cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Estimating photometric redshifts with artificial neural networks
Creators: name: Firth, Andrew E.
name: Lahav, Ofer
name: Somerville, Rachel S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A new approach to estimating photometric redshifts - using Artificial Neural Networks (ANNs) - is investigated. Unlike the standard template-fitting photometric redshift technique, a large spectroscopically-identified training set is required but, where one is available, ANNs produce photometric redshift accuracies at least as good as and often better than the template-fitting method. The Bayesian priors on the underlying redshift distribution are automatically taken into account. Furthermore, inputs other than galaxy colours - such as morphology, angular size and surface brightness - may be easily incorporated, and their utility assessed. Different ANN architectures are tested on a semi-analytic model galaxy catalogue and the results are compared with the template-fitting method. Finally the method is tested on a sample of ~ 20000 galaxies from the Sloan Digital Sky Survey. The r.m.s. redshift error in the range z < 0.35 is ~ 0.021.
description: Submitted to MNRAS, 9 pages, 9 figures, substantial improvements to paper structure
Additional file 2: of Characterization of high healthcare utilizer groups using administrative data from an electronic medical record database
Creators: name: Ng, Sheryl
name: Rahman, Nabilah
name: Ang, Ian
name: Srinath Sridharan
name: Sravan Ramachandran
name: Wang, Debby
name: Chuen Tan
name: Sue-Anne Toh
name: Tan, Xin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Marine Biology

description: Descriptive statistics for persistent and non-persistent high utilizers (HUs). (DOCX 19 kb)
Data management in distributed shared virtual worlds
Creators: name: Nedelec, Tanguy
Publisher: name: Freie Universität Berlin
Year: 2002
Subjects: subject: 000 Informatik, Informationswissenschaft, allgemeine Werke::000 Informatik, Wissen, Systeme::004 Datenverarbeitung; Informatik

description: Research efforts in Virtual Worlds domain have been mainly devoted to user interfaces, communication supports and consistency issues. To the best of our knowledge, no works clearly focused on the global problem of managing virtual world’s data. The promise of future large persistent virtual worlds, evolving during a long period of time and with large number of participants makes the question of data management even more crucial. This paper introduces the global problem of managing data in virtual worlds and reports our research work in using data management services for virtual worlds platforms.
Understanding the radio emission geometry of multi-component radio pulsars from retardation and aberration effects
Creators: name: Gupta, Y.
name: Gangadhara, R. T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have conducted a detailed analysis of the emission geometry of a handful of radio pulsars that have prominent, multiple-component profiles at meter wavelengths. From careful determination of the total number of emission components and their locations in pulse longitude, we find that all of the six pulsars show clear evidence for retardation and aberration effects in the conal emission beams. Using this information, coupled with a dipolar field geometry, we obtain estimates of the height and transverse location in the magnetosphere, for each of the emitting cones in these pulsars. These results support our earlier conclusions for PSR B0329+54 in that we find successive outer cones (in cases of multi-cone pulsars) being emitted at higher altitudes in the magnetosphere. The range of inferred heights is from ~200 to ~2200 km. The set of ``active'' field lines from which the conal emissions originate are located in the region from ~0.22 to ~0.74 of the polar cap radius. At the neutron star surface, these conal rings map to radii of a few to several tens of meters and the separation between successive rings is about 10 to 20 meters. We discuss the implications of these findings for the understanding of the pulsar emission geometry and for current theories and models of the emission mechanism.
description: 20 pages, 2 figures. Accepted for Astrophysical Journal, 2002
Eragrostis olivacea K. Schum.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Eragrostis
Eragrostis olivacea

