cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Defects in Jackiw-Teitelboim Quantum Gravity
Creators: name: Mertens, Thomas G.
name: Turiaci, Gustavo J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We classify and study defects in 2d Jackiw-Teitelboim gravity. We show these are holographically described by a deformation of the Schwarzian theory where the reparametrization mode is integrated over different coadjoint orbits of the Virasoro group. We show that the quantization of each coadjoint orbit is connected to 2d Liouville CFT between branes with insertions of Verlinde loop operators. We also propose an interpretation for the exceptional orbits. We use this perspective to solve these deformations of the Schwarzian theory, computing their partition function and correlators. In the process, we define two geometric observables: the horizon area operator $Φ_h$ and the geodesic length operator $L(γ)$. We show this procedure is structurally related to the deformation of the particle-on-a-group quantum mechanics by the addition of a chemical potential. As an example, we solve the low-energy theory of complex SYK with a U(1) symmetry and generalize to the non-abelian case.
description: 66 pages, v4: clarifications added, typos corrected, matches published version
Resonance--Assisted Tunneling in Deformed Optical Microdisks with a Mixed Phase Space
Creators: name: Fritzsch, Felix
name: Ketzmerick, Roland
name: Bäcker, Arnd
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: The life times of optical modes in whispering-gallery cavities crucially depend on the underlying classical ray dynamics and may be spoiled by the presence of classical nonlinear resonances due to resonance--assisted tunneling. Here we present an intuitive semiclassical picture which allows for an accurate prediction of decay rates of optical modes in systems with a mixed phase space. We also extend the perturbative description from near-integrable systems to systems with a mixed phase space and find equally good agreement. Both approaches are based on the approximation of the actual ray dynamics by an integrable Hamiltonian, which enables us to perform a semiclassical quantization of the system and to introduce a ray-based description of the decay of optical modes. The coupling between them is determined either perturbatively or semiclassically in terms of complex paths.
description: 15 pages, 7 figures
Coelogyne brevilabris M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne brevilabris

description: Coelogyne brevilabris (Ridl.) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum brevilabre Ridl., J. Malayan Branch Roy. Asiat. Soc. 1: 96 (1923).
 Coelogyne brevilamellata J.J.Sm., Bull. Jard. Bot. Buitenzorg, sér. 3, 11: 102 (1931).
 Homotypic synonym: Chelonistele brevilamellata (J.J.Sm.) Carr, Gard. Bull. Straits Settlem. 8: 217 (1935).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 104, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
title: Investigating the influence of situational factors on participative enterprise modelling
title: making a case for a qualitative research approach
titleType: Subtitle
Creators: name: Persson, Anne
Publisher: name: Freie Universität Berlin
Year: 2000
Subjects: subject: 000 Informatik, Informationswissenschaft, allgemeine Werke::000 Informatik, Wissen, Systeme::003 Systeme

description: Participative Enterprise Modelling (PEM) has been used in Information Systems Development and Business Development for some time now. Research has shown that the full and positive effects of PEM methods heavily depends on the ability of its users to manage situational factors, which characterise, influence and constrain development situations where it is used. Therefore, a shift must be made in method development, from the invention of new methods to the development of guidelines for the practical use of current methods in various situations. Such a shift calls for research into the complex relationships between situational factors in development processes. This paper discusses the challenges of investigating the impact of situational factors on PEM and outlines an approach to be used as part of ongoing research.
Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
Creators: name: Cuceu, Andrei
name: Farr, James
name: Lemos, Pablo
name: Font-Ribera, Andreu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate constraints on the Hubble constant ($H_0$) using Baryon Acoustic Oscillations (BAO) and baryon density measurements from Big Bang Nucleosynthesis (BBN). We start by investigating the tension between galaxy BAO measurements and those using the Lyman-$α$ forest, within a Bayesian framework. Using the latest results from eBOSS DR14 we find that the probability of this tension being statistical is $\simeq6.3\%$ assuming flat $Λ$CDM. We measure $H_0 = 67.6\pm1.1$ km s$^{-1}$ Mpc$^{-1}$, with a weak dependence on the BBN prior used, in agreement with results from Planck Cosmic Microwave Background (CMB) results and in strong tension with distance ladder results. Finally, we forecast the future of BAO $+$ BBN measurements of $H_0$, using the Dark Energy Spectroscopic Instrument (DESI). We find that the choice of BBN prior will have a significant impact when considering future BAO measurements from DESI.
