cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Histoire : benling gaoqiang de si xiongdi
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
“You Can’t Combat Nothing”
Creators: name: Sandford, Shannon
Publisher: name: On_Culture
Year: 2021

description: Amidst the powerfully democratizing, public spheres of Web 2.0, life writing has taken on new geographies and forms of mobility through webcomics. As an experimental mode of self-representation, webcomics are part of an urgent, digital turn in autobiographical writing, where speaking to one’s personal experiences also takes place within the social economies of the Internet. This paper analyzes webcomics as a compelling new dimension of autobiographical illness narrative, using Allie Brosh’s webcomic blog, Hyperbole and a Half, as its case study. Launched in 2009 on the free blog platform, Blogspot, Brosh’s deceptively simplistic aesthetic and comically dark representation of mental illness has since amassed near-cult following online. Drawing on the discipline of life writing and from comics studies, I aim to position Brosh’s webcomics within the field of graphic medicine and to explore how they might expand conventional understandings of illness within this contextual frame. Brosh’s work is a significant precursor to hybrid forms of illness narrative still emerging from digital spaces — this paper asks how webcomics capitalize on both the affordances of the Internet and the aesthetic of comics to connect audiences across vast distances with collective experiences of everyday illness.
description: On_Culture, No 11 (2021): Illness, Narrated
Structural transitions of monoolein bicontinuous cubic phase induced by inclusion of protein lysozyme solutions
Creators: name: Tanaka, S.
name: Maki, S.
name: Ataka, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Inclusion of protein lysozyme molecules in lipidic monoolein cubic phase induces a transition from a $\rm Pn\bar{3}m$ structure to $\rm Im\bar{3}m$ one. Small-angle X-ray scattering (SAXS) method with high intensity synchrotron radiation enabled us to follow closely the transition depending on the conditions of lysozyme solutions. We showed that concentrated lysozyme solutions induced the appearance of the $\rm Im\bar{3}m$ structure coexisting with the $\rm Pn\bar{3}m$ structure. From the relation between the lattice parameters of these two structures it was shown that they were related by the Bonnet transformation of underlying triply periodic minimal surfaces. We found that the transition also occurred at lower lysozyme concentration when NaCl induced attraction between lysozyme molecules. The origin of the transition was considered as a frustration in the cubic phase where lysozyme molecules were highly confined. A simple estimation of the frustration was given, which took into account of the translational entropy of lysozyme molecules. At the highest concentration of lysozyme and NaCl the $\rm Im\bar{3}m$ structure was found to disappear and left only the $\rm Pn\bar{3}m$ structure. This was probably either due to the crystallization or phase separation of lysozyme solutions ongoing microscopically, which absorbed lysozyme molecules from channels of the cubic phase and thus removed the frustration.
description: 8 pages, 5 figures
A Classically Singular Representation of $ su_q(n) $
Creators: name: Aizawa, N.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A \rep of \sun, which diverges in the limit of \cl, is investigated. This is an infinite dimensional and a non-unitary \rep, defined for the real value of $ q, \ 0 < q < 1. $ Each \irrep is specified by $ n $ continuous variables and one discrete variable. This \rep gives a new solution of the Yang-Baxter equation, when the R-matrix is evaluated. It is shown that a continuous variables can be regarded as a spectral parameter.
description: 8 pages, phyzzx, RCNP - 052
Destabilizing turbulence in pipe flow
Creators: name: Kühnen, J.
name: Song, B.
name: Scarselli, D.
name: Budanur, N.
name: Willis, A.
name: Riedl, M.
name: Avila, M.
name: Hof, B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Chaotic Dynamics (nlin.CD)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Turbulence is the major cause of friction losses in transport processes and it is responsible for a drastic drag increase in flows over bounding surfaces. While much effort is invested into developing ways to control and reduce turbulence intensities, so far no methods exist to altogether eliminate turbulence if velocities are sufficiently large. We demonstrate for pipe flow that appropriate distortions to the velocity profile lead to a complete collapse of turbulence and subsequently friction losses are reduced by as much as 95%. Counterintuitively, the return to laminar motion is accomplished by initially increasing turbulence intensities or by transiently amplifying wall shear. The usual measures of turbulence levels, such as the Reynolds number (Re) or shear stresses, do not account for the subsequent relaminarization. Instead an amplification mechanism measuring the interaction between eddies and the mean shear is found to set a threshold below which turbulence is suppressed beyond recovery.
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00286
Creators: name: de la Côte-d'Or, Archives départementales
name: CBMA/CG21/F.PETOT/2017
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00286, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Definitive calibration of CI, CO and dust as gas mass tracers across cosmic time
Creators: name: Dunne, Loretta
Publisher: name: Zenodo
Year: 2019

