cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
"susy.371467.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.
Accurate finite-difference micromagnetics of magnets including RKKY interaction -- analytical solution and comparison to standard micromagnetic codes
Creators: name: Suess, Dieter
name: Koraltan, Sabri
name: Slanovc, Florian
name: Bruckner, Florian
name: Abert, Claas
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Within this paper we show the importance of accurate implementations of the RKKY interactions for antiferromagnetically coupled ferromagnetic layers with thicknesses exceeding the exchange length. In order to evaluate the performance of different implementations of RKKY interaction, we develop a benchmark problem by deriving the analytical formula for the saturation field of two infinitely thick magnetic layers that are antiparallelly coupled. This benchmark problem shows that state-of-the-art implementations in commonly used finite-difference codes lead to errors of the saturation field that amount to more than 20% for mesh sizes of 2 nm which is well below the exchange length of the material. In order to improve the accuracy, we develop higher order cell based and nodal based finite-difference codes that significantly reduce the error compared to state-of-the-art implementations. For the second order cell based and first order nodal based finite element approach the error of the saturation field is reduced by about a factor of 10 (2% error) for the same mesh size of 2 nm.
"susy.371469.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.
'Mambear coca no es pintarse de verde la boca': Notas sobre el uso ritual de la coca amazónica
Creators: name: Echeverri, Juan Alvaro
name: Pereira, Edmundo
Publisher: name: Zenodo
Year: 2010
Subjects: coca
Murui
Witoto

description: Los datos históricos y etnológicos que presentamos en nuestro artículo en portugués (Echeverri y Pereira, 2005) nos sugieren que el manejo de la coca se expandió desde los Andes hasta las tierras bajas orientales, posiblemente en tiempos poscolombinos, primero hasta la región del alto Amazonas y más recientemente (es probable que sucediera no antes del siglo XIX) hasta el norte del río Putumayo. La expansión amazónica de la coca implicó el surgimiento de una nueva variedad de E. coca, la variedad ipadu, e importantes modificaciones tecnológicas en su procesamiento. A pesar de ser una adquisición relativamente reciente, la coca se incorporó en la mitología de los grupos que la emplean5. Este es el tema que exploramos en la primera sección de este artículo (a coca en los mitos: esposa o hermano), donde discutimos algunos relatos míticos de los uitoto y muinane (del interfluvio Caquetá-Putumayo) y de los yucuna y barasana (del norte del Caquetá). La comparación de estos relatos nos revela modos diferentes de representar la coca, que pueden tal vez señalar una frontera entre dos complejos culturales, al norte y al sur del Caquetá. Al sur, la coca es representada como una mujer que debe ser seducida; al norte, la coca es el cuerpo de un hombre consanguíneo (hermano, tío). Los relatos del norte del Caquetá enfatizan la adquisición de la planta y su expresión visible en los campos del cultivo o chagras; al contrario, al sur de este río, el énfasis recae en la adquisición del proceso técnico de su preparación. En la segunda sección (Hacer coca), abordamos el procesamiento de la coca en polvo en el marco de su teoría corporal y moral. Este sistema de conocimiento se revela sobre todo en los “consejos” o preceptos relativos al manejo de la planta y en los pasos de su transformación (cosechar, tostar, pilar, obtener cenizas y cernir). El producto de este proceso, la coca en polvo, es lo que se mambea, es decir, lo que se consume y se comparte. En la tercera sección (Mambear coca) introducimos el uso social de la coca en el ámbito del espacio ritual llamado mambeadero. En el mambeadero un hombre se sienta y habla por lo menos de tres asuntos: 1. defenderse y cazar; 2. enfriar y curar; y 3. ofrecer y dialogar. La discusión de estos asuntos nos revela que el mambeo de coca amazónico constituye una verdadera “cultura”, punto principal sobre el cual queremos tratar en este artículo.
Optical/Near-IR Polarization Survey of Sh 2-29: Magnetic Fields, Dense Cloud Fragmentations and Anomalous Dust Grain Sizes
Creators: name: Santos, Fábio P.
name: Franco, Gabriel A. P.
name: Roman-Lopes, Alexandre
name: Reis, Wilson
name: Román-Zúñiga, Carlos G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Sh 2-29 is a conspicuous star-forming region marked by the presence of massive embedded stars as well as several notable interstellar structures. In this research, our goals were to determine the role of magnetic fields and to study the size distribution of interstellar dust particles within this turbulent environment. We have used a set of optical and near-infrared polarimetric data obtained at OPD/LNA (Brazil) and CTIO (Chile), correlated with extinction maps, 2MASS data and images from DSS and Spitzer. The region's most striking feature is a swept out interstellar cavity whose polarimetric maps indicate that magnetic field lines were dragged outwards, pilling up along its borders. This led to a higher magnetic strength value ($\approx400\,μ$G) and an abrupt increase in polarization degree, probably due to an enhancement in alignment efficiency. Furthermore, dense cloud fragmentations with peak $A_{V}$ between 20 and 37 mag were probably triggered by its expansion. The presence of $24\,μ$m point-like sources indicates possible newborn stars inside this dense environment. A statistical analysis of the angular dispersion function revealed areas where field lines are aligned in a well-ordered pattern, seemingly due to compression effects from the HII region expansion. Finally, Serkowski function fits were used to study the ratio of the total-to-selective extinction, reveling a dual population of anomalous grain particles sizes. This trend suggests that both effects of coagulation and fragmentation of interstellar grains are present in the region.
description: 20 pages, 12 figures, 2 tables; Accepted for The Astrophysical Journal
"susy.371472.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.
Lactobacillus rodentium
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 rodentium

