drake, Rajeshwari Dutta, Denis Erkal, Sofia Feltzing, Anna Ferré-Mateu, Diane Feuillet, Francesca Figueras, Matteo Fossati, Elena Franciosini, Antonio Frasca, Michele Fumagalli, Anna Gallazzi, Rubén García-Benito, Nicola Gentile Fusillo, Marwan Gebran, James Gilbert, T M Gledhill, Rosa M González Delgado, Robert Greimel, Mario Giuseppe Guarcello, Jose Guerra, Marco Gullieuszik, Christopher P Haines, Martin J Hardcastle, Amy Harris, Misha Haywood, Amina Helmi, Nauzet Hernandez, Artemio Herrero, Sarah Hughes, Vid Irsic, Pascale Jablonka, Matt J Jarvis, Carme Jordi, Rohit Kondapally, Georges Kordopatis, Jens-Kristian Krogager, Francesco La Barbera, Man I Lam, Søren S Larsen, Bertrand Lemasle, Ian J Lewis, Emilie Lhomé, Karin Lind, Marcello Lodi, Alessia Longobardi, Ilaria Lonoce, Laura Magrini, Jesús Maíz Apellániz, Olivier Marchal, Amparo Marco, Nicolas F Martin, Tadafumi Matsuno, Sophie Maurogordato, Paola Merluzzi, Jordi Miralda-Escudé, Emilio Molinari, Giacomo Monari, Lorenzo Morelli, Christopher J Mottram, Tim Naylor, Ignacio Negueruela, Jose Onorbe, Elena Pancino, Sébastien Peirani, Reynier F Peletier, Lucia Pozzetti, Monica Rainer, Pau Ramos, Shaun C Read, Elena Maria Rossi, Huub J A Röttgering, Jose Alberto Rubi no-Martín, Jose Sabater Montes, José San Juan, Nicoletta Sanna, Ellen Schallig, Ricardo P Schiavon, Mathias Schultheis, Paolo Serra, Timothy W Shimwell, Sergio Simón-Díaz, Russell J Smith, Rosanna Sordo, Daniele Sorini, Caroline Soubiran, Else Starkenburg, Iain A Steele, John Stott, Remko Stuik, Eline Tolstoy, Crescenzo Tortora, Maria Tsantaki, Mathieu Van der Swaelmen, Reinout J van Weeren, Daniela Vergani, Marc A W Verheijen, Kristiina Verro, Jorick S Vink, Miguel Vioque, C Jakob Walcher, Nicholas A Walton, Christopher Wegg, Anne-Marie Weijmans, Wendy L Williams, Andrew J Wilson, Nicholas J Wright, Theodora Xylakis-Dornbusch, Kris Youakim, Stefano Zibetti, Cristina Zurita, Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Observatoire astronomique de Strasbourg (ObAS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), University of St Andrews. School of Physics and Astronomy, University of St Andrews. Centre for Contemporary Art, Universidad de Alicante. Departamento de Física Aplicada, Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, and Astrofísica Estelar (AE)
Subjects: Astrofísica, Cosmology and Nongalactic Astrophysics (astro-ph.CO), NDAS, FOS: Physical sciences, Surveys, surveys, QB Astronomy, spectrographs [Instrumentation], observations [Cosmology], Instrumentation and Methods for Astrophysics (astro-ph.IM), Galaxy: general, stars: general, Solar and Stellar Astrophysics (astro-ph.SR), general [Galaxy], QC, QB, instrumentation: spectrographs, general [Stars], Análisis de datos, Instrumentation spectrographs, Astronomy and Astrophysics, general [Galaxies], galaxies: general, Astrophysics - Astrophysics of Galaxies, QC Physics, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, [SDU]Sciences of the Universe [physics], Astrophysics of Galaxies (astro-ph.GA), MCP, cosmology: observations, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366$-$959\,nm at $R\sim5000$, or two shorter ranges at $R\sim20\,000$. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for $\sim$3 million stars and detailed abundances for $\sim1.5$ million brighter field and open-cluster stars; (ii) survey $\sim0.4$ million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey $\sim400$ neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in $z1$ million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at $z>2$. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator., 41 pages, 27 figures, accepted for publication by MNRAS
Published: 2023
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38. An unexpected demographic regime: The western necropolis of the Greek colony of Himera (Sicily, Italy) (550-409 BCE)

Author: Norma Lonoce, Gianpiero Dalla-Zuanna, Pier Francesco Fabbri, Stefano Vassallo, and Irene Barbiera
Subjects: Archeology
Published: 2023
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39. The mass burials from the western necropolis of the Greek colony of Himera (Sicily) related to the battles of 480 and 409 BCE

