cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lactobacillus hominis
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Lactobacillus
Lactobacillus hominis

description: Lactobacillus hominis
Lactobacillus hominis (ho’mi.nis. L. gen. n. hominis of a human being).
Lactobacillus hominis produces acid from galactose, glucose, fructose, mannose, cellobiose, maltose, lactose, sucrose, trehalose and raffinose. Mainly D-lactic acid (about 90 %) is produced from glucose [93]. The genome size is 1.93 Mbp and the mol% G+C content of DNA is 35.2.
Isolated from the human intestine.
Thetypestrainis 61DT=CRBIP 24.179 T =DSM 23910 T.
Genome sequence accession number: AYZP00000000.
16S rRNA gene accession number: FR681902.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2797, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Compendium chronologicum canoniae Rohrensis. A primo fundationis a[nno] 1133 usque ad an[num] 1682 perductum complectens acta et gesta abbatum 39: nec non privilegia s[anctis]s[imorum] pontificum, aliorumque principum litteras confirmat. Et c[etera] ac alia quaedam memorabilia. His ab a[nno] 1715 usque ad an[num] 1759 accedunt et continuantur facta et gesta reliquorum trium praelatorum, una cum aliis rebus memoratu dignis. (1v) Notandum. Animadversio. Praefatio. (3r) Compendium chronologicum. Ex parte prima annalium traductum comprehendens acta abbatum 13. (13v) Compendium chronolog[icum]. Ex parte secunda annalium desumptum complectens acta abbatum 12. (23v) Compendium chronologicum. Ex parte tertia annalium exceptum, continens acta abbatum 14. (37v) Compendium chronologicum prosequens acta et gesta reliquorum abbatum, aliasque res memorabiliores ab anno 1715 usque 1759. (56r) Index duplex. (66r) Appendix variorum pontificum, episcoporum, imperatorum, regum, aliorumque principum: Bullae, diplomata, ac litterae, quibus canoniae Rohrensi varia bona donantur.; [nach 1759]
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Entstehungsort: [Rohr]. - Entstehungszeit:
The interaction of the active nucleus with the host galaxy interstellar medium
Creators: name: Fabbiano, G.
name: Elvis, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Imaging X-ray spectroscopy of nearby AGNs, mostly with Chandra, has shown that extended soft (<2.5 keV) emission-line dominated X-ray biconical structures, of kiloparsec scale, are widespread in highly absorbed Compton Thick (CT) AGNs. The X-ray emission is complex, requiring both photoionized and shock-ionized gas. It originates from high ionization regions and is surrounded by cocoons of low ionization narrow line emission regions (LINERS). Bicone 3-6 keV continuum and 6.4 keV Fe Kalpha emission has been detected, contrary to the standard AGN model expectation that would confine this hard emission to the pc-size nuclear absorbing torus. Extended emission in the cross-cone direction, also requires modifications to the AGN standard model. A porous torus, with a significant fraction of escaping AGN continuum, and/or jet interaction with ISM creating a blow-back towards the nuclear region seem to be required. Here we discuss these results and their implications for both the AGN model and our understanding of AGN feedback. The finding of hot and highly photoionized gas on 10s parsecs to several kiloparsec scales demonstrates that all three feedback mechanisms are at work: radiation affects the inner molecular clouds of the host on a ~1 kpc scale; shocks of relativistic jets with the host ISM a few kpc from the central AGN; and photoionization of the ISM via winds on scales from pc to multiple kpc. These results demonstrate that X-rays are needed to develop a complete picture of AGN/host interaction along with radio continuum, mm and sub-mm molecular line emission, and optical/near-IR emission lines.
description: This is a review mostly based on Chandra results on the extended X-ray emission of AGNs. It will be included in the Section on Galaxies of the Handbook on X-ray and Gamma ray Astrophysics, A. Santangelo and C. Bambi (eds.), Springer. Comments welcome
"susy.371359.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
Puzza di uova marce sull’esopianeta Hd 189733 b
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2024

