cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Bulk superconductivity and role of fluctuations in the iron-based superconductor FeSe at high pressures
Creators: name: Gati, Elena
name: Böhmer, Anna E.
name: Bud'ko, Sergey L.
name: Canfield, Paul C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The iron-based superconductor FeSe offers a unique possibility to study the interplay of superconductivity with purely nematic as well magnetic-nematic order by pressure (p) tuning. By measuring specific heat under p up to 2.36GPa, we study the multiple phases in FeSe using a thermodynamic probe. We conclude that superconductivity is bulk across the entire p range and competes with magnetism. Our analysis suggests that superconducting and magnetic fluctuations exist over a wide temperature range above the respective bulk transition temperatures, whenever magnetism is present. These observations highlight similarities between FeSe and underdoped cuprate superconductors where fluctuations play a crucial role.
description: 7 pages, 4 figures + Supplementary Information
Additional file 1 of Prevalence of visceral artery involvement in patients with peripheral artery disease found on run-off MRA
Creators: name: Streckenbach, Felix
name: Meinel, Felix G.
name: Ammermann, Felix
name: Busse, Anke
name: Neumann, Andreas
name: Heller, Thomas
name: Weber, Marc-André
name: Beller, Ebba
Publisher: name: figshare
Year: 2021
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Marine Biology
subject: Hematology

description: Additional file 1: Supplementary Table 1. Visceral artery stenosis comparing tertiles of age groups.
The Chandra Deep Field-North Survey. XVI. The X-ray properties of moderate-luminosity Active Galaxies at z>4
Creators: name: Vignali, C.
name: Bauer, F. E.
name: Alexander, D. M.
name: Brandt, W. N.
name: Hornschemeier, A. E.
name: Schneider, D. P.
name: Garmire, G. P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present X-ray spectral analyses of the three z>4 Active Galactic Nuclei (AGNs) thus far spectroscopically identified in the Chandra Deep Field-North Survey, at redshifts of 5.186, 4.424, and 4.137. These analyses are made possible by the extremely deep exposure (2 Ms) and the low Chandra background. The rest-frame 2.5-40 keV spectra are the first for optically faint (two of the three sources have I>24) z>4 AGNs. The z=5.186 quasar is well fitted by a power-law model with photon index Gamma=1.8+/-0.3, consistent with those of lower-redshift, unobscured AGNs. The other two AGNs have flatter effective X-ray photon indices (Gamma approx 1.1-1.5), suggesting the presence of intrinsic absorption (provided their underlying X-ray continua are similar to those of lower-redshift AGNs). It is possible that the flat X-ray continuum of the z=4.424 AGN is partially related to its radio loudness. If the z=4.137 AGN suffers from X-ray absorption, the implied column density is N_H=2x10^23 cm^-2.
description: 4 pages, 3 figures, 2 tables, LaTeX emulateapj5.sty. Accepted for publication by The Astrophysical Journal Letters
Dusty Debris Around Solar-Type Stars: Temporal Disk Evolution
Creators: name: Spangler, C.
name: Sargent, A. I.
name: Silverstone, M. D.
name: Becklin, E. E.
name: Zuckerman, B.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using ISO-ISOPHOT we carried out a survey of almost 150 stars to search for evidence of emission from dust orbiting young main sequence stars, both in clusters and isolated systems. Over half of the detections are new examples of dusty stellar systems, and demonstrate that such dust can be detected around numerous stars older than a few x 10^6 years. Fluxes at 60 microns and either 90 or 100 microns for the new excess sources together with improved fluxes for a number of IRAS-identified sources are presented. Analysis of the excess luminosity relative to the stellar photosphere shows a systematic decline of this excess with stellar age consistent with a power law index of -2.
description: 33 pages, 3 figures, 7 tables; accepted for publication in ApJ
Additional file 3 of Evaluating implementation of the Transparency and Openness Promotion (TOP) guidelines: the TRUST process for rating journal policies, procedures, and practices
Creators: name: Mayo-Wilson, Evan
name: Grant, Sean
name: Supplee, Lauren
name: Kianersi, Sina
name: Amin, Afsah
name: DeHaven, Alex
name: Mellor, David
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Science Policy

description: Additional file 3.
Additional file 2 of Evaluating implementation of the Transparency and Openness Promotion (TOP) guidelines: the TRUST process for rating journal policies, procedures, and practices
Creators: name: Mayo-Wilson, Evan
name: Grant, Sean
name: Supplee, Lauren
name: Kianersi, Sina
name: Amin, Afsah
name: DeHaven, Alex
name: Mellor, David
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Science Policy

description: Additional file 2.
Additional file 1 of Evaluating implementation of the Transparency and Openness Promotion (TOP) guidelines: the TRUST process for rating journal policies, procedures, and practices
Creators: name: Mayo-Wilson, Evan
name: Grant, Sean
name: Supplee, Lauren
name: Kianersi, Sina
name: Amin, Afsah
name: DeHaven, Alex
name: Mellor, David
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Science Policy

