cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Band-4+5 Receiver Front-End: Idea and Initial Development in East Asia Consortium
Creators: name: Hwang, Yuh-Jing
name: C.-C. Chiong
name: C. Chien
name: C.-T. Ho
name: Ming-Jye Wang
name: T.-J. Chen
name: W.-C. Lu
name: Y.-P. Chang
name: H.-W. Chang
name: C.-P. Chiu
name: Yu Chieh Huang
name: J.-R. Nian
name: C.-C. Wang
name: F.-Y. Hsu
name: P.-A. Chen
name: L.-C. Lu
name: Patrick Koch
name: Bangwon Lee
name: Yue-Fang Kuo
name: Takafumi Kojima
name: Ishii Shun
name: Alvaro Gonzalez
Publisher: name: Zenodo
Year: 2024

description: We propose an upgrade to the ALMA Wideband Sensitivity Upgrade (WSU) by developing a new receiver with increased RF and IF bandwidth. The new receiver will cover the RF frequency of the original Band-4 and Band-5 with continuous frequency tuning over dual polarizations, dual sidebands with instantaneous intermediate frequency (IF) bandwidth up to 16 GHz per sideband and per polarization. Both the SIS-based receiver and HEMT-based receiver schemes are considered. The SIS-based receiver is considered as the baseline design, a sideband separation downconverter with the input fed by the ellipsoidal mirror pairs, corrugated feedhorn and the orthomode transducer form the cold cartridge assembly (CCA). The niobium-based SIS junctions will be fabricated to form mixer chips, and integrated into the mixer blocks with WR-5.44 waveguide 3-dB quadrature hybrid couplers, cryogenic IF low-noise amplifiers, and 2-20 GHz coaxial 3-dB quadrature hybrid couplers to form sideband separating down-converters.
For the HEMT-based receiver scheme, the cryogenic InP HEMT low-noise amplifiers (LNAs) chains cover 125 - 211 GHz operated in 15-K ambient temperature will be the key components, to suppress multiple reflection ripples, cryogenic 2SB mixers are considered.
To avoid the possible interference between LO and IF signals, the LO fundamental frequency are chosen in 24 - 32 GHz, followed by a frequency tripler to form the phase-lock loop with 72 - 96 GHz frequency tuning range.
Future of Observations in the mm/sub-mm Range: GARD's Novel Technologies for ALMA and Beyond
Creators: name: Joint, François
name: C. López
name: A. Pavolotsky
name: D. Meledin
name: I. Lapkin
name: V. Belitsky
name: V. Desmaris
Publisher: name: Zenodo
Year: 2024

description: The ALMA project has revolutionized mm and sub-mm radioastronomy, enhancing our cosmic understanding from planetary formation to the chemistry of the cosmos. GARD builds on this legacy, advancing the next generation of FIR instrumentation to extend technological limits.  This presentation will show several ground-breaking technologies developed at GARD, designed to enhance sensitivity, bandwidth, and the overall observational capabilities of future radio observatories. Central to our advancements is the development of wide-bandwidth SIS mixers, which are engineered to achieve a 56\% fractional bandwidth in the 211-375 GHz frequency range, effectively covering ALMA bands 6 and 7. By incorporating a metallic substrate and employing a metallic finline waveguide-to-substrate transition, these mixers are tailored to optimize the operational bandwidth of the receivers, and effectively addressing the challenges of dielectric losses. We also highlight significant advancements in the IF backend circuitry, featuring the integration of wideband superconducting bias-T alongside IF transformers and hybrid circuits. The hybrid circuits employ parallel plate coupled line couplers, enabling operation across a broad frequency range from 4 to 20 GHz. Finally, we showcase a quasi-optic, scalable dichroic mirror, initially designed for the Q-band (35-55 GHz) and potentially extendable to THz frequencies. We are exploring 3D printing technology for its manufacturing.
Predigt zur Eucharistiefeier mit der Edith-Stein-Gesellschaft beim Katholikentag in Regensburg am 31. Mai 2014
Creators: name: Wiesemann, Karl-Heinz
Publisher: name: Edith Stein Jahrbuch
Year: 2025

description: 1647268346
description: Edith Stein Jahrbuch, V. 21 (2015): Edith Stein Jahrbuch, Band 21
Robust temperatures and luminosities of cores in 1000 high-mass cluster-forming regions with ALMAGAL
Creators: name: Jones, Beth
name: Peter Schilke
name: Gary Fuller
name: Georgie Stroud
name: Tianwei Zhang
name: Thomas Möller
name: Álvaro Sánchez-Monge
name: Judith Beck
name: Eleonore Dann
name: The ALMAGAL Collaboration
name: Sergio Molinari
name: Cara Battersby
name: Paul Ho
Publisher: name: Zenodo
Year: 2024

description: In this contribution, I will show the intricate picture at 50 au of the IRAS 4A2 protostar within the ALMA LP FAUST. This protostar hosts a compact (below 100 au) hot (above 100 K) dense (above 10$^7$ cm$^{-3}$) region rich in prebiotic complex organic molecules, and launches a large bipolar jet. The combination of high angular (scales of 50 au) and spectral resolution (below 0.5 km/s) observations with multiline radiative transfer analysis, revealed the various component of the inner regions of the system: a stratified chemical and physical structure and a wide disk wind.
Complex chemistry during the early stages of star formation
Creators: name: Jørgensen, Jes
Publisher: name: Zenodo
Year: 2024

