cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Localizing the $γ$-ray emitting region in the blazar TXS 2013+370
Creators: name: Traianou, E.
name: Krichbaum, T. P.
name: Boccardi, B.
name: Angioni, R.
name: Rani, B.
name: Liu, J.
name: Ros, E.
name: Bach, U.
name: Sokolovsky, K. V.
name: Kiehlmann, S.
name: Gurwell, M.
name: Zensus, J. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The $γ$-ray production mechanism and its localization in blazars are still a matter of debate. The main goal of this paper is to constrain the location of the high-energy emission in the blazar TXS 2013+370 and to study the physical and geometrical properties of the inner jet region on sub-pc scales. VLBI observations at 86 GHz and space-VLBI at 22 GHz allowed us to image the jet base with an angular resolution of $\sim$0.4 pc. By employing CLEAN imaging and Gaussian model-fitting, we performed a thorough kinematic analysis, which provided estimates of the jet speed, orientation, and component ejection times. Additionally, we studied the jet expansion profile and used the information on the jet geometry to estimate the location of the jet apex. VLBI data were combined with single-dish measurements to search for correlated activity between the radio and $γ$-ray emission. The high-resolution VLBI imaging revealed the existence of a spatially bent jet, described by moving and stationary features. New jet features are observed to emerge from the core, accompanied by flaring activity in radio bands and $γ$ rays. The analysis of the transverse jet width profile constrains the location of the mm core to lie $\leq$ 2 pc downstream of the jet apex, and also reveals the existence of a transition from parabolic to conical jet expansion at a distance of $\sim$54 pc from the core, corresponding to $\sim$1.5$\times$10$^{\rm 6}$ Schwarzschild radii. The cross-correlation analysis reveals a strong correlation between the radio and $γ$-ray data, with the 1 mm emission lagging $\sim$49 days behind the $γ$ rays. Based on this, we infer that the high energy emission is produced at a distance of $\sim$1 pc from the VLBI core, suggesting that the seed photon fields for the external Compton mechanism originate either in the dusty torus or in the broad-line region.
description: 16 pages, 15 figures, accepted in A&A
Massive black hole remnants of the first stars II: optical and X-ray signatures in present-day galactic haloes
Creators: name: Islam, Ranty R.
name: Taylor, James E.
name: Silk, Joseph
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The first stars forming in minihaloes at redshifts greater than 20 may have been very massive and could have left behind massive black hole (MBH) remnants. In a previous paper we investigated the hierarchical merging of these MBHs and their associated haloes, using a semi-analytical approach consisting of a hierarchical merger tree algorithm and explicit prescriptions for the dynamics of merged substructure inside a larger host halo following a merger. One of the results was the prediction of a number of MBHs orbiting throughout present-day galactic haloes. In addition we determined the mass accretion rate of these MBHs assuming that they could in principle remain embedded in a gaseous core that is a remnant of the haloes with which the MBHs were associated before merging with the host system. On this basis we determine in this paper the bolometric, optical and X-ray luminosity functions for the accreting MBHs using thin disk and advection dominated accretion flow models. Our predicted MBH X-ray emissions are then compared with observations of ultra-luminous X-ray sources in galaxies. We find that the slope and normalisation of the predicted X-ray luminosity function are consistent with the observations.
description: 14 pages, 10 figures; updated to match published version
Copeptin combined with either non-high sensitivity or high sensitivity cardiac troponin for instant rule-out of suspected non-ST segment elevation myocardial infarction
Creators: name: Giannitsis, Evangelos
name: Slagman, Anna
name: Hamm, Christian W.
name: Gehrig, Stefan
name: Joern O. Vollert
name: Huber, Kurt
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Whether Copeptin combined with high sensitivity troponin below the respective decision cut-offs improves rule-out of NSTEMI and may predict all-cause death at 30-day is under debate. Data on 10,329 patients from 5 trials were pooled to evaluate the diagnostic and prognostic performance of an initial Copeptin below decision cut-off in combination with a (hs)-cTn below the uppler limit of normal (ULN) compared to a) the initial (hs)-cTn alone in the standard serial sampling strategy based on the 99th percentile and b) a single marker strategy (SMS) based on hs-cTn NPV for NSTEMI was higher for DMS than for the initial cTn, regardless assay sensitivity. The highest NPVs were observed with DMS vs. hs-cTn (99.4% [95% CI: 99.0%–99.6%] vs. 98.8% [98.4%–99.1%],) , and improved performance was consistent across all important subgroups including presentation <3 h, again irrespective of assay sensitivity. The point estimate of all NPVs for all-cause death exceeded 99.75%. In the label populations, DMS versus SMS demonstrated comparably high NPVs for rule-out of NSTEMI (99.4% [99.0%–99.6%] vs. 99.9% [99.2%–100.0%]), very low mortality after rule-out (0.1% [0.0%–0.4% vs. 0.0% [0.0%–1.2%]), but eligibility for rule-out was 2.4-fold higher (61.4% [59.9%–62.9%] vs. 25.3% [23.7%–26.9%]) with DMS than SMS. Findings from a large pooled cohort corroborate the safety of the dual marker strategy for instant rule-out of NSTEMI, extending evidence to hs-cTn. Copeptin below cut-off in combination with hs-cTn below ULN may be used in more than 2.4-times more patients presenting with suspected ACS than a single marker strategy based on very low hs-cTn, without the need to exclude very early presenters or other important subgroups.
