cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Mid-Infrared Imaging of Young Stellar Objects
Creators: name: Liu, Michael C.
name: Graham, James R.
name: Ghez, A. M.
name: Meixner, M.
name: Skinner, C. J.
name: Keto, Eric
name: Ball, Roger
name: Arens, J. F.
name: Jernigan, J. G.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present arcsecond resolution mid-infrared (8--13 $μ$m) images and photometry of four young stellar objects (YSOs)~--- L1551-IRS5, HL~Tau, AS~205, and AS~209 (V1121~Oph)~--- taken with the Berkeley Mid-Infrared Camera. For AS~205, a known T Tauri binary, we also present near-infrared JHK images and HKL$^{\prime}$ speckle imaging data. All three single stars are unresolved in our mid-IR images. Our data is the first to resolve in the mid-IR both components of the close binary AS~205 (projected separation $\sim$1.3$^{\prime \prime}$ (210~A.U.)). AS~205~North is the IR brighter star in our data while published observations find it to be the optically fainter star. Pre-main sequence evolutionary models suggest the AS~205 system is non-coeval; we discuss possible explanations for this result and comment on the circumstellar material and evolutionary status of this young binary. Nearly all of our objects exhibit changes in their mid-IR flux in measurements separated by intervals of days up to many years; the variations range from 30--300\%. We speculate that the cause of the variability lies in the accretion disks of these objects; the data suggest disk accretion rate fluctuations of nearly an order of magnitude. The existence of large mid-IR variability argues that simultaneous multiwavelength observations are needed for a proper analysis of YSO spectral energy distributions.
description: 27 pages (22 text and 5 figures) of uuencoded, gzipped Postscript
Coracias oriolus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Coraciiformes
Coraciidae
Coracias
Coracias oriolus

description: Coracias oriolus [spec. nov.]
C. flava alis caudaque nigris.
Ampelis flava, artibus nigris, rectricibus quinque exterioribus retrorsum flavis. Act. Stockh. 1750. p. 127. t. 3. f. 5.
Oriolus. Gesn. av ....
Galbula. Aldr. orn. 854. t. 857. 858.
Galbula benghalensis. Edw. av. 185. t. 185.
Picus nidum suspendens. Will. orn... t. 36. f. 6. & t. 38. f. 4. Jonst. av. 112. t. 41 f. 8. Raj. av. 68.
Flava avis benghalensis. Alb. av. 3. p. 19. t. 20.
Habitat in Europa, Asia, migratoria avis.
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 107-108, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Multiscale socio-ecological networks in the age of information
Creators: name: Lenormand, Maxime
name: Luque, Sandra
name: Langemeyer, Johannes
name: Tenerelli, Patrizia
name: Zulian, Grazia
name: Aalders, Inge
name: Chivulescu, Serban
name: Clemente, Pedro
name: Dick, Jan
name: van Dijk, Jiska
name: van Eupen, Michiel
name: Giuca, Relu C.
name: Kopperoinen, Leena
name: Lellei-Kovács, Eszter
name: Leone, Michael
name: Lieskovský, Juraj
name: Schirpke, Uta
name: Smith, Alison C.
name: Tappeiner, Ulrike
name: Woods, Helen
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Social and Information Networks (cs.SI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Interactions between people and ecological systems, through leisure or tourism activities, form a complex socio-ecological spatial network. The analysis of the benefits people derive from their interactions with nature -- also referred to as cultural ecosystem services (CES) -- enables a better understanding of these socio-ecological systems. In the age of information, the increasing availability of large social media databases enables a better understanding of complex socio-ecological interactions at an unprecedented spatio-temporal resolution. Within this context, we model and analyze these interactions based on information extracted from geotagged photographs embedded into a multiscale socio-ecological network. We apply this approach to 16 case study sites in Europe using a social media database (Flickr) containing more than 150,000 validated and classified photographs. After evaluating the representativeness of the network, we investigate the impact of visitors' origin on the distribution of socio-ecological interactions at different scales. First at a global scale, we develop a spatial measure of attractiveness and use this to identify four groups of sites. Then, at a local scale, we explore how the distance traveled by the users to reach a site affects the way they interact with this site in space and time. The approach developed here, integrating social media data into a network-based framework, offers a new way of visualizing and modeling interactions between humans and landscapes. Results provide valuable insights for understanding relationships between social demands for CES and the places of their realization, thus allowing for the development of more efficient conservation and planning strategies.
description: 10 pages, 6 figures + Appendix
Some Fixed Point Results for Contractive Type Conditions in Cone b-Metric Spaces and Applications
Creators: name: G.S. Saluja
Publisher: name: figshare
Year: 2018
Subjects: subject: 10104 Combinatorics and Discrete Mathematics (excl. Physical Combinatorics)
subject: FOS: Mathematics