description: Measuring molecular gas mass in galaxies relies on the use of tracers as cold H2 is invisible. Historically CO has been the workhorse tracer as it is the second most abundant molecule in the ISM. However, it is expensive to observe large samples (100,000), and at high redshift the ground state J=1-0 transition is either inaccessible or extremely challenging to detect. Two alternative tracers have recently received attention: thermal emission from cool dust traced via sub-mm radiation, and emission from atomic Carbon (CI). Both are claimed to be 'as or more reliable' than CO, both are easier to observe at high redshift and sub-mm dust emission has already been observed in very large samples of galaxies with Herschel. In this talk I present a cross-calibration of all three tracers - the first sample of normal galaxies with CO, CI and dust emission from ALMA, plus literature observations of ~300 sources which have two of the tracers. Combining them in a self-consistent manner we find that there is no requirement (or strong evidence for) a bimodal CO-H2 conversion as is commonly adopted in the literature for 'main-sequence' and 'ULIRG/SMG' type star formation. Our study shows that all types of galaxy (with high metallicity) across z=0-4 can be modelled with constant gas-to-dust, gas-to-CO and CI abundance (with intrinsic scatter but no clear trends). In order to accommodate the popular lower CO-H2 conversion in ULIRG/SMG, we have to postulate that they must also have a lower gas-to-dust ratio AND a much higher Carbon abundance. This violates Occam's razor which states that the simplest acceptable hypothesis is the most likely one to be true. Our 'best bet' values for the conversion factors are presented, which are very close to those found in the Milky Way ISM.
Additional file 2: of Low uptake of cervical cancer screening among HIV positive women in Gondar University referral hospital, Northwest Ethiopia: cross-sectional study design
Creators: name: Abebe Nega
name: Mulat Woldetsadik
name: Abebaw Gelagay
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Amharic version of the questionnaire. (DOCX 43 kb)
title: Histoire : shier ge tiaowu de gongzhu
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
The Madwoman in the Cellar
Creators: name: Wernitznig, Dagmar
Publisher: name: On_Culture
Year: 2021

description: By utilizing practical examples from the Abteilung für Psychatrie [psychiatric ward] at the Landeskrankenanstalt [province hospital] in Carinthia, Austria, in the wake of the two World Wars, this article seeks to explore the stories of hospitalized women and girls after armistices and peace treaties. Whereas the dialectics of conflict and resulting post-conflict traumas became increasingly accepted by medics for combatants during that time frame, this was not necessarily the case for comparable traumatic experiences of female civilians. Instead, for these patients, the Freudian definition of hysteria prevailed as a stereotypical ‘feminine’ symptom. Accordingly, post-war transitions from 1918 and 1945 onwards, with critical, sometimes even unstable, material and political infrastructures, consolidated a decidedly gender-related notion of trauma. This monopoly of trauma diagnoses, reserved for male patients, hence even resulted in misogyny towards institutionalized women, especially when they were refugees or displaced persons. As this study attempts to show, the mapping of mental illness or normality was heavily determined by sex, class, or ethnic background and in most instances served as an administrative tool for socio-political ends. The research for this contribution is based on archival work conducted for an ERC Advanced Grant, entitled “EIRENE — Post-War Transitions in Gendered Perspective: The Case of the North-Eastern Adriatic Region.”
description: On_Culture, No 11 (2021): Illness, Narrated
Mechanics of Interfacial Composite Materials
Creators: name: Subramaniam, Anand Bala
name: Abkarian, Manouk
name: Mahadevan, L.
name: Stone, Howard A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Recent experiments and simulations have demonstrated that particle-covered interfaces can exist in stable non-spherical shapes as a result of the steric jamming of the interfacially trapped particles, which confers the interface with solid-like properties. We provide an experimental and theoretical characterization of the mechanical properties of these armored objects, with attention given to the two-dimensional granular state of the interface. Small inhomogeneous stresses produce a plastic response while homogeneous stresses produce a weak elastic response. Shear-driven particle-scale rearrangements explain the basic threshold needed to obtain the near-perfect plastic deformation that is observed. Furthermore, the inhomogeneous stress state of the interface is exhibited experimentally by using surfactants to destabilize the particles on the surface. Since the interfacially trapped particles retain their individual characteristics, armored interfaces can be recognized as a kind of composite material with distinct chemical, structural and mechanical properties.
description: 7 pages, 6 Figures
title: 01_0752
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Caught in the act: disruption of a high-mass disk by anisotropic accretion
Creators: name: Sanchez-Monge, Alvaro
Publisher: name: Zenodo
Year: 2019