L’esopianeta Hd 189733 b, a 64 anni luce dalla Terra, è noto per il suo clima infernale. Ora, un nuovo studio della Johns Hopkins University ne svela un'altra bizzarra caratteristica: puzza di uova marce. Il pianeta ha infatti un'atmosfera composta prevalentemente da acido solfidrico, molecola che permetterà di carpire nuovi indizi su come lo zolfo potrebbe influenzare l'interno e le atmosfere dei mondi gassosi
On quantitative hypocoercivity estimates based on Harris-type theorems
Creators: name: Yoldaş, Havva
Publisher: name: arXiv
Year: 2022
Subjects: subject: Analysis of PDEs (math.AP)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 35B40, 35Q20, 35Q92, 37A25, 60J25

description: This review concerns recent results on the quantitative study of convergence towards the stationary state for spatially inhomogeneous kinetic equations. We focus on analytical results obtained by means of certain probabilistic techniques from the ergodic theory of Markov processes. These techniques are sometimes referred to as Harris-type theorems. They provide constructive proofs for convergence results in the $L^1$ (or total variation) setting for a large class of initial data. The convergence rates can be made explicit (both for geometric and sub-geometric rates) by tracking the constants appearing in the hypotheses. Harris-type theorems are particularly well-adapted for equations exhibiting non-explicit and non-equilibrium steady states since they do not require prior information on the existence of stationary states. This allows for significant improvements of some already-existing results by relaxing assumptions and providing explicit convergence rates. We aim to present Harris-type theorems, providing a guideline on how to apply these techniques to the kinetic equations at hand. We discuss recent quantitative results obtained for kinetic equations in gas theory and mathematical biology, giving some perspectives on potential extensions to nonlinear equations.
description: 40 pages, typos are corrected, new references are added and structure of the paper has changed
title: Rheumatic side effects of checkpoint inhibitors
title: Les effets indésirables rhumatologiques des inhibiteurs des checkpoints
Creators: name: Toufik, Hamza
Publisher: name: Revue Marocaine de Rhumatologie (RMR)
Year: 2020
Subjects: Immunothérapie; Cancers; Inhibiteurs des checkpoints; IRAEs rhumatologique.

description: Immunotherapy has revolutionized the management of cancer. The use of immune checkpoint inhibitors (ICI) is associated with a new group of adverse events -immun related adverse events- (IRAEs) which can affect all organs. Among these IRAEs, rheumatic complications are common and seem to have distinct pathophysiological, clinical, and therapeutic characteristics. In this review will be described, the mechanisms of action of ICI, the way in which they can cause rheumatic IRAEs, epidemiology, clinical presentation, and management of these complications.
description: L'immunothérapie a révolutionné la prise en charge thérapeutique des cancers. L'utilisation de la famille des inhibiteurs des checkpoints immunitaire (ICI) est associée à un nouveau groupe d'événements indésirables d'origine immunologique -immun related adverse events- (IRAEs) qui peuvent toucher tous les organes. Parmi ces IRAEs, les complications rhumatismales sont courantes et semblent présenter des caractéristiques distinctes sur les plans physiopathologiques, cliniques, et thérapeutiques. Dans cette revue seront décrits, les mécanismes d’action des ICI, la façon dont ils peuvent provoquer des IRAEs rhumatismales avec leur épidémiologie, leur présentation clinique, ainsi que leur prise en charge thérapeutique.
L’Etna erutta al chiarore della Via Lattea
Creators: Giuseppe Fiasconaro
Publisher: name: Media Inaf
Year: 2024

