cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MOESM1 of Integrative analysis of the cancer genome atlas and cancer cell lines encyclopedia large-scale genomic databases: MUC4/MUC16/MUC20 signature is associated with poor survival in human carcinomas
Creators: name: Jonckheere, Nicolas
name: Seuningen, Isabelle Van
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Figure S1. MUC4 Oncoprint in Cancer Cell Line Encyclopedia. MUC4 alterations were explored in Cancer Cell Line Encyclopedia dataset using cBioPortal webtool. The oncoprint represents the amplification, deletion, up regulation or in frame mutation.
The Effects of Starbursts and Low-Surface-Brightness Galaxies on Faint Galaxy Models
Creators: name: McLeod, B. A.
name: Rieke, M. J.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present models predicting the magnitude, redshift, and color distributions of field galaxies. We explore whether a fading starburst scenario can account for the observations of faint blue galaxies. We marginally rule out a starburst scenario with a local IMF because the models predict too many nearby faint galaxies that are not observed. A burst model with a truncated IMF reproduces the counts and redshift distributions well but produces too blue a population. We show that surface brightness selection has a significant effect on the distributions. In particular, adding a population of low-surface brightness galaxies, known to exist locally, can explain the counts for $B_J<23$. They do not, however, account for the steepness of the counts at fainter magnitudes. Finally we show that the colors of galaxies in a $K$-band selected sample are too blue to be consistent with a constant star-formation rate, passive-evolution model.
description: uuencoded compressed tar file, AAS LaTeXv3.0 includes 14 EPS figures (32 pages), separate Latex file for tables (4 pages), to appear in ApJ
MOESM1 of Stacking of a low-lignin trait with an increased guaiacyl and 5-hydroxyguaiacyl unit trait leads to additive and synergistic effects on saccharification efficiency in Arabidopsis thaliana
Creators: name: Vries, Lisanne De
name: Vanholme, Ruben
name: Acker, Rebecca Van
name: Meester, Barbara De
name: Sundin, Lisa
name: Boerjan, Wout
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Additional file 1. Graphs of the cellulose-to-glucose conversions over time. Cellulose-to-glucose conversions of the tra2 comt-1, c4h-3 comt-4, and 4cl1-1 comt-4 double mutants, wild type, and the corresponding parental lines, without, with acid and with alkaline pretreatment at the different timepoints. A) Cellulose-to-glucose conversion for tra2 comt-1 and its respective control lines. B) Cellulose-to-glucose conversion for c4h-3 comt-4 and its respective control lines. C) Cellulose-to-glucose conversion for 4cl1-1 comt-4 and its respective control lines. The conversions were calculated based on the saccharification efficiency and cellulose content (both on CWR basis) and are expressed as % cellulose converted to glucose. Measurements were done 6, 24, 48, and 72 and eventually 96 h after the saccharification enzymes were added to the samples. The error bars represent standard deviations (n = 10). The exact values and significances are presented in Additional file 2. The relative increases in saccharification efficiency compared to wild type are presented in Additional file 3.
New constraints on Galactic cosmic-ray propagation
Creators: name: Strong, A. W.
name: Moskalenko, I. V.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An extensive program for the calculation of galactic cosmic-ray propagation has been developed. Primary and secondary nucleons, primary and secondary electrons, secondary positrons and antiprotons are included. Fragmentation and energy losses are computed using realistic distributions for the interstellar gas and radiation fields. Models with diffusion and convection only do not account naturally for the observed energy dependence of B/C, while models with reacceleration reproduce this easily. The height of the halo propagation region is determined, using recent 10Be/9Be measurements, as greater than 4 kpc. The radial distribution of cosmic-ray sources required is broader than current estimates of the SNR distribution for all halo sizes. Our results include an estimate of cosmic-ray antiproton and positron spectra, and the Galactic diffuse gamma-ray emission (see accompanying paper: Moskalenko 1998b).
description: 4 pages including 6 ps-figures, latex2e, uses epsfig.sty, times.sty. To appear in: Proc. of 16th European Cosmic Ray Symposium (July 1998, Alcala), OG-2.5. More details can be found at http://www.gamma.mpe-garching.mpg.de/~aws/aws.html Some references are added
RR LYRAE VARIABLE STARS: PULSATIONAL CONSTRAINTS RELEVANT TO THE OOSTERHOFF CONTROVERSY
Creators: name: Bono, G.
name: Caputo, F.
name: Castellani, V.
name: Marconi, M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A solution to the old Oosterhoff controversy is proposed on the basis of a new theoretical pulsational scenario concerning RR Lyrae cluster variables (Bono and coworkers). We show that the observed constancy of the lowest pulsation period in both Oosterhoff type I (OoI) and Oosterhoff type II (OoII) prototypes (M3, M15) can be easily reproduced only by assuming the canonical evolutionary horizontal-branch luminosity levels of these Galactic globular clusters and therefore by rejecting the Sandage period shift effect (SPSE).
