cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Hyalopomatus biformis
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Hyalopomatus
Hyalopomatus biformis

description: Hyalopomatus biformis (Hartman, 1960)
(Figures 5E–H)
 Vermiliopsis biformis Hartman, 1960: 164. pl. 18, figs. 1–7. Type locality: Santa Catalina Basin, California, USA.— Hartman, 1969: 777–778, figs. 1–7, southern California, USA.
 Hyalopomatus biformis.— Zibrowius, 1971b: 1374 (transferred to the genus Hyalopomatus).
 Material examined. Twelve specimens: Alaska (USA), LACM-AHF N10714 (approx. 56º15’N, 158º09’W, Castle Bay, off Chignik Bay, Alaska King Crab Investigation, sta. D3–41, 38– 95 m, June 24, 1941, as? Apomatus sp.). California (USA), LACM-AHF 180, type (33º26’21”N, 118º52’41”W, Santa Catalina Basin, 13.6 km of S. Light. Santa Barbara Island, sta. 2130, on dead shells of brachiopods Lacqueus, mud, 1,280 m, June 26, 1952, as Vermiliopsis biformis); LACM-AHF s.n., 9 spec. (33º24’15–30”N, 118º21’33– 35”W, 0.5 km from Long Point Light, Santa Catalina Island, Velero IV, sta. 2128, sand, on dead Lacqueus shells, 77–122 m, June 25, 1952); MBL-SD s.n. (approx. 32º40’N, 117º25’W, off San Diego, RV, sta. B– 13, 116 m, Oct. 4, 2001).
 Diagnosis. Tube white, long, slender and sinuous, with longitudinal ridge, some specimens with peristomes. Opercular peduncle smooth, sometimes annulated (Fig. 5H). Operculum sub-oval to rounded (Figs 5F, H). Six thoracic chaetigers (Fig. 5E). Collar with chaetae (more or less) fin-and-blade, with basal denticulate expansion and smooth limba (Fig. 5G). “ Apomatus ” chaetae absent. Thoracic uncini with multiple rows of teeth and gouged peg.
 Habitat. Depth: 38– 1,280 m. In shelf, slope and canyon depths. On Lacqueus shells (brachiopods).
 Distribution. North-eastern Pacific. Alaska to California, USA (Hartman 1969).
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on page 21
The Wavelet Galerkin Operator
Creators: name: Dutkay, Dorin Ervin
Publisher: name: arXiv
Year: 2003
Subjects: subject: Operator Algebras (math.OA)
subject: Spectral Theory (math.SP)
subject: FOS: Mathematics

description: In connection to wavelet theory, we describe the peripheral spectrum of the transfer operator. The solution involves the analysis of certain representations of the algebra generated by two unitaries $U$ and $T$ that satisfy the commutation relation $UTU^{-1}=T^N$.
Supervised Domain Adaptation: A Graph Embedding Perspective and a Rectified Experimental Protocol
Creators: name: Hedegaard, Lukas
name: Sheikh-Omar, Omar Ali
name: Iosifidis, Alexandros
Publisher: name: arXiv
Year: 2020
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Domain Adaptation is the process of alleviating distribution gaps between data from different domains. In this paper, we show that Domain Adaptation methods using pair-wise relationships between source and target domain data can be formulated as a Graph Embedding in which the domain labels are incorporated into the structure of the intrinsic and penalty graphs. Specifically, we analyse the loss functions of three existing state-of-the-art Supervised Domain Adaptation methods and demonstrate that they perform Graph Embedding. Moreover, we highlight some generalisation and reproducibility issues related to the experimental setup commonly used to demonstrate the few-shot learning capabilities of these methods. To assess and compare Supervised Domain Adaptation methods accurately, we propose a rectified evaluation protocol, and report updated benchmarks on the standard datasets Office31 (Amazon, DSLR, and Webcam), Digits (MNIST, USPS, SVHN, and MNIST-M) and VisDA (Synthetic, Real).
description: 13 pages, 7 figures, 6 tables
Protis pacifica Moore 1923
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Protis
Protis pacifica

description: Protis pacifica Moore, 1923
(Figures 8B–C)
 Protis pacifica Moore, 1923: 253–254. Type locality: Off Santa Rosa Island, California, USA.
 Protis pacifica.— Hartman, 1969: 765–766, figs. 1–3, Southern California.
 Protis pacifica Zibrowius, 1969: 17–18, figs. 7a–e, (revision of the species).
 Material examined. Fifteen specimens: California (USA), LACM-AHF s.n., 4 spec. (33º29–26’N, 118º19– 21’W, San Pedro Channel, 8.8 km off Luria Point, Santa Catalina Island, Velero IV, sta. 1613, spec. on dorsal valve of Cyclopecten, 730–790 m, Oct. 2, 1948); LACM-AHF s.n., 11 spec. (33º486”N, 118º30’39”W, 10 km from Redondo Beach pier, Velero IV sta. 2151, 0.5 cuft grab, large burrow in packed clay, 530 m, Sept. 26, 1952).
 Diagnosis. Tube somewhat rugged, with one longitudinal ridge and two shallow grooves or ridges laterally. Operculum absent. Collar with fin-and-blade chaetae, with several teeth in middle section, with space between denticulate base and limb (Figs 8B–C). Thoracic membrane wide, forming an apron across abdomen.
 Habitat. Depth: 530–790 m. Slope, canyons. On Cyclopecten shells.
 Distribution. Only known from southern California (USA) (Zibrowius 1969).
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on page 35
Quantum group covariant (anti)symmetrizers, epsilon-tensors, vielbein, Hodge map and Laplacian
Creators: name: Fiore, Gaetano
Publisher: name: arXiv
Year: 2004
Subjects: subject: Quantum Algebra (math.QA)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 81R50, 17B37