description: 14 pages, 3 figures
The Dark Matter Phonon Coupling
Creators: name: Cox, Peter
name: Melia, Tom
name: Rajendran, Surjeet
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Generically, the effective coupling between the dark matter and an atom scales with the number of constituents in the atom, resulting in the effective coupling being proportional to the mass of the atom. In this limit, when the momentum transfer is also small, we show that the leading term in the scattering of a particle off the optical phonons of an array of atoms, whether in a crystal or in a molecule, vanishes. Next-generation dark matter direct detection experiments with sub-eV energy thresholds will operate in a regime where this effect is important, and the suppression can be up to order $10^6$ over naive expectations. For dark matter that couples differently to protons and neutrons, the suppression is typically of order $10-100$ but can be avoided through a judicious choice of material, utilising variations in nuclear ratios $Z/A$ to break the proportionality of the coupling to mass. We provide explicit illustrations of this effect by calculating structure factors for di-molecules and for the crystals NaI and sapphire.
description: 17 pages, 1 figure; v2: version published in PRD
Infrared Surface Brightness Fluctuations of the Coma Elliptical NGC 4874 and the Value of the Hubble Constant
Creators: name: Liu, Michael C.
name: Graham, James R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used the Keck I Telescope to measure K-band surface brightness fluctuations (SBFs) of NGC 4874, the dominant elliptical galaxy in the Coma cluster. We use deep HST WFPC2 optical imaging to account for the contamination due to faint globular clusters and improved analysis techniques to derive measurements of the SBF apparent magnitude. Using a new SBF calibration which accounts for the dependence of K-band SBFs on the integrated color of the stellar population, we measure a distance modulus of 34.99+/-0.21 mag (100+/-10 Mpc) for the Coma cluster. The resulting value of the Hubble constant is 71+/-8 km/s/Mpc, not including any systematic error in the HST Cepheid distance scale.
description: ApJ Letters, in press. Uses emulateapj5.sty
Observability of spherical photon orbits in near-extremal Kerr black holes
Creators: name: Igata, Takahisa
name: Ishihara, Hideki
name: Yasunishi, Yu
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the spherical photon orbits in near-extremal Kerr spacetimes. We show that the spherical photon orbits with impact parameters in a finite range converge on the event horizon. Furthermore, we demonstrate that the Weyl curvature near the horizon does not generate the shear of a congruence of such light rays. Because of this property, a series of images produced by the light orbiting around a near-extremal Kerr black hole several times can be observable.
description: 12 pages, 3 figures; v2: published version
Perkembangan Pendidikan Islam pada Periode Khulafāur Rāsyidīn dan Implikasinya terhadap Pengembangan Pendidikan Islam di Indonesia
Creators: name: Zebua, Rony Sandra Yofa
name: Ihsan, Miftahul
name: Nurjanah, Neneng
Publisher: name: figshare
Year: 2021
Subjects: subject: History
subject: 220403 Islamic Studies
subject: FOS: Philosophy, ethics and religion
subject: Education

description: Religious education for Muslim is Islamic Education originating from Al-Qur’an dan As Sunnah. This study elucidates the dynamic of the change and development of Islamic education in the era after the death of the prophet Muhammad shallallāhu 'alaihi wa sallam, especially in the period of Khulafāur Rāsyidīn. It was revealed how the education system had been implemented in each caliphate and the situation having influenced the educational system. The finding showed that the pattern of the education in the era of caliph Abu Bakar radhīyallāhu ‘anhu was generally still same as the system applied in the era of the prophet of Muhammad shallallāhu 'alaihi wa sallam. The massive development occurred in the period of caliph Umar bin Khatab radhīyallāhu ‘anhu which was continued with the caliph Utsman bin Affan radhīyallāhu ‘anhu. Nevertheless, there were some fundamental changes, especially in the regulation as well as the education method.
A non-intrusive approach for the reconstruction of POD modal coefficients through active subspaces
Creators: name: Demo, Nicola
name: Tezzele, Marco
name: Rozza, Gianluigi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: Reduced order modeling (ROM) provides an efficient framework to compute solutions of parametric problems. Basically, it exploits a set of precomputed high-fidelity solutions --- computed for properly chosen parameters, using a full-order model --- in order to find the low dimensional space that contains the solution manifold. Using this space, an approximation of the numerical solution for new parameters can be computed in real-time response scenario, thanks to the reduced dimensionality of the problem. In a ROM framework, the most expensive part from the computational viewpoint is the calculation of the numerical solutions using the full-order model. Of course, the number of collected solutions is strictly related to the accuracy of the reduced order model. In this work, we aim at increasing the precision of the model also for few input solutions by coupling the proper orthogonal decomposition with interpolation (PODI) --- a data-driven reduced order method --- with the active subspace (AS) property, an emerging tool for reduction in parameter space. The enhanced ROM results in a reduced number of input solutions to reach the desired accuracy. In this contribution, we present the numerical results obtained by applying this method to a structural problem and in a fluid dynamics one.
