cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 4 of PCSK9 promotes the progression and metastasis of colon cancer cells through regulation of EMT and PI3K/AKT signaling in tumor cells and phenotypic polarization of macrophages
Creators: name: Wang, Lu
name: Li, Shuangshuang
name: Luo, Huanhua
name: Lu, Qi
name: Yu, Shuwen
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer

description: Additional file 4: Supplemental Table S4. Primers used for qRT- PCR
Musca aequinoctialis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca aequinoctialis

description: Musca aequinoctialis [spec. nov.]
M. antennis setariis glabra nigra, capite testaceo, oculis brunneis, pedibus elongatis.
Habitat in America meridionali. Mus. De Geer.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 598, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The joint spectrum
Creators: name: Breuillard, Emmanuel
name: Sert, Cagri
Publisher: name: arXiv
Year: 2018
Subjects: subject: Dynamical Systems (math.DS)
subject: Group Theory (math.GR)
subject: Probability (math.PR)
subject: FOS: Mathematics

description: We introduce the notion of \emph{joint spectrum} of a compact set of matrices $S \subset GL_d(\mathbb{C})$, which is a multi-dimensional generalization of the joint spectral radius. We begin with a thorough study of its properties (under various assumptions: irreducibility, Zariski-density, domination). Several classical properties of the joint spectral radius are shown to hold in this generalized setting and an analogue of the Lagarias-Wang finiteness conjecture is discussed. Then we relate the joint spectrum to matrix valued random processes and study what points of it can be realized as Lyapunov vectors. We also show how the joint spectrum encodes all word metrics on reductive groups. Several examples are worked out in detail.
description: 52 pages, 6 figures. v3: minor changes
Low Pressure Negative Ion Drift Chamber for Dark Matter Search
Creators: name: Snowden-Ifft, D. P.
name: Martoff, C. J.
name: Burwell, J. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Weakly Interacting Massive Particles (WIMPs) are an attractive candidate for the dark matter thought to make up the bulk of the mass of our universe. We explore here the possibility of using a low pressure negative ion drift chamber to search for WIMPs. The innovation of drifting ions, instead of electrons, allows the design of a detector with exceptional sensitivity to, background rejection from, and signature of WIMPs.
description: 5 pages submitted to PRL
Comparison of Cannabis-Based Medicinal Product Formulations for Fibromyalgia: A Cohort Study
Creators: name: Sridharan, Surya
name: Erridge, Simon
name: Holvey, Carl
name: Coomber, Ross
name: Holden, Wendy
name: Rucker, James J.
name: Platt, Michael
name: Sodergren, Mikael H.
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Science Policy
subject: Mental Health

description: This cohort study aims to assess the outcomes of fibromyalgia patients enrolled in the UK Medical Cannabis Registry prescribed a homogenous selection of cannabis-based medicinal products (CBMPs). A cohort study of fibromyalgia patients treated with oils (Adven®, Curaleaf International, UK), dried flower (Adven®, Curaleaf International, UK) or both CBMPs was performed. Primary outcomes were changes from baseline at 1, 3, 6 and 12 months in validated patient-reported outcome measures. Secondary outcomes included descriptive analysis of adverse events. One hundred and forty-eight participants were treated with oils (n = 77; 52.03%), dried flower (n = 14; 9.46%) or both (n = 57; 38.51%). Improvements in the generalized anxiety disorder-7 questionnaire, single-item sleep quality scale, fibromyalgia symptom severity score and EQ-5D-5L Index values were observed at each follow up period compared to baseline (p < 0.050). Thirty-six (24.32%) patients experienced 648 adverse events. Improvements were observed across all primary outcomes with no differences observed across different formulations of CBMPs. Adverse events were reported by one-quarter of participants and were more likely to reported by cannabis naïve patients. This present work through focusing on a homogeneous group of CBMPs can help inform randomized controlled trials after observing signals of improvement associated with a specific cultivar of CBMPs.
A Test of the Standard Hypothesis for the Origin of the HI Holes in Holmberg II
Creators: name: Rhode, K. L.
name: Salzer, J. J.
name: Westpfahl, D. J.