description: GL_q(N)- and SO_q(N)-covariant deformations of the completely symmetric/antisymmetric projectors with an arbitrary number of indices are explicitly constructed as polynomials in the braid matrices. The precise relation between the completely antisymmetric projectors and the completely antisymmetric tensor is determined. Adopting the GL_q(N)- and SO_q(N)-covariant differential calculi on the corresponding quantum group covariant noncommutative spaces C_q^N, R_q^N, we introduce a generalized notion of vielbein basis (or "frame"), based on differential-operator-valued 1-forms. We then give a thorough definition of a SO_q(N)-covariant R_q^N-bilinear Hodge map acting on the bimodule of differential forms on R_q^N, introduce the exterior coderivative and show that the Laplacian acts on differential forms exactly as in the undeformed case, namely it acts on each component as it does on functions.
description: latex file, 24 pages. Some citations added and misprints corrected. Final version to appear in J. Phys. A Math. and Gen
Serpula watsoni Willey 1905
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Serpula
Serpula watsoni

description: Serpula watsoni Willey, 1905
(Figures 11L–M)
 Serpula watsoni Willey, 1905: 317, pl. 7, fig. 187, pl. 8, fig. 6. Type locality: Trincomalee, Sri Lanka (Ceylon).
 Serpula watsoni.— Imajima, 1977: 91–92, figs. 2a–j, Tsurihama (Japan).
 Serpula watsoni.— Imajima and ten Hove, 1984: 38–39, fig. 2, Truk, Ponape and Majuro Islands, Amoy (southern China Sea) and Australia.
 Material examined. Two specimens: Hawaii (USA), UMAR-Poly 96, 2 spec. (Hawaii inter-island cargo barge, HF–023, hull fouling community roughly two years old; barge only operates in Hawaii, coll. SG).
 Diagnosis. Tube white, rough, thick-walled, with five longitudinal ridges, lacks peristomes or alveoli. Opercular peduncle smooth, white, with marked constriction. Operculum symmetrical, deep; funnel with 37– 47 radii with blunt tips (Figs 11L–M). Collar with bayonet chaetae, with five blunt-short teeth, distal blade smooth.
 Habitat. Depth: intertidal to few meters. Fouling species.
 Distribution. Indo-Pacific. Sri Lanka, South China Sea, southern Japan, Australia, Micronesia, Hawaii (Imajima & ten Hove 1984).
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on pages 46-48
A Concurrent Fuzzy-Neural Network Approach for Decision Support Systems
Creators: name: Tran, Cong
name: Abraham, Ajith
name: Jain, Lakhmi
Publisher: name: arXiv
Year: 2004
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences
subject: I.2.0

description: Decision-making is a process of choosing among alternative courses of action for solving complicated problems where multi-criteria objectives are involved. The past few years have witnessed a growing recognition of Soft Computing technologies that underlie the conception, design and utilization of intelligent systems. Several works have been done where engineers and scientists have applied intelligent techniques and heuristics to obtain optimal decisions from imprecise information. In this paper, we present a concurrent fuzzy-neural network approach combining unsupervised and supervised learning techniques to develop the Tactical Air Combat Decision Support System (TACDSS). Experiment results clearly demonstrate the efficiency of the proposed technique.
Additional file 3 of The round goby genome provides insights into mechanisms that may facilitate biological invasions
Creators: name: Adrian-Kalchhauser, Irene
name: Blomberg, Anders
name: Larsson, Tomas
name: Musilova, Zuzana
name: Peart, Claire
name: Pippel, Martin
name: Solbakken, Monica
name: Suurväli, Jaanus
name: Walser, Jean-Claude
name: Wilson, Joanna
name: Rosenblad, Magnus Alm
name: Demian Burguera
name: Gutnik, Silvia
name: Michiels, Nico
name: Töpel, Mats
name: Pankov, Kirill
name: Schloissnig, Siegfried
name: Winkler, Sylke
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Evolutionary Biology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Plant Biology

