cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Sonnenfleckenzeichnung Nr. 29.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 10.02.1986, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Additional file 1: of Clinical classification of tissue perfusion based on the central venous oxygen saturation and the peripheral perfusion index
Creators: name: Huaiwu He
name: Long, Yun
name: Dawei Liu
name: Xiaoting Wang
name: Zhou, Xiang
Publisher: name: Figshare
Year: 2015
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Computational Biology

description: Results: difference between the patients with peripheral perfusion index (PI) â ¤0.6 and with PI >0.6 at 8Â h (T8) after resuscitation. (DOCX 19 kb)
COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
Creators: name: Brinch, Malte
name: Greve, Thomas R.
name: Weaver, John R.
name: Brammer, Gabriel
name: Ilbert, Olivier
name: Shuntov, Marko
name: Jin, Shuowen
name: Liu, Daizhong
name: Giménez-Arteaga, Clara
name: Casey, Caitlin M.
name: Davidson, Iary
name: Fujimoto, Seiji
name: Koekemoer, Anton M.
name: Kokorev, Vasily
name: Magdis, Georgios
name: McCracken, H. J.
name: McPartland, Conor J. R.
name: Mobasher, Bahram
name: Sanders, David B.
name: Toft, Sune
name: Valentino, Francesco
name: Zamorani, Giovanni
name: Zavala, Jorge
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We conduct a systematic search for protocluster candidates at $z \geq 6$ in the COSMOS field using the recently released COSMOS2020 source catalog. We select galaxies using a number of selection criteria to obtain a sample of galaxies that have a high probability of being inside a given redshift bin. We then apply overdensity analysis to the bins using two density estimators, a Weighted Adaptive Kernel Estimator and a Weighted Voronoi Tessellation Estimator. We have found 15 significant ($>4σ$) candidate galaxy overdensities across the redshift range $6\le z\le7.7$. The majority of the galaxies appear to be on the galaxy main sequence at their respective epochs. We use multiple stellar-mass-to-halo-mass conversion methods to obtain a range of dark matter halo mass estimates for the overdensities in the range of $\sim10^{11-13}\,M_{\rm \odot}$, at the respective redshifts of the overdensities. The number and the masses of the halos associated with our protocluster candidates are consistent with what is expected from the area of a COSMOS-like survey in a standard $Λ$CDM cosmology. Through comparison with simulation, we expect that all the overdensities at $z\simeq6$ will evolve into a Virgo-/Coma-like clusters at present (i.e., with masses $\sim 10^{14}-10^{15}\,M_{\rm \odot}$). Compared to other overdensities identified at $z \geq 6$ via narrow-band selection techniques, the overdensities presented appear to have $\sim10\times$ higher stellar masses and star-formation rates. We compare the evolution in the total star-formation rate and stellar mass content of the protocluster candidates across the redshift range $6\le z\le7.7$ and find agreement with the total average star-formation rate from simulations.
description: 52 pages, 32 figues, 18 tables, main text is 30 pages, appendix is 22 pages, to be published in ApJ
Surface oxides, carbides, and impurities on RF superconducting Nb and Nb3Sn: A comprehensive analysis
Creators: name: Sun, Zeming
name: Baraissov, Zhaslan
name: Dukes, Catherine A.
name: Dare, Darrah K.
name: Oseroff, Thomas
name: Thompson, Michael O.
name: Muller, David A.
