cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Machine-learning techniques applied to three-year exposure of ANAIS-112
Creators: name: Coarasa, I.
name: Apilluelo, J.
name: Amaré, J.
name: Cebrián, S.
name: Cintas, D.
name: García, E.
name: Martínez, M.
name: Oliván, M. A.
name: Ortigoza, Y.
name: de Solórzano, A. Ortiz
name: Puimedón, J.
name: Salinas, A.
name: Sarsa, M. L.
name: Villar, P.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: ANAIS is a direct dark matter detection experiment aiming at the confirmation or refutation of the DAMA/LIBRA positive annual modulation signal in the low energy detection rate, using the same target and technique. ANAIS-112, located at the Canfranc Underground Laboratory in Spain, is operating an array of 3$\times$3 ultrapure NaI(Tl) crystals with a total mass of 112.5 kg since August 2017. The trigger rate in the region of interest (1-6 keV) is dominated by non-bulk scintillation events. In order to discriminate these noise events from bulk scintillation events, robust filtering protocols have been developed. Although this filtering procedure works very well above 2 keV, the measured rate from 1 to 2 keV is about 50% higher than expected according to our background model, and we cannot discard non-bulk scintillation events as responsible of that excess. In order to improve the rejection of noise events, a Boosted Decision Tree has been developed and applied. With this new PMT-related noise rejection algorithm, the ANAIS-112 background between 1 and 2 keV is reduced by almost 30%, leading to an increase in sensitivity to the annual modulation signal. The reanalysis of the three years of ANAIS-112 data with this technique is also presented.
description: Contributed to the TAUP2021 Conference, August 2021. To be published in Journal of Physics: Conference Series
title: ADCO, Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Cart. 176 (11 H 8), f. 0171
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0171, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0171, 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
Nonergodicity and central limit behavior for systems with long-range interactions
Creators: name: Pluchino, Alessandro
name: Rapisarda, Andrea
Publisher: name: arXiv
Year: 2007
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Astrophysics (astro-ph)
subject: Nuclear Theory (nucl-th)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: In this paper we discuss the nonergodic behavior for a class of long-standing quasi-stationary states in a paradigmatic model of long-range interacting systems, i.e. the HMF model. We show that ensemble averages and time averages for velocities probability density functions (pdfs) do not coincide and in particular the latter exhibit a tendency to converge towards a q-Gaussian attractor instead of the usual Gaussian one predicted by the Central Limit Theorem, when ergodicity applies.
description: 7 pages, 5 figures, paper presented at the International SPIE Conference on Complex Systems, 5-7 December 2007, Canberra, Australia, http://spie.org/x12360.xml
Exotic energy injection with ExoCLASS: Application to the Higgs portal model and evaporating black holes
Creators: name: Stöcker, Patrick
name: Krämer, Michael
name: Lesgourgues, Julien
name: Poulin, Vivian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We devise a new user-friendly tool interfaced with the Boltzmann code CLASS to deal with any kind of exotic electromagnetic energy injection in the universe and its impact on anisotropies of the Cosmic Microwave Background. It makes use of the results from standard electromagnetic cascade calculations develop in the context of WIMP annihilation, generalized to incorporate any injection history. We first validate it on a specific WIMP scenario, the Higgs Portal model, confirming that the standard effective on-the-spot treatment is accurate enough. We then analyze the more involved example of evaporating Primordial Black Holes (PBHs) with masses in the range $[3\times10^{13},5\times10^{16}]$g, for which the standard approximations break down. We derive robust CMB bounds on the relic density of evaporating PBHs, ruling out the possibility for PBHs with a monochromatic distribution of masses in the range $[3\times10^{13},2.5\times10^{16}]$g to represent all of the Dark Matter in our Universe. Remarkably, we confirm with an accurate study that the CMB bounds are several orders of magnitude stronger than those from the galactic gamma-ray background in the range $[3\times10^{13},3\times10^{14}]$g. A future CMB experiment like CORE+, or an experiment attempting at measuring the 21 cm signal from the Dark Ages could greatly improve the sensitivity to these models.
description: 29 pages, 10 figures. Comments welcome
Interacting steps with finite-range interactions: Analytical approximation and numerical results
Creators: name: Jaramillo, Diego Felipe
name: Tellez, Gabriel
name: Gonzalez, Diego Luis
name: Einstein, Theodore L.
Publisher: name: American Physical Society
Year: 2013