description: Eragrostis olivacea K.Schum. in H.G.A.Engler (ed.), Pflanzenw. Ost-Afrikas, C: 114 (1895).
 Distribution: Ethiopia to S. Trop. Africa
 Specimens: MOSHI Bismark Hill, Greenway, P.J. 3823 (K, NH); Bismark Hill, Mwasumbi, L.B. 14126 (K); Kidia, Hemp, A. 1459 (NHT, UBT); Machame hut, Hemp, A. 2544 (NHT, UBT); Machame hut, Hemp, A. 2561 (NHT, UBT); Mandara Hut (=Bismark Hut), Hitchcock, A.S. 24615 (K); Mandara Hut (=Bismark Hut), Procter, J. 3739 (K, NH); Marangu, Volkens, G. 894 (K, NH); Marangu-Mandara track, Hemp, A. 2085 (NHT, UBT); Natiro, Hemp, A. 2185 (NHT, UBT); s. loc., Geilinger, W. 4357 (K); s. loc., Geilinger, W. s.n. (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 226, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Human detection of machine manipulated media
Creators: name: Groh, Matthew
name: Epstein, Ziv
name: Obradovich, Nick
name: Cebrian, Manuel
name: Rahwan, Iyad
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (cs.LG)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Recent advances in neural networks for content generation enable artificial intelligence (AI) models to generate high-quality media manipulations. Here we report on a randomized experiment designed to study the effect of exposure to media manipulations on over 15,000 individuals' ability to discern machine-manipulated media. We engineer a neural network to plausibly and automatically remove objects from images, and we deploy this neural network online with a randomized experiment where participants can guess which image out of a pair of images has been manipulated. The system provides participants feedback on the accuracy of each guess. In the experiment, we randomize the order in which images are presented, allowing causal identification of the learning curve surrounding participants' ability to detect fake content. We find sizable and robust evidence that individuals learn to detect fake content through exposure to manipulated media when provided iterative feedback on their detection attempts. Over a succession of only ten images, participants increase their rating accuracy by over ten percentage points. Our study provides initial evidence that human ability to detect fake, machine-generated content may increase alongside the prevalence of such media online.
Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
Creators: name: Hashimoto, Daiki
name: Macias, Oscar
name: Nishizawa, Atsushi J.
name: Hayashi, Kohei
name: Takada, Masahiro
name: Shirasaki, Masato
name: Ando, Shin'ichiro
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Searches for dark matter annihilation signals have been carried out in a number of target regions such as the Galactic Center and Milky Way dwarf spheroidal galaxies (dSphs), among a few others. Here we propose low surface brightness galaxies (LSBGs) asnovel targets for the indirect detection of dark matter emission. In particular, LSBGs are known to have very large dark matter contents and be less contaminated by extragalactic gamma-ray sources (e.g., blazars) compared to star forming galaxies. We report on an analysis that uses eight LSBGs (detected by Subaru Hyper Suprime-Cam survey data) with known redshifts to conduct a search for gamma-ray emission at the positions of these new objects in Fermi Large Area Telescope data. We found no excesses of gamma-ray emission and set constraints on the dark matter annihilation cross-section. We exclude (at the 95% C.L.) dark matter scenarios predicting a cross-section higher than 10^-23[cm^3/s] for dark matter particles of mass 10 GeV self-annihilating in the b_b channel. Although this constraint is weaker than the ones reported in recent studies using other targets, we note that in the near future, the number of detections of new LSBGs will increase by a few orders of magnitude. We forecast that with the use of the full catalog of soon-to-be-detected LSBGs the constraint will reach cross-section sensitivities of ~ 3*10^-25 [cm^3/s] for dark matter particles with masses less than 10 GeV.
description: 19 pages, 6 figures, accepted to JCAP
Polymerus (Poeciloscytus) lammesi Rinne 1989
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Polymerus
Polymerus lammesi

description: Polymerus (Poeciloscytus) lammesi Rinne, 1989
 Material examined. TEHRAN: Azad Bar, several specimens, 8.-10.vii.1995.
 Comments. On Galium spp. in wet mountain meadows at high altitudes. Extending from southern Finland and Sweden to Central Europe and the Balkan Peninsula, also known from the Khorasan province in Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 34, DOI: 10.5281/zenodo.5328235
MOESM1 of Improvement of isoprene production in Escherichia coli by rational optimization of RBSs and key enzymes screening
Creators: name: Li, Meijie
name: Chen, Hailin
name: Liu, Changqing
name: Guo, Jing
name: Xu, Xin
name: Zhang, Haibo
name: Nian, Rui
name: Xian, Mo
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Chemical Sciences not elsewhere classified
subject: Plant Biology
subject: Computational Biology

description: Additional file 1. Table S1 . Constructed plasmids and strains in this study; Table S2. Primers used in this study; Fig. S1. OD600 of strains constructed in this study. a. OD600 of strain engineered with IDI modification. b. OD600 of strain engineered with MK modification. c. OD600 of strain engineered with IspS modification. d. OD600 ofstrain engineered through combination of the three enzymes, IDIsa, MKmm and IspSib. e. OD600 of strain with modification of RBS sequence of MvaE. f. OD600of strain with modification of RBS sequence of ERG19. The black column indicated the OD600 of original strain. The white column indicated that OD600 of strain with only enzyme substitution. The gray column indicated the OD600of strain with RBS sequence optimization. The experiment was conducted in triplicate. Bar represents meanÂąs.d.; Fig. S2. Yields of strains constructed in this study. a. Yields of strain engineered with IDI modification. b. Yields of strain engineered with MK modification. c. Yields of strain engineered with IspS modification. d. Yields of strain engineered through combination of the three enzymes, IDIsa, MKmm and IspSib. e. Yields of strain with modification of RBS sequence of MvaE. f. Yields of strain with modification of RBS sequence of ERG19. The black column indicated the isoprene yields of original strain. The white column indicated that isoprene yields of strain with only enzyme substitution. The gray column indicated the isoprene yields of strain with RBS sequence optimization. The experiment was conducted in triplicate. Bar represents meanÂąs.d.
Polymerus (Poeciloscytus) vulneratus
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Polymerus
Polymerus vulneratus