description: In this paper, we establish some fixed point results for contractive type conditions in the framework of complete cone b-metric spaces and give some applications of our results. The results presented in this paper generalize, extend and unify several well-known comparable results in the existing literature.
HST Imaging of the Globular Clusters in the Fornax Cluster: Color and Luminosity Distributions
Creators: name: Grillmair, Carl J.
name: Forbes, Duncan A.
name: Brodie, Jean P.
name: Elson, Rebecca
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the luminosity and B-I color distribution of globular clusters for three early-type galaxies in the Fornax cluster using imaging data from the Wide Field/Planetary Camera 2 on the Hubble Space Telescope. The luminosity functions we derive are in most cases better than 50% complete down to B = 26.6. We find that the color distributions of globular clusters in the central region of NGC 1399 and its nearby neighbor NGC 1404 are bimodal and statistically indistinguishable. The metallicity spread, as inferred from the color distributions in these two galaxies, is very similar to that of M 87. NGC 1399's luminosity function is also very similar to that of M 87, and comparing their respective peak magnitudes indicates that the Fornax cluster is at very nearly the same distance from the Local Group as is the Virgo cluster. From this we derive H_0 = 82 +/- 8 km/s/Mpc, where the uncertainty reflects only the effects of random errors. The number of unresolved objects we find at a projected distance of 440 kpc from NGC 1399 is consistent with nothing more than compact background galaxies, though the small field of view of the WFPC2 does not allow us to put strong constraints on the number of intergalactic globular clusters. The luminosity function of objects detected around NGC 1316 is more nearly exponential than log-normal, and both the color and size distribution of these objects distinguishes them from the clusters surrounding NGC 1399. We suggest that these objects are more akin to old open clusters in the Galaxy than they are to globular clusters in typical early-type galaxies.
description: 32 pages, incl. 2 JPEG figures, AAS LaTeX, to be published in the Astronomical Journal
An investigation of body composition in relation to clinical outcomes and immune response in patients undergoing colorectal cancer surgery
Creators: name: Malietzis, Georgios
Publisher: name: Imperial College London
Year: 2015

description: Colorectal cancer (CRC), the second leading cause of cancer mortality in the UK, is on the rise. Cancer research often focuses on the molecular biology of a tumour, whereas the importance of the biology and condition of the tumour host - the patient - has been underappreciated. The aim of my thesis was to examine the assumption that a systemic (S) and local inflammatory response (IR) is related to the host Body Composition (BC) and also associated with clinical outcomes in patients treated for CRC. Chapter 4 concluded that specific BC profiles such, as the presence of myopenia was an independent predictor of poor survival. Chapter 5 determined the role of the neutrophil to lymphocyte ratio as a prognostic marker for patients with CRC undergoing curative resection. Chapter 6 used CT image analysis to confirm a strong relationship between SIR and muscle depletion in patients with CRC. In Chapter 7, laparoscopy and moderate preoperative SIR favoured preservation and restoration of muscle mass, postoperatively in patients treated for CRC. In Chapter 8.1 through flow cytometry analysis, it was shown that, in a selected group of CRC patients when compared to healthy controls, the circulating DCs were more activated and potentially lymph node homing. Chapter 8.2 built on this knowledge and confirmed associations between the DC phenotype and the disease and host’s BC characteristics. Chapter 9 examined the relationship of local IR with BC and its prognostic utility for CRC outcomes. Results suggested that CCR7 positive cell density at the tumor margin might be a novel prognostic biomarker to predict outcomes in patients with CRC. Overall this thesis highlights the importance of determining the BC profile and the IR of patients undergoing CRC treatment and this may lead to early identification of high-risk patients, allowing early optimisation and ultimately improving their outcomes.
Teratocephalus terrestris Butschli 1873
Creators: name: Thorne, Gerald
Publisher: name: Zenodo
Year: 1929
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Chromadorea
Rhabditida
Tetratocephalidae
Teratocephalus
Teratocephalus terrestris

description: Teratocephalus terrestris Bütschli, 1873.
This species is immediately distinguished by its small size, coarsely striated cuticle and long ﬁliform tail with its arcuate terminus. The head with its cutinous framework is an especially prominent feature.
This is one of the most widely distributed species in the western mountains but occurs only in small numbers.
Two specimens appeared in this collection. Fig. 15a—b
description: Published as part of Thorne, Gerald, 1929, Nematodes from the Summit of Long's Peak, Colorado, pp. 181 in Transactions of the American Microscopical Society 48 (2) on page 193, DOI: 10.2307/3222211, http://zenodo.org/record/10797374
Plectus cirratus Bastian 1865
Creators: name: Thorne, Gerald
Publisher: name: Zenodo
Year: 1929
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Chromadorea
Plectida
Plectidae
Plectus
Plectus cirratus