description: Additional file 1.
PSR J1740-5340: accretion inhibited by radio-ejection in a binary millisecond pulsar in the Globular Cluster NGC 6397
Creators: name: Burderi, Luciano
name: D'Antona, Francesca
name: Burgay, Marta
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an evolutionary scenario for the spin-up and evolution of binary millisecond pulsars, according to which the companion of the pulsar PSR J 1740-5340, recently discovered as a binary with orbital period of 32.5 hr in the Globular Cluster NGC 6397, is presently in a phase of ``radio-ejection'' mass loss from the system. At present, Roche lobe overflow due to the nuclear evolution of the pulsar companion and to systemic angular momentum losses by magnetic braking is still going on, but accretion is inhibited by the momentum exerted by the radiation of the pulsar on the matter at the inner Lagrangian point. The presence of this matter around the system is consistent with the long lasting irregular radio eclipses seen in the system. Roche lobe deformation of the mass losing component is also necessary to be compatible with the optical light curve. The "radio-ejection" phase had been recently postulated by us to deal with the problem of the lack of submillisecond pulsars (Burderi et al. 2001, ApJ, 560, L71).
description: Accepted for publication in The Astrophysical Journal
Pharmacokinetic similarity study comparing the biosimilar candidate, LY05008, with its reference product dulaglutide in healthy Chinese male subjects
Creators: name: Zhang, Qin
name: Sun, Cheng
name: Wu, Jinying
name: Wu, Juan
name: Zhang, Xuan
name: Liu, Yueyue
name: Dou, Changlin
name: Qin, Huilin
name: Zhang, Qian
name: Zhou, Renpeng
name: Hu, Wei
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Mathematical Sciences not elsewhere classified
subject: Mental Health

description: Dulaglutide, a glucagon-like peptide-1 (GLP-1) receptor agonist, has been approved for improving glycemic control and reducing the risk of cardiovascular (CV) adverse events. This study compared the pharmacokinetic (PK) profiles, safety, and immunogenicity of LY05008, a biosimilar candidate, to a licensed product dulaglutide in healthy Chinese male subjects. In this double-blind, open-label, parallel-group study, healthy Chinese male subjects were randomized 1:1 to receive either LY05008 or dulaglutide subcutaneously. Primary study endpoints were PK parameters such as the area under the concentration-time curve (AUC) from time zero to infinity (AUC0 – ∞), AUC from time zero to the last quantifiable concentration (AUC0–t), and maximum serum concentration (Cmax). Safety and immunogenicity profiles were also included for data analysis. 82 subjects were randomized to receive LY05008 (n = 41) or dulaglutide (n = 41). The 90% confidence intervals (CIs) of the geometric mean ratios (GMRs) of AUC0 – ∞, AUC0–t and Cmax of LY05008 to dulaglutide were all within the bioequivalence limits of 80%-125%. Other PK parameters, safety, and immunogenicity profiles were comparable across the two treatment groups. This study demonstrated PK similarity of LY05008, a dulaglutide biosimilar, to dulaglutide in healthy Chinese male subjects, with comparable safety and immunogenicity data. The trial is registered at the Chinese Clinical Trial Registry (Identifier No. ChiCTR2200066519).
Nonlinear perturbations from axion-gauge fields dynamics during inflation
Creators: name: Papageorgiou, Alexandros
name: Peloso, Marco
name: Unal, Caner
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study a variant of the Chromo-Natural Inflation (CNI) mechanism in which the inflaton interacts only gravitationally with the CNI fields. Integrating out all the non-dynamical scalar fields of the model results in a coupling between the perturbations of the inflaton and of the CNI pseudo-scalar which is significantly greater than the one obtained in the absence of the gauge CNI dynamics. We compute how this greater coupling impacts the power spectrum of the inflaton perturbations that are sourced nonlinearly by the unstable (tensor) gauge CNI modes, and we require that the amplitude of these modes is well below that of the linear perturbations. Combining this result with various constraints, including backreaction effects, the requirement of having observable and dominant sourced gravitational waves (GW), and the current upper bound on the tensor-to-scalar ratio, significantly constrains the range of parameter space where this model can produce an interesting GW signal.
description: 42 pages, 8 figures
Additional file 1: of A physical activity, nutrition and oral health intervention in nursery settings: process evaluation of the NAP SACC UK feasibility cluster RCT
Creators: name: Langford, Rebecca
name: Jago, Russell
name: White, James
name: Moore, Laurence
name: Papadaki, Angeliki
name: Hollingworth, William
name: Metcalfe, Chris
name: Ward, Dianne
name: Campbell, Rona
name: Wells, Sian
name: Kipping, Ruth
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: 60506 Virology
subject: FOS: Biological sciences

description: NAP SACC UK Logic Model. (PDF 427 kb)
Coelogyne graminea M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne graminea

