cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The driving force governing room temperature grain coarsening in thin gold films
Creators: name: Glushko, Oleksandr
name: Cordill, Megan J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Strong room-temperature grain coarsening in gold films on polyimide induced by cyclic uniaxial mechanical strain is demonstrated. Detailed electron backscatter diffraction analysis revealed that, in contrast to the predictions of shear-coupled grain boundary migration model, the grain coarsening is isotropic and coarsened grains do not exhibit any specific crystallographic orientations or misorientations to the neighboring grains. It is shown that a thermodynamic model where the driving force appears due to the difference in yield stresses between the grains with different sizes provides an adequate explanation of the experimental data.
Using Galaxy Cluster Peculiar Velocities to Constrain Cosmological Parameters
Creators: name: Peel, A.
name: Knox, L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Galaxy cluster peculiar velocities can be inferred from high-sensitivity, high-resolution multiple-frequency observations in the 30 to 400 GHz range. While galaxy cluster counts and power spectra are sensitive to the growth factor, peculiar velocities are sensitive to the time-derivative of the growth factor and are hence complementary. Using linear perturbation theory, we forecast constraints on Omega(matter), the Hubble constant today, and the dark-energy equation of state parameter, given 820 densely sampled cluster locations (near redshift 1) from a Lambda-CDM N-body simulation and 820 sparsely sampled cluster locations in a broader redshift range.
description: 4 pages, 2 figures, to appear in Proceedings of Dark Matter 2002, requires espcrc2.sty
Additional file 3 of Multimodal-based machine learning strategy for accurate and non-invasive prediction of intramedullary glioma grade and mutation status of molecular markers: a retrospective study
Creators: name: Ma, Chao
name: Wang, Liyang
name: Song, Dengpan
name: Gao, Chuntian
name: Jing, Linkai
name: Lu, Yang
name: Liu, Dongkang
name: Man, Weitao
name: Yang, Kaiyuan
name: Meng, Zhe
name: Zhang, Huifang
name: Xue, Ping
name: Zhang, Yupeng
name: Guo, Fuyou
name: Wang, Guihuai
Publisher: name: figshare
Year: 2023
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Additional file 3. Clinical characteristics of the patients and distribution of the ATRX and P53 mutation status across the primary and external validation cohorts. ATRX, alpha thalassemia/mental retardation syndrome X-linked; IQR, interquartile range; P53, tumor protein p53; WHO, World Health Organization.
Practical fixed-effects estimation methods for the three-way error-components model
Creators: name: Andrews, Martyn
name: Schank, Thorsten
name: Upward, Richard
name: Andrews, Martyn
name: Schank, Thorsten
name: Upward, Richard
Publisher: name: Unknown
Year: 2006
Subjects: subject: Research Methods/ Statistical Methods
subject: grouping
subject: linked employer–employee panel data
subject: fixed effects

description: Methods for fixed-effects estimation of the three-way error-components model are not yet standard. Where possible, we make the fixed-effects methods originally developed by Abowd, Kramarz, and Margolis (Econometrica 67: 251–333) for linked worker-firm data more accessible. We also show how these methods can be implemented in Stata. There is a caveat, however. If the researcher wants to recover estimates of the error components themselves, and the number of units at the higher level of aggregation is large, memory or matrix constraints may make using Stata to estimate the components themselves infeasible.
Alyma pallipes Arias 2004, new combination
Creators: name: Arias, Elizabeth T.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Elateridae
Alyma
Alyma pallipes

description: Alyma pallipes (Solier), new combination
(Figs. 1, 6, 14, 22, 34)
description: Published as part of Arias, Elizabeth T., 2004, A New Click Beetle Genus from Chilean Temperate Forests, ALYMA (Coleoptera: Elateridae: Pomachiliini), pp. 413-427 in The Coleopterists Bulletin 58 (3) on pages 413-427, DOI: 10.1649/523, http://zenodo.org/record/5345219
Sicyonidae Ortmann 1898
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Anthozoa
Actiniaria
Sicyonidae

