cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
3D intrinsic shapes of quiescent galaxies in observations and simulations
Creators: name: Zhang, Junkai
name: Wuyts, Stijn
name: Witten, Callum
name: Avery, Charlotte R.
name: Hao, Lei
name: Sharma, Raman
name: Shen, Juntai
name: Toshikawa, Jun
name: Villforth, Carolin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the intrinsic 3D shapes of quiescent galaxies over the last half of cosmic history based on their axial ratio distribution. To this end, we construct a sample of unprecedented size, exploiting multi-wavelength $u$-to-$K_s$ photometry from the deep wide area surveys KiDS+VIKING paired with high-quality $i$-band imaging from HSC-SSP. Dependencies of the shapes on mass, redshift, photometric bulge prominence and environment are considered. For comparison, the intrinsic shapes of quenched galaxies in the IllustrisTNG simulations are analyzed and contrasted to their formation history. We find that over the full $0 10^{11}\ M_{\odot}$, with the effect being most pronounced at lower redshifts. In TNG, the most massive galaxies feature the highest ex-situ stellar mass fractions, pointing to violent relaxation via mergers as the mechanism responsible for their 3D shape transformation. Larger differences between observed and simulated shapes are found at low to intermediate masses. At any mass, the most spheroidal quiescent galaxies in TNG feature the highest bulge mass fractions, and conversely observed quiescent galaxies with the highest bulge-to-total ratios are found to be intrinsically the roundest. Finally, we detect an environmental influence on galaxy shape, at least at the highest masses, such that at fixed mass and redshift quiescent galaxies tend to be rounder in denser environments.
description: Accepted by MNRAS. 18 pages, 11 figures, 2 tables
AI-Driven Bioinformatics Reveals Therapeutic Potential of Lactoferrin and MMP-8 in Lung Injury
Creators: name: Tang, Hexiao
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 320211
subject: Infectious diseases
classificationCode: 320212
subject: Intensive care
classificationCode: 320299
subject: Clinical sciences not elsewhere classified

description: This study addresses the high incidence and mortality of lung injury by identifying key genes using bioinformatics and experimental validation. We analyzed the GSE32707 dataset with R software, performing differential expression analysis, WGCNA, and machine learning. GO and KEGG enrichment, PPI network, immune infiltration, ceRNA network, and molecular docking analyses were conducted to explore mechanisms and therapeutic roles. We identified 506 DEGs, with 471 upregulated and 35 downregulated, enriched in immune processes. Machine learning identified LTF and MMP8 as key genes, associated with immune cell infiltration. MR analysis confirmed their causal relationship with lung injury risk. Validation in human, cells, and animal models supported these findings, providing a foundation for further clinical research.
Annotated Hardanger Fiddle
Creators: name: Mjelva, Olav Luksengård
name: Garmo, Astrid
name: Lartillot, Olivier
name: Gjertsen, Henrik Nordtun
name: Cyvin, Mattias
name: Monstad, Lars
name: Elowsson, Anders
name: Johansson, Mats Sigvard
Publisher: name: OSF
Year: 2023

description: Version 1.0, 8 Dec 2023
Version 2.0 in preparation (March 2025)
Several hour of recordings of Hardanger fiddle music, with note annotations of onsets, offsets and pitches, provided by the performers themselves. A subset of 18 minutes has also been annotated with beat onset positions by the performer as well as three expert musicians.
The tunes are performed by Olav Luksengård Mjelva, Astrid Garmo and Henrik Nordtun Gjertsen.
Project funded by the MIRAGE project and by the RITMO Centre.
Giant spectral renormalization and complex hybridization physics in a Kondo lattice system, CeCuSb2
Creators: name: Datta, Sawani
name: Pandeya, Ram Prakash
name: Dey, Arka Bikash
name: Gloskovskii, A.
name: Schlueter, C.
name: Peixoto, Thiago
name: Singh, Ankita
name: Thamizhavel, A.
name: Maiti, Kalobaran
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We investigate the electronic structure of a Kondo lattice system, CeCuSb2 exhibiting significant mass enhancement and Kondo-type behavior. We observe multiple features in the hard x-ray photoemission spectra of Ce core levels due to strong final-state effects. The depth-resolved data exhibit a significant change in relative intensity of the features with the surface sensitivity of the probe. The extracted surface and bulk spectral functions are different and exhibit a Kondo-like feature at higher binding energies in addition to the well and poorly screened features. The core-level spectra of Sb exhibit huge and complex changes as a function of the surface sensitivity of the technique. The analysis of the experimental data suggests that the two non-equivalent Sb sites possess different electronic structures and in each category, the Sb layers close to the surface are different from the bulk ones. An increase in temperature influences the Ce-Sb hybridization significantly. The plasmon-excitation-induced loss features are also observed in all core level spectra. All these results reveal the importance of Ce-Sb hybridizations and indicate that the complex renormalization of Ce-Sb hybridization may be the reason for the exotic electronic properties of this system.
description: 7 figures
On light surfaces in black hole thermodynamics
Creators: name: Pugliese, D.
name: Quevedo, H.
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We discuss the fundamentals of classical black hole (BH) thermodynamics in a new framework determined by light surfaces and their frequencies. This new approach allows us to study BH transitions inside the Kerr geometry. In the case of BHs, we introduce a new parametrization of the metric in terms of the maximum extractable rotational energy or, correspondingly, the irreducible mass, which is an alternative to the spin parametrization. It turns out that BH spacetimes with spins $a/M= \sqrt {8/9}$ and $a/M=1/\sqrt{2}$ show anomalies in the rotational energy extraction and surface gravity whereas the case $a/M=\sqrt{3}/2$ is of particular relevance to study the variations of the horizon area. We find the general conditions under which BH transitions can occur and express them in terms of the masses of the initial and final states. This shows that BH transitions in the Kerr geometry are not arbitrary but depend on the relationship between the mass and spin of the initial and final states. From an observational point of view, we argue that near the BH poles it is possible to detect photon orbits with frequencies that characterize the light surfaces analyzed in this work.
description: 23 double column pages, 12 multipanels figures, 1Table, To appear in EPJC
sj-docx-1-opp-10.1177_10781552211040725 - Supplemental material for Dangerous interaction of bitter melon (Momordica charantia) with pazopanib: A case of acute pancreatitis
Creators: name: Unsal, Oktay
name: Sütcüoğlu, Osman
name: Yazıcı, Ozan
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111299 Oncology and Carcinogenesis not elsewhere classified
subject: FOS: Clinical medicine
subject: 111599 Pharmacology and Pharmaceutical Sciences not elsewhere classified