Author: Pier Francesco Fabbri, Serena Viva, Matteo Valentino, Stefano Vassallo, Giorgia Vincenti, Roberto Cameriere, Norma Lonoce, Viva, Serena, Lonoce, Norma, Vincenti, Giorgia, Cameriere4, Roberto, Valentino, Matteo, Vassallo, Stefano, and Fabbri, Pier Francesco
Subjects: Archeology, Battle, History, Anthropology, media_common.quotation_subject, Ancient history, Mass graves, Greek colonization, Sicily, Himera, Battle, Weapons, media_common
Abstract: Throughout the ancient Greek world mass burials are rare. Of the 10,000 excavated burials in the western necropolis of the Greek colony of Himera (649-409) only 16 contained more than one individual; seven of these can in all possibility be traced back to the two battles fought by Himera against the Carthaginians in 480 and 409 BCE. Written sources (Diod. 11.20ff.) state that the Himerans, accompanied by numerous Greek allies, defeated the Carthaginian forces in the first conflict whereas the loss of Greek allied support in the second battle resulted in the city’s defeat and subsequent destruction. The anthropological and taphonomical study of the human remains aims at testing the archaeological hypothesis that individuals interred in the seven mass graves can be related to the two battles. Skeleton density (skeletons/m2), position, orientation and conservation levels of the individuals in the mass burials were analyzed and compared to a larger sample of 1,000 single burials from the same necropolis along with mass graves in other forensic and archaeological contexts. Sex, age-at-death, presence of skeletal stress indicators and perimortal traumas were recorded using standard anthropological methods. In the case of poorly preserved remains, sex was estimated using site-specific discriminant functions. While representing catastrophic samples, the results from the seven mass burials all lead to the assumption that the graves can be associated with the interment of warriors fallen in battle. Moreover, burial differences have permitted to distinguish the mass burials dating to 480 BCE from those attributed to 409 BCE.
Published: 2020
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40. Epigenetically induced ectopic expression of UNCX impairs the proliferation and differentiation of myeloid cells

Author: Giulia Daniele, Giorgia Simonetti, Caterina Fusilli, Ilaria Iacobucci, Angelo Lonoce, Antonio Palazzo, Mariana Lomiento, Fabiana Mammoli, Renè Massimiliano Marsano, Elena Marasco, Vilma Mantovani, Hilmar Quentmeier, Hans G Drexler, Jie Ding, Orazio Palumbo, Massimo Carella, Niroshan Nadarajah, Margherita Perricone, Emanuela Ottaviani, Carmen Baldazzi, Nicoletta Testoni, Cristina Papayannidis, Sergio Ferrari, Tommaso Mazza, Giovanni Martinelli, and Clelia Tiziana Storlazzi
Subjects: Diseases of the blood and blood-forming organs, RC633-647.5
Abstract: We here describe a leukemogenic role of the homeobox gene UNCX, activated by epigenetic modifications in acute myeloid leukemia (AML). We found the ectopic activation of UNCX in a leukemia patient harboring a t(7;10)(p22;p14) translocation, in 22 of 61 of additional cases [a total of 23 positive patients out of 62 (37.1%)], and in 6 of 75 (8%) of AML cell lines. UNCX is embedded within a low-methylation region (canyon) and encodes for a transcription factor involved in somitogenesis and neurogenesis, with specific expression in the eye, brain, and kidney. UNCX expression turned out to be associated, and significantly correlated, with DNA methylation increase at its canyon borders based on data in our patients and in archived data of patients from The Cancer Genome Atlas. UNCX-positive and -negative patients displayed significant differences in their gene expression profiles. An enrichment of genes involved in cell proliferation and differentiation, such as MAP2K1 and CCNA1, was revealed. Similar results were obtained in UNCX-transduced CD34+ cells, associated with low proliferation and differentiation arrest. Accordingly, we showed that UNCX expression characterizes leukemia cells at their early stage of differentiation, mainly M2 and M3 subtypes carrying wild-type NPM1. We also observed that UNCX expression significantly associates with an increased frequency of acute promyelocytic leukemia with PML-RARA and AML with t(8;21)(q22;q22.1); RUNX1-RUNX1T1 classes, according to the World Health Organization disease classification. In summary, our findings suggest a novel leukemogenic role of UNCX, associated with epigenetic modifications and with impaired cell proliferation and differentiation in AML.
Published: 2017
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41. Efficient source localization and tracking in reverberant environments using microphone arrays.