name: Radice, L. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The nearby irregular galaxy Holmberg II has been extensively mapped in HI using the Very Large Array (VLA), revealing intricate structure in its interstellar gas component (Puche et al. 1992). An analysis of these structures shows the neutral gas to contain a number of expanding HI holes. The formation of the HI holes has been attributed to multiple supernova events occurring within wind-blown shells around young, massive star clusters, with as many as 10-200 supernovae required to produce many of the holes. From the sizes and expansion velocities of the holes, Puche et al. assigned ages of ~10^7 to 10^8 years. If the supernova scenario for the formation of the HI holes is correct, it implies the existence of star clusters with a substantial population of late-B, A and F main sequence stars at the centers of the holes. Many of these clusters should be detectable in deep ground-based CCD images of the galaxy. In order to test the supernova hypothesis for the formation of the HI holes, we have obtained and analyzed deep broad-band BVR and narrow-band H-alpha images of Ho II. We compare the optical and HI data and search for evidence of the expected star clusters in and around the HI holes. We also use the HI data to constrain models of the expected remnant stellar population. We show that in several of the holes the observed upper limits for the remnant cluster brightness are strongly inconsistent with the SNe hypothesis described in Puche et al. Moreover, many of the HI holes are located in regions of very low optical surface brightness which show no indication of recent star formation. Here we present our findings and explore possible alternative explanations for the existence of the HI holes in Ho II, including the suggestion that some of the holes were produced by Gamma-ray burst events.
description: 30 pages, including 6 tables and 3 images. To appear in Astron. Journal (June 1999)
Inverse zero-sum problems for certain groups of rank three
Creators: name: Girard, Benjamin
name: Schmid, Wolfgang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Number Theory (math.NT)
subject: Combinatorics (math.CO)
subject: Group Theory (math.GR)
subject: FOS: Mathematics

description: The inverse problem associated to the Erdős-Ginzburg-Ziv constant and the $η$-constant is solved for finite abelian groups of the form $C_2 \oplus C_2 \oplus C_{2n}$ where $n \ge 2$ is an integer.
description: 16 pages
Additional file 7: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Ecology
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S7. Transgenic NAL8 gene silenced lines show similar leaf width and spikelet defects to the rice nal8 mutant. (A) Plant architecture of the wild-type TQ and the transgenic NAL8 RNAi silenced lines NAL8RNAi #1 and #2 at the reproductive stage. Scale bar = 15 cm. (B) Flag leaves of TQ and NAL8RNAi #1 and #2. Scale bar = 5 cm. (C) Mature panicles of ZH11 and NAL8RNAi #1 and #2. Scale bar = 5 cm. (D-K) Statistical comparisons of average flag leaf width (n = 20 plants) (D), average plant height (n = 20 plants) (E), average spikelet number (n = 20 plants) (F), average thousand seed weight (n = 20 plants) (G), average grain width (n = 20 plants) (H), average grain length (n = 20 plants) (I), average flag leaf length (n = 20 plants) (J) and the relative expression of NAL8 (n = 3 pooled tissues, three plants per pool) (K) in ZH11 and NAL8RNAi #1 and #2. Values in D-K are given as the mean ± SD. *P < 0.05; **P < 0.01 compared with the TQ control using Student’s t-test. The UBQ5 gene was used as an internal reference to normalize the gene expression data. (PDF 81 kb)
Changes in Pain and Mental Health Symptoms Associated with Prescribed Medicinal Cannabis Use: A One-Year Longitudinal Study
Creators: name: Halman, Andreas
name: Chenhall, Richard
name: Perkins, Daniel
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Chronic pain and mental health issues like depression and anxiety significantly contribute to disease burden in Western countries. While cannabinoids are suggested to have analgesic, anxiolytic and antidepressant properties, evidence, especially for long-term use, is inconclusive. This 12-month observational study evaluated the effects of prescribed medicinal cannabis for 96 patients suffering from pain, as well as sleep disturbances, depression and anxiety. Treatment outcomes for pain, depression, anxiety and sleep problems were assessed at 3, 6, and 12 months using validated instruments. Significant reductions were observed in pain scores and the interference of pain on daily functions, alongside improvements in mental health and sleep. Many patients reported notable improvements in pain severity and reduced use of pain medications in the first 6 months, with a decline at 12 months. Additionally, sustained improvements in depression, anxiety, stress and sleep were observed, with about half reporting substantial improvement. Adverse effects were common but mostly mild or moderate, most commonly dry mouth and sleepiness. These results show that prescribed medicinal cannabis treatment is associated with improvements in chronic pain and mental health symptoms, such as depression, anxiety and stress. However, findings also suggest reduced effectiveness with longer-term use, emphasizing the need for additional research.
Musca cibaria Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca cibaria

description: Musca cibaria [spec. nov.]