description: Figure S2. Phylogenetic tree of opsins constructed with individual exons.
A high-precision abundance analysis of the nuclear benchmark star HD 20
Creators: name: Hanke, Michael
name: Hansen, Camilla Juul
name: Ludwig, Hans-Günter
name: Cristallo, Sergio
name: McWilliam, Andrew
name: Grebel, Eva K.
name: Piersanti, Luciano
Publisher: name: arXiv
Year: 2020
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present our chemical abundance investigation of the metal-poor ([Fe/H]=-1.60 dex), r-process-enriched ([Eu/Fe]=0.73 dex) halo star HD 20 using novel and archival high-resolution spectra at outstanding signal-to-noise ratios. By combining one of the first asteroseismic gravity measurements in the metal-poor regime from a TESS light curve with non-LTE analyses of iron lines, we derive a set of highly accurate and precise stellar parameters. These allow us to delineate a chemical pattern comprised of solid detections of 48 elements, including 28 neutron-capture elements, which establishes HD 20 among the few benchmark stars that have almost complete patterns with low systematic dependencies on the stellar parameters. Our light-element (Z<30) abundances are representative of other, similarly metal-poor stars in the Galactic halo with contributions from core-collapse supernovae of type II. A comparison to the scaled solar r-pattern shows that the lighter neutron-capture elements (37
description: 23 pages (+10 pages appendix), 27 figures, 8 tables, revised version resubmitted to A&A
A comparison of some new and old robust ridge regression estimators
Creators: name: Ali, Sajid
name: Khan, Himmad
name: Shah, Ismail
name: Butt, Muhammad Moeen
name: Suhail, Muhammad
Publisher: name: Taylor & Francis
Year: 2019
Subjects: Space Science
Medicine
Molecular Biology
Environmental Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Ridge regression is used to circumvent the problem of multicollinearity among predictors and many estimators for ridge parameter k are available in the literature. However, if the level of collinearity among predictors is high, the existing estimators also have high mean square errors (MSE). In this paper, we consider some existing and propose new estimators for the estimation of ridge parameter k. Extensive Monte Carlo simulations as well as a real-life example are used to evaluate the performance of proposed estimators based on the MSE criterion. The results show the superiority of our proposed estimators compared to the existing estimators.
Orchesella bifasciata Nicolet 1842
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Orchesellidae
Orchesella
Orchesella bifasciata

description: Orchesella bifasciata Nicolet, 1842 *
Orchesella bifasciata Nicolet, 1842: 80.
DISTRIBUTION. — France. Bourlet 1845.
Corse. Poinsot-Balaguer 1978.
Savoie. Forêtde Mâcot-la-Plagne, 950- 2150 m (Loranger etal. 2001).
ÉCOLOGIE. — Loranger etal. 2001 (sol acide).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 385, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
All-optical frequency resolved optical gating for isolated attosecond pulse reconstruction
Creators: name: Yang, Zhen
name: Cao, Wei
name: Chen, Xi
name: Zhang, Jie
name: Mo, Yunlong
name: Xu, Huiyao
name: Mi, Kang
name: Zhang, Qingbin
name: Lan, Pengfei
name: Lu, Peixiang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We demonstrate an all-optical approach for precise characterization of attosecond extreme ultraviolet pulses. Isolated attosecond pulse is produced from high order harmonics using intense driving pulse with proper gating technique. When a weak field is synchronized with the driver, it perturbs the harmonics generation process via altering the accumulated phase of the electron trajectories. The perturbed harmonic spectrum can be formulated as a convolution of the unperturbed dipole and a phase gate, implying the validity of complete reconstruction of isolated attosecond pulses using conventional frequency resolved optical gating method. This in situ measurement avoids the central momentum approximation assumed in the widely used attosecond streaking measurement, providing a simple and reliable metrology for isolated attosecond pulse.
description: 5 pages, 4 figures
The local trace function of shift invariant subspaces
Creators: name: Dutkay, Dorin Ervin
Publisher: name: arXiv
Year: 2003
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics

description: We define the local trace function for subspaces of $\ltworn$ which are invariant under integer translation. Our trace function contains the dimension function and the spectral function defined by Bownik and Rzeszotnik and completely characterizes the given translation invariant subspace. It has properties such as positivity, additivity, monotony and some form of continuity. It behaves nicely under dilations and modulations. We use the local trace function to deduce, using short and simple arguments, some fundamental facts about wavelets such as the characterizing equations, the equality between the dimension function and the multiplicity function and some new relations between scaling functions and wavelets.
Additional file 4 of The round goby genome provides insights into mechanisms that may facilitate biological invasions
Creators: name: Adrian-Kalchhauser, Irene
name: Blomberg, Anders
name: Larsson, Tomas
name: Musilova, Zuzana
name: Peart, Claire
name: Pippel, Martin
name: Solbakken, Monica
name: Suurväli, Jaanus
name: Walser, Jean-Claude
name: Wilson, Joanna
name: Rosenblad, Magnus Alm
name: Demian Burguera
name: Gutnik, Silvia
name: Michiels, Nico
name: Töpel, Mats
name: Pankov, Kirill
name: Schloissnig, Siegfried
name: Winkler, Sylke
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Molecular Biology
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology
subject: Computational Biology

description: Figure S3. Hylogenetic tree of olfactory receptors, with the brances that are depicted collapsed in Fig. 3 expanded.
Kinematic Masses of Super Star Clusters in M82 from High-Resolution Near-Infrared Spectroscopy
Creators: name: McCrady, Nate
name: Gilbert, Andrea M.
name: Graham, James R.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using high-resolution (R~22,000) near-infrared (1.51 -- 1.75 microns) spectra from Keck Observatory, we measure the kinematic masses of two super star clusters in M82. Cross-correlation of the spectra with template spectra of cool evolved stars gives stellar velocity dispersions of sigma_r=15.9 +/- 0.8 km/s for MGG-9 and sigma_r=11.4 +/- 0.8 km/s for MGG-11. The cluster spectra are dominated by the light of red supergiants, and correlate most closely with template supergiants of spectral types M0 and M4.5. We fit King models to the observed profiles of the clusters in archival HST/NICMOS images to measure the half-light radii. Applying the virial theorem, we determine masses of 1.5 +/- 0.3 x 10^6 M_sun for MGG-9 and 3.5 +/- 0.7 x 10^5 M_sun for MGG-11. Population synthesis modelling suggests that MGG-9 is consistent with a standard initial mass function, whereas MGG-11 appears to be deficient in low-mass stars relative to a standard IMF. There is, however, evidence of mass segregation in the clusters, in which case the virial mass estimates would represent lower limits.
description: 16 pages, 8 figures; ApJ, in press
Spirobranchus spinosus Moore 1923
Creators: name: Bastida-Zavala, J. Rolando
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Sabellida
Serpulidae
Spirobranchus
Spirobranchus spinosus