description: Plectus cirratus Bastian, 1865.
 The females of this species correspond very closely to deMan’s description of Plectus cirratus and have been identiﬁed by Dr. Cobb and Dr. Steiner as being that species. However the rare males that occur in the Western states differ greatly from the single specimen collected by deMan but the writer feels that too much importance should not be attached to these occasional, aberrant forms.
Lip region distinctly set off. Four short, stout setae. Cutinous framework about the vestibule leading to the pharynx. Amphids with sensilla pouches located near the base of the pharynx. Front ovary on the right, the rear on the left side of the body. Several setae on the tail not shown by deMan but ﬁgured by Cobb. (4).
 The tail of the male bears a small acute, elevated ventral organ just on front of the anus and anterior to this is a series of four to six ventral supplements with long tube-like extensions reaching far back into the body, passing between the testes. These organs are very similar to those of the males of Plectus granulosus. There are two testes, the anterior ends being reﬂexed a distance equal to three times the body width.
About ﬁfty females and one male in this collection. Fig. 16 a, x1000. 16b x 200.
description: Published as part of Thorne, Gerald, 1929, Nematodes from the Summit of Long's Peak, Colorado, pp. 181 in Transactions of the American Microscopical Society 48 (2) on pages 193-194, DOI: 10.2307/3222211, http://zenodo.org/record/10797374
Coracias galbula Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Coraciiformes
Coraciidae
Coracias
Coracias galbula

description: Coracias galbula [spec. nov.]
C. fulva, capite dorso remigibusque nigris.
Icterus ex aureo nigroque varius. Catesb. car. 1. p. 48. t. 48.
Habitat in America.
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 108, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
An investigation into H2 production by sorbent enhanced steam reforming of biomass
Creators: name: Clough, Peter Thomas
Publisher: name: Imperial College London
Year: 2017

description: This thesis is based around the production of H2 via a process called Sorbent Enhanced Steam Reforming (SESR), which has the potential to drastically reduce CO2 emissions from H2 production therefore abating climate change. SESR is a combination of traditional Steam Methane Reforming (SMR) and Calcium Looping (CaL, a form of Carbon Capture and Storage, CCS), whereby the CaL sorbent removes CO2 from the gas stream and drives the reactions equilibrium to produce more H2. With the application of biomass as the fuel feedstock this process has the potential to produce H2 with net-negative CO2 emissions. Two main areas of work were conducted within this thesis, namely: examining the performance of CaL sorbents and novel sorbents under industrial conditions, and the development of combined multifunctional sorbent and catalyst particles for SESR with biomass. These particles were tested within a reactor that was specifically constructed for this set of work. A detailed investigation into the effects of various parameters on the rate of limestone calcination was conducted within an atmospheric fluidised bed reactor utilising high-temperatures and CO2 partial pressures. These conditions would typically be present within a CaL/SESR calciner and thus kinetic data with this environment was determined. Further to this, a single particle model was developed to shed light on the variances observed when calcining limestone in the presence of CO2 and steam or CO2 and N2. The application of a novel synthetic sorbent was also investigated under similar calcination conditions showing the impacts on the sorbents carrying capacity caused by high-temperature CO2 sintering. A mild-pressure, high-temperature spout-fluidised bed reactor was constructed for the purpose of continuous biomass feeding for SESR. Combined particles of catalyst, sorbent and a dicalcium silicate support were tested. These combined particles were manufactured utilising a simple and inexpensive method. An enhanced H2 yield of 120 gH2/kgbiomass was produced at ~75 % purity at a stoichiometric steam to carbon ratio.
The Canada France Redshift Survey VIII: Evolution of the clustering of galaxies from z~1
Creators: name: Fevre, O. Le
name: Hudon, D.
name: Lilly, S. J.
name: Crampton, D.
name: Hammer, F.
name: Tresse, L.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have used the projected two-point correlation function, $w(r_p)$, to investigate the spatial distribution of the 591 galaxies with secure redshifts between $0 \leq z \leq 1.3$ in the five CFRS fields. The slope of the two-point correlation function for the sample as a whole is $γ=1.64\pm0.05$, very similar to the local slope, and $γ$ is therefore not strongly evolving with redshift. However, the amplitude of the correlation function decreases strongly with increasing redshift, so that at $z\approx0.6$ it is a factor of 10 lower (for $q_0=0.5$) than for a similarly-selected local galaxy population, on scales $0.1
description: 17 pages, 10 figures
Gut microbial-host metabolic interactions following bariatric surgery
Creators: name: Phetcharaburanin, Jutarop
Publisher: name: Imperial College London
Year: 2018