M. antennis setariis laevis, vertice punctis tribus elevatis, abdomine cinereo adunco, pedibus elongatis.
Habitat in Culinis & in cibariis antiquis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 599, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Spin-2 Portal Dark Matter
Creators: name: Bernal, Nicolas
name: Dutra, Maira
name: Mambrini, Yann
name: Olive, Keith A.
name: Peloso, Marco
name: Pierre, Mathias
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We generalize models invoking a spin-2 particle as a mediator between the dark sector and the Standard Model. We show that a massive spin-2 messenger can efficiently play the role of a portal between the two sectors. The dark matter is then produced via a freeze-in mechanism during the reheating epoch. In a large part of the parameter space, production through the exchange of a massive spin-2 mediator dominates over processes involving a graviton with Planck suppressed couplings. We perform a systematic analysis of such models for different values of the spin-2 mass relative to the maximum and the final temperature attained at reheating.
description: 10 pages, 3 figures
Collective fields, Calogero-Sutherland model and generalized matrix models
Creators: name: Awata, H.
name: Matsuo, Y.
name: Odake, S.
name: Shiraishi, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: On the basis of the collective field method, we analyze the Calogero--Sutherland model (CSM) and the Selberg--Aomoto integral, which defines, in particular case, the partition function of the matrix models. Vertex operator realizations for some of the eigenstates (the Jack polynomials) of the CSM Hamiltonian are obtained. We derive Virasoro constraint for the generalized matrix models and indicate relations with the CSM operators. Similar results are presented for the $q$--deformed case (the Macdonald operator and polynomials), which gives the generating functional of infinitely many conserved charges in the CSM.
description: 13 pages, latex, no figures, a few references added
Musca scybalaria Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca scybalaria

description: Musca scybalaria [spec. nov.]
M. antennis setariis pilosa rufo-ferruginea hirta, alis puncto obscuriore.
Habitat in Stercore.
Similis M. stercorariae sed duplo major, & saturatius colorata.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 599, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Texas Spectroscopic Search for Ly$α$ Emission at the End of Reionization I. Constraining the Ly$α$ Equivalent Width Distribution at 6.0 < $z$ < 7.0
Creators: name: Jung, Intae
name: Finkelstein, Steven L.
name: Livermore, Rachael C.
name: Dickinson, Mark
name: Larson, Rebecca L.
name: Papovich, Casey
name: Song, Mimi
name: Tilvi, Vithal
name: Wold, Isak
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The distribution of Ly$α$ emission is an presently accessible method for studying the state of the intergalactic medium (IGM) into the reionization era. We carried out deep spectroscopic observations in order to search for Ly$α$ emission from galaxies with photometric redshifts $z$ = 5.5 - 8.3 selected from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). Utilizing data from the Keck/DEIMOS spectrograph, we explore a wavelength coverage of Ly$α$ emission at $z$ ~ 5 - 7 with four nights of spectroscopic observations for 118 galaxies, detecting five emission lines with ~ 5$σ$ significance: three in the GOODS-N and two in the GOODS-S field. We constrain the equivalent width (EW) distribution of Ly$α$ emission by comparing the number of detected objects with the expected number constructed from detailed simulations of mock emission lines that account for the observational conditions (e.g., exposure time, wavelength coverage, and sky emission) and galaxy photometric redshift probability distribution functions. The Ly$α$ EW distribution is well described by an exponential form, $\text{dN/dEW}\propto \text{exp(-EW/}W_0)$, characterized by the $e$-folding scale ($W_0$) of ~ 60 - 100$Å$ at 0.3 < $z$ < 6. By contrast, our measure of the Ly$α$ EW distribution at 6.0 < $z$ < 7.0 rejects a Ly$α$ EW distribution with $W_0$ > 36.4$Å$ (125.3$Å$) at 1$σ$ (2$σ$) significance. This provides additional evidence that the EW distribution of Ly$α$ declines at $z$ > 6, suggesting an increasing fraction of neutral hydrogen in the IGM at that epoch.
description: 16 pages, 12 figures, 3 tables, Submitted to ApJ
13CO(J=1-0) Depression in Luminous Starburst Mergers, Revisited
Creators: name: Taniguchi, Yoshiaki
name: Ohyama, Youichi
name: Sanders, D. B.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It is known that merging galaxies with luminous starbursts and high far-infrared luminosities tend to have higher $R_{1-0} =^{12}CO(J=1-0)/^{13}CO(J=1-0)$ integrated line intensity ratios ($R_{1-0} \simeq 20-50$) than normal spiral galaxies ($R_{1-0} \simeq 5-15$). Comparing far-infrared luminosities [L(FIR)] with those of ^{12}CO(J=1-0) and ^{13}CO(J=1-0) for a sample of normal and starburst galaxies, Taniguchi & Ohyama found that the observed high $R_{1-0}$ values for the luminous starburst mergers are attributed to their lower ^{13}CO line intensities by a factor of 3 on the average. They suggested the following two possibilities; in the luminous starburst mergers, 1) ^{13}CO is underabundant with respect to ^{12}CO, or 2) exitation and/or optical depth effects are responsible for the change in $R_{1-0}$. In this paper, we investigate the second possibility using higher transition data of both ^{12}CO and ^{13}CO emission lines. Applying the same method proposed by Taniguchi & Ohyama to both ^{12}CO(J=2-1) and ^{13}CO(J=2-1), we find that ^{13}CO(J=2-1) is also depressed with respect to ^{12}CO(J=2-1). This suggests that the ^{13}CO gas may be underabundant in the high-$R_{1-0}$ starburst mergers although we cannot rule out the possibility that excitation and optical depth effects are still affecting $R_{2-1}$, for example due to the large velocity widths in the CO emission lines. Additional observations of both ^{12}CO and ^{13}CO lines at $J \geq 3$ are required to better constrain the conditions of the molecular gas in luminous starburst galaxies.