Skyline del più grande vulcano attivo d’Europa, l’Etna, sotto una Via Lattea che domina il cielo. È lo scatto scelto dalla Nasa come immagine astronomica del giorno – o Apod, Astronomy picture of the day – del 5 luglio scorso. A realizzarlo, proprio mentre l’Etna dava spettacolo di sé con la sua attività effusiva, è un volto noto di Media Inaf, già autore di diverse Apod: l’astrofotografo Gianni Tumino
Edge magnetoplasmons in graphene
Creators: name: Petkovic, Ivana
name: Williams, F. I. B.
name: Glattli, D. Christian
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We have observed propagation of Edge Magneto-Plasmon (EMP) modes in graphene in the Quantum Hall regime by performing picosecond time of flight measurements between narrow contacts on the perimeter of micrometric exfoliated graphene. We find the propagation to be chiral with low attenuation and to have a velocity which is quantized on Hall plateaus. The velocity has two contributions, one arising from the Hall conductivity and the other from carrier drift along the edge, which we were able to separate by their different filling factor dependence. The drift component is found to be slightly less than the Fermi velocity as expected for graphene dynamics in an abrupt edge potential. The Hall conduction contribution is slower than expected and indicates a characteristic length in the Coulomb potential from the Hall charge of about 500 nm. The experiment illustrates how EMP can be coupled to the electromagnetic field, opening the perspective of GHz to THz chiral plasmonics applications to devices such as voltage controlled phase shifters, circulators, switches and compact, tunable ring resonators.
description: 17 pages, 8 figures
"susy.371360.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
Theoretical study of ThO for the electron electric dipole moment search
Creators: name: Skripnikov, L. V.
name: Petrov, A. N.
name: Titov, A. V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: An experiment to search for the electron electric dipole moment (\eEDM) on the metastable $H^3Δ_1$ state of ThO molecule was proposed and now in the final stage of preparation by the ACME collaboration [http://www.electronedm.org]. To interpret the experiment in terms of \eEDM\ and dimensionless constant $k_{T,P}$ characterizing the strength of the scalar T,P-odd electron-nucleus neutral current interaction, an accurate theoretical study of effective electric field on electron, Eeff, and $W_{T,P}$ constants is required. We report calculation of \Eeff\ (84 GV/cm) and a parameter of T,P-odd scalar neutral currents interaction, $W_{T,P}$ (116 kHz), together with the hyperfine structure constant, molecule frame dipole moment and $H^3Δ_1\to X^1Σ^+$ transition energy, which can serve as a measure of reliability of the obtained \Eeff\ and $W_{T,P}$ values. Besides, our results include a parity assignment and evaluation of the electric-field dependence for the magnetic $g$ factors for the $Ω$-doublets of $H^3Δ_1$.
"susy.371361.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
"susy.371362.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
"susy.371363.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
Stability of backward stochastic differential equations: the general case
Creators: name: Papapantoleon, Antonis
name: Possamaï, Dylan
name: Saplaouras, Alexandros
Publisher: name: arXiv
Year: 2021
Subjects: subject: Probability (math.PR)
subject: Optimization and Control (math.OC)
subject: Mathematical Finance (q-fin.MF)
subject: FOS: Mathematics
subject: FOS: Economics and business
subject: 60F15, 60F17, 60F25, 60G05, 60G07, 60G44, 60G048, 60G57, 60H05, 60H20

description: In this paper, we obtain stability results for backward stochastic differential equations with jumps (BSDEs) in a very general framework. More specifically, we consider a convergent sequence of standard data, each associated to their own filtration, and we prove that the associated sequence of (unique) solutions is also convergent. The current result extends earlier contributions in the literature of stability of BSDEs and unifies several frameworks for numerical approximations of BSDEs and their implementations.
description: 45 pages, final version, forthcoming in the Electronic Journal of Probability
Potremmo essere soli nella Via Lattea
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2024

Il motivo per cui non sono state trovate evidenze di civiltà extraterrestri avanzate – nonostante l'equazione di Drake preveda che nella nostra galassia dovrebbero essercene molte, in grado di comunicare con noi – potrebbe essere di natura geologica. Oceani, continenti e tettonica delle placche sembrano essere ingredienti indispensabili per l'evoluzione di civiltà attive e comunicative. Tutti i dettagli su Nature's Scientific Reports
"susy.371364.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
Phase diagrams of magnetopolariton gases
Creators: name: Kochereshko, V. P.
name: Durnev, M. V.
name: Besombes, L.
name: Mariette, H.
name: Sapega, V. F.
name: Axitopoulos, A.
name: Savenko, I. G.
name: Liew, T. C. H.
name: Shelykh, I. A.
name: Platonov, A. V.
name: Tsintzos, S. I.
name: Hatzopoulos, Z.
name: Lagoudakis, P.
name: Savvidis, P. G.
name: Schneider, C.
name: Amthor, M.
name: Metzger, C.
name: Kamp, M.
name: Hoefling, S.
name: Kavokin, A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The magnetic field effect on phase transitions in electrically neutral bosonic systems is much less studied than those in fermionic systems, such as superconducting or ferromagnetic phase transitions. Nevertheless, composite bosons are strongly sensitive to magnetic fields: both their internal structure and motion as whole particles may be affected. A joint effort of ten laboratories has been focused on studies of polariton lasers, where non-equilibrium Bose-Einstein condensates of bosonic quasiparticles, exciton-polaritons, may appear or disappear under an effect of applied magnetic fields. Polariton lasers based on pillar or planar microcavities were excited both optically and electrically. In all cases a pronounced dependence of the onset to lasing on the magnetic field has been observed. For the sake of comparison, photon lasing (lasing by an electron-hole plasma) in the presence of a magnetic field has been studied on the same samples as polariton lasing. The threshold to photon lasing is essentially governed by the excitonic Mott transition which appears to be sensitive to magnetic fields too. All the observed experimental features are qualitatively described within a uniform model based on coupled diffusion equations for electrons, holes and excitons and the Gross-Pitaevskii equation for exciton-polariton condensates. Our research sheds more light on the physics of non-equilibrium Bose-Einstein condensates and the results manifest high potentiality of polariton lasers for spin-based quantum logic applications.
description: 21 pages, 11 figures
Lactobacillus iners
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Lactobacillus
Lactobacillus iners