description: Obesity has emerged as one of the major global socioeconomic healthcare burdens at present. Bariatric surgery, especially Roux-en-Y gastric bypass (RYGB) has been largely utilised to treat individual suffering from morbid obesity. In the current study, a hyperinsulinemic obese Zucker rat model was employed to study two different weight loss approaches, RYGB and caloric restriction. To understand the host metabolic-microbial cross-talk, the two major analytical platforms including nuclear magnetic resonance (NMR) spectroscopy and 16S rRNA gene Illumina MiSeq sequencing were used in companion with multivariate statistical analysis to extract useful information from data with high complexity. The aim of this study was to 1) characterise the genotype-associated metabolic and microbial fingerprints; 2) investigate the dynamic changes in biofluids from RYGB-treated or caloric restriction-treated obese Zucker rats; 3) investigate genotype-related, RYGBinduced or caloric restriction-induced metabolic profiles and microbial shifts of the luminal contents; and 4) investigate the statistical correlation between metabolites and gut microbiota following either of the weight loss treatment. Metabolic observations of portal vein and peripheral blood plasma profiles in both obese and lean Zucker rats indicated the phenotype-independent absorption of short-chain fatty acids (SCFAs), choline and trimethylamine (TMA). However, phenotype-specific urinary host-microbial co-metabolites were revealed, suggesting distinct gut microbial metabolic activities in lean and obese Zucker rats. Furthermore, metabolic alterations induced by the RYGB surgery included the enhanced production of neuroactive metabolites, branchedchain amino acid (BCAA) catabolism, aromatic amino acid metabolism with lower lipogenesis and SCFA production. Even though caloric restriction demonstrated some health benefit-related biochemical and microbial markers, its effectiveness as a resolution for metabolic syndrome, especially type-2 diabetes mellitus has not been observed in this study in spite of the significant weight reduction.
Quantum mirrors of log Calabi-Yau surfaces and higher genus curve counting
Creators: name: Bousseau, Pierrick
Publisher: name: Imperial College London
Year: 2018

description: We present three results, at the intersection of tropical geometry, enumerative geometry, mirror symmetry and non-commutative algebra. 1. A correspondence between Block-Göttsche q-refined tropical curve counting and higher genus log Gromov-Witten theory of toric surfaces. 2. A correspondence between q-refined two-dimensional Kontsevich-Soibelman scattering diagrams and higher genus log Gromov-Witten theory of log Calabi-Yau surfaces. 3. A q-deformation of the Gross-Hacking-Keel mirror construction, producing a deformation quantization with canonical basis for the Gross-Hacking-Keel families of log Calabi-Yau surfaces. These results are logically dependent: the proof of the third result relies on the second, whose proof itself relies on the first. Nevertheless, each of them is of independent interest.
Additional file 4 of Day-to-day pattern of work and leisure time physical behaviours: are low socioeconomic status adults couch potatoes or work warriors?
Creators: name: Rasmussen, Charlotte Lund
name: Dumuid, Dorothea
name: Hron, Karel
name: Gupta, Nidhi
name: Jørgensen, Marie Birk
name: Nabe-Nielsen, Kirsten
name: Holtermann, Andreas
Publisher: name: figshare
Year: 2021
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Science Policy
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 4. Assessment of potential selection bias. Comparison of baseline characteristics between blue-collar workers excluded from and included in the study.
Split fermionic WIMPs evade direct detection
Creators: name: Ghorbani, Karim
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We consider a model with two gauge singlet fermionic WIMPs communicating with the SM particles by a singlet scalar mediator via a Higgs portal. While the light WIMP is stable and plays the role of the dark matter (DM) candidate, the heavy partner is a short-lived WIMP without contribution to the current DM relic density. Along with the coannihilation effects the heavy WIMP, acting as a mediator in $t$- and $u$-channel DM annihilation cross sections, has a significant effect in finding the viable parameter space against the direct detection constraints provided by XENON1t and LUX experiments. This is an extension to the minimal singlet fermionic DM model whose entire parameter space (except a resonance region) excluded by the latest direct detection experiments. It is found out that there are viable regions in the parameter space which evade direct detection upper bounds and respect the observed DM relic density by WMAP/Planck. We also found that the Fermi-LAT upper limits on the DM annihilation cross section into $b\bar b$ can exclude small regions of the viable parameter space which elude direct detection experiments. This model exemplifies a case within the WIMP paradigm whose DM candidate can escape direct detection experiments nontrivially. Such models are interesting to be studied in collider experiments like the LHC.
description: v2, 21 pages, discussion on indirect detection included, 6 figures added, matches version to appear in JHEP
Physical Representation-based Predicate Optimization for a Visual Analytics Database
Creators: name: Anderson, Michael R.
name: Cafarella, Michael
name: Ros, German
name: Wenisch, Thomas F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Databases (cs.DB)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Querying the content of images, video, and other non-textual data sources requires expensive content extraction methods. Modern extraction techniques are based on deep convolutional neural networks (CNNs) and can classify objects within images with astounding accuracy. Unfortunately, these methods are slow: processing a single image can take about 10 milliseconds on modern GPU-based hardware. As massive video libraries become ubiquitous, running a content-based query over millions of video frames is prohibitive. One promising approach to reduce the runtime cost of queries of visual content is to use a hierarchical model, such as a cascade, where simple cases are handled by an inexpensive classifier. Prior work has sought to design cascades that optimize the computational cost of inference by, for example, using smaller CNNs. However, we observe that there are critical factors besides the inference time that dramatically impact the overall query time. Notably, by treating the physical representation of the input image as part of our query optimization---that is, by including image transforms, such as resolution scaling or color-depth reduction, within the cascade---we can optimize data handling costs and enable drastically more efficient classifier cascades. In this paper, we propose Tahoma, which generates and evaluates many potential classifier cascades that jointly optimize the CNN architecture and input data representation. Our experiments on a subset of ImageNet show that Tahoma's input transformations speed up cascades by up to 35 times. We also find up to a 98x speedup over the ResNet50 classifier with no loss in accuracy, and a 280x speedup if some accuracy is sacrificed.
description: Camera-ready version of the paper submitted to ICDE 2019, In Proceedings of the 35th IEEE International Conference on Data Engineering (ICDE 2019)
A population study of the upper airway microbiota in Busselton, Western Australia
Creators: name: Turek, Elena Miroslavovna
Publisher: name: Imperial College London
Year: 2018