description: Polymerus (Poeciloscytus) vulneratus (Panzer, 1806)
 Material examined. GILAN: Dasht-e-Veel, 6 specimens, 20.-25.viii.1998, 8.-10.ix.2000; Gyssom, 1 specimen, 30.vi.-8.vii.1996; Rustam Abad – Salan Sar, 1 specimen, 8.-10.ix.2000; Tutkabon – Rudbar, several specimens, 25.v.-26.vi.1995, 26.v.-8.vii.1996. ARDABIL: Gareh Ghashlag, 1 specimen, 27.-28.vii.2004; Khalkhal, 2 specimens, 30.vii.1996, 10.-11.viii.2002. ZANJAN: Zanjan, 2 specimens, 13.-14.vii.2004. TEHRAN: Azad Bar, 3 specimens, 10.vii.1995; Shahrestenak, 1 specimen, 10.-12.vii.1995.
 Comments. In meadows on Galium spp. Also recorded from the Chenopodiaceae. Holopalaearctic.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 34, DOI: 10.5281/zenodo.5328235
Markov state models from short non-equilibrium simulations—Analysis and correction of estimation bias
Creators: name: Nueske, Feliks
name: Wu, Hao
name: Prinz, Jan-Hendrik
name: Wehmeyer, Christoph
name: Clementi, Cecilia
name: Noe, Frank
Publisher: name: Freie Universität Berlin
Year: 2017
Subjects: subject: Markov processes
subject: Singular values
subject: Relaxation times
subject: Trajectory models
subject: Eigenvalues
subject: 500 Naturwissenschaften und Mathematik::510 Mathematik

description: Many state-of-the-art methods for the thermodynamic and kinetic characterization of large and complex biomolecular systems by simulation rely on ensemble approaches, where data from large numbers of relatively short trajectories are integrated. In this context, Markov state models (MSMs) are extremely popular because they can be used to compute stationary quantities and long-time kinetics from ensembles of short simulations, provided that these short simulations are in “local equilibrium” within the MSM states. However, over the last 15 years since the inception of MSMs, it has been controversially discussed and not yet been answered how deviations from local equilibrium can be detected, whether these deviations induce a practical bias in MSM estimation, and how to correct for them. In this paper, we address these issues: We systematically analyze the estimation of MSMs from short non- equilibrium simulations, and we provide an expression for the error between unbiased transition probabilities and the expected estimate from many short simulations. We show that the unbiased MSM estimate can be obtained even from relatively short non-equilibrium simulations in the limit of long lag times and good discretization. Further, we exploit observable operator model (OOM) theory to derive an unbiased estimator for the MSM transition matrix that corrects for the effect of starting out of equilibrium, even when short lag times are used. Finally, we show how the OOM framework can be used to estimate the exact eigenvalues or relaxation time scales of the system without estimating an MSM transition matrix, which allows us to practically assess the discretization quality of the MSM. Applications to model systems and molecular dynamics simulation data of alanine dipeptide are included for illustration. The improved MSM estimator is implemented in PyEMMA of version 2.3.
HST observations of the cometary blue compact dwarf galaxy UGC 4483: a relatively young galaxy?
Creators: name: Izotov, Y. I.
name: Thuan, T. X.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present V and I photometry of the resolved stars in the cometary blue compact dwarf galaxy UGC 4483 using Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2) images. The resulting I vs. (V-I) color-magnitude diagram (CMD) reaches limiting magnitudes V = 27.5 mag and I = 26.5 mag for photometric errors less than 0.2 mag. It reveals not only a young stellar population of blue main-sequence stars and blue and red supergiants, but also an older evolved population of red giant and asymptotic giant branch stars. The measured magnitude I = 23.65 +/- 0.10 mag of the red giant branch tip results in a distance modulus (m-M) = 27.63 +/- 0.12, corresponding to a distance of 3.4 +/- 0.2 Mpc. The youngest stars are associated with the bright H II region at the northern tip of the galaxy. The population of older stars is found throughout the low-surface-brightness body of the galaxy and is considerably more spread out than the young stellar population, suggesting stellar diffusion. The most striking characteristics of the CMD of UGC 4483 are the very blue colors of the red giant stars and the high luminosity of the asymptotic giant branch stars. Both of these characteristics are consistent with either: 1) a very low metallicity ([Fe/H] = -2.4 like the most metal-deficient globular clusters) and an old age of 10 Gyr, or 2) a higher metallicity ([Fe/H] = -1.4 as derived from the ionized gas emission lines) and a relatively young age of the oldest stellar population in UGC 4483, not exceeding ~ 2 Gyr. Thus our data do not exclude the possibility that UGC 4483 is a relatively young galaxy having formed its first stars only ~ 2 Gyr ago.
description: 37 pages, 15 PS figures, to appear in ApJ
Additional file 1: of Evaluation of treatment response, drug resistance and HIV-1 variability among adolescents on first- and second-line antiretroviral therapy: a study protocol for a prospective observational study in the centre region of Cameroon (EDCTP READY-study)
Creators: name: Fokam, Joseph
name: Santoro, Maria
name: Takou, Desire
name: Anne-Esther Njom-Nlend
name: Ndombo, Paul
name: Kamgaing, Nelly
name: Kamta, Cedric
name: Essiane, Andre
name: Sosso, Samuel
name: Ndjolo, Alexis
name: Colizzi, Vittorio
name: Carlo-Federico Perno
Publisher: name: figshare
Year: 2019
Subjects: subject: Pharmacology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Supplementary digital contents (SDC). SDC 1: Overall summary of major timeline and activities. (DOCX 29 kb)
Dark-Ages Reionisation & Galaxy Formation Simulation XVI: The Thermal Memory of Reionisation
Creators: name: Davies, James E.
name: Mutch, Simon J.
name: Qin, Yuxiang
name: Mesinger, Andrei
name: Poole, Gregory B.
name: Wyithe, J. Stuart B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Intergalactic medium temperature is a powerful probe of the epoch of reionisation, as information is retained long after reionisation itself. However, mean temperatures are highly degenerate with the timing of reionisation, with the amount heat injected during the epoch, and with the subsequent cooling rates. We post-process a suite of semi-analytic galaxy formation models to characterise how different thermal statistics of the intergalactic medium can be used to constrain reionisation. Temperature is highly correlated with redshift of reionisation for a period of time after the gas is heated. However as the gas cools, thermal memory of reionisation is lost, and a power-law temperature-density relation is formed, $T = T_0(1+δ)^{1-γ}$ with $γ\approx 1.5$. Constraining our model against observations of electron optical depth and temperature at mean density, we find that reionisation likely finished at $z_{\rm{reion}} = 6.8 ^{+ 0.5} _{-0.8}$ with a soft spectral slope of $α= 2.8 ^{+ 1.2} _{-1.0}$. By restricting spectral slope to the range $[0.5,2.5]$ motivated by population II synthesis models, reionisation timing is further constrained to $z_{\rm{reion}} = 6.9 ^{+ 0.4} _{-0.5}$. We find that, in the future, the degeneracies between reionisation timing and background spectrum can be broken using the scatter in temperatures and integrated thermal history.
description: 17 pages, 17 figures, Accepted for publication in MNRAS
Additional file 3: of The role of clonal communication and heterogeneity in breast cancer
Creators: name: Martín-Pardillos, Ana
name: Chiva, Ángeles Valls
name: Vargas, Gemma Bande
name: Blanco, Pablo Hurtado
name: Cid, Roberto Piñeiro
name: Guijarro, Pedro
name: Hümmer, Stefan
name: Serrano, Eva Bejar
name: Rodriguez-Casanova, Aitor
name: Diaz-Lagares, Ángel
name: Castellvi, Josep
name: Miravet-Verde, Samuel
name: Serrano, Luis
name: Lluch-Senar, María
name: Sebastian, Víctor
name: Bribian, Ana
name: López-Mascaraque, Laura
name: López-López, Rafael
name: Cajal, Santiago Ramón Y
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Developmental Biology
subject: Cancer
subject: Plant Biology

