cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Analysis Based Blind Compressive Sensing
Creators: name: Wörmann, Julian
name: Hawe, Simon
name: Kleinsteuber, Martin
Publisher: name: arXiv
Year: 2013
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: In this work we address the problem of blindly reconstructing compressively sensed signals by exploiting the co-sparse analysis model. In the analysis model it is assumed that a signal multiplied by an analysis operator results in a sparse vector. We propose an algorithm that learns the operator adaptively during the reconstruction process. The arising optimization problem is tackled via a geometric conjugate gradient approach. Different types of sampling noise are handled by simply exchanging the data fidelity term. Numerical experiments are performed for measurements corrupted with Gaussian as well as impulsive noise to show the effectiveness of our method.
description: 7 pages, 2 figures
title: Model-Based Condition Monitoring of Modular Process Plants
Creators: name: Wetterich, Philipp
name: Kuhr, Maximilian M. G.
name: Pelz, Peter F.
Publisher: name: MDPI
Year: 2024

description: The process industry is confronted with rising demands for flexibility and efficiency. One way to achieve this is modular process plants, which consist of pre-manufactured modules with their own decentralized intelligence. Plants are then composed of these modules as unchangeable building blocks and can be easily re-configured for different products. Condition monitoring of such plants is necessary, but the available solutions are not applicable. The authors of this paper suggest an approach in which model-based symptoms are derived from a few measurements and observers that are based on the manufacturer’s knowledge. The comparisons of redundant observers lead to residuals that are classified to obtain symptoms. These symptoms can be communicated to the plant control and are inputs to an easily adaptable diagnosis. The implementation and validation at a modular mixing plant showcase the feasibility and potential of this approach.
Motherlogs
Creators: name: Khong, Diana
Publisher: name: Stanford Digital Repository
Year: 2023
Subjects: subject: Vietnam
subject: Death
subject: Imperialism
subject: Colonialism
subject: Death work
subject: Care work
subject: Ritual
subject: Death rites
subject: Justice
subject: Funeral rites and ceremonies

description: Motherlogs is a series of letters and journal entries that chronicle memories of my grandfather as I brace myself before, during and after his death. These letters vary in theme and tone, going from thoughtful, linear recollections to obscure, absurd and even meaningless memories. The letters have no clear chronological order. They are rift with emoticons, un-funny jokes, Ho Chi Minh quotes, childhood photos, my dorm room altars in hundreds of iterations, Spotify playlists, memories of what my grandpa missed while he was gone, and reenactments with him inserted.

As someone whose family’s displacement to the U.S. is the direct result of war, my family made the decision to bring my grandfather’s urn home to Vietnam as opposed to burying him in the States. In my grandmother’s mind, the U.S. will never be home — there is no assurance that future generations will stay. As a result, these letters will serve as both a eulogy to grandpa and a log of my eternal homecoming to Vietnam.
Electrical spin injection into graphene through monolayer hexagonal boron nitride
Creators: name: Yamaguchi, Takehiro
name: Inoue, Yoshihisa
name: Masubuchi, Satoru
name: Morikawa, Sei
name: Onuki, Masahiro
name: Watanabe, Kenji
name: Taniguchi, Takashi
name: Moriya, Rai
name: Machida, Tomoki
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We demonstrate electrical spin injection from a ferromagnet to a bilayer graphene (BLG) through a monolayer (ML) of single-crystal hexagonal boron nitride (h-BN). A Ni81Fe19/ML h-BN/BLG/h-BN structure is fabricated using a micromechanical cleavage and dry transfer technique. The transport properties across the ML h-BN layer exhibit tunnel barrier characteristics. Spin injection into BLG has been detected through non local magnetoresistance measurements.
description: 15 pages, 4 figures, accepted to Appl. Phys. Express
title: Música, sociedade e poder pelo prisma do vilancico religioso : o repertório da Capela Real de Lisboa no reinado de D. João IV (1640- 1656)
Creators: name: Lopes, Rui Cabral
Publisher: name: Universidade Lusíada Editora
Year: 2020