by any zines necessary: a life vest for teachers in crisis
Creators: name: Ward-Davies, Anastaszia
Publisher: name: The University of Melbourne
Year: 2025
Subjects: classificationCode: 390307
subject: Teacher education and professional development of educators
classificationCode: 360299
subject: Creative and professional writing not elsewhere classified
classificationCode: 360699
subject: Visual arts not elsewhere classified
classificationCode: 390412
subject: Teacher and student wellbeing
classificationCode: 390403
subject: Educational administration, management and leadership

description: This professional learning workbook zine is a creative output generated as part of a Doctor of Education with creative component. This zine brings together co-created knowledges about teacher wellbeing and professional learning in times of crisis and proposes an ongoing model of generative professional reflection and collaborative play.A flipbook version of this NTRO can be viewed hereThis NTRO item includes a compressed downloadable version of the zine and sample pages to view. For a high quality digital version, please contact me at ana.warddavies@unimelb.edu.au
Looking for ultralight dark matter near supermassive black holes
Creators: name: Bar, Nitsan
name: Blum, Kfir
name: Lacroix, Thomas
name: Panci, Paolo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Measurements of the dynamical environment of supermassive black holes (SMBHs) are becoming abundant and precise. We use such measurements to look for ultralight dark matter (ULDM), which is predicted to form dense cores ("solitons") in the centre of galactic halos. We search for the gravitational imprint of an ULDM soliton on stellar orbits near Sgr A* and by combining stellar velocity measurements with Event Horizon Telescope imaging of M87*. Finding no positive evidence, we set limits on the soliton mass for different values of the ULDM particle mass $m$. The constraints we derive exclude the solitons predicted by a naive extrapolation of the soliton-halo relation, found in DM-only numerical simulations, for $2\times10^{-20}~{\rm eV}\lesssim m\lesssim8\times10^{-19}~{\rm eV}$ (from Sgr A*) and $m\lesssim4\times10^{-22}~{\rm eV}$ (from M87*). However, we present theoretical arguments suggesting that an extrapolation of the soliton-halo relation may not be adequate: in some regions of the parameter space, the dynamical effect of the SMBH could cause this extrapolation to over-predict the soliton mass by orders of magnitude.
description: 9 pages + appendices, 5 + 2 figures. v2: some clarifications and references added; conclusions unchanged; version published in JCAP. v3: few typos corrected
Association of social group with both life-history traits and brain size in cooperatively breeding birds
Creators: name: Jiang, Ying
name: Jin, Long
name: Fu, Yi Qiang
name: Liao, Wen Bo
Publisher: name: Brill Online
Year: 2021
Subjects: classificationCode: 310499
subject: Evolutionary biology not elsewhere classified

description: Social group is associated with life-history traits and
can predict brain size variation in cooperative primates and some other mammal
groups, but such explicit relationships remain enigmatic in cooperatively
breeding birds. Indeed, some compositions of social group in cooperative
species (e.g., helper number and group size) would affect the fitness of
breeders by providing alloparental care. Here, we conducted comparative tests
of the relationship between the social group and both life-history traits and brain
size across 197 species of cooperatively breeding birds using phylogenetically
controlled comparative analyses. We did not find any correlations between
helper numbers and both life-history traits and brain size. However, we found
that maximum group size was positively associated with clutch size. Moreover,
average group size has positive associations with body mass and relative brain
size. Our findings suggest that helper numbers cannot promote variation in
relative brain size, while larger groups may predict bigger brains in
cooperatively breeding birds.
Quasi-polynomials and the singular $[Q,R]=0$ theorem
Creators: name: Loizides, Yiannis
Publisher: name: arXiv
Year: 2019
Subjects: subject: Symplectic Geometry (math.SG)
subject: FOS: Mathematics

description: In this short note we revisit the `shift-desingularization' version of the $[Q,R]=0$ theorem for possibly singular symplectic quotients. We take as starting point an elegant proof due to Szenes-Vergne of the quasi-polynomial behavior of the multiplicity as a function of the tensor power of the prequantum line bundle. We use the Berline-Vergne index formula and the stationary phase expansion to compute the quasi-polynomial, adapting an early approach of Meinrenken.
Model Independent analysis of MeV scale dark matter: I. Cosmological constraints
Creators: name: Choudhury, Debajyoti
name: Sachdeva, Divya
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recent results from several direct detection experiments have imposed severe constraints on the multi-GeV mass window for various dark matter (DM) models. However, many of these experiments are not sensitive to MeV scale DM as the corresponding recoil energies are, largely, lower than the detector thresholds. We reexamine the light scalar DM in a model-independent approach. In this first of a two-part work, we develop an appropriate methodology to determine the effective coupling of such a DM to hadrons, thereby allowing for the determination of the corresponding annihilation rates. We find that while the parameter space can be constrained using cosmological and astrophysical observations, a significantly large fraction is still viable. In the companion paper, we study the sensitivity of both direct detection experiments as well as colliders to such a DM.
description: 35 pages, 8 figures. arXiv admin note: substantial text overlap with arXiv:1711.03691
Coelogyne carnosulilabra M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne carnosulilabra

description: Coelogyne carnosulilabra (J.J.Sm.) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum carnosulilabrum J.J.Sm., Repert. Spec. Nov. Regni Veg. 32: 177 (1933).