description: Lactobacillus iners
Lactobacillus iners (in’ers. L. masc. adj. iners, inactive, lazy).
Lactobacillus iners grows on blood agar but not on MRS or Rogosa agar, reflecting a strict adaptation to the human vagina. L(+)-Lactic acid is producedfrom glucose, some strains produce acid from maltose but acid is not produced from lactose, mannitol, raffinose, ribose andsucrose [94]. The genome size is 1.27 Mbp and the mol% G+C content of DNA is 32.5.
One of the predominant species found in the human female lower genital tract; also occurs on human skin [95]
Thetypestrainis CCUG 28746 T =CIP 105923 T =DSM 13335 T =JCM 12513 T =LMG 18914 T.
Genome sequence accession number: AZET00000000.
16S rRNA gene accession number: Y16329.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2797, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
"susy.371365.pMSSM_M3muM1lsp.slha" of "Search for new phenomena with large jet multiplicities and missing transverse momentum using large-radius jets and flavour-tagging at ATLAS in 13 TeV $pp$ collisions"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2017

description: SLHA file for the pMSSM signal in Figure 6a
description: CERN-LHC. A search is presented for particles that decay producing a large jet multiplicity and invisible particles. The event selection applies a veto on the presence of isolated electrons or muons and additional requirements on the number of $b$-tagged jets and the scalar sum of masses of large-radius jets. Having explored the full ATLAS 2015--2016 dataset of LHC proton--proton collisions at $\sqrt{s}$=13 TeV, which corresponds to 36.1~fb$^{-1}$ of integrated luminosity, no evidence is found for physics beyond the Standard Model.The results are interpreted in the context of simplified models inspired by R-parity-conserving and R-parity-violating supersymmetry, where gluinos are pair-produced. More generic models within the phenomenological minimal supersymmetric Standard Model are also considered.
Quantifying the Predictability of ENSO Complexity Using a Statistically Accurate Multiscale Stochastic Model and Information Theory
Creators: name: Fang, Xianghui
name: Chen, Nan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Applications (stat.AP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: An information-theoretic framework is developed to assess the predictability of ENSO complexity, which is a central problem in contemporary meteorology with large societal impacts. The information theory advances a unique way to quantify the forecast uncertainty and allows to distinguish the predictability limit of different ENSO events. One key step in applying the framework to compute the information gain representing the predictability is to build a statistically accurate dynamical model. To this end, a recently developed multiscale stochastic model, which succeeds in capturing both the large-scale dynamics and many crucial statistical properties of the observed ENSO complexity, is incorporated into the information-theoretic framework. It is shown that different ENSO events possess very distinct predictability limits. In addition to the ensemble mean, the ensemble spread also has remarkable contributions to the predictability. While the information theory indicates that predicting the onset of the eastern Pacific El Niños is challenging, it reveals a universal tendency to convert strong predictability to skillful forecast for predicting many central Pacific El Niños about two years in advance. In addition, strong predictability is found for the La Niña events, corresponding to the effective discharge process. In the climate change scenario with the strengthening of the background Walker circulation, the predictability of sea surface temperature in central Pacific has a significant response with a notable increase in summer and fall. Finally, the Gaussian approximation is shown to be accurate in computing the information gain, which facilitates the use of more sophisticated models to study the ENSO predictability.
description: 19 figures
An O2If* star found in isolation in the backyard of NGC 3603
Creators: name: Roman-Lopes, A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this letter we communicate the identification of a new Galactic O2If* star (MTT 68) isolated at a projected linear distance of 3 pc from the centre of the star-burst cluster NGC 3603. From its optical photometry I computed a bolometric luminosity M_Bol = -10.7, which corresponds to a total stellar luminosity of 1.5 x 10^{6} L_Sun. It was found an interesting similarity between MTT 68 and the well known multiple system HD 93129. From Hubble Space Telescope F656N images of the NGC 3603 field, it was found that MTT 68 is actually a visual binary system with an angular separation of 0.38 arcsec, which corresponds to a projected (minimum) linear distance of r_(A-B) = 1.4 x 10^{-2} pc. This value is similar to that for the HD 93129A (O2If*) and HD 93129B (O3.5) pair, r_(A-B) = 3.0 x 10^{-2} pc. On the other hand, HD93129A has a third closer companion named HD 93129Ab (O3.5) at only 0.053 arcsec, and taking into account that the X-ray to total stellar luminosity ratio for the MTT 68 system (L_X/L_Bol 10^{-5}) is about two orders of magnitude above the canonical value expected for single stars, I suspect that the MTT 68 system probably hosts another massive companion not resolved by the HST archive images.