description: Supplemental material, sj-docx-1-opp-10.1177_10781552211040725 for Dangerous interaction of bitter melon (Momordica charantia) with pazopanib: A case of acute pancreatitis by Oktay Unsal, Osman Sütcüoğlu and Ozan Yazıcı in Journal of Oncology Pharmacy Practice
Praktikum Iz Softverskih Alata U Elektronici
Creators: name: Pejovic, Predrag
Publisher: name: Zenodo
Year: 2017
Subjects: free software
GNU/Linux
LaTeX
GNU Octave
gnuplot
wxMaxima
Python

description: This document contains presentation slides for Software Tools in Electronics course (Serbian: "Praktikum iz softverskih alata u elektronici"). The course covers basic usage of Ubuntu GNU/Linux operating system, including some command line tools, LaTeX, GNU Octave, gnuplot, Maxima and wxMaxima, and some basic Python programming, with emphasis in PyLab and SymPy.
sj-docx-1-ijs-10.1177_10668969211022708 - Supplemental material for Metastatic Liver Tumors in Surgical Pathology: Impact of Contemporary Diagnostic and Therapeutic Paradigms in a Tertiary Care Center
Creators: name: Armutlu, Ayşe
name: Saeed, Omer
name: Saxena, Romil
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 111599 Pharmacology and Pharmaceutical Sciences not elsewhere classified
subject: FOS: Clinical medicine
subject: 110323 Surgery

description: Supplemental material, sj-docx-1-ijs-10.1177_10668969211022708 for Metastatic Liver Tumors in Surgical Pathology: Impact of Contemporary Diagnostic and Therapeutic Paradigms in a Tertiary Care Center by Ayşe Armutlu, Omer Saeed and Romil Saxena in International Journal of Surgical Pathology
Code and Data set for "Theory of Nonlinear Spectroscopy of Quantum Magnets"
Creators: name: Srivastava, Anubhav
name: Birnkammer, Stefan
name: Sim, GiBaik
name: Knap, Michael
name: Knolle, Johannes
Publisher: name: Zenodo
Year: 2025

description: Change: The codes in Selection_Rules folder of Supp_Mat_Code_Zenodo generate figure S5 in supplementary material. The codes in Selection_Rules had a typo in formula for \chi_2 section which has been fixed. Scaling of data set for figure S5 has been re-adjusted.

Code and datasets for the manuscript "Theory of Nonlinear Spectroscopy of Quantum Magnets". The codes and datasets for Main text and Supplementary mater are stored in separate folders. Instructions.doc is provided wherever necessary.

Important: The codes generating datasets have been parallelised using joblib to use all cores available. If this is inconvenient for the user, the user must change num_cores in respective section of each code.
Additional file 1 of Latent class analysis of actigraphy within the depression early warning (DEW) longitudinal clinical youth cohort
Creators: name: Sequeira, Lydia
name: Fadaiefard, Pantea
name: Seat, Jovana
name: Aitken, Madison
name: Strauss, John
name: Wang, Wei
name: Szatmari, Peter
name: Battaglia, Marco
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mental Health

description: Additional file1 (DOCX 30 kb)
sj-docx-1-pie-10.1177_09544089211043014 - Supplemental material for Effect of process parameters on the diesel engine performance fuelled with Prosopis juliflora biodiesel response surface methodology approach
Creators: name: Sharma, Abhishek
name: Tyagi, Avdhesh
name: Singh, Yashvir
name: Singh, Nishant K
name: Pandey, Navneet K
Publisher: name: SAGE Journals
Year: 2022
Subjects: subject: 99999 Engineering not elsewhere classified
subject: FOS: Other engineering and technologies
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, sj-docx-1-pie-10.1177_09544089211043014 for Effect of process parameters on the diesel engine performance fuelled with Prosopis juliflora biodiesel response surface methodology approach by Abhishek Sharma, Avdhesh Tyagi, Yashvir Singh, Nishant K Singh and Navneet K Pandey in Proceedings of the Institution of Mechanical Engineers, Part E: Journal of Process Mechanical Engineering
Additional file 1 of MR-GGI: accurate inference of gene–gene interactions using Mendelian randomization
Creators: name: Oh, Wonseok
name: Jung, Junghyun
name: Joo, Jong Wha J.
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Statistics
subject: FOS: Mathematics