description: Coelogyne graminea (Ridl.) M.W.Chase & Schuit., comb. nov.
 Basionym: Platyclinis graminea Ridl., J. Fed. Malay States Mus. 6: 57 (1915).
 Homotypic synonym: Dendrochilum gramineum (Ridl.) Holttum, Gard. Bull. Singapore 11: 280 (1947).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 112, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Additional file 1: of A score model based on pancreatic steatosis and fibrosis and pancreatic duct diameter to predict postoperative pancreatic fistula after Pancreatoduodenectomy
Creators: name: Xingjun, Guo
name: Feng, Zhu
name: Meiwen, Yang
name: Jianxin, Jiang
name: Zheng, He
name: Jun, Gao
name: Tao, Huang
name: Rui, Zhao
name: Leida, Zhang
name: Min, Wang
name: Renyi, Qin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: Table S1. Demographic and Clinicopathologic Characteristics of Cohort (DOC 70 kb)
Additional file 1 of Research activities and critical appraisal skills among Saudi orthopedic residents
Creators: name: Al-Mohrej, Omar A.
name: Alsadoun, Nouf F.
name: Alshaalan, Fawaz N.
name: Alturki, Rayan I.
name: Al-Rabiah, Anwar M.
name: Hamdi, Nezar B.
name: Ilyas, Imran
name: AlHussainan, Thamer S.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 1. Study Questionnaire.
Near-Field Microlensing and Its Effects on Stellar Transit Observations by Kepler
Creators: name: Sahu, Kailash C.
name: Gilliland, Ronald L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, we explore the astrophysical implications of near-field microlensing and its effects on stellar transit observations, with a special emphasis on the Kepler mission. Kepler is a NASA-approved mission whose goal is to detect a large number of extrasolar, earth-like planets by obtaining near-continuous photometry of > 100,000 F, G, and K dwarfs for four years. The expected photometric precision of Kepler is 90 micromag (achieved in 15 minute samples), at which the effect of microlensing by a transiting companion can be significant. For example, for a solar-type primary transited by a white-dwarf secondary, the maximum depth of the transit is 0.01%, which is almost entirely compensated by the microlensing amplification when the white dwarf is at ~0.05 AU. The combined effect of microlensing and transit increases to a net amplification of 150 micromag at an orbital separation of 0.1 AU, and 2.4 millimag at an orbital separation of 1 AU. Thus, the effect of microlensing can be used to break the degeneracy between a planetary-mass object for which the microlensing effect is negligible, and a more massive object of the same size. For brown dwarfs at orbital separations of a few AU, the effect of microlensing is several percent of the transit depth, and hence the microlensing effect must be taken into account in deriving the physical parameters of the brown dwarf. The microlensing signal caused by a neutron star or a black hole in a binary can be several millimag, far exceeding the transit depth, and potentially detectable even from ground-based observations. Kepler will be sensitive to white dwarfs, neutron stars, and black holes in binaries through their microlensing signatures. These observations can be used to derive the frequency of such compact objects in binaries, and to determine their masses.
description: 34 pages, including 15 figures, Accepted for publication in Astrophysical Journal
Additional file 10 of Evaluating implementation of the Transparency and Openness Promotion (TOP) guidelines: the TRUST process for rating journal policies, procedures, and practices
Creators: name: Mayo-Wilson, Evan
name: Grant, Sean
name: Supplee, Lauren
name: Kianersi, Sina
name: Amin, Afsah
name: DeHaven, Alex
name: Mellor, David
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Science Policy

description: Additional file 10.
Additional file 5: of The impact of multimorbidity on foot health outcomes in podiatry patients with musculoskeletal foot pain: a prospective observational study
Creators: name: Hendry, Gordon
name: Fenocchi, Linda
name: Mason, Helen
name: Steultjens, Martijn
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Unadjusted and adjusted associations between multimorbidity and foot health outcomes. Table displays results of multivariate linear regression analyses for associations between multimorbidity and FHSQ outcomes at 3 and 6â months, which are unadjusted and adjusted for baseline FHSQ domain, age and BMI. (DOCX 14 kb)
The nature of the progenitor of the Type II-P supernova 1999em
Creators: name: Smartt, S. J.
name: Gilmore, G. F.
name: Tout, C. A.
name: Hodgkin, S. T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high quality ground-based VRI images of the site of the Type II-P SN1999em (in NGC1637) taken before explosion, which were extracted from the CFHT archive. We determine a precise position of the SN on these images to an accuracy of 0.17''. The host galaxy is close enough (7.5 +/- 0.5 Mpc) that the bright supergiants are resolved as individual objects, however we show that there is no detection of an object at the SN position before explosion that could be interpreted as the progenitor star. By determining the sensitivity limits of the VRI data, we derive bolometric luminosity limits for the progenitor. Comparing these to standard stellar evolutionary tracks which trace evolution up to the point of core carbon ignition, we initially derive an upper mass limit of approximately 12M_sol. However we present evolutionary calculations that follow 7-12M_sol stars throughout their C-burning lifetime and show that we can restrict the mass of the progenitor even further. Our calculations indicate that progenitors initially of 8-10M_sol, undergoing expected mass loss, can also be excluded because a second dredge up sends them to somewhat higher luminosities than a star of initially 12M_sol. These results limit the progenitor's initial main-sequence mass to a very narrow range of 12 +/- 1 M_sol. We discuss the similarities between the Type II-P SNe 1999em and 1999gi and their progenitor mass limits, and suggest that SN Type II-P originate only in intermediate mass stars of 8-12M_sol, which are in the red supergiant region and that higher mass stars produce the other Type II sub-types. (Abridged).
description: Replaced with accepted version to appear in ApJ, 30 pages, inc. 6 figures
Additional file 1 of Diabetic microvascular complications are associated with reduced global longitudinal strain independent of atherosclerotic coronary artery disease in asymptomatic patients with diabetes mellitus: a cross-sectional study
Creators: name: Pararajasingam, Gokulan
name: Heinsen, Laurits Juhl
name: Larsson, Johanna
name: Andersen, Thomas Rueskov
name: Løgstrup, Brian Bridal
name: Auscher, Søren
name: Hangaard, Jørgen
name: Møgelvang, Rasmus
name: Egstrup, Kenneth
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Marine Biology
subject: Cancer