description: Estudos em homenagem ao professor António Martins da Cruz / coord. José de Matos Correia, Ricardo Leite Pinto. - Lisboa : Universidade Lusíada, 2020. - P. 981-996.
Additional file 1 of Relationship between vitamin D and asthma from gestational to adulthood period: a meta-analysis of randomized clinical trials
Creators: name: Sobczak, Marharyta
name: Pawliczak, Rafal
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Figure S1. Risk of bias of included studies.
On the 5-Minute Oscillations of Photospheric and Chromospheric Swirls
Creators: name: Liu, Jiajia
name: Jess, David
name: Erdélyi, Robert
name: Mathioudakis, Mihalis
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Swirls are ubiquitous in the solar atmosphere. They are believed to be related to the excitation of different modes of magnetohydrodynamic waves and pulses, as well as spicules. However, statistical studies of their collective behaviour are rare. In this paper, we aim to study the collective, as well as the behaviour of individual photospheric and chromospheric swirls detected by the automated swirl detection algorithm (ASDA) from observations obtained by the Swedish 1-m Solar Telescope and the Hinode satellite. Detailed analysis of six different parameters of photospheric and chromospheric swirls is performed employing the wavelet analysis. Two clusters of periods with significant wavelet power, one from $3-8$ minutes and the other from $10-14$ minutes, have been found. The former coincides with the dominant period of the global $p$-mode spectrum. Wavelet and Fast Fourier Transform (FFT) analysis of example swirls also reveals similar periods. These results suggest that global $p$-modes might be important for triggering photospheric and thus chromospheric swirls. A novel scenario of global $p$-modes providing energy and mass fluxes to the upper solar atmosphere via generating swirls, Alfvén pulses and spicules is then proposed.
description: 8 figures and 3 tables, to be published in A&A
Variable stars in the residual light curves of OGLE-IV eclipsing binaries towards the Galactic Bulge
Creators: name: Ádám, Rozália Z.
name: Hajdu, Tamás
name: Bódi, Attila
name: Hajdu, Róbert
name: Szklenár, Tamás
name: Molnár, László
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. The Optical Gravitational Lensing Experiment (OGLE) observed around 450,000 eclipsing binaries (EBs) towards the Galactic Bulge. Decade-long photometric observations such as these provide an exceptional opportunity to thoroughly examine the targets. However, observing dense stellar fields such as the Bulge may result in blends and contamination by close objects. Aims. We searched for periodic variations in the residual light curves of EBs in OGLE-IV and created a new catalogue for the EBs that contain `background' signals after the investigation of the source of the signal. Methods. From the about half a million EB systems, we selected those that contain more than 4000 data points. We fitted the EB signal with a simple model and subtracted it. To identify periodical signals in the residuals, we used a GPU-based phase dispersion minimisation python algorithm called cuvarbase and validated the found periods with Lomb-Scargle periodograms. We tested the reliability of our method with artificial light curves. Results. We identified 354 systems where short-period background variation was significant. In these cases, we determined whether it is a new variable or just the result of contamination by an already catalogued nearby one. We classified 292 newly found variables into EB, $δ$ Scuti, or RR Lyrae categories, or their sub-classes, and collected them in a catalogue. We also discovered four new doubly eclipsing systems and one eclipsing multiple system with a $δ$ Scuti variable, and modelled the outer orbits of the components.
description: 22 pages, 17 figures, 7 tables, accepted for publication in Astronomy & Astrophysics
The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions
Creators: name: Rodriguez-Puebla, A.
name: Avila-Reese, V.
name: Drory, N.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We infer the local stellar-to-halo/subhalo mass relations (MRs) for central and satellite galaxies separately. We constraint this relations by using several combinations of observational data, consisting of the total galaxy stellar mass function, its decomposition into centrals and satellites, and the projected two-point correlation functions measured in different stellar mass bins. The differences among the resulting MRs are within the model-fit uncertainties (which are very small, smaller than the intrinsic scatter between galaxy and halo mass), no matter what combination of data are used. We also constrain the values of the intrinsic scatter around the central-halo (CH) and satellite-subhalo (SS) MRs assuming them to be constant: sigma_c= 0.168+-0.051 dex and sigma_s = 0.172+-0.057 dex, respectively. The CH and SS MRs are actually different, in particular when we take the subhalo mass at the present-day epoch instead of at their accretion time. We calculate several population statistics. We find that the central galaxy is not on average within the mass distribution of the most-massive satellite, even for cluster-sized halos, i.e., centrals are not a mere realization of the high-end of the satellite mass function; however for > 3x10^13 msun halos, ~15% of centrals could be. We also find that the probabilities of MW-sized halos of having N Magellanic-Clouds (MCs)-sized satellites agree well with observational measures; for a halo mass of 2x10^12 msun, the probability to have 2 MCs is 5.4%, but if we exclude those systems with satellites larger than the MCs, then the probability decreases to <2.2%.
description: 18 pages, 7 figures. Accepted for publication in ApJ. Some references were added
The Nature of Starbursts: III. The Spatial Distribution of Star Formation
Creators: name: McQuinn, Kristen B. W.
name: Skillman, Evan D.
name: Dalcanton, Julianne J.
name: Cannon, John M.
name: Dolphin, Andrew E.
name: Holtzman, Jon
name: Weisz, Daniel R.
name: Williams, Benjamin F.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We map the spatial distribution of recent star formation over a few x 100 Myr timescales in fifteen starburst dwarf galaxies using the location of young blue helium burning stars identified from optically resolved stellar populations in archival Hubble Space Telescope observations. By comparing the star formation histories from both the high surface brightness central regions and the diffuse outer regions, we measure the degree to which the star formation has been centrally concentrated during the galaxies' starbursts, using three different metrics for the spatial concentration. We find that the galaxies span a full range in spatial concentration, from highly centralized to broadly distributed star formation. Since most starbursts have historically been identified by relatively short timescale star formation tracers (e.g., Halpha emission), there could be a strong bias towards classifying only those galaxies with recent, centralized star formation as starbursts, while missing starbursts that are spatially distributed.
description: 28 pages, 14 figures, 2 tables
Additional file 1 of amica: an interactive and user-friendly web-platform for the analysis of proteomics data
Creators: name: Didusch, Sebastian
name: Madern, Moritz
name: Hartl, Markus
name: Baccarini, Manuela
Publisher: name: figshare
Year: 2023
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences

description: Additional file 1: Supplementary Material — File 1. Link to a user manual demonstrating every available function and output graphics, as well as extensive tutorials.
„... mit den Tunnels und den Gleisen ..." Die Alte Eisenbahn im Eggegebirge (Kr. Paderborn)
Creators: name: Jürgens, Fritz
name: Wolpert, Nils
Publisher: name: Mitteilungen der Deutschen Gesellschaft für Archäologie des Mittelalters und der Neuzeit
Year: 2017

description: [nicht vorhanden / not available]
description: Mitteilungen der Deutschen Gesellschaft für Archäologie des Mittelalters und der Neuzeit, Bd. 30 (2017): Mitteilungen der DGAMN: Globalisierung
Spectral classification of young stars using conditional invertible neural networks I. Introducing and validating the method
Creators: name: Kang, Da Eun
name: Ksoll, Victor F.
name: Itrich, Dominika
name: Testi, Leonardo
name: Klessen, Ralf S.
name: Hennebelle, Patrick
name: Molinari, Sergio
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Aims. We introduce a new deep learning tool that estimates stellar parameters (such as effective temperature, surface gravity, and extinction) of young low-mass stars by coupling the Phoenix stellar atmosphere model with a conditional invertible neural network (cINN). Our networks allow us to infer the posterior distribution of each stellar parameter from the optical spectrum. Methods. We discuss cINNs trained on three different Phoenix grids: Settl, NextGen, and Dusty. We evaluate the performance of these cINNs on unlearned Phoenix synthetic spectra and on the spectra of 36 Class III template stars with well-characterised stellar parameters. Results. We confirm that the cINNs estimate the considered stellar parameters almost perfectly when tested on unlearned Phoenix synthetic spectra. Applying our networks to Class III stars, we find good agreement with deviations of at most 5--10 per cent. The cINNs perform slightly better for earlier-type stars than for later-type stars like late M-type stars, but we conclude that estimations of effective temperature and surface gravity are reliable for all spectral types within the network's training range. Conclusions. Our networks are time-efficient tools applicable to large amounts of observations. Among the three networks, we recommend using the cINN trained on the Settl library (Settl-Net), as it provides the best performance across the largest range of temperature and gravity.
description: 29 pages, 19 figures, Accepted for publication by Astronomy & Astrophysics on 10. April
Spatial profiles of collimated laser Compton-scattering $γ$-ray beams
Creators: name: Ari-Izumi, Takashi
name: Gheorghe, Ioana
name: Filipescu, Dan
name: Hashimoto, Satoshi
name: Miyamoto, Shuji
name: Utsunomiya, Hiroaki
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: The intensity and energy spatial distributions of collimated laser Compton scattering (LCS) $γ$-ray beams and of the associated bremsstrahlung beams have been investigated as functions of the electron beam energy, electron beam phase space distribution, laser optics conditions and laser polarization. We show that the beam halo is affected to different extents by variations in the above listed parameters. In the present work, we have used laser Compton scattering simulations performed with the \texttt{eliLaBr} code (https://github.com/dan-mihai-filipescu/eliLaBr) and real LCS and bremsstrahlung $γ$-ray beams produced at the NewSUBARU synchrotron radiation facility. A 500~$μ$m MiniPIX X-ray camera was used as beamspot monitor in a wide $γ$-ray beam energy range between 1.73~MeV and 38.1~MeV.
The true meaning of dreams
Creators: name: Gewargis, Youash Arkhiom
Publisher: name: International Journal of Dream Research
Year: 2016

description: Dream  researchers have failed to solve the dream's riddle. The main reason is that almost all have adopted the content-approach, initiated by the two prominent pioneers, Sigmund Freud and Carl Jung.  In this  study dreams will be viewed from an entirely different vantage point: Dreams are seen as  a component of a more intricate mechanism,  run by the brainstem and in collaboration with the peripheral  nervous system's two parts, namely the  parasympathetic and sympathetic nervous systems; the vision; pontes and a few muscles. This complex mechanism takes over the task of safeguarding the living organisms (mostly viviparous  mammals and birds) during the sleep---a physiologically dictated slumber that all  living organisms must undergo, to regenerate and rejuvenate.  At sleep, the body functions are lowered to the  minimum permissible level of their respective operations, and sustained  at such a dangerous level,  without  allowing  the  body from slipping into the impermissible and  undesirable territories; thence  obtaining the best regeneration and rejuvenation results for the  perpetually operating  body organs, like central brain and the heart, prior to the start of a new  cycle of normal duties.  In this study,  the role of each  component of this complex defence-mechanism will be thoroughly  explained; and how together they  safeguard the organism   from  two main risks within, that surface out mostly during the deep- sleep level.
description: International Journal of Dream Research, Vol 9, No 2 (October 2016)
Additional file 2 of Relationship between vitamin D and asthma from gestational to adulthood period: a meta-analysis of randomized clinical trials
Creators: name: Sobczak, Marharyta
name: Pawliczak, Rafal
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Figure S2. Funnel plots for the associations of between vitamin D supplementation and asthma.
Additional file 1 of Initial development of tools to identify child abuse and neglect in pediatric primary care
Creators: name: Hanson, Rochelle F.
name: Zhu, Vivienne
name: Are, Funlola
name: Espeleta, Hannah
name: Wallis, Elizabeth
name: Heider, Paul
name: Kautz, Marin
name: Lenert, Leslie
Publisher: name: figshare
Year: 2023
Subjects: Medicine
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Cancer
Science Policy