description: The star formation process is intimately related to the existence of disks, which mediate the accretion onto the star, and energetic outflows, which help to remove angular momentum from the system. Over the last years, this paradigm has been widely favoured for stars of all masses: from low-mass through B-type stars up to the most massive O-type stars. However, for O-type stars (L > 10^5 Lsun, M_star > 20 Msun) there is still less than a handful clear cut cases of detected disks. We have used ALMA to search for disk candidates around O-type protostars. Observations of six regions at a resolution of 0.2 arcsec provided us with evidence of three possible rotating disks. In this poster we present the results for G29.96-0.02, a well-known high-mass star-forming region for which rotating structures were claimed in the past. Our 0.2- arcsec resolution ALMA observations reveal a new and interesting scenario where the disk is not what it was thought to be, and an energetic and collimated outflow plays a dominant role. The observational findings are consistent with the existence of non-isotropic and non-steady accretion as seen in numerical simulations. This irregular accretion onto the massive disk has a profound impact by changing the disk plane orientation. This, in turn, modifies the orientation of the outflow which disrupts the outer parts of the disk. Under these circumstances, dense gas originally associated with the disk is pushed away by the outflow. This is observed in G29.96-0.02, where the spatial distribution and velocity field of complex organic molecules such as CH3CN or CH3CH2CN - typically found tracing the dense gas disk in massive stars - appear tracing the base of the outflow. Complementing this, we find evidence for a possible compact disk (600 au in size) perpendicular to the current outflow axis. All together, G29.96-0.02 seems to constitute a unique case of a (truncated) disk around an O-type protostar, caught in the act of being disrupted by anisotropic accretion.
MC^2: A deeper look at ZwCl 2341.1+0000 with Bayesian galaxy clustering and weak lensing analyses
Creators: name: Benson, Bryant
name: Wittman, David M.
name: Golovich, Nathan
name: Jee, M. James
name: van Weeren, Reinout J.
name: Dawson, William A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: ZwCl 2341.1+0000, a merging galaxy cluster with disturbed X-ray morphology and widely separated ($\sim$3 Mpc) double radio relics, was thought to be an extremely massive ($10-30 \times 10^{14} M_\odot$) and complex system with little known about its merger history. We present JVLA 2-4 GHz observations of the cluster, along with new spectroscopy from our Keck/DEIMOS survey, and apply Gaussian Mixture Modeling to the three-dimensional distribution of 227 confirmed cluster galaxies. After adopting the Bayesian Information Criterion to avoid overfitting, which we discover can bias total dynamical mass estimates high, we find that a three-substructure model with a total dynamical mass estimate of $9.39 \pm 0.81 \times 10^{14} M_\odot$ is favored. We also present deep Subaru imaging and perform the first weak lensing analysis on this system, obtaining a weak lensing mass estimate of $5.57 \pm 2.47 \times 10^{14} M_\odot$. This is a more robust estimate because it does not depend on the dynamical state of the system, which is disturbed due to the merger. Our results indicate that ZwCl 2341.1+0000 is a multiple merger system comprised of at least three substructures, with the main merger that produced the radio relics occurring near to the plane of the sky, and a younger merger in the North occurring closer to the line of sight. Dynamical modeling of the main merger reproduces observed quantities (relic positions and polarizations, subcluster separation and radial velocity difference), if the merger axis angle of $\sim$10$^{+34}_{-6}$ degrees and the collision speed at pericenter is $\sim$1900$^{+300}_{-200}$ km/s.
q-deformed superconformal algebra on quantum superspace
Creators: name: Kobayashi, Tatsuo
name: Uematsu, Tsuneo
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A quantum deformation of 4-dimensional superconformal algebra realized on quantum superspace is investigated. We study the differential calculus and the action of the quantum generators corresponding to $sl_q(1|4)$ which act on the quantum superspace. We derive deformed $su(1|2,2)$ algebras from the deformed $sl(1|4)$ algebra. Through a contraction procedure we obtain a deformed super-Poincar{é} algebra.
description: 11 pages, KUCP-56, LaTeX file
Electronic structures of UX$_3$ (X=Al, Ga, and In) studied by photoelectron spectroscopy
Creators: name: Fujimori, Shin-ichi
name: Kobata, Masaaki
name: Takeda, Yukiharu
name: Okane, Tetsuo
name: Saitoh, Yuji
name: Fujimori, Atsushi
name: Yamagami, Hiroshi
name: Haga, Yoshinori
name: Yamamoto, Etsuji
name: Ōnuki, Yoshichika
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The electronic structures of UX$_3$ (X=Al, Ga, and In) were studied by photoelectron spectroscopy to understand the relationship between their electronic structures and magnetic properties. The band structures and Fermi surfaces of UAl$_3$ and UGa$_3$ were revealed experimentally by angle-resolved photoelectron spectroscopy (ARPES), and they were compared with the result of band-structure calculations. The topologies of the Fermi surfaces and the band structures of UAl$_3$ and UGa$_3$ were explained reasonably well by the calculation, although bands near the Fermi level ($E_\mathrm{F}$) were renormalized owing to the finite electron correlation effect. The topologies of the Fermi surfaces of UAl$_3$ and UGa$_3$ are very similar to each other, except for some minor differences. Such minor differences in their Fermi surface or electron correlation effect might take an essential role in their different magnetic properties. No significant changes were observed between the ARPES spectra of UGa$_3$ in the paramagnetic and antiferromagnetic phases, suggesting that UGa$_3$ is an itinerant weak antiferromagnet. The effect of chemical pressure on the electronic structures of UX$_3$ compounds was also studied by utilizing the smaller lattice constants of UAl$_3$ and UGa$_3$ than that of UIn$_3$. The valence band spectrum of UIn$_3$ is accompanied by a satellite-like structure on the high-binding-energy side. The core-level spectrum of UIn$_3$ is also qualitatively different from those of UAl$_3$ and UGa$_3$. These findings suggest that the U~$5f$ states in UIn$_3$ are more localized than those in UAl$_3$ and UGa$_3$.
description: 12 pages, 8 figures
The early stages at substellar formation in Lupus 1 and 3 clouds
Creators: name: Santamaría-Miranda, Alejandro
Publisher: name: Zenodo
Year: 2019