description: 12 pages, 2 tables, and 6 figures. Accepted for publications in The Astrophysical Journal, Part 1
Phase boundaries, nucleation rates and speed of crystal growth of the water-to-ice transition under an electric field: a simulation study
Creators: name: Zaragoza, Alberto
name: Espinosa, Jorge R
name: Ramos, Regina
name: Cobos, José Antonio
name: Aragones, Juan Luis
name: Vega, Carlos
name: Sanz, Eduardo
name: Ramírez, Jorge
name: Valeriani, Chantal
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We investigate with computer simulations the effect of applying an electric field on the water-to-ice transition. We use a combination of state-of-the-art simulation techniques to obtain phase boundaries and crystal growth rates (direct coexistence), nucleation rates (seeding) and interfacial free energies (seeding and mold integration). First, we consider ice Ih, the most stable polymorph in the absence of a field. Its normal melting temperature, speed of crystal growth and nucleation rate (for a given supercooling) diminish as the intensity of the field goes up. Then, we study polarised cubic ice, or ice Icf, the most stable solid phase under a strong electric field. Its normal melting point goes up with the field and, for a given supercooling, under the studied field (0.3 V/nm) ice Icf nucleates and grows at a similar rate as Ih with no field. The net effect of the field would be then that ice nucleates at warmer temperatures, but in the form of ice Icf. The main conclusion of this work is that reasonable electric fields (not strong enough to break water molecules apart) are not relevant in the context of homogeneous ice nucleation at 1 bar.
Additional file 8: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: Developmental Biology
subject: Plant Biology

description: Figure S8. Transgenic rice plants overexpressing NAL8 show no obvious developmental effects. (A) Plant architecture of the wild-type ZH11 and transgenic NAL8-overexpressing lines NAL8OE #1 and #2 at the reproductive stage. Scale bar = 15 cm. (B) Flag leaves of ZH11 and NAL8OE #1 and #2. Scale bar = 5 cm. (C) Mature panicles of ZH11 and NAL8OE #1 and #2. Scale bar = 5 cm. (D-K) Statistical comparisons of average flag leaf width (n = 20 plants) (D), average plant height (n = 20 plants) (E), average spikelet number (n = 20 plants) (F), average thousand seed weight (n = 20 plants) (G), average grain width (n = 20 plants) (H), average grain length (n = 20 plants) (I), average flag leaf length (n = 20 plants) (J) and the relative expression of NAL8 (n = 3 pooled tissues, three plants per pool) (K) in ZH11 and NAL8OE #1 and #2. Values in (D-K) are given as the mean ± SD. *P < 0.05; **P < 0.01 compared with the ZH11 control using Student’s t-test. The UBQ5 gene was used as an internal reference to normalize the gene expression data. (PDF 79 kb)
Musca stercoraria Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca stercoraria

description: Musca stercoraria [spec. nov.]
M. antennis setariis pilosa grisea hirta, alis puncto obscuriore. Fn. svec. 1068.
Reaum. ins. 4. t. 27. f. 1-3.
Habitat in Stercore.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 599, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
An ab initio perspective on scanning tunneling microscopy measurements of the tunable Kondo resonance of the TbPc$_2$ molecule on a gold substrate
Creators: name: Vrubel, Ivan I.
name: Pervishko, Anastasiia A.
name: Herper, Heike
name: Brena, Barbara
name: Eriksson, Olle
name: Yudin, Dmitry
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: With recent advances in the areas of nanostructure fabrication and molecular spintronics the idea of using single molecule magnets as building blocks for the next generation electronic devices becomes viable. A particular example represents a metal-organic complex in which organic ligands surround a rare-earth element or transition metal. Recently, it was explicitly shown that the relative position of the ligands with respect to each other can be reversibly changed by the external voltage without any need of the chemical modification of the sample. This opens a way of the electrical tuning of the Kondo effect in such metal-organic complexes. In this work, we present a detailed and systematic analysis of this effect in TbPc$_2$ from an ab initio perspective and compare the obtained results with the existing experimental data.