Channel Discord and Distortion
Creators: name: Zhang, Wei-Wei
name: Sanders, Yuval R.
name: Sanders, Barry C.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Discord, originally notable as a signature of bipartite quantum correlation,in fact can be nonzero classically, i.e., arising from noisy measurements by one of the two parties. Here we redefine classical discord to quantify channel distortion,in contrast to the previous restriction of classical discord to a state,and we then show a monotonic relationship between classical (channel) discord and channel distortion. We show that classical discord is equivalent to (doubly stochastic) channel distortion by numerically discovering a monotonic relation between discord and total-variation distance for a bipartite protocol with one party having a noiseless channel and the other party having a noisy channel. Our numerical method includes randomly generating doubly stochastic matrices for noisy channels and averaging over a uniform measure of input messages. Connecting discord with distortion establishes discord as a signature of classical, not quantum, channel distortion.
description: 24 pages, 2 figures
Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
Creators: name: Venn, Kim
name: Kielty, Collin
name: Sestito, Federico
name: Starkenburg, Else
name: Martin, Nicolas
name: Aguado, David S.
name: Arentsen, Anke
name: Bonifacio, Piercarlo
name: Caffau, Elisabetta
name: Hill, Vanessa
name: Jablonka, Pascale
name: Lardo, Carmela
name: Mashonkina, Lyudmilla
name: Navarro, Julio F.
name: Sneden, Chris
name: Thomas, Guillaume
name: Youakim, Kris
name: Gonzalez-Hernandez, Jonay I.
name: Janssen, Ruben Sanchez
name: Carlberg, Ray
name: Malhan, Khyati
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A chemo-dynamical analysis of 115 metal-poor candidate stars selected from the narrow-band Pristine photometric survey is presented based on CFHT high-resolution ESPaDoNS spectroscopy. We have discover 28 new bright (V < 15) stars with [Fe/H]0, and a metal-poor star with very low [Mg/Fe]. The kinematics and orbits for all of the highly probable metal-poor candidates are determined by combining our precision radial velocities with Gaia DR2 proper motions. Some stars show unusual kinematics for their chemistries, including planar orbits, unbound orbits, and highly elliptical orbits that plunge deeply into the Galactic bulge (Rperi < 0.5 kpc); also, eight stars have orbital energies and actions consistent with the Gaia-Enceladus accretion event. This paper contributes to our understanding of the complex chemo-dynamics of the metal-poor Galaxy, and increases the number of known bright metal-poor stars available for detailed nucleosynthetic studies.
description: Submitted to MNRAS, 19 pages (22 figures), and 7 tables
Tetracanthella corsica Potapov & Deharveng 2005, n. sp.
Creators: name: Potapov, Mikhail
name: Deharveng, Louis
Publisher: name: Zenodo
Year: 2005
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Tetracanthella
Tetracanthella corsica

description: Tetracanthella corsica n. sp.
(Fig. 2)
 TYPE MATERIAL. — Corsica. Valdo-Niello forest, no date, R. Dallai leg., holotype and 4 paratypes (MNHN); 2 paratypes (MSPU); 2 paratypes (Department of Evolutionary Biology, University of Siena). — Evisa, Aitone forest, meadow, 950 m, 4.IV.1976, L. Deharveng leg. (sample # Co 007), 1 paratype (MNHN). — Albertacce, Valdo-Niello forest, under rotten wood, 1200 m, 4.IV.1976, L. Deharveng leg. (sample # Co 005), 2 paratypes (MNHN). — Lonca, no date, J. Orousset leg., 1 paratype (MNHN).
ETYMOLOGY. — The name refers to the island of Corsica where the species has been found.
DISTRIBUTION. — Restricted to Corsica.
DESCRIPTION
Body length 0.9 mm. Pigment present, including antennae (more exact description impossible because pigmentation is partly lost). Dorsal plates polygonal, from 0.5 to 2 times as long as diameter of mesochaeta socket from head to Abd. I; from Abd. II to VI, up to six times as long as a mesochaeta socket, specially around the smooth areas (Fig. 2E); laterally and around the chaetae, polygons are much smaller. Canals between polygons well marked. Smooth fields present on Abd. IV and V (Fig. 2E), and on Abd. III in some specimens. Dorsal mesochaetae of medium size, in posterior row of Abd. IV not longer than on other parts of body (Md/p1 = 2.3-2.7). Mesochaetae not shortened in axial part of tergites: Abd. IV with p3 slightly longer than p1. Macrochaetae rather long, pointed (Fig. 2D).