 Homotypic synonym: Dendrochilum ovatum J.J.Sm., Bull. Jard. Bot. Buitenzorg, sér. 3, 10: 30 (1928), nom. illeg.
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 105, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
On the Column Density of AGN Outflows: the Case of NGC 5548
Creators: name: Arav, Nahum
name: de Kool, Martijn
name: Korista, Kirk T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We re-analyze the HST high resolution spectroscopic data of the intrinsic absorber in NGC 5548 and find that the C IV absorption column density is at least four times larger than previously determined. This increase arises from accounting for the kinematical nature of the absorber and from our conclusion that the outflow does not cover the narrow emission line region in this object. The improved column density determination begins to bridge the gap between the high column densities measured in the X-ray and the low ones previously inferred from the UV lines. Combined with our findings for outflows in high luminosity quasars these results suggest that traditional techniques for measuring column densities: equivalent width, curve-of-growth and Gaussian modeling, are of limited value when applied to absorption associated with AGN outflows.
description: Published ApJ version (566, 699), including a new figure with FUSE data and a useful algebraic expression for the optical depth solution
On the detectability of distant Compton-thick obscured quasars
Creators: name: Fabian, A. C.
name: Wilman, R. J.
name: Crawford, C. S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Chandra and XMM-Newton have resolved the 2-8 keV X-ray Background (XRB) into point sources. Many of the fainter sources are obscured active galactic nuclei (AGN) with column densities in the range of 10^22-10^23 pcmsq, some of which have quasar-like luminosities. According to obscuration models, the XRB above 8 keV is dominated by emission from Compton-thick AGN, with column densities exceeding 1.5 times 10^24 pcmsq. Here, we consider whether Compton-thick quasars are detectable by Chandra and XMM-Newton by their direct (i.e. not scattered) X-ray emission. Detectability is optimized if the objects individually have a high luminosity and high redshift, so that the direct emission has a significant flux in the observed band. Using a simple galaxy formation model incorporating accreting black holes, in which quasars build most of their mass in a Compton-thick manner before expelling the obscuring matter, we predict that moderately deep 100 ks Chandra and XMM-Newton exposures may contain a handful of detectable Compton-thick quasars. Deep Ms or more Chandra images should contain 50-100 distant, optically-faint, Compton-thick sources. In passing we show that radiation pressure can be as effective in expelling the obscuring gas as quasars winds, and yields a black hole mass proportional to the velocity dispersion of the host bulge to the fourth power.
description: 5 pages, accepted for publication in MNRAS
Forming Globular Cluster Systems in a Semi-analytic Scheme
Creators: name: Beasley, Michael A.
name: Baugh, Carlton M.
name: Forbes, Duncan A.
name: Sharples, Ray M.
name: Frenk, Carlos S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We apply the semi-analytical galaxy formation code of Cole et al. to investigate the formation of globular cluster (GC) systems in hierarchical clustering scenarios. The nature of the model allows us to investigate the properties of GC systems and their parent galaxies within a cosmological framework, over a wide dynamic range of mass and time resolution. Assuming GCs form during mergers of gaseous systems, the metal-rich peak of the classical 'bimodal' metallicity distribution of GCs naturally falls out of our model, where such merging occurs over a wide range of redshifts. The physical origin of old, metal-poor GCs (the metal-poor peak) is harder to understand, since their formation must be decoupled from the ongoing star formation in these systems at high redshift (z~5). Within the context of semi-analytic models in general, a possible solution lies in a cut-off in the GC formation efficiency at a characteristic local star formation rate.
description: 6 pages, 4 figures. Contributed talk given at the ESO workshop "Extragalactic Globular Cluster Systems", August 2002, Garching, ed. M. Kissler-Patig, Springer-Verlag
Populations of X-ray binaries and the dynamical history of their host galaxies
Creators: name: Wu, Kinwah
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The observed luminosity distributions of X-ray sources indicate the presence of several populations of X-ray binaries in the nearby galaxies. Each population has its formation and evolutionary history, depending on the host environment. The features seen in the log N($>$S) -- log S curves for different types of galaxies and for different galactic components can be reproduced by a birth-death model, in which the lifespans of the binaries are inversely proportional to their X-ray brightness. Conversely, the dynamical history of a galaxy can be inferred from the luminosity distributions of its X-ray binary populations.
description: accepted for publication in Publ. Astron Soc. Australia, text is revised
Enhancement of alpha-Elements in Dynamical Models of Elliptical Galaxies
Creators: name: Tantalo, R.
name: Chiosi, C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we present a quantitative analysis of the chemical abundances in "monolithic" N-body-Tree-SPH models of elliptical galaxies to determine whether the ratio [alpha/Fe] increases with the galaxy mass as suggested by observational data.
