cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MAXIMUS: Exploiting the Full Power of OzPoz
Creators: name: Colless, Matthew
name: Taylor, Keith
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a new multi-object spectrograph for the VLT. MAXIMUS (MAXimum MUltiplex Spectrograph) will fully exploit the multiplexing capabilities of the OzPoz fibre positioner in order to extend and complement FLAMES and VIMOS in covering observational parameter space, and to meet the increasing demand for multi-object spectroscopy by ESO users in the next decade.
description: 6 pages, to appear in the proceedings of the ESO Workshop on Future VLT Instrumentation, eds J. Bergeron and G. Monnet, ESO Astrophysics Symposia (Springer)
Next Generation EPICS Interface to Abstract Data
Creators: name: Hill, J.
name: Lange, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Computer and information sciences
subject: c.2.4

description: The set of externally visible properties associated with process variables in the Experimental Physics and Industrial Control System (EPICS) is predefined in the EPICS base distribution and is therefore not extensible by plug-compatible applications. We believe that this approach, while practical for early versions of the system with a smaller user base, is now severely limiting expansion of the high-level application tool set for EPICS. To eliminate existing barriers, we propose a new C++ based interface to abstract containerized data. This paper describes the new interface, its application to message passing in distributed systems, its application to direct communication between tightly coupled programs co-resident in an address space, and its paramount position in an emerging role for EPICS - the integration of dissimilar systems.
description: Poster at International Conference on Accelerator and Large Experimental Physics Control Systems, San Jose, CA, Nov 2001, (THAP014) 3 pages, PDF
Stenosagola egmontensis Park and Carlton, new species
Creators: name: Park, J. - S.
name: Carlton, C. E.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenosagola
Stenosagola egmontensis

description: Stenosagola egmontensis Park and Carlton, new species
 Type Material. Holotype. NEW ZEALAND: TARANAKI (TK): ♂ (wingless male), aedeagus dissected and mounted in balsam on a clear plastic card, “ NEW ZEALAND TK Pouakai Saddle 1220m Pouakai Ra 3 Dec 1975, J.S. Dugdale ”, “Litter 75/204”, “ N.Z. Arthropod Collection, NZAC Private Bag 92170 AUCKLAND New Zealand”, “ HOLOTYPE Stenosagola egmontensis Park and Carlton des. 2013”.  Paratypes (n  = 5: 2 males, 3 females). NEW ZEALAND: NELSON (TK): 2♂♂ 3♀♀ (1♂ 1♀, slide-mounted), same data as holotype (NZAC).
 Etymology. This species is named after the type locality, Egmont National Park, Taranaki (TK).
 Diagnosis. Specimens of S. egmontensis are similar in appearance to those of S. stewartensis but can be distinguished by the shape of the male genitalia (Fig. 4c) and the depression of the basodorsal margin of the male profemur (Fig. 4g, arrow). Members of this species can be separated from those of S. gracilis, S. pseudogracilis, S. clarkei, S. ramsayi, S. domettensis, and S. eylesi by the dull dorsal surface of the head (Figs. 1h–i).
 Description. Length 1.5–1.6 mm (Fig. 1h–i). Head: Wingless male head approximately 1.24 times, female 1.19 times longer than wide (Fig. 4e). Wingless male eye approximately 0.80 times, female 0.65 times as long as temple (Fig. 4e). Wingless male antennomere 3 subquadrate, 4–5 slightly longer than wide, 6–7 subquadrate. Female antennomere 3 subquadrate, 4 slightly longer than wide, 5–7 subquadrate. Thorax: Pronotum subquadrate, approximately 0.90 times longer than wide (Fig. 4f). Wingless male elytra approximately 1.59 times, female 1.45 times longer than pronotum. Wingless male meso- and metaventrites trapezoidal, approximately 1.41 times, female 1.30 times longer than pronotum. Basodorsal margin of male profemur concave (Fig. 4g, arrow). Aedeagus: Left apical lobe of male genitalia acute, longer than right apical lobe, right apical lobe folded over left (Fig. 4c). Left paramere slightly longer than right, setae present anteriorly (Fig. 4c).
 Distribution. Taranaki (TK), New Zealand (Fig. 5, black circle).
 Habitat. Specimens of this species were collected by sifting leaf litter.
description: Published as part of Park, J. - S. & Carlton, C. E., 2013, A Revision of the New Zealand GenusStenosagolaBroun, 1921 (Coleoptera: Staphylinidae: Pselaphinae: Faronitae), pp. 335-359 in The Coleopterists Bulletin 67 (3) on page 344, DOI: 10.1649/0010-065X-67.3.335, http://zenodo.org/record/10100754
A two-pronged approach for studying G-quadruplexes in cancer: integrating fluorescence lifetime imaging and genomics methods
Creators: name: Robinson, Jenna
Publisher: name: Imperial College London
Year: 2023