description: We calculate an analytical expression for the terrace-width distribution P(s) for an interacting step system with nearest- and next-nearest-neighbor interactions. Our model is derived by mapping the step system onto a statistically equivalent one-dimensional system of classical particles. The validity of the model is tested with several numerical simulations and experimental results. We explore the effect of the range of interactions q on the functional form of the terrace-width distribution and pair correlation functions. For physically plausible interactions, we find modest changes when next-nearest neighbor interactions are included and generally negligible changes when more distant interactions are allowed. We discuss methods for extracting from simulated experimental data the characteristic scale-setting terms in assumed potential forms.
Dynamical Scaling Implications of Ferrari, Prähofer, and Spohn’s Remarkable Spatial Scaling Results for Facet-Edge Fluctuations
Creators: name: Einstein, Theodore L.
name: Pimpinelli, Alberto
Publisher: name: Springer
Year: 2014

description: Spurred by theoretical predictions from Spohn and coworkers (Phys. Rev. E 69, 035102(R) (2004)), we rederived and extended their result heuristically as well as investigated the scaling properties of the associated Langevin equation in curved geometry with an asymmetric potential. With experimental colleagues we used STM line scans to corroborate their prediction that the fluctuations of the step bounding a facet exhibit scaling properties distinct from those of isolated steps or steps on vicinal surfaces. The correlation functions was shown to go as t 0.15(3) decidedly different from the t 0.26(2) behavior for fluctuations of isolated steps. From the exponents, we were able to categorize the universality, confirming the prediction that the non-linear term of the KPZ equation, long known to play a central role in non-equilibrium phenomena, can also arise from the curvature or potential-asymmetry contribution to the step free energy. We also considered, with modest Monte Carlo simulations, a toy model to show that confinement of a step by another nearby step can modify as predicted the scaling exponents of the step’s fluctuations. This paper is an expansion of a celebratory talk at the 95th Rutgers Statistical Mechanics Conference, May 2006.
title: CO(1-0) in z gtrsim 4 Quasar Host Galaxies: No Evidence for Extended Molecular Gas Reservoirs
Creators: name: Riechers, DA
name: Walter, F
name: Carilli, CL
name: Knudsen, KK
name: Lo, KY
name: Benford, DJ
name: Staguhn, JG
name: Hunter, TR
name: Bertoldi, F
name: Henkel, C
name: Menten, KM
name: Weiss, Axel
name: Yun, Min
name: Scoville, NZ
Publisher: name: University of Massachusetts Amherst
Year: 2006
Subjects: subject: cosmology: observations; galaxies: active; galaxies: formation; galaxies: high-redshift; galaxies: ISM; galaxies: starburst
subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://iopscience.iop.org/0004-637X/650/2/604/
description: We present 12CO(J = 1 → 0) observations of the high-redshift quasi-stellar objects (QSOs) BR 1202-0725 (z = 4.69), PSS J2322+1944 (z = 4.12), and APM 08279+5255 (z = 3.91) using the NRAO Green Bank Telescope (GBT) and the MPIfR Effelsberg 100 m telescope. We detect, for the first time, the CO ground-level transition in BR 1202-0725. For PSS J2322+1944 and APM 08279+5255, our observations result in line fluxes that are consistent with previous NRAO Very Large Array (VLA) observations, but they reveal the full line profiles. We report a typical lensing-corrected velocity-integrated intrinsic 12CO(J = 1 → 0) line luminosity of L = 5 × 1010 K km s-1 pc2 and a typical total H2 mass of M(H2) = 4 × 1010 M for the sources in our sample. The CO/FIR luminosity ratios of these high-z sources follow the same trend as seen for low-z galaxies, leading to a combined solution of log LFIR = (1.39 ± 0.05) log LCO - 1.76. It has previously been suggested that the molecular gas reservoirs in some quasar host galaxies may exhibit luminous, extended 12 CO(J = 1 → 0) components that are not observed in the higher J CO transitions. Using the line profiles and the total intensities of our observations and large velocity gradient (LVG) models based on previous results for higher J CO transitions, we derive that emission from all CO transitions is described well by a single gas component in which all molecular gas is concentrated in a compact nuclear region. Thus, our observations and models show no indication of a luminous extended, low surface brightness molecular gas component in any of the high-redshift QSOs in our sample. If such extended components exist, their contribution to the overall luminosity is limited to at most 30%.
Retrieval of diurnal cycles in "depth" and "skin" SSTs from the new generation ABI/AHI geostationary sensors with ACSPO
Creators: name: Petrenko, Boris
Publisher: name: Zenodo
Year: 2017