description: Family Sicyonidae Ortmann, 1898  Sometimes called rock shrimps, members of this family usually have a well-calcified exoskeleton. The dorsal midline of the carapace and abdomen bear a carina, often with prominent teeth. The rostrum is conspicuous. In life, these shrimps bury into sand or shelly sand. They are edible, and are fished commercially in many warm-temperate areas worldwide.
 The only species of this family resident in the area is Sicyonia ingentis. Two other species have been collected in southern California during El Niño periods. Sicyonia penicillata Lockington, 1879 has been collected from the Palos Verdes Peninsula to off Torrey Pines State Beach, San Diego County (Montagne & Cadien 2001, fig. 1.) This species has a large dark spot on the branchial region of the carapace. Divers have photographed occasional individuals of S. picta Faxon, 1893 off Santa Catalina I., California. This species has a large eye-like marking on the posterolateral part of the carapace. Unlike S. penicillata, S. picta has no tooth on the dorsal midpoint of the carapace. See Hendrickx (1996: figs. 56, 58) for illustrations. Both of these species usually range from the Gulf of California and the southern end of Baja California, Mexico southward.
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on page 25
First order phase transitions in the square lattice "easy-plane" J-Q model
Creators: name: Desai, Nisheeta
name: Kaul, Ribhu K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the quantum phase transition between the superfluid and valence bond solid in "easy-plane" J-Q models on the square lattice. The Hamiltonian we study is a linear combination of two model Hamiltonians: (1) an SU(2) symmetric model, which is the well known J-Q model that does not show any direct signs of a discontinuous transition on the largest lattices and is presumed continuous, and (2) an easy plane version of the J-Q model, which shows clear evidence for a first order transition even on rather small lattices of size $L\approx16$. A parameter $0\leqλ\leq 1$ ($λ=0$ being the easy-plane model and $λ=1$ being the SU(2) symmetric J-Q model) allows us to smoothly interpolate between these two limiting models. We use stochastic series expansion (SSE) quantum Monte Carlo (QMC) to investigate the nature of this transition as $λ$ is varied - here we present studies for $λ=0,0.5,0.75,0.85,0.95$ and $1$. While we find that the first order transition weakens as $λ$ is increased from 0 to 1, we find no evidence that the transition becomes continuous until the SU(2) symmetric point, $λ=1$. We thus conclude that the square lattice superfluid-VBS transition in the two-component easy-plane model is generically first order.
Diffusion NMR Methods Applied to Xenon Gas for Materials Study
Creators: name: Mair, R. W.
name: Rosen, M. S.
name: Wang, R.
name: Cory, D. G.
name: Walsworth, R. L.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report initial NMR studies of i) xenon gas diffusion in model heterogeneous porous media, and ii) continuous flow laser-polarized xenon gas. Both areas utilize the Pulsed Gradient Spin Echo techniques in the gas-phase, with the aim of obtaining more sophisticated information than just translational self-diffusion coefficients - a brief overview of this area is provided in the introduction. The heterogeneous or multiple-length scale model porous media consisted of random packs of mixed glass beads of two different sizes. We focus on observing the approach of the time-dependent gas diffusion coefficient, D(t), (an indicator of mean squared displacement) to the long-time asymptote, with the aim of understanding the long-length scale structural information that may be derived from a heterogeneous porous system. The Pade approximation is used to interpolate D(t) data between the short and long time limits. Initial studies of continuous flow laser-polarized xenon gas demonstrate velocity-sensitive imaging of much higher flows than can generally be obtained with liquids (20 - 200 mm/s). Gas velocity imaging is, however, found to be limited to a resolution of about 1 mm/s due to the high diffusivity of gases compared to liquids. We also present the first gas-phase NMR scattering, or diffusive-diffraction, data: namely, flow-enhanced structural features in the echo attenuation data from laser-polarized xenon flowing through a 2 mm glass bead pack.
description: single pdf file including all figures
Supplemental text including sequences of seven housekeeping genes, primer sequences and sequences of 96 dual barcodes
Creators: name: Yu-Chieh Liao
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Supplemental text including sequences of seven housekeeping genes, primer sequences and sequences of 96 dual barcodes
A Survey for Infall Motions toward Starless Cores. II. $CS (2-1)$ and $N_2H^+ (1-0)$ Mapping Observations
Creators: name: Lee, Chang Won
name: Myers, Philip C.
name: Tafalla, Mario
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of an extensive mapping survey of 53 `starless' cores in the optically thick line of CS 2-1 and the optically thin lines of N2H+ 1-0 and C18O 1-0. The purpose of this survey was to search for signatures of extended inward motions. This study finds 10 `strong' and 9 `probable' infall candidates, based on $δV_{CS}$ analysis and on the spectral shapes of CS lines. From our analysis of the blue-skewed CS spectra and the $δV_{CS}$ parameter, we find typical infall radii of 0.06-0.14 pc. Also, using a simple two layer radiative transfer model to fit the profiles, we derive one-dimensional infall speeds, half of whose values lie in the range of 0.05-0.09 km s$^{-1}$. These values are similar to those found in L1544 by Tafalla et al., and this result confirms that infall speeds in starless cores are generally faster than expected from ambipolar diffusion in a strongly sub-critical core. In addition, the observed infall regions are too extended to be consistent with the `inside-out' collapse model applied to a very low-mass star. In the largest cores, the spatial extent of the CS spectra with infall asymmetry is larger than the extent of the $\rm N_2H^+$ core by a factor of 2-3. All these results suggest that extended inward motions are a common feature in starless cores, and that they could represent a necessary stage in the condensation of a star-forming dense core.
description: Two tex files for manuscript and tables, and 38 figures. To appear in ApJS
title: Authoring Justice. How to get home
title: How to get home
titleType: AlternativeTitle
Creators: name: Goloșceapov, Evghenii Alexandrovici
Publisher: name: Global Campus of Human Rights
Year: 2024

description: We are pleased to share the final outcomes of the online course “Authoring Justice”, showcasing excerpts of the participants' Capstone Projects, which were designed to be either standalone long-form works or components of books they are now beginning to write. The authors are human rights advocates, lawyers, professors, and researchers from across the globe and their pieces cover a wide range of topics, particularly in areas where human rights are at risk of being overlooked or undermined. This Capstone Project excerpt contains 'How to get home' by Evghenii Alexandrovici Goloșceapov
Testing for cross-sectional dependence in panel-data models
Creators: name: De Hoyos, Rafael E.
name: Sarafidis, Vasilis
name: De Hoyos, Rafael E.
name: Sarafidis, Vasilis
Publisher: name: Unknown
Year: 2006
Subjects: subject: Research Methods/ Statistical Methods
subject: xtcsd
subject: panel data
subject: cross-sectional dependence