description: Additional file 1. Multivariable linear regression model of global longitudinal strain in patients with and without significant coronary artery disease.
Additional file 4: of The impact of multimorbidity on foot health outcomes in podiatry patients with musculoskeletal foot pain: a prospective observational study
Creators: name: Hendry, Gordon
name: Fenocchi, Linda
name: Mason, Helen
name: Steultjens, Martijn
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy

description: Cross-tabulation contingency table of perceptions of foot pain change according to multimorbidity group. Table displays results of cross-tabulation frequencies and chi-square sensitivity analysis of associations between group membership and perceptions of foot pain change. (DOCX 12 kb)
DeepICP: An End-to-End Deep Neural Network for 3D Point Cloud Registration
Creators: name: Lu, Weixin
name: Wan, Guowei
name: Zhou, Yao
name: Fu, Xiangyu
name: Yuan, Pengfei
name: Song, Shiyu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Computational Geometry (cs.CG)
subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: We present DeepICP - a novel end-to-end learning-based 3D point cloud registration framework that achieves comparable registration accuracy to prior state-of-the-art geometric methods. Different from other keypoint based methods where a RANSAC procedure is usually needed, we implement the use of various deep neural network structures to establish an end-to-end trainable network. Our keypoint detector is trained through this end-to-end structure and enables the system to avoid the inference of dynamic objects, leverages the help of sufficiently salient features on stationary objects, and as a result, achieves high robustness. Rather than searching the corresponding points among existing points, the key contribution is that we innovatively generate them based on learned matching probabilities among a group of candidates, which can boost the registration accuracy. Our loss function incorporates both the local similarity and the global geometric constraints to ensure all above network designs can converge towards the right direction. We comprehensively validate the effectiveness of our approach using both the KITTI dataset and the Apollo-SouthBay dataset. Results demonstrate that our method achieves comparable or better performance than the state-of-the-art geometry-based methods. Detailed ablation and visualization analysis are included to further illustrate the behavior and insights of our network. The low registration error and high robustness of our method makes it attractive for substantial applications relying on the point cloud registration task.
description: 10 pages, 6 figures, 3 tables, typos corrected, experimental results updated, accepted by ICCV 2019
Spectral mapping of the spiral structures in IP Pegasi on the decline from an outburst
Creators: name: Baptista, Raymundo
name: Haswell, Carole A.
name: Thomas, Gino
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (abridged) We report eclipse mapping of time resolved spectroscopy of the dwarf nova IP Pegasi on the late decline from the May 1993 outburst. The spiral arms are still visible some 8 days after the onset of the outburst. Their fractional contribution to the continuum emission is similar to that measured close to outburst maximum, whereas their orientation is rotated by 58 degrees with respect to the spirals seen in the eclipse map at outburst maximum. Velocity-resolved light curves across the Halpha and the HeI lines show the classical rotational disturbance, with the blue side of the line being eclipsed earlier than the red side. The differences between the Halpha and the HeI maps are significant. The spiral arms are clearly seen in the HeI maps, with the receding arm being stronger in the red side while the approaching arm is stronger in the blue side of the line. The analysis of the Halpha maps suggests that this emission arises mainly from a large and vertically-extended region which we interpret as an outflowing (and spiraling) disc wind. The spectrum of the uneclipsed light is dominated by a strong, blueshifted and narrow Halpha emission line superimposed on a red continuum and can be understood as a combination of emission from an M5V secondary star plus optically thin emission from the outer parts of the vertically-extended disc wind. The inner disc regions show an emission line spectrum with a strong and broad Halpha component superimposed on a flat continuum. This is in marked contrast with the results from the spectral mapping of nova-like variables of comparable inclination and mass ratio and suggests that intrinsically different physical conditions hold in the inner disc regions of outbursting dwarf novae and nova-like systems.
description: To appear in Mon. Not. R. Ast. Soc., 12 pages, 10 figures, coded with MNRAS latex style
Additional file 1 of Influenza a virus triggers acute exacerbation of chronic obstructive pulmonary disease by increasing proinflammatory cytokines secretion via NLRP3 inflammasome activation
Creators: name: Ji, Shuang
name: Dai, Meng-Yuan
name: Huang, Yun
name: Ren, Xiang-Chun
name: Jiang, Meng-Long
name: Qiao, Jin-Ping
name: Zhang, Wen-Ying
name: Xu, Yuan-Hong
name: Shen, Ji-Long
name: Zhang, Ren-Quan
name: Fei, Guang-He
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1. Table S2. TableS3. Subject characteristics. Figure S1. Isolation,purification, identification, and culture of human bronchial epithelial cells. A The cell growth stateswere observed and photographed under the inverted microscope. The pictures ofcultured cells were taken on day 1, 4, 7, 14, respectively. (Scale bar = 200 µm, originalmagnification: ×100; scale bar = 100 µm, originalmagnification: ×200). B The isolated NHBE and DHBE cells were cultured for 14 days, then probed with anti-human CK17/19antibody. Immunofluorescence of positive CK17/19 staining (green), DAPI stainedfor nuclear content (blue) (scale bar = 100 µm, originalmagnification: ×200). C HE and immunocytochemistry of positive CK17/19 staining (scale bar=100 µm, originalmagnification: ×200). Figure S2. Characteristics of COPD rat model. Rats were exposed to cigarette smoke or normal air for 12weeks and then infected with IAV on the last day of exposure. Blood gas analysis and pulmonary function test were conducted. A Partial pressure O2(PaO2) and Partial pressure CO2(PaCO2) B Oxyhemoglobin saturation (SaO2) C Special airwayresistance (SRaw) D Special airwayconductivity (SGaw) E Air volume per minute (MV) F Maximumexpiratory volume (EV) G Peakexpiratory flow (PEF) H Peak inspiratory flow (PIF). I HE-stained lung sections from rats 7 days’post-infection with 2.5×103 PFU of IAV and treatment with 10 mg/kg MCC950 or salinecontrol. Images shown are representative of 8 rats for each condition,Scale bars, 200 µm. Data are presented as the mean ± SD of eight rats per group. FigureS3. Increased levels of IL-1β and IL-18 in serum and BALF in AECOPD patients. The levels of IL-1β and IL-18 in serum and BALF were significantelevated in IAV positive group compare to IAV negative group. (* denote P<0.05,*** denotes P<0.001).
Coelogyne graminoides M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne graminoides