description: 12 pages, 7 figures, 4 tables. To appear in Astronomy and Astrophisics
"Ravellings" a/r/tographic exhibition flyer
Creators: name: Ward-Davies, Anastaszia
Publisher: name: The University of Melbourne
Year: 2025
Subjects: classificationCode: 390412
subject: Teacher and student wellbeing
classificationCode: 390101
subject: Creative arts, media and communication curriculum and pedagogy
classificationCode: 390306
subject: Secondary education
classificationCode: 390307
subject: Teacher education and professional development of educators
classificationCode: 360602
subject: Fine arts
classificationCode: 360601
subject: Crafts

description: This graduate a/r/tographic exhibition, Ravellings, was installed in the Kwong Lee Dow building at studioFive (room 507) for three weeks in 2025. It brings together the da[r]tafacts and data-(a/r/t) that constitute 50% of the Doctor of Education thesis, What happens in the in-between?This NTRO contains the invitation flyer with links to download the professional learning workbook zine, 'by any zines necessary'.
Additional file 4: of An evolutionary approach to recover genes predominantly expressed in the testes of the zebrafish, chicken and mouse
Creators: name: Fouchécourt, Sophie
name: Picolo, Floriane
name: Elis, Sébastien
name: Lécureuil, Charlotte
name: Thélie, Aurore
name: Govoroun, Marina
name: Brégeon, Mégane
name: Papillier, Pascal
name: Jean-Jacques Lareyre
name: Monget, Philippe
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Figure S1. relative mRNA expression level in mouse tissues (T: testis; M: muscle; Ep: epididymis; Li: liver; S: spleen; B: brain; K: kidney; H: heart. N=6 adult males) determined by qRT-PCR for 20 genes (see primers supplemental Table 5) among the 68 of interest (Additional file 3: Table S3A). The testis level is arbitrarily equal to 100. Normalisation was performed with Rpl19 housekeeping mRNA level. (PDF 44 kb)
Additional file 6: of Active eukaryotes in drinking water distribution systems of ground and surface waterworks
Creators: name: Inkinen, Jenni
name: Balamuralikrishna Jayaprakash
name: Sallamaari Siponen
name: Anna-Maria Hokajärvi
name: Pursiainen, Anna
name: Ikonen, Jenni
name: Ryzhikov, Ivan
name: Täubel, Martin
name: Kauppinen, Ari
name: Paananen, Jussi
name: Miettinen, Ilkka
name: Torvinen, Eila
name: Kolehmainen, Mikko
name: Pitkänen, Tarja
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Boxplot of alpha-diversity Shannon values grouped by cold water, hot water, and biofilms in each DWDSs A–E (DNA + RNA) (Figure S2). Boxplot of alpha-diversity Shannon values in cold water (Figure S3). (PDF 255 kb)
Systematic classification of two loop d = 4 Dirac neutrino mass models and the Diracness-dark matter stability connection
Creators: name: Chuliá, Salvador Centelles
name: Cepedello, Ricardo
name: Peinado, Eduardo
name: Srivastava, Rahul
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We provide a complete systematic classification of all two-loop realizations of the dimension four operator for Dirac neutrino masses. Our classification is multi-layered, starting first with a classification in terms of all possible distinct two-loop topologies. Then we discuss the possible diagrams for each topology. Model-diagrams originating from each diagram are then considered. The criterion for genuineness is also defined and discussed at length. Finally, as examples, we construct two explicit models which also serve to highlight the intimate connection between the Dirac nature of neutrinos and dark matter stability.
description: matches published version
Additional file 7: of Active eukaryotes in drinking water distribution systems of ground and surface waterworks
Creators: name: Inkinen, Jenni
name: Balamuralikrishna Jayaprakash
name: Sallamaari Siponen
name: Anna-Maria HokajĂ¤Rvi
name: Pursiainen, Anna
name: Ikonen, Jenni
name: Ryzhikov, Ivan
name: TĂ¤Ubel, Martin
name: Kauppinen, Ari
name: Paananen, Jussi
name: Miettinen, Ilkka
name: Torvinen, Eila
name: Kolehmainen, Mikko
name: PitkĂ¤Nen, Tarja
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
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: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Heatmap clustering analysis by activity recovery (%) of 66 Amoebozoa OTUs (Figure S4.), 139 Fungi OTUs (Figure S5.), 110 Metazoa (animal) OTUs (Figure S6.), 84 Chloroplastida OTUs (Figure S7), 234 Alveolata OTUs (Figure S8.), 148 Stramenopiles OTUs (Figure S9.), and 127 Rhizaria OTUs (Figure S10.). Red color represents a high activity recovery, i.e., relative abundance (%) is higher in RNA than DNA; blue color represents a low activity recovery. (PDF 613 kb)
title: Board Capital and Firm Growth-Options: A Study of Their Impact on Auditors' and Investors' Assessments of Board Effectiveness, Firm Performance and Risk
Creators: name: Smith, Kevin John
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Boards of directors
subject: Auditors
subject: Stockholders
subject: Corporate governance
subject: Social capital

description: Boards of directors are considered to be the lynchpin of corporate governance in Australia (Gillan, 2006) and the roles boards play have been subject to considerable scrutiny and research. It is accepted that boards play multiple roles in governing corporations (Johnson, Daily, & Ellstrand, 1996; Nicholson & Kiel, 2007). However, there is a concern that the current regulatory emphasis on the monitoring and control role does not always lead to optimum corporate governance outcomes (Cohen, Krishnamoorthy, & Wright, 2008; MacAvoy & Millstein, 2004) and that firm performance may be degraded. This research avoids the specific focus on particular board roles and definitions and takes a more holistic view of boards through an examination of board capital. Board capital, which comprises the human capital (Becker, 1964) and the social capital (Burt, 1992; Nahapiet & Ghoshal, 1998) of the directors, culminates in a board’s capability to perform across all its various roles. In addition, a firm’s future growth-options (Pindyck, 1998) are examined as these have been shown to influence a firm’s governance mechanisms (Hutchinson & Gul, 2004) and outcomes particularly through their interaction with board capital.