description: That the healthy lungs are sterile has been a subject of much debate. Recent studies employing culture independent techniques have focused on investigating the diseased lungs with little still being done to characterise the bacteria which sustain the healthy lung ecosystem. The Busselton Health Study (BHS) is a long running epidemiological study that focuses on defining and characterizing common diseases. Recently addition of oropharyngeal (throat) swabs to the BHS sample collection has occurred. The main aims of this thesis therefore were to assess the upper airway microbiome in healthy individuals and evaluate the changes to the bacterial composition under disease and environmental stress (smoking). A random population sample of 529 participants was studied consisting of 60 current-smokers, 216 ex-smokers and 253 never-smokers, out of which there were 77 asthmatics, 46 subjects with gastro-esophageal reflux disease (GERD), 19 patients with diabetes and 387 healthy individuals. Bacterial DNA was extracted from all swabs and 16S rRNA gene qPCR and next generation sequencing performed. The results indicated that airways of healthy individuals contain a diverse collection of bacteria. Through application of weighted correlation network analysis (WCNA), these bacteria were seen to work together in tight networks. As the BHS cohort is a general population sample no severe disease phenotypes were noted, hence limited changes in bacterial community structure of participants with disease compared to healthy participants were seen. Smoke exposure however had a profound effect on the microbiome, with current-smokers exhibiting a significant drop in bacterial burden, diversity and a change in community structure. There was depletion of Haemophillus spp. and Neisseria spp. in current-smokers, and a strong positive relationship with streptococci. Notably within the first few years after cessation of smoking the bacterial community of the airways appears to regenerate with an increase in community diversity. A streptococci specific quantification assay and sequencing method (based on the map gene) was established in order to dissect further the relationship at the species level of the genus Streptococcus with current-smoking. This identified an increased dominance of Streptococcus salivarius (an opportunistic pathogen) in current-smokers. In conclusion, a healthy airway microbiome contains a rich community of microorganisms. This is significantly impacted by smoking, leading to loss of diversity and a community dominated by streptococci. Diversity however can be restored if smoking cessation occurs.
Plectus parvus Bastian 1865
Creators: name: Thorne, Gerald
Publisher: name: Zenodo
Year: 1929
Subjects: Biodiversity
Taxonomy
Animalia
Nematoda
Chromadorea
Plectida
Plectidae
Plectus
Plectus parvus