name: Liepe, Matthias U.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: Applied Physics (physics.app-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Surface structures on radio-frequency (RF) superconductors are crucially important in determining their interaction with the RF field. Here we investigate the surface compositions, structural profiles, and valence distributions of oxides, carbides, and impurities on niobium (Nb) and niobium-tin (Nb3Sn) in situ under different processing conditions. We establish the underlying mechanisms of vacuum baking and nitrogen processing in Nb and demonstrate that carbide formation induced during high-temperature baking, regardless of gas environment, determines subsequent oxide formation upon air exposure or low-temperature baking, leading to modifications of the electron population profile. Our findings support the combined contribution of surface oxides and second-phase formation to the outcome of ultra-high vacuum baking (oxygen processing) and nitrogen processing. Also, we observe that vapor-diffused Nb3Sn contains thick metastable oxides, while electrochemically synthesized Nb3Sn only has a thin oxide layer. Our findings reveal fundamental mechanisms of baking and processing Nb and Nb3Sn surface structures for high-performance superconducting RF and quantum applications
Sonnenfleckenzeichnung Nr. 78.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.04.1986, 07:45, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Cooperative Change Detection for Online Power Quality Monitoring
Creators: name: Li, Shang
name: Wang, Xiaodong
Publisher: name: arXiv
Year: 2014
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper considers the real-time power quality monitoring in power grid systems. The goal is to detect the occurrence of disturbances in the nominal sinusoidal voltage/current signal as quickly as possible such that protection measures can be taken in time. Based on an autoregressive (AR) model for the disturbance, we propose a generalized local likelihood ratio (GLLR) detector which processes meter readings sequentially and alarms as soon as the test statistic exceeds a prescribed threshold. The proposed detector not only reacts to a wide range of disturbances, but also achieves lower detection delay compared to the conventional block processing method. Then we further propose to deploy multiple meters to monitor the power signal cooperatively. The distributed meters communicate wirelessly to a central meter, where the data fusion and detection are performed. In light of the limited bandwidth of wireless channels, we develop a level-triggered sampling scheme, where each meter transmits only one-bit each time asynchronously. The proposed multi-meter scheme features substantially low communication overhead, while its performance is close to that of the ideal case where distributed meter readings are perfectly available at the central meter.
In search of Majorana
Creators: name: Sarma, Sankar Das
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Majorana particles are the same as their antiparticle, and their analogues in condensed matter may be a platform for quantum computing. We describe the search for these modes in semiconductor heterostructures and how disorder is a limiting factor.
description: 17 pages, 4 figures
Additional file 2: of Network-based analysis of genetic variants associated with hippocampal volume in Alzheimerâ  s disease: a study of ADNI cohorts
Creators: name: Song, Ailin
name: Jingwen Yan
name: Sungeun Kim
name: Risacher, Shannon
name: Wong, Aaron
name: Saykin, Andrew
name: Shen, Li
name: Greene, Casey
Publisher: name: Figshare
Year: 2016
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Quantile-quantile plot showing the deviation of the distribution of p-values in the ADNI-2 dataset from the uniform expected under the null. We did not observe inflation of p-values for the ADNI-2 dataset. (PDF 77Â kb)
Jurisdictional remedies for corporate rights in Ukraine: Sub-standard remedies in corporate disputes
Creators: name: Kostruba, Anatoliy
Publisher: name: figshare
Year: 2022
Subjects: subject: 180121 Legal Practice, Lawyering and the Legal Profession
subject: FOS: Law
subject: 180107 Conflict of Laws (Private International Law)
subject: 180124 Property Law (excl. Intellectual Property Law)
subject: Law
subject: 180104 Civil Law and Procedure
subject: 180119 Law and Society
subject: 189999 Law and Legal Studies not elsewhere classified

description: In the context of the European integration processes taking place in Ukraine, there is a convergence of the national legal system with the legal principles and provisions of the European Union, including in the field of corporate legal relations. The main purpose of this study was an independent study of problematic issues that arise upon the implementation of sub-standard remedies in corporate disputes to develop author’s conclusions and recommendations to ensure sustainable and effective law enforcement practices. The methodological framework of this study included the principles of cognition of social phenomena in their historical development, interrelation, and interdependence, a dialectical approach to the study of theory and practice, the history and current state of law. The leading methods were historical, comparative legal, and dialectical. Based on the results of the investigation, the study covered the leading issues of the state of modern legal regulation of sub-standard remedies in corporate disputes in Ukraine; analysed the main issues of theoretical certainty regarding sub-standard remedies in corporate disputes and suggested new vectors of reforms concerning further improvement of law enforcement practice. The author’s conclusion on the need to ensure the unity of law enforcement practice by introducing changes to the legislation of Ukraine towards detailed regulation of sub-standard remedies in corporate disputes, which also correlates with the reformation vectors of development of Ukraine in the context of European integration, will become a stable basis for further scientific research and legislative transformations in the field under study.