description: postscript file of 7 pages and 2 figures; one non postcript figure is available upon request; for any problem please write to marcella@astr1pi.difi.unipi.it
Coexistence of valence-bond formation and topological order in the Frustrated Ferromagnetic $J_1$-$J_2$ Chain
Creators: name: Agrapidis, Cliò Efthimia
name: Drechsler, Stefan-Ludwig
name: Brink, Jeroen van den
name: Nishimoto, Satoshi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Frustrated one-dimensional (1D) magnets are known as ideal playgrounds for new exotic quantum phenomena to emerge. We consider an elementary frustrated 1D system: the spin-$\frac{1}{2}$ ferromagnetic ($J_1$) Heisenberg chain with next-nearest-neighbor antiferromagnetic ($J_2$) interactions. On the basis of density-matrix renormalization group calculations we show the existence of a finite spin gap at $J_2/|J_1|>1/4$ and we find the ground state in this region to be a valence bond solid (VBS) with spin-singlet dimerization between third-neighbor sites. The VBS is the consequence of spontaneous symmetry breaking through order by disorder. Quite interestingly, this VBS state has a Affleck-Kennedy-Lieb-Tasaki-type topological order. This is the first example of a frustrated spin chain in which quantum fluctuations induce gapped topological order.
description: 16 pages, 9 Figures, Submission to SciPost
Tests of Spurious Transport in Smoothed Particle Hydrodynamics
Creators: name: Lombardi, James C.
name: Sills, Alison
name: Rasio, Frederic A.
name: Shapiro, Stuart L.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have performed a series of systematic tests to evaluate the effects of spurious transport in three-dimensional smoothed particle hydrodynamics (SPH) calculations. Our tests investigate (i) particle diffusion, (ii) shock heating, (iii) numerical viscosity, and (iv) angular momentum transport. The results are useful for quantifying the accuracy of the SPH scheme, especially for problems where shear flows or shocks are present, as well as for problems where true hydrodynamic mixing is relevant. We examine the different forms of artificial viscosity (AV) which have been proposed by Monaghan, by Hernquist & Katz, and by Balsara. For each form, our tests suggest a single set of values for the AV parameters $α$ and $β$ (coefficients of the linear and quadratic terms) which are appropriate in a large number of situations. We also discuss how these parameters should be adjusted depending on the goals of the particular application. We find that both the Hernquist & Katz and Balsara forms introduce relatively small amounts of numerical viscosity. Furthermore, both Monaghan's and Balsara's AV do well at treating shocks and at limiting the amount of spurious mixing. For these reasons, we endorse the Balsara AV for use in a broad range of applications.
description: 49 pages, 26 figures as 30 postscript files, submitted to The Journal of Computational Physics
KMT-2016-BLG-1820 and KMT-2016-BLG-2142: Two Microlensing Binaries Composed of Planetary-mass Companions and Very-Low-Mass Primaries
Creators: name: Jung, Youn Kil
name: Hwang, Kyu-Ha
name: Ryu, Yoon-Hyun
name: Gould, Andrew
name: Han, Cheongho
name: Yee, Jennifer C.
name: Albrow, Michael D.
name: Chung, Sun-Ju
name: Shin, In-Gu
name: Shvartzvald, Yossi
name: Zang, Weicheng
name: Cha, Sang-Mok
name: Kim, Dong-Jin
name: Kim, Hyoun-Woo
name: Kim, Seung-Lee
name: Lee, Chung-Uk
name: Lee, Dong-Joo
name: Lee, Yongseok
name: Park, Byeong-Gon
name: Pogge, Richard W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the analyses of two short-timescale $(t_{\rm E} \sim 5~{\rm days})$ microlensing events, KMT-2016-BLG-1820 and KMT-2016-BLG-2142. In both light curves, the brief anomalies were clearly captured and densely covered by the Korea Microlensing Telescope Network survey. From these analyses, we find that both events have small Einstein radii of $θ_{\rm E} = 0.12~{\rm mas}$, suggesting that the binary-lens systems are composed of very low-mass components and/or are located much closer to the lensed stars than to Earth. From Bayesian analyses, we find that these binaries have total system masses of $0.043_{-0.018}^{+0.043}~M_{\odot}$ and $0.088_{-0.041}^{+0.120}~M_{\odot}$, implying that they are well within the very-low-mass regime. The estimated lens-component masses indicate that the binary lenses consist of a giant-planet/brown-dwarf pair (KMT-2016-BLG-1820), and a dark/faint object pair (KMT-2016-BLG-2140) that are located near the deuterium-burning and hydrogen-burning mass limits, respectively. Both lens systems are likely to be in the Galactic disk with estimated distances of about $6$ kpc and $7$ kpc. The projected lens-components separations are $1.1$ AU and $0.8$ AU, and the mass ratios are $0.11$ and $0.20$. These prove that the microlensing method is effective to identify these closely-separated very-low-mass binaries having low mass-ratios.
description: 20 pages, 7 figures, 3 tables. Accepted for publication in AJ
Lemur tardigradus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Lemuridae
Lemur
Lemur tardigradus

description: Lemur tardigradus [spec. nov.]
