cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Optical Variability of the T Tauri Star HH30
Creators: name: Wood, Kenneth
name: Wolk, Scott
name: Stanek, K. Z.
name: Leussis, George
name: Stassun, Keivan
name: Wolff, Michael
name: Whitney, Barbara
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report results of VRI photometric monitoring of the T Tauri star plus disk system HH30. We find that HH30 is highly variable over timescales of a few days with Delta V~1.5 mag, Delta I~1.1 mag. Furthermore we find hints of periodicity with periodograms indicating possible periods of 11.6 and 19.8 days. The VRI photometry is available through the anonymous ftp service. We model the variability with Monte Carlo radiation transfer simulations for a spotted star plus disk system and find that the large variability is best reproduced with a single hot spot and circumstellar grains that are larger than typical interstellar grains. The apparent existence of a single hot spot and the need for larger, more forward throwing grains is consistent with previous modeling of HST imagery.
description: 7 pages, 3 figures. Accepted for ApJ Letters
title: Histoire : wandou gongzhu
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Nonlinear magnetotransport in interacting chiral nanotubes
Creators: name: De Martino, A.
name: Egger, R.
name: Tsvelik, A. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Nonlinear transport through interacting single-wall nanotubes containing a few impurities is studied theoretically. Extending the Luttinger liquid theory to incorporate trigonal warping and chirality effects, we derive the current contribution $I_e$ {\sl even} in the applied voltage $V$ and {\sl odd} in an orbital magnetic field $B$, which is non-zero only for chiral tubes and in the presence of interactions.
description: 4 pages, 1 figure, minor changes, to appear in PRL
Advances in Image Fidelity: Radio Interferometer and Single-Dish Data Combination
Creators: name: Plunkett, Adele
Publisher: name: Zenodo
Year: 2019

description: We have formed an international working group for investigating and implementing techniques for data combination of interferometry and single dish observations. In this poster, we will present the proceedings of the recent workshop "Improving Image Fidelity on Astronomical Data: Radio Interferometer and Single-Dish Data Combination," held at the Lorentz Center in August 2019. The methodology of the workshop was to convene the leading experts in interferometry and single-dish combination techniques across the world, with the aim to understand, compare, and test the various methods. A combination of scientific talks from key invited speakers; technical talks covering the various techniques; and a number of hands-on sessions to test and work on the different combination methods will be summarized in this poster. The expected outcome of the workshop included user-guides for the respective existing methods, specifying means for evaluation and guidelines as to which method could perform better under which circumstances, and assessing the need for new techniques and/or implementation of methods into CASA. These techniques are important for ALMA to fully utilize observations from 12m, 7m, and Total Power (TP) arrays, and scientifically critical for mm-wave studies of diverse topics including star formation, extragalactic sources, characterization of solar features, the evolution of stars and planetary nebulae — all of which depend on high spatial dynamic range observations that provide information on both the diffuse, extended emission and compact, localized objects where astrophysical processes happen.
Perturbative treatment of intercenter coupling in Redfield theory
Creators: name: Kleinekathoefer, Ulrich
name: Kondov, Ivan
name: Schreiber, Michael
Publisher: name: arXiv
Year: 2000
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The quantum dynamics of coupled subsystems connected to a thermal bath is studied. In some of the earlier work the effect of intercenter coupling on the dissipative part was neglected. This is equivalent to a zeroth-order perturbative expansion of the damping term with respect to the intercenter coupling. It is shown numerically for two coupled harmonic oscillators that this treatment can lead to artifacts and a completely wrong description, for example, of a charge transfer processes even for very weak intercenter coupling. Here we perform a first-order treatment and show that these artifacts disappear. In addition, we demonstrate that the thermodynamic equilibrium population is almost reached even for strong intercenter coupling strength.
Supplementary Methods and Figures from Integration of genomic and ecologic methods inform management of an undescribed, yet highly exploited, sardine species
Creators: name: Coelho, Jéssica Fernanda Ramos
name: Mendes, Liana de Figueiredo
name: Di Dario, Fabio
name: Carvalho, Pedro Hollanda
name: Dias, Ricardo Marques
name: Lima, Sergio Maia Queiroz
name: Verba, Julia Tovar
name: Pereira, Ricardo J.
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310399
subject: Ecology not elsewhere classified
classificationCode: 310499
subject: Evolutionary biology not elsewhere classified
classificationCode: 310509
subject: Genomics