description: Published as part of Potapov, Mikhail & Deharveng, Louis, 2005, Three new species of Tetracanthella (Collembola, Isotomidae) from western Europe, pp. 85-93 in Zoosystema 27 (1) on page 89, DOI: 10.5281/zenodo.5390855
Phase transitions in geometrothermodynamic model of charged generalized-NUT black holes
Creators: name: Grushevskaya, Halina
name: Krylova, Nina
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Modern cosmological models are constructed in the framework of thermodynamic approaches developed within a Van der Waals-Maxwell theory of the first-order phase transitions. In the present work we study a geometrothermodynamics of two-dimensional first-order phase transition with the distribution of relaxation times in a configuration space which describes a spacetime with Newman-Unti-Tamburino-like metric. We utilized the geometrothermodynamical approach to construct the model of a charged generalized-NUT black hole. We reveal following features of the black-hole phase transition: there are series of bifurcations of pitchfork type in dependences of the Gibbs free energy on the Hawking temperature, and although a scalar Berwald curvature of space changes sign in the phase transition, black-hole stability depends on sign of the curvature after the transition.
Noncommutative Chern-Simons Soliton
Creators: name: Ghosh, Subir
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We have studied the noncommutative extension of the relativistic Chern-Simons-Higgs model, in the first non-trivial order in $θ$, with only spatial noncommutativity. Both Lagrangian and Hamiltonian formulations of the problem have been discussed, with the focus being on the canonical and symmetric forms of the energy-momentum tensor. In the Hamiltonian scheme, constraint analysis and the induced Dirac brackets have been provided. The spacetime translation generators and their actions on the fields are discussed in detail. The effects of noncommutativity on the soliton solutions have been analysed thoroughly and we have come up with some interesting observations. Considering the {\it{relative}} strength of the noncommutative effects, we have shown that there is a universal character in the noncommutative correction to the magnetic field - it depends {\it{only}} on $θ$. On the other hand, in the cases of all other observables of physical interest, such as the potential profile, soliton mass or the electric field, $θ$ as well as $τ$, (comprising solely of commutative Chern-Simons-Higgs model parameters), appear on similar footings. This phenomenon is a new finding which has come up in the present analysis. Lastly, we have pointed out a generic problem in the NC extension of the models, in the form of a mismatch between the BPS dynamical equation and the full variational equations of motion, to $O(θ)$. This mismatch indicates that the analysis is not complete as it brings in to fore the ambiguities in the definition of the energy-momentum tensor in a noncommutative theory.
description: 21 pages
A Biomarker Based Severity Progression Indicator for COVID-19: The Kuwait Prognosis Indicator Score
Creators: name: Jamal, Mohammad H.
name: Doi, Suhail A.
name: AlYouha, Sarah
name: Almazeedi, Sulaiman
name: Mohannad Al-Haddad
name: Al-Muhaini, Ali
name: Al-Ghimlas, Fahad
name: Chowdhury, Muhammad E.
name: D Salman Al-Sabah
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: Science Policy
subject: 60506 Virology

description: COVID-19 is a worldwide pandemic that is mild in most patients but can result in a pneumonia like illness with progression to acute respiratory distress syndrome and death. Predicting the disease severity at time of diagnosis can be helpful in prioritizing hospital admission and resources. We prospectively recruited 1096 consecutive patients of whom 643 met the inclusion criterion with COVID-19 from Jaber Hospital, a COVID-19 facility in Kuwait, between 24 February and 20 April 2020. The primary endpoint of interest was disease severity defined algorithmically. Predefined risk variables were collected at the time of PCR based diagnosis of the infection. Prognostic model development used 5-fold cross-validated regularized logit regression. The model was externally validated against data from Wuhan, China. There were 643 patients with clinical course data of whom 94 developed severe COVID-19. In the final model, age, CRP, procalcitonin, lymphocyte percentage, monocyte percentages and serum albumin were independent predictors of a more severe illness course. The final prognostic model demonstrated good discrimination, and both discrimination and calibration were confirmed with an external dataset. We developed and validated a simple score calculated at time of diagnosis that can predict patients with severe COVID-19 disease reliably and that has been validated externally. The KPI score calculator is now available online at covidkscore.com
Tetracanthella fluorina Raynal 1972
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Tetracanthella
Tetracanthella fluorina

description: Tetracanthella fluorina Raynal, 1972
Tetracanthella fluorina Raynal, 1972: 611.
DISTRIBUTION. — Aveyron. Picde Kaymard (Raynal 1972; Deharveng 1987).