description: Additional file 1. CAN ACS-Survey.
Electron neutrino and antineutrino appearance in the full MINOS data sample
Creators: name: Adamson, P.
name: Anghel, I.
name: Backhouse, C.
name: Barr, G.
name: Bishai, M.
name: Blake, A.
name: Bock, G. J.
name: Bogert, D.
name: Cao, S. V.
name: Cherdack, D.
name: Childress, S.
name: Coelho, J. A. B.
name: Corwin, L.
name: Cronin-Hennessy, D.
name: de Jong, J. K.
name: Devan, A. V.
name: Devenish, N. E.
name: Diwan, M. V.
name: Escobar, C. O.
name: Evans, J. J.
name: Falk, E.
name: Feldman, G. J.
name: Frohne, M. V.
name: Gallagher, H. R.
name: Gomes, R. A.
name: Goodman, M. C.
name: Gouffon, P.
name: Graf, N.
name: Gran, R.
name: Grzelak, K.
name: Habig, A.
name: Hahn, S. R.
name: Hartnell, J.
name: Hatcher, R.
name: Himmel, A.
name: Holin, A.
name: Hylen, J.
name: Irwin, G. M.
name: Isvan, Z.
name: Jaffe, D. E.
name: James, C.
name: Jensen, D.
name: Kafka, T.
name: Kasahara, S. M. S.
name: Koizumi, G.
name: Kordosky, M.
name: Kreymer, A.
name: Lang, K.
name: Ling, J.
name: Litchfield, P. J.
name: Lucas, P.
name: Mann, W. A.
name: Marshak, M. L.
name: Mathis, M.
name: Mayer, N.
name: Medeiros, M. M.
name: Mehdiyev, R.
name: Meier, J. R.
name: Messier, M. D.
name: Miller, W. H.
name: Mishra, S. R.
name: Sher, S. Moed
name: Moore, C. D.
name: Mualem, L.
name: Musser, J.
name: Naples, D.
name: Nelson, J. K.
name: Newman, H. B.
name: Nichol, R. J.
name: Nowak, J. A.
name: Ochoa-Ricoux, J. P.
name: O'Connor, J.
name: Oliver, W. P.
name: Orchanian, M.
name: Pahlka, R. B.
name: Paley, J.
name: Patterson, R. B.
name: Pawloski, G.
name: Phan-Budd, S.
name: Plunkett, R. K.
name: Qiu, X.
name: Radovic, A.
name: Rebel, B.
name: Rosenfeld, C.
name: Rubin, H. A.
name: Sanchez, M. C.
name: Schneps, J.
name: Schreckenberger, A.
name: Schreiner, P.
name: Sharma, R.
name: Sousa, A.
name: Tagg, N.
name: Talaga, R. L.
name: Thomas, J.
name: Thomson, M. A.
name: Tinti, G.
name: Toner, R.
name: Torretta, D.
name: Tzanakos, G.
name: Urheim, J.
name: Vahle, P.
name: Viren, B.
name: Weber, A.
name: Webb, R. C.
name: White, C.
name: Whitehead, L.
name: Wojcicki, S. G.
name: Yang, T.
name: Zwaska, R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report on $ν_e$ and $\barν_e$ appearance in $ν_μ$ and $\barν_μ$ beams using the full MINOS data sample. The comparison of these $ν_e$ and $\barν_e$ appearance data at a 735 km baseline with $θ_{13}$ measurements by reactor experiments probes $δ$, the $θ_{23}$ octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for $\barν_μ\rightarrow\barν_e$. Our data disfavor 31% (5%) of the three-parameter space defined by $δ$, the octant of the $θ_{23}$, and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sin$^2(2θ_{13})$sin$^2(θ_{23})$ that is consistent with reactor experiments.
Leading components and pressure-induced color changes in N-doped lutetium hydride
Creators: name: Tao, Xiangru
name: Yang, Aiqin
name: Yang, Shuxiang
name: Quan, Yundi
name: Zhang, Peng
Publisher: name: arXiv
Year: 2023
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Recent experimental study by Dias {\it et al.} claims to have discovered room-temperature superconductivity in lutetium-nitrogen-hydrogen system at 1 GPa [Nature 615, 244 (2023)], which sheds light on the long-held dream of ambient superconductivity. However, all follow-up experiments found no evidence of superconductivity. The compositions and the crystal structures of the lutetium-nitrogen-hydrogen system remain unknown. By employing the density functional theory based structure prediction algorithm, we suggest that in lutetium-nitrogen-hydrogen the major component is LuH$_2$ (Fm$\bar{3}$m), together with minor LuN (Fm$\bar{3}$m). The blue LuH$_2$ at ambient pressure will turn into purple and red color at higher pressures, possibly accompanied by the formation of vacancies at hydrogen-sites. In LuH$_2$ and LuN, the density of states at the Fermi level is dominated by the Lu-5d orbitals, while those from hydrogen and nitrogen are very small, leading to the absence of superconductivity in these two compounds. Nitrogen-doping to LuH$_2$ fails to enhance the superconductivity as well. In this work, we identify the leading components in N-doped lutetium hydride, explain its intriguing color changes under pressure, and elucidate why superconductivity is absent in the follow-up experiments.
Mass measurements and 3D orbital geometry of PSR J1933$-$6211
Creators: name: Geyer, M.
name: Krishnan, V. Venkatraman