description: Additional file 1. Figure 1. A directed acyclic graph for Mendelian randomization.
Solar Flare Heating with Turbulent Suppression of Thermal Conduction
Creators: name: Allred, Joel C.
name: Kerr, Graham S.
name: Emslie, A. Gordon
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: During solar flares plasma is typically heated to very high temperatures, and the resulting redistribution of energy via thermal conduction is a primary mechanism transporting energy throughout the flaring solar atmosphere. The thermal flux is usually modeled using Spitzer's theory, which is based on local Coulomb collisions between the electrons carrying the thermal flux and those in the background. However, often during flares, temperature gradients become sufficiently steep that the collisional mean free path exceeds the temperature gradient scale size, so that thermal conduction becomes inherently non-local. Further, turbulent angular scattering, which is detectable in nonthermal widths of atomic emission lines, can also act to increase the collision frequency and so suppress the heat flux. Recent work by Emslie & Bian (2018) extended Spitzer's theory of thermal conduction to account for both non-locality and turbulent suppression. We have implemented their theoretical expression for the heat flux (which is a convolution of the Spitzer flux with a kernel function) into the RADYN flare-modeling code and performed a parameter study to understand how the resulting changes in thermal conduction affect flare dynamics and hence the radiation produced. We find that models with reduced heat fluxes predict slower bulk flows, less intense line emission, and longer cooling times. By comparing features of atomic emission lines predicted by the models with Doppler velocities and nonthermal line widths deduced from a particular flare observation, we find that models with suppression factors between 0.3 to 0.5 relative to the Spitzer value best reproduce observed Doppler velocities across emission lines forming over a wide range of temperatures. Interestingly, the model that best matches observed nonthermal line widths has a kappa-type velocity distribution function.
description: Accepted by the Astrophysical Journal. 12 pages, 6 figures
sj-docx-1-heb-10.1177_10901981231159679 – Supplemental material for Predictors of Food and Physical Activity Tracking Among Young Adults
Creators: name: O’Loughlin, Erin K.
name: Marashi, Maryam
name: Sabiston, Catherine M.
name: Lucibello, Kristen M.
name: Sylvestre, Marie-Pierre
name: O’Loughlin, Jennifer L.
Publisher: name: SAGE Journals
Year: 2023
Subjects: subject: 111708 Health and Community Services
subject: FOS: Health sciences
subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology
subject: 110319 Psychiatry (incl. Psychotherapy)
subject: FOS: Clinical medicine
subject: 111799 Public Health and Health Services not elsewhere classified
subject: Sociology
subject: FOS: Sociology

description: Supplemental material, sj-docx-1-heb-10.1177_10901981231159679 for Predictors of Food and Physical Activity Tracking Among Young Adults by Erin K. O’Loughlin, Maryam Marashi, Catherine M. Sabiston, Kristen M. Lucibello, Marie-Pierre Sylvestre and Jennifer L. O’Loughlin in Health Education & Behavior
Sun-as-a-star spectroscopic observations of the line-of-sight velocity of a solar eruption on October 28, 2021
Creators: name: Xu, Yu
name: Tian, Hui
name: Hou, Zhenyong
name: Yang, Zihao
name: Gao, Yuhang
name: Bai, Xianyong
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: The propagation direction and true velocity of a solar coronal mass ejection, which are among the most decisive factors for its geo-effectiveness, are difficult to determine through single-perspective imaging observations. Here we show that Sun-as-a-star spectroscopic observations, together with imaging observations, could allow us to solve this problem. Using observations of the Extreme-ultraviolet Variability Experiment onboard the Solar Dynamics Observatory, we found clear blue-shifted secondary emission components in extreme ultraviolet spectral lines during a solar eruption on October 28, 2021. From simultaneous imaging observations, we found that the secondary components are caused by a mass ejection from the flare site. We estimated the line-of-sight (LOS) velocity of the ejecta from both the double Gaussian fitting method and the red-blue asymmetry analysis. The results of both methods agree well with each other, giving an average LOS velocity of the plasma of $\sim 423~\rm{km~s^{-1}}$. From the $304$ Å~image series taken by the Extreme Ultraviolet Imager onboard the Solar Terrestrial Relation Observatory-A (STEREO-A) spacecraft, we estimated the plane-of-sky (POS) velocity from the STEREO-A viewpoint {to be around $587~\rm{km~s^{-1}}$}. The full velocity of the bulk motion of the ejecta was then computed by combining the imaging and spectroscopic observations, which turns out to be around $596~\rm{km~s^{-1}}$ with an angle of $42.4^\circ$ to the west of the Sun-Earth line and $16.0^\circ$ south to the ecliptic plane.
description: accepted by ApJ
Additional file 1 of Contextualising the job demands–resources model: a cross-sectional study of the psychosocial work environment across different healthcare professions
Creators: name: Gynning, Britta Elsert
name: Karlsson, Elin
name: Teoh, Kevin
name: Gustavsson, Per
name: Christiansen, Filip
name: Brulin, Emma
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Supplementary Material 1.
sj-docx-1-nms-10.1177_14614448231157640 – Supplemental material for Shielding citizens? Understanding the impact of political advertisement transparency information
Creators: name: Dobber, Tom
name: Kruikemeier, Sanne
name: Helberger, Natali
name: Goodman, Ellen
Publisher: name: SAGE Journals
Year: 2023
Subjects: subject: 200199 Communication and Media Studies not elsewhere classified
subject: FOS: Media and communications