description: Cellular function and nucleic acid structure are inextricably linked in biology. Whilst DNA often exists as a double helical structure in vivo, G-quadruplexes (G4s) - that form in DNA and RNA regions rich in guanines - are an alternative nucleic acid structure that have attracted attention due to their significant enrichment in cancer cells. Through diverse interactions with regulatory proteins, G4s are thought to regulate gene expression which may allow cancer cells to rapidly respond to external stressors such as drug treatment. In my PhD, I have taken a two-pronged approach to map and image G4s in cancer cells, particularly in the model of drug-resistant ovarian cancer. The first genomics-based method aimed to link G4s to transcriptional networks in drugresistant cancer, utilising CUT&Tag, ChIP-, ATAC- and RNA- sequencing. Through this study, I found that G4 formation, specifically at previously unstudied non-promoter sites, was associated with elevated expression of genes that are critical for modulating the drug response. The second approach used to study G4s was based on the design and characterisation of small-molecule, fluorescent probes that allow G4s to be globally visualised in different cancer cell lines. Most fluorescence intensity probes fail to achieve sufficient G4 binding selectivity to robustly detect G4s in a complex cellular environment. In my work, I have taken a novel approach to visualise G4s that considers the fluorescence lifetime of a probe rather than its fluorescence intensity. Specifically, I have developed the first fluorescence lifetime probe validated for imaging the emerging roles of RNA G4s within cells.
Additional file 1: of Dietary restriction during the treatment of cancer: results of a systematic scoping review
Creators: name: Shingler, Ellie
name: Perry, Rachel
name: Mitchell, Alexandra
name: England, Clare
name: Perks, Claire
name: Herbert, Georgia
name: Ness, Andy
name: Atkinson, Charlotte
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology

description: Search terms used in the Medline database search. (DOCX 13 kb)
Isospin and density dependences of nuclear matter symmetry energy coefficients II
Creators: name: Braghin, Fabio L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Symmetry energy coefficients of explicitly isospin asymmetric nuclear matter at variable densities (from .5$ρ_0$ up to 2 $ρ_0$) are studied as generalized screening functions. An extended stability condition for asymmetric nuclear matter is proposed. We find the possibility of obtaining stable asymmetric nuclear matter even in some cases for which the symmetric nuclear matter limit is unstable. Skyrme-type forces are extensively used in analytical expressions of the symmetry energy coefficients derived as generalized screening functions in the four channels of the particle hole interaction producing alternative behaviors at different $ρ$ and $b$ (respectively the density and the asymmetry coefficient). The spin and spin-isospin coefficients, with corrections to the usual Landau Migdal parameters, indicate the possibility of occurring instabilities with common features depending on the nuclear density and n-p asymmetry. Possible relevance for high energy heavy ions collisions and astrophysical objects is discussed.
description: 16 pages (latex) plus twelve figures in four eps files, to be published in I.J.M.P. E
Deep Learning for Classification of Hyperspectral Data: A Comparative Review
Creators: name: Audebert, Nicolas
name: Saux, Bertrand
name: Lefèvre, Sébastien
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Neural and Evolutionary Computing (cs.NE)
subject: Image and Video Processing (eess.IV)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In recent years, deep learning techniques revolutionized the way remote sensing data are processed. Classification of hyperspectral data is no exception to the rule, but has intrinsic specificities which make application of deep learning less straightforward than with other optical data. This article presents a state of the art of previous machine learning approaches, reviews the various deep learning approaches currently proposed for hyperspectral classification, and identifies the problems and difficulties which arise to implement deep neural networks for this task. In particular, the issues of spatial and spectral resolution, data volume, and transfer of models from multimedia images to hyperspectral data are addressed. Additionally, a comparative study of various families of network architectures is provided and a software toolbox is publicly released to allow experimenting with these methods. 1 This article is intended for both data scientists with interest in hyperspectral data and remote sensing experts eager to apply deep learning techniques to their own dataset.
Additional file 1 of The impact and outcomes of cancer-macrophage fusion
Creators: name: Li, Mengtao
name: Basile, John R.
name: Mallya, Sanjay
name: Lin, Yi-Ling
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Supplementary Material 1
Stenosagola ramsayi Park and Carlton, new species
Creators: name: Park, J. - S.
name: Carlton, C. E.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenosagola
Stenosagola ramsayi