description: Model parameters of ecological niche models and molecular analyses.
title: Economic Sustainability Plan for Adams, Massachusetts: Ten Year Projection Plan
Creators: name: (:Unkn) Unknown
Publisher: name: University of Massachusetts Amherst
Year: 1998
Subjects: subject: Adams
subject: Massachusetts
subject: Sustainability
subject: Regionalism
subject: Transportation
subject: Infrastructure
subject: Education
subject: Labor
subject: Historic Preservation
subject: Economic Policy
subject: Economics
subject: Environmental Policy
subject: Environmental Studies
subject: Growth and Development
subject: Recreation, Parks and Tourism Administration
subject: Regional Economics

description: The Center for Economic Development at the University of Massachusetts, in Amherst, is part of the Landscape Architecture and Regional Planning Department, and is funded by the Economic Development Administration of the U.S. Department of Commerce, and the University of Massachusetts.
description: The client for this project is James Leitch, The town administrator for the Town of Adams. In addition, we are working in close conjunction with the Center for Economic Technology (C.E.T.). The purpose of this project is to assist Adams in the creation of a ten year economic action plan, which is only one-third of Adams proposed Comprehensive Sustainability Plan. The Comprehensive Plan is to be completed by the merger of three plans: the 1997 University of Massachusetts Landscape Architecture Studio Report on environmental elements within the Town, our 1998 Economic Action Plan, and a Social Plan, to be developed by the Town. The projects intent is to create an updated business inventory, to inventory and analyze existing conditions in Adams as well as the region, and to make recommendations on short (Less than one year), medium (one to five years), and long (five to ten years) terms. Our inventory of the existing conditions includes over 16 economic activities in the town of Adams and the region. The final step of our project is to assign sustainable characteristics to each of the economic activities found in the existing conditions and recommendations inventory. The characteristics are the key components which connect our report with the Comprehensive Sustainability Report. The end products of this report are three charts detailing the current state of the town and the region, recommendations for ten-year action steps, and sustainable characteristics for each economic activity. In addition, we are providing the town with an updated business inventory of all existing businesses in Adams and recommendations on recruitment of compatible businesses.
title: Histoire : yeying
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: Histoire : xiaoyida de huar
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Thermal dileptons as QCD matter probes at SIS
Creators: name: Seck, Florian
name: Galatyuk, Tetyana
name: Rapp, Ralf
name: Stroth, Joachim
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Electromagnetic radiation is emitted during the whole course of a heavy-ion collision and can escape from the collision zone without further interactions. This makes it an ideal tool to study the properties of hot and dense QCD matter. To model the space-time evolution of the collision at SIS energies a coarse-graining approach is used to convert transport simulations into meaningful temperatures and densities. These parameters serve as input for the determination of the pertinent radiation of thermal dileptons based on an in-medium $ρ$ spectral function that describes available spectra at ultrarelativistic collision energies. The resulting excitation function of the thermal excess radiation provides a baseline for future measurements by the HADES and CBM experiments at GSI/FAIR, and experiments proposed at NICA and J-PARC.
description: 5 pages, 5 figures, contribution to FAIRness 2017 - FAIR next generation scientists - 5th Edition Workshop (May 28, 2017 to June 3, 2017 in Sitges, Spain)
Current status of ALMA EOC polarization commissioning, past, present, and future
Creators: name: Cortes, Paulo
Publisher: name: Zenodo
Year: 2019

description: Here we present the current status of ALMA polarization. We are showing a summary of current capabilities along with new observing modes planned for cycle7. Additionally, we are showing the mid to long term picture of how ALMA polarization will evolve in the coming years and how it will fit with ALMA 2030 vision.
Super-resolution Imaging of the Protoplanetary Disks using Sparse Modeling
Creators: name: Yamaguchi, Masayuki
Publisher: name: Zenodo
Year: 2019