description: Supplemental material, sj-docx-1-nms-10.1177_14614448231157640 for Shielding citizens? Understanding the impact of political advertisement transparency information by Tom Dobber, Sanne Kruikemeier, Natali Helberger and Ellen Goodman in New Media & Society
Testing High-Energy Emission Models for Blazars with X-ray Polarimetry
Creators: name: Peirson, Abel L.
name: Liodakis, Ioannis
name: Romani, Roger W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Both leptonic and hadronic emission processes may contribute to blazar jet emission; which dominates in blazars's high energy emission component remains an open question. Some intermediate synchrotron peaked blazars transition from their low to high energy emission components in the X-ray band making them excellent laboratories to probe both components simultaneously, and good targets for the newly launched Imaging X-ray Polarimetry Explorer. We characterize the spectral energy distributions for three such blazars: CGRaBS~J0211+1051, TXS~0506+056, and S5~0716+714, predicting their X-ray polarization behavior by fitting a multizone polarized leptonic jet model. We find that a significant detection of electron synchrotron dominated polarization is possible with a 300~ks observation for S5~0716+714 and CGRaBS~J0211+1051 in their flaring states, while even 500~ks observations are unlikely to measure synchrotron self-Compton polarization. Importantly, non-leptonic emission processes like proton synchrotron are marginally detectable for our brightest ISP, S5~0716+714, during a flaring state. Improved {\it IXPE} data reduction methods or next generation telescopes like {\it eXTP} are needed to confidently measure SSC polarization.
description: Accepted to ApJ. 7 pages, 3 figures, 2 tables
Diagnostics for PopIII galaxies and Direct Collapse Black Holes in the early universe
Creators: name: Nakajima, K.
name: Maiolino, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Forthcoming observational facilities will make the exploration of the early universe routine, likely probing large populations of galaxies at very low metallicities. It will therefore be important to have diagnostics that can solidly identify and distinguish different classes of objects in such low metallicity regimes. We use new photoionisation models to develop diagnostic diagrams involving various nebular lines. We show that combinations of these diagrams allow the identification and discrimination of the following classes of objects in the early universe: PopIII and Direct Collapse Black Holes (DCBH) in pristine environments, PopIII and DCBH embedded in slightly enriched ISM (Z~10^{-5}-10^{-4}), (metal poor) PopII and AGN in enriched ISM. Diagnostics involving rest-frame optical lines (that will be accessible by JWST) have a better discriminatory power, but also rest-frame UV diagnostics can provide very useful information. Interestingly, we find that metal lines such as [OIII] 5007A and CIV 1549A can remain relatively strong (about a factor of 0.1-1 relative H-beta and HeII 1640A, respectively), even in extremely metal poor environments (Z~10^{-5}-10^{-4}), which could be embedding PopIII galaxies and DCBH.
description: 14 pages, 9 figures. Accepted for publication in MNRAS
sj-pdf-1-qjp-10.1177_17470218231163007 – Supplemental material for Recognition of facial expressions in autism: Effects of face masks and alexithymia
Creators: name: Gehdu, Bayparvah Kaur
name: Tsantani, Maria
name: Press, Clare
name: Gray, Katie LH
name: Cook, Richard
Publisher: name: SAGE Journals
Year: 2023
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Supplemental material, sj-pdf-1-qjp-10.1177_17470218231163007 for Recognition of facial expressions in autism: Effects of face masks and alexithymia by Bayparvah Kaur Gehdu, Maria Tsantani, Clare Press, Katie LH Gray and Richard Cook in Quarterly Journal of Experimental Psychology
Code and Data set for "Theory of Nonlinear Spectroscopy of Quantum Magnets"
Creators: name: Srivastava, Anubhav
name: Birnkammer, Stefan
name: Sim, GiBaik
name: Knap, Michael
name: Knolle, Johannes
Publisher: name: Zenodo
Year: 2025

description: Update: Please refer to version2 of the code. We have made some changes in the code generating figure S5(Symmetric and anti-symmetric channel for radiated electric field) in the Supplementary material

Code and datasets for the manuscript "Theory of Nonlinear Spectroscopy of Quantum Magnets". The codes and datasets for Main text and Supplementary mater are stored in separate folders. Instructions.doc is provided wherever necessary.