description: Plectus parvus Bastian, 1865.
The ﬁgures and measurements are almost sufficient to describe this tiny species. The striae are ﬁne and are interrupted on the lateral ﬁelds by two distinct wings. The front ovary is on the right, the rear on the left, side of the body. The eggs are huge and at times the ovaries are crowded until the reﬂexed portion passes the vulva. Fig. 18a-b.
This active little species is one of the most common nemas found in the mountain soils. About twenty specimens in this collection.
description: Published as part of Thorne, Gerald, 1929, Nematodes from the Summit of Long's Peak, Colorado, pp. 181 in Transactions of the American Microscopical Society 48 (2) on page 195, DOI: 10.2307/3222211, http://zenodo.org/record/10797374
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 191
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 191, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 191, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Spiral Structure In The Circum-nuclear Disk At The Center Of The Galaxy NGC 4258
Creators: name: Maoz, Eyal
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations of line emission from water masers near the center of the galaxy NGC 4258 have recently provided compelling evidence for rotating disk of gas, viewed nearly edge-on, surrounding a massive black hole (Miyoshi etal. 1995). We show that the disk is only marginally stable to radial perturbations - a stability regime where weak non-axisymmetric disturbances tend to grow via the swing amplification effect, forming a ragged, multi-armed spiral pattern similar to that observed in Sc galaxies. This suggests a natural explanation for the apparent clustering of the high-velocity emission sources into several distinct clumps, and for the observed regularity in the distance intervals between them. The clumps of sources appear at the intersections of the spiral arms and the radial line of longest coherent gain path, and are thus spaced apart at the characteristic crest-to-crest radial distance between the arms. This interpretation implies an H_2 density and disk thickness of about 1.8x10^{10} (Q/1.6)^{-1} cm^{-3}, and 0.003(Q/1.6) pc at a radius of 0.2 pc, respectively, where the local value of the stability parameter is 1.2 < Q < 2.
description: To Appear in ApJ (Letters), 10 pages, 1 figure, uuencoded + compressed postscript
Corticosteroid insensitivity in airways disease
Creators: name: Macedo, Patricia
Publisher: name: Imperial College London
Year: 2016

description: Corticosteroids (CS) are the most widely used and effective anti-inflammatory agents. In severe asthma, despite high doses of CS, patients remain symptomatic, whereas in COPD, CS fail to halt progression of the disease, highlighting the need for alternative anti-inflammatory agents. The hypothesis investigated in this thesis was that inflammation in severe asthma and COPD was less responsive to inhibition by corticosteroids. In COPD, cells of the monocyte-macrophage lineage did not demonstrate corticosteroid insensitivity compared to smoking and non-smoking controls in response to LPS. In response to IFNγ stimulation, CXCL9 release from peripheral blood mononuclear cells (PBMC) from COPD patients was significantly higher than from controls. JAK-STAT inhibitors significantly reduced the secretion of CXCR3 chemokines compared to dexamethasone. PBMC from subjects with severe asthma not on regular prednisolone exhibited corticosteroid insensitivity compared to non-severe asthmatics and severe asthmatics on regular prednisolone in terms of suppression of IL-6 release. There was a very variable response to a 2-week course of prednisolone amongst patients with severe asthma. 5 p38 MAPK inhibitors were tested in alveolar macrophages, monocyte-derived macrophages and PBMC, and they suppressed release of inflammatory cytokines from COPD, severe asthma and controls. Examination of bronchial biopsies revealed that severe asthmatic patients had significantly increased basement membrane thickness and smooth muscle area compared to non-severe asthma. There was a significant negative correlation between airways hyper-responsiveness and the SBM thickness, suggesting that the extracellular matrix may influence airway contractility. Inhibition of the p38 and JAK-STAT pathways had a greater ability to suppress induced cytokine release than dexamethasone in inflammatory cells from COPD and asthma. A 2-week course of prednisolone improved asthma control and quality of life scores in patients with severe asthma. CS use does not prevent airway wall remodelling in severe asthma. Together, these data highlight the need for alternative anti-inflammatory agents.
Ricci Soliton and Conformal Ricci Soliton in Lorentzian β -Kenmotsu Manifold
Creators: name: Tamalika Dutta
name: Arindam Bhattacharyya
Publisher: name: figshare
Year: 2018
Subjects: subject: 10104 Combinatorics and Discrete Mathematics (excl. Physical Combinatorics)
subject: FOS: Mathematics