description: Lactobacillusrodentium
Lactobacillusrodentium (ro.den‘ti.um. L. gen. pl. n. rodentium of gnawers, referring to the fact that the micro-organism was isolated from wild rodents).
Lactobacillusrodentium utilizes glucose, fructose, maltose, melibiose and sucrose, but not ribose, mannitol or trehalose [108]. Thegenome size is 1.52 Mbp and the mol% G+C content of DNA is 34.0.
Isolated from the colon of wild mice (Mus musculus) and other rodent species [55, 108].
Thetypestrainis MYMRS/TLU1 T = DSM 24759 T =CCM 7945 T.
Genome sequence accession number: BFBY00000000.
16S rRNA gene accession number: HQ851022.
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 2800, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
Eolagurus przewalskii
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Eolagurus
Eolagurus przewalskii

description: Eolagurus przewalskii (Büchner, 1889). Wiss. Res. Przewalski Cent.-Asien, Reisen, Zool., I:(Säugeth.), p. 127. TYPE LOCALITY: China, Qinghai (Tsinghai), Tsaidam region, shore of Iche-zaidemin Nor. DISTRIBUTION: From S Xinjiang and N Xizang in W China, east through Quinghai and N Gansu to S Mongolia and Nei Mongol; limits unknown. COMMENTS: This very distinctive species was incorrectly united with E. luteus by Corbet (1978c) but treated as separate by Allen (1940), Corbet and Hill (1991), and Gromov and Polyakov (1977).
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 513, 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.", "Corbet, G. B., and J. E. Hill. 1991. A world list of mammalian species. Third ed. British Museum (Natural History) Publications, London, 243 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)."]}
"susy.371468.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.
Cool Tobacco Breath: the uses and meanings of tobacco among the People of the Centre
Creators: name: Echeverri, Juan Alvaro
Publisher: name: Zenodo
Year: 2015
Subjects: tabaco
Murui
Witoto