Sonnenfleckenzeichnung Nr. 117.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.06.1986, 09:15, erstellt von Marco Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Stability of the cascading gauge theory de Sitter DFPs
Creators: name: Buchel, Alex
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study stability of the Dynamical Fixed Points (DFPs) of the cascading gauge theory at strong coupling in de Sitter space-time. We compute the spectra of the perturbative fluctuations and identify stable/unstable DFPs, characterized by the ratio of the strong coupling scale $Λ$ of the gauge theory and the Hubble constant $H$ of the background space-time. We discover a new phenomenon in the spectrum of gravitational fluctuations of a non-conformal holographic model: distinct branches of the fluctuations for $H\gg Λ$ coalesce for sufficiently low $\frac{H}Λ$, leading to the removal of some excited modes from the spectrum. We establish that, at least in a dual supergravity approximation, cascading gauge theory does not have a stable DFP for $H\in (H_{crit_1},H_{crit_2})$. Initial states of the theory for $H>H_{crit_2}$ evolve to a stable DFP with unbroken chiral symmetry; while for $H< H_{crit_1}$ the states evolve to a de Sitter vacuum with spontaneously broken chiral symmetry.
description: 90 pages, 14 figures
Symmetries for the 4HDM: extensions of cyclic groups
Creators: name: Shao, Jiazhen
name: Ivanov, Igor P.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Multi-Higgs models equipped with global symmetry groups, either exact or softly broken, offer a rich framework for constructions beyond the Standard Model and lead to remarkable phenomenological consequences. Knowing all the symmetry options within each class of models can guide its phenomenological exploration, as confirmed by the vast literature on the two- and three-Higgs-doublet models. Here, we begin a systematic study of finite non-abelian symmetry groups which can be imposed on the scalar sector of the four-Higgs-doublet model (4HDM) without leading to accidental symmetries. In this work, we derive the full list of such non-abelian groups available in the 4HDM that can be constructed as extensions of cyclic groups by their automorphism groups. This list is remarkably restricted but it contains cases which have not been previously studied. Since the methods we develop may prove useful for other classes of models, we present them in a pedagogical manner.
description: v2: 36 pages, 2 tables, additional clarifications, matches the published version
Thermal excitation of plasmons for near-field thermophotovoltaics
Creators: name: Guo, Yu
name: Molesky, Sean
name: Hu, Huan
name: Cortes, Cristian L.
name: Jacob, Zubin
Publisher: name: arXiv
Year: 2014
Subjects: subject: Optics (physics.optics)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The traditional approaches of exciting plasmons consist of using electrons (eg: electron energy loss spectroscopy) or light (Kretchman and Otto geometry) while more recently plasmons have been excited even by single photons. A different approach: thermal excitation of a plasmon resonance at high temperatures using alternate plasmonic media was proposed by S. Molesky et.al., Opt. Exp. 21.101, A96-A110, (2013). Here, we show how the long-standing search for a high temperature narrow band near-field emitter for thermophotovoltaics can be fulfilled by high temperature plasmonics. We also describe how to control Wein's displacement law in the near-field using high temperature epsilon-near-zero metamaterials. Finally, we show that our work opens up an interesting direction of research for the field of slow light: thermal emission control.
Sonnenfleckenzeichnung Nr. 273.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 29.11.1986, 08:30, erstellt von Marco Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Microscopic examinations of Co valences and spin states in electron-doped LaCoO$_{3}$
Creators: name: Tomiyasu, Keisuke
name: Koyama, Syun-Ichi
name: Watahiki, Masanori
name: Sato, Mika
name: Nishihara, Kazuki
name: Takahashi, Yuki
name: Onodera, Mitsugi
name: Iwasa, Kazuaki
name: Nojima, Tsutomu
name: Nojiri, Hiroyuki
name: Okamoto, Jun
name: Huang, Di-Jing
name: Yamasaki, Yuuichi
name: Nakao, Hironori
name: Murakami, Youichi
Publisher: name: arXiv
Year: 2015
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We studied the Co valences and spin states in electron-doped LaCo$_{1-y}$Te$_{y}$O$_3$ by measuring x-ray absorption spectra and electron spin resonance. The low-temperature insulating state involves the low-spin Co$^{3+}$ ($S=0$) and the high-spin Co$^{2+}$ state, which is described by $g=3.8$ and $j_{\rm eff}=1/2$. The results, in concurrence with the electron-hole asymmetry confirmed in electrical resistivity, coincide with a spin-blockade phenomenon in this system. Further, we discuss the $g$ factor in terms of the strong covalent-bonding nature and consider multiple origins of this phenomenon.
description: 7 pages, 5 figures, and 1 table
The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope -- IV. Aperture Masking Interferometry
Creators: name: Sivaramakrishnan, Anand
name: Tuthill, Peter
name: Lloyd, James P.
name: Greenbaum, Alexandra Z.
name: Thatte, Deepashri
name: Cooper, Rachel A.