description: The formation of brown dwarfs is still under debate. While the latest discoveries point towards a scaled-down version of the star formation process, other models, such as embryo ejection or stellar disk fragmentation, may not be discarded. Here we present our latest ALMA cycle 3 (band 6) continuum observations of Lupus 1 and 3 star formation regions based on previous ASTE/AzTEC observations and a set of previously known class II substellar objects from the literature. We classify these sources using the spectral energy distribution obtained from archival data. We report nine new sources that could be classified as either prestellar cores or deeply embedded protostar candidates, three new class I objects, and one new class II. Additionally we also detected six previously known class II systems, some of them in the boundary between brown dwars and very low mass stars. We probe the turbulent fragmentation and core collapse formation scenarios for the prestellar cores or deeply embedded protostar candidates and we compare the dust masses of the disk for the class II objects with previous studies. We also present ALMA cycle 5 band 7 data of Par-Lup3-4 where we witness for first time the presence of the base of a compact bipolar molecular cavity in radio and an optical jet in a very low mass star, close to the boundary to brown dwarfs, suggesting a scale down version of low mass star formation.
Continuants, run lengths, and Barry's modified Pascal triangle
Creators: name: Shallit, Jeffrey
name: Spiegelhofer, Lukas
Publisher: name: arXiv
Year: 2017
Subjects: subject: Combinatorics (math.CO)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: Primary: 05A10, Secondary: 05A19, 11A55, 11A63

description: We show that the $n$'th diagonal sum of Barry's modified Pascal triangle can be described as the continuant of the run lengths of the binary representation of $n$. We also obtain an explicit description for the row sums.
description: 5 pages
The Broad-Line and Narrow-Line Regions of the LINER NGC 4579
Creators: name: Barth, A. J.
name: Ho, L. C.
name: Filippenko, A. V.
name: Rix, H. -W.
name: Sargent, W. L. W.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of an extremely broad H-alpha emission line in the LINER nucleus of NGC 4579. From ground-based observations, the galaxy was previously known to contain a Type 1 nucleus with a broad H-alpha line of FWHM = 2300 km/s and FWZI ~ 5000 km/s. New spectra obtained with the Hubble Space Telescope and a 0.2 arcsec-wide slit reveal an H-alpha component with FWZI ~ 18,000 km/s. The line is not obviously double-peaked, but it does possess shoulders on the red and blue sides which resemble the H-alpha profiles of double-peaked emitters such as NGC 4203 and NGC 4450. This similarity suggests that the very broad H-alpha profile in NGC 4579 may represent emission from an accretion disk. Three such objects have been found recently in two HST programs which have targeted a total of 30 galaxies, demonstrating that double-peaked or extremely broad-line emission in LINERs must be much more common than would be inferred from ground-based surveys. The ratio of the narrow [S II] 6716, 6731 lines shows a pronounced gradient indicating a steep rise in density toward the nucleus. The direct detection of a density gradient within the inner arcsecond of the narrow-line region confirms expectations from previous observations of linewidth-critical density correlations in several LINERs.
description: 8 pages, includes 3 figures. To appear in The Astrophysical Journal
ALCHEMI: The ALMA Comprehensive High-resolution Extragalactic Molecular Inventory
Creators: name: Martín, Sergio
Publisher: name: Zenodo
Year: 2019