name: Freire, P. C. C.
name: Kramer, M.
name: Antoniadis, J.
name: Bailes, M.
name: Bernadich, M. C. i
name: Buchner, S.
name: Cameron, A. D.
name: Champion, D. J.
name: Karastergiou, A.
name: Keith, M. J.
name: Lower, M. E.
name: Osłowski, S.
name: Possenti, A.
name: Parthasarathy, A.
name: Reardon, D. J.
name: Serylak, M.
name: Shannon, R. M.
name: Spiewak, R.
name: van Straten, W.
name: Verbiest, J. P. W.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: PSR J1933$-$6211 is a 3.5-ms pulsar in a 12.8-d orbit with a white dwarf (WD). Its high proper motion and low dispersion measure result in such significant interstellar scintillation that high signal-to-noise detections require long observing durations or fortuitous timing. We turn to the sensitive MeerKAT telescope and, combined with historic Parkes data, leverage PSR J1933$-$6211's kinematic and relativistic effects to constrain its 3D orbital geometry and the component masses. We obtain precise proper motion and parallax estimates, and measure their effects as secular changes in the Keplerian orbital parameters: a variation in orbital period of $7(1) \times 10^{-13}$ s s$^{-1}$ and a change in projected semi-major axis of $1.60(5) \times 10^{-14}$ s s$^{-1}$. A self-consistent analysis of all kinematic and relativistic effects yields a distance of $1.6^{+0.2}_{-0.3}$ kpc, an orbital inclination, $i = 55(1)$ deg and a longitude of the ascending node, $Ω= 255^{+8}_{-14}$ deg. The probability densities for $Ω$ and $i$ and their symmetric counterparts, ($180-i$, $360-Ω$), are seen to depend on the fiducial orbit used to measure the time of periastron passage. We investigate this unexpected dependence and rule out software-related causes using simulations. Nevertheless, we constrain the pulsar and WD masses to $1.4^{+0.3}_{-0.2}$ M$_\odot$ and $0.43(5)$ M$_\odot$ respectively. These strongly disfavour a helium-dominated WD. The orbital similarities between PSRs J1933$-$6211 and J1614$-$2230 suggest they underwent Case A Roche lobe overflow, an extended evolution while the companion star is still on the Main Sequence. However, with a mass of $\sim 1.4$ M$_\odot$, PSR J1933$-$6211 has not accreted significant matter. This highlights the low accretion efficiency of the spin-up process and suggests that observed neutron star masses are mostly a result of supernova physics.
description: 16 pages, 7 figures. Abstract shortened to adhere to ArXiv limit
Quantum hydrodynamics
Creators: name: Tsubota, Makoto
name: Kobayashi, Michikazu
name: Takeuchi, Hiromitsu
Publisher: name: arXiv
Year: 2012
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: Quantum hydrodynamics in superfluid helium and atomic Bose-Einstein condensates (BECs) has been recently one of the most important topics in low temperature physics. In these systems, a macroscopic wave function appears because of Bose-Einstein condensation, which creates quantized vortices. Turbulence consisting of quantized vortices is called quantum turbulence (QT). The study of quantized vortices and QT has increased in intensity for two reasons. The first is that recent studies of QT are considerably advanced over older studies, which were chiefly limited to thermal counterflow in 4He, which has no analogue with classical traditional turbulence, whereas new studies on QT are focused on a comparison between QT and classical turbulence. The second reason is the realization of atomic BECs in 1995, for which modern optical techniques enable the direct control and visualization of the condensate and can even change the interaction; such direct control is impossible in other quantum condensates like superfluid helium and superconductors. Our group has made many important theoretical and numerical contributions to the field of quantum hydrodynamics of both superfluid helium and atomic BECs. In this article, we review some of the important topics in detail. The topics of quantum hydrodynamics are diverse, so we have not attempted to cover all these topics in this article. We also ensure that the scope of this article does not overlap with our recent review article (arXiv:1004.5458), "Quantized vortices in superfluid helium and atomic Bose--Einstein condensates", and other review articles.
description: 102 pages, 29 figures, 1 table
D2.3 Meta Report of the YouCount Experiences with Case Study Implementation
Creators: name: Ridley, Julie
name: Turda, Maria
name: Brattbakk, Ingar
name: Norvoll, Reidun
Publisher: name: Zenodo
Year: 2023