description: 8 pages, 5 figures
Waves and Solitons in the Continuum Limit of the Calogero-Sutherland Model
Creators: name: Polychronakos, Alexios P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We examine a collection of particles interacting with inverse-square two-body potentials in the thermodynamic limit. We find explicit large-amplitude density waves and soliton solutions for the motion of the system. Waves can be constructed as coherent states of either solitons or phonons. Therefore, either solitons or phonons can be considered as the fundamental excitations. The generic wave is shown to correspond to a two-band state in the quantum description of the system, while the limiting cases of solitons and phonons correspond to particle and hole excitations.
description: Version to appear in Physical Rerview Letters; contains some new results and explanations
Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
Creators: name: Patel, Ekta
name: Besla, Gurtina
name: Mandel, Kaisey
name: Sohn, Sangmo Tony
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: High precision proper motion (PM) measurements are available for approximately 20% of all known dwarf satellite galaxies of the Milky Way (MW). Here we extend the Bayesian framework of Patel et al. (2017b) to include all MW satellites with measured 6D phase space information and apply it with the Illustris-Dark simulation to constrain the MW's mass. Using the properties of each MW satellite individually, we find that the scatter among mass estimates is reduced when the magnitude of specific orbital angular momentum (j) is adopted rather than their combined instantaneous positions and velocities. We also find that high j satellites (i.e. Leo II) constrain the upper limits for the MW's mass and low j satellites rather than the highest speed satellites (i.e. Leo I and LMC), set the lower mass limits. When j of all classical satellites is used to simultaneously estimate the MW's mass, we conclude the halo mass is $0.85^{+0.23}_{-0.26}\times 10^{12} \rm \, M_{\odot}$ (including Sagittarius dSph) and $0.96^{+0.29}_{-0.28} \times 10^{12} \rm \, M_{\odot}$ (excluding Sagittarius dSph), cautioning that low j satellites on decaying orbits like Sagittarius dSph may bias the distribution. These estimates markedly reduce the current factor of two spread in the mass range of the MW. We also find a well-defined relationship between host halo mass and satellite j distribution, which yields the prediction that upcoming PMs for ultra-faint dwarfs should reveal j within $ 5\times10^3 - 10^4$ kpc km s$^{-1}$. This is a promising method to significantly constrain the cosmologically expected mass range for the MW and eventually M31 as more satellite PMs become available.
description: 20 pages, 7 figures, submitted to ApJ
Eigendecomposition-Free Sampling Set Selection for Graph Signals
Creators: name: Sakiyama, Akie
name: Tanaka, Yuichi
name: Tanaka, Toshihisa
name: Ortega, Antonio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper addresses the problem of selecting an optimal sampling set for signals on graphs. The proposed sampling set selection (SSS) is based on a localization operator that can consider both vertex domain and spectral domain localization. We clarify the relationships among the proposed method, sensor position selection methods in machine learning, and conventional SSS methods based on graph frequency. In contrast to the conventional graph signal processing-based approaches, the proposed method does not need to compute the eigendecomposition of a variation operator, while still considering (graph) frequency information. We evaluate the performance of our approach through comparisons of prediction errors and execution time.
Safety of Naldemedine for Opioid-Induced Constipation – A Systematic Review and Meta-Analysis
Creators: name: Wobbe, Bastian
name: Gerner, Maximilian
name: Köhne, Claus-Henning
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Space Science
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Naldemedine is a peripheral acting µ-opioid receptor antagonist approved by the Food and Drug Administration to treat opioid-induced constipation. Concerns about side effects like opioid withdrawal prevent its widespread use, especially for cancer patients. We performed this systematic review and meta-analysis to evaluate existing safety data of naldemedine treating opioid-induced constipation following the PRISMA guidelines. We searched PubMed and the Cochrane Library on April 16th 2024 to identify studies evaluating naldemedine treatment among patients with opioid-induced constipation. Our analysis found no differences between groups comparing naldemedine therapy with placebo-control for treatment-emergent adverse events (OR = 1.06; 95%-CI: 0.91–1.24), serious adverse events (OR = 1.02; 95%-CI: 0.76–1.38). We found no increased risk for opioid withdrawal, while an increased risk for gastrointestinal disorders (OR = 2.08; 95%-CI: 1.72–2.51), particularly higher incidences of diarrhea (OR = 2.44; 95%-CI: 1.81–3.29) and abdominal pain (OR = 3.31; 95%-CI: 2.16–5.06) were found. In the cancer subgroup, treatment-emergent and serious adverse events were more frequent. However, no increased risk for opioid withdrawal was observed. This analysis confirms naldemedine’s overall safety in treating opioid-induced constipation, with manageable gastrointestinal side effects. However, the higher adverse events in cancer patients require further investigation to ensure safe use in this population.