TAXONOMIE. — Deharveng 1987 (redescription).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 368, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Additional file 8 of Construction of a novel gene-based model for prognosis prediction of clear cell renal cell carcinoma
Creators: name: Zedan Zhang
name: Enyu Lin
name: Hongkai Zhuang
name: Xie, Lu
name: Xiaoqiang Feng
name: Jiumin Liu
name: Yuming Yu
Publisher: name: figshare
Year: 2020
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
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: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Additional file 8: Figure S5. PCA plot of GSE29609 dataset from GEO. A PCA plot shows that there are two clusters in the dataset, which means the dataset has batch effect. B Colorized the two clusters. C PCA plot of the data after normalization. GEO, Gene Expression Omnibus; PCA, principal component analysis.
13C isotope effects on infrared bands of quenched carbonaceous composite (QCC)
Creators: name: Wada, S.
name: Onaka, T.
name: Yamamura, I.
name: Murata, Y.
name: Tokunaga, A. T.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate carbon isotope effects on the infrared bands of a laboratory analogue of carbonaceous dust, the quenched carbonaceous composite (QCC), synthesized from a plasma gas of methane with various 12C/13C ratios. Peak shifts to longer wavelengths due to the substitution of 12C by 13C are clearly observed in several absorption bands. The shifts are almost linearly proportional to the 13C fraction. New features associated with 13C are not seen, indicating that the infrared bands in the QCC are not very localized vibration modes but come from vibrations associated with rather large carbon structures. An appreciable peak shift is detected in the 6.2 micron band, which is attributed to a carbon-carbon vibration. A peak shift in an out-of-plane bending mode of aromatic C--H at 11.4 micron is also observed, while only a small shift is detected in the 3.3 micron band, which arises from a C--H stretching mode. The present experiment suggests that peak shifts in the unidentified infrared (UIR) bands, particularly in the 6.2 micron band, should be detectable in celestial objects with low 12C/13C ratios (< 10). The isotopic shifts seen in the QCC are discussed in relation to the variations in the UIR band peaks observed in post-asymptotic giant branch stars and planetary nebulae. The observed peak shift pattern of the UIR bands is qualitatively in agreement with the isotopic shifts in the QCC except for the 7.7 micron band complex although the observed shifts in the UIR bands are larger than those inferred from derived isotope ratios for individual objects. The present investigation suggests that part of the observed variations in the UIR band peaks may come from the isotopic effects.
description: 12 pages, 7 figures, Accepted for Publication in A&A
Exposure to variable doses of nickel oxide nanoparticles disturbs serum biochemical parameters and oxidative stress biomarkers from vital organs of albino mice in a sex-specific manner
Creators: name: Hussain, Malik Fiaz
name: Ashiq, Muhammad Naeem
name: Muhammd Gulsher
name: Akbar, Atif
name: Furhan Iqbal
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
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: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: This study was designed to report the biological effect of nickel oxide nanoparticles (NiO NPs) in albino mice. Five weeks old albino mice of both sex were intraperitoneally injected either with 20 mg (low dose) or 50 mg/mL saline/kg body weight (high dose) of NiO NPs for 14 days. Saline-treated controls were maintained in parallel. Complete blood count, selected serum biochemical parameters and oxidative stress biomarkers from vital organs were determined in all subjects. Male mice treated with NiO NPS had increased blood urea nitrogen, elevated superoxide dismutase (SOD) in liver elevated MDA in liver, kidney and heart and reduced catalase activity in heart and kidney. Female mice treated with NiO NPs had significantly reduced serum albumin and total proteins, SOD in lungs and elevated MDA in liver. We are reporting that intraperitoneal injections of NiO NPs for 14 days drastically affect blood serum parameters and oxidative stress biomarkers from vital organs of albino mice. Toxic effects of NiO NPs were dose and sex dependent and they were more pronounced at higher dose and in male mice.
VALUING MEXICAN PHILOSOPHY: SUSPECT ENDEAVOR OR LIFE-AFFIRMING PATH? by Amy A. Oliver
Creators: name: Philosophy, the Journal of Mexican
Publisher: name: figshare
Year: 2022
Subjects: subject: Philosophy
subject: FOS: Philosophy, ethics and religion
subject: 220399 Philosophy not elsewhere classified
subject: 220316 Philosophy of Specific Cultures (incl. Comparative Philosophy)

description: ABSTRACT: This essay begins by juxtaposing Mexican philosophy with world philosophies and philosophy writ large, then offers assessment of salient moments in the history of Mexican philosophy (including indigenous contributions, Sor Juana, anti-positivist thinkers, and innovative philosophical concepts/terms) and suggests their applicability to North American life. The essay concludes by highlighting a few areas that could benefit from ongoing philosophical reflection by Mexicans in an increasingly challenging human rights context.
Hydroides salazarvallejoi Bastida-Zavala & ten Hove 2003
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Hydroides
Hydroides salazarvallejoi

description: Hydroides salazarvallejoi Bastida-Zavala & ten Hove, 2003
(Figure 6Q)
 Hydroides salazarvallejoi.— Bastida-Zavala & ten Hove, 2003b: 101, fig. 12N. Type locality: Santa Marta, Colombia (Atlantic side).