description: This D2.3 Meta Report of the YouCount Experiences with Case Study Implementation is rooted in WP2 and the implementation of hands-on youth citizen social science (Y-CSS).  In particular it addresses the work of Tasks 2.1 to 2.10 which include laying the foundations and planning multi-disciplinary research teams that include professional researchers, students and young people as Youth Citizen Scientists (YCS), recruiting and engaging YCS, students and stakeholders, developing and refining research methods to explore social inclusion with YCS and conducting co-creative research with young people. The primary focus is on case experiences with implementing the social inclusion sub study. It therefore provides details of the 10 local cases in nine countries in a multiple case study of co-creative Y-CSS in Europe and their experiences.  The cross case thematic analysis builds on the individual case reports, extracts from the evaluation self-reports and notes from consortium or WP2 discussions. 

This Report comprises six parts: (1) background and contextual overview of YouCount’s aims and intentions in implementing the multiple case study of hands-on Y-CSS; (2) planning and establishing Y-CSS; (3) recruitment, training and support of YCS; (4) methodologies adopted by the local cases including the designs, methods and data analysis conducted; (5) what co-creation meant in practice; (6) summary and conclusions. 

The main target groups for this Deliverable are those interested in how Y-CSS can be conducted in practice, either as practitioner, scientists or evaluator of best practices.
The nightmare protection hypothesis: An experimental inquiry
Creators: name: Flockhart, Carson
name: Gackenbach, Jayne Isabel
Publisher: name: International Journal of Dream Research
Year: 2017
Subjects: threat simulation, nightmare protection, combat centric, dreams, video games

description: Using the ideas generated in Revonsuo and Valli’s Threat Simulation model of the function of dreaming, previous research looked at how military personal’s dreams were associated with video game play. A nightmare protection effect was found and replicated using an undergraduate student population. Based on the previous findings, in this study an experimental manipulation was conducted where male participants engaged in one of three computer tasks, including gaming and search. All participants also viewed a frightening movie clip. Following the laboratory session respondents were asked to report a dream. The Threat Simulation method of coding dreams was used to assess threat in participant’s dreams. The major hypothesis was that playing a combat centric game would be more likely to result in behaviors in the dream which were less nightmarish after seeing the frightening movie clip, relative to playing a creative video game or doing a computer search task. The results support the thesis for high end male gamers playing combat centric video games close in time to being exposed to a frightening film clip. These young men are either not perceiving the same danger in their follow-up dream as threatening or that the content is not as scary as those without a recent experience of combat centric gaming.
description: International Journal of Dream Research, Vol 10, No 1 (April 2017)
Investigating the large-scale environment of wide-angle tailed radio galaxies in the local Universe
Creators: name: Missaglia, V.
name: Paggi, A.
name: Massaro, F.
name: Capetti, A.
name: Baldi, R. D.
name: Kraft, R. P.
name: Paolillo, M.
name: Tramacere, A.
name: Campana, R.
name: Pillitteri, I.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a statistical analysis of the large-scale (up to 2 Mpc) environment of an homogeneous and complete sample, both in radio and optical selection, of wide-angle tailed radio galaxies (WATs) in the local Universe (i.e., with redshifts $z\lesssim$ 0.15). The analysis is carried out using the parameters obtained from cosmological neighbors within 2 Mpc of the target source. Results on WATs large-scale environments are then compared with that of Fanaroff-Riley type I (FR Is) and type II (FR IIs) radio galaxies, listed in two others homogeneous and complete catalogs, and selected with the same criterion adopted for the WATs catalog. We obtain indication that at low redshift WATs inhabit environments with a larger number of galaxies than that of FR Is and FR IIs. In the explored redshift range, the physical size of the galaxy group/cluster in which WATs reside appears to be almost constant with respect to FR Is and FR IIs, being around 1 Mpc. From the distribution of the concentration parameter, defined as the ratio between the number of cosmological neighbors lying within 500 kpc and within 1 Mpc, we conclude that WATs tend to inhabit the central region of the group/cluster in which they reside, in agreement with the general paradigm that WATs are the cluster BCG.
description: 8 pages, 5 figures, 1 table. Accepted for publication on A&A
Toward a better understanding of the mid-infrared emission in the LMC
Creators: name: Paradis, D.
name: Mény, C.
name: Demyk, K.
name: Noriega-Crespo, A.
name: Ristorcelli, I.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this paper we aim to constrain for the first time the dust emission in the mid-to-far infrared domain, in the LMC, with the use of the Spitzer IRS and MIPS SED data, combined with Herschel data. We also consider UV extinction predictions derived from modeling. We selected 10 regions observed as part of the SAGE-Spec program, to probe dust properties in various environments (diffuse, molecular and ionized regions). All data were smoothed to the 40arcsec angular resolution. The SEDs were modeled with DustEM models, using the standard Mathis RF, as well as three additional RFs, with stellar clusters ages ranging from 4 Myr to 600 Myr. Standard dust models used to reproduce the Galactic diffuse medium are clearly not able to reproduce the dust emission in the MIR wavelength domain. This analysis evidences the need of adjusting parameters describing the dust size distribution and shows a clear distinct behavior according to the type of environments. In addition, whereas the small grain emission always seems to be negligible at long wavelengths in our Galaxy, the contribution of this small dust component could be more important than expected, in the submm-mm range, in the LMC averaged SED. Properties of the small dust component of the LMC are clearly different from those of our Galaxy. Its abundance, significantly enhanced, could be the result of large grains shattering due to strong shocks or turbulence. In addition, this grain component in the LMC systematically shows smaller grain size in the ionized regions compared to the diffuse medium. Predictions of extinction curves show significantly distinct behaviors depending on the dust models but also from one region to another. Comparison of model predictions with the LMC mean extinction curve shows that no model gives satisfactory agreement using the Mathis radiation field while using a harder radiation field tends to improve the agreement
description: Accepted for publication in A&A
D2.3 Meta Report of the YouCount Experiences with Case Study Implementation
Creators: name: Ridley, Julie
name: Turda, Maria
name: Brattbakk, Ingar
name: Norvoll, Reidun
Publisher: name: Zenodo
Year: 2023