description: In this paper we have studied quasi conformal curvature tensor, Ricci tensor, projective curvature tensor, pseudo projective curvature tensor in Lorentzian β -Kenmotsu manifold admitting Ricci soliton and conformal Ricci soliton.
Multivariable Iterative Learning Control Design Procedures: from Decentralized to Centralized, Illustrated on an Industrial Printer
Creators: name: Blanken, Lennart
name: Oomen, Tom
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Iterative Learning Control (ILC) enables high control performance through learning from measured data, using only limited model knowledge in the form of a nominal parametric model. Robust stability requires robustness to modeling errors, often due to deliberate undermodeling. The aim of this paper is to develop a range of approaches for multivariable ILC, where specific attention is given to addressing interaction. The proposed methods either address the interaction in the nominal model, or as uncertainty, i.e., through robust stability. The result is a range of techniques, including the use of the structured singular value (SSV) and Gershgorin bounds, that provide a different trade-off between modeling requirements, i.e., modeling effort and cost, and achievable performance. This allows control engineers to select the approach that fits the modeling budget and control requirements. This trade-off is demonstrated in a case study on an industrial flatbed printer.
Resonant feedback for axion and hidden sector dark matter searches
Creators: name: Daw, Edward J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Resonant feedback circuits are proposed as an alternative to normal modes of conducting wall cavities or lumped circuits in searches for hidden sector particles. The proposed method offers several potential advantages over the most sensitive axion searches to date, that employ cavity resonators, including coverage of a wider range of axion masses, the ability to probe many axion masses simultaneously, and the elimination of experimentally troublesome mechanical tuning rod mechanisms. After an outline of the proposed method, we present a noise budget for a straw-man experiment configuration. We show that the proposed experiment has the potential to probe the axion mass range 2-40 micro-eV with 38 days of integration time. Other existing and proposed resonant searches for hidden sector particles may also benefit from this approach to detection.
description: 10 pages, 6 figures
Structure and kinematics of the peculiar galaxy NGC 128
Creators: name: D'Onofrio, M.
name: Capaccioli, M.
name: Merluzzi, P.
name: Zaggia, S.
name: Boulesteix, J.
name: .
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This is a multiband photometric and spectroscopic study of the peculiar S0 galaxy NGC128. We present results from broad (B and R) and narrow band optical CCD photometry, near (NIR) and far (FIR) infrared observations, long slit spectroscopy, and Fabry-Perot interferometry (CIGALE). The peculiar peanut shape morphology of the galaxy is observed both at optical and near-infrared wavelengths. The stellar disk is thick and distorted (arc-bended), with a color asymmetry along the major axis due to the presence of a large amount of dust, estimated through NIR and FIR data of ~6x10^6 M_sun, in the region of interaction with the companion galaxy NGC127. The color maps are nearly uniform over the whole galaxy, but for the major axis asymmetry, and a small gradient toward the center indicating the presence of a redder disk-like component. The H_alpha image indeed reveals the existence of a tilted gaseous ``disk'' around the center, oriented with the major axis toward the companion galaxy NGC127. Long slit and CIGALE data confirm the presence of gas in a disk-like component counter-rotating and inclined approximately of 50 deg. to the line of sight. The mass of the gas disk in the inner region is ~2.7x10^4 M_sun. The stellar velocity field is cylindrical up to the last measured points of the derived rotation curves, while the velocity dispersion profiles are typical for an S0 galaxy, but for an extended constant behaviour along the minor axis.
description: accepted for pubblication in A&A Suppl
Additional file 1 of Receipt of medications for opioid use disorder among youth engaged in primary care: data from 6 health systems
Creators: name: Bagley, Sarah M.
name: Chavez, Laura
name: Braciszewski, Jordan M.
name: Akolsile, Mary
name: Boudreau, Denise M.
name: Lapham, Gwen
name: Campbell, Cynthia I.
name: Bart, Gavin
name: Yarborough, Bobbi Jo H.
name: Samet, Jeffrey H.
name: Saxon, Andrew J.
name: Rossom, Rebecca C.
name: Binswanger, Ingrid A.
name: Murphy, Mark T.
name: Glass, Joseph E.
name: Bradley, Katharine A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Table S1. International Classification of Diseases, Ninth and Tenth Revision, Clinical Modification codes used to define Opioid Use Disorder (OUD).
HST Observations of the Luminous IRAS Source FSC10214+4724: A Gravitationally Lensed Infrared Quasar
Creators: name: Eisenhardt, Peter R.
name: Armus, Lee
name: Hogg, David W.
name: Soifer, B. T.
name: Neugebauer, G.
name: Werner, Michael W.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an image of the redshift 2.3 IRAS source FSC10214+4724 at 0.8 microns obtained with the HST WFPC2 Planetary Camera. The source appears as an unresolved (< 0.06") arc 0.7" long, with significant substructure along its length. The arc is centered near an elliptical galaxy 1.18" to the north. An unresolved component 100 times fainter than the arc is clearly detected on the opposite side of this galaxy. The most straightforward interpretation is that FSC 10214+4724 is gravitationally lensed by the foreground elliptical galaxy, with the faint component a counterimage of the IRAS source. The brightness of the arc in the HST image is then magnified by ~100 and the intrinsic source diameter is ~0.01" (80 pc) at 0.25 microns rest wavelength. The bolometric luminosity is probably amplified by a smaller factor (~30), yielding an intrinsic luminosity ~2E13 solar luminosities. A detailed lensing model is presented which reproduces the observed morphology and relative flux of the arc and counterimage, and correctly predicts the position angle of the lensing galaxy. The model also predicts reasonable values for the velocity dispersion, mass, and mass-to-light ratio of the lensing galaxy. A redshift for the lensing galaxy of ~0.9 is consistent with the measured surface brightness profile from the image, as well as with the galaxy's SED.
description: 27 pages, 7 PS fig, uses aastex macros, to appear ApJ 10 April 1996
title: ADCO, Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Cart. 172 (11 H 69), 115 folios, f. 0188
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0188, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0188, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
A small-world search for quantum speedup: How small-world interactions can lead to improved quantum annealer designs
Creators: name: Katzgraber, Helmut G.
name: Novotny, M. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: There are many factors that influence the design of quantum annealing processing units. Here we address the issue of improving quantum annealing processing unit designs from the point of view of the critical behavior of spin glasses. It has been argued [Phys. Rev. X 4, 021008 (2014)] that among the most difficult Ising spin-glass ground-state problems are those related to lattices which exhibit a finite-temperature spin-glass transition. Here, we show that adding small-world couplers between qubits (spins) to the native quasi-planar quantum processing unit graph results in a topology where a disordered Ising system can undergo a finite-temperature spin-glass transition, even when an Ising spin glass on the quasi-planar native graph does not display a transition into a glassy phase at any finite temperature. To ensure that these systems can be engineered with current fabrication techniques, using large-scale Monte Carlo simulations we demonstrate that highly-constrained systems restricted to a few fabrication layers and with fixed coupler angles can also exhibit a finite-temperature spin-glass transition. This indicates that these systems might be mean-field-like, which also means that embedding highly-nonplanar problems might be simplified when compared to the underlying native topology. Our results are illustrated using the quasi-planar Chimera topology currently used in the D-Wave Systems Inc. quantum annealing machines, as well as standard two-dimensional square lattices. The presented approach can be generalized to other topologies.
description: 12 pages, 13 figures, interactive 3D versions of some figures in the ancillary material
Coracias aurea Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Coraciiformes
Coraciidae
Coracias
Coracias aurea