 Diagnosis. For a revised description see Bastida-Zavala and ten Hove (2003b).
 Habitat. Depth: 0–1 m. Docks and rocks. Brackish and marine water.
 Distribution. Amphi-American. Caribbean Sea; Costa Rica, Panama and Ecuador (Bastida-Zavala & ten Hove 2003a-b).
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on page 29
Photobiomodulation modulates inflammation and oral microbiome: a pilot study
Creators: name: Zanotta, Nunzia
name: Ottaviani, Giulia
name: Campisciano, Giuseppina
name: Poropat, Augusto
name: Bovenzi, Massimo
name: Rupel, Katia
name: Gobbo, Margherita
name: Comar, Manola
name: Di Lenarda, Roberto
name: Biasotto, Matteo
name: Zacchigna, Serena
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Introduction: Oral mucositis (OM) is a severe side effect in patients undergoing anticancer therapies, which negatively impacts on their quality of life often leading to either the interruption of the therapy. Photobiomodulation (PBM) is emerging as an effective strategy allowing a faster wound healing. Objectives: This pilot study aims at verifying whether PBM modulates the inflammatory response in patients and its effect on the oral microbiome composition. Materials and methods: Buccal swabs were collected from four patients affected by OM, both on ulcerated and clinically healthy areas, before and on the last day of PBM therapy, as well as on the first day after treatment discontinuation. The concentration of 38 cytokines and the composition of oral microbiome were measured. Results: Most of the pro-inflammatory cytokines were reduced, whereas anti-inflammatory cytokines resulted up-regulated by PBM. In addition, PBM influenced the composition of oral microbiome, by decreasing the amount of pathogenic species and promoting the growth of commensal bacteria. These changes were even more evident when separately analysing patients who clinically responded to PBM and the only patient who did not respond. Conclusions: PBM reduces inflammatory burden in patients affected by OM and positively influences the composition of the oral microbiome.
Hydroides tenhovei Bastida-Zavala & de Leon-Gonzalez 2002
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Hydroides
Hydroides tenhovei

description: Hydroides tenhovei Bastida-Zavala & de León-González, 2002
(Figure 6T)
 Hydroides tenhovei Bastida-Zavala & de León-González, 2002: 389–394, figs. 2A–M, 3A–H. Type locality: Cabo San Lazaro, Western coast of Baja California Sur, Mexico.
 Diagnosis. For a revised description see Bastida-Zavala and ten Hove (2003b).
 Habitat. Depth: 27–30 m. On an artificial substrate: a flat and hard PVC structure surrounded by soft-bottom.
 Distribution. Only known from the western coast of Baja California Sur (Mexico) (Bastida-Zavala & ten Hove 2003b).
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on page 30
Meta-analysis of human and mouse ALS astrocytes reveals multi-omic signatures of inflammatory reactive states.
Creators: name: Ziff, Oliver J
name: Clarke, Benjamin E
name: Taha, Doaa M
name: Crerar, Hamish
name: Luscombe, Nicholas M
name: Patani, Rickie
Publisher: name: The Francis Crick Institute
Year: 2022
Subjects: subject: Neurosciences
subject: FOS: Clinical medicine
subject: Tumour Biology
subject: Gene Expression
subject: Genetics & Genomics
subject: Cell Biology
subject: Stem Cells
subject: Computational & Systems Biology

description: Astrocytes contribute to motor neuron death in amyotrophic lateral sclerosis (ALS), but whether they adopt deleterious features consistent with inflammatory reactive states remains incompletely resolved. To identify inflammatory reactive features in ALS human induced pluripotent stem cell (hiPSC)-derived astrocytes, we examined transcriptomics, proteomics, and glutamate uptake in VCP-mutant astrocytes. We complemented this by examining other ALS mutations and models using a systematic meta-analysis of all publicly-available ALS astrocyte sequencing data, which included hiPSC-derived astrocytes carrying SOD1, C9orf72, and FUS gene mutations as well as mouse ALS astrocyte models with SOD1 G93A mutation, Tardbp deletion, and Tmem259 (also known as membralin) deletion. ALS astrocytes were characterized by up-regulation of genes involved in the extracellular matrix, endoplasmic reticulum stress, and the immune response and down-regulation of synaptic integrity, glutamate uptake, and other neuronal support processes. We identify activation of the TGFB, Wnt, and hypoxia signaling pathways in both hiPSC and mouse ALS astrocytes. ALS changes positively correlate with TNF, IL1A, and complement pathway component C1q-treated inflammatory reactive astrocytes, with significant overlap of differentially expressed genes. By contrasting ALS changes with models of protective reactive astrocytes, including middle cerebral artery occlusion and spinal cord injury, we uncover a cluster of genes changing in opposing directions, which may represent down-regulated homeostatic genes and up-regulated deleterious genes in ALS astrocytes. These observations indicate that ALS astrocytes augment inflammatory processes while concomitantly suppressing neuronal supporting mechanisms, thus resembling inflammatory reactive states and offering potential therapeutic targets.