description: Figure S3. Homing capacity of parental, clonal cell lines and an equal mix of all cell lines. Analysis of lung metastasis. Hematoxylin/eosin staining. Complete lung reconstruction (scale bar = 400 μm). (PDF 823 kb)
Eragrostis papposa Steud., Nomencl. Bot. 1840
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Eragrostis
Eragrostis papposa

description: Eragrostis papposa (Roem. & Schult.) Steud., Nomencl. Bot., ed. 2, 1: 564 (1840).
 Distribution: SE. Spain to NW. Africa, NE. & E. Trop. Africa to Myanmar.
 Specimens: none (see text).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 226, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Additional file 1 of Amelioration of olfactory dysfunction in a mouse model of Parkinson’s disease via enhancing GABAergic signaling
Creators: name: Liu, Xing-Yang
name: Wang, Ke
name: Deng, Xian-Hua
name: Wei, Yi-Hua
name: Guo, Rui
name: Liu, Sui-Feng
name: Zhu, Yi-Fan
name: Zhong, Jia-Jun
name: Zheng, Jing-Yuan
name: Wang, Meng-Dan
name: Ye, Qiu-Hong
name: He, Jian-Quan
name: Guo, Kai-Hang
name: Zhu, Jun-Rong
name: Huang, Shu-Qiong
name: Chen, Ze-Xu
name: Lv, Chong-Shan
name: Wen, Lei
Publisher: name: figshare
Year: 2023
Subjects: Cell Biology
Molecular Biology
Neuroscience
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Computational Biology