description: This paper discusses the uses and meaning of tobacco for the People of the Centre, relying mostly on insights from two elders: Kɨneraɨ (Hipólito Candre), an Ocaina- Witoto man who lived in the Igaraparaná River, introduced above, and Enokakuiodo (Oscar Román-Jitdutjaaño), who lives in the Middle Caquetá region, whom I will introduce in the next section.
Higher order extensions of the Gaussian effective potential
Creators: name: Siringo, Fabio
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: A variational method is discussed, extending the Gaussian effective potential to higher orders. The single variational parameter is replaced by trial unknown two-point functions, with infinite variational parameters to be optimized by the solution of a set of integral equations. These stationary conditions are derived by the self-energy without having to write the effective potential, making use of a general relation between self-energy and functional derivatives of the potential. This connection is proven to any order and verified up to second order by an explicit calculation for the scalar theory. Among several variational strategies, the methods of minimal sensitivity and of minimal variance are discussed in some detail. For the scalar theory, at variance with other post-Gaussian approaches, the pole of the second-order propagator is shown to satisfy the simple first-order gap equation that seems to be more robust than expected. By the method of minimal variance, nontrivial results are found for gauge theories containing fermions, where the first-order Gaussian approximation is known to be useless.
description: Last version: minor changes in the text, and reference update
The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets
Creators: name: Liu, Michael C.
name: Magnier, Eugene A.
name: Deacon, Niall R.
name: Allers, Katelyn N.
name: Dupuy, Trent J.
name: Kotson, Michael C.
name: Aller, Kimberly M.
name: Burgett, W. S.
name: Chambers, K. C.
name: Draper, P. W.
name: Hodapp, K. W.
name: Jedicke, R.
name: Kudritzki, R. -P.
name: Metcalfe, N.
name: Morgan, J. S.
name: Kaiser, N.
name: Price, P. A.
name: Tonry, J. L.
name: Wainscoat, R. J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have used Pan-STARRS1 to discover an extremely red late-L dwarf, which has (J-K)_MKO = 2.84 and (J-K)_2MASS = 2.78, making it the reddest known field dwarf and second only to 2MASS J1207-39b among substellar companions. Near-IR spectroscopy shows a spectral type of L7 and reveals a triangular H-band continuum and weak alkali (K I and Na I) lines, hallmarks of low surface gravity. Near-IR astrometry from the Hawaii Infrared Parallax Program gives a distance of 24.6+/-1.4 pc and indicates a much fainter J-band absolute magnitude than field L dwarfs. The position and kinematics of PSO J318-22 point to membership in the beta Pictoris moving group. Evolutionary models give a temperature of 1160 (-40,+30) K and a mass of 6.5 (-1.0, +1.3) Mjup, making PSO J318-22 one of the lowest mass free-floating objects in the solar neighborhood. This object adds to the growing list of low-gravity field L dwarfs and is the first to be strongly deficient in methane relative to its estimated temperature. Comparing their spectra suggests that young L dwarfs with similar ages and temperatures can have different spectral signatures of youth. For the two objects with well constrained ages (PSO J318-22 and 2MASS J0355+11), we find their temperatures are ~400 K cooler than field objects of similar spectral type but their luminosities are comparable, i.e., these young L dwarfs are very red and unusually cool but not "underluminous." Altogether, PSO J318-22 is the first free-floating object with the colors, magnitudes, spectrum, luminosity, and mass that overlap the young dusty planets around HR 8799 and 2MASS J1207-39.
description: ApJ Letters, in press. Version 2 incorporates tiny cosmetic changes to match final published version, including a revised Figure 1 that uses the most recent AB Pic b photometry from Biller et al (2013)
Silicon Pore Optics
Creators: name: Barrière, Nicolas M.
name: Bavdaz, Marcos
name: Collon, Maximilien J.
name: Ferreira, Ivo
name: Girou, David
name: Landgraf, Boris
name: Vacanti, Giuseppe
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Silicon Pore Optics (SPO) uses commercially available monocrystalline double-sided super-polished silicon wafers as a basis to produce mirrors that form lightweight high-resolution X-ray optics. The technology has been invented by cosine Measurement Systems and the European Space Agency (ESA) and developed together with scientific and industrial partners to mass production levels. It leverages techniques and processes developed over decades by the semiconductor industry to handle, process, and clean silicon wafers and plates. SPO is an enabling technology for large space-borne X-ray telescopes such as Athena and ARCUS, operating in the 0.2 to 12 keV band, with angular resolution aiming for 5 arc seconds. SPO has also shown to be a versatile technology that can be further developed for gamma-ray optics, medical applications and for material research.
description: 37 pages, 41 figures, invited contribution to Section 2 of the Handbook for X-ray and Gamma-ray Astrophysics, "Optics for X-ray Astrophysics", section editors: Jessica Gaskin, Daniele Spiga, and Rene Hudec
"susy.371470.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.
Updated dissemination and exploitation plan M36
Creators: name: Ugarelli, Rita
name: Rambæk, Ida
Publisher: name: Zenodo
Year: 2024
Subjects: Water smart solutions
Circular economy
Knowledge sharing
Marketplace
Water recycling and reuse
Environment, resources and sustainability
Sustainability transition
Symbiosis between industry and water utilities