description: Presentation given at the 18th GHRSST science meeting (XVIII), Qingdao, China, June 5 - 9, 2017
A numerical approach to stochastic inflation and primordial black holes
Creators: name: Tomberg, Eemeli
Publisher: name: arXiv
Year: 2021
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Certain models of cosmic inflation produce strong cosmological perturbations at short length scales, which may later collapse into primordial black holes. To find the statistics of these strong perturbations and the ensuing black holes, it is necessary to go beyond linear perturbation theory. Stochastic inflation provides a way to take the leading non-linear effects into account. In this contribution, I discuss recent progress in numerical computations of stochastic inflation. A numerical approach can include more of the non-linearities than an analytical calculation, and can be applied to single-field inflationary models with any potential.
description: 5 pages, 2 figures. Based on Phys.Rev.Lett. 127 (2021) 10, 101302, arXiv:2012.06551. Proceedings of the 17th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2021)
The High Density Region of QCD from an Effective Model
Creators: name: De Pietri, R.
name: Feo, A.
name: Seiler, E.
name: Stamatescu, I. -O.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the high density region of QCD within an effective model obtained in the frame of the hopping parameter expansion and choosing Polyakov-type loops as the main dynamical variables representing the fermionic matter. This model still shows the so-called sign problem, a difficulty peculiar to non-zero chemical potential, but it permits the development of algorithms which ensure a good overlap of the simulated Monte Carlo ensemble with the true one. We review the main features of the model and present results concerning the dependence of various observables on the chemical potential and on the temperature, in particular of the charge density and the Polykov loop susceptibility, which may be used to characterize the various phases expected at high baryonic density. In this way, we obtain information about the phase structure of the model and the corresponding phase transitions and cross over regions, which can be considered as hints about the behaviour of non-zero density QCD.
description: 7 pages, 5 figures, talk presented at the XXVth International Symposium on Lattice Field Theory, July 30 - August 4 2007, Regensburg, Germany
How "Hot Precursors" Modify Island Nucleation: A Rate-Equation Model
Creators: name: Morales-Cifuentes, Josue R.
name: Einstein, Theodore L.
name: Pimpinelli, Alberto
Publisher: name: American Physical Society
Year: 2014

description: We propose a novel island nucleation and growth model explicitly including transient (ballistic) mobility of the monomers deposited at rate F, assumed to be in a hot precursor state before thermalizing.
Neutron Stars: Formed, Spun and Kicked
Creators: name: Kalogera, Vassiliki
name: Valsecchi, Francesca
name: Willems, Bart
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: One of the primary goals when studying stellar systems with neutron stars has been to reveal the physical properties of progenitors and understand how neutron star spins and birth kicks are determined. Over the years a consensus understanding had been developed, but recently some of the basic elements of this understanding are being challenged by current observations of some binary systems and their theoretical interpretation. In what follows we review such recent developments and highlight how they are interconnected; we particularly emphasize some of the assumptions and caveats of theoretical interpretations and examine their validity (e.g., in connection to the unknown radial velocities of pulsars or the nuances of multi-dimensional statistical analysis). The emerging picture does not erase our earlier understanding; instead it broadens it as it reveals additional pathways for neutron star formation and evolution: neutron stars probably form at the end of both core collapse of Fe cores of massive stars and electron-capture supernovae of ONeMg cores of lower-mass stars; birth kicks are required to be high (well in excess of 100 km/s) for some neutron stars and low (< 100 km/s) for others depending on the formation process; and spin up may occur not just through Roche-lobe overflow but also through wind accretion or phases of hypercritical accretion during common envelope evolution.
description: 9 pages,4 figures, proceedings paper for 40 Years of Pulsars Conference
Additional file 15: of Comparative analysis of binding patterns of MADS-domain proteins in Arabidopsis thaliana
Creators: name: Aerts, Niels
name: Bruijn, Suzanne De
name: Mourik, Hilda Van
name: Angenent, Gerco
name: Dijk, Aalt Van
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Plasma Physics
subject: Plant Biology
subject: Computational Biology

description: Table S7. Top 5 most occurring extensions on the 5′ side and the 3′ side of the CArG-box and the top 5 combinations of 5′ and 3′ extensions. CArG-boxes were defined de novo by MEME-ChIP as described in the Material and Methods section. For each CArG-box like sequence, positions 1 and 10 were defined by comparing the sequence to the canonical CArG-box (CC(A/T)6GG. Position 1 was defined as the position that corresponds to the first C in the canonical CArG-box and position 10 was defined as the position that corresponds to the last G in the canonical CArG-box. Also, the strand defined by MEME-ChIP was taken to distinguish the 5′ and the 3′ sides. Subsequently, the three nucleotides on the 5′ side of position 1 and on the 3′ side of position 10 were counted for each CArG-box. The top 5 most occurring extensions and extension combinations were defined for (A) AG, (B) AP1, (C) AP3, (D) FLC, (E) PI, (F) SEP3, (G) SOC1 and (H) SVP. (PDF 95 kb)
Triangular lattice gas with first- and second-neighbor exclusions: Continuous transition in the four-state Potts universality class
Creators: name: Bartelt, N. C.
name: Einstein, Theodore L.
Publisher: name: American Physical Society
Year: 1984