name: Vandal, Thomas
name: Kammerer, Jens
name: Sanchez-Bermudez, Joel
name: Pope, Benjamin J. S.
name: Blakely, Dori
name: Albert, Loïc
name: Cook, Neil J.
name: Johnstone, Doug
name: Martel, André R.
name: Volk, Kevin
name: Soulain, Anthony
name: Artigau, Étienne
name: Lafrenière, David
name: Willott, Chris J.
name: Parmentier, Sébastien
name: Ford, K. E. Saavik
name: McKernan, Barry
name: Vila, M. Begoña
name: Rowlands, Neil
name: Doyon, René
name: Desdoigts, Louis
name: Fullerton, Alexander W.
name: De Furio, Matthew
name: Goudfrooij, Paul
name: Holfeltz, Sherie T.
name: LaMassa, Stephanie
name: Maszkiewicz, Michael
name: Meyer, Michael R.
name: Perrin, Marshall D.
name: Pueyo, Laurent
name: Sahlmann, Johannes
name: Sohn, Sangmo Tony
name: Teixeira, Paula S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The James Webb Space Telescope's Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3-5 \micron~wavelengths, and a bright limit of $\simeq 4$ magnitudes in W2. We describe the NIRISS Aperture Masking Interferometry (AMI) mode to help potential observers understand its underlying principles, present some sample science cases, explain its operational observing strategies, indicate how AMI proposals can be developed with data simulations, and how AMI data can be analyzed. We also present key results from commissioning AMI. Since the allied Kernel Phase Imaging (KPI) technique benefits from AMI operational strategies, we also cover NIRISS KPI methods and analysis techniques, including a new user-friendly KPI pipeline. The NIRISS KPI bright limit is $\simeq 8$ W2 magnitudes. AMI (and KPI) achieve an inner working angle of $\sim 70$ mas that is well inside the $\sim 400$ mas NIRCam inner working angle for its circular occulter coronagraphs at comparable wavelengths.
description: 30 pages, 10 figures
Additional file 1: Table S2. of Telomere shortening leads to an acceleration of synucleinopathy and impaired microglia response in a genetic mouse model
Creators: name: Scheffold, Annika
name: Holtman, Inge
name: Dieni, Sandra
name: Nieske Brouwer
name: Sarah-Fee Katz
name: Jebaraj, Billy
name: Kahle, Philipp
name: Hengerer, Bastian
name: AndrĂŠ Lechel
name: Stilgenbauer, Stephan
name: Boddeke, Erik
name: Eggen, Bart
name: Karl-Lenhard Rudolph
name: Biber, Knut
Publisher: name: Figshare
Year: 2016
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Plant Biology
subject: 60506 Virology

description: Primer sequences which were used for RT-PCR. (DOC 40 kb)
HAHE: Hierarchical Attention for Hyper-Relational Knowledge Graphs in Global and Local Level
Creators: name: Luo, Haoran
name: E, Haihong
name: Yang, Yuhao
name: Guo, Yikai
name: Sun, Mingzhi
name: Yao, Tianyu
name: Tang, Zichen
name: Wan, Kaiyang
name: Song, Meina
name: Lin, Wei
Publisher: name: arXiv
Year: 2023
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Link Prediction on Hyper-relational Knowledge Graphs (HKG) is a worthwhile endeavor. HKG consists of hyper-relational facts (H-Facts), composed of a main triple and several auxiliary attribute-value qualifiers, which can effectively represent factually comprehensive information. The internal structure of HKG can be represented as a hypergraph-based representation globally and a semantic sequence-based representation locally. However, existing research seldom simultaneously models the graphical and sequential structure of HKGs, limiting HKGs' representation. To overcome this limitation, we propose a novel Hierarchical Attention model for HKG Embedding (HAHE), including global-level and local-level attention. The global-level attention can model the graphical structure of HKG using hypergraph dual-attention layers, while the local-level attention can learn the sequential structure inside H-Facts via heterogeneous self-attention layers. Experiment results indicate that HAHE achieves state-of-the-art performance in link prediction tasks on HKG standard datasets. In addition, HAHE addresses the issue of HKG multi-position prediction for the first time, increasing the applicability of the HKG link prediction task. Our code is publicly available.
description: Accepted by ACL 2023 main conference
Detection of a large fraction of atomic gas not associated with star-forming material in M17 SW
Creators: name: Perez-Beaupuits, J. P.