description: Stenosagola ramsayi Park and Carlton, new species
 Type Material. Holotype. NEW ZEALAND: TARANAKI (TK): ♂ (winged male), “New Zealand: TK: Mt. Messenger, 182m 23 I 1972, G.W. Ramsay Litter 72/66”, “ HOLOTYPE Stenosagola ramsayi Park and Carlton des. 2013”.  Paratypes (n  = 11: 7 males, 4 females). NEW ZEALAND: NELSON (NN): 1♂, Gouland Downs, 792m, Heaphy Tk., 5 II 1966, J.I. Townsend, Moss 66/66 (NZAC); TARANAKI (TK): 2♂♂ 4♀♀ (1♂ 1♀, slide-mounted), same data as holotype (NZAC). 1♂, Pouakia Hump, 1220m, 3 XII 1975, A.K. Walker, Moss 75/211 (NZAC); 1♂, Hump Plateau, 1220m, Pouakai Ra., 3 XII 1975, J.S. Dugdale, litter 75/199 (NZAC); WELLINGTON (WN): 1♂ (slide-mounted), Balance Bridge, 18 I 1959, R. A. Cumber (NZAC); 1♂, W Lk Wairarapa Res., 15 VII 1995, decayed Nothofagus, J.T. Nunn.
 Etymology. This species is named for the collector of the holotype, G. W. Ramsay.
 Diagnosis. S pe c i m e n s o f S. r am sa y i a r e similar in appearance to those of S. gracilis, S. pseudogracilis, S. clarkei, S. domettensis, and S. eylesi but can be distinguished by the shape of the male genitalia (Fig. 4d). Members of this species can be separated from those of S. egmontensis and S. stewartensis by the glossy dorsal surface of the head (Fig. 1j–l).
 Description. Length 1.6–1.7 mm (Fig. 1j–l). Head: Winged male head approximately 1.46 times, wingless male 1.36 times, female 1.39 times longer than wide. Winged male eye approximately 1.06 times, wingless male 0.69 times, female 0.59 times as long as temple. Winged male antennomere 3 subquadrate, 4 longer than wide, 5–6 subquadrate, 7 transverse. Wingless male antennomere 3 subquadrate, 4 slightly longer than wide, 5–6 subquadrate, 7 slightly transverse. Female antennomere 3–4 subquadrate, 5–7 transverse. Thorax: Pronotum approximately 1.05 times longer than wide. Winged male elytra approximately 1.75 times, wingless male and female 1.26 times longer than pronotum. Winged male meso- and metaventrites trapezoidal, approximately 1.54, wingless male 1.17 times, female 1.12 times longer than pronotum. Aedeagus: Left apical lobe of male genitalia equal in width and shorter than right (Fig. 4d). Left paramere broader than right, setae present anteriorly (Fig. 4d).
 Distribution. Wellington (WN), New Zealand (Fig. 5, black squares).
 Habitat. Specimens of this species were collected by sifting leaf or moss litter.
description: Published as part of Park, J. - S. & Carlton, C. E., 2013, A Revision of the New Zealand GenusStenosagolaBroun, 1921 (Coleoptera: Staphylinidae: Pselaphinae: Faronitae), pp. 335-359 in The Coleopterists Bulletin 67 (3) on pages 344-345, DOI: 10.1649/0010-065X-67.3.335, http://zenodo.org/record/10100754
Additional file 1: of Evaluating the quality of the 1000 genomes project data
Creators: name: Saurabh Belsare
name: Levy-Sakin, Michal
name: Mostovoy, Yulia
name: Durinck, Steffen
name: Chaudhuri, Subhra
name: Xiao, Ming
name: Peterson, Andrew
name: Pui-Yan Kwok
name: Somasekar Seshagiri
name: Wall, Jeffrey
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Figure S1. Representative distribution of INFO scores for chromosome 1 in HG00250 in (a) experimental SNPs (b) all 1000G SNPs. Figure S2. Imputation error in experimental SNPs after filtering low INFO score (
Upgrade of Spring-8 Beamline Network with Vlan Technology Over Gigabit Ethernet
Creators: name: Ishii, M.
name: Fukui, T.
name: Furukawa, Y.
name: Nakatani, T.
name: Ohata, T.
name: Tanaka, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences
subject: C.2.1

description: The beamline network system at SPring-8 consists of three LANs; a BL-LAN for beamline component control, a BL-USER-LAN for beamline experimental users and an OA-LAN for the information services. These LANs are interconnected by a firewall system. Since the network traffic and the number of beamlines have increased, we upgraded the backbone of BL-USER-LAN from Fast Ethernet to Gigabit Ethernet. And then, to establish the independency of a beamline and to raise flexibility of every beamline, we also introduced the IEEE802.1Q Virtual LAN (VLAN) technology into the BL-USER-LAN. We discuss here a future plan to build the firewall system with hardware load balancers.
description: 3 pages, 2 figure, 8th International Conference on Accelerator and Large Experimental Physics Control Systems (PSN TUAP056), San Jose, CA, USA, November 27-30
Stokes waves with constant vorticity: II. folds, gaps and fluid bubbles
Creators: name: Dyachenko, Sergey A.
name: Hur, Vera Mikyoung
Publisher: name: arXiv
Year: 2019
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: 76B15