description: Coracias aurea [spec. nov.]
C. flavo-fulva, gula tectricibus primariis extremitateque rectricum nigris.
Paradisea flavo-fulva. Mus. Ad. Fr. 1. p. 15.
Paradisea aurea. Edw. Av. 112. t. 112.
Habitat in Asia.
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 108, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Semifull Line (Block) Signed Graphs
Creators: name: V. Lokesha
name: P. S. Hemavathi
name: S. Vijay
Publisher: name: figshare
Year: 2018
Subjects: subject: 10104 Combinatorics and Discrete Mathematics (excl. Physical Combinatorics)
subject: FOS: Mathematics

description: In this paper we introduced the new notions semifull signed graph and semifull line (block) signed graph of a signed graph and its properties are obtained. Also, we obtained the structural characterizations of these notions. Further, we presented some switching equivalent characterizations.
A magnetic model for acoustic modes in roAp stars
Creators: name: Zita, E. J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The mechanism for excitation of p-modes in rapidly oscillating, peculiar A (roAp, or cool chemically peculiar, CP) stars is unknown. Observations strongly suggest that acoustic modes in roAp stars are causally linked to the stars' magnetic field. We propose that small fluctuations in the shape of the mean magnetic field drive magnetosonic waves, which are observed as p-modes in these stars. The dynamic edge region of roAp stars is a force-free spherical shell. When strongly coupled to the magnetic field, a force-free plasma can oscillate about a minimum in its mean magnetic energy. We describe the stable eigenmodes for this energy minimum in a spherical shell with an open boundary. The wavenumbers, frequencies, and energies of resulting oscillations are consistent with observations of p-modes in roAp stars. Our magnetic model for p-mode oscillations in stars does not invoke convection or opacity mechanisms. We also suggest the possibility of a nonlinear dynamo for such magnetic stars, which lack the convection needed for the usual (-( dynamo.
Path Related n-Cap Cordial Graphs
Creators: name: A. Nellai Murugan
name: P. Iyadurai Selvaraj
Publisher: name: figshare
Year: 2018
Subjects: subject: 10104 Combinatorics and Discrete Mathematics (excl. Physical Combinatorics)
subject: FOS: Mathematics

description: A graph G is a finite non-empty set of objects called vertices together with a set of unordered pairs of distinct vertices of G which is called edges.