name: Stutzki, J.
name: Ossenkopf, V.
name: Spaans, M.
name: Gusten, R.
name: Wiesemeyer, H.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We probe the column densities and masses traced by the ionized and neutral atomic carbon with spectrally resolved maps, and compare them to the diffuse and dense molecular gas traced by [C I] and low-$J$ CO lines toward the star-forming region M17SW. We mapped a 4.1pc x 4.7pc region in the [C I] 609 m$μ$ line using the APEX telescope, as well as the CO isotopologues with the IRAM 30m telescope. We analyze the data based on velocity channel maps that are 1 km/s wide. We correlate their spatial distribution with that of the [C II] map obtained with SOFIA/GREAT. Optically thin approximations were used to estimate the column densities of [C I] and [C II] in each velocity channel. The spatial distribution of the [C I] and all CO isotopologues emission was found to be associated with that of [C II] in about 20%-80% of the mapped region, with the high correlation found in the central (15-23 km/s ) velocity channels. The excitation temperature of [C I] ranges between 40 K and 100 K in the inner molecular region of M17 SW. Column densities in 1 km/s channels between ~10$^{15}$ and ~10$^{17}$ cm$^{-2}$ were found for [C I]. Just ~20% of the velocity range (~40 km/s) that the [C II] line spans is associated with the star-forming material traced by [C I] and CO. The total gas mass estimated from the [C II] emission gives a lower limit of ~4.4x10$^3$ $M_{\odot}$. At least 64% of this mass is not associated with the star-forming material in M17SW. We also found that about 36%, 17%, and 47% of the [C II] emission is associated with the HII, HI, and H_2 regimes, respectively. Comparisons with the H41$α$ line shows an ionization region mixed with the neutral and part of the molecular gas, in agreement with the clumped structure and dynamical processes at play in M17SW. These results are also relevant to extra-galactic studies in which [C II] is often used as a tracer of star-forming material.
description: 21 pages + 6 pages of appendix, 32 figures in total, accepted for publication on A&A (10/12/2014) Relevant calibrated data cubes are available on CDS
Maxwell-scalar system and scalar field with impurity: novel approach to find nontrivial solutions
Creators: name: Andrade, I.
name: Bazeia, D.
name: Marques, M. A.
name: Menezes, R.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work, we investigate a Maxwell-scalar model that couples the scalar and gauge fields through the electric permittivity and another model, in which the scalar field lives in the presence of impurity. By considering a single spatial dimension, we determine the conditions under which the model with impurity can be seen as an effective model for the Maxwell-scalar system, having similar solutions. This correspondence shows that the impurity can be used to describe the presence of a charge density, and we use it to verify that the impurity-free case, which supports minimum energy configurations, is related to the case of point charges. We also investigate a class of impurities which modifies the core of the scalar field, and find the corresponding nontrivial charge densities and electric fields. In particular, the asymptotic behavior in terms of the impurity is also studied, leading to solutions exhibiting long-range or quasi-compact profile.
description: 30 pages, 6 figures; title changed, new text and references added. To appear in Chaos, Solitons and Fractals
Sonnenfleckenzeichnung Nr. 190.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 22.08.1986, 07:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Major Statistical Series of the U.S. Department of Agriculture: How They Are Constructed and Used
Creators: name: Agricultural Marketing Service
name: Agricultural Research Service
name: Farmer Cooperative Service
name: Foreign Agricultural Service
name: Agricultural Marketing Service
name: Agricultural Research Service
name: Farmer Cooperative Service
name: Foreign Agricultural Service
Publisher: name: Unknown
Year: 1957
Subjects: Agricultural and Food Policy
Research Methods/ Statistical Methods

description: Vol. 1 : Agricultural Prices and Parity. Vol. 2 : Agricultural Production and Efficiency. Vol. 3 : Gross and Net Farm Income. Vol. 4 : Agricultural Marketing Costs and Charges. Vol. 5 : Consumption and Utilization of Agricultural Products. Vol. 6 : Land Values and Farm Finance. Vol. 7 : Farm Population, Employment, and Levels of Living. Vol. 8 : Crop and Livestock. Vol. 9 : Farmer Cooperatives. Vol. 10: Market News.