Important: The codes generating datasets have been parallelised using joblib to use all cores available. If this is inconvenient for the user, the user must change num_cores in respective section of each code.
Additional file 1 of The relation between resident-related factors and care problems in nursing homes: a multi-level analysis
Creators: name: Bouchmal, Suleyman
name: Goërtz, Yvonne M. J.
name: Hacking, Coen
name: Winkens, Bjorn
name: Aarts, Sil
Publisher: name: figshare
Year: 2024
Subjects: subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Supplementary Material 1.
sj-pdf-2-imr-10.1177_03000605231190453 - Supplemental material for Comparison of two joint-preserving treatments for osteonecrosis of the femoral head: core decompression and core decompression with additional cancellous bone grafting
Creators: name: Woerner, Michael
name: Voelkl, Korbinian
name: Bliemel, Christopher
name: Ferner, Felix
name: Weber, Markus
name: Renkawitz, Tobias
name: Grifka, Joachim
name: Craiovan, Benjamin
Publisher: name: SAGE Journals
Year: 2023
Subjects: subject: Health and Community Services
subject: Cardiology
subject: Dentistry not elsewhere classified
subject: Emergency Medicine
subject: Endocrinology
subject: Geriatrics and Gerontology
subject: Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: Nursing not elsewhere classified
subject: Nutrition and Dietetics not elsewhere classified
subject: Oncology and Carcinogenesis not elsewhere classified
subject: Orthopaedics
subject: Sports Medicine
subject: Otorhinolaryngology
subject: Aged Health Care
subject: Paediatrics
subject: Pharmacology and Pharmaceutical Sciences not elsewhere classified
subject: Psychology not elsewhere classified
subject: Psychiatry (incl. Psychotherapy)
subject: Public Health and Health Services not elsewhere classified
subject: Respiratory Diseases
subject: Sociological Methodology and Research Methods
subject: Surgery

description: Supplemental material, sj-pdf-2-imr-10.1177_03000605231190453 for Comparison of two joint-preserving treatments for osteonecrosis of the femoral head: core decompression and core decompression with additional cancellous bone grafting by Michael Woerner, Korbinian Voelkl, Christopher Bliemel, Felix Ferner, Markus Weber, Tobias Renkawitz, Joachim Grifka and Benjamin Craiovan in Journal of International Medical Research
Der Augustiner Felice Milensio als paepstlicher Berichtterstatter am Regensburger Reichstag des Jahres 1608
Creators: name: Piper, Anton
Publisher: name: Römische Quartalschrift
Year: 1970

description: Römische Quartalschrift, Bd. 5 (1891): Römische Quartalschrift, Band 5
Additional file 2 of The relation between resident-related factors and care problems in nursing homes: a multi-level analysis
Creators: name: Bouchmal, Suleyman
name: Goërtz, Yvonne M. J.
name: Hacking, Coen
name: Winkens, Bjorn
name: Aarts, Sil
Publisher: name: figshare
Year: 2024
Subjects: subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Supplementary Material 2.
D5.1.1 & D5.1.3 Regulatory review and CO₂ hazards
Creators: name: de Carvalho, Eric
name: Daniel, Guillaume
name: Etemad, Hamid
name: Leisner, Marius
name: Vroegrijk, Erik
Publisher: name: Zenodo
Year: 2023

description: The EverLoNG project aims to encourage the uptake of SBCC by demonstrating its use on board LNG-fuelled ships and moving it closer to market readiness. This report has been prepared to meet the requirements of EverLoNG project deliverables D5.1.1 and D5.1.3 and consists of three main sections:• Identify applicable safety and environmental standards and codes.• Major hazard of CO2 loss of containment• Assessment of technology novelty