description: 5 pages, 4 figures, accepted for publication on MNRAS letters
Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing Survey
Creators: name: Sklias, P.
name: Zamojski, M.
name: Schaerer, D.
name: Dessauges-Zavadsky, M.
name: Egami, E.
name: Rex, M.
name: Rawle, T.
name: Richard, J.
name: Boone, F.
name: Simpson, J. M.
name: Smail, I.
name: van der Werf, P.
name: Altieri, B.
name: Kneib, J. P.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Multi-wavelength, optical to IR/sub-mm observations of 5 strongly lensed galaxies identified by the Herschel Lensing Survey, plus two well-studied lensed galaxies, MS1512-cB58 and the Cosmic Eye, for which we also provide updated Herschel measurements, are used to determine the physical properties of z~1.5-3 star-forming galaxies close to or below the detection limits of blank fields. We constrain their stellar and dust content, determine star formation rates and histories, dust attenuation and extinction laws, and other related properties. We perform SED-fits of the full photometry of each object as well for the optical and infrared parts separately, exploring various parameters, including nebular emission. The IR observations and emission line measurements, where available, are used a posteriori constraints on the models. Besides the various stellar population models we explore, we use the observed IR/UV ratio to estimate the extinction and create "energy conserving models", that constrain most accurately the physical properties of our sources. Our sample has a median lensing-corrected IR luminosity ~ 3e11 Lsun, stellar masses between 2e9 and 2e11 Msun, and IR/UV luminosity ratios spanning a wide range. The dust masses of our galaxies are in the range 2 to 17e7 Msun, extending previous studies at the same redshift down to lower masses. We do not find any particular trend of the dust temperature Tdust with IR luminosity, suggesting an overall warmer dust regime at our redshift regardless of luminosity. Lensing enables us to study the detailed physical properties of individual IR-detected z~1.5-3 galaxies up to a factor ~10 fainter than achieved with deep blank field observations. We demonstrate that multi-wavelength observations combining stellar and dust emission can constrain star formation histories and extinction laws of star-forming galaxies.
description: 27 pages, 19 figures
Via libera ai lanciatori spaziali europei
Creators: Rossella Spiga
Publisher: name: Media Inaf
Year: 2024

Il Consiglio dell'Agenzia spaziale europea ha deciso di aprire la strada alla commercializzazione del lanciatore Vega, arrivando finalmente alla risoluzione di un nodo importante sui servizi di lancio europei e sulla continuità dell'accesso europeo allo spazio. Con un commento di Patrizia Caraveo
RGE, the naturalness problem and the understanding of the Higgs mass term
Creators: name: Bian, Ligong
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The naturalness problem might be studied on the complex two dimensional plane with the technique of dimensional regularization(DREG). The Renormalization group equation(RGE) of the Higgs mass on the plane suggests the Higgs mass approaches zero at ultraviolate (UV) scale, the scale can be Planck scale when the top quark pole mass $M_{t}=168$ GeV. The real issue of the naturalness problem in the sense of Wilsonian renormalization group method is not about quadratic divergences but the rescaling effect. The Higgs mass can be considered to be one composed mass. All terms in the lagrangian in this scenario are marginal terms and no relevant terms are left, thus no rescaling effect to cause the naturalness problem anymore. RGE of the vacuum expectation value (VEV) in the Landau gauge up to two-loop order is studied. Scale-dependent behavior of the composed Higgs mass shows that we can have one tiny Higgs mass at high energy scale, even around the Planck scale, when $M_{t}\leq170.7$ GeV.
description: 16pages, 9figures, accepted for publication as a Regular Article in Physical Review D
Jwst cattura la drammatica fusione quasar-galassie
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2024