description: Spirobranchus spinosus Moore, 1923
(Figures 13B–C)
 Spirobranchus spinosus Moore, 1923: 248–250, pl. 18, fig. 47. Type locality: Off Santa Barbara Island, California, USA. Spirobranchus spinosus.— Hartman, 1969: 775–776, figs. 1–5, Southern California, USA.
 Material examined. More than 20 specimens: California (Mexico), USNM 17109, type (approx. 33º22– 24’N, 119º39–44’W, off Santa Barbara, R / V Albatross, sta. 4417, 68 m, April 12, 1904). Baja California (Mexico), ECOSUR s.n., UMAR-Poly 104, 20+ spec. (approx. 31º53–54’N, 116º41–43’W, Villas las Rosas, near Sauzal, low tide, rock plain with seagrass Phylospadix, molluscs, 1 m, March 6, 2004, coll. SISV, NEV, MATH & PSS).
 Diagnosis. Tube bluish with prominent longitudinal ridge, lacking peristomes or alveoli. Opercular peduncle with wide wings. Operculum calcareous, circular or pear-shaped; plate with five short thin spines (one lost, noted by the fracture mark on plate), arising from middle of opercular plate, with 5–8 spinules on each (Figs 13B–C). Radioles arranged in spire with up to four whorls. Thoracic membrane extends to last thoracic chaetiger, forming short ventral apron. Collar with “ Spirobranchus ” chaetae coarsely serrated in subapical section.
 Measurements. TL=20.5 mm, THL=3.8 mm, THW=2.2 mm, POL=6.7 mm, OL=2.3 mm, OW=2.2 mm, SL=1.5 mm.
 Habitat. Depth: 1–68 m. On rocks with seagrass Phylospadix.
 Distribution. Temperate Eastern Pacific. California (USA) to Baja California (Mexico) (Hartman 1969).
 Taxonomic remarks. Spirobranchus spinosus was considered a part of the S. giganteus complex (cf. ten Hove 1970), but elevated to full species by Fiege and ten Hove (1999: 363). The specimens revised here, with five to seven spines (Figs 13B–C), is different from the other Spirobranchus species recorded from the Eastern Pacific (S. cf. gaymardi, S. incrassatus) and more similar to S. dendropoma (Gulf of Mexico) or S. tetraceros (Indo-Pacific) (cf. ten Hove 1970; Bastida-Zavala & Salazar-Vallejo 2001). The measurements also indicate that this is a smaller species of Spirobranchus, from different ecological conditions (temperate waters).
 Remarks. Gotshall (1994: 42) recorded to S. spinosus with pinkish tubes.
description: Published as part of Bastida-Zavala, J. Rolando, 2008, Serpulids (Annelida: Polychaeta) from the Eastern Pacific, including a brief mention of Hawaiian serpulids, pp. 1-61 in Zootaxa 1722 on page 51
A multi-frequency ALMA characterization of substructures in the GM Aur protoplanetary disk
Creators: name: Huang, Jane
name: Andrews, Sean M.
name: Dullemond, Cornelis P.
name: Oberg, Karin I.
name: Qi, Chunhua
name: Zhu, Zhaohuan
name: Birnstiel, Tilman
name: Carpenter, John M.
name: Isella, Andrea
name: Macias, Enrique
name: McClure, Melissa K.
name: Perez, Laura M.
name: Teague, Richard
name: Wilner, David J.
name: Zhang, Shangjia
Publisher: name: arXiv
Year: 2020
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The protoplanetary disk around the T Tauri star GM Aur was one of the first hypothesized to be in the midst of being cleared out by a forming planet. As a result, GM Aur has had an outsized influence on our understanding of disk structure and evolution. We present 1.1 and 2.1 mm ALMA continuum observations of the GM Aur disk at a resolution of ~50 mas (~8 au), as well as HCO$^+$ $J=3-2$ observations at a resolution of ~100 mas. The dust continuum shows at least three rings atop faint, extended emission. Unresolved emission is detected at the center of the disk cavity at both wavelengths, likely due to a combination of dust and free-free emission. Compared to the 1.1 mm image, the 2.1 mm image shows a more pronounced "shoulder" near R~40 au, highlighting the utility of longer-wavelength observations for characterizing disk substructures. The spectral index $α$ features strong radial variations, with minima near the emission peaks and maxima near the gaps. While low spectral indices have often been ascribed to grain growth and dust trapping, the optical depth of GM Aur's inner two emission rings renders their dust properties ambiguous. The gaps and outer disk ($R>100$ au) are optically thin at both wavelengths. Meanwhile, the HCO$^+$ emission indicates that the gas cavity is more compact than the dust cavity traced by the millimeter continuum, similar to other disks traditionally classified as "transitional."
description: 31 pages, 15 figures, accepted by ApJ. Self-calibration and imaging scripts, images, and self-calibrated visibilities available at https://zenodo.org/record/3628656#.XjEXyRNKiYV
Pebble drift and planetesimal formation in protoplanetary discs with embedded planets
Creators: name: Eriksson, Linn E. J.
name: Johansen, Anders
name: Liu, Beibei
Publisher: name: arXiv
Year: 2020
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Nearly-axisymmetric gaps and rings are commonly observed in protoplanetary discs. The leading theory regarding the origin of these patterns is that they are due to dust trapping at the edges of gas gaps induced by the gravitational torques from embedded planets. If the concentration of solids at the gap edges becomes high enough, it could potentially result in planetesimal formation by the streaming instability. We test this hypothesis by performing global 1-D simulations of dust evolution and planetesimal formation in a protoplanetary disc that is perturbed by multiple planets. We explore different combinations of particle sizes, disc parameters, and planetary masses, and find that planetesimals form in all these cases. We also compare the spatial distribution of pebbles from our simulations with protoplanetary disc observations. Planets larger than one pebble isolation mass catch drifting pebbles efficiently at the edge of their gas gaps, and depending on the efficiency of planetesimal formation at the gap edges, the protoplanetary disc transforms within a few 100,000 years to either a transition disc with a large inner hole devoid of dust or to a disc with narrow bright rings. For simulations with planetary masses lower than the pebble isolation mass, the outcome is a disc with a series of weak ring patterns but no strong depletion between the rings. Lowering the pebble size artificially to 100 micrometer-sized "silt", we find that regions between planets get depleted of their pebble mass on a longer time-scale of up to 0.5 million years. These simulations also produce fewer planetesimals than in the nominal model with millimeter-sized particles and always have at least two rings of pebbles still visible after 1 Myr.
description: Accepted in A&A
The Response to a Perturbation in the Reflection Amplitude
Creators: name: Feinberg, Joshua
Publisher: name: arXiv
Year: 2004
Subjects: subject: Mathematical Physics (math-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We apply inverse scattering theory to calculate the functional derivative of the potential $V(x)$ and wave function $ψ(x,k)$ of a one-dimensional Schrödinger operator with respect to the reflection amplitude $r(k)$.
description: 16 pages, no figures
Renormalization of the Classical Bosonic String
Creators: name: Kakushadze, Zura
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss a renormalization procedure for a classical bosonic string coupled to a massless scalar field. The classical equations of motion for this system are non-renormalizable if the number of spacetime dimensions exceeds four. Our analysis indicates that string excitation modes must be included to make the string a finite object.
description: 8 pages; this paper was written in 1992 and published in a journal in 1993, without being uploaded to arXiv at that time
Cheumatopsyche lobata Marlier 1943
Creators: name: Oláh, János
name: Johanson, Kjell Arne
name: Barnard, Peter C.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Hydropsychidae
Cheumatopsyche
Cheumatopsyche lobata