L. ecaudatus. Mus. Ad. Fr. 1. p. 3.
Simia ecaudata, unguibus indicis subulatis. Syst. nat. 5. n. 2.
Species Simiarum inter Mammalia plurimae, sed paucissimae rite descriptae & cognitae, plurimae obscurae ignorantur.
Simiae suspectae, memores, petulantes, imitatores, gesticulatores, indociles, minantur, rident, cibos bucca macerant, pediculos venantur, tactu excellunt, natos ulnis gerunt, menstruant, terrefactae cacant immundae, urinae mea tu saepe distincto a vulva figula res.
Animal cynocephalum tardigradum. Seb. mus. 1. p. 55. t. 35. f. 1. 2. & t. 47. f. 1.
Animal elegantissimum robinsoni. Raj. quadr. 161.
Habitat in Zeylona.
Statura Sciuri, subferruginea, linea dorsali subfusca; Gula albidiore. Linea longitudinalis oculis interjecta alba. Facies tecta. Auriculae urceolatae, intus bifoliatae. Pedum palmae plantaeque nudae. Ungues rotundati: indicum plantarum vero subulati. Cauda fere nulla. Mammae 2 in pectore; 2 in abdomine versus pectus.
Animal tardigradum, auditu excellens, monogamum.
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 pages 29-30, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Minimizers of the dynamical Boulatov model
Creators: name: Geloun, Joseph Ben
name: Kegeles, Alexander
name: Pithis, Andreas G. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We study the Euler-Lagrange equation of the dynamical Boulatov model which is a simplicial model for 3d Euclidean quantum gravity augmented by a Laplace-Beltrami operator. We provide all its solutions on the space of left and right invariant functions that render the interaction of the model an equilateral tetrahedron. Surprisingly, for a non-linear equation of motion, the solution space forms a vector space. This space distinguishes three classes of solutions: saddle points, global and local minima of the action. Our analysis shows that there exists one parameter region of coupling constants for which the action admits degenerate global minima.
description: closest to published version
Distributed State Estimation Using Intermittently Connected Robot Networks
Creators: name: Khodayi-mehr, Reza
name: Kantaros, Yiannis
name: Zavlanos, Michael M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Robotics (cs.RO)
subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: This paper considers the problem of distributed state estimation using multi-robot systems. The robots have limited communication capabilities and, therefore, communicate their measurements intermittently only when they are physically close to each other. To decrease the distance that the robots need to travel only to communicate, we divide them into small teams that can communicate at different locations to share information and update their beliefs. Then, we propose a new distributed scheme that combines (i) communication schedules that ensure that the network is intermittently connected, and (ii) sampling-based motion planning for the robots in every team with the objective to collect optimal measurements and decide a location for those robots to communicate. To the best of our knowledge, this is the first distributed state estimation framework that relaxes all network connectivity assumptions, and controls intermittent communication events so that the estimation uncertainty is minimized. We present simulation results that demonstrate significant improvement in estimation accuracy compared to methods that maintain an end-to-end connected network for all time.
Supersonic Turbulence and the Fragmentation of a Cold Medium
Creators: name: Padoan, Paolo
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The role played by velocity fields in the fragmentation of a cold medium and in the formation of protostars is studied. The velocity field is modeled with a compressible turbulent flow. A supersonic turbulent velocity field can fragment the medium into clumps of mass smaller than a local Jeans' mass, and therefore stabilize the medium against the formation of protostars. Based on this idea, the protostar formation efficiency and the protostar mass distribution are determined as functions of the following ambient parameters: average density $n_{0}$, average temperature $T_{0}$, r.m.s. turbulent velocity $σ_{v,0}$ (or its Mach number ${\cal{M}}_{t}$), postshock cooling time (e.g. chemistry). The main results are: i) the protostar mass distribution and its dependence on the ambient parameters are quantified; ii) the characteristic protostar mass is $M_{J,cl}\propto n_{0}^{-1/2}T_{0}^{2} σ_{v,0}^{-1}$; iii) the protostar formation efficiency $e$ is higher for larger mean density, larger mean temperature, lower velocity dispersion on a given scale and longer postshock cooling time (e.g. lower metallicity): $e\propto n_{0}^{{3/2}(β-1)}T_{0}^{β-1} σ_{v,0}^{-5(β-1)}L_{0}^{3(β-1)}$, where $β>1$ is the exponent of the clump mass distribution; iv) the efficiency is quite sensitive to the ambient parameters and therefore to the dynamical evolution of the star forming system.