description: This article describes a new Stata routine, xtcsd, to test for the presence of cross-sectional dependence in panels with many cross-sectional units and few time-series observations. The command executes three different testing procedures—namely, Friedman’s (Journal of the American Statistical Association 32: 675–701) (FR) test statistic, the statistic proposed by Frees (Journal of Econometrics 69: 393–414), and the cross-sectional dependence (CD) test of Pesaran (General diagnostic tests for cross-section dependence in panels [University of Cambridge, Faculty of Economics, Cambridge Working Papers in Economics, Paper No. 0435]). We illustrate the command with an empirical example.
Maps related to polar spaces preserving a Weyl distance or an incidence condition
Creators: name: De Schepper, A.
name: Van Maldeghem, H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: Let $Ω_i$ and $Ω_j$ be the sets of elements of respective types $i$ and $j$ of a polar space~$Δ$ of rank at least $3$, viewed as a Tits-building. For any Weyl distance $δ$ between $Ω_i$ and $Ω_j$, we show that $δ$ is characterised by $i$ and $j$ and two additional numerical parameters $k$ and $\ell$. We consider permutations $ρ$ of $Ω_i \cup Ω_j$ that preserve a single Weyl distance $δ$. Up to a minor technical condition on $\ell$, we prove that, up to trivial cases and two classes of true exceptions, $ρ$ is induced by an automorphism of the Tits-building associated to $Δ$, which is always a type-preserving automorphism of $Δ$ (and hence preserving all Weyl-distances), unless $Δ$ is hyperbolic, in which case there are outer automorphisms. For each class of exceptions, we determine a Tits-building $Δ'$ in which $Δ$ naturally embeds and is such that $ρ$ is induced by an automorphism of $Δ'$. At the same time, we prove similar results for permutations preserving a natural incidence condition. These yield combinatorial characterisations of all groups of algebraic origin which are the full automorphism group of some polar space as the automorphism group of many bipartite graphs.
Omophoita hispicornis Bechyne 1955
Creators: name: Duckett, Catherine N.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Chrysomelidae
Omophoita
Omophoita hispicornis

description: Omophoita hispicornis (Bechyne´) New Combination
 Longasphera hispicornis Bechyné 1955: 184. Holotype: Brazil: Minas Gerais: Uberaba. Frey Collection, Basel.
description: Published as part of Duckett, Catherine N., 2004, Longasphaera Bechyné (Coleoptera: Chrysomelidae: Galerucinae: Alticini: Oedionychina) a New Synonym of Omophoita Chevrolat, pp. 652-655 in The Coleopterists Bulletin 58 (4) on page 654, DOI: 10.1649/714, http://zenodo.org/record/5345361
Cosmological Hydrogen Reionization with Three Dimensional Radiative Transfer
Creators: name: Razoumov, Alexei O.
name: Norman, Michael L.
name: Abel, Tom
name: Scott, Douglas
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new calculations of the inhomogeneous process of cosmological reionization by carefully following the radiative transfer in pre-computed hydrodynamical simulations of galaxy formation. These new computations represent an important step on the way towards fully self-consistent and adaptive calculations which will eventually cover the enormous range of scales from the sizes of individual mini-halos to the mean free path of ionizing photons in the post-overlap Universe. The goal of such simulations is to include enough realistic physics to accurately model the formation of early structures and the end of the `dark ages'. Our new calculations demonstrate that the process by which the ionized regions percolate the Universe is complex, and that the idea of voids being ionized before overdense regions is perhaps too simplistic. It seems that observational information pertaining to the reionization epoch may now be in our grasp, through the detection of Gunn-Peterson troughs at z~6. If so, then the comparison of information from many lines of sight with simulations such as ours may allow us to disentangle details of the ionization history and trace the early formation of structure.
description: 21 pages, 5 figures, uses AASTeX, accepted to the Astrophysical Journal, extra movie available at http://cosmos.ucsd.edu/~razoumov/fig/movie_sai.mpg
Polyonyx quadriungulatus Glassell 1935
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Porcellanidae
Polyonyx
Polyonyx quadriungulatus