Long-lived heavy neutral leptons with a displaced shower signature at CMS
Creators: name: Cottin, Giovanna
name: Helo, Juan Carlos
name: Hirsch, Martin
name: Peña, Cristián
name: Wang, Christina
name: Xie, Si
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the LHC discovery potential in the search for heavy neutral leptons (HNL) with a new signature: a displaced shower in the CMS muon detector, giving rise to a large cluster of hits forming a displaced shower. A new Delphes module is used to model the CMS detector response for such displaced decays. We reinterpret a dedicated CMS search for neutral long-lived particles decaying in the CMS muon endcap detectors for the minimal HNL scenario. We demonstrate that this new strategy is particularly sensitive to active-sterile mixings with $τ$ leptons, due to hadronic $τ$ decays. HNL masses between $\sim 1 - 6$ GeV can be accessed for mixings as low as $|V_{τN}|^{2}\sim 10^{-7}$, probing unique regions of parameter space in the $τ$ sector.
description: 16 pages, 3 figures. Minor edits in v2 and extra references; matches version accepted for publication in JHEP
MOESM1 of GAGA factor, a positive regulator of global gene expression, modulates transcriptional pausing and organization of upstream nucleosomes
Creators: name: Tsai, Shih-Ying
name: Yuh-Long Chang
name: Swamy, Krishna
name: Ruei-Lin Chiang
name: Der-Hwa Huang
Publisher: name: Figshare
Year: 2016
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 1. Figure S1. Analyses of RNA-Pol in Gaf mutants. Figure S2. RNA-Pol Hypo-p and Ser-2p are not affected by GAF on polytene chromosomes. Figure S3. Comparison of GAF target genes identified in different reports. Figure S4. Verification of gene expression by microarray studies. Figure S5. Procedures of statistical analyses of GAF and RNA-Pol ChIP-seq data. Figure S6. The abundance of different GAF binding motifs among targets. Figure S7. Reduction promoterproximal RNA-Pol in the Gaf mutant. Figure S8. Comparison of paused genes identified in different reports. Figure S9. Comparion of nucleosome profiles. Figure S10. Analyses of GAFâ  s effects on eye development. Figure S11. Comparison of target genes for GAF, NELF and NURF.
Cosmological simulations with disformally coupled symmetron fields
Creators: name: Hagala, R.
name: Llinares, C.
name: Mota, D. F.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate statistical properties of the distribution of matter at redshift zero in disformal gravity by using N-body simulations. The disformal model studied here consists of a conformally coupled symmetron field with an additional exponential disformal term. We conduct cosmological simulations to discover the impact of the new disformal terms in the matter power spectrum, halo mass function, and radial profile of the scalar field. We calculated the disformal geodesic equation and the equation of motion for the scalar field. We then implemented these equations into the N-body code ISIS, which is a modified gravity version of the code RAMSES. The presence of a conformal symmetron field increases both the power spectrum and mass function compared to standard gravity on small scales. Our main finding is that the newly added disformal terms tend to counteract these effects and can make the evolution slightly closer to standard gravity. We finally show that the disformal terms give rise to oscillations of the scalar field in the centre of the dark matter haloes.
description: Updated version to reflect the journal accepted paper. Added one figure. 7 pages, 7 figures
Sonnenfleckenzeichnung Nr. 123.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.06.1986, 08:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Investigating Primordial Black Hole Dark Matter with 16 years of SPI data
Creators: name: Berteaud, Joanna
name: Calore, Francesca
name: Iguaz, Joaquim
name: Serpico, Pasquale Dario
name: Siegert, Thomas
Publisher: name: Zenodo
Year: 2022
Subjects: dark matter
primordial black holes
SPI
diffuse MeV emission

description: Dark matter (DM), while accounting for more than 68% of the energy density of the Universe, still keeps its nature secret. Many candidates have been put forward, sharing one similarity: being massive, in order to reproduce the observed gravitational effects attributed to DM. The higher end of the mass scale discloses non-particle theoretical candidates: Primordial Black Holes (PBHs). Microlensing and gravitational waves, among other probes, already helped constraining the PBH contribution to DM for masses from 10^22 to 10^35 g, but the asteroid mass range, from 10^17 to 10^22 g, remains mostly unconstrained. In this talk, I will present how the diffuse Galactic MeV emission, newly determined by Siegert et al. (2022) from 16 years of SPI data, helped us stretching up the constraints into the asteroid mass range. Using the predictions for black hole evaporation, we demonstrated that PBHs cannot account for all the DM if their mass is smaller than 4x10^17 g.