Author: Fabio Antonacci, Davide Lonoce, Marco Motta, Augusto Sarti, and Stefano Tubaro
Published: 2005
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42. COVID-19: yesterday, today and tomorrow. The quality of COVID-19 management and the evaluation of the 'Health' chapter of the Recovery Plan

Author: De Belvis, Antonio, Lonoce, N., Banchieri, G., Scelsi, Silvia, Amoddeo, C. E., Raco, M., De Mattia, Egidio, and DI Stanislao, F.
Subjects: Local health, Italy, Humans, COVID-19, Recovery Plan, Health Facilities, Digital healthcare, Quality management, Settore MED/42 - IGIENE GENERALE E APPLICATA, Pandemics, Delivery of Health Care
Abstract: The COVID-19 pandemic represented an unprecedented challenge for the healthcare world and the introduction of a new stronger and believable project plays a fundamental role for the quality of work and the provision of qualitative care.The survey provided by Italian Association for the Quality of Health and Social Care (ASIQUAS) aims to examines the impact of "Health" chapter included in the Recovery Plan, through the assessment of management quality of the COVID-19 pandemic.Starting from a literature review, in September 2021, a web-based survey has been conducted and administered by e-mail. It has been taken into account measures widely used by different healthcare structures in order to analyze the projects implemented in the face of pandemic and to evaluate the new real possibility to invest funds in new healthcare structures and projects.The survey consists of 19 multiple choices and respondents were from different types of structures, including regional departments and regional health agencies (1.4%), universities, research centers and scientific hospitalization and treatment institutes (IRCCS) (11%), hospitals and university polyclinics (34.2%), Local Health Authorities (39.7%), socio-health organizations and Others (13.7%). The pandemic has highlighted many vulnerabilities at both hospitals and territorial level. The major weaknesses revealed by the survey are mainly due to the lack of support from new staff units and poor availability of specific training tools for COVID-19 procedures. The Recovery Plan is still unclear with a lot of concern about the implementation and many limits of diffusion.It becomes essential to guarantee a new effective and interoperative model of integration. Today we can start more aware for the implementation of a system closer to everyone's needs, making shortcomings the new strength and starting point.
Published: 2022

43. Neurological Involvement in Multisystem Inflammatory Syndrome in Children: Clinical, Electroencephalographic and Magnetic Resonance Imaging Peculiarities and Therapeutic Implications. An Italian Single-Center Experience

Author: Stefania Maria, Bova, Ludovica, Serafini, Pietro, Capetti, Andrea Riccardo, Dallapiccola, Chiara, Doneda, Arianna, Gadda, Luisa, Lonoce, Alessandra, Vittorini, Savina, Mannarino, Pierangelo, Veggiotti, and Mirko, Gambino
Subjects: Pediatrics, Perinatology and Child Health
Abstract: ObjectiveTo describe neurological involvement in multisystem inflammatory syndrome in children (MIS-C) and to evaluate whether neurological manifestations are related to the degree of multiorgan involvement and inflammation.MethodsThe authors conducted a retrospective analysis of clinical, electroencephalographic (EEG), neuroradiological (MRI), and CSF parameters in 62 children with MIS-C (45 M, age 8 months—17 years, mean age 9 years) hospitalized between October 1, 2020 and March 31, 2022.ResultsNeurological involvement was documented in 58/62 (93.5%) patients. Altered mental status was observed in 29 (46.7%), focal neurological signs in 22 (35.4%), and non-specific symptoms in 54 (87%). EEG was performed in 26/62 children: 20 showed EEG slowing, diffuse or predominantly over the posterior regions. Ten patients underwent brain MRI: three showed a cytotoxic lesion of the corpus callosum. CSF analysis, performed in six patients, was normal. On the basis of the clinical and EEG findings, two profiles of neurological involvement were identified: 16/62 (26%) patients presented encephalitis with rapid-onset encephalopathy, focal neurological signs, and EEG slowing; 42/62 (68%) showed mild neurological involvement with mild or non-specific neurological signs. All patients received intravenous immunoglobulin and methylprednisolone (MTP), low-molecular-weight heparin, and therapeutic-dose anticoagulant treatment. Children with severe encephalopathy received intravenous MTP at 30 mg/kg/day for 3 days, obtaining rapid clinical and EEG improvement. Neurological assessment at discharge was normal in all cases. Children with encephalitis were younger than those without (median age 5 and 10 years, respectively); no differences between the two groups were found in the other parameters: comorbidities, fever, number of organs and systems involved, shock, hospitalization, pediatric intensive care unit admission, non-invasive ventilation, inotropic support, laboratory data.ConclusionNeurological involvement in MIS-C is frequent but not serious in most cases: around two thirds of the affected children had mild and short-lasting symptoms. It seems to be related to age, but not to the degree of multiorgan involvement and inflammation. In children with acute immune-mediated encephalitis, the clinical picture was dominated by encephalopathy that disappeared with immunomodulatory therapy. Neurological assessment allowed timely diagnosis and treatment.
Published: 2022