description: Supplementary Material 1
The signatures of the new particles $h_2$ and $Z_{μτ}$ at e-p colliders in the $U(1)_{L_μ-L_τ}$ model
Creators: name: Hou, Jin-Xin
name: Yue, Chong-Xing
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Considering the superior performances of the future e-p colliders, LHeC and FCC-eh, we discuss the feasibility of detecting the extra neutral scalar $h_{2}$ and the light gauge boson $Z^{}_{μτ}$, which are predicted by the ${U(1)}_{L^{}_μ - L^{}_τ}$ model. Taking into account the experimental constraints on the relevant free parameters, we consider all possible production channels of $h_{2}$ and $Z^{}_{μτ}$ at e-p colliders and further investigate their observability through the optimal channels in the case of the beam polarization P($e^{-}$)= -0.8. We find that the signal significance above 5$σ$ of $h_{2}$ as well as $Z^{}_{μτ}$ detecting can be achieved via $e^{-}p\to{e^{-}jh_{2}(\to{Z_{μτ}Z_{μτ}})}\to~e^{-}j+/\!\!\!\!{E}^{}_{T}$ process and a 5$σ$ sensitivity of $Z^{}_{μτ}$ detecting can be gained via $e^{-}p\to{e^{-}jh_{1}(\to{Z^{}_{μτ}Z^{}_{μτ}})\to}~e^{-}j+/\!\!\!\!{E}^{}_{T}$ process at e-p colliders with appropriate parameter values and a designed integrated luminosity. However, the signals of $h_{2}$ decays into pair of SM particles are difficult to be detected.
description: 22 pages, 9 figures, references added and typos are corrected
No Supermassive Black Hole in M33?
Creators: name: Merritt, David
name: Ferrarese, Laura
name: Joseph, Charles L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze optical long-slit spectroscopy of the nucleus of M33 obtained from the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. Rather than the steep rise expected within the radius of influence of a supermassive black hole, the velocity dispersion drops significantly within the inner parsec. Dynamical modelling yields an estimated upper limit of 3000 solar masses for the mass of a central compact object. This upper limit is however consistent within the uncertainties with the mass predicted by the M-sigma relation, which is between 2000 and 20,000 solar masses. We therefore can not conclude that the presence of a massive black hole in the nucleus of M33 would require a different formation mechanism from that of the black holes detected in galaxies with more luminous bulges.
description: 10 pages, 4 postscript figures
Taylorilygus apicalis
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Taylorilygus
Taylorilygus apicalis

description: Taylorilygus apicalis (Fieber, 1861)
 Material examined. GILAN: Rasht, 1 specimen, iv.-vi.1995.
 Comments. In hilly steppes on plants such as Pulicaria and Matricaria. Cosmopolitan in tropical and subtropical regions.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 34, DOI: 10.5281/zenodo.5328235
Additional file 1: of Characterization of high healthcare utilizer groups using administrative data from an electronic medical record database
Creators: name: Ng, Sheryl
name: Rahman, Nabilah
name: Ang, Ian
name: Srinath Sridharan
name: Sravan Ramachandran
name: Wang, Debby
name: Chuen Tan
name: Sue-Anne Toh
name: Tan, Xin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Marine Biology
subject: 60506 Virology

description: Top 5 common conditions in Year 1 high utilizer (HU) groups by visit frequency. (DOCX 19 kb)
Dynamical self-assembly of dipolar active Brownian particles in two dimensions
Creators: name: Liao, Guo-Jun
name: Hall, Carol K.
name: Klapp, Sabine H. L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Based on Brownian Dynamics (BD) simulations, we study the dynamical self-assembly of active Brownian particles with dipole-dipole interactions, stemming from a permanent point dipole at the particle center. The propulsion direction of each particle is chosen to be parallel to its dipole moment. We explore a wide range of motilities and dipolar coupling strengths and characterize the corresponding behavior based on several order parameters. At low densities and low motilities, the most important structural phenomenon is the aggregation of the dipolar particles into chains. Upon increasing the particle motility, these chain-like structures break, and the system transforms into a weakly correlated isotropic fluid. At high densities, we observe that the motility-induced phase separation is strongly suppressed by the dipolar coupling. Once the dipolar coupling dominates the thermal energy, the phase separation disappears, and the system rather displays a flocking state, where particles form giant clusters and move collective along one direction. We provide arguments for the emergence of the flocking behavior, which is absent in the passive dipolar system.
Oscillatory mean-field dynamos with spherically symmetric, isotropic alpha
Creators: name: Stefani, Frank
name: Gerbeth, Gunter
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Until recently, the existence of oscillatory mean-field dynamos of the alpha^2-type with spherically symmetric and isotropic alpha was an open question. We find such dynamos by means of an evolutionary strategy, and we illustrate the spectral properties of the corresponding dynamo operators.
description: 4 pages, 7 figures
Radiative decays in bottomonium beyond the long wave length approximation
Creators: name: Bruschini, R.
name: González, P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We revisit the nonrelativistic quark model description of electromagnetic radiative decays in bottomonium. We show that even for the simplest spectroscopic quark model the calculated widths can be in good agreement with data once the experimental masses of bottomonium states and the photon energy are properly implemented in the calculation. For transitions involving the lower lying spectral states this implementation can be easily done via the Long Wave Length approximation. For transitions where this approximation does not apply we develop a new method of implementing the experimental energy dependencies.
description: 28 pages, 7 tables
What we can learn from children!  "Spirituality is a natural human predisposition"" Relational spirituality Hay and Nye; Spirituality as intelligence  K Adams, B Hyde "experiences can heal-D Thomas + D Scott "Children's experiences will feel normal to them."+ Spirituality as interconnected processes
Creators: name: E Peck Jr, Charles
Publisher: name: Knowledge Commons
Year: 2025
Subjects: subject: Spirituality in art
subject: Spirituality--Social aspects
subject: Spirituality--Health aspects
subject: Spirituality--Psychology
subject: Spirituality in literature
subject: British Association for Early Childhood Education
subject: National Academy of Early Childhood Programs (U.S.)
subject: Dougy Center for Grieving Children