Osservate con il telescopio spaziale James Webb le interazioni tra un lontanissimo quasar e due galassie satelliti massicce nell’universo lontano, a meno di un miliardo di anni dopo il Big Bang. Lo studio, guidato da Roberto Decarli e Federica Loiacono dell’Inaf di Bologna, conferma che si tratta un sistema estremamente evoluto, sia in termini di massa che di evoluzione chimica
Origine della vita? La risposta di Marte
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2024

Per indagare i processi chimici che potrebbero aver originato le prime molecole organiche sulla Terra, si può osservare Marte. Dall’analisi di alcuni campioni del rover Curiosity sono infatti emerse evidenze in favore di un processo, chiamato fotolisi, che sarebbe avvenuto nell’atmosfera del Pianeta rosso e avrebbe preparato il terreno alla formazione di queste molecole
Emotion Regulation and Dynamics of Moral Concerns During the Early COVID-19 Pandemic
Creators: name: Guo, Siyi
name: Burghardt, Keith
name: Rao, Ashwin
name: Lerman, Kristina
Publisher: name: arXiv
Year: 2022
Subjects: subject: Social and Information Networks (cs.SI)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: The COVID-19 pandemic has upended daily life around the globe, posing a threat to public health. Intuitively, we expect that surging cases and deaths would lead to fear, distress and other negative emotions. However, using state-of-the-art methods to measure sentiment, emotions, and moral concerns in social media messages posted in the early stage of the pandemic, we see a counter-intuitive rise in positive affect. We hypothesize that the increase of positivity is associated with a decrease of uncertainty and emotion regulation. Finally, we identify a partisan divide in moral and emotional reactions that emerged after the first US death. Overall, these results show how collective emotional states have changed since the pandemic began, and how social media can provide a useful tool to understand, and even regulate, diverse patterns underlying human affect.
Basics of Fourier Analysis for High-Energy Astronomy
Creators: name: Belloni, T. M.
name: Bhattacharya, D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The analysis of time variability, whether fast variations on time scales well below the second or slow changes over years, is becoming more and more important in high-energy astronomy. Many sophisticated tools are available for data analysis and complex practical aspects are described in technical papers. Here, we present the basic concepts upon which all these techniques are based. It is intended as a condensed primer of Fourier analysis, dealing with fundamental aspects that can be examined in detailed elsewhere. It is not intended to be a presentation of detailed Fourier tools for data analysis, but the reader will find the theoretical basis to understand available analysis techniques.
description: 38 pages, 18 figures. This Chapter will appear in the Section "Timing Analysis" of the "Handbook of X-ray and Gamma-ray Astrophysics" (Editors in chief: C. Bambi and A. Santangelo)
Così ticchetta l’orologio più preciso al mondo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2024

Realizzato al Jila con un gas ultrafreddo di atomi di stronzio intrappolati in un reticolo ottico, non perde più di un secondo ogni 30 miliardi di anni. La sua accuratezza è tale da poter misurare le dilatazioni del tempo dovute a effetti di relatività generale anche a scale microscopiche. Le potenziali applicazioni vanno dalla ricerca di giacimenti minerari ai computer quantistici e alla navigazione interplanetaria
The AstroSat Observatory
Creators: name: Singh, Kulinder Pal
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: AstroSat is India's first Ultra-violet (UV) and X-ray astronomy observatory in space. The satellite was launched by the Indian Space Research Organisation on a Polar Satellite Launch Vehicle on 28 September 2015 from Sriharikota Range north of Chennai on the eastern coast of India. AstroSat carries five scientific instruments and one auxiliary instrument. Four of these consist of co-aligned telescopes and detectors mounted on a common deck of the satellite to observe stars and galaxies simultaneously in the near- and far-UV wavelengths and a broad range of X-ray energies (0.3 to 80 keV). The fifth instrument consists of three X-ray detectors and is mounted on a rotating platform on a side that is oriented 90 degrees with respect to the other instruments to scan the sky for X-ray transients. An auxiliary instrument monitors the charged particle environment in the path of the satellite.
description: 37 pages, 27 figures. This chapter will appear in "Section III (X-ray missions) of the first volume (X-ray Experimental Techniques and Missions), of the "Handbook of X-ray and Gamma-ray Astrophysics" (Section editors: Arvind Parmar, Shuang-Nan Zhang, Andrea Santangelo; Editors in chief: C. Bambi and A. Santangelo)
Pryms of non-cyclic triple coverings and log canonical models of the spin moduli space of genus 2
Creators: name: Lange, Herbert
name: Ortega, Angela
Publisher: name: arXiv
Year: 2013
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14H10, 14H30, 14H40