description: Polyonyx quadriungulatus Glassell, 1935
(Fig. 37F)
 Polyonyx quadriungulatus Glassell, 1935: 93, pl. 9. — Haig 1956: 80; 1960: 236, pl. 41, fig. 2; text fig. 12 (1). — Haig et al. 1970: 26. — Kudenov & Haig 1974: 105. — Jensen 1995: 76, fig. 154.
 Diagnosis. Front convex or concave in dorsal view, with short fringe of setae. Carapace subovate, 1.2 –1.4 times as broad as long. Chelipeds unequal. Merus with broad, rounded lobe on anterior margin; posterior margin fringed with fine setae. Carpus with anterior margin bearing high lamellar crest, anterior, posterior margins fringed with setae. Chela slender, dorsal surface swollen, without crest in major cheliped; outer margin with sharp crest lined with row of granules, thick fringe of setae extending nearly to apex of dactyl, gape of fingers with scattered short setae. In major chela, dactyl crosses over fixed finger at apex of chela. Pereopods 2–4 smooth, all segments with fringe of fine setae. Merus with fringe of fine setae. Propodus with pair of movable spinules at distal end of posterior margin, single movable spine posterior to them, one on middle or proximal third of posterior margin. Dactyl with 4 fixed spines, distal three large, proximal one small. Telson with 7 plates. Carapace length to 13.5 mm.
 Color in life. Carapace, chelipeds dark brown, mottled with green, red; pereopods 2–4 lighter, banded (Glassell 1935).
 Habitat and depth. Strictly symbiotic, living in pairs within tubes of polychaete Chaetopterus variopedatus (Renier, 1804), intertidal zone to 46 m.
 Range. Santa Rosa I., California to Punta San Eugenio, Baja California, Mexico, Gulf of California at Puerto Peñasco, Loreto, and El Mogote. Type locality Estero de Punta Banda, Baja California, Mexico.
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on pages 159-160
Black holes with supertranslation field, "large transformations" and Israel theorem
Creators: name: Iofa, Mikhail Z.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: An axial-symmetric vacuum solution of the Einstein equations containing a supertranslation field diffeomorphic to the Schwarzschild solution is discussed in the context of Israel theorem. The metric satisfies all conditions of the Israel theorem, except for the condition on the form of the metric at spatial infinity. Nevertheless, following the steps of the proof of the theorem we show that the proof applies to the metric with supertranslation field and the (transformed) metric used in the proof is spherically symmetric. We explain the source of the seeming discrepancy connected with the use of "large" transformations changing supertranslation field in the metric.
description: 8 pages. Completely new discussion.Published version
Noise-Driven Mechanism for Pattern Formation
Creators: name: Buceta, J.
name: Ibanes, M.
name: Sancho, J. M.
name: Lindenberg, Katja
Publisher: name: arXiv
Year: 2002
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We extend the mechanism for noise-induced phase transitions proposed by Ibanes et al. [Phys. Rev. Lett. 87, 020601-1 (2001)] to pattern formation phenomena. In contrast with known mechanisms for pure noise-induced pattern formation, this mechanism is not driven by a short-time instability amplified by collective effects. The phenomenon is analyzed by means of a modulated mean field approximation and numerical simulations.
Die Große Schnittstelle. Bericht über die 14. Kampagne in Tall Mozan/Urkeš: Ausgrabungen im Gebiet AA, Juni-Oktober 2001
Creators: name: Buccellati, Giorgio
name: Kelly-Buccellati, Marilyn
Publisher: name: figshare
Year: 2019
Subjects: Archaeology

description: Buccellati, G., and M. Kelly-Buccellati. 2002. “Die Große Schnittstelle. Bericht über die 14. Kampagne in Tall Mozan/Urkeš: Ausgrabungen im Gebiet AA, Juni-Oktober 2001.” Mitteilungen der Deutschen Orient-Gesellschaft zu Berlin 134: 103–30.
Gastroptychus perarmatus
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Chirostylidae
Gastroptychus
Gastroptychus perarmatus