description: The dissemination and exploitation plan summarizes the consortium’s strategy and the concrete actions that should be made to disseminate and exploit the results generated by the project. This report defines and reports the dissemination and exploitation activities that have been and will be carried out during and after the project’s life span. It contains the WIDER UPTAKE dissemination strategy, which is adopted to reach different types of audiences (stakeholders, general public, etc.), followed by a complete overview of the activity plan and the activities fulfilled. The wide range of dissemination activities has targeted and will target (until the end of the project) several types of communities, including water utilities, policy makers, researchers, and technology providers. The general public is also approached through the website, social media, Community of Practice and press coverage of the WIDER UPTAKE achievements and research results. The innovations of the project have been disseminated through several events, and efforts towards this goal are being made on a regular basis. The dissemination and use of the new developments will continue after the project’s lifecycle, through the exploitation of research results and by pursuing possibilities of marketing via the established Water Europe Market Place. The Dissemination and Exploitation Plan (DEP) was not a fixed document but evolved during the project’s lifespan. This is the last version of the DEP, which finally evolved into its final form, i.e., this Deliverable 6.5 (due on M36). Nevertheless, the dissemination activities will continue until the end of the project and beyond.
Star Forming Regions
Creators: name: Sciortino, Salvatore
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Since the '80s the \textit{Einstein} observatory has shown the Young Stellar Objects (YSOs), emit X-rays with luminosities, in the 0.3--8 keV bandpass, up to $\rm 10^3$--$\rm 10^4$ times than the Sun and that the X-ray emission is highly variable. ROSAT has confirmed the pervasiveness of X-ray emission from YSOs and ASCA has provided evidence that the emission of Class I YSOs is largely originating from optical thin-plasma at temperature of 1-50 $\times 10^6$ K. These intrinsic, unexpected, properties and the transformational capabilities of the \textit{Chandra} and \textit{XMM-Newton} observatories has made X-rays a powerful tool to trace the star formation process up to distance of a few kpc around the Sun. Starting from the early evidences of the '80s and the intriguing questions they raised, I will summarize the results obtained and how they have influenced our current understanding of physical processes at work and I will discuss some of the still open issues and some of the likely avenues that next generation X-ray observatory will open.
description: Invited chapter for the "Handbook of X-ray and Gamma-ray Astrophysics" (Eds. C. Bambi and A. Santangelo, Springer Nature, 2022), accepted (42 pages, 7 figures)
"susy.371471.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.371473.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.
Comparison between FactSage and Thermo-calc simulations from Influence of impurities on the use of Fe-based powder as sustainable fuel
Creators: name: Choisez, Laurine
name: Van Ende, Marie-Aline
name: Bruyr, Zakarie
name: Contino, Francesco
name: Jacques, Pascal J.
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 460207
subject: Modelling and simulation

description: 240314_Supplementary1_ComparisonTC_FS.docx
Eothenomys Miller 1896
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Eothenomys