description: High-resolution observations of protoplanetary disks with radio interferometers are crucial for understanding the planet formation process. Recent observations using Atacama Large Millimeter/submillimeter Array (ALMA) have revealed various small-scale structures in disks. In interferometric observations, the observed data are an incomplete set of Fourier components of the radio source image. The image reconstruction is therefore essential in obtaining the images in real space. The CLEAN technique has been widely used, but recently, a new technique using the sparse modeling (SpM) approach is suggested. This technique directly solves a set of undetermined equations and has been shown to behave better than the CLEAN technique based on mock observations with VLBI (Very Long Baseline Interferometry). However, it has never been applied to ALMA-like connected interferometers nor real observational data. In this work, for the first time, the SpM technique is applied to observation al data sets taken by ALMA. We evaluate the performance of the technique by comparing the resulting images with those derived by the CLEAN technique. We use two sets of ALMA archival data at Band 7 ( 350GHz) for the protoplanetary disk around HD 142527. One is taken in the intermediate- baseline array configuration, and the other is in the longer-baseline array configuration. The image resolutions reconstructed from these data sets are different by a factor of 3. We compare images reconstructed using SpM and CLEAN. We find that the SpM technique can successfully reconstruct the overall disk emission. The previously known disk structures appear on both images made by the SpM and CLEAN at its nominal resolutions. Remarkably, the image reconstructed from intermediate-baseline data using the SpM technique matches very well with that obtained from longer-baseline data using the CLEAN technique with the accuracy of 90 % on the image domain. Following up on the success of applying t he new imaging to the data of protoplanetary disks, we analyze the archival ALMA data of snapshot survey of protoplanetary disks, which are not spatially resolved but indicate the existence of an inner hole by investigating the visibility profile as a function of uv-distance. We then apply SpM imaging to reconstruct the images at higher spatial resolution than the nominal resolution and find a ring-like distribution of bright dust continuum emission for several disks.
DSS for best e-commerce selection using AHP-WASPAS and AHP-MOORA methods
Creators: name: Mahendra, Gede Surya
Publisher: name: figshare
Year: 2021
Subjects: subject: 80609 Information Systems Management
subject: FOS: Computer and information sciences
subject: Information Systems
subject: 80605 Decision Support and Group Support Systems
subject: 170202 Decision Making
subject: FOS: Psychology

description: eIQ Consumer Pulse 2019 determines the 6 largest e-commerce in Indonesia, namely Blibli, Bukalapak,JD.id, Lazada Indonesia, Shopee and Tokopedia. This is due to an increase in e-commerce transactions. The COVID-19 pandemic, which emphasizes social distancing and physical distancing, has also played a role in increasing thesetransactions. Indonesia is also predicted to become the market leader in Southeast Asia due to this. On the otherhand, each e-commerce customer has their preferences in choosing e-commerce to use in transactions. Variouscriteria make customers confused due to intense competition between e-commerce companies. DSS is a solutionin choosing the right e-commerce for each customer's preferences. The AHP-WASPAS and AHP-MOORA methodscan be used in calculations for determining favorite e-commerce in Indonesia. The CRISP-DM framework alsohelps in preparing the research flow well. 3 decision-makers are used to provide weighting criteria using AHP. Theresults of this study indicate that the Tokopedia alternative is the best e-commerce, with a preference value of0.8964 for AHP-WASPAS and 0.4245 for AHP-MOORA. The second and third places are Bukalapak and Lazada,respectively. The weighting of the criteria by the decision-maker, the alternative normalization process and thecalculation technique for the preference value have a significant impact on the ranking results.
Prospective Human Validation of Artificial Intelligence Interventions in Cardiology: A Scoping Review
Creators: name: Tian, Nelly
name: Vahabi, Maryam
name: Huang, Steven
name: Moosavi, Amirhossein
name: Motamedivafa, Bahar
name: Rafid Mahmood
name: Sun, Christopher
name: Liu, Peter
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Physical Sciences and Mathematics
subject: Cardiology
subject: Medicine and Health Sciences
subject: Medical Specialties
subject: Computer Sciences
subject: Artificial Intelligence and Robotics

description: Scoping review of current prospectively human validated models in the field of cardiology.
A New Look at Simple Inhomogeneous Chemical Evolution
Creators: name: Oey, M. S.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A rudimentary, one-zone, closed-box model for inhomogeneous chemical evolution is offered as an alternative reference than the Simple model in the limit of no mixing. The metallicity distribution functions (MDFs) of Galactic halo and bulge stars can be matched by varying a single evolutionary parameter, nQ. Q is the filling factor of contaminating regions and n is the number of star-forming generations. Therefore, Q and n have equivalent roles, and combinations of n and Q yield systems with different metallicities at any given age. The model also revises interpretation of observed MDFs. Unevolved systems probe the parent distribution of metal production f(z), for example, the high-metallicity tail of the halo distribution agrees with a power-law f(z).
description: Accepted by ApJ Letters. 4 pages, 4 figures, uses emulateapj.sty. Also available at http://www.stsci.edu/~oey Revised Figures 3 and 4
Models of radial velocities and transit light curves
Creators: name: Díaz, Rodrigo F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Research in extrasolar-planet science is data-driven. With the advent of radial-velocity instruments like HARPS and HARPS-N, and transit space missions like Kepler, our ability to discover and characterise extrasolar planets is no longer limited by instrumental precision but by our ability to model the data accurately. This chapter presents the models that describe radial-velocity measurements and transit light curves. I begin by deriving the solution of the two-body problem and from there, the equations describing the radial velocity of a planet-host star and the distance between star and planet centres, necessary to model transit light curves. Stochastic models are then presented and I delineate how they are used to model complex physical phenomena affecting the exoplanet data sets, such as stellar activity. Finally, I give a brief overview of the processes of Bayesian inference, focussing on the construction of likelihood functions and prior probability distributions. In particular, I describe different methods to specify ignorance priors.
description: Lecture presented at the IVth Azores International Advanced School in Space Sciences on "Asteroseismology and Exoplanets: Listening to the Stars and Searching for New Worlds" (arXiv:1709.00645), which took place in Horta, Azores Islands, Portugal in July 2016
COMPARISON OF SPEED AND AGILITY BETWEEN COLLEGE MEN KABADDI AND KHO-KHO PLAYERS
Creators: name: Kiran Kumar Goud Solthi* & Dr. P. Senthil**
Publisher: name: Zenodo
Year: 2021