description: The Stokes wave problem in a constant vorticity flow is formulated, by virtue of conformal mapping techniques, as a nonlinear pseudodifferential equation, involving the periodic Hilbert transform, which becomes the Babenko equation in the irrotational flow setting. The associated linearized operator is self-adjoint, whereby the modified Babenko equation is efficiently solved by means of the Newton-Conjugate Gradient method. For strong positive vorticity, a `fold' appears in the wave speed versus amplitude plane, and a `gap' as the vorticity strength increases, bounded by two touching waves, whose profile contacts with itself at the trough line, enclosing a bubble of air. More folds and gaps follow for stronger vorticity. Touching waves at the beginnings of the lowest gaps tend to the limiting Crapper wave as the vorticity strength increases indefinitely, while the profile encloses a circular bubble of fluid in rigid body rotation at the ends of the gaps. Touching waves at the beginnings of the second gaps tend to the circular vortex wave on top of the limiting Crapper wave in the infinite vorticity limit, and the circular vortex wave on top of itself at the ends of the gaps. Touching waves for higher gaps accommodate more circular bubbles of fluid.
Additional file 5 of The impact and outcomes of cancer-macrophage fusion
Creators: name: Li, Mengtao
name: Basile, John R.
name: Mallya, Sanjay
name: Lin, Yi-Ling
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Supplementary Material 5
An Algebraic Pairing Model with Sp(4) Symmetry and its Deformation
Creators: name: Sviratcheva, K. D.
name: Georgieva, A. I.
name: Draayer, J. P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A fermion realization of the compact symplectic sp(4) algebra provides a natural framework for studying isovector pairing correlations in nuclei. While these correlations manifest themselves most clearly in the binding energies of 0^+ ground states, they also have a large effect on the energies of excited states, including especially excited 0^+ states. In this article we consider non-deformed as well as deformed algebraic descriptions of pairing through the reductions of sp_{(q)}(4) to different realizations of u_{(q)}(2) for single-j and multi-j orbitals. The model yields a classification scheme for completely paired 0^{+} states of even-even and odd-odd nuclei in the 1d_{3/2}, 1f_{7/2}, and 1f_{5/2}2p_{1/2}2p_{3/2}1g_{9/2} shells. Phenomenological non-deformed and deformed isospin-breaking Hamiltonians are expressed in terms of the generators of the dynamical symmetry groups Sp(4) and Sp_{q}(4). These Hamiltonians are related to the most general microscopic pairing problem, including isovector pairing and isoscalar proton-neutron interaction along with non-linear interaction in the deformed extension. In both the non-deformed and deformed cases the eigenvalues of the Hamiltonian are fit to the relevant Coulomb corrected experimental 0^{+} energies and this, in turn, allows us to estimate the interaction strength parameters, to investigate isovector-pairing properties and symmetries breaking, and to predict the corresponding energies. While the non-deformed theory yields results that are comparable to other theories for light nuclei, the deformed extension, which takes into account higher-order interactions between the particles, gives a better fit to the data. The multi-shell applications of the model provide for reasonable predictions of energies of exotic nuclei.
description: 19 pages, 5 figures minor changes; improvements to achieve a better and clearer presentation of our messages and ideas
Stenosagola stewartensis Park and Carlton, new species
Creators: name: Park, J. - S.
name: Carlton, C. E.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenosagola
Stenosagola stewartensis

description: Stenosagola stewartensis Park and Carlton, new species
 Type Material. Holotype. NEW ZEALAND: STEWART ISLAND (SI): ♂ (wingless male, slide-mounted), “New Zealand: SI: Bigs Cape I, S Peak, 250′ 11 XI 1968, J. McBurney Litter 68/185 ”, “ HOLOTYPE Stenosagola stewartensis Park and Carlton des. 2013”.
 Etymology. This species is named after the type locality, Stewart Island (SI).
 Diagnosis. Specimens of S. stewartensis are similar in appearance to those of S. egmontensis but can be distinguished by the shape of the male genitalia (Fig. 4j). Members of this species can be separated those of S. gracilis, S. pseudogracilis, S. clarkei, S. ramsayi, S. domettensis, and S. eylesi by the dull dorsal surface of the head (Fig. 1p).
 Description. Length 1.7 mm (Fig. 1p). Head: Wingless male head approximately 1.13 times longer than wide, eye 0.89 times longer than temple. Wingless male antennomere 3–5 subquadrate, 6–7 slightly transverse. Thorax: Pronotum approximately 0.92 times longer than wide. Wingless male elytra approximately 1.43 times longer than pronotum. Wingless male meso- and metaventrites trapezoidal, approximately 1.27 longer than pronotum. Aedeagus: Apical lobe of male genitalia with two branches; main lobe bifid apically, minor lobe divided from ventral base of main lobe, longer and narrower (Fig. 4j). Left paramere slightly broader than right, setae present at tip and middle (Fig. 4j).
 Distribution. Stewart Island (SI), New Zealand (Fig. 5, white square).
 Habitat. The unique holotype was collected by sifting leaf litter.
description: Published as part of Park, J. - S. & Carlton, C. E., 2013, A Revision of the New Zealand GenusStenosagolaBroun, 1921 (Coleoptera: Staphylinidae: Pselaphinae: Faronitae), pp. 335-359 in The Coleopterists Bulletin 67 (3) on page 346, DOI: 10.1649/0010-065X-67.3.335, http://zenodo.org/record/10100754
MOESM1 of Initial management of diabetic ketoacidosis and prognosis according to diabetes type: a French multicentre observational retrospective study
Creators: name: Balmier, Adrien
name: Dib, Fadia
name: Serret-Larmande, Arnaud
name: Montmollin, Etienne
name: Pouyet, Victorine
name: Sztrymf, Benjamin
name: Megarbane, Bruno
name: Abirami Thiagarajah
name: Dreyfuss, Didier
name: Jean-Damien Ricard
name: Roux, Damien
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Science Policy
subject: 60506 Virology

description: Additional file 1: Table S1. Metabolic complications (hypoglycaemia, hypokalaemia, hypophosphatemia) according to the type of diabetes.
A Wilson Group of Non-Uniformly Exponential Growth
Creators: name: Bartholdi, Laurent
Publisher: name: arXiv
Year: 2002
Subjects: subject: Group Theory (math.GR)
subject: Metric Geometry (math.MG)
subject: FOS: Mathematics
subject: 20E08, 20F05