Trigonometric Solutions of the WDVV Equations from Root Systems
Creators: name: Martini, R.
name: Hoevenaars, L. K.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences
subject: 35C05; 81T60

description: By introduction of an additional variable and addition of a Weyl invariant correction term to the perturbative prepotential in five-dimensional Seiberg-Witten theory we construct solutions of the WDVV equations of trigonometric type for all crystallographic root systems.
description: 4 pages, 1 table
Massive black hole remnants of the first stars III: observational signatures from the past
Creators: name: Islam, Ranty R.
name: Taylor, James E.
name: Silk, Joseph
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The first stars forming in minihaloes at redshifts greater than 20 may have been very massive and could have left behind massive black hole (MBH) remnants. In previous papers we investigated the hierarchical merging of these `seed' MBHs and their associated haloes, using a semi-analytical approach consisting of a hierarchical merger tree algorithm and explicit prescriptions for the dynamics of merged substructure inside a larger host halo following a merger. We also estimated accretion luminosities for these MBHs and found them to be consistent with observations of ultra-luminous X-ray point sources. Here we compute the strength of gravitational wave events as MBHs merge to grow from seed mass MBH at high redshifts to those that we predict to reside in galaxy haloes today. If MBHs merge efficiently we predict that some 10^4 - 10^5 events per year could be observed, that fall just within the sensitivity limits of the proposed LISA gravitational wave observatory. The collapse of the first massive stars to form MBHs may be accompanied by gamma ray bursts (GRBs). If this is the case and GRBs are in principle observable out to the redshifts of first star formation, we find that about 10^5 - 10^6 GRBs per year could be detected. As merging MBH binaries reach their last stable orbits before final coalescence a fraction of the gravitational wave energy may be released as a pulse of gamma rays (for instance, through interaction with material enveloping a merging MBH binary). This fraction has to be in the range between 10^{-14} - 10^{-10} for MBH mergers to be less luminous than GBRs, yet detectable out to cosmological distances with upcoming GRB detector missions.
description: 12 pages, 8 figures; updated to match published version
Tetracanthella gallica Deharveng 1987
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Tetracanthella
Tetracanthella gallica

description: Tetracanthella gallica Deharveng, 1987 **
Tetracanthella gallica Deharveng, 1987: 44.
DISTRIBUTION. — Savoie. Massif du Beaufortin à Roselend etmassif dela Vanoiseà Val Thorens, 2300 à 2800 m (Deharveng 1987).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 368, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Supplementary document for Independent transmitted and reflected colors enabled by Fano resonant optical coatings - 6293197.pdf
Creators: name: Teng, Xinyue
name: Song, Maowen
name: Ren, Yongze
name: Lin, Peicheng
name: Zhang, Yanzeng
name: Xu, Ting
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplementary Material
Additional file 7 of Construction of a novel gene-based model for prognosis prediction of clear cell renal cell carcinoma
Creators: name: Zedan Zhang
name: Enyu Lin
name: Hongkai Zhuang
name: Xie, Lu
name: Xiaoqiang Feng
name: Jiumin Liu
name: Yuming Yu
Publisher: name: figshare
Year: 2020
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: Additional file 7: Figure S4. Time-dependent ROC analysis of the five prognosis-related genes in 1-, 3- and 5-year OS prediction. A C9orf135. B DPP6. C PLG. D ATP6V0D2. E PADI1. ROC, receiver operating characteristic.
In vitro evaluation of Annona muricata L. (Soursop) leaf methanol extracts on inhibition of tumorigenicity and metastasis of breast cancer cells
Creators: name: Naik, Aditi Venkatesh
name: Sellappan, Krishnan
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: The present study evaluates the in-vitro anti-tumorigenic potential of leaf methanol extracts of Annona muricata (LMAM). The cytotoxic activity was assessed in MCF-7 cells by MTT assay at various concentrations ranging from 25–250µg/mL. MCF-7 cells were treated with 50 and 100 µg/mL LMAM for 24 h. To detect LMAM-induced apoptosis; Hoescht 33342 staining along with Cell cycle analysis, Annexin-PI probe as well as oxidative stress damage by reactive oxygen species (ROS) measurements were determined using flow cytometric analysis. While caspase-3 expression levels were studied employing the qRT-PCR method. LMAM exhibited significant inhibition of MCF-7 cells with an IC50 value of 85.55 µg/mL. Hoescht staining showed marked morphological features characteristic of apoptosis in LMAM treated cells. Cell cycle analysis confirmed the proven capability of LMAM showing a 30% rise in G1 phase upon treatment with 100 µg/mL LMAM, thus inducing cell cycle arrest at G1 phase and a rise in sub G0–G1 population paralleled with a decrease in S phase. Flow cytometric analysis with Annexin V-FITC-PI staining indicated an increase in the early and late apoptotic population with a 3.38% and 19.47% rise respectively when treated with 100 µg/mL LMAM. Treatment with 100 µg/mL LMAM caused an increase in intracellular ROS with MFI value 3334.08. Upregulation of caspase-3 was observed with a 2.18 and 32.47 fold increase compared to control in MCF-7 cells cultured at 50 µg/mL and 100 µg/mL LMAM respectively suggesting caspase-dependent apoptosis. LMAM proved as a potent ethno-chemopreventive agent and a potential lead in cancer treatment attributable to the synergistic interactive properties of phytoconstituents.