Relationship between attachment style and love style on married students in Azad University, Falavarjan Branch in 2012
Creators: name: Shooshtarizadeh, Shahnaz
name: Rezaei, Behrooz
name: Jamalpoor Fatemeh
name: Rahmanian Marzie
Publisher: name: Zenodo
Year: 2014
Subjects: Attachment style
love style
mental health

description: Abstract Introduction: Attachment is a specific pattern that is considered vital for many communities to have a healthy development. Individual attachment styles are able to affect the interpersonal relationships broadly. Many studies suggests that people regarding to attachment style, use different coping strategies. The purpose of this study is to investigate the relationship between attachment styles and love ones among married students. Method: This study is a cross- sectional research. The sample consisted of 100 married students studying in Islamic Azad University, Flavarjan Branch selected by randomized method. Data was collected using Adult Attachment Scale (Collins & Read, 1990) and Sternberg's Triangular Love Scale. Data was analyzed with Pearson Correlation Coefficient and Multiple Regression tests, using SPSS Software. Results: Results showed that avoidant style was significantly and positively correlated with triangular love styles (p<.05). The anxious- ambivalent style was significantly correlated only with passion and commitment (p<.05). However secure attachment style was not related to triangular love styles (i.e. passion, intimacy and commitment) (p<.05). Conclusion: Attachment styles are able to predict triangular love styles (i.e. passion, intimacy and commitment). Keywords: Attachment style, love style, mental health
FairVis: Visual Analytics for Discovering Intersectional Bias in Machine Learning
Creators: name: Cabrera, Ángel Alexander
name: Epperson, Will
name: Hohman, Fred
name: Kahng, Minsuk
name: Morgenstern, Jamie
name: Chau, Duen Horng
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: The growing capability and accessibility of machine learning has led to its application to many real-world domains and data about people. Despite the benefits algorithmic systems may bring, models can reflect, inject, or exacerbate implicit and explicit societal biases into their outputs, disadvantaging certain demographic subgroups. Discovering which biases a machine learning model has introduced is a great challenge, due to the numerous definitions of fairness and the large number of potentially impacted subgroups. We present FairVis, a mixed-initiative visual analytics system that integrates a novel subgroup discovery technique for users to audit the fairness of machine learning models. Through FairVis, users can apply domain knowledge to generate and investigate known subgroups, and explore suggested and similar subgroups. FairVis' coordinated views enable users to explore a high-level overview of subgroup performance and subsequently drill down into detailed investigation of specific subgroups. We show how FairVis helps to discover biases in two real datasets used in predicting income and recidivism. As a visual analytics system devoted to discovering bias in machine learning, FairVis demonstrates how interactive visualization may help data scientists and the general public understand and create more equitable algorithmic systems.
description: Accepted as a VAST conference paper to IEEE VIS'19
The Strategy to Build Educative Interaction in Islamic Education on Online Learning Setting
Creators: name: Zebua, Rony Sandra Yofa
Publisher: name: figshare
Year: 2021
Subjects: Education

description: Nowadays, online learning has forced educational stakeholders to sufficiently involve online learning by handling the fundamental difference from traditional learning platforms. While educative interaction is vital but very limited to online learning, the teachers should condition the new environment to enable the learning process. However, educative interaction on online learning requires exact syntax to help the teachers implement it correctly. Therefore, this study aimed to identify the implementation of educative learning on online learning and formulate the syntax to help teachers create educative interaction. The study focused on Islamic and Character Education subjects. The research method is qualitative, using in-depth interviews to gather the data. The informants were from 2 different elementary schools. The study result revealed two types of syntax for educative interaction on online learning: the syntax of educative interaction on real-time chatting app and syntax of educative interaction on the video conference app. Every syntax has similar general phases: preparation, introduction, core, and closing. However, every phase has different details, adjusted to the service provided by the application used. Eventually, the teachers' competence and spirit and supporting infrastructure become the primary factors in maximizing the interaction. Besides, application choice determines the strategy that will be done.