description: Cheumatopsyche lobata Marlier, 1943
Fig. 31
 Cheumatopsyche lobata Marlier, 1943: 10.
 Type locality: Zaire.
 Remarks: The holotype genitalia (in ISNB), mounted on a permanent microscope slide, are partially damaged and highly distorted. Three males labelled as paratype (in MRAC) lacking abdomens and 1 complete female were all examined. Forewing pattern is given in Fig. 31.
description: Published as part of Oláh, János, Johanson, Kjell Arne & Barnard, Peter C., 2008, Revision of the Oriental and Afrotropical species of Cheumatopsyche Wallengren (Hydropsychidae, Trichoptera), pp. 1-171 in Zootaxa 1738 on page 75
Association between Site-of-Care and the Cost and Modality of Radiotherapy for Prostate Cancer: Analysis of Medicare Beneficiaries from 2015 to 2017
Creators: name: Tringale, Kathryn R.
name: Gennarelli, Renee L.
name: Gillespie, Erin F.
name: Mitchell, Aaron P.
name: Zelefsky, Michael J.
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Among 84,447 radiotherapy (RT) courses for Medicare beneficiaries age ≥ 65 with prostate cancer treated with external beam RT (EBRT), brachytherapy, or both, 42,608 (51%) were delivered in hospital-affiliated and 41,695 (49%) in freestanding facilities. Freestanding centers were less likely to use EBRT + brachytherapy than EBRT (OR 0.84 [95%CI 0.84–0.84]; p p p
Constraints on a Cardassian model from SNIa data - revisited
Creators: name: Godlowski, Wlodzimierz
name: Szydlowski, Marek
name: Krawiec, Adam
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss some observational constraints resulting only from SNIa observations, imposed on the behavior of the original flat Cardassian model, and its extension with the curvature term included. We test the models using the Perlmutter SN Ia data as well as the new Knop and Tonry samples. We estimate the Cardassian model parameters using the best-fitting procedure and the likelihood method. In the fitting procedure we use the density variables for matter, Cardassian fluid and curvature, and include the errors in redshift measurements. For the Perlmutter sample in the non-flat Cardassian model we obtain the high or normal matter density universe ($Ω_{m,0} \ge 0.3$), while for the flat Cardassian model we have the high density universe. For sample A in the high density universe we also find the negative values of estimates of $n$ which can be interpreted as the phantom fluid effect. For the likelihood method we get that a nearly flat universe is preferred. We show that, if we assume that the matter density is 0.3, then $n \approx 0$ in the flat Cardassian model, which corresponds to the Perlmutter model with the cosmological constant. Testing with the Knop and Tonry SN Ia samples show no significant differences.
description: RevTeX4, 14 pages, 8 figures; new supernovae data by Knop (v.2) and Tonry (v.3) were used for the model estimation
The Final State of Black Strings and p-Branes, and the Gregory-Laflamme Instability
Creators: name: Park, Mu-In
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: It is shown that the usual entropy argument for the Gregory-Laflamme (GL) instability for $some$ appropriate black strings and $p$-branes gives surprising agreement up to a few percent. This may provide a strong support to the GL's horizon fragmentation, which would produce the array of higher-dimensional Schwarzschild-type's black holes finally. On the other hand, another estimator for the size of the black hole end-state relative to the compact dimension indicates a second order (i.e., smooth) phase transition for some $other$ appropriate compactifications and total dimension of spacetime wherein the entropy argument is not appropriate. In this case, Horowitz-Maeda-type's non-uniform black strings or $p$-branes can be the final state of the GL instability.
description: More emphasis on a second order phase transition. The computation result is unchanged
Bar-Induced Evolution of Dark Matter Cusps
Creators: name: Holley-Bockelmann, Kelly
name: Weinberg, Martin
name: Katz, Neal
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The evolution of a stellar bar transforms not only the galactic disk, but also the host dark matter halo. We present high resolution, fully self-consistent N-body simulations that clearly demonstrate that dark matter halo central density cusps flatten as the bar torques the halo. This effect is independent of the bar formation mode and occurs even for rather short bars. The halo and bar evolution is mediated by resonant interactions between orbits in the halo and the bar pattern speed, as predicted by linear Hamiltonian perturbation theory. The bar lengthens and slows as it loses angular momentum, a process that occurs even in rather warm disks. We demonstrate that the bar and halo response can be critically underestimated for experiments that are unable to resolve the relevant resonant dynamics; this occurs when the phase space in the resonant region is under sampled or plagued by noise.
description: 28 pages, 21 figures. Submitted to MNRAS
Cheumatopsyche unicalcarata Mey 1992
Creators: name: Oláh, János
name: Johanson, Kjell Arne
name: Barnard, Peter C.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Hydropsychidae
Cheumatopsyche
Cheumatopsyche unicalcarata