The regulatory framework exists and is currently being expanded for the implementation of ship-based carbon capture (SBCC). The risks associated with SBCC installations are credible but well understood, with well-established safeguards and design principles available from other parts of the marine industry, like LNG-fuelled vessels. The authors hope with publicising this document, that designers, shipyards, ship-owners & -operators and reviewers obtain detailed insight in the risks associated with the technology, leading to inherently safer designs and a smooth approval process. In short, ship-based carbon capture can be implemented today.
A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor member HIP 94235
Creators: name: Zhou, George
name: Wirth, Christopher P.
name: Huang, Chelsea X.
name: Venner, Alexander
name: Franson, Kyle
name: Quinn, Samuel N.
name: Bouma, L. G.
name: Kraus, Adam L.
name: Mann, Andrew W.
name: Newton, Elisabeth. R.
name: Dragomir, Diana
name: Heitzmann, Alexis
name: Lowson, Nataliea
name: Douglas, Stephanie T.
name: Battley, Matthew
name: Gillen, Edward
name: Triaud, Amaury
name: Latham, David W.
name: Howell, Steve B.
name: Hartman, J. D.
name: Tofflemire, Benjamin M.
name: Wittenmyer, Robert A.
name: Bowler, Brendan P.
name: Horner, Jonathan
name: Kane, Stephen R.
name: Kielkopf, John
name: Plavchan, Peter
name: Wright, Duncan J.
name: Addison, Brett C.
name: Mengel, Matthew W.
name: Okumura, Jack
name: Ricker, George
name: Vanderspek, Roland
name: Seager, Sara
name: Jenkins, Jon M.
name: Winn, Joshua N.
name: Daylan, Tansu
name: Fausnaugh, Michael
name: Kunimoto, Michelle
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The TESS mission has enabled discoveries of the brightest transiting planet systems around young stars. These systems are the benchmarks for testing theories of planetary evolution. We report the discovery of a mini-Neptune transiting a bright star in the AB Doradus moving group. HIP 94235 (TOI-4399, TIC 464646604) is a Vmag=8.31 G-dwarf hosting a 3.00 -0.28/+0.32 Rearth mini-Neptune in a 7.7 day period orbit. HIP 94235 is part of the AB Doradus moving group, one of the youngest and closest associations. Due to its youth, the host star exhibits significant photometric spot modulation, lithium absorption, and X-ray emission. Three 0.06% transits were observed during Sector-27 of the TESS Extended Mission, though these transit signals are dwarfed by the 2% peak-to-peak photometric variability exhibited by the host star. Follow-up observations with CHEOPS confirmed the transit signal and prevented the erosion of the transit ephemeris. HIP 94235 is part of a 50 AU G-M binary system. We make use of diffraction limited observations spanning 11 years, and astrometric accelerations from Hipparchos and Gaia, to constrain the orbit of HIP 94235 B. HIP 94235 is one of the tightest stellar binaries to host an inner planet. As part of a growing sample of bright, young planet systems, HIP 94235 b is ideal for follow-up transit observations, such as those that investigate the evaporative processes driven by high-energy radiation that may sculpt the valleys and deserts in the Neptune population.
description: Accepted for publication in AJ
Wavelet analysis of MAXI J1535-571 with Insight-HXMT
Creators: name: Chen, X.
name: Wang, W.
name: You, B.
name: Tian, P. F.
name: Liu, Q.
name: Zhang, P.
name: Ding, Y. Z.
name: Qu, J. L.
name: Zhang, S. N.
name: Song, L. M.
name: Lu, F. J.
name: Zhang, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In this paper, wavelet analysis is used to study spectral-timing properties of MAXI J1535-571 observed by Insight-HXMT. The low-frequency quasi-periodic oscillations (QPOs) are detected in nine observations. Based on wavelet analysis, the time intervals with QPO and non-QPO are isolated separately, and the corresponding spectra with QPO and non-QPO are analyzed. We find that the spectra with QPO (hereafter QPO spectra) are softer than those without QPO (hereafter non-QPO spectra) in the hard intermediate state (HIMS). While in the soft intermediate state (SIMS), the QPO spectra are slightly harder. The disk temperature of QPO regime is slightly lower during HIMS, but becomes higher during SIMS. The cutoff energies of QPO spectra and non-QPO spectra do not show significant differences. The flux ratio of the disk to total flux is higher for the time intervals with non-QPO than that of QPO regime. We propose that these differences in the spectral properties between QPO and non-QPO regimes could be explained in the scenario of Lense-Thirring precession, and the reversal of the QPO/non-QPO behavior between HIMS and SIMS may be associated with appearance/disappearance of a type-B QPO which might origin from the precession of the jet.
description: 13 pages, 9 figures in main part, and 3 figures in the appendix; MNRAS in press, the first submission in 2021-06
Additional file 1 of Leveraging large-scale multi-omics evidences to identify therapeutic targets from genome-wide association studies
Creators: name: Lessard, Samuel
name: Chao, Michael
name: Reis, Kadri
name: Beauvais, Mathieu
name: Rajpal, Deepak K.
name: Sloane, Jennifer
name: Palta, Priit
name: Klinger, Katherine
name: de Rinaldis, Emanuele
name: Shameer, Khader
name: Chatelain, Clément
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Figure S1. Gold standard gene enrichment by genomic features. Figure S2. Precision and recall of gold standard genes for different genomic features as well as causal candidate prioritization approach. Figure S3. F1 scores for each considered features and prioritization scheme. Figure S4. Enriched colocalizing cell types and tissues by disease categories. Figure S5. Enrichment of clinical success stratified by GWAS source. Figure S6. Predicted directionality and drug mechanism of action stratified by GWAS source. Figure S7. Predicted direction of effect of gene expression on disease risk. Figure S8. Concordance between the predicted effect of gene expression on disease risk by MR and mMoA of approved drugs. Figure S9. Association between IL6 and diseases, supported by MR, colocalization and ABC. Figure S10. Association between IL6R and diseases, supported by MR, colocalization and ABC.
The Effects of Disk Induced Apsidal Precession on Planets Captured into Mean Motion Resonance
Creators: name: Murray, Zachary
name: Hadden, Sam
name: Holman, Matthew J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The process of migration into resonance capture has been well studied for planetary systems where the gravitational potential is generated exclusively by the star and planets. However, massive protoplanetary disks add a significant perturbation to these models. In this paper we consider two limiting cases of disk-induced precession on migrating planets and find that small amounts of precession significantly affect the equilibrium reached by migrating planets. We investigate these effects with a combination of semi-analytic models of the resonance and numerical integrations. We also consider the case of the disk's dispersal, which can excite significant libration amplitude and can cause ejection from resonance for large enough precession rates. Both of these effects have implications for interpreting the known exoplanet population and may prove to be important considerations as the population of well-characterized exoplanet systems continues to grow.
Supernovae and photoionizing feedback in spiral arm molecular clouds
Creators: name: Bending, Thomas J. R.
name: Dobbs, Clare L.
name: Bate, Matthew R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We explore the interplay between supernovae and the ionizing radiation of their progenitors in star forming regions. The relative contributions of these stellar feedback processes are not well understood, particularly on scales greater than a single star forming cloud. We focus predominantly on how they affect the interstellar medium. We re-simulate a 500 pc^2 region from previous work that included photoionization and add supernovae. Over the course of 10 Myr more than 500 supernovae occur in the region. The supernovae remnants cool very quickly in the absence of earlier photoionization, but form much larger and more spherical hot bubbles when photoionization is present. Overall, the photoionization has a significantly greater effect on gas morphology and the sites of star formation. However, the two processes are comparable when looking at their effect on velocity dispersion. When combined, the two feedback processes increase the velocity dispersions by more than the sum of their parts, particularly on scales above 5 pc.
description: 12 pages, 9 figures
Drag reduction on a transonic airfoil
Creators: name: Quadrio, Maurizio
name: Chiarini, Alessandro
name: Banchetti, Jacopo
name: Gatti, Davide
name: Memmolo, Antonio
name: Pirozzoli, Sergio
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Flow control for turbulent skin-friction drag reduction is applied to a transonic airfoil to improve its aerodynamic performance. The study is based on direct numerical simulations (with up to 1.8 billions cells) of the compressible turbulent flow around a supercritical airfoil, at Reynolds and Mach numbers of $Re_\infty= 3 \times 10^5$ and $M_\infty =0.7$. Control via spanwise forcing is applied over a fraction of the suction side of the airfoil. Besides locally reducing friction, the control modifies the shock wave and significantly improves the aerodynamic efficiency of the airfoil by increasing lift and decreasing drag. Hence, the airfoil can achieve the required lift at a lower angle of attack and with a lower drag. Estimates at the aircraft level indicate that substantial savings are possible; when control is active, its energy cost becomes negligible thanks to the small application area. We suggest that skin-friction drag reduction should be considered not only as a goal, but also as a tool to improve the global aerodynamics of complex flows.
Gravitational Effects on Quantum Coherence in Neutrino Oscillation
Creators: name: Ettefaghi, M. M.
name: Arani, R. Ramezani
name: Lotfi, Z. S. Tabatabaei
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper, we investigate the quantum coherence for two flavor neutrinos propagating in a Schwarzschild metric. In fact, this issue is explored both qualitatively via calculating the parameter $K_{3}$ in Leggett-Garg inequality (LGI) and also quantitatively by evaluating the $l_{1}$-norm, ${\cal C}(ρ)$. Using the weak field approximations, we show that the gravitational effects decrease the maximum value of $K_{3}$ for some intervals of energy such a way that there is no violation, while it leaves the maximum amount of the quantum coherence, ${\cal C}(ρ)$ unchanged.
description: 21 pages, 2 figures, to appear in Phys. Rev. D
Max Hermann (Hrsg.) / Siegfried Szamatolski (Hrsg.): Lateinische Literaturdenkmäler des XV. und XVI. Jahrhunderts
Creators: name: Schlecht, Joseph
Publisher: name: Römische Quartalschrift
Year: 1970