description: This note constructs a finitely generated group $W$ whose word-growth is exponential, but for which the infimum of the growth rates over all finite generating sets is 1 -- in other words, of non-uniformly exponential growth. This answers a question by Mikhael Gromov. The construction also yields a group of intermediate growth $V$ that locally resembles $W$ in that (by changing the generating set of $W$) there are isomorphic balls of arbitrarily large radius in $V$ and $W$'s Cayley graphs.
description: 6 pages, 2 figures
Large-Scale Analysis of Pop-Up Scam on Typosquatting URLs
Creators: name: Dam, Tobias
name: Klausner, Lukas Daniel
name: Buhov, Damjan
name: Schrittwieser, Sebastian
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Today, many different types of scams can be found on the internet. Online criminals are always finding new creative ways to trick internet users, be it in the form of lottery scams, downloading scam apps for smartphones or fake gambling websites. This paper presents a large-scale study on one particular delivery method of online scam: pop-up scam on typosquatting domains. Typosquatting describes the concept of registering domains which are very similar to existing ones while deliberately containing common typing errors; these domains are then used to trick online users while under the belief of browsing the intended website. Pop-up scam uses JavaScript alert boxes to present a message which attracts the user's attention very effectively, as they are a blocking user interface element. Our study among typosquatting domains derived from the Alexa Top 1 Million list revealed on 8255 distinct typosquatting URLs a total of 9857 pop-up messages, out of which 8828 were malicious. The vast majority of those distinct URLs (7176) were targeted and displayed pop-up messages to one specific HTTP user agent only. Based on our scans, we present an in-depth analysis as well as a detailed classification of different targeting parameters (user agent and language) which triggered varying kinds of pop-up scams.
description: 9 pages, 11 figures
Additional file 2 of The impact and outcomes of cancer-macrophage fusion
Creators: name: Li, Mengtao
name: Basile, John R.
name: Mallya, Sanjay
name: Lin, Yi-Ling
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Supplementary Material 2
Clustering Properties of Galaxies at z~4 in the Subaru/XMM Deep Survey Field
Creators: name: Ouchi, Masami
name: Shimasaku, Kazuhiro
name: Okamura, Sadanori
name: Doi, Mamoru
name: Furusawa, Hisanori
name: Hamabe, Masaru
name: Kimura, Masahiko
name: Komiyama, Yutaka
name: Miyazaki, Masayuki
name: Miyazaki, Satoshi
name: Nakata, Fumiaki
name: Sekiguchi, Maki
name: Yagi, Masafumi
name: Yasuda, Naoki
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the clustering properties of about 1200 z~4 Lyman Break Galaxy (LBG) candidates with i'<26 which are selected by color from deep BRi' imaging data of a 618 arcmin^2 area in the Subaru/XMM-Newton Deep Field taken with Subaru Prime Focus Camera. The contamination and completeness of our LBG sample are evaluated, on the basis of the Hubble Deep Field North (HDFN) objects, to be 17% and 45%, respectively. We derive the angular correlation function over theta = 2''-1000'', and find that it is fitted fairly well by a power law, omega(theta)=A_omega theta^{-0.8}, with A_omega = 0.71 +/- 0.26. We then calculate the correlation length r0 (in comoving units) of the two-point spatial correlation function xi(r) = (r/r0)^{-1.8} from A_omega using the redshift distribution of LBGs derived from the HDFN, and find r0=2.7 (+0.5/-0.6) h^{-1} Mpc in a Lambda-dominated universe (Omega_m=0.3 and Omega_Lambda=0.7). This is twice larger than the correlation length of the dark matter at z~4 predicted from an analytic model by Peacock & Dodds but about twice smaller than that of bright galaxies predicted by a semi-analytic model of Baugh et al. We find an excess of omega(theta) on small scales (theta < 5'') departing from the power law fit over 3 sigma significance levels. Interpreting this as due to galaxy mergers, we estimate the fraction of galaxies undergoing mergers in our LBG sample to be 3.0 +/- 0.9%, which is significantly smaller than those of galaxies at intermediate redshifts.
description: 9 pages, 4 figures, to be published in ApJ Letters
Proteroscelio antennalis Brues 1937
Creators: name: Johnson, Norman F.
name: Musetti, Luciana
name: Masner, Lubomír
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Scelionidae
Proteroscelio
Proteroscelio antennalis