description: Coelogyne graminoides (Carr) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum graminoides Carr, Gard. Bull. Straits Settlem. 8: 229 (1935).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 112, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Additional file 1: of Effect of disease-modifying anti-rheumatic drugs on bone structure and strength in psoriatic arthritis patients
Creators: name: Simon, David
name: Kleyer, Arnd
name: Bayat, Sara
name: Tascilar, Koray
name: Kampylafka, Eleni
name: Meinderink, Timo
name: Schuster, Louis
name: Petrov, Ramona
name: Anna-Maria Liphardt
name: Juergen Rech
name: Schett, Georg
name: Hueber, Axel
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: Table S1. Regression models. (DOCX 18 kb)
Robust model comparison tests of DAMA/LIBRA annual modulation
Creators: name: Krishak, Aditi
name: Dantuluri, Aisha
name: Desai, Shantanu
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We evaluate the statistical significance of the DAMA/LIBRA claims for annual modulation using three independent model comparison techniques, viz frequentist, information theory, and Bayesian analysis. We fit the data from the DAMA/LIBRA experiment to both cosine and a constant model, and carry out model comparison by choosing the constant model as the null hypothesis. For the frequentist test, we invoke Wilk's theorem and calculate the significance using $Δχ^2$ between the two models. For information theoretical tests, we calculate the difference in Akaike Information Criterion (AIC) and Bayesian Information criterion (BIC) between the two models. We also compare the two models in a Bayesian context by calculating the Bayes factor. We also search for higher harmonics in the DAMA/LIBRA data using generalized Lomb-Scargle periodogram. We finally test the sensitivity of these model comparison techniques in discriminating between pure noise and a cosine signal using synthetic data. This is the first proof of principles application of AIC, BIC as well as Bayes factor to the DAMA data. All our analysis codes along with the data used in this work have been made publicly available.
description: 13 pages, 2 figures. Additional sections on searches for higher harmonics and sensitivity of model comparison tests used here in distinguishing real signals from noise with synthetic data
Additional file 1 of Individualization of PEEP and tidal volume in ARDS patients with electrical impedance tomography: a pilot feasibility study
Creators: name: Becher, Tobias
name: Buchholz, Valerie
name: Hassel, Daniel
name: Meinel, Timo
name: Schädler, Dirk
name: Frerichs, Inéz
name: Weiler, Norbert
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1. Protocol for adjustment of VT and PEEP with EIT, treatment courses of individual patients during EIT-based adjustment, individual patient results and patient example with EIT screenshots
Additional file 1: of PIWI-interacting RNA-36712 restrains breast cancer progression and chemoresistance by interaction with SEPW1 pseudogene SEPW1P RNA
Creators: name: Tan, Liping
name: Mai, Dongmei
name: Zhang, Bailin
name: Jiang, Xiaobing
name: Zhang, Jialiang
name: Bai, Ruihong
name: Ye, Ying
name: Li, Mei
name: Pan, Ling
name: Su, Jiachun
name: Zheng, Yanfen
name: Liu, Zexian
name: Zuo, Zhixiang
name: Zhao, Qi
name: Li, Xiaoxing
name: Huang, Xudong
name: Yang, Jie
name: Tan, Wen
name: Zheng, Jian
name: Lin, Dongxin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Hematology
subject: Plant Biology
subject: Virology
subject: Computational Biology