Lifetime Limit of LSP from Cosmological Light Elements
Creators: name: Kim, Jihn E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: From the present cosmic abundance of the light elements, one can obtain a lifetime bounds of LSP. From the consideration of deuterium, we obtain $τ_χ \ge 10^6$ s.
description: Latex file of 5 pages with two eps figures. Talk presented at cosmo-98, Asilomar, CA, Nov., 1998
TRIB3 expression in human adipose tissue
Creators: name: Lee, Seul Ki
name: Park, Chan Yoon
name: Kim, Jimin
name: Kim, Donguk
name: Choe, Han
name: Kim, Jong-Hyeok
name: Hong, Joon Pio
name: Lee, Yeon Ji
name: Heo, Yoonseok
name: Park, Hye Soon
name: Jang, Yeon Jin
Publisher: name: figshare
Year: 2021
Subjects: subject: 110107 Metabolic Medicine
subject: FOS: Clinical medicine

description: supplementary table and figures for article
B2 1144+35: A Giant Low Power Radio Galaxy with Superluminal Motion
Creators: name: Giovannini, G.
name: Taylor, G. B.
name: Arbizzani, E.
name: Bondi, M.
name: Cotton, W. D.
name: Feretti, L.
name: Lara, L.
name: Venturi, T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on centimeter VLA and VLBI observations of the giant, low power radio galaxy 1144+35. These observations are sensitive to structures on scales from less than 1 parsec to greater than 1 megaparsec. Diffuse steep spectrum lobes on the megaparsec scale are consistent with an age of $\sim$ 10$^8$ years. On the parsec scale, a complex jet component is seen to move away from the center of activity with an apparent velocity 2.7 h$^{-1}_{50}$ c. It shows a central spine -- shear layer morphology. A faint parsec scale counterjet is detected and an intrinsic jet velocity of 0.95 c and angle to the line of sight of 25$^\circ$ are derived, consistent with an intrinsically symmetric ejection. The central spine in the parsec scale jet is expected to move at a higher velocity and a Lorentz factor $γ$ $\sim$ 15 has been estimated near the core.The age of this inner VLBI structure is $\sim$ 300 years. Assuming a constant angle to the line-of-sight, the jet velocity is found to decrease from 0.95 c at 20 mas (32 pc on the plane of the sky) to 0.02 c at 15 arcsec (24 kpc on the plane of the sky). These findings lend credence to the claim that (1) even the jets of low power radio galaxies start out relativistic; and (2) these jets are decelerated to subrelativistic velocities by the time they reach kiloparsec scales.
description: 21 pages, 16 separated figures. A version with figures and table in the text is available at: ftp://terra.bo.cnr.it/papers/journals - it is a ps gzipped file, named giovannini_apr99.gz (792kb) - ApJ in press
Weak Control for Human-in-the-loop Systems
Creators: name: Inoue, Masaki
name: Gupta, Vijay
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In this letter, we propose a control framework for human-in-the-loop systems, in which many human decision makers are involved in the feedback loop composed of a plant and a controller. The novelty of the framework is that the decision makers are weakly controlled; in other words, they receive a set of admissible control actions from the controller and choose one of them in accordance with their private preferences. For example, the decision makers can decide their actions to minimize their own costs or by simply relying on their experience and intuition. A class of controllers which output set-valued signals is proposed, and it is shown that the overall control system is stable independently of the decisions made by the humans. Finally, a learning algorithm is applied to the controller that updates the controller parameters to reduce the achievable minimal costs for the decision makers. Effective use of the algorithm is demonstrated in a numerical experiment.
Counts, Sizes and Colors of Faint Infrared Selected Galaxies
Creators: name: Saracco, P.
name: D'Odorico, S.
name: Moorwood, A.
name: Cuby, J. G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Deep J and Ks band images covering a $5\times5$ arcmin area centered on the NTT Deep Field have been obtained during the Science Verification of SOFI at the NTT. These images were made available via the Web in early June. The preliminary results we have obtained by the analysis of these data are the following: 1) the counts continue to rise with no evidence of a turnover or of a flattening down to the limits of the survey (Ks=22.5 and J=24); 2) we find a slope $dlog(N)/dm\sim$0.37 in agreement with most of the faintest surveys but much steeper than the Hawaii survey; 3) fainter than Ks$\sim19$ and J$\sim20$, the median J-K color of galaxies shows a break in its reddening trend turning toward bluer colors; 4) faint bluer galaxies also display a larger compactness index, and a smaller apparent size.
description: 8 pages, 5 figures, proc. of the Euroconference on "The Evolution of Galaxies on Cosmological Timescale", to appear in Ap&SS
Symplectic no-core configuration interaction framework for ab initio nuclear structure
Creators: name: McCoy, Anna E.