description: We show that the moduli spaces of non-triple cyclic coverings of genus 2 curves and that of even spin curves of genus 2 are birationally isomorphic via the Prym map. We describe the log canonical models of the moduli space of even spin curves of genus 2 and use this to extend the above birational map.
description: 24 pages, 1 figure
Chiral phonons in binary compounds $A$Bi ($A$ = K, Rb, Cs) with P2$_1$/c structure
Creators: name: Skórka, Jakub
name: Kapcia, Konrad J.
name: Jochym, Paweł T.
name: Ptok, Andrzej
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Binary compounds $A$Bi ($A$ = K, Rb, Cs) crystallize in P2$_1$/c structure containing both clockwise and anticlockwise chiral chains of Bi atoms. Electronic band structure exhibits the insulating nature of these systems, with the band gap about $0.25$ eV. The presented study of dynamical properties confirm a stability of the system with P2$_1$/c symmetry. The crystal structure contains the quasi-one-dimensional Bi chains, exhibiting four-fold-like rotational ``local'' symmetry. Nevertheless, the system formally posses two-fold rotational symmetry. Independently of the absence of the three-fold (or higher) rotational symmetry axes for the whole crystal, the chiral modes propagate along the Bi atom chains in these systems. We discuss basic properties of these modes in monoatomic chiral chains. We show that the two-fold rotational symmetry axis affects the main properties of the chiral phonons, which are not realized at the high-symmetry points, but along some paths between them in the reciprocal space. In addition, in the doped system, the chiral phonons possess non-zero total angular momentum.
description: 17 pages, 7 figures
Nuove esercitazioni di impatto con un asteroide
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2024

Sebbene non siano note minacce significative di impatto di asteroidi in futuro, esercitarsi su scenari ipotetici consente di esplorare i rischi, le opzioni di risposta e le opportunità di collaborazione fra agenzie ed enti preposti alla difesa planetaria a livello internazionale. Davide Farnocchia racconta l’ultima esercitazione della Nasa, la quinta nella storia a simulare il rischio di impatto di un asteroide sulla Terra
Single Quasiparticle Trapping in Aluminum Nanobridge Josephson Junctions
Creators: name: Levenson-Falk, E. M.
name: Kos, F.
name: Vijay, R.
name: Glazman, L.
name: Siddiqi, I.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present microwave measurements of a high quality factor superconducting resonator incorporating two aluminum nanobridge Josephson junctions in a loop shunted by an on-chip capacitor. Trapped quasiparticles (QPs) shift the resonant frequency, allowing us to probe the trapped QP number and energy distribution and to quantify their lifetimes. We find that the trapped QP population obeys a Gibbs distribution above 75 mK, with non-Poissonian trapping statistics. Our results are in quantitative agreement with the Andreev bound state model of transport, and demonstrate a practical means to quantify on-chip QP populations and validate mitigation strategies in a cryogenic environment.
Alticola albicauda
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Alticola
Alticola albicauda