description: Using phenomenological renormalization (transfer-matrix scaling), we have reexamined the phase transition of a triangular lattice gas with particles having both nearest- and second-nearest-neighbor exclusions. Widely accepted classical studies indicated that disordering of the ordered (p(2x2)) state is first order. In contradiction, we show that the transition is second order; its exponents are consistent with the four-state Potts model universality class, in accord with its Landau-Ginzburg-Wilson Hamiltonian classification.
Chemical insight from density functional modeling of molecular adsorption: Tracking the bonding and diffusion of anthracene derivatives on Cu(111) with molecular orbitals
Creators: name: Wyrick, Jonathan
name: Einstein, Theodore L.
name: Bartels, Ludwig
Publisher: name: AIP
Year: 2015

description: We present a method of analyzing the results of density functional modeling of molecular adsorption in terms of an analogue of molecular orbitals. This approach permits intuitive chemical insight into the adsorption process. Applied to a set of anthracene derivates (anthracene, 9,10-anthraquinone, 9,10-dithioanthracene, and 9,10-diselenonanthracene), we follow the electronic states of the molecules that are involved in the bonding process and correlate them to both the molecular adsorption geometry and the species’ diffusive behavior. We additionally provide computational code to easily repeat this analysis on any system.
Additional file 8: of Dose constraints in the rectum and bladder following carbon-ion radiotherapy for uterus carcinoma: a retrospective pooled analysis
Creators: name: Okonogi, Noriyuki
name: Fukahori, Mai
name: Wakatsuki, Masaru
name: Ohkubo, Yu
name: Kato, Shingo
name: Miyasaka, Yuhei
name: Tsuji, Hiroshi
name: Nakano, Takashi
name: Kamada, Tadashi
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Computational Biology

description: Table S3. Correlation between dose-volume histogram parameters and late morbidities of the rectum in the 24 fractions group. This table summarizes the doseâ volume histogram parameters from V10 to V60, D5cc, D2cc, and Dmax according to the grading of rectal morbidity in the 24 fractions group. (DOCX 16 kb)
Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
Creators: name: Drakos, Nicole E.
name: Villasenor, Bruno
name: Robertson, Brant E.
name: Hausen, Ryan
name: Dickinson, Mark E.
name: Ferguson, Henry C.
name: Furlanetto, Steven R.
name: Greene, Jenny E.
name: Madau, Piero
name: Shapley, Alice E.
name: Stark, Daniel P.
name: Wechsler, Risa H.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In the next decade, deep galaxy surveys from telescopes such as the James Webb Space Telescope and Roman Space Telescope will provide transformational data sets that will greatly enhance the understanding of galaxy formation during the epoch of reionization (EoR). In this work, we present the Deep Realistic Extragalactic Model (DREaM) for creating synthetic galaxy catalogs. Our model combines dark matter simulations, subhalo abundance matching and empirical models, and includes galaxy positions, morphologies, and spectral energy distributions (SEDs). The resulting synthetic catalog extends to redshifts $z \sim 12 $, and galaxy masses $\log_{10}(M/M_{\odot}) = 5 $ covering an area of $1\, {\rm deg}^2$ on the sky. We use DREaM to explore the science returns of a $1\, {\rm deg}^2$ \emph{Roman} UDF, and to provide a resource for optimizing ultra-deep survey designs. We find that a \emph{Roman} UDF to $\sim 30\,m_{\rm AB}$ will potentially detect more than $10^6$ $M_{\rm UV}7$, offering an unparalleled dataset for constraining galaxy properties during the EoR. Our synthetic catalogs and simulated images are made publicly available to provide the community with a tool to prepare for upcoming data.
description: 39 pages, 27 figures. Submitted to ApJ. Comments welcome
The twist-3 parton distribution function e(x) in large-Nc chiral theory
Creators: name: Cebulla, C.
name: Ossmann, J.
name: Schweitzer, P.
name: Urbano, D.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The chirally-odd twist-3 parton distribution function e(x) of the nucleon is studied in the large-Nc limit in the framework of the chiral quark-soliton model. It is demonstrated that in spite of properties not shared by other distribution functions, namely the appearance of a delta(x)-singularity and quadratic divergences in e(x), an equally reliable calculation is possible. Among the most remarkable results obtained in this work is the fact that the coefficient of the delta(x)-singularity can be computed exactly in this model, avoiding involved numerics. Our results complete existing studies in literature.
description: 16 pages, 9 figures
Radiative Transfer Model based Bias Correction in INSAT-3D/3DR Thermal Observations to Improve Sea Surface Temperature Retrieval
Creators: name: Gangwar, Rishi K.
Publisher: name: Zenodo
Year: 2017