description: Gastroptychus perarmatus (Haig, 1968)
(Fig. 33M)
 Chirostylus perarmatus Haig, 1968: 272, figs. 1–3. — Wicksten 1989b: 315.
 Gastroptychus perarmatus. — Baba & Haig 1990: 859.
 Diagnosis. Rostrum as in G. iaspis. Carapace excluding rostrum 1.5–1.6 times as long as greatest width. Lateral margins nearly straight posteriorly; strong anterolateral spine and row of small lateral spines. Gastric region with numerous small spines and spinules interspersed with larger spines, most prominent an epigastric pair. Midcervical groove distinctly anterior to halfway point of carapace. Anterior branchial region with several large, small spines; cardiac region with pair prominent spines, few smaller ones; regions posterior to cervical groove with numerous, closely set large, small spines in irregular longitudinal rows. Tergum of abdominal somite 1 with transverse row of 12–18 spines. Tergum of somite 2 with transverse row of small spines, pointed granules, and pointed tubercles at junction with pleura; pleura with small spines on anterolateral margin, dorsal surface. Tergum of somites 3, 4 unarmed except for 1–3 spines on surface. Tergum of somite 5 with 4 longitudinal rows of spines, each outer row at junction with pleuron; pleura with small spines on surface. Tergum of somite 6 bearing numerous large, small spines; pleura with few spines on surface. Eyestalk barely reaching end of rostral spine; cornea dilated. Length of chelipeds about 6 times length of carapace excluding rostrum. Merus, carpus, palm with regular longitudinal rows of spines. Pereopods 2–4 slender, merus, carpus with 6 rows of spines; propodus with dorsal, mesial, dorsolateral rows of spines, ventral margin with row of closely set movable spinules; length of dactyl less than 0.33 times length of propodus, with ventral spinules, terminating in acute corneous claw. Carapace length excluding rostrum: male 20.5 mm, female 16.0 mm.
 Color in life. Not reported. Bright pink after a few weeks of preservation in alcohol, soon fading to white (Haig 1968).
 Habitat and depth. Green mud bottom or on antipatharians; from 229–366 m.
 Range. From north of Anacapa I. to Coronado Bank, California. Type locality north of Anacapa I., from 34˚ 05.8' N, 119˚ 23.3' W to 34˚ 6.0' N, 119˚ 24.3' W.
 Remarks. Two specimens collected off Coronado Bank in 366 m were clinging to a branch of black coral, order Antipatharia.
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on page 145
Proof of the feasibility of a nanocell-based wide-range optical magnetometer
Creators: name: Klinger, Emmanuel
name: Azizbekyan, Hrayr
name: Sargsyan, Armen
name: Leroy, Claude
name: Sarkisyan, David
name: Papoyan, Aram
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We present an experimental scheme performing scalar magnetometry based on the fitting of Rb D$_2$ line spectra recorded by derivative selective reflection spectroscopy from an optical nanometric-thick cell. To demonstrate its efficiency, the magnetometer is used to measure the inhomogeneous magnetic field produced by a permanent neodimuim-iron-boron alloy ring magnet at different distances. The computational tasks are realized by relatively cheap electronic components: an Arduino Due board for the external control of the laser and acquisition of spectra, and a Raspberry Pi computer for the fitting. The coefficient of variation of the measurements remains under $5\%$ in the magnetic field range of 40 - 200 mT, limited only by the size of the oven and translation stage used in our experiment. The proposed scheme is expected to operate with a high measurement precision also for stronger magnetic fields ($>500~$mT), in the hyperfine Paschen-Back regime, where the evolution of the atomic transitions can be calculated with a high accuracy.
description: 6 pages, 2 figures
The Long-Period Orbit of the Dwarf Nova V630 Cassiopaeia
Creators: name: Orosz, Jerome A.
name: Thorstensen, John R.
name: Honeycutt, R. Kent
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present extensive spectroscopy and photometry of the dwarf nova V630 Cassiopeiae. A late-type (K4-5) absorption spectrum is easily detectable, from which we derive the orbital parameters. We find a spectroscopic period of P=2.56387 +/- (4 times 10^{-5}) days and a semiamplitude of K_2=132.9 +/- 4.0 km/s. The resulting mass function, which is a firm lower limit on the mass of the white dwarf, is then f(M)=0.624 +/- 0.056 solar masses. The secondary star is a ``stripped giant'', and using relations between the core mass and the luminosity and the core mass and the radius we derive a lower limit of M_2 > 0.165 solar masses for the secondary star. The rotational velocity of the secondary star is not resolved in our spectra and we place a limit of V_rot*sin(i) < 40 km/s. The long-term light curve shows variations of up to 0.4 mag on short (1-5 days) time scales, and variations of 0.2-0.4 mag on longer (3-9 months) time scales. In spite of these variations, the ellipsoidal light curve of the secondary star is easily seen when the data are folded on the spectroscopic ephemeris. Ellipsoidal models fit to the mean light curve give an inclination in the range 66.96 < i < 78.08 degrees (90 per cent confidence). This inclination range, and the requirement that M_2 > 0.165 solar masses and V_rot*sin(i) < 40 km/s yields a white dwarf mass of M_1=0.977^{+0.168}_{-0.098} solar masses and a secondary star mass of M_2=0.172^{+0.029}_{-0.012} solar masses (90 per cent confidence limits). Our findings confirm the suggestion of Warner (1994), namely that V630 Cas is rare example of a dwarf nova with a long orbital period.
description: 8 pages, 9 figures, to appear in MNRAS
The effect of using Filtered Containment Venting System on variation in dose with distance in the prompt accident consequence assessment
Creators: name: Wadayama, Kodai
name: Kojo, Retsu
name: Niisoe, Tamon
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: In a nuclear emergency, consequence assessment based on the plant conditions using a simple method is important for a prompt response. Response Technical Manual (RTM-96) is a manual calculation method for prompt dose projection at arbitrary distances by converting pre-calculated doses with the conversion factor based on distance and weather. However, the ‘conversion factor’ in RTM-96 does not consider accident scenarios with filtered containment venting system (FCVS). Therefore, in this study, we defined the ratio of effective dose between 1 km and an arbitrary distance as the ‘Distance Conversion Factor (DCF)’ and aimed to clarify the difference between DCFs by accident scenarios, focusing on the presence or absence of FCVS. The results showed that the differences in DCFs for different accident scenarios were minor in the case of no rainfall. In contrast, in the case of rainfall, DCF differed significantly with scenarios with FCVS and those with containment failure. Therefore, the authors propose that DCFs with rainfall should be calculated separately for several representative accident scenarios rather than uniformly for all accident scenarios, as in the conventional method. The results can contribute to developing a new prompt consequence assessment method, such as RTM-96, which considers FCVS.
Additional file 4 of Identification and population genetic analyses of copy number variations in six domestic goat breeds and Bezoar ibexes using next-generation sequencing
Creators: name: Guo, Jiazhong
name: Zhong, Jie
name: Liu, George E.
name: Yang, Liu
name: Li, Li
name: Chen, Guangling
name: Song, Tianzeng
name: Zhang, Hongping
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 4: Figure S2. Results of validation for the identification of CNVs using an independent run of deep sequencing data.
Supplemental text including sequences of seven housekeeping genes and sequences of 96 dual barcodes
Creators: name: Yu-Chieh Liao
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Supplemental text including sequences of seven housekeeping genes and sequences of 96 dual barcodes
Cryptolithodes sitchensis Brandt 1853
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Lithodidae
Cryptolithodes
Cryptolithodes sitchensis