Laminatubus alvini ten Hove & Zibrowius 1986
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Laminatubus
Laminatubus alvini

description: Laminatubus alvini ten Hove & Zibrowius, 1986
(Figures 7B–D)
 Laminatubus alvini ten Hove & Zibrowius, 1986: 21–24, figs. 1, 2a, 3. Type locality: 0º47.69’N, 86º07.74’W, off Ecuador.
 Diagnosis. Tube thick-walled, smooth, with a longitudinal sinuous ridge. Opercular peduncle smooth. Operculum radially or slightly bilaterally symmetrical, with bulbous proximal part and rounded to inverted saucerlike distal plate (Figs 7B–C). Thoracic membrane extends to second chaetiger. Collar with “ Spirobranchus ” chaetae, coarsely serrated in the subapical section (Fig. 7D).
 Habitat. Depth: 2,451–2,842 m. Near to hydrothermal vents.
 Distribution. Tropical Eastern Pacific. From four hydrothermal vent areas (approx. 1°, 10°, 13° and 21°N) (ten Hove & Zibrowius 1986).
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on page 30
Radio and submillimetre observations of wind structure in zeta Pup
Creators: name: Blomme, R.
name: Van de Steene, G. C.
name: Prinja, R. K.
name: Runacres, M. C.
name: Clark, J. S.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present radio and submillimetre observations of the O4I(n)f star zeta Pup, and discuss structure in the outer region of its wind (~ 10-100 R*). The properties of bremsstrahlung, the dominant emission process at these wavelengths, make it sensitive to structure and allow us to study how the amount of structure changes in the wind by comparing the fluxes at different wavelengths. To look for variability, we acquired 3.6 and 6 cm observations with the Australia Telescope Compact Array (ATCA). We supplemented these with archive observations from the NRAO Very Large Array (VLA). We did not find variability at more than the +- 20 % level. The long integration time does allow an accurate determination of the fluxes at 3.6 and 6 cm. Converting these fluxes into a mass loss rate, we find Mdot = 3.5 x 10^{-6} Msun/yr. This value confirms the significant discrepancy with the mass loss rate derived from the Halpha profile, making zeta Pup an exception to the usually good agreement between Halpha and radio mass loss rates. We also observed zeta Pup at 850 mum with the James Clerk Maxwell Telescope (JCMT) and at 20 cm with the VLA. A smooth wind model shows that the millimetre fluxes are too high compared to the radio fluxes. While recombination of helium in the outer wind cannot be discounted as an explanation, the wealth of evidence for structure strongly suggests this as the explanation for the discrepancy. Model calculations show that the structure needs to be present in the inner ~ 70 R* of the wind, but that it decays significantly, or maybe even disappears, beyond that radius.
description: 13 pages, 8 figures, to be published in Astronomy and Astrophysics
On the associated family of Delaunay surfaces
Creators: name: Kilian, M
Publisher: name: arXiv
Year: 2003
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53A10

description: We use the DPW method to obtain the associate family of Delaunay surfaces and derive a formula for the neck size of the surface in terms of the entries of the holomorphic potential.
description: 9 pages
Tetracanthella emucronata Deharveng 1987
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Isotomidae
Tetracanthella
Tetracanthella emucronata

description: Tetracanthella emucronata Deharveng, 1987 **
Tetracanthella emucronata Deharveng, 1987: 47.
DISTRIBUTION. — Alpes-Maritimes. Massif du Margareis, vers 2500 m (Deharveng 1987).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 368, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Additional file 6 of Construction of a novel gene-based model for prognosis prediction of clear cell renal cell carcinoma
Creators: name: Zedan Zhang
name: Enyu Lin
name: Hongkai Zhuang
name: Xie, Lu
name: Xiaoqiang Feng
name: Jiumin Liu
name: Yuming Yu
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
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: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: Computational Biology

description: Additional file 6: Figure S3. The type of gene alteration among 628 patietns/696 samples in 3 publicly datasets including TCGA from cBioportal. 23 (3%) patients have gene alternation.