description: Alticola albicauda (True, 1894). Proc. U. S. Natl. Mus., 17: 12. TYPE LOCALITY: India, Baltistan, Braldu Valley. DISTRIBUTION: Recorded only from the Himalayan portions of Baltistan and Kashmir, NW India. SYNONYMS: acmaeus. COMMENTS: Subgenus Alticola. Although usually included in A. roylei (Corbet, 1978c; Ellerman and Morrison-Scott, 1951; Gromov and Polyakov, 1977), the diagnostic traits of albicauda that set it apart as a distinct species were earlier pointed out by Hinton (1926). Schwarz's (1939) acmaeus identifies a geographic variant of the same species.
description: Published as part of Guy G. Musser & Michael D. Carleton, 1993, Order Rodentia - Family Muridae, pp. 501-755 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 502, DOI: 10.5281/zenodo.7353098
description: {"references": ["Corbet, G. B. 1978 c. The mammals of the Palaearctic region: A taxonomic review. British Museum (Natural History), London, 314 pp.", "Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Gromov, I. M., and I. Ya. Polyakov. 1977. Fauna SSSR, Mlekopitayushchie, tom 3, vyp. 8 [Fauna of the USSR, vol. 3, pt. 8, Mammals]. Polevki [Voles (Microtinae)]. Nauka, Moscow-Leningrad, 504 pp. (in Russian).", "Schwarz, E. 1939. On mountain-voles of the genus Alticola Blanford: A taxonomic and genetic analysis. Proceedings of the Zoological Society of London, ser. B, 108: 663 - 668."]}
Lactobacillus intestinalis
Creators: name: Zheng, Jinshui
name: Wittouck, Stijn
name: Salvetti, Elisa
name: Franz, Charles M. A. P.
name: Harris, Hugh M. B.
name: Mattarelli, Paola
name: O'Toole, Paul W.
name: Pot, Bruno
name: Vandamme, Peter
name: Walter, Jens
name: Watanabe, Koichi
name: Wuyts, Sander
name: Felis, Giovanna E.
name: Gänzle, Michael G.
name: Lebeer, Sarah
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Bacteria
Firmicutes
Bacilli
Lactobacillales
Lactobacillaceae
Lactobacillus
Lactobacillus intestinalis

description: Lactobacillus intestinalis
Lactobacillus intestinalis (in.tes.tina’lis. N.L. masc. adj. intestinalis, pertaining to the intestine).
Lactobacillus intestinalis produces DL-lactic acid from glucose, mannose, fructose, galactose, sucrose and mannitol, but not from arabinose, xylose, rhamnose and trehalose [96]. The genome size is 2.01 Mbp and the mol% G+C content of DNA is 35.4.
Isolated from the intestines of rats, mice and pigs.
Thetypestrainis Th4 T =ATCC 49335 T =CCUG 30727 T =CIP 104793 T =DSM 6629 T =JCM 7548 T =LMG 14196 T.
Genome sequence accession number: AZGN00000000.
16S rRNA gene accession number: AJ306299.
description: Published as part of Zheng, Jinshui, Wittouck, Stijn, Salvetti, Elisa, Franz, Charles M. A. P., Harris, Hugh M. B., Mattarelli, Paola, O'Toole, Paul W., Pot, Bruno, Vandamme, Peter, Walter, Jens, Watanabe, Koichi, Wuyts, Sander, Felis, Giovanna E., Gänzle, Michael G. & Lebeer, Sarah, 2020, A taxonomic note on the genus Lactobacillus: Description of 23 novel genera, emended description of the genus Lactobacillus Beijerinck 1901, and union of Lactobacillaceae and Leuconostocaceae, pp. 2782-2858 in International Journal of Systematic and Evolutionary Microbiology 70 on page 2797, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
A Bologna l’estate è tempo di scienza
Creators: Antonio De Blasi
Publisher: name: Media Inaf
Year: 2024

Tutto il mese di luglio il quartiere San Donato-San Vitale di Bologna sarà all’insegna dell’astronomia, con sette eventi di divulgazione scientifica organizzati da Sofos Aps e Inaf-Oas per Bologna Estate 2024. Si parte venerdì con un incontro letterario, ospite Maria Giulia Andretta, autrice di “Stregati dalla Luna” e “Dalla Terra a Marte”
Maxima of the Q-index: graphs with bounded clique number
Creators: name: de Abreu, Nair Maria Maia
name: Nikiforov, Vladimir
Publisher: name: arXiv
Year: 2013
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05C50

description: This paper gives a tight upper bound on the spectral radius of the signless Laplacian of graphs of given order and clique number. More precisely, let G be a graph of order n, let A be its adjacency matrix, and let D be the diagonal matrix of the row-sums of A. If G has clique number r, then the largest eigenvalue q(G) of the matrix Q=A+D satisfies q(G)<= 2(1-1/r)n. If G is a complete regular r-partite graph, then equality holds in the above inequality. This result confirms a conjecture of Hansen and Lucas.
description: 10 pages, corrected a typo