description: Cryptolithodes sitchensis Brandt, 1853
(Fig. 40B, Pl. 6B)
 Cryptolithodes sitchensis Brandt, 1853: 254. — Holmes 1900: 125, pl. 2, figs. 21–25. — Schmitt 1921: 155, pl. 20, figs. 3, 4, fig. 100. — Johnson & Snook 1927: 339, fig. 287. — Makarov 1962: 268, figs. 108, 109. — Haig & Abbott 1980: 583, figs. 24.8 a–g. — Hart 1982: 76, fig. 22. — Ricketts et al. 1985: 171, fig. 139. — Odenweller 1972: 240, figs. 1, 2. — Dawson 1989: 317. — Jensen 1995: 71, fig. 138. — Kuris et al. 2007: 648.
 Diagnosis. Carapace covering most of body, pereopods, about 1.3 times as wide and long, with lateral extensions almost as long as rostrum, with dorsal tubercles, low teeth along lateral margins. Rostrum widened distally, usually ending in distinct anterolateral angles, sometimes with small median tooth. Chelipeds smooth, unequal. Pereopods 2–4 smooth, flat. Abdomen flat, triangular. Carapace length to 68 mm.
 Color in life. Orange, mottled, ivory, red, pink with red spots; see color photographs by Haig & Abbott (1980: figs. 24.8 a–g).
 Habitat and depth. Rocky reefs and tide pools, lowest intertidal zone to 17 m.
 Range. Sitka, Alaska to Point Loma, California. Type locality Sitka, Alaska. This crab is uncommon south of Point Conception.
 Remarks. These little crabs sometimes bear injuries around the rim of the carapace. At times, two or more of these crabs will grip each other by the rim of the carapace. Whether this activity constitutes mating behavior or aggression is unknown.
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on page 166
Planetary nebulae as mass tracers of their parent galaxies: biases in the estimate of the kinematical quantities
Creators: name: Napolitano, Nicola R.
name: Arnaboldi, Magda
name: Freeman, Kenneth C.
name: Capaccioli, Massimo
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Multi-object and multi-fiber spectrographs on 4 and 8 meter telescopes make it possible to use extragalactic planetary nebulae (PNe) in the outer halos of early-type galaxies as kinematical tracers, where classical techniques based on integrated stellar light fail. Until now, published PNe radial velocity samples are small, with only a few tens of radial velocity measurements (except for a few cases like NGC 5128 or M31), causing uncertainties in the mass and angular momentum estimates based on these data. To quantify these uncertainties, we have made equilibrium models for spherical galaxies, with and without dark matter, and via Montecarlo simulations we produce radial velocity samples with different sizes. We then apply, to these discrete radial velocity fields, the same standard kinematical analysis as it is commonly done with small samples of observed PNe radial velocities. By comparison of the inferred quantities with those computed from the analytical model, we test for systematic biases and establish a robust procedure to infer the angular momentum distribution and radial velocity dispersion profiles from such samples.
description: 18 pages, 26 figures, A&A 2001, in press
Poverty, Inequality and Conflict
Creators: name: Kanbur, Ravi
name: Kanbur, Ravi
Publisher: name: Unknown
Year: 2007
Subjects: Public Economics

description: While there is a general view that poverty and inequality can lead to conflict and are therefore in this sense security issues, the precise nature of the links is less well appreciated. Focusing on conflicts within states, this paper draws out the links based on the recent economics literature, and discusses their implications for policy. It is argued that while inequality is a natural concomitant of economic processes, particularly those driven by the market, its implications for security emerge when unequal outcomes align with socio-political cleavages. Such an alignment can turn a benign outcome, in which increasing inequality might even help economic efficiency, into one in which conflict worsens the climate for investment even before, in the extreme, a collapse of the social order. A careful assessment of the intersection between economic outcomes and social divisions is necessary in designing policies and interventions for growth and poverty reduction.
Glyptolithodes cristatipes
Creators: name: Wicksten, Mary K.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Lithodidae
Glyptolithodes
Glyptolithodes cristatipes