description: Preface: Edna's story of her struggle with the death of her father: "I began to understand then, that everything I needed to overcome the turmoil that I was experiencing, was within myself … Spirituality became a part of my life, and was repeatedly looked upon for understanding in other situations. My spirituality is a part of my very existence that is made up of hopes, mysteries, and values. It is shown in my interactions with others, and in my writing … It is the light of being that gives meaning and understanding to everything and everyone that I encounter. I give thanks to the spirituality within me."
You wouldn't ordinarily think a 12-year-old could write something as sophisticated and profound as that – but this was written by "Edna (12), struggling with the death of her father," One small study revealed that 68 out of 125 people who are grieving – not surprisingly – engage spirituality
Spirituality is a natural human predisposition. It is more primal than institutional religion and concerns a person's sense of connectedness with self, others, and the world (or cosmos). Kate Adams Bishop Grosseteste University College Lincoln & Brendan Hyde Australian Catholic University
Setting the stage: The Neuroscience Map-Model of Morals = a Model of intricate complex interrelationships Funk and Gazzanigna observe that: "Morality is a set of complex emotional and cognitive processes that is reflected across many brain domains. Some of them are recurrently found to be indispensable in order to emit a moral judgment, but none of them is uniquely related to morality……Some of the emotions processed are more central to morality than others, but all emotions contribute to moral judgment given specific contextual situations…..The neural circuits of brain regions implicated in morality overlap with those that regulate other behavioral processes, suggesting that there is probably no undiscovered neural substrate that uniquely supports moral cognition."  Brain Architecture of human morality, Funk and Gazzanigna) The model presented by the neuroscience of music is a similar model – of overlapping and intricately connected processes. There is no reason to think spiritual processes would be any different. For instance, a close analysis of Jean MacPhail's experience reveals a synthesis process involved in setting things in order – and "putting her house in order" in dealing with her mother's death as a young girl.
Chandra X-ray Observations of the Quadruply Lensed Quasar RX J0911.4+0551
Creators: name: Morgan, Nicholas D.
name: Chartas, George
name: Malm, Michael
name: Bautz, Mark W.
name: Burud, Ingunn
name: Hjorth, Jens
name: Jones, Stephen
name: Schechter, Paul L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from X-ray observations of the quadruply lensed quasar RX J0911.4+0551 using data obtained with the Advanced CCD Imaging Spectrometer (ACIS) on board the Chandra X-ray Observatory. The 29 ks observation detects a total of ~404 X-ray photons (0.3 to 7.0 keV) from the four images of the lensed quasar. Deconvolution of the aspect corrected data resolves all four lensed images, with relative positions in good agreement with optical measurements. When compared to contemporaneous optical data, one of the lensed images (component A3) is dimmer by a factor of ~6 in X-rays with respect to the 2 brighter images (components A1 and A2). Spectral fitting for the combined images shows significant intrinsic absorption in the soft (0.2 to 2.4 keV) energy band, consistent with the mini-BAL nature of this quasar, while a comparison with ROSAT PSPC observations from 1990 shows a drop of ~6.5 in the total soft bandpass flux. The observations also detect ~157 X-ray photons arising from extended emission of the nearby cluster (peaked ~42" SW of RXJ0911.4+0551) responsible for the large external shear present in the system. The Chandra observation reveals the cluster emission to be complex and non-spherical, and yields a cluster temperature of kT = 2.3^{+1.8}_{-0.8} keV and a 2.0 to 10 keV cluster luminosity within a 1 Mpc radius of L_X = 7.6_{-0.2}^{+0.6} x 10^{43} ergs/s (error bars denote 90% confidence limits). Our mass estimate of the cluster within its virial radius is 2.3^{+1.8}_{-0.7} x 10^{14} solar, and is a factor of 2 smaller than, although consistent with, previous mass estimates based on the observed cluster velocity dispersion.
description: 16 pages, 3 figures (figure 1 is color ps). Accepted by ApJ
Kaon form factor in holographic QCD
Creators: name: Abidin, Zainul
name: Hutauruk, Parada T. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The kaon form factor in the spacelike region is calculated using a holographic QCD model with the "bottom-up" approach. We found that our result for the kaon form factor in low $Q^2$ has a remarkable agreement with the existing data, where $Q^2$ is the four-momentum transfer squared. The charge radius of the kaon, as well as the kaon decay constant, are found to be in a good agreement with the experiment data. We then predict the kaon form factor in the asymptotic region (larger $Q^2$) showing $1/Q^2$ behavior, which is consistent with the perturbative QCD prediction.
description: 8 pages, 3 figures, to appear in Phys. Rev. D
The formation of stars in groups
Creators: name: Williams, Jonathan
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations of the dust and gas around embedded stellar clusters reveal some of the processes involved in their formation and evolution. Large scale mass infall with rates dM/dt=4e-4 solar masses/year is found to be disrupted on small scales by protostellar outflows. Observations of the size and velocity dispersion of clusters suggest that protostellar migration from their birthplace begins at very early times and is a potentially useful evolutionary indicator.
description: 8 page conference proceedings for "The Earliest Phases of Massive Star Birth" (Third Boulder Hot Star Workshop), ed. P. Crowther
Το 17ο Παγκόσμιο Συνέδριο Φιλοσοφίας: Φιλοσοφία και Πολιτισμός
Creators: name: Μπαρτζελιώτης, Λεωνίδας Κ.
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 1 (1984)
Anapus freyi
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Anapus
Anapus freyi