AGN feedback in a galaxy merger: Multi-phase, galaxy-scale outflows including a fast molecular gas blob ~6 kpc away from IRAS F08572+3915
Creators: name: Herrera-Camus, R.
name: Janssen, A.
name: Sturm, E.
name: Lutz, D.
name: Veilleux, S.
name: Davies, R.
name: Shimizu, T.
name: González-Alfonso, E.
name: Rupke, D. S. N.
name: Tacconi, L.
name: Genzel, R.
name: Cicone, C.
name: Maiolino, R.
name: Contursi, A.
name: Graciá-Carpio, J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: To understand the role that AGN feedback plays in galaxy evolution we need in-depth studies of the multi-phase structure and energetics of galaxy-wide outflows. In this work we present new, deep ($\sim$50 hr) NOEMA CO(1-0) line observations of the molecular gas in the powerful outflow driven by the AGN in the ultra-luminous infrared galaxy IRAS F08572+3915. We spatially resolve the outflow, finding that its most likely configuration is a wide-angle bicone aligned with the kinematic major axis of the rotation disk. The molecular gas in the wind reaches velocities up to approximately $\pm$1200 km s$^{-1}$ and transports nearly 20% of the molecular gas mass in the system. We detect a second outflow component located $\sim$6 kpc north-west from the galaxy moving away at $\sim$900 km s$^{-1}$, which could be the result of a previous episode of AGN activity. The total mass and energetics of the outflow, which includes contributions from the ionized, neutral, warm and cold molecular gas phases is strongly dominated by the cold molecular gas. In fact, the molecular mass outflow rate is higher than the star formation rate, even if we only consider the gas in the outflow that is fast enough to escape the galaxy, which accounts for about $\sim$40% of the total mass of the outflow. This results in an outflow depletion time for the molecular gas in the central $\sim$1.5 kpc region of only $\sim3$ Myr, a factor of $\sim2$ shorter than the depletion time by star formation activity.
description: 17 pages, 11 figures, accepted for publication in A&A
Copeptin combined with either non-high sensitivity or high sensitivity cardiac troponin for instant rule-out of suspected non-ST segment elevation myocardial infarction
Creators: name: E Giannitsis
name: A Slagman
name: CW Hamm
name: S Gehrig
name: JO Vollert
name: K Huber
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Background. Whether Copeptin combined with high sensitivity troponin below the respective decision cutoffs improves rule-out of NSTEMI and may predict all-cause death at 30-day is under debate. Methods. Data on 10,329 patients from 5 trials were pooled to evaluate the diagnostic and prognostic performance of an initial Copeptin below decision cutoff in combination with a (hs-(cTn) below the uppler limit of normal (ULN) compared to a) the initial (hs)-cTn alone in the standard serial sampling strategy based on the 99th percentile and b) a single marker strategy (SMS) based on hs-cTn Results. NPV for NSTEMI was higher for DMS than for the initial cTn, regardless assay sensitivity. The highest NPVs were observed with DMS vs. hs-cTn (99.4% [95%-CI: 99.0%-99.6%] vs. 98.8% [98.4%-99.1%],) , and improved performance was consistent across all important subgroups including presentation <3 hours, again irrespective of assay sensitivity. The point estimate of all NPVs for all-cause death exceeded 99.75%. In the label populations, DMS versus SMS demonstrated comparably high NPVs for rule-out of NSTEMI (99.4% [99.0%-99.6%] vs. 99.9% [99.2%-100.0%]), very low mortality after rule-out (0.1% [0.0%-0.4% vs. 0.0% [0.0%-1.2%]), but eligibility for rule-out was 2.4-fold higher (61.4% [59.9%-62.9%] vs. 25.3% [23.7%-26.9%]) with DMS than SMS. Conclusion. Findings from a large pooled cohort corroborate the safety of the dual marker strategy for instant rule-out of NSTEMI, extending evidence to hs-cTn. Copeptin below cutoff in combination with hs-cTn below ULN may be used in more than 2.4-times more patients presenting with suspected ACS than a single marker strategy based on very low hs-cTn, without the need to exclude very early presenters or other important subgroups.
Steady state velocity distributions of an oscillated granular gas
Creators: name: Moon, Sung Joon
name: Swift, J. B.
name: Swinney, Harry L.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We use a three-dimensional molecular dynamics simulation to study the single particle distribution function of a dilute granular gas driven by a vertically oscillating plate at high accelerations ($15g - 90g$). We find that the density and the temperature fields are essentially time-invariant above a height of about 35 particle diameters, where typically 20% of the grains are contained. These grains form the nonequilibrium steady state granular gas with a Knudsen number unity or greater. In the steady state region, the distribution function of horizontal velocities (scaled by the local horizontal temperature) is found to be nearly independent of height, even though the hydrodynamic fields vary with height. The high energy tails of the distribution functions are described by a stretched exponential $\sim \exp(-{\cal B}c_x^α)$, where $α$ depends on the normal coefficient of restitution $e$ ($1.2 < α< 1.6$), but $α$ does not vary for a wide range of the friction parameter. We find that the distribution function of a {\it frictionless} inelastic hard sphere model can be made similar to that of a frictional model by adjusting $e$. However, there is no single value of $e$ that mimics the frictional model over a range of heights.
description: submitted to Phys. Rev. E; to appear after a few more small changes