description: Glyptolithodes cristatipes (Faxon, 1893)
(Fig. 39E, F)
 Rhinolithodes cristatipes Faxon, 1893:163.
 Glyptolithodes cristatipes. — Faxon 1895: 43, pl. 7, fig. 2, 2a–2c. — Haig 1974: 161, fig. 5. — Baez & Andrade 1979: 222, pl. 1, fig. 2. — Wicksten 1982: 247. — Wicksten 1989b: 314. — Dawson 1989: 317. — Martin et al. 1997: 83, figs. 2, 3 (extensive synonymy). — Hendrickx & Harvey 1999: 374.
 Diagnosis (after Haig 1974 and Martin et al. 1997). Carapace subtriangular, tuberculate; gastric area raised into conical prominence, crescent-shaped ridge on each branchial region, cardiac area enclosed in deep fossa. Ridges, prominences more marked in juvenile than adult. Rostrum straight, triangular. Anterolateral margin of carapace with 5 teeth. Chelipeds unequal, right one larger; coxa granulated, lower margin of ischium, merus with 3–4 blunt teeth, upper surface of merus toothed. Pereopods 2–4 with crest along anterior margin. Abdomen tubeculate. Juveniles with more spines than adults, carapace more angular, appendages more stout, short. Carapace length to 71.4 mm.
 Color in life. Not reported.
 Habitat and depth. Continental shelf and slope, 183–800 m.
 Range. Palos Verdes Peninsula, California to off Valparaiso, Chile. Type locality Gulf of Panama (Albatross sta. 3354, 7˚ 9' 45" N, 80˚ 50' 0" W). Hendrickx & Harvey (1999) mistakenly reported the species from "Palo Alto, California", but the record in fact came from off the Palos Verdes Peninsula, Los Angeles County, California.
description: Published as part of Wicksten, Mary K., 2012, Decapod Crustacea of the Californian and Oregonian Zoogeographic Provinces 3371, pp. 1-307 in Zootaxa 3371 on pages 166-167
Burgess bounds for short character sums evaluated at forms
Creators: name: Pierce, Lillian B.
name: Xu, Junyan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: In this work we establish a Burgess bound for short multiplicative character sums in arbitrary dimensions, in which the character is evaluated at a homogeneous form that belongs to a very general class of "admissible" forms. This $n$-dimensional Burgess bound is nontrivial for sums over boxes of sidelength at least $q^β$, with $β> 1/2 - 1/(2(n+1))$. This is the first Burgess bound that applies in all dimensions to generic forms of arbitrary degree. Our approach capitalizes on a recent stratification result for complete multiplicative character sums evaluated at rational functions, due to the second author.
description: 28 pages
The Next Geminga: Deep Multiwavelength Observations of a Neutron Star Identified with 3EG J1835+5918
Creators: name: Halpern, J. P.
name: Gotthelf, E. V.
name: Mirabal, N.
name: Camilo, F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe Chandra, HST, and radio observations that reveal a radio-quiet but magnetospherically active neutron star in the error circle of the high-energy gamma-ray source 3EG J1835+5918, the brightest of the unidentified EGRET sources at high Galactic latitude. A Chandra ACIS-S spectrum of the ultrasoft X-ray source RX J1836.2+5925, suggested by Mirabal & Halpern as the neutron star counterpart of 3EG J1835+5918, requires two components: a blackbody of T~3x10^5 K and a hard tail that can be parameterized as a power law of photon index Gamma~2. An upper limit of d < 800 pc can be derived from the blackbody fit under an assumption of R = 10 km. Deep optical imaging with the HST STIS CCD failed to detect this source to a limit of V > 28.5, thus f_X/f_V > 6000 and d > 250 pc assuming the X-ray fitted temperature for the full surface. Repeated observations with the 76 m Lovell telescope at Jodrell Bank place an upper limit of < 0.1 mJy on the flux density at 1400 MHz for a pulsar with P > 0.1 s, and < 0.25 mJy for a ~10 ms pulsar at the location of RX J1836.2+5925. All of this evidence points to an older, possibly more distant version of the highly efficient gamma-ray pulsar Geminga, as the origin of the gamma-rays from 3EG J1835+5918.
description: 4 pages, 4 figures, accepted for publication in ApJ Letters
title: 02_0734
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Corales
Creators: name: Tello-Musi, José Luis
name: Ugalde, Diana
name: Simoes, Nuno
name: Guerra, Alberto
Publisher: name: Zenodo
Year: 2019
Subjects: subject: Biodiversity
subject: Caribbean
subject: Coral
subject: Ecology
subject: FOS: Biological sciences
subject: Ecosystem Ecology
subject: Gulf of Mexico
subject: Marine Biodiversity
subject: Marine Biology
subject: Marine Ecology
subject: Marine Environment
subject: Species diversity