description: The emergence of complex organic molecules in the interstellar medium is a fundamental puzzle of astrochemistry. Targeted observations with ALMA have opened the door to high-sensitivity spectral surveys over wide bandwidths to elucidate the chemical complexity of young stars in a systematic manner. Concerted efforts along these lines are needed to reveal the complex organic inventories and isotopic ratios depending on the physical environment and evolutionary past. Ultimately they will can address how much diversity in organic inventories we can expect for emerging planetary systems. In this talk I will present the first results of our ALMA Large Program ``Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS)''. The aim of the program is to perform unbiased line surveys of 11 nearby Solar-type protostars. The targeted protostars are known hosts of complex organic molecules and sample different natal environments and evolutionary stages thereby starting to address the relative importance of ``nature'' versus ``nurture'' for the resulting protostellar chemistry. I will discuss the potential for extending such studies to explore much wider parts of parameter space after the Wideband Sensitivity Upgrade as well as some of the challenges that must be tackled with such rich datasets.
Tables S1-S2, Figures S1-S6 from Home and hub: pet trade and traditional medicine impact reptile populations in source locations and destinations
Creators: name: Dufour, Pauline C.
name: Miot, Elliott F.
name: So, Tsz Chun
name: Tang, Shun Long
name: Jones, Emily E.
name: Kong, Tsz Ching
name: Yuan, Felix Landry
name: Sung, Yik-Hei
name: Dingle, Caroline
name: Bonebrake, Timothy C.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Environmental Science
subject: Ecology
subject: FOS: Biological sciences

description: Supplemental tables and figures with details regarding specimens used in the study, shop survey results, and details of the stable isotope analysis results.
Summary of wide-band receiver optics studies at NAOJ over the last decade
Creators: name: Kaneko, Keiko
Publisher: name: Zenodo
Year: 2024

description: The WSU will come with a large increase in the overall data-rate. The data volume will pose substantial challenges for astronomers to access, to recalibrate, reimage, and recombine the data according to their needs as well as to analyze the products. We describe the coming and planed developments for the ALMA Science Archive to allow astronomers to better deal with the WSU ALMA data and thus maximise the science return for the observatory.
ALMA WSU: Data Processing Challenges and Opportunities
Creators: name: Kepley, Amanda
Publisher: name: Zenodo
Year: 2024

description: The ALMA Wideband Sensitivity Upgrade (WSU) will increase the maximum number of channels ALMA is capable of producing from 15,000 to 1.2 million. This increase in the aggregate number of channels presents new challenges for processing ALMA data. In this talk, I will present estimates of the predicted distribution of WSU data properties -- including data rates, visibility data volumes, and product sizes -- based on extrapolations of current ALMA use patterns and compare them to the data properties ALMA is capable of producing today. I will also outline the current challenges with ALMA data processing and discuss ways to address these challenges in the WSU era
Black-body radiation for twist-deformed space-time
Creators: name: Daszkiewicz, Marcin
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this article we formally investigate the impact of twisted space-time on black-body radiation phenomena, i.e. we derive the $θ$-deformed Planck distribution function as well as we perform its numerical integration to the $θ$-deformed total radiation energy. In such a way we indicate that the space-time noncommutativity very strongly damps the black-body radiation process. Besides we provide for small parameter $θ$ the twisted counterparts of Rayleigh-Jeans and Wien distributions respectively.
description: 11 pages, 4 figures, Latex source. arXiv admin note: substantial text overlap with arXiv:1412.5922, arXiv:1302.0827
Effects of inter-group violence on children’s and adolescents’ morality
Creators: name: Parra, Maria
Publisher: name: University of Chicago
Year: 2022
Subjects: subject: morality
subject: intergroup violence
subject: children and adolescents

description: This paper systematically reviews the empirical literature on the morality of children and adolescents exposed to inter-group violence and examine whether there is sufficient evidence to claim that exposure to this form of violence exerts an effect and in what direction. The literature review was guided by the PRISMA standards for systematic reviews to search APA PsycNET, PubMed, Web of Science and Google Scholar. Twenty-three empirical articles from 11 countries around the world were retrieved and analyzed for sociodemographic characteristics of the population, characteristics of the conflict and violence, research design, moral outcomes evaluated and effects reported for each, and main findings of the study. Opinion articles, reviews, unpublished papers, dissertations and qualitative study were excluded. Among the findings, most studies found an increase on aggressive behavior, hostility, violence, distribution of resources, and retaliation. While there are mixed results for empathy and pro-sociality. Most studies measured aggressive behavior or pro-social behavior and relied on self-reports - few used behavioral tasks. Also, 60% of the studies were conducted in an ongoing conflict and only 1 study measured long-term effects (10 years after the conflict). Overall, most studies suggest that there is an effect of inter-group violence exposure during childhood and adolescence on moralityand that it is usually negative. However, the few results showing positive outcomes, no effects, and mediators and moderators, also point towards the conclusion that whether the violence of inter-group conflicts exerts an effect and in what direction, depends on other variables. Avenues for future research are delineated.
Detecting Corrosion Using Unsupervised Learning
Creators: name: Atwakyire
name: , Chen
name: Siyuan
Publisher: name: Zenodo
Year: 2023
Subjects: Clustering
Machine Learning
Corrosion