Coelogyne carnosa M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne carnosa

description: Coelogyne carnosa (Ridl.) M.W.Chase & Schuit., comb. nov.
 Basionym: Platyclinis carnosa Ridl., J. Fed. Malay States Mus. 6: 56 (1915).
 Homotypic synonym: Dendrochilum carnosum (Ridl.) Holttum, Gard. Bull. Singapore 11: 280 (1947).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 105, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
SIGMA Observations of the Bursting Pulsar GRO J1744-28
Creators: name: Mejia, J.
name: Villela, T.
name: Goldoni, P.
name: Lebrun, F.
name: Bouchet, L.
name: Jourdain, E.
name: Roques, J. -P.
name: Mandrou, P.
name: Kuznetsov, S.
name: Khavenson, N.
name: Dyachkov, A.
name: Chulkov, I.
name: Novikov, B.
name: Shuhanov, K.
name: Tserenin, I.
name: Sheikhet, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of the GRANAT/SIGMA hard X-/soft gamma-ray long-term monitoring of the Galactic Center (GC) region concerning the source GRO J1744-28, discovered on 1995 Dec. 2 by CGRO/BATSE. SIGMA observed the region containing the source in 14 opportunities between 1990 and 1997. In two of these observing sessions, corresponding to March 1996 and March 1997, GRO J1744-28 was detected with a confidence level greater than 5(sigma) in the 35-75 keV energy band without detection in the 75-150 keV energy band. For the other sessions, upper limits of the flux are indicated. The particular imaging capabilities of the SIGMA telescope allow us to identify, specifically, the source position in the very crowded GC region, giving us a mean flux of (73.1 +/- 5.5)E-11 and (44.7 +/- 6.4)E-11 ergs cm^-2 s^-1 in the 35-75 keV energy band, for the March 1996 and March 1997 observing sessions, respectively. Combining the March 1997 SIGMA and BATSE observations, we found evidence pointing to the type-II nature of the source bursts for this period. For the same observing campaigns, spectra were obtained in the 35 to 150 keV energy band. The best fit corresponds to an optically thin thermal Bremsstrahlung with F(50 keV)=(3.6 +/- 0.6)E-4 phot cm^-2 s^-1 keV^-1 and kT(Bremss)=28 +/- 7 keV, for the first campaign, and F(50 keV)=(2.3 +/- 0.7)E-4 phot cm^-2 s^-1 keV^-1 and kT(Bremss)=18 (+12/-7) keV, for the second. This kind of soft spectrum is typical of binary sources containing a neutron star as the compact object, in contrast to the harder spectra typical of systems containing a black hole candidate
description: Accepted for publication in the Astrophysical Journal, 4 pages, 4 figures
J-PLUS: Synthetic galaxy catalogues with emission lines for photometric surveys
Creators: name: Izquierdo-Villalba, David
name: Angulo, Raul E.
name: Orsi, Alvaro
name: Hurier, Guillaume
name: Vilella-Rojo, Gonzalo
name: Bonoli, Silvia
name: López-Sanjuan, Carlos
name: Alcaniz, Jailson
name: Cenarro, Javier
name: Cristóbal-Hornillos, David
name: Dupke, Renato
name: Ederoclite, Alessandro
name: Hernández-Monteagudo, Carlos
name: Marín-Franch, Antonio
name: Moles, Mariano
name: de Oliveira, Claudia Mendes
name: Sodré, Laerte
name: Varela, Jesús
name: Ramió, Héctor Vázquez
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a synthetic galaxy lightcone specially designed for narrow-band optical photometric surveys. To reduce time-discreteness effects, unlike previous works, we directly include the lightcone construction in the \texttt{L-Galaxies} semi-analytic model applied to the subhalo merger trees of the {\tt Millennium} simulation. Additionally, we add a model for the nebular emission in star-forming regions, which is crucial for correctly predicting the narrow/medium-band photometry of galaxies. Explicitly, we consider, individually for each galaxy, the contribution of 9 different lines: $\rm Lyα$ (1216Å), \Hb (4861Å), \Ha (6563Å), {\oii} (3727Å, 3729Å), {\oiii} (4959Å, 5007Å), $\rm [\ion{Ne}{III}]$ (3870Å), {\oi} (6300Å), $\rm [\ion{N}{II}]$ (6548Å, 6583Å), and $\rm [\ion{S}{II}]$ (6717Å, 6731Å). We validate our lightcone by comparing galaxy number counts, angular clustering, and \Ha, \Hb, {\oii} and {\oiiiFd} luminosity functions to a compilation of observations. As an application of our mock lightcones, we generate catalogues tailored for J-PLUS, a large optical galaxy survey featuring 5 broad and 7 medium band filters. We study the ability of the survey to correctly identify, with a simple \textit{three filter method}, a population of emission-line galaxies at various redshifts. We show that the $4000Å$ break in the spectral energy distribution of galaxies can be misidentified as line emission. However, all significant excess (larger than 0.4 magnitudes) can be correctly and unambiguously attributed to emission line galaxies. Our catalogues are publicly released to facilitate their use in interpreting narrow-band surveys and for quantifying the impact of line emission in broad band photometry.