description: 12 pages. Figures are included. Uuencoded compressed postscript. Accepted for publication by MNRAS
Equations of Motion for the Standard Model Effective Field Theory: Theory and Applications
Creators: name: Barzinji, Abdurrahman
name: Trott, Michael
name: Vasudevan, Anagha
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The equations of motion for the Standard Model Effective Field Theory (SMEFT) differ from those in the Standard Model. Corrections due to local contact operators modify the equations of motion and impact matching results at sub-leading order in the operator expansion. As a consequence, a matching coefficient in $\mathcal{L}^{(n)}$ (for operators of dimension $n$) can be dependent on the basis choice for $\mathcal{L}^{(m
description: 5pp + appendix, 2 figures. V2: Updated to PRD version
Additional file 2: of Regional expiratory time constants in severe respiratory failure estimated by electrical impedance tomography: a feasibility study
Creators: name: Karagiannidis, Christian
name: Waldmann, Andreas
name: Róka, Péter
name: Schreiber, Tina
name: Strassmann, Stephan
name: Windisch, Wolfram
name: Böhm, Stephan
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: Figure S1. Coefficient of variation in EIT-derived τ calculations in 14 patients. (PDF 1276 kb)
Galactic Extinction from Colors and Counts of Field Galaxies in WFPC2 Frames: An Application to GRB 970228
Creators: name: Gonzalez, Rosa A.
name: Fruchter, Andrew S.
name: Dirsch, Boris
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We develop the ``simulated extinction method'' to measure average foreground Galactic extinction from field galaxy number-counts and colors. The method comprises simulating extinction in suitable reference fields by changing the isophotal detection limit. This procedure takes into account selection effects, in particular, the change in isophotal detection limit (and hence in isophotal magnitude completeness limit) with extinction, and the galaxy color--magnitude relation. We present a first application of the method to the HST WFPC2 images of the gamma-ray burster GRB 970228. Four different WFPC2 high-latitude fields, including the HDF, are used as reference to measure the average extinction towards the GRB in the F606W passband. From the counts, we derive an average extinction of A_V = 0.5 mag, but the dispersion of 0.4 mag between the estimates from the different reference fields is significantly larger than can be accounted by Poisson plus clustering uncertainties. Although the counts differ, the average colors of the field galaxies agree well. The extinction implied by the average color difference between the GRB field and the reference galaxies is A_V = 0.6 mag, with a dispersion in the estimated extinction from the four reference fields of only 0.1 mag. All our estimates are in good agreement with the value of 0.81\pm0.27 mag obtained by Burstein & Heiles, and with the extinction of 0.78\pm0.12 measured by Schlegel et al. from maps of dust IR emission. However, the discrepancy between the widely varying counts and the very stable colors in these high-latitude fields is worth investigating.
description: 14 pages, 2 figures; submitted to the Astrophysical Journal
ON THE QUALITATIVE PROPERTIES OF FUTURES MARKET EQUILIBRIUM
Creators: name: Magill, Michael
name: Nermuth, Manfred
name: Magill, Michael
name: Nermuth, Manfred
Publisher: name: Unknown
Year: 1985
Subjects: Research Methods/ Statistical Methods

description: This paper studies the qualitative properties of a model of futures market equilibrium. We characterise the bias (backwardation or contango) in the futures price, the extent to which output is hedged by producers and the output that is produced relative to the case where there is no uncertainty. We show that only three cases can arise and give precise conditions under which these three cases arise when the number of speculators is very large. The conditions involve the nature of the stochastic dependence between the spot price and the random returns that speculators earn on markets in the rest of the economy. *Department of Economics, University of Southern California, Los Angeles, California, 90089-0152, U.S.A. Support from the National Science Foundation (SES 8200432) is gratefully acknowledged. tInstitut fUr Wirtschaftswissenschaften, University of Vienna, Liechtensteinstrasse 13/11, A-1090 Vienna, Austria
The epoch of structure formation in blue mixed dark matter models
Creators: name: Borgani, Stefano
name: Lucchin, Francesco
name: Matarrese, Sabino
name: Moscardini, Lauro
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent data on the high--redshift abundance of damped Ly$α$ systems are compared with theoretical predictions for `blue' (i.e. $n>1$) Mixed Dark Matter models. The results show that decreasing the hot component fraction $Ω_ν$ and/or increasing the primordial spectral index $n$ implies an earlier epoch of cosmic structure formation. However, we also show that varying $Ω_ν$ and $n$ in these directions makes the models barely consistent with the observed abundance of galaxy clusters. Therefore, requiring at the same time observational constraints on damped Ly$α$ systems and cluster abundance to be satisfied represents a challenge for the Mixed Dark Matter class of models.