description: Anapus freyi (Fieber, 1864)
 Material examined. ARDABIL: Khemes, 1 specimen, 7.-9.vii.2002.
 Comments. In meadows in hills. Eastern Palaearctic, extending from Ukraine and southern European Russia to Siberia. New for Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 34, DOI: 10.5281/zenodo.5328235
Β' Πανελλήνιο Συνέδριο Φιλοσοφίας: Η φιλοσοφία σήμερα
Creators: name: Ζαχαρίου, Ανδρέας
name: Μούκανος, Δημήτριος
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 1 (1984)
Additional file 1: of Intratumor heterogeneity comparison among different subtypes of non-small-cell lung cancer through multi-region tissue and matched ctDNA sequencing
Creators: name: Zhang, Yaxiong
name: Chang, Lianpeng
name: Yang, Yunpeng
name: Fang, Wenfeng
name: Guan, Yanfang
name: Wu, Aiwei
name: Hong, Shaodong
name: Zhou, Huaqiang
name: Chen, Gang
name: Chen, Xi
name: Zhao, Shen
name: Zheng, Qiufan
name: Pan, Hui
name: Zhang, Lanjun
name: Long, Hao
name: Yang, Haoxian
name: Wang, Xin
name: Wen, Zhesheng
name: Wang, Junye
name: Yang, Hong
name: Xia, Xuefeng
name: Zhao, Yuanyuan
name: Hou, Xue
name: Ma, Yuxiang
name: Zhou, Ting
name: Zhang, Zhonghan
name: Zhan, Jianhua
name: Huang, Yan
name: Zhao, Hongyun
name: Zhou, Ningning
name: Yi, Xin
name: Zhang, Li
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Table S1. List of target regions of the pan-cancer 1021-gene panel. (DOCX 37 kb)
Unusual Broad Absorption Line Quasars from the Sloan Digital Sky Survey
Creators: name: Hall, Patrick B.
name: Anderson, S. F.
name: Strauss, M. A.
name: York, D. G.
name: Richards, G. T.
name: Fan, X.
name: Knapp, G. R.
name: Schneider, D. P.
name: Berk, D. E. Vanden
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Sloan Digital Sky Survey has confirmed the existence of populations of broad absorption line (BAL) quasars with various unusual properties. We present and discuss twenty-three such objects and consider the implications of their wide range of properties for models of BAL outflows and quasars in general. We have discovered one BAL quasar with a record number of absorption lines. Two other similarly complex objects with many narrow troughs show broad MgII absorption extending longward of their systemic host galaxy redshifts. This can be explained as absorption of an extended continuum source by the rotation-dominated base of a disk wind. Five other objects have absorption which removes an unprecedented ~90% of all flux shortward of MgII. The absorption in one of them has varied across the ultraviolet with an amplitude and rate of change as great as ever seen. This same object may also show broad H-beta absorption. Numerous reddened BAL quasars have been found, including at least one reddened mini-BAL quasar with very strong FeII emission. The five reddest objects have continuum reddenings of E(B-V)~0.5, and in two of them we find strong evidence that the reddening curve is even steeper than that of the SMC. We have found at least one object with absorption from FeIII but not FeII. This may be due to a high column density of moderately high-ionization gas, but the FeIII level populations must also be affected by some sort of resonance. Finally, we have found two luminous, probably reddened high-redshift objects which may be BAL quasars whose troughs partially cover different regions of the continuum source as a function of velocity.
description: ApJS in press. 50 pages, 27 bitmapped figures. Full resolution paper available at http://archive.stsci.edu/sdss/prepared_ds.html or http://astro.princeton.edu/~pathall/ftp/sb1-aas.ps.gz; full-resolution figures alone at http://astro.princeton.edu/~pathall/ftp/sb1-figs.ps.gz A non-technical writeup on some of these objects is available at http://www.starstuff.org/cgi-bin/authorsearch.idq?author=Pat+Hall
Adventure Sport Tourism in Wales: Assessing the role, impact and development of Welsh language use
Creators: name: Bear, Olivia
name: Hardman, Alun
name: St Leger, Lana
name: Jennings, George
Publisher: name: Cardiff Metropolitan University
Year: 2024
Subjects: classificationCode: 440406
subject: Rural community development
classificationCode: 350804
subject: Tourism marketing
classificationCode: 470208
subject: Culture, representation and identity