description: Materials and Methods (DOCX 32 kb)
Magnolia ferruginea P. Parm.
Creators: name: Turner, I. M.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Magnoliales
Magnoliaceae
Magnolia
Magnolia ferruginea

description: 16. Magnolia ferruginea P.Parm.
Bulletin scientifique de la France et de la Belgique 27: 203, 263, 264, 325, pl. IX, fig. 24 (1896), nom. illeg., non M. ferruginea Hort. ex W.Wats. (Bulletin of Miscellaneous Information Kew: 305 [1889]).
— Type: India, T.S. Ralph s.n. (holo-, P [P01964102]).
Fissistigma fulgens (Hook.f. & Thomson) Merr.: Philippine Journal of Science 15: 131 (1919) (Annonaceae) (Turner 2011).
description: Published as part of Turner, I. M., 2012, The taxa described by Paul Évariste Parmentier in Histoire des Magnoliacées, pp. 237-249 in Adansonia (3) (3) 34 (2) on page 241, DOI: 10.5252/a2012n2a3, http://zenodo.org/record/5205948
The development of a dense urban air pollution monitoring network
Creators: name: Shahraiyni, Hamid Taheri
name: Sodoudi, Sahar
name: Kerschbaumer, Andreas
name: Cubasch, Ulrich
Publisher: name: Freie Universität Berlin
Year: 2015
Subjects: subject: Artificial neural networks
subject: input variable selection
subject: urban areas
subject: Berlin
subject: PM10 monitoring network
subject: 500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::551 Geologie, Hydrologie, Meteorologie

description: The importance of air pollution monitoring networks in urban areas is well known because of their miscellaneous applications. At the beginning of the 1990s, Berlin had more than 40 particulate matter monitoring stations, whereas, by 2013, there were only 12 stations. In this study, a new and free–of–charge methodology for the densifying of the PM10 monitoring network of Berlin is presented. It endeavors to find the non–linear relationship between the hourly PM10 concentration of the still–operating PM10 monitoring stations and the shut–down stations by using the Artificial Neural Network (ANN), and, consequently, the results of the shut–down stations were simulated and re–constructed. However, input–variables selection is a pre–requisite for any ANN simulation, and hence a new fuzzy–heuristic input selection has been developed and joined to the ANN for the simulation. The hourly PM10 concentrations of the 20 shut–down stations were simulated and re–constructed. The mean error, bias and absolute error of the simulations were 27.7%, –0.03 (μg/m3), and 7.4 (μg/m3), respectively. Then, the simulated hourly PM10 concentration data were converted to a daily scale and the performance of ANN models which were developed for the simulation of the daily PM10 data were evaluated (correlation coefficient >0.94). These appropriate results imply the ability of the developed input selection technique to make the appropriate selection of the input variables, and it can be introduced as a new input variable selection for the ANN. In addition, a dense PM10 monitoring network was developed by the combination of both the re–constructed (20 stations) and the current (12 stations) stations. This dense monitoring network was applied in order to determine a reliable mean annual PM10 concentration in the different areas in Berlin in 2012.
Infrared Observations and Modeling of one of the Coolest T Dwarfs, Gl 570D
Creators: name: Geballe, T. R.
name: Saumon, D.
name: Leggett, S. K.
name: Knapp, G. R.
name: Marley, M. S.
name: Lodders, K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained a good quality R$\sim$400 0.8-2.5 $μ$m spectrum and accurate photometry of Gl 570D, one of the coolest and least luminous brown dwarfs currently known. The spectrum shows that Gl 570D has deeper absorptions in the strong water and methane bands at 1.12-1.17 $μ$m, 1.33-1.45 $μ$m, 1.62-1.88 $μ$m, and 2.20-2.45 $μ$m and is both bluer at J-K and redder at $K-L^{\prime}$ than previously observed T dwarfs. Data analysis using model spectra coupled with knowledge of the well-understood primary implies that for the same surface gravity, Gl 570D is about 160 K cooler than Gl 229B. For an age range of 2-5 Gyr Gl 570D has an effective temperature in the range 784-824 K, a log gravity in the range 5.00-5.27 cm s$^{-2}$, and a luminosity in the range 2.88-2.98 $\times$ 10$^{-6}$ L$_\odot$.
description: 22 pages (Latex) and 4 figures (postscript); accepted for publication by ApJ (main journal)
Coelogyne hamata M. W. Chase & Schuit. 2021, comb. nov.
Creators: name: Chase, Mark W.
name: Gravendeel, Barbara
name: Sulistyo, Bobby P.
name: Wati, Richa Kusuma
name: Schuiteman, André
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Orchidaceae
Coelogyne
Coelogyne hamata