description: Presentation given at the 18th GHRSST science meeting (XVIII), Qingdao, China, June 5 - 9, 2017
Additional file 1: of Hematuria as a risk factor for progression of chronic kidney disease and death: findings from the Chronic Renal Insufficiency Cohort (CRIC) Study
Creators: name: Orlandi, Paula
name: Fujii, Naohiko
name: Roy, Jason
name: Hsiang-Yu Chen
name: L. Lee Hamm
name: Sondheimer, James
name: He, Jiang
name: Fischer, Michael
name: Hernan Rincon-Choles
name: Krishnan, Geetha
name: Townsend, Raymond
name: Shafi, Tariq
name: Chi-Yuan Hsu
name: Kusek, John
name: Daugirdas, John
name: Feldman, Harold
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: Computational Biology

description: Proportional Hazards Plots. Scaled Schoenfeld Residuals Plots by year of follow-up examining if the Proportional Hazards Assumption is valid. (DOCX 26Â kb)
Competing growth processes induced by next-nearest-neighbor interactions: Effects on meandering wavelength and stiffness
Creators: name: Blel, Sonia
name: Hamouda, Ajmi BH.
name: Mahjoub, B.
name: Einstein, Theodore L.
Publisher: name: American Physical Society
Year: 2017

description: In this paper we explore the meandering instability of vicinal steps with a kinetic Monte Carlo simulations (kMC) model including the attractive next-nearest-neighbor (NNN) interactions. kMC simulations show that increase of the NNN interaction strength leads to considerable reduction of the meandering wavelength and to weaker dependence of the wavelength on the deposition rate F. The dependences of the meandering wavelength on the temperature and the deposition rate obtained with simulations are in good quantitative agreement with the experimental result on the meandering instability of Cu(0 2 24) (T. Maroutian et al., Phys. Rev. B 64, 165401 (2001)). The effective step stiffness is found to depend not only on the strength of NNN interactions and the Ehrlich-Schwoebel barrier, but also on F. We argue that attractive NNN interactions intensify the incorporation of adatoms at step edges and enhance step roughening. Competition between NNN and nearest-neighbor interactions results in an alternative form of meandering instability which we call “roughening-limited” growth, rather than attachment-detachment-limited growth that governs the Bales-Zangwill instability.
Preliminary diet record of hinge-back tortoise Kinixys zombensis: a potential seed disperser?
Creators: name: Lloyd, Kyle
name: Parker, Daniel
Publisher: name: figshare
Year: 2021
Subjects: subject: Zoology
subject: FOS: Biological sciences