description: Cheumatopsyche unicalcarata Mey, 1992
 Cheumatopsyche unicalcarata Mey, 1992: 263.
 Type locality: Kenya.
description: Published as part of Oláh, János, Johanson, Kjell Arne & Barnard, Peter C., 2008, Revision of the Oriental and Afrotropical species of Cheumatopsyche Wallengren (Hydropsychidae, Trichoptera), pp. 1-171 in Zootaxa 1738 on page 80
Systematic Variations of CO J=2-1/1-0 Ratio in The Barred Spiral Galaxy M83
Creators: name: Koda, J.
name: Sawada, T.
name: Sakamoto, K.
name: Hirota, A.
name: Egusa, F.
name: Boissier, S.
name: Calzetti, D.
name: Meyer, J. Donovan
name: Elmegreen, B. G.
name: de Paz, A. Gil
name: Harada, N.
name: Ho, L. C.
name: Kobayashi, M. I. N.
name: Kuno, N.
name: Martin, S.
name: Muraoka, K.
name: Nakanishi, K.
name: Scoville, N.
name: Seibert, M.
name: Vlahakis, C.
name: Watanabe, Y.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present spatial variations of the CO J=2-1/1-0 line ratio in M83 using Total Power array data from ALMA. While the intensities of these two lines correlate tightly, the ratio varies over the disk, with a disk average ratio of 0.69, and shows the galactic center and a two-arm spiral pattern. It is high (>0.7) in regions of high molecular gas surface density, but ranges from low to high ratios in regions of low surface density. The ratio correlates well with the spatial distributions and intensities of FUV and IR emissions, with FUV being the best correlated. It also correlates better with the ratio of IR intensities (70/350mic), a proxy for dust temperature, than with the IR intensities. Taken together, these results suggest either a direct or indirect link between the dust heating by the interstellar radiation field and the condition of GMCs, even though no efficient mechanism is known for a thermal coupling of dust and bulk gas in GMCs.
description: Accepted for ApJ Letters
Cheumatopsyche excisa
Creators: name: Oláh, János
name: Johanson, Kjell Arne
name: Barnard, Peter C.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Hydropsychidae
Cheumatopsyche
Cheumatopsyche excisa