description: NGC 253 is the one of the brightest molecular emitters outside the Galaxy and therefore the more suited candidate for deep molecular surveys. In this presentatio i will summarize the current status of the ALCHEMI project which an ALMA large program consisting of an unbiased line survey from ALMA bands 3, 4, 6, and 7 (85-370 GHz), whose scope was extended this Cycle to also cover Band 5. In particular i will focus on the first results on the low resolution data from the 7m compact array which already shows an unprecedented molecular richness as well as first look into the chemistry revealed at the highest resolution. Despite of being observed at every wavelengths for decades, ALMA keeps unveiling new details on its central molecular zone. Additionally to ALCHEMI, I will present results from deep observations spin-off ALMA projects which were going in parallel to this survey which targetted isotopic ratio based on the double isotopologue 13C18O, deuteration, and vibrational emission in NGC 253.
Digital Nonlinearity Compensation in High-Capacity Optical Fibre Communication Systems: Performance and Optimisation
Creators: name: Xu, Tianhua
name: Shevchenko, Nikita A.
name: Karanov, Boris
name: Liga, Gabriele
name: Lavery, Domaniç
name: Killey, Robert I.
name: Bayvel, Polina
Publisher: name: arXiv
Year: 2017
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: C.2.5
subject: 94A12

description: Meeting the ever-growing information rate demands has become of utmost importance for optical communication systems. However, it has proven to be a challenging task due to the presence of Kerr effects, which have largely been regarded as a major bottleneck for enhancing the achievable information rates in modern optical communications. In this work, the optimisation and performance of digital nonlinearity compensation are discussed for maximising the achievable information rates in spectrally-efficient optical fibre communication systems. It is found that, for any given target information rate, there exists a trade-off between modulation format and compensated bandwidth to reduce the computational complexity requirement of digital nonlinearity compensation.
description: Invited paper
Additional file 6: of Results of a feasibility cluster randomised controlled trial of a peer-led school-based intervention to increase the physical activity of adolescent girls (PLAN-A)
Creators: name: Sebire, Simon
name: Jago, Russell
name: Banfield, Kathryn
name: Edwards, Mark
name: Campbell, Rona
name: Kipping, Ruth
name: Blair, Peter
name: Bryar Kadir
name: Garfield, Kirsty
name: Matthews, Joe
name: Lyons, Ronan
name: Hollingworth, William
Publisher: name: figshare
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Exploratory interaction of the intervention effect on weekday MVPA at Time 1 and Time 2 and peer supporter status. Exploratory interaction of the intervention effect on weekday MVPA at Time 1 and Time 2 and peer supporter status. (DOCX 13 kb)
ALMA Polarimetry reveals the properties of protoplanetary disks with rotating jets: clues on grains
Creators: name: Bacciotti, Francesca
Publisher: name: Zenodo
Year: 2019

description: We have obtained ALMA polarimetric data at 870 microns (Band 7) and 0."2 resolution for the protoplanetary disks around DG Tau and CW Tau, two T Tauri systems with well known rotating jets. In both targets the results are consistent with dust self-scattering being at the origin of the polarization pattern (Bacciotti et al., 2018, ApJ 865, L12). The polarization maps highlight structural details not derivable from the analysis of the total emission alone. Such substructures are likely related to changes in the optical depth, and can betray a change in the physical structure of the disk. The has been confirmed by subsequent ALMA observations by our group (Podio et al., 2019, A&A 623, L6). The measured values of the polarization fraction give constraints to the maximum size of the grains giving rise to observed patterns. This size is found to be in the range 50 - 150 microns in our targets. Meanwhile, the polarization maps combined with dust opacity estimates give constrai nts on the scale height of such grains. Overall, we find that these grains are larger and more settled toward the midplane in CW Tau than in DG Tau. These results confirm that polarization can be a fundamental complement to observations in total emission, for the investigation of the structure and of the evolution of protoplanetary disks. The promising prospects of such investigations with ALMA will be discussed.
Through the Eyes of Peter Pan
Creators: name: Tscheschel, Janin
Publisher: name: On_Culture
Year: 2021