description: Thirteen faecal samples were collected directly from different, individual tortoises at Enseleni Nature Reserve, South Africa (28°41'S 32°00'E) during wet season months (December 2012 – January 2013). Twenty-six tortoises were found in total but only half produced faecal samples whilst being handled. Hinge-back tortoises aestivate during dry season months (May-September; Boycott & Bourquin, 2000) and so no faecal samples were collected during this time. Individual tortoises were identified by making notches along the marginal scutes of sampled tortoises. Tortoises were found in subtropical coastal forest (Figure 1c) and grassland (Figure 1d). Faecal samples were passed through two sieves of different apertures (5.0 mm and 0.5 mm, respectively) and inspected using a dissecting microscope. We recognised seven broad food groups: woody vegetation (including tree and shrub leaves, sticks, and bark), grass, seeds and fruit, fungi, insects, millipedes, and snails (only when shells were present). Where possible, we further identified food items to at least the genus level using field guides (Scholtz & Holm, 1985; Gryzenhout, 2010) and expert advice (M. Hamer, T. Dold, J. Midgley, J. Dames pers. comm.). Identification was assisted by comparing food items to plant and invertebrate reference specimens, and opportunistic observations of tortoises feeding at the study site. The number of food groups present in each faecal sample were recorded and converted to a frequency of occurrence (expressed as a percentage of the total number of food groups present in each faecal sample; following MacDonald & Mushinsky, 1988).
Additional variables were measured when tortoises were captured that do not appear in the publication and are unlikely to be reported in the peer-reviewed literature. These include individual identification, date of capture, time of capture, habitat type, coordinates, age, sex, weight, carapace dimensions, number of ticks per body part, and number of ticks upon recapture. Carapace dimensions were measured using a caliper and weight was measured by suspending the tortoise in a material sheet from a fishing scale. Ticks were counted with the naked eye and individuals sampled for identification. Refer to the following publication for more information about the sampled ticks in this study: Horak, I.G., Pearcy, A. & Lloyd, K.J. 2017. Parasites of domestic and wild animals in South Africa. LI. Ticks infesting leopard tortoises Stigmochelys pardalis, hingeback tortoises Kinixys zombensis and angulate tortoises Chersina angulate. Onderstepoort Journal of Veterinary Research 84(1): a1303. https://doi.org/10.4102/ojvr.v84i1.1303
title: ADCO, Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Cart. 198-01 (11 H 1055), 185 folios, f. 0119
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2019
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0119, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les domaines de Saint-Jean de Losne et Losne (XVIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 198-01 (11 H 1055), 185 folios, f. 0119, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Gravitational Orbits and the Lambert Problem
Creators: name: Gatland, Ian R
Publisher: name: arXiv
Year: 2021
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: The Lambert problem is to determine the gravitational orbit between two points that has a specified time of flight, allowing the second point to be a moving target such as a satellite. After a review of gravitational orbits, a solution of the Lambert problem is presented using the path equation directly. However, because the time interval is specified, the solution requires a search procedure. An example is given to illustrate the method.
description: 6 pages. 1 figure. In press
title: AzTEC/ASTE 1.1-mm survey of the AKARI Deep Field South: source catalogue and number counts
Creators: name: Hatsukade, B
name: Kohno, K
name: Aretxaga, I
name: Austermann, JE
name: Ezawa, H
name: Hughes, DH
name: Ikarashi, S
name: Iono, D
name: Kawabe, R
name: Khan, S
name: Matsuo, H
name: Matsuura, S
name: Nakanishi, K
name: Oshima, T
name: Perera, T
name: Scott, KS
name: Shirahata, M
name: Takeuchi, TT
name: Yamura, Y
name: Tanaka, K
name: Tosaki, T
name: Wilson, GW
name: Yun, Min
Publisher: name: University of Massachusetts Amherst
Year: 2010
Subjects: subject: * galaxies: evolution; * galaxies: formation; * galaxies: high-redshift; * galaxies: starburst
subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2010.17658.x/abstract
description: We present results of a 1.1-mm deep survey of the AKARI Deep Field South (ADF-S) with AzTEC mounted on the Atacama Submillimetre Telescope Experiment (ASTE). We obtained a map of 0.25-deg2 area with an rms noise level of 0.32–0.71 mJy. This is one of the deepest and widest maps thus far at millimetre and submillimetre wavelengths. We uncovered 198 sources with a significance of 3.5σ–15.6σ, providing the largest catalogue of 1.1-mm sources in a contiguous region. Most of the sources are not detected in the far-infrared bands of the AKARI satellite, suggesting that they are mostly at z≥ 1.5 given the detection limits. We constructed differential and cumulative number counts in the ADF-S, the Subaru/XMM–Newton Deep Field and the SSA 22 field surveyed by AzTEC/ASTE, which provide currently the tightest constraints on the faint end. The integration of the best-fitting number counts in the ADF-S finds that the contribution of 1.1-mm sources with fluxes of ≥1 mJy to the cosmic infrared background (CIB) at 1.1 mm is 12–16 per cent, suggesting that the large fraction of the CIB originates from faint sources of which the number counts are not yet constrained. We estimate the cosmic star formation rate density contributed by 1.1-mm sources with ≥1 mJy using the best-fitting number counts in the ADF-S and find that it is lower by about a factor of 5–10 compared to those derived from UV/optically selected galaxies at z∼ 2–3. The fraction of stellar mass of the present-day universe produced by 1.1-mm sources with ≥1 mJy at z≥ 1 is ∼20 per cent, calculated by the time integration of the star formation rate density. If we consider the recycled fraction of >0.4, which is the fraction of materials forming stars returned to the interstellar medium, the fraction of stellar mass produced by 1.1-mm sources decreases to ≲10 per cent.
Fragmentation approach to the point-island model with hindered aggregation: Accessing the barrier energy
Creators: name: Gonzalez, Diego Luis
name: Pimpinelli, Alberto
name: Einstein, Theodore L.
Publisher: name: American Physical Society
Year: 2017