description: This D2.3 Meta Report of the YouCount Experiences with Case Study Implementation is rooted in WP2 and the implementation of hands-on youth citizen social science (Y-CSS).  In particular it addresses the work of Tasks 2.1 to 2.10 which include laying the foundations and planning multi-disciplinary research teams that include professional researchers, students and young people as Youth Citizen Scientists (YCS), recruiting and engaging YCS, students and stakeholders, developing and refining research methods to explore social inclusion with YCS and conducting co-creative research with young people. The primary focus is on case experiences with implementing the social inclusion sub study. It therefore provides details of the 10 local cases in nine countries in a multiple case study of co-creative Y-CSS in Europe and their experiences.  The cross case thematic analysis builds on the individual case reports, extracts from the evaluation self-reports and notes from consortium or WP2 discussions. 

This Report comprises six parts: (1) background and contextual overview of YouCount’s aims and intentions in implementing the multiple case study of hands-on Y-CSS; (2) planning and establishing Y-CSS; (3) recruitment, training and support of YCS; (4) methodologies adopted by the local cases including the designs, methods and data analysis conducted; (5) what co-creation meant in practice; (6) summary and conclusions. 

The main target groups for this Deliverable are those interested in how Y-CSS can be conducted in practice, either as practitioner, scientists or evaluator of best practices.

 

This version 2 is the same as version 1, but included names of internal scientific reviewers.
Cumulative physical uncertainty in modern stellar models I. The case of low-mass stars
Creators: name: Valle, G.
name: Dell'Omodarme, M.
name: Moroni, P. G. Prada
name: Degl'Innocenti, S.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Using our updated stellar evolutionary code, we quantitatively evaluate the effects of the uncertainties in the main physical inputs on the evolutionary characteristics of low mass stars from the main sequence to the zero age horizontal branch (ZAHB). We calculated more than 3000 stellar tracks and isochrones, with updated solar mixture, by changing the following physical inputs within their current range of uncertainty: 1H(p,nu e+)2H, 14N(p,gamma)15O, and triple-alpha reaction rates, radiative and conductive opacities, neutrino energy losses, and microscopic diffusion velocities. We performed a systematic variation on a fixed grid, in a way to obtain a full crossing of the perturbed input values. The effect of the variations of the chosen physical inputs on relevant stellar evolutionary features, such as the turn-off luminosity, the central hydrogen exhaustion time, the red-giant branch (RGB) tip luminosity, the helium core mass, and the ZAHB luminosity in the RR Lyrae region are statistically analyzed. For a 0.9 Msun model, the cumulative uncertainty on the turn-off, the RGB tip, and the ZAHB luminosities accounts for $\pm$ 0.02 dex, $\pm$ 0.03 dex, and $\pm$ 0.045 dex respectively, while the central hydrogen exhaustion time varies of about $\pm$ 0.7 Gyr. The most relevant effect is due to the radiative opacities uncertainty; for the later evolutionary stages the second most important effect is due to the triple-alpha reaction rate uncertainty. For an isochrone of 12 Gyr, we find that the isochrone turn-off log luminosity varies of $\pm$ 0.013 dex, the mass at the isochrone turn-off varies of $\pm$ 0.015 Msun, and the difference between ZAHB and turn-off log-luminosity varies of $\pm$ 0.05 dex. The effect of the physical uncertainty affecting the age inferred from turn-off luminosity and from the vertical method are of $\pm$ 0.375 Gyr and $\pm$ 1.25 Gyr respectively.
description: Accepteted for pubblication in A&A. The abstract is shortened to fill in the arxiv abstract field
Stripe Instabilities of Geometries with Hyperscaling Violation
Creators: name: Iizuka, Norihiro
name: Maeda, Kengo
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the dynamical stripe instabilities on the geometries with hyperscaling violation in the IR, which asymptotically approach AdS_4 in the UV. The instabilities break the translational invariance spontaneously and are induced by the axion term ~ a F \wedge F in the bulk action. We first study the perturbation equations in the probe limit, and find that there is a strong correlation between the stripe instabilities caused by the axion term and parameters of the theories which determine the IR hyperscaling violation. Contrary to the IR AdS_2 case, the effect of the axion term for the stripe instabilities can be enhanced/suppressed at low temperature depending on the parameters. For a certain one-parameter family of the hyperscaling violation, we find the onset of the stripe instability analytically in the axion coupling tuned model. For more generic parameter range of hyperscaling violation, we study the instability onset by searching for the zero mode numerically on the full geometries. We also argue that quite analogous results hold, after taking into account the graviton fluctuation, i.e., beyond the probe limit.
description: 17 pages, 7 figures. v2: references added
Additional file 1 of The effect of a roving nurse mentor on household coverage and quality of care provided by community health worker teams in South Africa: a longitudinal study with a before, after and 6 months post design
Creators: name: Goudge, Jane
name: Babalola, Olukemi
name: Malatji, Hlologelo
name: Levin, Jonathan
name: Thorogood, Margaret
name: Griffiths, Frances
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy

description: Additional file 1: Supplementary Table 1. Description of dwellings and households. Supplementary Table 2. Description of household respondents. Supplementary Table 3. Factors associated with being visited (unadjusted and adjusted regression analysis): both sites combined.
Improving nuclear data evaluations with predictive reaction theory and indirect measurements
Creators: name: Escher, Jutta
name: Bergstrom, Kirana
name: Chimanski, Emanuel
name: Gorton, Oliver
name: In, Eun Jin
name: Kruse, Michael
name: Péru, Sophie
name: Pruitt, Cole
name: Rahman, Rida
name: Shinkle, Emily
name: Thapa, Aaina
name: Younes, Walid
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Nuclear reaction data required for astrophysics and applications is incomplete, as not all nuclear reactions can be measured or reliably predicted. Neutron-induced reactions involving unstable targets are particularly challenging, but often critical for simulations. In response to this need, indirect approaches, such as the surrogate reaction method, have been developed. Nuclear theory is key to extract reliable cross sections from such indirect measurements. We describe ongoing efforts to expand the theoretical capabilities that enable surrogate reaction measurements. We focus on microscopic predictions for charged-particle inelastic scattering, uncertainty-quantified optical nucleon-nucleus models, and neural-network enhanced parameter inference.
description: 4 pages, 4 figures, proceedings contribution for Nuclear Data 2022
Jenseits von Mann und Frau. Körper als Bühne
Creators: name: Juneja, Monica
Publisher: name: Ruperto Carola
Year: 2017

description: Porträts an indischen Mogulhöfen der Frühmoderne weisen eine überraschende Besonderheit auf: Ob Frauen oder Männer abgebildet werden, ist oft kaum zu unterscheiden. Damit stehen die Gemälde in deutlichem Gegensatz zu Beschreibungen in verschriftlichten Überlieferungen und Texten, in denen zum Beispiel die Körperlichkeit des idealen Herrschers mit machtvollen männlichen Attributen charakterisiert wird. Die gemalten Darstellungen konzentrieren sich demgegenüber darauf, die Schichtzugehörigkeit und die Insignien der Macht jenseits von Individualität und Geschlecht zu visualisieren: Der Körper wird zur Bühne.
description: Ruperto Carola, Nr. 10 (2017): Frau & Mann
Katharine Louisa, Viscountess Amberley, With Two Dogs
Creators: name: (:Unav)
Publisher: name: Columbia University
Year: 2019
Subjects: Dogs
Suffragists

description: "Kate Stanley (Lady Amberley [illeg])" below, not in Thomas Carlyle's hand: "Kate. Reinecke. Argos" image shows woman with two dogs, both on hind legs
Gap Symmetry and Stability Analysis in the Multi-Orbital Fe-Based Superconductors
Creators: name: Fischer, Mark H
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The iron-based superconductors allow for a zoo of possible order parameters due to their orbital degrees of freedom. These order parameters are often written in an orbital basis, as this allows to distinguish their different symmetry. Unlike in standard single-band superconductors, where electrons of the same band - and hence, energy - are paired, a general order parameter in such a multi-orbital system also contains pairing of electrons belonging to different bands. As this corresponds to pairing of electrons of different energy, such order parameters are energetically less stable. Here, we present a simple criterion for a stability analysis of the orbital part of the gap function based on the basic principle that electrons of equal energy are paired in the superconducting state. This not only allows to find the most stable states, but also to identify the terms in a (tight-binding) Hamiltonian suppressing any given superconducting state. Our approach thus allows to identify the minimal Hamiltonian necessary to compare competing instabilities.
Star formation associated with the infrared dust bubble N68
Creators: name: Zhang, Chuan-Peng
name: Wang, Jun-Jie
Publisher: name: arXiv
Year: 2012
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigated the environment of the infrared dust bubble N68 and searched for evidence of triggered star formation in its surroundings. We performed a multiwavelength study of the nebula with data taken from several large-scale surveys: GLIMPSE, MIPSGAL, IRAS, NVSS, GRS, and JCMT. We analyzed the spectral profile and the distribution of the molecular gas (^{13}CO J = 1 - 0 and J = 3 - 2), and the dust in the environment of the N68. The position-velocity diagram clearly shows that the N68 may be expanding outward. We used two three-color images of the mid-infrared emission to explore the physical environment, and one color-color diagram to investigate the distribution of young stellar objects (YSOs). We found that the 24 μm emission is surrounded by the 8.0 μm emission. Morphologically, the 1.4 GHz continuum correlates strongly with the 24 μm emission, and the ^{13}CO J = 1 - 0 and J = 3 - 2 emissions correlate well with the 8.0 μm emission. We investigated two compact cores located at the shell of the N68. The spectral intensity ratios of ^{13}CO J = 3 - 2 to J = 1 - 0 range from 5 to 0.3. In addition, young star objects, masers, IRAS, and UC HII regions distribute at the shell of bubble. The active region may be triggered by the expanding of the bubble N68.
description: 10 pages, 11 figures, submited to RAA