description: This article discusses to what extent the documentary film, through its aesthetic strategies and narrative style, spotlights the topic of mental illness, contributing to society’s acceptance of this taboo topic. The 2016 documentary Life, Animated, which integrates animations into its presentation, gives insights into the concrete possibilities of negotiating the topic of mental disorders. A discourse-analytical examination embeds the film in a larger context and focuses on the crisis of the documentary film under the sign of hybrid forms combining fact and fiction. The article shows how these hybrid formats both question the documentary film’s claim to reality and offer the opportunity to find images conveying inner states, and highlights that an extension of the possibilities of representation, such as the integration of animation in documentaries, allows conditions that are completely unknown to the viewers to be immersively experienced, thereby contributing to their de-stigmatization.
description: On_Culture, No 11 (2021): Illness, Narrated
РАЗРАБОТКА АВТОМАТИЧЕСКОЙ  СИСТЕМЫ УПРАВЛЕНИЯ ТЕМПЕРАТУРЫ И ВЛАЖНОСТИ В ПОМЕЩЕНИЯХ.
Creators: name: Муродов, Ойбек
Publisher: name: Zenodo
Year: 2024

description: В статье рассматриваются автоматизированные системы управления температуры и влажности в производственных комнат. Вначале выдано общая информация про систем охлаждения их виды и свойства а также проанализировано типовое и различные построения систем управления температурой и влажностью производственных комнат, а далее рассматривается внедрение данных технологий в подобные системы.
Complex Scaling of the Faddeev Equations
Creators: name: Kolganova, E. A.
name: Motovilov, A. K.
name: Ho, Y. K.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: In this work we compare two different approaches to calculation of the three-body resonances on the basis of Faddeev differential equations. The first one is the complex scaling approach. The second method is based on an immediate calculation of resonances as zeros of the three-body scattering matrix continued to the physical sheet.
description: 6 pages, Talk presented at the International Conference "Modern Trends in Computational Physics" (July 2000, Dubna, Russia)
Material Shifts
Creators: name: McKenna, Emma
Publisher: name: On_Culture
Year: 2021

description: A body changed by illness demands new narrative modes. In this article, I use autotheory to foreground my experience of struggling with symptoms of endometriosis. I enter into conversation with feminist disability scholars who have theorized chronic illness and endometriosis as a disability, and think through some of the socio-economic effects of doing so, particularly within academia. I examine how an experimental arts-based practice can be a method of narrating chronic illness. Situated within a disability art aesthetic, I use textiles to represent a chronic pain episode. These images argue for the inherent worthiness of non-normative female embodiment.
description: On_Culture, No 11 (2021): Illness, Narrated
Synchronization is optimal in non-diagonalizable networks
Creators: name: Nishikawa, Takashi
name: Motter, Adilson E.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Chaotic Dynamics (nlin.CD)
subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: We consider the problem of maximizing the synchronizability of oscillator networks by assigning weights and directions to the links of a given interaction topology. We first extend the well-known master stability formalism to the case of non-diagonalizable networks. We then show that, unless some oscillator is connected to all the others, networks of maximum synchronizability are necessarily non-diagonalizable and can always be obtained by imposing unidirectional information flow with normalized input strengths. The extension makes the formalism applicable to all possible network structures, while the maximization results provide insights into hierarchical structures observed in complex networks in which synchronization plays a significant role.
description: 4 pages, 1 figure; minor revision
Blogging to Let Go
Creators: name: Joutseno, Astrid
Publisher: name: On_Culture
Year: 2021

description: Illness memoirs gained popularity in the last decades of the 20th century. From the early 21st century, illness narratives proliferate online. This article examines illness life writing and near-death narratives by mothers living with stage IV cancer. I read two blogs, Suspicious Country by Nina Riggs and Julie Yip-Williams: My Cancer Fighting Journey by Julie Yip-Williams, and their published memoirs. I draw from life writing studies, motherhood studies, queer death studies, and narrative medicine, analyzing the overlap of mothering and illness in the contexts of life writing and medicine. Working with Eve Sedgwick’s reparative practice, I suggest that while illness, dying, and mothering appear incompatible at first, narrating from this position holds the possibility of sustenance and the potential for redefining how stories of ill and dying mothers are told. The blogs and memoirs are counter-narratives to the healing imperatives and closure demanded by the normative cancer narrative. They flesh out an approach to living with illness and dying, while writing about it. The article illustrates how illness blogging constructs an entangled story of grief, loss, and joy which becomes an instrument in living with the acute awareness of dying.
description: On_Culture, No 11 (2021): Illness, Narrated
CARBON CAPTURE AND STORAGE
Creators: name: Maanav Shah* & Jyoti Sangle**
Publisher: name: Zenodo
Year: 2024