description: The code shows an in-depth analysis of corrosion-related data through the application of machine learning, with a primary focus on clustering algorithms. The script begins by loading essential libraries, setting up a robust warning handling system, and importing corrosion data from an Excel file. Data preprocessing follows, involving initial exploration and handling of missing values through median replacement. The core of the script revolves around machine learning clustering techniques. It starts by normalizing features and determining optimal clusters using the K-Means algorithm, visualizing results through an elbow curve and 3D plots. The script then explores alternative clustering methods, including Hierarchical Clustering, and Affinity Propagation and evaluates their performance. The script concludes with comprehensive results and visualization sections, presenting tabular and graphical comparisons of clustering algorithms based on metrics such as Silhouette Score, Calinski-Harabasz Index, and Davies-Bouldin Index. The distribution of variables within clusters is visualized, and variable similarity within a specific cluster compared to the overall dataset is analyzed using pair plots, heatmaps, and distribution plots. Overall, this script offers a detailed exploration of corrosion data, providing valuable insights into the relationships between variables within distinct clusters.
GPU Spectrometer for the Total Power Array
Creators: name: Kim, Jongsoo
name: Jongsuk Hong
name: Won-Kee Park
name: Heesun Yoon
name: Manabu Watanabe
name: Scott Zang
name: Susumu Nakayama
name: Makoto Shizugami
name: Isaac Goicovich
name: Shinya Ikebe
name: Takeshi Kamazaki
Publisher: name: Zenodo
Year: 2024

description: The rapid advancement in GPU (Graphic Processing Unit) technology, driven by the growing needs of artificial intelligence, has paved the way for significant improvements in astronomical data processing.  The launch of the NVIDIA Grace Hopper superchip is a major breakthrough. It speeds up the transfer of data from antennas to GPU memory and greatly increases processing power. In light of these advancements, we propose the development of a new Total Power GPU Spectrometer (TPGS) to replace the existing ACA Spectrometer (ACAS) for the upcoming WSU phase. The TPGS is designed to produce full polarization products by processing digitized signals from each of the four TP antennas. It will play a crucial role in the calibration of pointing and focus for the antennas, thanks to its ability to generate cross-correlation products. Utilizing a FFX (Filter-FFT-Multiplication) architecture, the TPGS methodically processes data on a per spectral window basis, accommodating digitized signals across a vast 20 GHz bandwidth for each polarization, sideband, and antenna. This system uses a polyphase filter to isolate a specific spectral window, and then applies a Fast Fourier Transform (FFT) to the filtered signal to calculate auto-correlation. This design's flexibility in selecting spectral window bandwidths and FFT sizes ensures it meets the varied bandwidths and spectral resolutions for each spectral window.
Equine Polyclonal Antibodies Immunotherapy Against Covid-19/SARS-COV2-VOC
Creators: name: Belledant, A.
name: Luckowiak, J.
name: Delgado, R.
name: Rodriguez, E.
name: Veas, F.
Publisher: name: Zenodo
Year: 2022
Subjects: SARS-COV-2