44. Subchromosomal painting libraries (SCPLs) from somatic cell hybrids

Author: Rocchi, M., Antonacci, R., Marzella, R., Finelli, P., Cassano, C., Lonoce, A., Cino, C., Forabosco, A., Archidiacono, N., Henriques-Gil, N., editor, Parker, J. S., editor, and Puertas, M. J., editor
Published: 1997
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45. Stellar Population and Elemental Abundance Gradients of Early-type Galaxies

Author: Anja Feldmeier-Krause, Wendy Freedman, and Ilaria Lonoce
Subjects: Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Computer Science::Information Retrieval, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics::Galaxy Astrophysics
Abstract: The evolution of galaxies is imprinted in their stellar populations. Several stellar population properties in massive early-type galaxies have been shown to correlate with intrinsic galaxy properties like the galaxy's central velocity dispersion, suggesting that stars formed in an initial collapse of gas (z~2). However, stellar populations change as a function of galaxy radius, and it is not clear how local gradients of individual galaxies are influenced by global galaxy properties and galaxy environment. In this paper, we study the stellar populations of eight early-type galaxies as a function of radius. We use optical spectroscopy (~4000-8600 \r{A}) and full-spectral fitting to measure stellar population age, metallicity, IMF slope, and nine elemental abundances (O, Mg, Si, Ca, Ti, C, N, Na, Fe) out to 1 R_e for each galaxy individually. We find a wide range of properties, with ages ranging from 3-13 Gyr. Some galaxies have a radially constant, Salpeter-like IMF, and other galaxies have a super-Salpeter IMF in the center, decreasing to a sub-Salpeter IMF at ~0.5 R_e. We find a global correlation of the central [Z/H] to the central IMF and the radial gradient of the IMF for the eight galaxies, but local correlations of the IMF slope to other stellar population parameters hold only for subsets of the galaxies in our sample. Some elemental abundances also correlate locally with each other within a galaxy, suggesting a common production channel. Those local correlations appear only in subsets of our galaxies indicating variations of the stellar content among different galaxies., Comment: 20 pages, 11 figures, 4 tables (37 pages, 17 figures, 6 tables incl. Appendix). Accepted for publication in ApJ
Published: 2021

46. A rare but recurrent t(8;13)(q24;q14) translocation in B-cell chronic lymphocytic leukaemia causing MYC up-regulation and concomitant loss of PVT1, miR-15/16 and DLEU7

Author: Macchia, Gemma, Lonoce, Angelo, Venuto, Santina, Macrí, Ettore, Palumbo, Orazio, Carella, Massimo, Lo Cunsolo, Crocifissa, Iuzzolino, Paolo, Hernández-Sánchez, María, Hernandez-Rivas, Jesus M., and Storlazzi, Clelia T.
Published: 2016
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47. Sepolture bisome dalle necropoli della colonia greca di Himera: interpretazione e analisi demografica

Author: Viva S., Lonoce N., Fabbri P. F., M. Chiovaro e R. Sapia (a cura di), Viva, S., Lonoce, N., and Fabbri, P. F.
Subjects: Sicilia, Himera, Necropoli, Sepolture bisome, Demografia
Abstract: Double burials, ie simultaneous depositions of two individuals, are rare occurrence in ancient Greece, so their discovery is always received with great interest. In the necropolises of Himera, only 15 double burials were discovered, out of over 13000 excavated tombs. With the exception of these and the mass graves relating to the battles of 480 and 409 BC, the necropolises of Himera are characterized by single burials. The taphonomic analyses, aimed at demonstrating the simultaneity of double burials, and the anthropological analyses to determine sex and age at death, show a skeletal sample that is decidedly heterogeneous by type of tomb, sex and age. Given the variety of the composition of the double burials it seems that there is no rule except simultaneous death and probably a bond between the people buried together.
Published: 2020

48. Management of pneumonia in emergency department: utility of chest radiography reviewed by a pediatric pneumologist and a pediatric radiologist

Author: Gian Vincenzo Zuccotti, Marco Morelli, Martina Pascuzzi, Andrea Farolfi, Luisa Lonoce, Michele Ghezzi, and Salvatore Zirpoli
Subjects: Pneumonia, medicine.medical_specialty, business.industry, Radiography, Pediatric Radiologist, Emergency medicine, medicine, Emergency department, medicine.disease, business
Published: 2021
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49. Barrier Impairment and Type 2 Inflammation in Allergic Diseases: The Pediatric Perspective

Author: Ghezzi, Michele, primary, Pozzi, Elena, additional, Abbattista, Luisa, additional, Lonoce, Luisa, additional, Zuccotti, Gian Vincenzo, additional, and D’Auria, Enza, additional
Published: 2021
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50. Stellar Population and Elemental Abundance Gradients of Early-type Galaxies*

Author: Feldmeier-Krause, A., primary, Lonoce, I., additional, and Freedman, W. L., additional
Published: 2021
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