description: This review paper provides a comprehensive analysis of the latest developments in carbon capture and storage (CCS) technologies, with a particular focus on two prominent carbon capture methods: Direct Air Capture (DAC) and Post Combustion Capture (PCC). The paper explores the underlying principles, technological advancements, and current challenges associated with these methods. Furthermore, it delves into the various techniques employed for storing captured carbon, emphasizing the significance of carbon sequestration. The first section of the paper elucidates the principles behind DAC, highlighting its potential as a direct and scalable solution for reducing atmospheric carbon dioxide levels. The second part of the paper focuses on carbon storage techniques, emphasizing the critical role of carbon sequestration in mitigating climate change.
The Simplicial Characterisation of TS networks: Theory and applications
Creators: name: Gupte, Neelima
name: Thyagu, N. Nirmal
name: Chutani, Malayaja
Publisher: name: arXiv
Year: 2017
Subjects: subject: Methodology (stat.ME)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We use the visibility algorithm to construct the time series networks obtained from the time series of different dynamical regimes of the logistic map. We define the simplicial characterisers of networks which can analyse the simplicial structure at both the global and local levels. These characterisers are used to analyse the TS networks obtained in different dynamical regimes of the logisitic map. It is seen that the simplicial characterisers are able to distinguish between distinct dynamical regimes. We also apply the simplicial characterisers to time series networks constructed from fMRI data, where the preliminary results indicate that the characterisers are able to differentiate between distinct TS networks.
description: 11 pages, 2 figures, 4 tables. Accepted for publication in Proceedings of the 4th International Conference on Applications in Nonlinear Dynamics (ICAND 2016)
Dyonic Black Holes in String Theory
Creators: name: Cheng, Guang-Jiun
name: Hsu, Rue-Ron
name: Lin, Wei-Fu
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: An exact solution of the low-energy string theory representing static, spherical symmetric dyonic black hole is found. The solution is labeled by their mass, electric charge, magnetic charge and asymptotic value of the scalar dilaton. Some interesting properties of the dyonic black holes are studied. In particular, the Hawking temperature of dyonic black holes depends on both the electric and magnetic charges, and the extremal ones, which have nonzero electric and magnetic charges, have zero temperature but nonzero entropy. These properties are quite different from those of electrically (or magnetically) charged dilaton black holes found by Gibbons {\it et al.} and Garfinkle {\it et al.}, but are the same as those of the dyonic black holes found by Gibbons and Maeda. After this paper was submitted for publication, D. Wiltshire told us that solutions, eqs.(22)-(28), are related to Gibbons-Maeda dyonic black hole solutions by a coordinate transformation and some parameters reparametization \cite{26}. And, we were also informed that many of our results were previously obtained by Kallosh {\it et al.} \cite{27}. The dyonic black hole solutions, eqs.(22)-(28), are also related to those of reference \cite{27} by another coordinate
description: 20 pages, 2 figures not included, LATEX, revised version
Sounding diffuse molecular gas with ALMA as a mean to prove that the CO-dark gas is molecular
Creators: name: Gerin, Maryvonne
Publisher: name: Zenodo
Year: 2019