description: The highly contagious SARS-CoV-2 virus has generated an unprecedented pandemic with global dramatic health and socioeconomic consequences. Despite the progression of the global use of efficient vaccines, an increased transmissibility of variants of concern (VOC) is predominantly observed. Besides effective vaccination campaigns and new approved antivirals, hundreds of thousand patients have still been admitted to ICU in Europe in the first half of 2022. Passive immunotherapies based on monoclonal antibodies have shown a drop of neutralization potency against VoCs. A polyclonal approach might be effective to neutralize fast-evolving VoCs and prevent worsening medical conditions for hospitalized patients at risks. The main objective of the the European EPIC-CROWN-2 consortium is to rapidly assess, in multicentric clinical trials (phase IIa/b) an EMA-authorized antiviral immunotherapy based on potent and broad equine neutralizing anti-SARS-CoV-2 polyclonal F(ab')2 antibodies in COVID-19 patients, including VOC carriers.
On $C_J$ and $C_T$ in the Gross-Neveu and $O(N)$ Models
Creators: name: Diab, Kenan
name: Fei, Lin
name: Giombi, Simone
name: Klebanov, Igor R.
name: Tarnopolsky, Grigory
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We apply large $N$ diagrammatic techniques for theories with double-trace interactions to the leading corrections to $C_J$, the coefficient of a conserved current two-point function, and $C_T$, the coefficient of the stress-energy tensor two-point function. We study in detail two famous conformal field theories in continuous dimensions, the scalar $O(N)$ model and the Gross-Neveu model. For the $O(N)$ model, where the answers for the leading large $N$ corrections to $C_J$ and $C_T$ were derived long ago using analytic bootstrap, we show that the diagrammatic approach reproduces them correctly. We also carry out a new perturbative test of these results using the $O(N)$ symmetric cubic scalar theory in $6-ε$ dimensions. We go on to apply the diagrammatic method to the Gross-Neveu model, finding explicit formulae for the leading corrections to $C_J$ and $C_T$ as a function of dimension. We check these large $N$ results using regular perturbation theory for the Gross-Neveu model in $2+ε$ dimensions and the Gross-Neveu-Yukawa model in $4-ε$ dimensions. For small values of $N$, we use Pade approximants based on the $4-ε$ and $2+ε$ expansions to estimate the values of $C_J$ and $C_T$ in $d=3$. For the $O(N)$ model our estimates are close to those found using the conformal bootstrap. For the GN model, our estimates suggest that, even when $N$ is small, $C_T$ differs by no more than $2\%$ from that in the theory of free fermions. We find that the inequality $C_T^{\textrm{UV}} > C_T^{\textrm{IR}}$ applies both to the GN and the scalar $O(N)$ models in $d=3$.
description: 62 pages, 34 figures. v2: minor improvements, references added
Quantum phase diagram of $J_1-J_2$ Heisenberg $S=1/2$ antiferromagnet in honeycomb lattice: a modified spin wave study
Creators: name: Ghorbani, Elaheh
name: Shahbazi, Farhad
name: Mosadeq, Hamid
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Using modified spin wave (MSW) method, we study the $J_1-J_2$ Heisenberg model with first and second neighbor antiferromagnetic exchange interactions. For symmetric $S=1/2$ model, with the same couplings for all the equivalent neighbors, we find three phase in terms of frustration parameter ${\barα=J_2/J_1}$: (1) a commensurate collinear ordering with staggered magnetization (N{é}el.I state) for $0\leq{\barα}\lesssim 0.207$ , (2) a magnetically gapped disordered state for $0.207\lesssim{\barα}\lesssim 0.369$, preserving all the symmetries of the Hamiltonian and lattice, hence by definition is a quantum spin liquid (QSL) state and (3) a commensurate collinear ordering in which two out of three nearest neighbor magnetizations are antiparallel and the remaining pair are parallel (N{é}el.II state), for $0.396\lesssim{\barα}\leq 1$. We also explore the phase diagram of distorted $J_1-J_2$ model with $S=1/2$. Distortion is introduced as an inequality of one nearest neighbor coupling with the other two. This yields a richer phase diagram by the appearance of a new gapped QSL, a gapless QSL and also a valence bond crystal (VBC) phase in addition to the previously three phases found for undistorted model.
What are we doing and what do we need to do: the roadmap of OA in Spanish University Presses
Creators: name: De Páiz, María Isabel
name: López Carreño, Rosana
Publisher: name: Zenodo
Year: 2023

description: In Spain the publishing of Journals in Universities Presses is mainly done using Diamond Open Access. At the time the Universities’ Governing bodies signed the 2003 Berlin Declaration on Open Access, their Universities Presses began to study, work and change their methods and workflow[1]. After CSIC did, on 22th octubre 2009, Salamanca University Press open its OJS: previously it digitised all its previously published journals for their publication in the platform. Nowadays, a big number of our repositories are in the first 160 ranking of global repositories as Ranking Web show (Isidro Aguillo, Laboratorio de Cibermetría, CSIC): https://repositories.webometrics.info/en/portals: Rank 67, Revistas científicas de la Universidad de Murcia, with 27.100 items o documentos Rank 86: Revistas Universidad de Navarra, 17.600 Rank 100: Revistas Científicas Universidad de Granada, 12.300 Rank 109: EUSAL Revistas Universidad de Salamanca, 9.540 Rank 101: Revistas Científicas de la Universitat de Barcelona RCUB, 11.500 Rank 110: Revistas Universidad Pontificia Comillas ICAI ICADE, 9.090 Rank 147: Portal de Revistas de la UNED, 3.890 Rank 151: Revistas electrónicas de la Universidad de Jaén, 3.440 Rank 152: Revistes Digitals ReDi Universitat Autònoma de Barcelona, 3.370 Rank 153: PoliPapers Universitat Politécnica de Valencia, 3.310 As of today, Spanish University Presses have not any government support, or any political plan or strategy regarding about Open Science. In fact, all Departments of Spanish administration (central, autonomical or local) largely ignore what Spain's University Presses do and what are their problems. The principal focus of this poster is to provide data about journal production (for example, how many offers XML-JATS), rights policies, ethics requirements, but above all, our sostenibility. Also to explain we need in order to ensure that open science becomes a common and shared practice, encouraged by the whole international ecosystem of higher education, research and innovation. [1] The first University to sign the Berlin Declarations was Universitat Jaume I, on 10th of october 2005 (nº 136). Its repository: http://repositori.uji.es/xmlui/handle/10234/10
description: This poster was presented during the 4th Open Science Fair (25-27 September, Madrid, Spain)
Supplementary material from Foot shape is related to load-induced shape deformations, but neither are good predictors of plantar soft tissue stiffness
Creators: name: Schuster, Robert W.
name: Cresswell, Andrew G.
name: Kelly, Luke A.
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: 110601 Biomechanics
subject: FOS: Health sciences

description: This file contains a detailed description of the nerve block application for plantar soft tissue measurements, a detailed discussion of the measured plantar aponeurosis stiffness values and a link to the foot shape and deformation principal component animations.
ALMA Band 8 version2 receiver upgrade project
Creators: name: Kojima, Takafumi
name: Tetsuhiro Minamidani
name: Ryo Sakai
name: Hiroaki Imada
name: Keiko Kaneko
name: Sho Masui
name: Kazunori Uemizu
name: Kazumasa Makise
name: Akihira Miyachi
name: Shohei Ezaki
name: Tomonori Tamura
Publisher: name: Zenodo
Year: 2024