description: This Infographic is a product of BDMY (https://www.bdmy.org.mx) project, that was produced with funds of the Harte Research Institute for Gulf of Mexico Studies, and CONABIO (Mexico).
 The information in the infographic was reviewed and validated by a group of specialists in the taxon. CC-BY-NC-ND
Relativistic corrections to the multiple scattering effect on the Sunyaev-Zel'dovich effect in the isotropic approximation
Creators: name: Itoh, Naoki
name: Kawana, Youhei
name: Nozawa, Satoshi
name: Kohyama, Yasuharu
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We extend the formalism for the calculation of the relativistic corrections to the Sunyaev-Zel'dovich effect for clusters of galaxies and include the multiple scattering effects in the isotropic approximation. We present the results of the calculations by the Fokker-Planck expansion method as well as by the direct numerical integration of the collision term of the Boltzmann equation. The multiple scattering contribution is found to be very small compared with the single scattering contribution. For high-temperature galaxy clusters of kT=15keV, the ratio of the both contributions is -0.2% in the Wien region. In the Rayleigh--Jeans region the ratio is -0.03%. Therefore the multiple scattering contribution is safely neglected for the observed galaxy clusters.
description: 13 pages, 3 figures, MNRAS style file (mn.sty) is used, submitted to MNRAS
Interpreting and Improving Adversarial Robustness of Deep Neural Networks with Neuron Sensitivity
Creators: name: Zhang, Chongzhi
name: Liu, Aishan
name: Liu, Xianglong
name: Xu, Yitao
name: Yu, Hang
name: Ma, Yuqing
name: Li, Tianlin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Deep neural networks (DNNs) are vulnerable to adversarial examples where inputs with imperceptible perturbations mislead DNNs to incorrect results. Despite the potential risk they bring, adversarial examples are also valuable for providing insights into the weakness and blind-spots of DNNs. Thus, the interpretability of a DNN in the adversarial setting aims to explain the rationale behind its decision-making process and makes deeper understanding which results in better practical applications. To address this issue, we try to explain adversarial robustness for deep models from a new perspective of neuron sensitivity which is measured by neuron behavior variation intensity against benign and adversarial examples. In this paper, we first draw the close connection between adversarial robustness and neuron sensitivities, as sensitive neurons make the most non-trivial contributions to model predictions in the adversarial setting. Based on that, we further propose to improve adversarial robustness by constraining the similarities of sensitive neurons between benign and adversarial examples which stabilizes the behaviors of sensitive neurons towards adversarial noises. Moreover, we demonstrate that state-of-the-art adversarial training methods improve model robustness by reducing neuron sensitivities which in turn confirms the strong connections between adversarial robustness and neuron sensitivity as well as the effectiveness of using sensitive neurons to build robust models. Extensive experiments on various datasets demonstrate that our algorithm effectively achieves excellent results.
description: Accepted by IEEE Transaction on Image Processing
Metadata record for the manuscript: A Tyrosine Kinase Inhibitor- Induced Interferon Response Positively Associates with Clinical Response in EGFR-Mutant Lung Cancer
Creators: name: Gurule, Natalia J.
name: McCoach, Caroline E.
name: Hinz, Trista K.
name: Merrick, Daniel T.
name: Bokhoven, Adriaan Van
name: Kim, Jihye
name: Patil, Tejas
name: Calhoun, Jacob
name: Nemenoff, Raphael A.
name: Tan, Aik Choon
name: Doebele, Robert C.
name: Heasley, Lynn E.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biological Sciences not elsewhere classified
subject: Oncology and Carcinogenesis not elsewhere classified
subject: Cancer
subject: Immunology
subject: FOS: Clinical medicine
subject: Medical and Health Sciences not elsewhere classified

description: Summary

This
metadata record provides details of the data supporting the claims of the
related manuscript: “A Tyrosine Kinase Inhibitor- Induced
Interferon Response Positively Associates with Clinical Response in EGFR-Mutant
Lung Cancer”.

The
related study explored rapid transcriptional responses induced by tyrosine
kinase inhibitors (TKIs) early in cancer treatment that associate with the
range of patient responses

Type of data:
RNA sequencing

Subject of
data: EGFR mutant cell lines treated in vitro with osimertinib; Homo sapiens: tumour biopsies of 8 EGFR
mutant lung cancer patients; NU/NU mice

Data
access

The RNA sequencing data are openly
available in the Gene Expression Omnibus
(GEO) repository via the following accession: https://identifiers.org/geo:GSE165019. Additional files available at GEO are: PC9_ in
vitro_genes.fpkm_table.xlsx, H1650_in_vitro_genes.fpkm_table.xlsx, 4006_ in
vitro_genes.fpkm_table.xlsx,H1975_in_vitro_genes.fpkm_table.xlsx, EarlyRebiopsy_genes.fpkm_table.xslx,
invivoH1650_ PC9 _AZD9291 _genes.fpkm_table.xlsx. All the GEO data will be made publicly available within one year of the
publication of the article.

Other data generated and analysed
during the related study are in the following Prism and Excel files: Figure2.pzfx,
Figure3.pzfx, Figure5.pzfx, SF1.pzfx, SF3.pzfx, SF.4pzfx, S5.pzfx, S6.pzfx, SuppTable1.xslx,
SuppTable2.xlsx, SuppTable3.xslx. These files are not openly available, but can
be made available upon written request to the corresponding authors.

Human subject data (de-identified
and anonymised) can be made available upon request to the corresponding
authors.

Corresponding author(s) for this study

Lynn
E. Heasley, PhD, Department of Craniofacial Biology, School of Dental Medicine,
University of Colorado Anschutz Medical Campus, 12801 E. 17th Ave, Aurora, CO
80045, Lynn.Heasley@cuanschutz.edu and Robert C. Doebele, MD, PhD, Division of
Medical Oncology, Department of Medicine, School of Medicine, University of
Colorado Anschutz Medical Campus, 12801 E. 17th Ave, Aurora, CO 80045,
Robert.Doebele@cuanschutz.edu

Study
approval

Institutional
Review Board of the University of Colorado approved protocol (COMIRB #15-2316)
and the University of California, San Francisco approved protocol (CC IRB #
13-6512).