description: The purpose of the study was to compare the speed and agility between college men kabaddi and kho-kho players.  To achieve this purpose of the study, sixty men players studying in and around the Colleges in Warangal District, Telangana, India were selected as subjects at random.  Among them, thirty kabaddi players and thirty kho-kho players were selected. The following variables namely speed and agility were selected as criterion variables.  All the subjects of two groups were tested on selected dependent variables by using 50 mts run and shuttle run. The independent ‘t’ ratio was used to analyze the significant difference, if any between groups.  The .05 level of confidence was fixed as the level of significance to test the ‘t’ ratio obtained, which was considered as an appropriate. The results of the study showed that there was a significant difference between college men kabaddi and kho-kho players on speed and agility.
title: Histoire : ye tiane
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Solar Astronomy with ALMA
Creators: name: Wedemeyer, Sven
Publisher: name: Zenodo
Year: 2019

description: Solar observing with ALMA is offered as a non-standard mode since Cycle 4. The requirements for such observations are different from many other observations with ALMA in the sense that the mapped atmospheric layers of the Sun evolve on very short timescales and the primary beam being filled with complex emission. High-cadence (snapshot) imaging is needed for such a dynamic target but is very challenging. The effort and time that went into developing the observing mode seems well justified given that ALMA provides a new complementary view at a part of the solar atmosphere that is still elusive in many aspects. The solar observing campaigns with ALMA are co-ordinated with a number of space-borne and ground-based telescopes covering the UV to IR range. Co-ordinating such strictly simultaneous multi-telescope observations adds another layer of complexity but results in rich data sets covering all layers of the solar atmosphere while probing different properties of the atmospheric gas. Since Cycle 4, the imaging procedures for solar ALMA observations have been significantly improved and science-ready data are being produced. I will give a brief overview over ALMA's diagnostic potential for the Sun and challenges with carrying out solar observations and post-processing the data. First examples for Band 3 and Band 6 data are presented and illustrate the dynamic nature of the solar atmosphere, featuring, among other things, the imprint of magnetic fields and propagating shock waves.
Additional file 3 of Trends in, and factors associated with, HIV infection amongst tuberculosis patients in the era of anti-retroviral therapy: a retrospective study in England, Wales and Northern Ireland
Creators: name: Winter, Joanne
name: Stagg, Helen
name: Smith, Colette
name: Lalor, Maeve
name: Davidson, Jennifer
name: Brown, Alison
name: Brown, James
name: Zenner, Dominik
name: Lipman, Marc
name: Pozniak, Anton
name: Abubakar, Ibrahim
name: Delpech, Valerie
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Table S1 HIV testing amongst TB cases, stratified by ethnicity and year, in England, Wales and Northern Ireland from 2011 to 2014. Table S2 Results from univariable and two multivariable logistic regression models of factors associated with HIV infection, excluding year, in notified tuberculosis cases in England, Wales and Northern Ireland, for the periods 2000–2014 and 2010–2014. Table S3 Sensitivity analyses, excluding TB cases with HIV co-infection where the match between the HIV and tuberculosis datasets was weak, for two multivariable logistic regression models of factors associated with HIV co-infection in notified tuberculosis cases in England, Wales and Northern Ireland, in 2000–2014 and 2010–2014. (DOCX 33 kb)
The MCUCN simulation code for ultracold neutron physics
Creators: name: Zsigmond, G.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Ultracold neutrons (UCN) have very low kinetic energies 0-300 neV, thereby can be stored in specific material or magnetic confinements for many hundreds of seconds. This makes them a very useful tool in probing fundamental symmetries of nature (for instance charge-parity violation by neutron electric dipole moment experiments) and contributing important parameters for the Big Bang nucleosynthesis (neutron lifetime measurements). Improved precision experiments are in construction at new and planned UCN sources around the world. MC simulations play an important role in the optimization of such systems with a large number of parameters, but also in the estimation of systematic effects, in benchmarking of analysis codes, or as part of the analysis. The MCUCN code written at PSI has been extensively used for the optimization of the UCN source optics and in the optimization and analysis of (test) experiments within the nEDM project based at PSI. In this paper we present the main features of MCUCN and interesting benchmark and application examples.
title: Histoire : huangdi de xinzhuang
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
title: Histoire : jianding de xibing
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Perancangan Sistem Pendukung Keputusan Dengan Metode Ahp-Vikor Dalam Penentuan Pengembangan Ekowisata Pedesaan (Decision Support System Design With Ahp-Vikor Method In Determination Of Rural Ecotourism Development)
Creators: name: Mahendra, Gede Surya
Publisher: name: figshare
Year: 2021
Subjects: subject: 80609 Information Systems Management
subject: FOS: Computer and information sciences
subject: Information Systems
subject: 80605 Decision Support and Group Support Systems
subject: 170202 Decision Making
subject: FOS: Psychology