description: We have initiated an upgrade project for the existing Atacama Large Millimeter/submillimeter Array (ALMA) Band 8 (radio frequency: 385-500 GHz) receiver cartridge with a substantially improved second-generation version, referred to here as ``Band 8v''. This project is originated from significant advances in receiver technologies in the last decade, such as high critical current density superconductor-insulator-superconductor (SIS) mixers, wideband cryogenic low-noise amplifier, and high-performance waveguide components. These will allow us to realize a fundamentally re-designed receiver to cover a substantially wider intermediate frequency (IF) band with lower and flatter receiver noise temperature.  In addition to those goals, lessons learned through the development, operation, and maintenance of the current ALMA Band 8 receiver cartridges will be appropriately addressed through this upgrade. In addition to those goals, lessons learned through the development, operation, and maintenance of the current ALMA Band 8 receiver cartridges will be appropriately addressed through this upgrade.
Appendices from Reservoir population ecology, viral evolution and the risk of emerging infectious disease
Creators: name: Nuismer, Scott L.
name: Basinski, Andrew J.
name: Schreiner, Courtney
name: Whitlock, Alexander
name: Remien, Christopher H.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Health Care
subject: Diseases
subject: 111706 Epidemiology
subject: FOS: Health sciences

description: The ecology and life history of wild animals influences their potential to harbour infectious disease. This observation has motivated studies identifying empirical relationships between traits of wild animals and historical patterns of spillover and emergence into humans. Although these studies have identified compelling broad-scale patterns, they are generally agnostic with respect to underlying mechanisms. Here, we develop mathematical models that couple reservoir population ecology with viral epidemiology and evolution to clarify existing verbal arguments and pinpoint the conditions that favour spillover and emergence. Our results support the idea that average lifespan influences the likelihood of an animal serving as a reservoir for human infectious disease. At the same time, however, our results show that the magnitude of this effect is sensitive to the rate of viral mutation. Our results also demonstrate that viral pathogens causing persistent infections or a transient immune response within the reservoir are more likely to fuel emergence. Genetically explicit stochastic simulations enrich these mathematical results by identifying relationships between the genetic basis of transmission and the risk of spillover and emergence. Together, our results clarify the scope of applicability for existing hypotheses and refine our understanding of emergence risk.
Individual Treatment Effect Prediction for ALS Patients
Creators: name: Seibold, Heidi
name: Zeileis, Achim
name: Hothorn, Torsten
Publisher: name: arXiv
Year: 2016
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: A treatment for a complicated disease may be helpful for some but not all patients, which makes predicting the treatment effect for new patients important yet challenging. Here we develop a method for predicting the treatment effect based on patient char- acteristics and use it for predicting the effect of the only drug (Riluzole) approved for treating Amyotrophic Lateral Sclerosis (ALS). Our proposed method of model-based ran- dom forests detects similarities in the treatment effect among patients and on this basis computes personalised models for new patients. The entire procedure focuses on a base model, which usually contains the treatment indicator as a single covariate and takes the survival time or a health or treatment success measurement as primary outcome. This base model is used both to grow the model-based trees within the forest, in which the patient characteristics that interact with the treatment are split variables, and to com- pute the personalised models, in which the similarity measurements enter as weights. We applied the personalised models using data from several clinical trials for ALS from the PRO-ACT database. Our results indicate that some ALS patients benefit more from the drug Riluzole than others. Our method allows shifting from stratified medicine to person- alised medicine and can also be used in assessing the treatment effect for other diseases studied in a clinical trial.
Menschenwürde im Licht der Phänomenologie Edith Steins
Creators: name: Lebech, Mette
Publisher: name: Edith Stein Jahrbuch
Year: 2025

description: 1647268281
description: Edith Stein Jahrbuch, V. 21 (2015): Edith Stein Jahrbuch, Band 21
Detailed NLTE abundance analysis of 20 Nuclear Stellar Cluster/Disk stars
Creators: name: Thorsbro, Brian
Publisher: name: Zenodo
Year: 2023

description: We present a detailed NLTE abundance analysis of 20 stars in the Nuclear Star Cluster and the Nuclear Stellar Disk using recently calculated NLTE departure coefficients. We compare the to results with an equivalent analysis of stars located in the disk further out in the Galaxy. Similar to previously analysed and published silicon abundances for the same set of stars, we show that even for elements such as calcium and titanium there is a significant difference between stars located in the Nuclear Stellar Cluster/Disk and stars located further out in the Milky Way disk.
Design and experiment of electronic speckle shearing phase-shifting pattern interferometer
Creators: name: Xu, Tianhua
name: Jing, Chao
name: Jing, Wencai
name: Zhang, Hongxia
name: Jia, Dagong
name: Zhang, Yimo
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Optics (physics.optics)
subject: FOS: Physical sciences
subject: 78A55