description: The value of AST for revitalising rural economies has been widely recognised (Costa and Chalip, 2005). Beyond economic worth, AST provision has long been associated with individual wellness and lifestyle, the educational development of children and adolescents, and a mechanism for teambuilding and co-operation for employers (Finch & Legg, 2019). The aim of this PhD research is to identify and evaluate how Welsh language is currently used within the sphere of Adventure Sport Tourism (AST) and will explore the potential social, cultural, and professional contribution that the language can make in this field. This paper presents the review of literature focused on a current key challenge in Wales, undertaken to develop the research design to explore this further.
Α' Διεθνές Συνέδριο για τον Δημόκριτο
Creators: name: Πόταγα, Άννα
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 1 (1984)
Neutrino Heating in an Inhomogeneous Big Bang Nucleosynthesis Model
Creators: name: Lara, J. F.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The effect of the heating of neutrinos by scattering with electrons and positrons and by e-e+ annihilation on nucleosynthesis is calculated for a spherically symmetric baryon inhomogeneous model of the universe. The model has a high baryon density core and a low density outer region. The heating effect is calculated by solving the Boltzmann Transport Equation for the distribution functions of electron and muon/tau neutrinos. For a range of baryon-to-photon ratio = [ 0, 1.5 ] x 10^-10 and distance scale = [ 10^2, 10^8 ] cm the heating effect increases the mass fraction of He4 by a range of [1, 2] x 10^-4. The change of the value of the mass fraction of He4 appears similiar to the change caused by an upward shift in the value of the baryon-to-photon ratio. But the change to deuterium is a decrease in abundance ratio Y(d)/Y(p) on the order of 10^-3, one order less than the decrease due to a shift in baryon-to-photon ratio.
description: 6 Pages, LaTeX, 6 Postscript Figures, to appear in "The 20th Texas Symposium on Relativistic Astrophysics", (Austin, TX, December 11-15, 2000), ed. J. Craig Wheeler and Hugo Martel
Additional file 1 of Sulfur-Doped Alkylated Graphene Oxide as High-Performance Lubricant Additive
Creators: name: Ma, Jun
name: Xiao, Yunpeng
name: Sun, Yuanbao
name: Hu, Jianqiang
name: Wang, Yuelun
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 1: Figure S1. The relationship between the average friction coefficient and the concentration of AS-GO modified by butylamine, octylamine, laurylamine, and octadecylamine in PAO (a) and 928 (b) oils. Figure S2. The maximum nonseizure load (PB) value while SA-GO (prepared by sulfur-doped GO and butylamine (a), laurylamine (b), and octadecylamine (c), the oxidation time of the GO is 24 hours) is applied as lubrication additive with certain concentration in PAO4 base oil. Figure S3. The maximum nonseizure load (PB) value while SA-GO (prepared by sulfur doped GO and butylamine (a), laurylamine (b), and octadecylamine (c), the oxidation time of the GO is 24 hours) is applied as lubrication additive with certain concentration in 928 lubrication oil. Figure S4. The surface morphology and EDS spectrum of steel ball that pure 928 aviation lubrication oil is applied as lubricant
Ο Καρλ Μαρξ και η φιλοσοφία
Creators: name: Λάζου-Βούτου, Άννα
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 1 (1984)
Euryopicoris nitidus
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Euryopicoris
Euryopicoris nitidus

description: Euryopicoris nitidus (Meyer-Dür, 1843)
 Material examined. ARDABIL: 20-30 km E of Khalkhal, 1 specimen, 21.vii.1996.
 Comments. On grasses in mountain meadows. Palaearctic. New for Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 34, DOI: 10.5281/zenodo.5328235
Eragrostis racemosa Steud., Syn. Pl. Glumac.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Eragrostis
Eragrostis racemosa

description: Eragrostis racemosa (Thunb.) Steud., Syn. Pl. Glumac. 1: 271 (1854).
 Distribution: Eritrea to S. Africa, Seychelles, Madagascar
 Specimens: MOSHI Holili, Hemp, A. 2891 (NHT, UBT); Kilema, Hemp, A. 2112 (NHT, UBT); Kirua, Hemp, A. 1699 (NHT, UBT); Lerang’wa, Grimshaw, J.M. 931271 (K); Mwika, Hemp, A. 2051 (NHT, UBT); s. loc., Schlieben, H.J. 4995 (NH).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 226, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816