name: Caprio, Mark A.
name: Dytrych, Tomas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We introduce a symplectic no-core configuration interaction (SpNCCI) framework for ab initio nuclear structure calculations, in a correlated many-body basis which encodes an approximate Sp(3,R) symmetry of the nucleus. Such a scheme potentially provides a means of restricting the many-body space to include only those highly-excited configurations which dominantly contribute to the nuclear wave function. We examine the symplectic symmetry structure arising in an illustrative ab initio SpNCCI calculation for 6Li. We observe both the dominance of symplectic symmetry in individual wave functions and the emergence of families of states related by symplectic symmetry.
description: 14 pages, 5 figures; presented at Advanced Many-Body and Statistical Methods in Mesoscopic Systems III, Busteni, Romania, September 4-8, 2017; submitted to Ann. Acad. Rom. Sci. Ser. Chem. Phys. Sci
Additional file 9: of NAL8 encodes a prohibitin that contributes to leaf and spikelet development by regulating mitochondria and chloroplasts stability in rice
Creators: name: Chen, Ke
name: Guo, Tao
name: Li, Xin-Min
name: Yang, Yi-Bing
name: Dong, Nai-Qian
name: Shi, Chuan-Lin
name: Ye, Wang-Wei
name: Shan, Jun-Xiang
name: Lin, Hong-Xuan
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Developmental Biology
subject: Marine Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S9. Grain phenotypes of the NAL8 transgenic lines. (A) Mature rice grains of ZH11 and the transgenic NAL8OE overexpression lines. Scale bar = 2 mm. (B) Mature rice grains of TQ and the transgenic NAL8RNAi gene silencing lines. Scale bar = 2 mm. (C) Mature rice grains of ZH11 and the transgenic NAL8CRISPR transgenic lines. Scale bar = 2 mm. (D) Mature rice grains of TQ, the nal8 mutant and the transgenic two NAL8com complementation lines in the nal8 genetic background. Scale bar = 2 mm. (PDF 118 kb)
Musca fimetaria Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Anthomyiidae
Musca
Musca fimetaria

description: Musca fimetaria [spec. nov.]
M. antennis setariis pilosa livens glabrata, alis puncto obscuriore.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 599, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Smoothed Particle Hydrodynamics Simulations of Ultra-Relativistic Shocks with Artificial Viscosity
Creators: name: Siegler, S.
name: Riffert, H.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a fully Lagrangian conservation form of the general relativistic hydrodynamic equations for perfect fluids with artificial viscosity in a given arbitrary background spacetime. This conservation formulation is achieved by choosing suitable Lagrangian time evolution variables, from which the generic fluid variables rest-mass density, 3-velocity, and thermodynamic pressure have to be determined. We present the corresponding equations for an ideal gas and show the existence and uniqueness of the solution. On the basis of the Lagrangian formulation we have developed a three-dimensional general relativistic Smoothed Particle Hydrodynamics (SPH) code using the standard SPH formalism as known from non-relativistic fluid dynamics. One-dimensional simulations of a shock tube and a wall shock are presented. With our method we can model ultra-relativistic fluid flows including shocks with relativistic gamma-factors of even 1000.
description: 24 pages, 24 postscript figures, submitted to the Astrophysical Journal
Rhinella mirandaribeiroi
Creators: name: Moreno, Julian Sebastián Ramirez
name: Giaretta, Ariovaldo Antonio
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Amphibia
Anura
Bufonidae
Rhinella
Rhinella mirandaribeiroi

description: Rhinella mirandaribeiroi (Cerrado vs. Topotypes)
Morphologic and Morphometric
Morphometric variable values can be found in Table 1. The topotypes of R. mirandaribeiroi are morphologically similar to B. g. lutzi and other specimens from the Cerrado, and they can be diagnosed from most species in the group by: granular or continuous cranial crests, low supraorbital crest, infraorbital crest extending usually beyond the postorbital crest, generally discontinuous reduced maxillary crest, and absence of a parietal crest (Figures 1–2). Loreal region clearly visible in dorsal view, tympanum very close to the postorbital crest (DTP 0.4–1.0% CRC), a usually present clear longitudinal vertebral line, and a light cream or yellowish ventral side, with or without pigmentation. Neither morphological nor morphometric characters allowed for the diagnosis between populations.
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Acoustics
We found conserved parameters of call features among samples. All evaluated specimens have advertisement calls consisting of regular series of pulsed notes (trills) that can last up to 11 seconds. The call has ascending amplitude modulation, with the initial notes generally having low amplitude and then quickly reaching the maximum, which is maintained up the end. The notes consist of three to five concatenated pulses (without intervals of silence). No acoustic feature was different among the evaluated populations.