description: PROTEROSCELIO ANTENNALIS BRUES   Figures 1–2
description: Published as part of Johnson, Norman F., Musetti, Luciana & Masner, Lubomír, 2008, The Cretaceous Scelionid Genus Proteroscelio Brues (Hymenoptera: Platygastroidea), pp. 1-8 in American Museum Novitates 3603 (1) on page 3, DOI: 10.1206/0003-0082(2008)3603[1:TCSGPB]2.0.CO;2, http://zenodo.org/record/5389182
Additional file 4 of The impact and outcomes of cancer-macrophage fusion
Creators: name: Li, Mengtao
name: Basile, John R.
name: Mallya, Sanjay
name: Lin, Yi-Ling
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Supplementary Material 4
Volume uncertainty assessment method of asteroid models from disk-integrated visual photometry
Creators: name: Bartczak, P.
name: Dudziński, G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The need for more accurate asteroid models is perhaps secondary to the need to measure their quality. The uncertainties of models' parameters propagate to quantities like volume or density -- the most important and informative properties of asteroids -- affecting conclusions about their physical nature. Our knowledge on shapes and spins of small solar system bodies comes mostly from visual, disk-integrated photometry. In this work we present a method for asteroid model uncertainty assessment based on visual photometry (lightcurves and sparse-in-time absolute measurements) allowing the determination of realistic volume uncertainty, as well as spin axis orientation, rotational period and local surface features. The sensitivity analysis is conducted by creating clones of the nominal model and accepting the ones that fit the observations within a confidence level. The uncertainties of model parameters are extracted from the extreme values found in the accepted clone population. Creation of such population of clones enables the conversion of a deterministic asteroid model into stochastic one, and can be utilized to create observation predictions with error bars. The method was used to assess the uncertainties of fictitious test models and real targets, i.e. (21) Lutetia, (89) Julia, (243) Ida, (433) Eros and (162173) Ryugu. We conclude that volumes, and subsequently, densities of asteroids derived from lightcurve-based models likely have vastly understated uncertainties, the biggest source of which is the inability to establish the extent of the model along its spin axis.
Funnel Flows from Disks to Magnetized Stars
Creators: name: Koldoba, A. V.
name: Lovelace, R. V. E.
name: Ustyugova, G. V.
name: Romanova, M. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This work considers flows from an accretion disk corotating with the aligned dipole magnetic field of a rotating star. Ideal magnetohydrodynamics (MHD) is assumed with the pressure and density related as $p \propto ρ^γ$ and with $ρ{\bf v}^2 \ll {\bf B}^2/4π$, where ${\bf v}$ is the flow velocity. This limit corresponds to the Alfvén radius for the disk accretion larger than the corotation radius. Transonic flows, which go from subsonic motion near the disk to supersonic inflow near the star, are shown to be possible only for a narrow range of $R_d \sim r_c \equiv (GM/Ω^2)^{1/3}$, where $R_d$ is the radius at which the dipole field line intersects the disk, $r_c$ the corotation radius, $M$ the mass of the star, and $Ω$ its angular rotation rate. The transonic flows have very different behaviors for $γ> 7/5$ and $< 7/5$. In both cases, the plasma flow velocity ${\bf v}$ (which is parallel to ${\bf B}$) increases with decreasing distance $R$ from the star. However, for $γ>7/5$, the Mach number ${\cal M} \equiv |{\bf v}|/c_s$ (with $c_s$ the sound speed) initially increases with $R$ decreasing from $R_d$, but for $R$ decreasing from $\approx 0.22 R_d$ (for $γ=5/3$)the Mach number surprisingly {\it decreases}. In the other limit, $γ< 7/5$, ${\cal M}$ increases monotonically with decreasing $R$. Application of these results is made to funnel flows to rotating magnetized neutron stars and young stellar objects.
description: 7 pages, 7 figures, submitted to ApJ
Camptotylus linae
Creators: name: Konstantinov, Fedor V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Camptotylus
Camptotylus linae

description: Camptotylus linae (Puton, 1881)   Figures 10, 16, 34, 40
description: Published as part of Konstantinov, Fedor V., 2008, Review of the genus Camptotylus Fieber, 1860 (Heteroptera: Miridae) with description of two new species, pp. 1-24 in American Museum Novitates 3606 (1) on page 10, DOI: 10.1206/0003-0082(2008)3606[1:ROTGCF]2.0.CO;2, http://zenodo.org/record/5389228
Stenosagola butcheri Park and Carlton, new species
Creators: name: Park, J. - S.
name: Carlton, C. E.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenosagola
Stenosagola butcheri

description: Stenosagola butcheri Park and Carlton, new species
 Type Material. Holotype. NEW ZEALAND: WAIKATO (WO): 1♂ (winged male), “ NEW ZEALAND WO Mt Karioi 11 Oct 1981 C.F. Butcher Litter 81/95”, “ N.Z. Arthropod Collection, NZAC Private Bag 92170 AUCKLAND New Zealand”, “ HOLOTYPE Stenosagola butcheri Park and Carlton des. 2013”.  Paratypes (n  = 2 males). NEW ZEALAND: AUCKLAND (AK): 1♂ (slide-mounted), Clevedon Scenic Reser. 0.5km N Clevedon, 20m, III-19-2010 D.S. Chandler, sift forest litter by stream (DSC); NORTHLAND (ND): 1♂ (slide-mounted), Mangamuka summit, 400m, 15 XII 1976, N.M. May, litter 76/108 (NZAC).
 Etymology. This species is named for the collector of the holotype, C. F. Butcher.
 Diagnosis. Specimens of S. butcheri are similar in appearance to those of other members of the connata group but can be distinguished by the shape of the male genitalia (Fig. 12e).
 Description. Length 1.2–1.3 mm (Fig. 7l–m). Head: Winged male head approximately 1.52 times, wingless male 1.50 times longer than wide. Winged male eye approximately 1.59 times, wingless male 0.9 times longer than temple. Winged male antennomeres 3–8 subquadrate, 9–10 transverse. Wingless male antennomeres 3–7 subquadrate, 8 slightly transverse, 9–10 transverse. Thorax: Pronotum as long as wide. Winged male elytra approximately 1.89, wingless male 1.29 times longer than pronotum. Winged male meso- and metaventrites trapezoidal, approximately1.65 times, wingless male 1.19 times longer than pronotum. Aedeagus: Apical lobe of male genitalia emarginate and bent to right (Fig. 12e). Left paramere longer than right, bearing setae apically (Fig. 12e).
 Distribution. Northern part of North Island, New Zealand (Fig. 14, black squares).
 Habitat. All specimens were collected by sifting forest litter.
description: Published as part of Park, J. - S. & Carlton, C. E., 2013, A Revision of the New Zealand GenusStenosagolaBroun, 1921 (Coleoptera: Staphylinidae: Pselaphinae: Faronitae), pp. 335-359 in The Coleopterists Bulletin 67 (3) on pages 356-357, DOI: 10.1649/0010-065X-67.3.335, http://zenodo.org/record/10100754
The ESRF TANGO control system status
Creators: name: Chaize, JM.
name: Goetz, A.
name: Klotz, WD.
name: Meyer, J.
name: Perez, M.
name: Taurel, E.
name: Verdier, P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences
subject: C.2.4;D.1.3