description: Indonesia is famous for its beautiful natural scenery, but there are still ecotourism issues related to developing its potential. There is a need to increase the capacity of the community to be able to develop a tourist village so that an increase in foreign exchange income. The results of the recommendations from the SPK can help stakeholders, and to solve the problem of determining the development of rural ecotourism by using a combination of AHP-VIKOR methods. AHP is a functional hierarchy with input from human perception, and the VIKOR method can select effective and efficient criteria for determining the outcome of decisions with many attributes and several criteria. This study uses 8 criteria, namely Biological, Physical Environment, Culture, Infrastructure, Institutional, Human Resources, Social Society, and Accessibility. The alternative data in this study are 9 data, namely Singapadu Tengah Village, Batubulan Village, Kerta Village, Taro Village, Mas Village, Kedisan Village, Kemenuh Village, Singapadu Kaler Village, and Kendran Village. The assessment of each tourism village data has been validated in previous studies. The results of this study indicate that Batubulan Village with a preference value of 0.96 is a tourism village that can be given assistance in developing rural ecotourism.
 Indonesia terkenal berkat panorama alam indah, namun masih terdapat permasalahan ekowisata terkait dengan pengembangan potensinya. Perlu adanya peningkatan kapasitas masyarakat agar mampu mengembangkan desa wisata sehingga terjadi peningkatan pendapatan devisa. Hasil rekomendasi dari SPK dapat membantu stakeholders, dan untuk memecahkan permasalahan penentuan pegembangan ekowisata pedesaan dengan menggunakan kombinasi metode AHP- VIKOR. AHP adalah hierarki fungsional dengan input dari persepsi manusia, dan metode VIKOR dapat memilih kriteria yang efektif dan efisien untuk menentukan hasil keputusan dengan banyak atribut dan beberapa kriteria. Penelitian ini menggunakan 8 kriteria, yaitu Bio Hayati, Lingkungan Fisik, Budaya, Infrastruktur, Kelembagaan, SDM, Sosial Masyarakat, dan Aksesibilitas. Data alternatif pada penelitian ini sebanyak 9 data, yaitu Desa Singapadu Tengah, Desa Batubulan, Desa Kerta, Desa Taro, Desa Mas, Desa Kedisan, Desa Kemenuh, Desa Singapadu Kaler, dan Desa Kendran. Penilaian dari masing-masing data desa wisata telah divalidasi pada penelitian sebelumnya. Hasil dari penelitian ini menunjukkan Desa Batubulan dengan nilai preferensi 0,96 merupakan desa wisata yang dapat diberikan bantuan pengembangan ekowisata pedesaan.
title: Histoire : GJW
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Role of Inelastic Tunneling through the Barrier in Scanning Tunneling Microscope Experiments on Cuprates
Creators: name: Pilgram, S.
name: Rice, T. M.
name: Sigrist, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The tunneling path between the CuO2-layers in cuprate superconductors and a scanning tunneling microscope tip passes through a barrier made from other oxide layers. This opens up the possibility that inelastic processes in the barrier contribute to the tunneling spectra. Such processes cause one or possibly more peaks in the second derivative current-voltage spectra displaced by phonon energies from the density of states singularity associated with superconductivity. Calculations of inelastic processes generated by apical O-phonons show good qualitative agreement with recent experiments reported by Lee et al.[1]. Further tests to discriminate between these inelastic processes and coupling to planar phonons are proposed.
description: 4 pages, 4 figures
Molecular Gas in Optically Bright QSOs
Creators: name: Yoon, Ilsang
Publisher: name: Zenodo
Year: 2019