description: An electronic speckle shearing phase-shifting pattern interferometer (ESSPPI) based on Michelson interferometer was based in this paper. A rotatable mirror driven by a step motor in one of its reflective arm is used to generate an adjustable shearing and the mirror driven by piezoelectric transducer (PZT) in the other reflective arm was used to realize phaseshifting. In the experiments, the deformation of an aluminum plate with the same extern-force on different positions and different forces on the same position is measured. Meanwhile, the phase distribution and phase-unwrap image of the aluminum plate with the extern-force on its center position is obtained by the four-step phase-shifting method.
description: 3 pages
The Star-formation History and Accretion-Disk Fraction Among the K-Type Members of the Scorpius-Centaurus OB Association
Creators: name: Pecaut, Mark J.
name: Mamajek, Eric E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present results of a spectroscopic survey for new K- and M-type members of Scorpius-Centaurus (Sco-Cen), the nearest OB Association (~100-200 pc). Using an X-ray, proper motion and color-magnitude selected sample, we obtained spectra for 361 stars, for which we report spectral classifications and Li and Halpha equivalent widths. We identified 156 new members of Sco-Cen, and recovered 51 previously published members. We have combined these with previously known members to form a sample of 493 solar-mass (~0.7-1.3 Msun) members of Sco-Cen. We investigated the star-formation history of this sample, and re-assessed the ages of the massive main-sequence turn-off and the G-type members in all three subgroups. We performed a census for circumstellar disks in our sample using WISE infrared data and find a protoplanetary disk fraction for K-type stars of 4.4$^{+1.6}_{-0.9}$% for Upper Centaurus-Lupus and Lower Centaurus-Crux at ~16 Myr and 9.0$^{+4.0}_{-2.2}$% for Upper Scorpius at ~10 Myr. These data are consistent with a protoplanetary disk e-folding timescale of ~4-5 Myr for ~1 Msun stars, twice that previously quoted (Mamajek 2009), but consistent with the Bell et al. revised age scale of young clusters. Finally, we construct an age map of Scorpius-Centaurus which clearly reveals substructure consisting of concentrations of younger and older stars. We find evidence for strong age gradients within all three subgroups. None of the subgroups are consistent with being simple, coeval populations which formed in single bursts, but likely represents a multitude of smaller star formation episodes of hundreds to tens of stars each.
description: Accepted for publication in MNRAS; 32 pages, 16 figures, 13 tables; Electronic tables to be available in Vizier, temporarily available for download at http://www.pas.rochester.edu/~mpecaut/tmp/
„Wohl zu beachten: nicht Aristoteles allein, auch Plato und Augustin“ (3. Teil)
Creators: name: Urban, Bernd
Publisher: name: Edith Stein Jahrbuch
Year: 2025

description: 1647268265
description: Edith Stein Jahrbuch, V. 21 (2015): Edith Stein Jahrbuch, Band 21
Interfacial spin-orbit torque without bulk spin-orbit coupling
Creators: name: Emori, Satoru
name: Nan, Tianxiang
name: Belkessam, Amine M.
name: Wang, Xinjun
name: Matyushov, Alexei D.
name: Babroski, Christopher J.
name: Gao, Yuan
name: Lin, Hwaider
name: Sun, Nian X.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: An electric current in the presence of spin-orbit coupling can generate a spin accumulation that exerts torques on a nearby magnetization. We demonstrate that, even in the absence of materials with strong bulk spin-orbit coupling, a torque can arise solely due to interfacial spin-orbit coupling, namely Rashba-Eldestein effects at metal/insulator interfaces. In magnetically soft NiFe sandwiched between a weak spin-orbit metal (Ti) and insulator (Al$_2$O$_3$), this torque appears as an effective field, which is significantly larger than the Oersted field and sensitive to insertion of an additional layer between NiFe and Al$_2$O$_3$. Our findings point to new routes for tuning spin-orbit torques by engineering interfacial electric dipoles.
Inverse correlation between quasiparticle mass and Tc in a cuprate high-Tc superconductor
Creators: name: Putzke, C.
name: Malone, L.
name: Badoux, S.
name: Vignolle, B.
name: Vignolles, D.
name: Tabis, W.
name: Walmsley, P.
name: Bird, M.
name: Hussey, N. E.
name: Proust, C.
name: Carrington, A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Close to a zero temperature transition between ordered and disordered electronic phases, quantum fluctuations can lead to a strong enhancement of the electron mass and to the emergence of competing phases such as superconductivity. A correlation between the existence of such a quantum phase transition and superconductivity is quite well established in some heavy fermion and iron-based superconductors and there have been suggestions that high temperature superconductivity in the copper oxide materials (cuprates) may also be driven by the same mechanism. Close to optimal doping, where the superconducting transition temperature $T_c$ is maximum in the cuprates, two different phases are known to compete with superconductivity: a poorly understood pseudogap phase and a charge ordered phase. Recent experiments have shown a strong increase in quasiparticle mass $m^*$ in the cuprate YBa$_2$Cu$_3$O$_{7-δ}$ as optimal doping is approached suggesting that quantum fluctuations of the charge ordered phase may be responsible for the high-$T_c$ superconductivity. We have tested the robustness of this correlation between $m^*$ and $T_c$ by performing quantum oscillation studies on the stoichiometric compound YBa$_2$Cu$_4$O$_8$ under hydrostatic pressure. In contrast to the results for YBa$_2$Cu$_3$O$_{7-δ}$, we find that in YBa$_2$Cu$_4$O$_8$ the mass decreases as $T_c$ increases under pressure. This inverse correlation between $m^*$ and $T_c$ suggests that quantum fluctuations of the charge order enhance $m^*$ but do not enhance $T_c$.
description: 11 pages includes supplementary information
Revealing the gas properties of the most typical planet-forming disks
Creators: name: Kurtovic, Nicolas
Publisher: name: Zenodo
Year: 2024