description: TANGO is an object oriented control system toolkit based on CORBA presently under development at the ESRF. IN this paper, the TANGO philosophy is briefly presented. All the existing tools developed around TANGO will also be presented. This include a code genrator, a WEB interface to TANGO objects, an administration tool and an interface to LabView. Finally, an xample of a TANGO device server for OPC device is given.
description: 3 pages
Table S1 from Proximal Partners of the Organellar N-terminal Acetyltransferase NAA60: Insights into Golgi Structure and Transmembrane Protein Topology
Creators: name: Tanco, Sebastian
name: Jonckheere, Veronique
name: Tharkeshwar, Arun Kumar
name: Bogaert, Annelies
name: Gevaert, Kris
name: Anneart, Wim
name: Van Damme, Petra
Publisher: name: The Royal Society
Year: 2025
Subjects: classificationCode: 310803
subject: Plant cell and molecular biology
classificationCode: 310902
subject: Animal cell and molecular biology

description: NAA60 BioID Interaction Profiling
Excitation of localized graphene plasmons by a metallic slit
Creators: name: Bludov, Yuliy V.
name: Peres, Nuno M. R.
name: Vasilevskiy, Mikhail I.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this paper we show that graphene surface plasmons can be excited when an electromagnetic wave packet impinges on a single metal slit covered with graphene. The excitation of the plasmons localized over the slit is revealed by characteristic peaks in the absorption spectrum. It is shown that the position of the peaks can be tuned either by the graphene doping level or by the dielectric function of the material filling the slit. The whole system forms the basis for a plasmonic sensor when the slit is filled with an analyte.
description: 10 pages, 6 figures
Application of Doppler Broadened Gamma Spectroscopy to Study the Surface of Graphene
Creators: name: Weiss, A. H.
name: Chirayath, V. A.
name: Gladen, R. W.
name: Fairchild, A. J.
name: Chrysler, M. D.
name: Sterne, P. A.
name: Koymen, A. R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present Doppler broadened gamma spectra, obtained using the newly developed advanced positron beam at the University of Texas at Arlington, from a sample consisting of 6 to 8 layers of graphene (MLG) on polycrystalline Cu. The kinetic energy of the positron beam was varied form 2 eV to 20 keV allowing for a depth resolved measurement. The ratio curves formed by dividing the measured Doppler broadened gamma spectra obtained at low positron kinetic energies (~2eV) to the gamma spectra obtained at 20 keV were compared to ratio curves found by dividing the calculated spectra of bulk graphite to bulk Cu. The ratio curves obtained from the measured results show qualitative agreement with those obtained from the calculated spectra. In particular, both sets of curves indicate a much reduced intensity at high momentum. The agreement between the measured and calculated curves is consistent with the hypothesis that the 2eV spectra correspond to the Doppler broadened spectra from the thin overlayer of Graphene (which we anticipate should be similar to the spectra obtained from bulk graphite) and that the spectra taken at 20 keV corresponds to bulk Cu due to the fact that most of the positrons implanted at this energy annihilate in the Cu substrate. The results taken at 2 eV provide evidence that it is possible to obtain chemically sensitive information from the top atomic layers of surfaces (both internal and external) from an analysis of the high momentum tail of the Doppler broadened gamma spectra obtained from the annihilation of positrons at the surface.
description: Presented at 18th International Conference on Positron Annihilation, August 19-24, 2018 | Orlando, USA. The following article has been accepted by AIP Conference Proceedings. After it is published, it will be found at https://aip.scitation.org/journal/apc
Extraction of the n structure function $F_2^n$ from inclusive scattering data on composite nuclei
Creators: name: Rinat, A. S.
name: Taragin, M. F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We consider a generalized convolution, linking Structure Functions (SF) $F^N_2$ for nucleons, $F^A_2$ for a physical nucleus and $f^{PN,A}$ for a nucleus, composed of point-nucleons. In order to extract $F_2^n$ we employ data on $F_2^{p,A}$ and the computed $f^{PN,A}$. Only for $Q^2\approx 3.5 {\rm GeV}^2$ do data permit the extraction of $F_2^A(x,3.5)$ over a sufficiently wide $x$-range. Applying Mellin transforms, the above relation between SF turns into an algebraic one, which one solves for the Mellin transform of the unknown $F_2^n$. We present inversion methods leading to the desired $F_2^n$, all using a parametrization for $C(x,Q^2)=F_2^n(x,Q^2)/F_2^p(x,Q^2)$. Imposing motivated constraints, the simplest parametrization leaves one free parameter $C(x=1,Q^2)$. For $Q^2= 3.5 {\rm GeV}^2$ its average over several targets and different methods is $=0.54\pm0.03$. We argue that for the investigated $Q^2$, $C(x\to 1,3.5)$ is determined by the nucleon-elastic ($NE$) part of SF. The calculated value is near the extracted one and both are close to the SU(6) limit 2/3.
description: 14 pages,1 Fig, tex file
Solution to Rubel's question about differentially algebraic dependence on initial values
Creators: name: Katriel, Guy
Publisher: name: arXiv
Year: 2002
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 34A09; 12H05