description: We study the effect of hindered aggregation on the island formation process in a one- (1D) and two-dimensional (2D) point-island model for epitaxial growth with arbitrary critical nucleus size i. In our model, the attachment of monomers to preexisting islands is hindered by an additional attachment barrier, characterized by length la. For la=0 the islands behave as perfect sinks while for la?? they behave as reflecting boundaries. For intermediate values of la, the system exhibits a crossover between two different kinds of processes, diffusion-limited aggregation and attachment-limited aggregation. We calculate the growth exponents of the density of islands and monomers for the low coverage and aggregation regimes. The capture-zone (CZ) distributions are also calculated for different values of i and la. In order to obtain a good spatial description of the nucleation process, we propose a fragmentation model, which is based on an approximate description of nucleation inside of the gaps for 1D and the CZs for 2D. In both cases, the nucleation is described by using two different physically rooted probabilities, which are related with the microscopic parameters of the model (i and la). We test our analytical model with extensive numerical simulations and previously established results. The proposed model describes excellently the statistical behavior of the system for arbitrary values of la and i=1, 2, and 3.
The Poisson bracket on free null initial data for gravity
Creators: name: Reisenberger, Michael P.
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Free initial data for general relativity on a pair of intersecting null hypersurfaces are well known, but the lack of a Poisson bracket and concerns about caustics have stymied the development of a constraint free canonical theory. Here it is pointed out how caustics and generator crossings can be neatly avoided and a Poisson bracket on free data is given. On sufficiently regular functions of the solution spacetime geometry this bracket matches the Poisson bracket defined on such functions by the Hilbert action via Peierls' prescription. The symplectic form is also given in terms of free data.
description: 4 pages,1 figure. Some changes to text to improve clarity of presentation, this is the final published version
Patterns of Organics on Substrates with Metallic Surface States: Why? So??
Creators: name: Einstein, Theodore L.
name: Bartels, Ludwig
name: Morales-Cifuentes, Josue R.
Publisher: name: JSVSS
Year: 2018

description: This paper modestly expands an invited talk at ISSS-8 with the same title. After reviewing the relevant interactions between adsorbates on substrates with metallic surface states (especially Cu(111)), it focuses on organic adsorbates. Of particular interest are those which form honeycomb lattices with pores of various sizes. The nature of the confined states derived from the surface-state electrons is discussed as their effect on admolecules inside the pores.
Additional file 1: of Design and implementation of an m-health data model for improving health information access for reproductive and child health services in low resource settings using a participatory action research approach
Creators: name: Thobias, Joseph
name: Achilles Kiwanuka
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy

description: KII and FGD Guides: This file contains key informant interview probing questions that were used during data collection for RCH service providers, traditional birth attendants, community leaders and community health workers. Additionally, it contains probing questions for the focus group discussion used to interview community members. (DOCX 16 kb)
Kinetic-thermodynamic model for carbon incorporation during step-flow growth of GaN by metalorganic vapor phase epitaxy
Creators: name: Inatomi, Y.
name: Kangawa, Y.
name: Pimpinelli, Alberto
name: Einstein, Theodore L.
Publisher: name: American Physical Society
Year: 2019

description: Relationships between concentration of unintentionally doped carbon in GaN and its metalorganic vapor phase epitaxy conditions were investigated theoretically. A kinetic-thermodynamic model which considers kinetic behavior of adsorbed atoms on vicinal surface was proposed.
Strain-Controlled Magnetic and Optical Properties of Monolayer 2H-TaS e2
Creators: name: Chowdhury, Sugata
name: Simpson, Jeffrey R.
name: Einstein, Theodore L.
name: Hight Walker, Angela R.
Publisher: name: American Physical Society
Year: 2019