description: Uuencoded compressed tar file containing 6 page TeX file and 4 postscript figures. Uses mn.sty and psfig.sty. To appear in MNRAS. Main change: inclusion of a discussion of the constraints coming from the cluster abundances
Lemur catta Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Lemuridae
Lemur
Lemur catta

description: Lemur catta [spec. nov.]
L. cauda annulata.
Simia-Sciurus madagascariensis, sive Maucauco. Edv. av. 199. t. 199.
Habitat in Madagascar.
Statura Felis, subcinerea. Oculorum regiones nigrae. Caput acuminatum. Aures tectae. Cauda longa, picta annulis atris cinereisque. Ungues subulati: pollicibus plantarum rotundiores; scandit ut Simia, sed tardiuscule. Habitu accedit ad Genettam auctorum.
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 30, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Dynamic time-of-use electricity pricing for residential demand response: design and analysis of the Low Carbon London smart-metering trial
Creators: name: Schofield, James
Publisher: name: Imperial College London
Year: 2015

description: This thesis describes the trial design and analysis of the Low Carbon London (LCL) residential dynamic Time-of-Use (dToU) trial. This trial investigated the potential for dToU tariffs to deliver residential demand response to the Supplier, where it may contribute to system balancing through Supply Following (SF) actions, and to the distribution network operator (DNO), where it may be used for network Constraint Management (CM). 5,533 households from the London area participated in the trial and their consumption was measured at 30 minute resolution. 1,119 of these received the dToU tariff, which subjected them to CM and SF price events that were designed according to the specific requirements of these respective use cases. A novel, data driven, engagement ranking index was developed that allowed stratification of subsequent results into sets of the most engaged consumers, who may be indicative of a future populace that is more experienced/engaged in home energy management. Demand response (DR) was calculated relative to baseline model that used the dToU group mean demand as an input, with aggregate response levels calculated over a range of time, socio-economic and household occupancy related variables. Taking a network perspective, the reliability of CM event response was examined and two simple linear models presented as candidate predictors of response level, which was found to be consistent with an 8% reduction in demand. The network capacity contribution of residential DR was theorised to consist of two components: “mean response” and “variance response”, and the real impact of these was investigated using the LCL gathered data. Potential risks to the network from low price induced demand spikes were explored empirically using the SF event data and the times of highest risk were identified. The extensive metadata set gathered from trial participants was processed into some 200 numerical variables. A correlation analysis was performed which was visualised using weighted correlation network graphs. A number of parameters were found to predict response level, but responsiveness (the level of deliberate engagement) could only be reliably measured by engagement rank.
Encoding Electronic Spectra in Quantum Circuits with Linear T Complexity
Creators: name: Babbush, Ryan
name: Gidney, Craig
name: Berry, Dominic W.
name: Wiebe, Nathan
name: McClean, Jarrod
name: Paler, Alexandru
name: Fowler, Austin
name: Neven, Hartmut
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We construct quantum circuits which exactly encode the spectra of correlated electron models up to errors from rotation synthesis. By invoking these circuits as oracles within the recently introduced "qubitization" framework, one can use quantum phase estimation to sample states in the Hamiltonian eigenbasis with optimal query complexity $O(λ/ ε)$ where $λ$ is an absolute sum of Hamiltonian coefficients and $ε$ is target precision. For both the Hubbard model and electronic structure Hamiltonian in a second quantized basis diagonalizing the Coulomb operator, our circuits have T gate complexity $O({N + \log (1/ε}))$ where $N$ is number of orbitals in the basis. This enables sampling in the eigenbasis of electronic structure Hamiltonians with T complexity $O(N^3 /ε+ N^2 \log(1/ε)/ε)$. Compared to prior approaches, our algorithms are asymptotically more efficient in gate complexity and require fewer T gates near the classically intractable regime. Compiling to surface code fault-tolerant gates and assuming per gate error rates of one part in a thousand reveals that one can error correct phase estimation on interesting instances of these problems beyond the current capabilities of classical methods using only about a million superconducting qubits in a matter of hours.
description: 39 pages, 25 figures, 9 tables; fixed minor errors from v1
Lemur volans Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Primates
Lemuridae
Lemur
Lemur volans

description: Lemur volans [spec. nov.]