description: Römische Quartalschrift, Bd. 5 (1891): Römische Quartalschrift, Band 5
The SAMI Galaxy Survey: The Link Between [$α$/Fe] and Kinematic Morphology
Creators: name: Watson, Peter J.
name: Davies, Roger L.
name: van de Sande, Jesse
name: Brough, Sarah
name: Croom, Scott M.
name: D'Eugenio, Francesco
name: Glazebrook, Karl
name: Groves, Brent
name: López-Sánchez, Ángel R.
name: Scott, Nicholas
name: Vaughan, Sam P.
name: Walcher, C. Jakob
name: Bland-Hawthorn, Joss
name: Bryant, Julia J.
name: Goodwin, Michael
name: Lawrence, Jon S.
name: Lorente, Nuria P. F.
name: Owers, Matt S.
name: Richards, Samuel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We explore a sample of 1492 galaxies with measurements of the mean stellar population properties and the spin parameter proxy, $λ_{R_{\rm{e}}}$, drawn from the SAMI Galaxy Survey. We fit a global $\left[α/\rm{Fe}\right]$-$σ$ relation, finding that $\left[α/\rm{Fe}\right]=(0.395\pm0.010)\rm{log}_{10}\left(σ\right)-(0.627\pm0.002)$. We observe an anti-correlation between the residuals $Δ\left[α/\rm{Fe}\right]$ and the inclination-corrected $λ_{\,R_{\rm{e}}}^{\rm{\,eo}}$, which can be expressed as $Δ\left[α/\rm{Fe}\right]=(-0.057\pm0.008)λ_{\,R_{\rm{e}}}^{\rm{\,eo}}+(0.020\pm0.003)$. The anti-correlation appears to be driven by star-forming galaxies, with a gradient of $Δ\left[α/\rm{Fe}\right]\sim(-0.121\pm0.015)λ_{\,R_{\rm{e}}}^{\rm{\,eo}}$, although a weak relationship persists for the subsample of galaxies for which star formation has been quenched. We take this to be confirmation that disk-dominated galaxies have an extended duration of star formation. At a reference velocity dispersion of 200 km s$^{-1}$, we estimate an increase in half-mass formation time from $\sim$0.5 Gyr to $\sim$1.2 Gyr from low- to high-$λ_{\,R_{\rm{e}}}^{\rm{\,eo}}$ galaxies. Slow rotators do not appear to fit these trends. Their residual $α$-enhancement is indistinguishable from other galaxies with $λ_{\,R_{\rm{e}}}^{\rm{\,eo}}\lessapprox0.4$, despite being both larger and more massive. This result shows that galaxies with $λ_{\,R_{\rm{e}}}^{\rm{\,eo}}\lessapprox0.4$ experience a similar range of star formation histories, despite their different physical structure and angular momentum.
description: 12 pages, 9 figures
Additional file 1 of Extracellular vesicles produced by HIV-1 Nef-expressing cells induce myelin impairment and oligodendrocyte damage in the mouse central nervous system
Creators: name: Schenck, Jessica K.
name: Karl, Molly T.
name: Clarkson-Paredes, Cheryl
name: Bastin, Ashley
name: Pushkarsky, Tatiana
name: Brichacek, Beda
name: Miller, Robert H.
name: Bukrinsky, Michael I.
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Supplementary Material 1.
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Deriving Inclination Angle and Velocity of the Protostellar Jets from their SiO Knots
Creators: name: Jhan, Kai-Syun
name: Lee, Chin-Fei
name: Johnstone, Doug
name: Liu, Tie
name: Liu, Sheng-Yuan
name: Hirano, Naomi
name: Tatematsu, Kenichi
name: Dutta, Somnath
name: Moraghan, Anthony
name: Shang, Hsien
name: Lee, Jeong-Eun
name: Li, Shanghuo
name: Liu, Chun-Fan
name: Hsu, Shih-Ying
name: Kwon, Woojin
name: Sahu, Dipen
name: Liu, Xun-Chuan
name: Kim, Kee-Tae
name: Luo, Qiuyi
name: Qin, Sheng-Li
name: Sanhueza, Patricio
name: Bronfman, Leonardo
name: Qizhou, Zhang
name: Eden, David
name: Traficante, Alessio
name: Lee, Chang Won
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have selected six sources (G209.55-19.68S2, G205.46-14.56S1$_{-}$A, G203.21-11.20W2, G191.90-11.21S, G205.46-14.56S3, and G206.93-16.61W2) from the Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic Cold Clumps (ALMASOP), in which these sources have been mapped in the CO (J=2-1), SiO (J=5-4), and C$^{18}$O (J=2-1) lines. These sources have high-velocity SiO jets surrounded by low-velocity CO outflows. The SiO jets consist of a chain of knots. These knots have been thought to be produced by semi-periodical variations in jet velocity. Therefore, we adopt a shock-forming model, which uses such variations to estimate the inclination angle and velocity of the jets. We also derive the inclination angle of the CO outflows using the wide-angle wind-driven shell model, and find it to be broadly consistent with that of the associated SiO jets. In addition, we apply this shock-forming model to another three protostellar sources with SiO jets in the literature -- HH 211, HH 212, and L1448C(N) -- and find that their inclination angle and jet velocity are consistent with those previously estimated from proper motion and radial velocity studies.
Additional file 4 of Leveraging large-scale multi-omics evidences to identify therapeutic targets from genome-wide association studies
Creators: name: Lessard, Samuel
name: Chao, Michael
name: Reis, Kadri
name: Beauvais, Mathieu
name: Rajpal, Deepak K.
name: Sloane, Jennifer
name: Palta, Priit
name: Klinger, Katherine
name: de Rinaldis, Emanuele
name: Shameer, Khader
name: Chatelain, Clément
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4. Funding statements and references for all eQTL and pQTL datasets used for this manuscript.
Prof. Dr. Sepp: Die Religion der alten Deutschen und ihr Fortbestand in Volkssagen, Aufzügen und Festbräuchen bis zur Gegenwart, mit durchgreifender Religions-Vergleichung
Creators: name: Meister, Aloys
Publisher: name: Römische Quartalschrift
Year: 1970