description: Planets are formed from the gas and dust in disks around young stars, both of which will benefit from the Wideband Sensitivity Upgrade. However, the largest limitation to analyzing the emission from these disks will continue to be the limited angular resolution and image reconstruction methods. In this talk, I will present how visibility-based techniques can efficiently recover the gas morphology and brightness temperature in compact and faint disks, where image-based techniques are unable to operate. These techniques will be crucial to optimize the recovery of information of the improved spectral scan capabilities. These results are part of Kurtovic \& Pinilla
Electromagnetic Counterparts to Black Hole Mergers Detected by LIGO
Creators: name: Loeb, Abraham
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Mergers of stellar-mass black holes (BHs), such as GW150914 observed by LIGO, are not expected to have electromagnetic counterparts. However, the Fermi GBM detector identified of a gamma-ray transient 0.4 s after the gravitational wave (GW) signal GW150914 with consistent sky localization. I show that the two signals might be related if the BH binary detected by LIGO originated from two clumps in a dumbbell configuration that formed when the core of a rapidly rotating massive star collapsed. In that case, the BH binary merger was followed by a gamma-ray burst (GRB) from a jet that originated in the accretion flow around the remnant BH. A future detection of a GRB afterglow could be used to determine the redshift and precise localization of the source. A population of standard GW sirens with GRB redshifts would provide a new approach for precise measurements of cosmological distances as a function of redshift.
description: 4 pages, accepted for publication in ApJ Letters
ALMA PI science with subarrays - Making ALMA observations post WSU even more efficient
Creators: name: König, Sabine
name: Carmen Toribio
name: Sebastien Muller
name: Daniel Tafoya
name: Sabine König
name: Tobia Carozzi
name: Ignacio Toledo
name: Sven Wedemeyer
name: Ivan Martí-Vidal
Publisher: name: Zenodo
Year: 2024

description: The Wide Sensitivity Upgrade (WSU) project for ALMA will increase the sensitivity of observations with larger instantaneous spectral bandwidths, improved receiver performances, and better correlator quantization. However, certain aspects of ALMA observations post WSU could even further be improved by implementing a sub-array observing mode for PI science - simultaneous observations using subgroups of antennas of the ALMA main array. The impact of such an observing mode would be particularly strong on multi-wavelength studies, the investigation of transient phenomena, and time domain astronomy, as well as coordinated observations with other facilities. This poster will present some typical science cases and specific programs that could benefit from a PI sub-array observing mode, with a potential for further increasing the efficiency of ALMA observations in the post-WSU era.
The 2X-HI disks of spiral galaxies
Creators: name: Koribalski, B. S.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The outskirts of galaxies - especially the very extended HI disks of galaxies - are strongly affected by their local environment. I highlight the giant 2X-HI disks of nearby galaxies (M 83, NGC 3621, and NGC 1512), studied as part of the Local Volume HI Survey (LVHIS), their kinematics and relation to XUV disks, signatures of tidal interactions and accretion events, the MHI - DHI relation as well as the formation of tidal dwarf galaxies. - Using multi-wavelength data, I create 3D visualisations of the gas and stars in galaxies, with the shape of their warped disks obtained through kinematic modelling of their HI velocity fields.
description: 3 pages, incl. one page of colour figures; Proceedings of the IAU Symposium No. 321, 2016, Formation and Evolution of Galaxy Outskirts, eds. A. Gil de Paz, J. Knapen, & J. Lee
Science drivers and technical considerations for an ALMA  Focal Plane Array
Creators: name: Magdis, Georgios
name: Francesca Rizzo
Publisher: name: Zenodo
Year: 2024

description: The deployment of focal plane arrays (FPAs) is a very promising approach/upgrade that can unlock ALMA's full scientific potential by exploiting its unique sensitivity and resolving capabilities to their maximum, while increasing its mapping speed and efficiency. In this talk I will discuss the main science drivers, the scientific impact and the technical considerations for this endeavor that we are currently putting together as part of the  recently commenced 3-years ALMA development study: ``Scientific opportunities and technical considerations for the development of ALMA focal plane arrays''.
Modelling and Verifying the AODV Routing Protocol
Creators: name: van Glabbeek, Rob
name: Höfner, Peter
name: Portmann, Marius
name: Tan, Wee Lum
Publisher: name: arXiv
Year: 2015
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences
subject: C.2.2; F.3.1; F.3.2