description: Testing the evolutionary connection between ULIRGs and QSO hosts has been a key component in the study of both galaxy types and suggests that optically bright QSOs might still reside in molecular gas-rich environments with ongoing star formation. We present here a study of the molecular gas properties of a sample of z < 0.3 luminous Palomar-Green (PG) QSO hosts. This study consists of two components: The first is an IRAM 30m Telescope survey of CO emission from the PG QSO hosts, which shows that a significant fraction (30%) of PG QSO hosts are indeed molecular gas-rich. The second is a pilot ALMA observational study of CO(3-2) emission from 4 PG QSO hosts with 200-500 pc spatial and 10km/s velocity resolution. Our high- resolution ALMA observations reveal a diverse morphology and kinematics of the molecular gas in these hosts and show that the properties of the star formation rate in the high-density region in the vicinity of AGN are similar to that of ULIRGs. However, the current high-resolution ALMA observation misses large scale diffuse faint emission and indicates that lower resolution ALMA observations are required to have a complete picture of the molecular gas in the QSO hosts
title: Histoire : Kamnyu tshupa
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Electronic Supplementary Materials from Interaction of MLE with CLAMP zinc finger is involved in proper MSL proteins binding to chromosomes in Drosophila
Creators: name: Tikhonova, Evgeniya
name: Revel-Muroz, Anastasia
name: Georgiev, Pavel
name: Maksimenko, Oksana
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 3105
subject: Genetics
subject: FOS: Biological sciences
classificationCode: 310509
subject: Genomics
classificationCode: 310803
subject: Plant cell and molecular biology
classificationCode: 310902
subject: Animal cell and molecular biology

description: Dupplementary Figures and Tables
Additional file 1: of Targeting tumour re-wiring by triple blockade of mTORC1, epidermal growth factor, and oestrogen receptor signalling pathways in endocrine-resistant breast cancer
Creators: name: Ribas, Ricardo
name: Pancholi, Sunil
name: Rani, Aradhana
name: Schuster, Eugene
name: Guest, Stephanie
name: Nikitorowicz-Buniak, Joanna
name: Nikiana Simigdala
name: Thornhill, Allan
name: Avogadri-Connors, Francesca
name: Cutler, Richard
name: Alshad Lalani
name: Dowsett, Mitch
name: Johnston, Stephen
name: Lesley-Ann Martin
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Plant Biology
subject: 60506 Virology

description: Figure S1. IC50 values for the anti-proliferative effect of RAD001 and neratinib in relation to the ESR1, ERBB2, and PIK3CA mutational status in endocrine-resistant and -sensitive BC cell lines. (a) Mutational or wt status is depicted in grey and white, respectively, for ESR1, ERBB2, and PIK3CA. (b) Varying degrees of expression of genes encoding proteins targeted by fulvestrant, neratinib, and RAD001 showing heterogeneity in the cell lines tested. (c,d) Cells were treated in the absence or presence of exogenous oestradiol (E2) (0.01Â nM) and doubling concentrations of (c) RAD001 or (d) neratinib. Treatments were performed at day 1 and day 3 after seeding. After 6Â days of treatment, cell viability was analysed using a cell titer-glo assay and IC50 values were plotted. (PDF 156 kb)
title: Histoire : Kamnyu tWji
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Perancangan Metode AHP-MOORA Pada Sistem Pendukung Keputusan Pemilihan Paket Wisata
Creators: name: Mahendra, Gede Surya
Publisher: name: figshare
Year: 2021
Subjects: subject: 80609 Information Systems Management
subject: FOS: Computer and information sciences
subject: Information Systems
subject: 80605 Decision Support and Group Support Systems
subject: 170202 Decision Making
subject: FOS: Psychology