description: Coelogyne hamata (Schltr.) M.W.Chase & Schuit., comb. nov.
 Basionym: Dendrochilum hamatum Schltr., Repert. Spec. Nov. Regni Veg. 9: 340 (1911).
description: Published as part of Chase, Mark W., Gravendeel, Barbara, Sulistyo, Bobby P., Wati, Richa Kusuma & Schuiteman, André, 2021, Expansion of the orchid genus Coelogyne (Arethuseae; Epidendroideae) to include Bracisepalum, Bulleyia, Chelonistele, Dendrochilum, Dickasonia, Entomophobia, Geesinkorchis, Gynoglottis, Ischnogyne, Nabaluia, Neogyna, Otochilus, Panisea and Pholidota, pp. 94-134 in Phytotaxa 510 (2) on page 113, DOI: 10.11646/phytotaxa.510.2.1, http://zenodo.org/record/5426332
Hydrodynamics of Relativistic Blast Waves in a Density-Jump Medium and Their Emission Signature
Creators: name: Dai, Z. G.
name: Lu, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze in detail the hydrodynamics and afterglow emission of an ultrarelativistic blast wave when it expands in a density-jump medium. Such a medium is likely to appear in the vicinity of gamma-ray bursts (GRBs) associated with massive stars. The interaction of the blast wave with this medium is described through a reverse shock and a forward shock. We show that the reverse shock is initially relativistic if the factor of a density jump ($α$) is much larger than 21, and Newtonian if $1
description: minor changes, accepted for publication in ApJ Letters
title: Die Sprachwissenschaft
title: Ihre Aufgaben, Methoden und bisherigen Ergebnisse
titleType: Subtitle
Creators: name: Gabelentz, Georg Von Der
name: Ringmacher, Manfred
name: McElvenny, James
Publisher: name: Freie Universität Berlin
Year: 2016
Subjects: subject: 400 Sprache::410 Linguistik

description: Die Sprachwissenschaft ist das Hauptwerk des deutschen Sinologen und Sprachwissenschaftlers Georg von der Gabelentz (1840–1893), eines Vertreters der humboldtschen Richtung der Sprachforschung im neunzehnten Jahrhundert. Als es erschien, wurde das Buch von einer Fachlinguistik, die sich schon längst auf den positivistischen Weg der Junggrammatiker begeben hatte, nur kühl rezipiert. Ab der Mitte des 20. Jahrhunderts wurde das Buch jedoch immer öfter als Bindeglied zwischen den Denkströmungen des 19. Jahrhunderts und dem aufkommenden Strukturalismus des 20. Jahrhunderts betrachtet. Das Buch erschien in zwei Auflagen; die erste zu Gabelentz' Lebzeiten, im Jahr 1891, und die zweite posthum im Jahr 1901, die von Albrecht Graf von der Schulenburg (1865–1902), einem Neffen und Schüler Gabelentz', erheblich überarbeitet und erweitert wurde. Diese kritische Ausgabe bietet zum ersten Mal den Text der beiden Auflagen in einer Form dar, die es dem Leser ermöglicht, die beiden Auflagen leicht zu vergleichen. Dadurch stellt diese Ausgabe eine wertvolle Quelle für historiographische Forschung zum Stand der Linguistik an der Schwelle zum 20. Jahrhundert dar.
description: Die Sprachwissenschaftis the magnum opus of the German sinologist and linguist Georg von der Gabelentz (1840-1893), a late 19th-century representative of the Humboldtian tradition of linguistic research. The book exists in two versions: a first edition of 1891 and a second posthumous edition of 1901, revised and expanded by Albrecht Graf von der Schulenburg (1865–1902), a nephew and pupil of Gabelentz. This critical edition presents for the first time the text of the two editions in a form that allows them to be easily compared. It represents a valuable resource for historiographical research into linguistics on the eve of the 20th century.
Small weight code words arising from the incidence of points and hyperplanes in PG($\boldsymbol{n,q}$)
Creators: name: Adriaensen, Sam
name: Denaux, Lins
name: Storme, Leo
name: Weiner, Zsuzsa
Publisher: name: arXiv
Year: 2019
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05B25, 94B05