Topotypical population of R. mirandaribeiroi (Soure, Marajó Island)
In the type locality, males vocalize after rains at night in shallow puddles formed along dirt roads on the outskirts of the city. The immediate surroundings of these vocalization sites were open anthropogenic environments with pasture or cultivated areas. Syntopic anurans include Leptodactylus fuscus, Scinax x-signatus, Boana raniceps, S. fuscomarginatus, Physalaemus ephippifer, and Adenomera hylaedactyla. The advertisement call consists of a sequence of approximately 126 notes and lasts around 4 seconds, emitted at a rate of 8 calls per minute with 33 notes per second. The calls reach maximum amplitude rapidly and remain constant until the end (Figure 3). The notes have a duration of about 20 ms and contain 3−4 pulses per note. The dominant frequency is around 2800 Hz. Further details in Table 2.
description: Published as part of Moreno, Julian Sebastián Ramirez & Giaretta, Ariovaldo Antonio, 2025, The identity of Rhinella mirandaribeiroi (Gallardo, 1965) (Anura: Bufonidae) and its diagnosis in relation to Rhinella granulosa (Spix, 1824), pp. 105-128 in Zootaxa 5588 (1) on pages 107-111, DOI: 10.11646/zootaxa.5588.1.4, http://zenodo.org/record/14896118
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0557
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0557, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0557, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Limits on the Reconstruction of a Single Dark Energy Scalar Field Potential from SNe Ia Data
Creators: name: Piloyan, Arpine
name: Pavluchenko, Sergey
name: Amendola, Luca
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this paper we perform a reconstruction of the scalar field potential responsible for cosmic acceleration using SNe Ia data. After describing the method, we test it with real SNe Ia data-Union2.1 and JLA SNe datasets. We demonstrate that with the current data precision level, the full reconstruction is not possible. We discuss the problems which arise during the reconstruction process and the ways to overcome them.
description: 14 pages, 5 figures, published in Particles in the Special Issue Selected Papers from "The Modern Physics of Compact Stars and Relativistic Gravity 2017"
Dimensional Perturbation Theory on the Connection Machine
Creators: name: Germann, Timothy C.
name: Herschbach, Dudley R.
name: Boghosian, Bruce M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A recently developed linear algebraic method for the computation of perturbation expansion coefficients to large order is applied to the problem of a hydrogenic atom in a magnetic field. We take as the zeroth order approximation the $D \rightarrow \infty$ limit, where $D$ is the number of spatial dimensions. In this pseudoclassical limit, the wavefunction is localized at the minimum of an effective potential surface. A perturbation expansion, corresponding to harmonic oscillations about this minimum and higher order anharmonic correction terms, is then developed in inverse powers of $(D-1)$ about this limit, to 30th order. To demonstrate the implicit parallelism of this method, which is crucial if it is to be successfully applied to problems with many degrees of freedom, we describe and analyze a particular implementation on massively parallel Connection Machine systems (CM-2 and CM-5). After presenting performance results, we conclude with a discussion of the prospects for extending this method to larger systems.
description: 19 pages, REVTeX
ASCA and ROSAT observations of NGC5548: discrepant spectral indices
Creators: name: Iwasawa, K.
name: Fabian, A. C.
name: Nandra, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on simultaneous ASCA and ROSAT observations of the Seyfert galaxy NGC5548 made during the ASCA Performance Verification phase. Spectral features due to a warm absorber and reflection are clearly seen in the X-ray spectra. We find that the continuum spectral shape differs between the ASCA and ROSAT datasets. The photon-index obtained from the ROSAT PSPC exceeds that from the ASCA SIS about 0.4. The discrepancy is clear even in the 0.5-2 keV energy band over which both detectors are sensitive. The spectra cannot be made consistent by choosing a more complex model. The problem likely lies in the response curve (estimated effective area) of one, or both, detectors. There may be important consequences for a wide range of published results.
description: 9 pages, accepted for publication in MNRAS
Metodología de la enseñanza del lenguaje y la redacción en espacios universitarios. Entrevista a Lenin Pantoja Torres
Creators: name: Delgado Del Aguila, Jesús Miguel
Publisher: name: figshare
Year: 2022
Subjects: classificationCode: 390405
subject: Educational technology and computing

description: Delgado Del Aguila, Jesús Miguel (2022). «Metodología de la enseñanza del lenguaje y la redacción en espacios universitarios. Entrevista a Lenin Pantoja Torres», en: Pucara. Revista de Humanidades. Cuenca, Ecuador: Universidad de Cuenca. Vol. 1, n.° 33, pp. 1-5. Disponible en https://doi.org/10.18537/puc.33.01.09