description: Abstract—Wisatawan milenial menjadi pasar menjanjikan untuk pariwisata Indonesia mengingat jumlahnya mencapai lebih dari 300 juta orang secara global hingga 2030, berdasarkan proyeksi Organisasi Pariwisata Dunia (UNWTO). Metode AHP (Analytic Hierarchy Process) adalah suatu teori umum tentang pengukuran yang digunakan untuk menemukan skala rasio, baik dari perbandingan berpasangan yang diskrit maupun berkelanjutan dan MOORA adalah suatu proses yang secara bersamaan dapat mengoptimalkan dua atau lebih yang saling bertentangan pada beberapa kendala. Urgensi dari penelitian ini apabila tidak segera dikerjakan akan menimbulkan persaingan tidak sehat antar sesama pelaku wisata, ketimpangan informasi wisata antara pelaku wisata satu dengan lainnya, munculnya mafia pariwisata, monopoli harga yang tidak sewajarnya, sehingga menimbulkan persepsi yang tidak baik terhadap pariwisata di Bali. Tujuan dari penelitian ini adalah membantu pembuat keputusan memberikan pilihan dan mengambil keputusan yang tepat, akurat dan cepat. Teknik pengumpulan data yang dilakukan dengan cara membaca literatur, dokumen atau arsip yang menjadi subjek penelitian dengan pihak terkait. Subjek penelitian yakni paket wisata di Bali. Berikut disajikan hasil ranking dari nilai rekomendasi paket wisata berdasarkan metode AHP-MOORA. Berdasarkan 38 alternatif yang telah diujikan dengan metode AHP-MOORA, mendapatkan hasil berupa Paket21 merupakan rekomendasi tertinggi dengan nilai preferensi sebesar 0,088, dan Paket10 menjadi peringkat terakhir dengan nilai preferensi 0.022. Hasil penelitian bahwa pemilihan paket wisata menjadi lebih objektif karena user tidak menentukan alternatif yang akan dipilih secara langsung. Diharapkan penelitian ini dapat menambahkan uji singnifikansi, penambahan kriteria dan pengembangan metode pada studi kasus lain.Keywords—AHP ; MOORA ; Paket Wisata ; SPK
Effects of Environment and Energy Injection on Gamma-Ray Burst Afterglows
Creators: name: Dai, Z. G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: There is growing evidence that some long gamma-ray bursts (GRBs) arise from the core collapse of massive stars, and thus it is inevitable that the environments of these GRBs are preburst stellar winds or dense media. We studied, for the first time, the wind model for afterglows based on the Blandford-McKee self-similar solution of a relativistic shock, and suggested that GRB 970616 is an interactor with a stellar wind. We also proposed a dense medium model for some afterglows, e.g., the steepening in the light curve of the R-band afterglow of GRB 990123 may be caused by the adiabatic shock which has evolved from an ultrarelativistic phase to a nonrelativistic phase in a dense medium. We further discussed the dense medium model in more details, and investigated the effects of synchrotron self absorption and energy injection. A shock in a dense medium becomes nonrelativistic rapidly after a short relativistic phase. The afterglow from the shock at the nonrelativistic stage decays more rapidly than at the relativistic stage. Since some models for GRB energy sources predicted that a strongly magnetic millisecond pulsar may be born during GRB formation, we discussed the effect of such a pulsar on the evolution of the nonrelativistic shock through magnetic dipole radiation. We found that in the pulsar energy injection case, the dense medium model fits very well all the observational data of GRB 980519. Recently, we combined the dense medium model with the pulsar energy injection effect to provide a good fit to the optical afterglow data of GRB 000301C.
description: 7 pages, To appear in the proceedings of the First KIAS International Workshop on Astrophysics: Explosive Phenomena in Astrophysical Compact Objects, Seoul, Korea; 24-27 May 2000
SM1 from Backspin in Ruellia ciliatiflora does not maximize seed dispersal range, but provides moderate dispersal range that is robust to launch conditions
Creators: name: Hesse-Withbroe, Joseph L.
name: Whitaker, Dwight L.
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 320203
subject: Clinical microbiology