description: 8. Cheumatopsyche excisa species group
 The species in this species group have a bilobed segment X (Fig. 8), with long apicoventral setal lobes; and the harpagones are bilobed. The species in the group are morphologically close to the species in the C. dubitans species group, from which they are easily distinguished by the bilobed harpagones. The segment X is usually bilobed; some species, i.e. C. capronita and C. carna have a plate-like setaless mesocaudal lobe with a convex apical margin in dorsal view. The apicoventral setal lobes are produced into long, straight or dorsomesad curving processes, encircling the wide and deep dorsal and lateral interlobular gaps, and dominating the apex of segment X. The pair of wart-like lateral setose areas are located centrally or distally on segment X. This group is distributed in the South-East Asian mainland and archipelagoes.
description: Published as part of Oláh, János, Johanson, Kjell Arne & Barnard, Peter C., 2008, Revision of the Oriental and Afrotropical species of Cheumatopsyche Wallengren (Hydropsychidae, Trichoptera), pp. 1-171 in Zootaxa 1738 on page 80
The Association of Airflow Obstruction with Occupational Exposures in a Sample of Rural Adults in Iowa
Creators: name: P. K. Henneberger
name: M. J. Humann
name: X. Liang
name: B. C. Doney
name: K. M. Kelly
name: J. M. Cox-Ganser
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Medicine
subject: Biotechnology
subject: Geology
subject: FOS: Earth and related environmental sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: A recent article reported that occupational exposure to vapor-gas, dust, and fumes (VGDF) was more common in a sample of rural adults than in a sample of adults in urban settings. In another study of the same urban adults, airflow obstruction (AO) was associated with occupational VGDF and the combination of smoking and occupational exposure. The goal of the current study was to determine if similar associations were evident in the sample of rural adults. We analyzed enrollment data from the Keokuk County Rural Health Study (KCRHS), which investigated the health of rural residents in Iowa. We used the same methods as the study of urban adults. A job-exposure matrix (JEM) assigned an occupational VGDF exposure level based on each participants’ last reported job. The health outcome was AO, defined as both the forced expiratory volume in one second (FEV1) and the FEV1/forced vital capacity (FVC) ratio p
Dimensional Reduction in Bose-Condensed Alkali-Metal Vapors
Creators: name: Salasnich, L.
name: Parola, A.
name: Reatto, L.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Other Condensed Matter (cond-mat.other)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We investigate the effects of dimensional reduction in atomic Bose-Einstein condensates (BECs) induced by a strong harmonic confinement in the cylindric radial direction or in the cylindric axial direction. The former case corresponds to a transition from 3D to 1D in cigar-shaped BECs, while the latter case corresponds to a transition from 3D to 2D in disc-shaped BECs. We analyze the first sound velocity in axially-homogeneous cigar-shaped BECs and in radially-homogeneous disc-shaped BECs. We consider also the dimensional reduction in a BEC confined by a harmonic potential both in the radial direction and in the axial direction. By using a variational approach, we calculate monopole and quadrupole collective oscillations of the BEC. We find that the frequencies of these collective oscillations are related to the dimensionality and to the repulsive or attractive inter-atomic interaction.
description: to be published in Phys. Rev. A; related papers can be found at http://www.mi.infm.it/salasnich/tdqg.html
Orchesella devergens Handschin 1924
Creators: name: Thibaud, Jean-Marc
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Collembola
Entomobryomorpha
Orchesellidae
Orchesella
Orchesella devergens

description: Orchesella devergens Handschin, 1924
Orchesella devergens Handschin, 1924: 145.
DISTRIBUTION. — Tarn. Sidobre (Izarra 1969).
description: Published as part of Thibaud, Jean-Marc, 2017, Catalogue des collemboles de France, pp. 297-436 in Zoosystema 39 (3) on page 385, DOI: 10.5252/z2017n3a1, http://zenodo.org/record/5496272
Additional file 32 of The round goby genome provides insights into mechanisms that may facilitate biological invasions
Creators: name: Adrian-Kalchhauser, Irene
name: Blomberg, Anders
name: Larsson, Tomas
name: Musilova, Zuzana
name: Peart, Claire
name: Pippel, Martin
name: Solbakken, Monica
name: Suurväli, Jaanus
name: Walser, Jean-Claude
name: Wilson, Joanna
name: Rosenblad, Magnus Alm
name: Demian Burguera
name: Gutnik, Silvia
name: Michiels, Nico
name: Töpel, Mats
name: Pankov, Kirill
name: Schloissnig, Siegfried
name: Winkler, Sylke
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Computational Biology

description: Detailed methods for 3’ and 5’ RACE of epigenetic regulators.
Interferometric observations of the supergiant stars alpha Orionis and alpha Herculis with FLUOR at IOTA
Creators: name: Perrin, G.
name: Ridgway, S. T.
name: Foresto, V. Coudé du
name: Mennesson, B.
name: Traub, W. A.
name: Lacasse, M. G.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the observations in the K band of the red supergiant star alpha Orionis and of the bright giant star alpha Herculis with the FLUOR beamcombiner at the IOTA interferometer. The high quality of the data allows us to estimate limb-darkening and derive precise diameters in the K band which combined with bolometric fluxes yield effective temperatures. In the case of Betelgeuse, data collected at high spatial frequency although sparse are compatible with circular symmetry and there is no clear evidence for departure from circular symmetry. We have combined the K band data with interferometric measurements in the L band and at 11.15 micron. The full set of data can be explained if a 2055 K layer with optical depths $τ_{K}=0.060\pm0.003$, $τ_{L}=0.026\pm0.002$ and $τ_{11.15μm}=2.33\pm0.23$ is added 0.33 $R_{\star}$ above the photosphere providing a first consistent view of the star in this range of wavelengths. This layer provides a consistent explanation for at least three otherwise puzzling observations: the wavelength variation of apparent diameter, the dramatic difference in limb darkening between the two supergiant stars, and the previously noted reduced effective temperature of supergiants with respect to giants of the same spectral type. Each of these may be simply understood as an artifact due to not accounting for the presence of the upper layer in the data analysis. This consistent picture can be considered strong support for the presence of a sphere of warm water vapor, proposed by Tsuji (2000) when interpreting the spectra of strong molecular lines.
description: Accepter for publication by Astronomy and Astrophysics
title: Wholeness in fragments: Coleridge's Shakespearean criticism
Creators: name: Lee, Kyung-Ook
Publisher: name: University of Glasgow
Year: 2000
Subjects: subject: Comparative literature.