description: First-principles calculations are used to probe the effects of mechanical strain on the magnetic and optical properties of monolayer (ML) 2H?TaSe2. A complex dependence of these physical properties on strain results in unexpected spin behavior, such as ferromagnetism under uniaxial, in-plane, tensile strain and a lifting of the Raman-active E? phonon degeneracy.
The Galactic Bulge: A Review
Creators: name: Minniti, Dante
name: Zoccali, Manuela
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Milky Way is the only galaxy for which we can resolve individual stars at all evolutionary phases, from the Galactic center to the outskirt. The last decade, thanks to the advent of near IR detectors and 8 meter class telescopes, has seen a great progress in the understanding of the Milky Way central region: the bulge. Here we review the most recent results regarding the bulge structure, age, kinematics and chemical composition. These results have profound implications for the formation and evolution of the Milky Way and of galaxies in general. This paper provides a summary on our current understanding of the Milky Way bulge, intended mainly for workers on other fields.
description: 10 pages, 8 Postscript figures, uses iaus.cls To appear in Proceedings of IAU Symp. 245 on "Formation and Evolution of Galaxy Bulges", (held at Oxford, July 16-20 2007), Eds. Martin Bureau, Lia Athanassoula, and Beatriz Barbuy
title: ADCO, Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Cart. 23 (G 127), 310 folios, f. 00417
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2011
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00417, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00417, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
A gravitational-wave probe of effective quantum gravity
Creators: name: Alexander, Stephon
name: Finn, Lee Samuel
name: Yunes, Nicolas
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The Green-Schwarz anomaly-cancelling mechanism in string theories requires a Chern-Simons term in the Einstein-Hilbert action, which leads to an amplitude birefringence of spacetime for the propagation of gravitational waves. While the degree of birefringence may be intrinsically small, its effects on a gravitational wave will accumulate as the wave propagates. The proposed Laser Interferometer Space Antenna (LISA) will be sensitive enough to observe the gravitational waves from sources at cosmological distances great enough that interesting bounds on the Chern-Simons may be found. Here we evaluate the effect of a Chern-Simons induced spacetime birefringence to the propagation of gravitational waves from such systems. We find that gravitational waves from in coalescing binary black hole system are imprinted with a signature of Chern-Simons gravity. This signature appears as a time-dependent change in the apparent orientation of the binary's orbital angular momentum with respect to the observer line-of-sight, with the change magnitude reflecting the integrated history of the Chern-Simons coupling over the worldline of a radiation wavefront. While spin-orbit coupling in the binary system will also lead to an evolution of the system's orbital angular momentum, the time dependence and other details of this \emph{real} effect are different than the \emph{apparent} effect produced by Chern-Simons birefringence, allowing the two effects to be separately identified.
description: 14 pages, no figures, submitted to Phys. Rev. D
Ecoliteracy: Foundation of Vocationally Specific Sustainability Education
Creators: name: Bauer, Eric Douglas
Publisher: name: Griffith University
Year: 2016
Subjects: Ecoliteracy
Ecological knowledge
Conservation of natural resources

description: There is ample evidence that human actions are continuously and progressively straining planetary processes and systems vital for the wellbeing of the planet, as well as people themselves (WWF, 2012, 2014). Education has a key role to play in addressing these challenges. The role of technical and vocational education and training (TVET) in addressing these challenges has also been recognized. However, little is understood about the preparedness of TVET educators, specialists in their vocational areas, to address environmental and sustainability issues. This action research study examines the relationship between educator ecoliteracy and educator ability to develop and deliver vocationally specific sustainability education, in a single TVET college in Canada. The research study was undertaken over a 3-year period and involved 43 participants in total. Findings indicate that educators’ ecological knowledge, their collegial relationships and institutional processes are all significant in supporting attempts to revise vocational curriculum. Professional learning to improve vocational educators’ ecoliteracy requires more than deepening ecological knowledge, however. Also required is an understanding of the science of contemporary ecological issues and the relationship of those issues to broader socio-cultural and economic activities. In order to consider curriculum revision, educators thus need to personally value and prioritize such education as essential to the development of vocational competency amongst their students. Improving the ecoliteracy of the educator community, therefore, requires more than simply developing knowledge and skill in the scientific language of ecology; it also requires opportunities for educators to participate in institutional sustainability policies and practices
Proof of the bulk-edge correspondence through a link between topological photonics and fluctuation-electrodynamics
Creators: name: Silveirinha, Mario G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The bulk-edge correspondence links the Chern-topological numbers with the net number of unidirectional states supported at an interface of the relevant materials. This fundamental principle is perhaps the most consequential result of topological photonics, as it determines the precise physical manifestations of nontrivial topological features. Even though the bulk-edge correspondence has been extensively discussed and used in the literature, it seems that in the general photonic case with dispersive materials it has no solid mathematical foundation and is essentially a conjecture. Here, I present a rigorous demonstration of this fundamental principle by showing that the thermal fluctuation-induced light-angular momentum spectral density in a closed cavity can be expressed in terms of the photonic gap Chern number, as well as in terms of the net number of unidirectional edge states. In particular, I highlight the rather fundamental connections between topological numbers in Chern-type photonic insulators and the fluctuation-induced light-momentum
description: to be published in PRX