description: We prove that, for generic systems of polynomial differential equations, the dependence of the solution on the initial conditions is not differentially algebraic. This answers, in the negative, a question posed by L.A. Rubel.
Bayesian leave-one-out cross-validation for large data
Creators: name: Magnusson, Måns
name: Andersen, Michael Riis
name: Jonasson, Johan
name: Vehtari, Aki
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (stat.ML)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Model inference, such as model comparison, model checking, and model selection, is an important part of model development. Leave-one-out cross-validation (LOO) is a general approach for assessing the generalizability of a model, but unfortunately, LOO does not scale well to large datasets. We propose a combination of using approximate inference techniques and probability-proportional-to-size-sampling (PPS) for fast LOO model evaluation for large datasets. We provide both theoretical and empirical results showing good properties for large data.
description: Accepted to ICML 2019. This version is the submitted paper
Wind Circulation in Selected Rotating Magnetic Early-B Stars
Creators: name: Smith, Myron A.
name: Groote, Detlef
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The rotating magnetic B stars have oblique dipolar magnetic fields and often anomalous helium and metallic compositions. These stars develop co-rotating torus-shaped clouds by channelling winds from their magnetic poles to an anchored planar disk over the magnetic equator. The line absorptions from the cloud can be studied as the complex rotates and periodically occults the star. We describe an analysis of the clouds of four stars (HD184927, beta Cep, sigma Ori E, and HR6684). From line synthesis models, we find that the metallic compositions are spatially uniform over the stars' surfaces. Next, using the Hubeny CIRCUS code, we demonstate that periodic UV continuum fluxes can be explained by the absorption of low-excitation lines. The analysis also quantifies the cloud temperatures, densities, and turbulences, which appear to increase inward toward the stars. The temperatures range from about 12,000K for the weak Fe lines up to temperatures of 33,000K for N V absorptions, which is in excess of temperatures expected from radiative equilibrium. The spectroscopic hallmark of this stellar class is the presence of strong C IV and N V resonance line absorptions at occultation phases and of redshifted emissions at magnetic pole-on phases. The emissions have characteristics which seem most compatible with the generation of high-energy shocks at the wind-cloud interface, as predicted by Babel.
description: 19 pages, Latex plus 6 figures A&A single-spaced, accepted by Astronomy & Astrophysics. Files available by ftp at nobel.stsci.edu/pub/aapaper/
Forming one of the most massive objects in the Universe: The quadruple merger in Abell 1758
Creators: name: Schellenberger, Gerrit
name: David, Laurence P.
name: O'Sullivan, Ewan
name: Vrtilek, Jan M.
name: Haines, Chris P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Abell1758 is a system of two galaxy clusters, a more massive, northern cluster and a southern cluster. Both parts are undergoing major merger events at different stages. Although the mass of the merger constituents provides enough energy to produce visible shock fronts in the X-ray, none have been found to date. We present detailed temperature and abundance maps based on Chandra ACIS data, and identify several candidates for shocks and cold fronts from a smoothed gradient map of the surface brightness. One candidate can be confirmed as the missing shock front in the northern cluster through X-ray spectroscopy. Non-thermal radio emission observed with the GMRT confirms the presence of radio halos in the northern and southern clusters, and shows evidence for a relic in the periphery of the southern cluster. We do not find evidence for shocked gas between A1758N and A1758S.
description: accepted by ApJ, 24 pages, 16 figures
Hydrostatic Expansion and Spin Changes During Type I X-Ray Bursts
Creators: name: Cumming, Andrew
name: Morsink, Sharon M.
name: Bildsten, Lars
name: Friedman, John L.
name: Holz, Daniel E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present calculations of the spin-down of a neutron star atmosphere due to hydrostatic expansion during a Type I X-ray burst. We show that (i) Cumming and Bildsten overestimated the spin-down of rigidly-rotating atmospheres by a factor of two, and (ii) general relativity has a small (5-10%) effect on the angular momentum conservation law. We rescale our results to different neutron star masses, rotation rates and equations of state, and present some detailed rotational profiles. Comparing with recent observations of large frequency shifts in MXB 1658-298 and 4U 1916-053, we find that the spin-down expected if the atmosphere rotates rigidly is a factor of two to three less than the observed values. If differential rotation is allowed to persist, we find that the upper layers of the atmosphere spin down by an amount comparable to the observed values; however, there is no compelling reason to expect the observed spin frequency to be that of only the outermost layers. We conclude that hydrostatic expansion and angular momentum conservation alone cannot account for the largest frequency shifts observed during Type I bursts.
description: Submitted to the Astrophysical Journal (13 pages, including 4 figures)