L. caudatus, membran� ambiente volitans. �
Cato-Simius volans camelli. Pet. gaz. 14. t. 9. f. 8. Act. angl. 277. n. 1065.
Vespertilio admirabilis. Bont. jav. 68. t. 69.
Felis volans ternatea. Seb. mus. 1. p. 93. t. 58. f. 2. 3.
Habitat in Asia.
Membrana more Sciuri volantis s. Muris volantis a capite ad manus, a manibus per latera ad plantas, a plantis ad apicem caudae expansa. Ungues acuti. Mammae duae pectorales. Edit fructus arborum. Ex mammis videtur Lemuribus s. Simiis proximum Animalculum, sed nobis non visum; ulterius examinent autoptae.
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 30, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The Universal Rotation Curve of Spiral Galaxies: I. the Dark Matter Connection
Creators: name: Persic, M.
name: Salucci, P.
name: Stel, F.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a homogeneous sample of about 1100 rotation curves (RCs) and relative surface photometry to investigate (out to 2 optical radii and over 6 mag) the main mass structure properties of spirals. We confirm the strong dependence on luminosity for both the profile and the amplitude of RCs. Spiral RCs show the striking feature that a single parameter, the luminosity, dictates the rotation velocity at any radius for all objects, so revealing the existence of a universal RC. At high luminosity, there is a slight discrepancy between the profiles of RCs and those predicted from the luminous matter (LM) distributions: this implies a small, yet detectable, amount of dark matter (DM). At low luminosities the failure of the LM prediction is most severe, and DM is the only relevant mass component. Some of the derived scaling properties between dark and luminous galactic structure parameters are: (a) the DM/LM mass ratio at the optical radius scales inversely with luminosity; (b) the halo core radius is comparable to the optical radius, but shrinks for lower luminosities; (c) the central halo density scales as L^{-0.7}; (d) the halo virial mass scales as L^{0.5}. Such scaling properties can be represented as a curve in the luminosity-(DM/LM ratio)-(DM core radius)-(central DM density) space, which acts as the spirals' counterpart to the FP of ellipticals.
description: 22 pg. in MN-style LaTex (w. 16 figs. + 3 tables); replaced with the published version, in an effort to satisfy the continuing considerable offprint request rate. (A few typos corrected.)
Vespertilio Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Vespertilio

description: Vespertilio [gen. nov.]
Dentes erecti, acuti, approximati: primores 4 aequalcs.
Manus palmatae, volitantes membrana corpus cingente.
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 31, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1 of Evaluation of the college-based HIV/AIDS education policy in Beijing, China: a mixed method approach
Creators: name: Zheng, Yunting
name: Zhang, Xin
name: Sun, Xinying
name: Shi, Yuhui
name: Chang, Chun
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 1:. Policy structure ability grading. Table A1 Policy structure ability grading system.
Submillimeter Observations of the Ultraluminous BAL Quasar APM 08279+5255
Creators: name: Lewis, Geraint F.
name: Chapman, Scott C.
name: Ibata, Rodrigo A.
name: Irwin, Michael J.
name: Totten, Edward J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: With an inferred bolometric luminosity of $5\times10^{15}{\rm \lsun}$, the recently identified z=3.87, broad absorption line quasar APM 08279+5255 is apparently the most luminous object currently known. As half of its prodigious emission occurs in the infrared, APM 08279+5255 also represents the most extreme example of an Ultraluminous Infrared Galaxy. Here, we present new submillimeter observations of this phenomenal object; while indicating that a vast quantity of dust is present, these data prove to be incompatible with current models of emission mechanisms and reprocessing in ultraluminous systems. The influence of gravitational lensing upon these models is considered and we find that while the emission from the central continuum emitting region may be significantly enhanced, lensing induced magnification cannot easily reconcile the models with observations. We conclude that further modeling, including the effects of any differential magnification is required to explain the observed emission from APM 08279+5255.