Ultrafast dynamic conductivity and scattering rate saturation of photoexcited charge carriers in silicon investigated with a midinfrared continuum probe
Creators: name: Meng, Fanqi
name: Thomson, Mark D.
name: Sernelius, Bo E.
name: Jörger, Michael
name: Roskos, Hartmut G.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We employ ultra-broadband terahertz-midinfrared probe pulses to characterize the optical response of photoinduced charge-carrier plasmas in high-resistivity silicon in a reflection geometry, over a wide range of excitation densities (10^{15}-10^{19} cm^{-3}) at room temperature. In contrast to conventional terahertz spectroscopy studies, this enables one to directly cover the frequency range encompassing the resultant plasma frequencies. The intensity reflection spectra of the thermalized plasma, measured using sum-frequency (up-conversion) detection of the probe pulses, can be modeled well by a standard Drude model with a density-dependent momentum scattering time of approx. 200 fs at low densities, reaching approx. 20 fs for densities of approx. 10^{19} cm^{-3}, where the increase of the scattering rate saturates. This behavior can be reproduced well with theoretical results based on the generalized Drude approach for the electron-hole scattering rate, where the saturation occurs due to phase-space restrictions as the plasma becomes degenerate. We also study the initial sub-picosecond temporal development of the Drude response, and discuss the observed rise in the scattering time in terms of initial charge-carrier relaxation, as well as the optical response of the photoexcited sample as predicted by finite-difference time-domain simulations.
description: 9 pages, 4 figures
The Near Infrared Imager and Slitless Spectrograph for JWST -- V. Kernel Phase Imaging and Data Analysis
Creators: name: Kammerer, Jens
name: Cooper, Rachel A.
name: Vandal, Thomas
name: Thatte, Deepashri
name: Martinache, Frantz
name: Sivaramakrishnan, Anand
name: Chaushev, Alexander
name: Stolker, Tomas
name: Lloyd, James P.
name: Albert, Loïc
name: Doyon, René
name: Sallum, Steph
name: Perrin, Marshall D.
name: Pueyo, Laurent
name: Mérand, Antoine
name: Gallenne, Alexandre
name: Greenbaum, Alexandra
name: Sanchez-Bermudez, Joel
name: Blakely, Dori
name: Johnstone, Doug
name: Volk, Kevin
name: Martel, Andre
name: Goudfrooij, Paul
name: Meyer, Michael R.
name: Willott, Chris J.
name: De Furio, Matthew
name: Dang, Lisa
name: Radica, Michael
name: Noirot, Gaël
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Kernel phase imaging (KPI) enables the direct detection of substellar companions and circumstellar dust close to and below the classical (Rayleigh) diffraction limit. We present a kernel phase analysis of JWST NIRISS full pupil images taken during the instrument commissioning and compare the performance to closely related NIRISS aperture masking interferometry (AMI) observations. For this purpose, we develop and make publicly available the custom "Kpi3Pipeline" enabling the extraction of kernel phase observables from JWST images. The extracted observables are saved into a new and versatile kernel phase FITS file (KPFITS) data exchange format. Furthermore, we present our new and publicly available "fouriever" toolkit which can be used to search for companions and derive detection limits from KPI, AMI, and long-baseline interferometry observations while accounting for correlated uncertainties in the model fitting process. Among the four KPI targets that were observed during NIRISS instrument commissioning, we discover a low-contrast (~1:5) close-in (~1 $λ/D$) companion candidate around CPD-66~562 and a new high-contrast (~1:170) detection separated by ~1.5 $λ/D$ from 2MASS~J062802.01-663738.0. The 5-$σ$ companion detection limits around the other two targets reach ~6.5 mag at ~200 mas and ~7 mag at ~400 mas. Comparing these limits to those obtained from the NIRISS AMI commissioning observations, we find that KPI and AMI perform similar in the same amount of observing time. Due to its 5.6 times higher throughput if compared to AMI, KPI is beneficial for observing faint targets and superior to AMI at separations >325 mas. At very small separations (<100 mas) and between ~250-325 mas, AMI slightly outperforms KPI which suffers from increased photon noise from the core and the first Airy ring of the point-spread function.