description: Eothenomys Miller, 1896. N. Am. Fauna, 12:45. TYPE SPECIES: Arvicola melanogaster Milne-Edwards, 1871. SYNONYMS: Anteliomys, Aschizomys, Caryomys. COMMENTS: Revised by Corbet (1978c), who also included Phaulomys (a genus we separate from Eothenomys) and Aschizomys (which we include in Alticola). Eothenomys is closely related to Hyperacrius, Alticola, and Clethrionomys, all of which are usually placed in the Clethrionomyini (Gromov and Polyakov, 1977; Hooper and Hart, 1962; Koenigswald, 1980).
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 513, 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.", "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).", "Hooper, E. T., and B. S. Hart. 1962. A synopsis of Recent North American microtine rodents. Miscellaneous Publications, Museum of Zoology, University of Michigan, 120: 1 - 68.", "Koenigswald, W. von. 1980. Schmelzstruktur und Morphologie in den Molaren der Arvicolidae (Rodentia). Abhandlungen der Senckenbergischen Naturforschenden Gesellschaft, 539: 1 - 129."]}
"susy.371474.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.
A thermodynamic formalism for continuous time Markov chains with values on the Bernoulli Space: entropy, pressure and large deviations
Creators: name: Lopes, Artur O.
name: Neumann, Adriana
name: Thieullen, Philippe
Publisher: name: arXiv
Year: 2013
Subjects: subject: Dynamical Systems (math.DS)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: Through this paper we analyze the ergodic properties of continuous time Markov chains with values on the one-dimensional spin lattice 1,...,d}^N (also known as the Bernoulli space). Initially, we consider as the infinitesimal generator the operator $L={\mc L}_A -I$, where \mc L_A is a discrete time Ruelle operator (transfer operator), and A:{1,...,d}^N \to R is a given fixed Lipschitz function. The associated continuous time stationary Markov chain will define the\emph{a priori}probability. Given a Lipschitz interaction V:\{1,...,d\}^{\bb N}\to \mathbb{R}, we are interested in Gibbs (equilibrium) state for such $V$. This will be another continuous time stationary Markov chain. In order to analyze this problem we will use a continuous time Ruelle operator (transfer operator) naturally associated to V. Among other things we will show that a continuous time Perron-Frobenius Theorem is true in the case V is a Lipschitz function. We also introduce an entropy, which is negative, and we consider a variational principle of pressure. Finally, we analyze large deviations properties for the empirical measure in the continuous time setting using results by Y. Kifer.
description: to appear Journ. of Stat. Physics
Lactobacillus taiwanensis
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 taiwanensis

description: Lactobacillus taiwanensis
Lactobacillus taiwanensis (tai.wa.nen’sis. N.L. masc. adj. taiwanensis of Taiwan, referring to the origin of the type strain).
L. taiwanensis produces both D- and L-lactic acid enantiomers from glucose fermentation. Fructose, mannose, maltose, lactose, sucrose and trehalose are also fermented. No acid is produced from raffinose or ribose [109]. The genome size is 1.88 Mbp and the mol% G+C content of DNA is 34.0.
Occurs in the mouse gastrointestinal tract [55] but also isolated from silage cattle feed.
Thetypestrainis FIRDI 006 T =BCRC 17755 T =DSM 21401 T.
Genome sequence accession number: AYZG00000000.
16S rRNA gene accession number: EU487512.
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 2800, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
What do non-relativistic CFTs tell us about Lifshitz spacetimes?
Creators: name: Keeler, Cynthia
name: Knodel, Gino
name: Liu, James T.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the reconstructability of (d+2)-dimensional bulk spacetime from (d+1)-dimensional boundary data, particularly concentrating on backgrounds which break (d+1)-dimensional Lorentz invariance. For a large class of such spacetimes, there exist null geodesics which do not reach the boundary. Therefore classically we expect some information is trapped in the bulk and thus invisible at the boundary. We show that this classical intuition correctly predicts the quantum situation: whenever there are null geodesics which do not reach the boundary, there are also "trapped scalar modes" whose boundary imprint is exponentially suppressed. We use these modes to show that no smearing function exists for pure Lifshitz spacetime, nor for any flow which includes a Lifshitz region. Indeed, for any (planar) spacetime which breaks (d+1)-dimensional Lorentz invariance at any radius, we show that local boundary data cannot reconstruct complete local bulk data.
description: references added
Eothenomys chinensis
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Eothenomys
Eothenomys chinensis