description: 12 Pages with Two figures. Accepted for publication in the Astrophysical Journal Letters
DeepAffinity: Interpretable Deep Learning of Compound-Protein Affinity through Unified Recurrent and Convolutional Neural Networks
Creators: name: Karimi, Mostafa
name: Wu, Di
name: Wang, Zhangyang
name: Shen, Yang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Biomolecules (q-bio.BM)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Biological sciences
subject: FOS: Computer and information sciences

description: Motivation: Drug discovery demands rapid quantification of compound-protein interaction (CPI). However, there is a lack of methods that can predict compound-protein affinity from sequences alone with high applicability, accuracy, and interpretability. Results: We present a seamless integration of domain knowledges and learning-based approaches. Under novel representations of structurally-annotated protein sequences, a semi-supervised deep learning model that unifies recurrent and convolutional neural networks has been proposed to exploit both unlabeled and labeled data, for jointly encoding molecular representations and predicting affinities. Our representations and models outperform conventional options in achieving relative error in IC$_{50}$ within 5-fold for test cases and 20-fold for protein classes not included for training. Performances for new protein classes with few labeled data are further improved by transfer learning. Furthermore, separate and joint attention mechanisms are developed and embedded to our model to add to its interpretability, as illustrated in case studies for predicting and explaining selective drug-target interactions. Lastly, alternative representations using protein sequences or compound graphs and a unified RNN/GCNN-CNN model using graph CNN (GCNN) are also explored to reveal algorithmic challenges ahead. Availability: Data and source codes are available at https://github.com/Shen-Lab/DeepAffinity Supplementary Information: Supplementary data are available at http://shen-lab.github.io/deep-affinity-bioinf18-supp-rev.pdf
description: https://github.com/Shen-Lab/DeepAffinity
On the interpretation of clustering from the angular APM Galaxy Survey
Creators: name: Gaztañaga, Enrique
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze the uncertainties in the amplitudes of the spatial correlation functions estimated from angular correlations in a sample from the APM Galaxy Survey, with $b_J=17-20$. We model the uncertainties in the selection function and in the evolution of clustering. In particular we estimate $σ_8^{APM}$, the rms galaxy number fluctuations in spheres of radius at $8 \Mpc$, from the measured angular variance in the APM. The uncertainty in $σ_8^{APM}$ has three main contributions: 8\% from sampling and selection function uncertainties, 7\% from the uncertainty in the evolution of clustering and 3\% from the uncertainty in the value of $Ω_0$. Including all these contributions, we find $σ_8^{APM}$ is in the range $0.78-1.08$. If the galaxy clustering in the APM evolves as expected from gravitational clustering of matter fluctuations, then $σ_8^{APM}=0.95 \pm 0.07$ ($1.00 \pm 0.08$) for $Ω_0 \simeq 1$ ($Ω_0 \simeq 0$), close to the values for nearby optical samples. On the other hand, if we assume that clustering evolution is fixed in comoving coordinates $σ_8^{APM}=0.83 \pm 0.05$ ($0.87 \pm 0.06$), closer to the results for nearby IRAS samples. The final uncertainty in the range of values for the hierarchical amplitudes $S_J\equiv \xibar_J/\xibar_2^{J-1}$ is typically twice the estimated sampling errors, with the highest values for the case of less clustering evolution. We compare our estimates with other results and discuss the implications for models of structure formation.
description: 11 pages plus 12 figures, uuencoded compress postscript
Additional file 2: of Molecular and cellular characterizations of human cherubism: disease aggressiveness depends on osteoclast differentiation
Creators: name: Kadlub, Natacha
name: Sessiecq, Quentin
name: Mandavit, Marion
name: LâHermine, Aurore
name: Badoual, Cecile
name: Galmiche, Louise
name: Berdal, Ariane
name: Descroix, Vianney
name: Picard, Arnaud
name: AmĂŠlie Coudert
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology
subject: Computational Biology

description: Primary, control and secondary antibodies for manual immunohistochemistry. NFATc1 (nuclear factor of activated T cells cytoplasmic 1), RANK-L (receptor of activated nuclear factor kappa B ligand), OPG (osteoprotegerin), RANK (receptor of activated nuclear factor kappa B), IL (interleukin), TNF-R1 (Tumor necrosis factor receptor 1). (DOCX 15 kb)
The Nature of the Mid-Infrared Background Radiation in the Galactic Bulge from the IRTS Observations
Creators: name: Chan, K. W.
name: Roellig, T. L.
name: Onaka, T.
name: Yamamura, I.
name: Tanabe, T.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the Mid-Infrared Spectrometer (MIRS) on board the Infrared Telescope in Space (IRTS) we obtained the 4.5 to 11.7 micron spectra of the stellar populations and diffuse interstellar medium in the Galactic bulge (l = 8.7 degree, b = 2.9, 4.0, 4.7, and 5.7 degree). Below galactic latitudes of 4.0 degree, the mid-infrared background spectra in the bulge are similar to the spectra of M and K giants. The UIR emission bands (6.2, 7.7, 8.6, and 11.3 micron) are also detected in these regions and likely arise from the diffuse interstellar medium in the disk. Above galactic latitudes of 4.0 degree, the mid-infrared background spectra are similar to the spectra of those oxygen-rich evolved stars with high mass-loss rates detected by IRAS. One likely interpretation is that this background emission arises predominantly from those stars with very low luminosities that have not been detected by IRAS. The age for such low-luminosity evolved stars could be 15 Gyr, and the existence of a large number of evolved stars with high mass-loss rates in the bulge has a significant impact on our understanding of the stellar content in the Galactic bulge.