description: 34 pages, 17 figures, accepted for publication in PASP
Additional file 3: of Feasibility of controlling hookworm infection through preventive chemotherapy: a simulation study using the individual-based WORMSIM modelling framework
Creators: name: Coffeng, Luc
name: Bakker, Roel
name: Montresor, Antonio
name: Vlas, Sake De
Publisher: name: Figshare
Year: 2015
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Computational Biology

description: Methods and results of analyses for sampling error in Kato-Katz slides and the association between mean and aggregation of egg counts in populations. (PDF 1238 kb)
MOESM4 of Avian Tembusu virus infection effectively triggers host innate immune response through MDA5 and TLR3-dependent signaling pathways
Creators: name: Shilong Chen
name: Guifeng Luo
name: Yang, Zhou
name: Shuncheng Lin
name: Shaoying Chen
name: Wang, Song
name: Mohsan Goraya
name: Xiaojuan Chi
name: Xiancheng Zeng
name: Chen, Ji-Long
Publisher: name: Figshare
Year: 2016
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology
subject: Computational Biology

description: Additional file 4 ATMUV infection causes significant up-regulation of TLR3 and MDA5. RT-PCR was performed to examine the mRNA expression of TLR3 and MDA5 in CEF (A), chickens (B) and 293T cells (C) at the indicated time after ATMUV infection, respectively.
The interaction of transmission intensity, mortality, and the economy: a retrospective analysis of the COVID-19 pandemic
Creators: name: Morgenstern, Christian
name: Laydon, Daniel J.
name: Whittaker, Charles
name: Mishra, Swapnil
name: Haw, David
name: Bhatt, Samir
name: Ferguson, Neil M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Applications (stat.AP)
subject: Machine Learning (cs.LG)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: The COVID-19 pandemic has caused over 6.4 million registered deaths to date and has had a profound impact on economic activity. Here, we study the interaction of transmission, mortality, and the economy during the SARS-CoV-2 pandemic from January 2020 to December 2022 across 25 European countries. We adopt a Bayesian Mixed Effects model with auto-regressive terms. We find that increases in disease transmission intensity decreases Gross domestic product (GDP) and increases daily excess deaths, with a longer lasting impact on excess deaths in comparison to GDP, which recovers more rapidly. Broadly, our results reinforce the intuitive phenomenon that significant economic activity arises from diverse person-to-person interactions. We report on the effectiveness of non-pharmaceutical interventions (NPIs) on transmission intensity, excess deaths, and changes in GDP, and resulting implications for policy makers. Our results highlight a complex cost-benefit trade off from individual NPIs. For example, banning international travel increases GDP and reduces excess deaths. We consider country random effects and their associations with excess changes in GDP and excess deaths. For example, more developed countries in Europe typically had more cautious approaches to the COVID-19 pandemic, prioritising healthcare, and excess deaths over economic performance. Long term economic impairments are not fully captured by our model, as well as long term disease effects (Long Covid). Our results highlight that the impact of disease on a country is complex and multifaceted, and simple heuristic conclusions to extract the best outcome from the economy and disease burden are challenging.
Light Higgsino Decays as a Probe of the NMSSM
Creators: name: Dutta, Bhaskar
name: Gao, Yu
name: Shakya, Bibhushan
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: In the Next-to Minimal Supersymmetric Standard Model (NMSSM), a sizable coupling $λ$ between the singlet and Higgs fields can naturally accommodate the observed Higgs boson mass of 125 GeV. This large coupling also results in a large separation between the Higgsino and singlino mass scales in the neutralino sector to evade stringent constraints from direct detection experiments. Most of the natural parameter space in this setup therefore contains light Higgsinos that can decay into the singlino and the 125 GeV Higgs. If the Higgsinos are to be light enough to be produced at the LHC, the mass gap $m_{\tildeχ^0_2} -(m_{\tildeχ^0_1} +m_h)$ is generally fairly low, resulting in small missing energy. We study the collider phenomenology of this process and demonstrate that the 4$b+j+{E\!\!\!\!/_{\rm T}}$ signal arising from $pp\rightarrow\tildeχ_i^0\tildeχ_j^0jj$ process can be a viable channel to search for this low mass gap region at the 14 TeV LHC. In addition, we find that a potential signal from the LHC search, in tandem with direct detection experiments, can distinguish the NMSSM from the analogous process in the MSSM, where the bino plays the role of the singlino, for positive values of the $μ$ parameter even when the additional singlet-dominated (pseudo)scalars are absent or indistinguishable from the Higgs in the decay.
description: 10 pages, 5 figures, 2 tables
Sonnenfleckenzeichnung Nr. 261.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 12.11.1986, 11:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1986

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)