description: Eothenomys chinensis (Thomas, 1891). Ann. Mag. Nat. Hist., ser. 6, 8:117. TYPE LOCALITY: China, W Sichuan, Kiatingfu. DISTRIBUTION: Recorded only from Sichuan and Yunnan between 2000-4000 m (Corbet, 1978c). SYNONYMS: tarquinus, wardi. COMMENTS: The type-species of Anteliomys (see Hinton, 1926).
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 513, 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."]}
Detailed evolution of the temperature, phase and gas emissions from Influence of impurities on the use of Fe-based powder as sustainable fuel
Creators: name: Choisez, Laurine
name: Van Ende, Marie-Aline
name: Bruyr, Zakarie
name: Contino, Francesco
name: Jacques, Pascal J.
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 460207
subject: Modelling and simulation

description: 240314_Supplementary2_DetailedSimulations.docx
GerardM_tables_figures_ESM from Experimental elevated temperature affects bumblebee foraging and flight speed
Creators: name: Gérard, Maxence
name: Gardelin, Erika
name: Lehmann, Philipp
name: Roberts, Kevin  T
name: Sepulveda, Guadalupe
name: Sisquella, Clara
name: Baird, Emily
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310901
subject: Animal behaviour

description: Figures S1-S3; Tables S1-S6
Disentangling representations in Restricted Boltzmann Machines without adversaries
Creators: name: Fernandez-de-Cossio-Diaz, Jorge
name: Cocco, Simona
name: Monasson, Remi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: A goal of unsupervised machine learning is to build representations of complex high-dimensional data, with simple relations to their properties. Such disentangled representations make easier to interpret the significant latent factors of variation in the data, as well as to generate new data with desirable features. Methods for disentangling representations often rely on an adversarial scheme, in which representations are tuned to avoid discriminators from being able to reconstruct information about the data properties (labels). Unfortunately adversarial training is generally difficult to implement in practice. Here we propose a simple, effective way of disentangling representations without any need to train adversarial discriminators, and apply our approach to Restricted Boltzmann Machines (RBM), one of the simplest representation-based generative models. Our approach relies on the introduction of adequate constraints on the weights during training, which allows us to concentrate information about labels on a small subset of latent variables. The effectiveness of the approach is illustrated with four examples: the CelebA dataset of facial images, the two-dimensional Ising model, the MNIST dataset of handwritten digits, and the taxonomy of protein families. In addition, we show how our framework allows for analytically computing the cost, in terms of log-likelihood of the data, associated to the disentanglement of their representations.
description: Minor corrections. Accepted for publication in Physical Review X
Transition fronts for inhomogeneous monostable reaction-diffusion equations via linearization at zero
Creators: name: Tao, Tianyu
name: Zhu, Beite
name: Zlatos, Andrej
Publisher: name: arXiv
Year: 2013
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We prove existence of transition fronts for a large class of reaction-diffusion equations in one dimension, with inhomogeneous monostable reactions. We construct these as perturbations of corresponding front-like solutions to the linearization of the PDE at $u=0$. While a close relationship of the solutions to the two PDEs has been well known and exploited for KPP reactions (and our method is an extension of such ideas from [15]), to the best of our knowledge this is the first time such an approach has been used in the construction and study of fronts for non-KPP monostable reactions.
Eothenomys custos
Creators: name: Musser, Guy G.
name: Carleton, Michael D.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Muridae
Eothenomys
Eothenomys custos

description: Eothenomys custos (Thomas, 1912). Ann. Mag. Nat. Hist., ser. 8, 9:517. TYPE LOCALITY: China, Yunnan, Atuntsi, 11,500 -12,500 ft. DISTRIBUTION: Recorded only from mtns of Sichuan and Yunnan, where it occurs up to 4200 m (Corbet, 1978c). SYNONYMS: hintoni, rubelius, rubellus. COMMENTS: Listed as a species of Anteliomys by Hinton (1926).
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 pages 513-514, 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."]}
"susy.371475.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.
Lactobacillus ultunensis
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 ultunensis