description: This paper presents a formal specification of the Ad hoc On-Demand Distance Vector (AODV) routing protocol using AWN (Algebra for Wireless Networks), a recent process algebra which has been tailored for the modelling of Mobile Ad Hoc Networks and Wireless Mesh Network protocols. Our formalisation models the exact details of the core functionality of AODV, such as route discovery, route maintenance and error handling. We demonstrate how AWN can be used to reason about critical protocol properties by providing detailed proofs of loop freedom and route correctness.
description: arXiv admin note: substantial text overlap with arXiv:1312.7645
Thermoelectrics with Coulomb coupled quantum dots
Creators: name: Thierschmann, Holger
name: Sánchez, Rafael
name: Sothmann, Björn
name: Buhmann, Hartmut
name: Molenkamp, Laurens W.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this article we review the thermoelectric properties of three terminal devices with Coulomb coupled quantum dots (QDs) as observed in recent experiments [1,2]. The system we consider consists of two Coulomb-blockade QDs one of which can exchange electrons with only a single reservoir (heat reservoir) while the other dot is tunnel coupled to two reservoirs at a lower temperature (conductor). The heat reservoir and the conductor interact only via the Coulomb-coupling of the quantum dots. It has been found that two regimes have to be considered. In the first one heat flow between the two systems is small. In this regime thermally driven occupation fluctuations of the hot QD modify the transport properties of the conductor system. This leads to an effect called thermal gating. Experiment have shown how this can be used to control charge flow in the conductor by means of temperature in a remote reservoir. We further substantiate the observations with model calculations and implications for the realization of an all-thermal transistor are discussed. In the second regime, heat flow between the two systems is relevant. Here the system works as a nano scale heat engine, as proposed recently [3]. We review the conceptual idea, its experimental realization and the novel features arising in this new kind of thermoelectric device such as decoupling of heat and charge flow.
description: 18 pages, 10 figures, submitted to Comptes Rendue Physique
Supplementary Materials for: Niche construction through a Goldilocks principle maximizes fitness for a nest-sharing brood parasite
Creators: name: Antonson, Nicholas D.
name: Schelsky, Wendy M.
name: Tolman, Deryk
name: Kilner, Rebecca M.
name: Hauber, Mark E.
Publisher: name: The Royal Society
Year: 2022
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: 60801 Animal Behaviour

description: This pdf includes: Supplementary Materials and Methods, Supplementary Results Supplementary Figures S1-S5, Supplementary Table S1, Supplementary References
Working with Nonassociative Geometry and Field Theory
Creators: name: Barnes, Gwendolyn E.
name: Schenkel, Alexander
name: Szabo, Richard J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We review aspects of our formalism for differential geometry on noncommutative and nonassociative spaces which arise from cochain twist deformation quantization of manifolds. We work in the simplest setting of trivial vector bundles and flush out the details of our approach providing explicit expressions for all bimodule operations, and for connections and curvature. As applications, we describe the constructions of physically viable action functionals for Yang-Mills theory and Einstein-Cartan gravity on noncommutative and nonassociative spaces, as first steps towards more elaborate models relevant to non-geometric flux deformations of geometry in closed string theory.
description: 20 pages; v2: Reference added; Contribution to the proceedings of the Corfu Summer Institute on Elementary Particle Physics and Gravity, September 1-26, 2015, Corfu, Greece; Final version published in Proceedings of Science
Empath: Understanding Topic Signals in Large-Scale Text
Creators: name: Fast, Ethan
name: Chen, Binbin
name: Bernstein, Michael
Publisher: name: arXiv
Year: 2016
Subjects: subject: Computation and Language (cs.CL)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Human language is colored by a broad range of topics, but existing text analysis tools only focus on a small number of them. We present Empath, a tool that can generate and validate new lexical categories on demand from a small set of seed terms (like "bleed" and "punch" to generate the category violence). Empath draws connotations between words and phrases by deep learning a neural embedding across more than 1.8 billion words of modern fiction. Given a small set of seed words that characterize a category, Empath uses its neural embedding to discover new related terms, then validates the category with a crowd-powered filter. Empath also analyzes text across 200 built-in, pre-validated categories we have generated from common topics in our web dataset, like neglect, government, and social media. We show that Empath's data-driven, human validated categories are highly correlated (r=0.906) with similar categories in LIWC.
description: CHI: ACM Conference on Human Factors in Computing Systems 2016
Einfühlung und Mystik in der phänomenologischen Betrachtung Edith Steins
Creators: name: Caruso, Rosalia
Publisher: name: Edith Stein Jahrbuch
Year: 2025

description: 1647268176
description: Edith Stein Jahrbuch, V. 21 (2015): Edith Stein Jahrbuch, Band 21
Other_details_for_the_two_experiments from Environmental control of social goals: using Pavlovian-to-instrumental transfer to test cue-based pro-self and pro-social outcome responses
Creators: name: Qin, Kaiyang
name: Marien, Hans
name: Custers, Ruud
name: Aarts, Henk
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: 179999 Psychology and Cognitive Sciences not elsewhere classified
subject: FOS: Psychology
subject: 60801 Animal Behaviour
subject: FOS: Biological sciences

description: The supplementary material contains details about the normality test, details of the charities, and descriptives of the data
Adaptive strategy for joint measurements
Creators: name: Uola, Roope
name: Luoma, Kimmo
name: Moroder, Tobias
name: Heinosaari, Teiko
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We develop a technique to find simultaneous measurements for noisy quantum observables in finite-dimensional Hilbert spaces. We use the method to derive lower bounds for the noise needed to make incompatible measurements jointly measurable. Using our strategy together with recent devel- opments in the field of one-sided quantum information processing we show that the attained lower bounds are tight for various symmetric sets of quantum measurements. We use this characterisation to prove the existence of so called 4-Specker sets in the qubit case.
description: 11 pages, 7 figures, comments are welcome!