description: Coleridge's Shakespearean criticism is mostly composed of fragments-sometimes in the form of lectures, sometimes as notes, and sometimes scribbled on the blank leaves of pamphlets. In his lectures from 1808 to 1819 on literature, Coleridge seldom adhered to the prospectus. In many cases they ended up as fragments. Critics are divided between those who insist that Coleridge's criticism is distinguished by the consistency of its principles and methodology and those who insist on its fragmentariness. The purpose of the thesis is to reveal the wholeness of a Shakespearean criticism that consists of fragments. Some critics such as Thomas MacFarland claim that fragmentation is the distinguishing condition of the Romantic era. According to him, a diasperactive form; that is, an actual incompleteness striving toward a hypothetical unity is common in the art of an era in which the fragment functions as the symbol for the whole. Lee Lust Brown argues that Coleridge hypothesised a textual whole which was both more than and prior to its parts and yet his own writing manifests a degree of literal fragmentation. He takes the fragment as a synecdoche of wholeness and claims that textual wholeness is not so much lost as deferred or displaced in the question of its possibility. Agreeing with these critics, I argue for the wholeness of Coleridge's Shakespearean criticism. In so doing, first of all, I deal with the representative schools of Shakespearean criticism before or contemporary with Coleridge, those of his predecessors and of the German Idealists, because these constitute the two main sources informing Coleridge's Shakespearean criticism. Considering that Coleridge's Shakespearean criticism is closely linked to his poetic principles, I try to define his poetic principles-the concept of nature, organicism, and imagination. I deal with Coleridge's criticism of Shakespeare under three heads; Shakespeare as an artist, Shakespeare's poetic works, and their appreciation. In chapter one, in order to trace the background of Coleridge's Shakespearean criticism, I discuss the two distinctive schools of Shakespearean criticism contemporary with Coleridge; i.e., the British school and the German school. In chapter two, I deal with the poetical principles that form the ground of Coleridge's Shakespearean criticism; that is, the concept of nature, organicism and imagination. In chapter three, I show how a unified ideal of Shakespeare can be drawn from the fragments. In chapter four, I begin by tracing Coleridge's insistence that Shakespeare's drama is an instance, indeed the highest instance, of all art. In chapter five, I deal with Coleridge's appreciation of Shakespeare's work. Finally, I discuss Coleridge's idea of the perfect audience for Shakespeare's plays, the audience that the plays imply. In conclusion I offer a general view of Coleridge's Shakespearean criticism and indicate its crucial place in critical history. (Abstract shortened by ProQuest.).
mFLICA: An R package for Inferring Leadership of Coordination From Time Series
Creators: name: Amornbunchornvej, Chainarong
Publisher: name: arXiv
Year: 2020
Subjects: subject: Social and Information Networks (cs.SI)
subject: Econometrics (econ.EM)
subject: Computation (stat.CO)
subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences
subject: FOS: Economics and business
subject: G.3
subject: 62-04, 62M10

description: Leadership is a process that leaders influence followers to achieve collective goals. One of special cases of leadership is the coordinated pattern initiation. In this context, leaders are initiators who initiate coordinated patterns that everyone follows. Given a set of individual-multivariate time series of real numbers, the mFLICA package provides a framework for R users to infer coordination events within time series, initiators and followers of these coordination events, as well as dynamics of group merging and splitting. The mFLICA package also has a visualization function to make results of leadership inference more understandable. The package is available on Comprehensive R Archive Network (CRAN) at https://CRAN.R-project.org/package=mFLICA.
description: The latest version of R package can be found at https://github.com/DarkEyes/mFLICA
Chandra observations of the X-ray luminous star-forming galaxy merger Arp~299
Creators: name: Zezas, A.
name: Ward, M. J.
name: Murray, S. S.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report results of a Chandra observation of the X-ray luminous star-forming galaxy Arp299 (NGC3690/IC694). We detect 18 discrete X-ray sources with luminosities above ~10^39 erg\s (0.5-8.0 keV band), which contribute ~40% of the total galactic emission in this band. The remaining emission is associated with a diffuse component spatially coincident with regions of widespread star-formation. We detect X-ray emission from both nuclei. One of the discrete sources within the complex nuclear region of NGC 3690 is found to have a very hard spectrum and therefore we associate it with the origin of the AGN-like spectrum that has also been detected at high X-ray energies using Beppo-SAX.
description: 7 pages, 2 figures, to appear in ApJ Lett