description: Studies of the dust continuum emission and extinction, and of the gamma ray emission show that a fraction of the interstellar gas is not traced by the combination of HI 21 cm and CO J=1-0 emission lines. The nature and physical conditions of this so called CO-dark gas are debated. We have used ALMA to search for molecular absorption towards distant quasars in the field of view of molecular clouds (Chamaelon, Taurus-Auriga, Galactic Bulge). We show that HCO+ absorption, tracing the presence of diffuse molecular hydrogen, is detected down to reddening values approaching the threshold for H2 formation (E(B-V) ~ 0.1 mag), and that the detected amount of molecular gas explains the presence of CO-dark gas. CO is detected toward a subset of sources with column densities at the same level as those derived from FUV spectra, that are too low to produce a detectable J=1-0 emission. The CO-dark gas is dynamically active with complex HCO+, HCN, CCH and CO line profiles. The CO line profiles are narrower that those from HCO+ , providing further support for a tight coupling of the gas dynamics and chemistry. This work also confirms that HCO+ is the most sensitive tracer of diffuse molecular gas at millimeter wavelengths, with a mean abundance relative to H2 of 3x10-9, firmly established by several comparisons with other, independent column density determinations.
Predicting Optimal Lengths of Random Knots
Creators: name: Dobay, Akos
name: Sottas, Pierre-Edouard
name: Dubochet, Jacques
name: Stasiak, Andrzej
Publisher: name: arXiv
Year: 2000
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: In thermally fluctuating long linear polymeric chain in solution, the ends come from time to time into a direct contact or a close vicinity of each other. At such an instance, the chain can be regarded as a closed one and thus will form a knot or rather a virtual knot. Several earlier studies of random knotting demonstrated that simpler knots show their highest occurrence for shorter random walks than more complex knots. However up to now there were no rules that could be used to predict the optimal length of a random walk, i.e. the length for which a given knot reaches its highest occurrence. Using numerical simulations, we show here that a power law accurately describes the relation between the optimal lengths of random walks leading to the formation of different knots and the previously characterized lengths of ideal knots of the corresponding type.
ASCA Observations of GX 354-0 and KS 1731-260
Creators: name: Narita, T.
name: Grindlay, J. E.
name: Barret, D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on ASCA observations of the low mass X-ray binaries GX 354-0 and KS 1731-260. The spectrum of GX 354-0 is best described as a power-law or a Comptonized spectrum with tau ~ 5 and kT ~ 8 keV and a residual at ~6.5 keV. The residual may be a disk reflection or a Compton broadened Gaussian line from the hot inner ADAF-like coronal region. The absorption column density to the source is 2.9e22 cm^-2. No soft thermal component was detected. The spectrum from KS 1731-260 is softer and it is best fit with a two component model with a column density of 1.1e22 cm^-2. The likely interpretation is emission from a Comptonizing cloud with an optical depth tau>12 and either a neutron star or a disk blackbody emission. We discuss the likely location of the Comptonizing cloud for both sources within the context of several proposed emission models.
description: Accepted for publication in the Astrophysical Journal
“Untenanted by any tangible form”
Creators: name: Däwes, Birgit
Publisher: name: On_Culture
Year: 2021

description: In the current Covid-19 crisis, masks have become a ubiquitous sight in social situations. As visual signifiers of both protection and containment, they emblematize the very risk which they serve to prevent. Departing from the multiple functions of the mask in Edgar Allan Poe’s “The Masque of the Red Death” — a story published decades before the emergence of modern virology — this paper reads recent fictionalizations of pandemics as diagnostic tools of larger social, political, and cultural shifts. Taking Poe’s story as a programmatic blueprint, my interest is particularly in the correlation between (narrative) representation and political power in contexts of illness. Given that minorities are often disproportionally affected by, and blamed for, epidemics, my analysis targets not only the discursive and semantic strategies of “outbreak narratives” (Priscilla Wald), but the complicity of these strategies in notions of cultural difference. Through the trope of the mask, I argue, the nexus of “the visible and invisible” that Foucault sees at the heart of modern medicine can be reconceptualized along narratological lines. In addition to more detailed analyses of Ling Ma’s Severance (2018) and Lawrence Wright’s The End of October (2020), my reading also relies on novels by other contemporary authors.
description: On_Culture, No 11 (2021): Illness, Narrated
Resolving the source of the massive protostellar accretion outburst in NGC6334I-MM1B
Creators: name: Hunter, Todd
Publisher: name: Zenodo
Year: 2019

description: Though evidence for episodic accretion is now commonplace toward low mass protostars, the recent extraordinary outburst in the massive protostellar cluster NGC6334I (Hunter et al. 2017) marks only the second large episodic accretion event observed toward a deeply embedded massive protostar and casts new light on the tumultuous lives of these young objects. The unexpectedly large factor of increase in millimeter continuum emission was accompanied by an unprecedented simultaneous flaring of 10 maser transitions detected by the long-term bi-weekly maser monitoring program at the Hartebeesthoek Radio Astronomy Observatory (HartRAO) (MacLeod et al. 2018). The dust emission and water and methanol masers have now remained in the outburst state for over four years. The combination of VLA and ALMA imaging (Brogan et al. 2018) pinpointed the origin of the outburst to a hypercompact HII region MM1B that is driving a compact well-collimated outflow traced by water masers, their proper motions, and a number of thermal molecular tracers of warm dense gas. The pre-outburst strength of the HCHII region and its bolometric luminosity are consistent with a deeply-embedded central protostar of early B- type, but it has dimmed dramatically in its free-free emission at centimeter wavelengths despite the large increase in luminosity. This combination of observations suggest a reduction in uv photons due to the rapid accretion of sufficient mass to cause the protostellar photosphere to expand and radiate at a much larger luminosity, but with a lower effective temperature. To explore this exciting possibility, we will present new ALMA images with the finest-ever resolution toward this object (<50 au) acquired during Cycle 6, along with the results from two new epochs of VLA monitoring of the continuum and maser emission.