description: Let $C_{n-1}(n,q)$ be the code arising from the incidence of points and hyperplanes in the Desarguesian projective space PG($n,q$). Recently, Polverino and Zullo proved that within this code, all non-zero code words of weight at most $2q^{n-1}$ are scalar multiples of either the incidence vector of one hyperplane, or the difference of the incidence vectors of two distinct hyperplanes. We improve this result, proving that when $q>17$ and $q\notin\{25,27,29,31,32,49,121\}$, all code words of weight at most $(4q-\sqrt{8q}-\frac{33}{2})q^{n-2}$ are linear combinations of incidence vectors of hyperplanes through a fixed $(n-3)$-space. Depending on the omitted value for $q$, we can lower the bound on the weight of $c$ to obtain the same results.
Metallicity and Kinematics of M31's Outer Stellar Halo from a Keck Spectrocscopic Survey
Creators: name: Reitzel, David B.
name: Guhathakurta, Puragra
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present multislit CaII near-infrared triplet spectroscopy with the Keck 10-m telescope/LRIS of 99 M31 halo red giant candidates in the apparent mag range 200.6 dex, spans the full 2dex range over which [Fe/H] measurement methods are calibrated, and has a mean/median value around =-1.9 to -1.1dex and possibly higher since the high-[Fe/H] end of the distribution is not well constrained by our sample. Our data on M31 field halo giants suggest that they are more metal-rich than their Milky Way counterparts, similar to M31 and Milky Way globular clusters, consistent with a scenario in which the halo is built from accretion of small stellar subsystems. There are 4 stars in the secure M31 sample with unusually strong Ca lines (>~solar [Fe/H]) at a common velocity of -340km/s close to M31's systemic velocity, similar to what might be expected for M31 disk giants on the minor axis. The M31 disk would have to be large and/or warped to account for these stars. More likely, these stars are metal-rich debris from a past accretion event in M31's halo.
description: 98 pages, including 4 tables and 24 figures; Accepted for publication in the July, 2002 edition of the Astronomical Journal
Imaging recoil ions from optical collisions between ultracold, metastable neon isotopes
Creators: name: Ohayon, B.
name: Rahangdale, H.
name: Chocron, J.
name: Kosloff, R.
name: Heber, O.
name: Ron, G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We present an experimental scheme which combines the well established method of velocity-mapimaging, with a cold trapped metastable neon target. The device is used for obtaining the branching ratios and recoil-ion energy distributions for the penning ionization process in optical collisions of ultracold metastable neon. The potential depth of the highly excited dimer potential is extracted and compared with theoretical calculations. The simplicity to construct, characterize and apply such a device, makes it a unique tool for the low-energy nuclear physics community, enabling opportunities for precision measurements in beta- and beta-delayed-neutron decays of cold, trapped, short-lived radioactive isotopes.
Clustered Star Formation in W75 N
Creators: name: Shepherd, D. S.
name: Testi, L.
name: Stark, D. P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present 2" to 7" resolution 3 mm continuum and CO(J=1-0) line emission and near infrared Ks, H2, and [FeII] images toward the massive star forming region W75 N. The CO emission uncovers a complex morphology of multiple, overlapping outflows. A total flow mass of greater than 255 Msun extends 3 pc from end-to-end and is being driven by at least four late to early-B protostars. More than 10% of the molecular cloud has been accelerated to high velocities by the molecular flows (> 5.2 km/s relative to v{LSR}) and the mechanical energy in the outflowing gas is roughly half the gravitational binding energy of the cloud. The W75 N cluster members represent a range of evolutionary stages, from stars with no apparent circumstellar material to deeply embedded protostars that are actively powering massive outflows. Nine cores of millimeter-wavelength emission highlight the locations of embedded protostars in W75 N. The total mass of gas & dust associated with the millimeter cores ranges from 340 Msun to 11 Msun. The infrared reflection nebula and shocked H2 emission have multiple peaks and extensions which, again, suggests the presence of several outflows. Diffuse H2 emission extends about 0.6 parsecs beyond the outer boundaries of the CO emission while the [FeII] emission is only detected close to the protostars. The infrared line emission morphology suggests that only slow, non-dissociative J-type shocks exist throughout the pc-scale outflows. Fast, dissociative shocks, common in jet-driven low-mass outflows, are absent in W75 N. Thus, the energetics of the outflows from the late to early B protostars in W75 N differ from their low-mass counterparts -- they do not appear to be simply scaled-up versions of low-mass outflows.
description: Astrophysical Journal, in press. 23 pages plus 10 figures (jpg format). See http://www.aoc.nrao.edu/~dshepher/science.shtml for reprint with full resolution figures