description: Römische Quartalschrift, Bd. 5 (1891): Römische Quartalschrift, Band 5
Infrared study of the layered, magnetic insulator Mn(Bi$_{0.07}$Sb$_{0.93}$)$_2$Te$_4$ at low temperatures
Creators: name: Köpf, M.
name: Lee, S. H.
name: Kumar, H.
name: Mao, Z. Q.
name: Kuntscher, C. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Topological insulators with intrinsic magnetic ordering, potentially hosting rare quantum effects, recently attracted extensive attention. MnBi$_2$Te$_4$ is the first established example. The Sb-doped variant Mn(Bi$_{1-x}$Sb$_x$)$_2$Te$_4$ shows a great variety of electronic properties depending on the Sb content~$x$, such as shifts in the Fermi level and the Neel temperature $T_{\mathrm N}$, and the change of the free charge carrier type from $n$- to $p$-type at high Sb substitution ratios. Here, we investigate the effect of magnetic ordering on the bulk electronic structure of Mn(Bi$_{1-x}$Sb$_x$)$_2$Te$_4$ with high Sb content $x=0.93$ by temperature-dependent reflectivity measurements over a broad frequency range. We observe anomalies in the optical response across $T_{\mathrm N}$ when the antiferromagnetic order sets, which suggests a coupling between the magnetic ordering and the electronic structure of the material.
description: 7 pages, 4 figures
title: "Ritratto di uomo", Arte romana, inv. LXXVIb (ITA/EN)
title: Scheda catalogo digitale Borghese
titleType: AlternativeTitle
Creators: name: Clementi, Jessica
name: Galleria Borghese
Publisher: name: Galleria Borghese
Year: 2024

description: Pubblicazione delle schede delle opere conservate nel museo ed estratte dal catalogo digitale di Galleria Borghese, nelle due versioni esistenti online, in italiano e inglese.

Collegamento al catalogo digitale:

ITA: https://www.collezionegalleriaborghese.it/

EN: https://www.collezionegalleriaborghese.it/en