description: 10 pages, 3 figures, to be published in ApJ Letters
O Porto do itaqui no tribunal marítimo de 2016 a 2018
Creators: name: DAVID LUIZ SILVA FERREIRA
Publisher: name: edufma
Year: 2023

description: FERREIRA, David Luiz Silva, MATOS, Hélio Trindade de. O porto do itaqui no tribunal marítimo de 2016 a 2018. In: Tópicos estratégicos portuários. Volume III. São Luís-MA: EDUFMA, 2023.p.29-43.
MOESM10 of Integrative analysis of the cancer genome atlas and cancer cell lines encyclopedia large-scale genomic databases: MUC4/MUC16/MUC20 signature is associated with poor survival in human carcinomas
Creators: name: Jonckheere, Nicolas
name: Seuningen, Isabelle Van
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer

description: Additional file 10: Figure S7. MUC4, MUC16 and MUC20 expression in bladder, colorectal, lung, stomach, skin and ovarian cancer datasets. MUC4, MUC16 and MUC20 mRNA expression was evaluated in datasets to analyze whether the mRNA level differed between normal and tumor tissues. (A) GSE13507 contains 165 bladder cancer and 58 ANT samples. (B) GSE30219 contains 14 normal lung, 85 adenocarcinomas and 61 squamous cancer samples. (C) GSE40967 contains 566 colorectal cancers and 19 normal mucosae. (D) GSE27342 contains 80 tumors and 80 paired ANT tissues. (E) GSE4587 contains 2 normal, 2 melanomas and 2 metastatic melanomas. (F) GSE14407 contains 12 ovarian adenocarcinomas and 12 normal ovary samples. Statistical analyses were performed using paired t-test (*p<0.05, **p<0.01).
Additional file 1: of Regional expiratory time constants in severe respiratory failure estimated by electrical impedance tomography: a feasibility study
Creators: name: Karagiannidis, Christian
name: Waldmann, Andreas
name: PĂŠter RĂłka
name: Schreiber, Tina
name: Strassmann, Stephan
name: Windisch, Wolfram
name: BĂśhm, Stephan
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology

description: Figure S2. Image reconstruction and segmentation of corresponding CT scan. (PDF 6665 kb)
Physical constraints on the halo mass function
Creators: name: Porciani, C.
name: Ferrini, F.
name: Lucchin, F.
name: Matarrese, S.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyse the effect of two relevant physical constraints on the mass multiplicity function of dark matter halos in a Press--Schechter type algorithm. Considering the random--walk of linear Gaussian density fluctuations as a function of the smoothing scale, we simultaneously i) account for mass semi--positivity and ii) avoid the cloud--in--cloud problem. It is shown that the former constraint implies a severe cutoff of low--mass objects, balanced by an increase on larger mass scales. The analysis is performed both for scale--free power--spectra and for the standard cold dark matter model. Our approach shows that the well--known ``infrared" divergence of the standard Press--Schechter mass function is caused by unphysical, negative mass events which inevitably occur in a Gaussian distribution of density fluctuations.
description: Revised version (accepted for publication in MNRAS) including a new comparison with numerical results, a new appendix and new references. uuencoded gzip'ed tar archive containing many LaTex files (the main file is mass.tex). 16 pages with 6 figures (all included)
Additional file 1: of Molecular and cellular characterizations of human cherubism: disease aggressiveness depends on osteoclast differentiation
Creators: name: Kadlub, Natacha
name: Sessiecq, Quentin
name: Mandavit, Marion
name: LâHermine, Aurore
name: Badoual, Cecile
name: Galmiche, Louise
name: Berdal, Ariane
name: Descroix, Vianney
name: Picard, Arnaud
name: AmĂŠlie Coudert
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology

description: Primary antibodies used for automated immunohistochemistry. AE1-AE3 (pan cytokeratin), CD (cluster differentiation). (DOCX 14 kb)
Vespertilio vampyrus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Vespertilio
Vespertilio vampyrus

description: Vespertilio vampyrus [spec. nov.]
V. ecaudatus, naso simplici, membrana inter femora divisa.
Vespertilio cauda nulla. Syst. nat. 7.
Canis volans ternatanus orientalis. Seb. mus. 1. p. 91. t. 57. f. 1. 2.
Vespertilio ingens. Clus. exot. 94. Edv. av. 180. t. 180. f. 2. 4.
Habitat in Asia.
Noctu haurit sanguinem dormientium, cristas Gallorum & lacrymas palmarum.
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 31, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206