description: In this document, the equation of motion of a thin, flat, spinning disc moving in a fluid medium is derived using Newtonian mechanics and thin airfoil theory. Additionally, the process of extracting aerodynamic coefficients from videos of flying Ruellia ciliatiflora seeds is outlined.
Motion of a vortex line near the boundary of a semi-infinite uniform condensate
Creators: name: Mason, Peter
name: Berloff, Natalia G.
name: Fetter, Alexander L.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We consider the motion of a vortex in an asymptotically homogeneous condensate bounded by a solid wall where the wave function of the condensate vanishes. For a vortex parallel to the wall, the motion is essentially equivalent to that generated by an image vortex, but the depleted surface layer induces an effective shift in the position of the image compared to the case of a vortex pair in an otherwise uniform flow. Specifically, the velocity of the vortex can be approximated by $U \approx (\hbar/2m)(y_0-\sqrt 2 ξ)^{-1}$, where $y_0$ is the distance from the center of the vortex to the wall, $ξ$ is the healing length of the condensate and $m$ is the mass of the boson.
description: submitted to Phys Rev A
Excitonic Resonance Effects and Davydov Splitting in Circularly Polarized Raman Spectra of Few-Layer WSe2
Creators: name: Kim, Sanghun
name: Kim, Kangwon
name: Lee, Jae-Ung
name: Cheong, Hyeonsik
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Few-layer tungsten diselenide (WSe2) is investigated using circularly polarized Raman spectroscopy with up to eight excitation energies. The main E2g1 and A1g modes near 250 cm-1 appear as a single peak in the Raman spectrum taken without consideration of polarization but are resolved by using circularly polarized Raman scattering. The resonance behaviors of the E2g1 and A1g modes are examined. Firstly, both the E2g1 and A1g modes are enhanced near resonances with the exciton states. The A1g mode exhibits Davydov splitting for trilayers or thicker near some of the exciton resonances. The low-frequency Raman spectra show shear and breathing modes involving rigid vibrations of the layers and also exhibit strong dependence on the excitation energy. An unidentified peak at ~19 cm-1 that does not depend on the number of layers appears near resonance with the B exciton state at 1.96 eV (632.8 nm). The strengths of the intra- and inter-layer interactions are estimated by comparing the mode frequencies and Davydov splitting with the linear chain model, and the contribution of the next-nearest-neighbor interaction to the inter-layer interaction turns out to be about 34% of the nearest-neighbor interaction. Fano resonance is observed for 1.58-eV excitation, and its origin is found to be the interplay between two-phonon scattering and indirect band transition.
description: 45 pages, 20 figures (including Supplementary Information)
Residual Gauge Fixing in Light-Front QCD
Creators: name: Zhang, Wei-Min
name: Harindranth, Avaroth
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Understanding the nontrivial features of light-front QCD is a central goal in current investigations of nonperturbative light-front field theory. We find that, with the choice of light-front gauge with antisymmetric boundary conditions for the field variables, the residual gauge freedom is fixed and the light-front QCD vacuum is trivial. The nontrivial structure in light-front QCD is determined by non-vanishing asymptotic physical (transverse) gauge fields at longitudinal infinity, which are responsible for nonzero topological winding number.
description: 10, OSU-NT-#93-0128
title: ADCO, Deuxième cartulaire ou Grand cartulaire de l'abbaye de Molesme, Cart. 143 (7 H 7), 153 fol, f. 0097v
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/2009
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: Corpus Burgundiae Medii Aevi
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Chartes de la Bourgogne du Moyen Âge

description: Deuxième cartulaire ou Grand cartulaire de l'abbaye de Molesme, Archives départementales de la Côte-d'Or, Cart. 143 (7 H 7), 153 fol, f. 0097v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Deuxième cartulaire ou Grand cartulaire de l'abbaye de Molesme, Archives départementales de la Côte-d'Or, Cart. 143 (7 H 7), 153 fol, f. 0097v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb137389344
description: Provenance: abbaye de Molesme
description: Provenance: http://www.wikidata.org/entity/Q334044
title: Histoire : Kamnyu tWji2
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Air Quality in the Italian Regions
Creators: name: Leogrande, Angelo
Publisher: name: Zenodo
Year: 2024

description: Istat calculates the value of air quality in the Italian regions. The data refers to the Italian regionsbetween 2010 and 2021. Air quality is defined as the percentage of valid measurements higher thanthe reference value for health defined by the WHO (10 μg/m³), out of the total measurements validannual average PM2.5 concentrations for all station types (urban and suburban traffic, urban industrialand urban and suburban, rural background).
title: Histoire : Kamnyu zgo
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2016
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Biased Galaxy Formation And Measurements Of Beta
Creators: name: Berlind, Andreas A.
name: Narayanan, Vijay K.
name: Weinberg, David H.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Measurements of the cosmological density parameter Omega using techniques that exploit the gravity-induced motions of galaxies constrain, in linear perturbation theory, the degenerate parameter combination beta = Omega^{0.6}/b, where the linear bias parameter b is the ratio of the fluctuation amplitudes of the galaxy and mass distributions. However, the relation between the galaxy and mass density fields depends on the complex physics of galaxy formation, and it can in general be non-linear, stochastic, and perhaps non-local. The one-parameter linear bias model is almost certainly oversimplified, which leads to the obvious question: What is the quantity beta that is actually measured by different techniques? To address this question, we estimate beta from galaxy distributions that are constructed by applying a variety of locally biased galaxy formation models to cosmological N-body simulations. We compare the values of beta estimated using three different techniques: a density-density comparison similar to the POTENT analysis, a velocity-velocity comparison similar to the VELMOD analysis, and an anisotropy analysis of the redshift-space power spectrum. In most cases, we find that beta estimated using all three methods is similar to the asymptotic value of Omega^{0.6}/b_{sigma}(R) at large R, where b_{sigma}(R) is the ratio of rms galaxy fluctuations to rms mass fluctuations on scale R. Thus, something close to the conventional interpretation of beta continues to hold even for complex bias models. Moreover, we find that beta estimates made using these three methods should, in principle, agree with each other. It is thus unlikely that non-linear or scale-dependent bias is responsible for the discrepancies that exist among current measurements of beta from different techniques.
description: 26 pages including 9 eps figures. Submitted to ApJ