description: Lactobacillus ultunensis
Lactobacillus ultunensis (ul.tun.en’sis. N.L. masc. adj. ultunensis pertaining to Ultuna, the site of Swedish University of Agricultural Sciences in Uppsala, Sweden).
Lactobacillus ultunensis produces both D- and L-lactate from glucose. Acid isproduced from galactose, fructose, mannose, cellobiose, maltose, lactose, sucrose, and trehalose. Acid isnot produced from arabinose, ribose, rhamnose and melezitose. Growth occurs at 42 but not at 45 °C [98]. The genome size of the type strain is 2.16 Mbp and the mol% G+C content of DNAis 36.0.
Isolated from a biopsy of a healthy human gastric mucosa.
Thetypestrainis Kx146C1 T = CCUG 48460 T =DSM 16047 T =JCM 16177 T =LMG 22117 T.
Genome sequence accession number: AZFO00000000.
16S rRNA gene accession number: AY253660.
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 2800, DOI: 10.1099/ijsem.0.004107, http://zenodo.org/record/4730536
X-ray polarimetry-timing
Creators: name: Ingram, Adam
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: X-ray polarimetry-timing is the characterization of rapid variability in the X-ray polarization degree and angle. As for the case of spectral-timing, it provides causal information valuable for reconstructing indirect maps of the vicinity of compact objects. To call X-ray polarimetry-timing a young field is somewhat of an understatement, given that the first X-ray mission truly capable of enabling polarimetry-timing analyses has only just launched at the time of writing. Now is therefore an exciting time for the field, in which we have theoretical predictions and are eagerly awaiting data. This Chapter discusses the theoretical expectations and also describes the data analysis techniques that can be used.
description: Invited chapter for the "Handbook of X-ray and Gamma-ray Astrophysics" (Eds. C. Bambi and A. Santangelo, Springer Singapore, 2022). 42 pages, 17 figures
Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
Creators: name: Ragone-Figueroa, Cinthia
name: Granato, Gian Luigi
name: Murante, Giuseppe
name: Borgani, Stefano
name: Cui, Weiguang
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We analyze the basic properties of Brightest Cluster Galaxies (BCGs) produced by state of the art cosmological zoom-in hydrodynamical simulations. These simulations have been run with different sub-grid physics included. Here we focus on the results obtained with and without the inclusion of the prescriptions for supermassive black hole (SMBH) growth and of the ensuing Active Galactic Nuclei (AGN) feedback. The latter process goes in the right direction of decreasing significantly the overall formation of stars. However, BCGs end up still containing too much stellar mass, a problem that increases with halo mass, and having an unsatisfactory structure. This is in the sense that their effective radii are too large, and that their density profiles feature a flattening on scales much larger than observed. We also find that our model of thermal AGN feedback has very little effect on the stellar velocity dispersions, which turn out to be very large. Taken together, these problems, which to some extent can be recognized also in other numerical studies typically dealing with smaller halo masses, indicate that on one hand present day sub-resolution models of AGN feedback are not effective enough in diminishing the global formation of stars in the most massive galaxies, but on the other hand they are relatively too effective in their centers. It is likely that a form of feedback generating large scale gas outflows from BCGs precursors, and a more widespread effect over the galaxy volume, can alleviate these difficulties.
description: 17 pages, 14 figures, accepted for publication on MNRAS, comments welcome
X-ray Halos around Massive Galaxies: Data and Theory
Creators: name: Bogdan, Akos
name: Vogelsberger, Mark
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: The presence of gaseous X-ray halos around massive galaxies is a basic prediction of all past and modern structure formation simulations. The importance of these X-ray halos is further emphasized by the fact that they retain signatures of the physical processes that shape the evolution of galaxies from the highest redshift to the present day. In this review, we overview our current observational and theoretical understanding of hot gaseous X-ray halos around nearby massive galaxies and we also describe the prospects of observing X-ray halos with future instruments.
description: Accepted chapter of the Section on Galaxies for the Handbook of X-ray and Gamma-ray Astrophysics (Springer, eds. Banbi & Santangelo)