description: Published in A&A; Mock catalogue available at https://www.j-plus.es/ancillarydata/mock\_galaxy\_lightcone
Biomarker of long-chain n-3 fatty acid intake and breast cancer: Accumulative evidence from an updated meta-analysis of epidemiological studies
Creators: name: Yang, Bo
name: Ren, Xiao L.
name: Wang, Zhi Y.
name: Wang, Liang
name: Zhao, Feng
name: Guo, Xiao J.
name: Li, Duo
Publisher: name: Taylor & Francis
Year: 2018
Subjects: Medicine
Cell Biology
Biotechnology
Biological Sciences not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Objective: We aimed to summarize the up-to-date epidemiology evidence on biomarkers of long-chain (LC) n-3 fatty acid (FA) intake in relation to breast cancer (BC). Methods: Epidemiology studies determining FA levels in biospecimen (circulating blood or adipose tissue (AT)) were identified from PubMed, EMBASE, and Cochrane Library databases until March 2018. Multivariate-adjusted risk ratios (RRs) with 95% confidence intervals (CIs) were pooled using a random-effect model. Difference in biospecimen proportions of LC n-3 FA between BC cases and non-cases were analyzed as a standardized mean difference (SMD). Results: Thirteen cohort and eleven case-control studies were eligible for the present meta-analysis. The estimated SMD was -0.14 (95% CI: -0.27, -0.11) for LC n-3 FA and -0.27 (95% CI: -0.42, -0.11) for LC n-3/n-6 FA ratio. When comparing the top tertiles with the bottom baseline levels, circulating LC n-3 FA was significantly associated with a lower risk of BC (RR: 0.84, 95% CI: 0.74, 0.96), but not AT (RR: 1.02, 95% CI: 0.70, 1.48). Significant inverse dose-response associations were observed for each 1% increment of circulating 20:5n-3 and 22:6n-3. Conclusion: This meta-analysis highlights that circulating LC n-3 FA as a biomarker of intake may be an independent predictive factor for BC, especially 20:5n-3 and 22:6n-3.
THE STRATEGY OF ISLAMIC CHARACTER EDUCATION WITH ROLE MODEL AND HABITUATION METHOD ON ONLINE LEARNING
Creators: name: Zebua, Rony Sandra Yofa
name: Sunarti
Publisher: name: figshare
Year: 2021
Subjects: subject: 130313 Teacher Education and Professional Development of Educators
subject: FOS: Educational sciences
subject: Education

description: Massive development in technology has enforced the educational system to be able to adjust its activity. While maintaining conventional learning environment in character education is challenging, online learning environment provides different characteristics that require distinct strategies to meet the learning objectives. It requires different syntax to implement learning methods for character education on online setting. However, previous studies rarely discussed about character education syntaxes for online learning. Thus, this study aimed to fill the gap by synthesizing the syntax and strategies of implementing some learning methods in character education through online learning. It was chosen Islamic and Character Education as the subject and role model and habituation methods as the focus of the study. This study is a qualitative study using in-depth interview as data collection technique. The informants were teachers experiencing in implementing role model and habituation methods on online learning. The research findings showed that the general syntax of online learning is started from preparation, preliminary activity, core activity, closing, and strengthening activities. Preparation and strengthening activities are conducted in unscheduled time while the other activities are conducted in scheduled time. The proposed syntax is given but further studies are required to testify the syntax for different situations.
Additional file 5: of Active eukaryotes in drinking water distribution systems of ground and surface waterworks
Creators: name: Inkinen, Jenni
name: Balamuralikrishna Jayaprakash
name: Sallamaari Siponen
name: Anna-Maria HokajĂ¤Rvi
name: Pursiainen, Anna
name: Ikonen, Jenni
name: Ryzhikov, Ivan
name: TĂ¤Ubel, Martin
name: Kauppinen, Ari
name: Paananen, Jussi
name: Miettinen, Ilkka
name: Torvinen, Eila
name: Kolehmainen, Mikko
name: PitkĂ¤Nen, Tarja
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Evolutionary Biology
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: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry

description: Top 50 operational taxonomic units (OTUs) in DWDS A (Table S4.), DWDS B (Table S5.), DWDS C (Table S6.), DWDS D (Table S7.) and DWDS E (Table S8.) (PDF 223 kb)