cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
First Investigation of the Clustering Environment of Damped Lyman Alpha Absorbers at z=4
Creators: name: Gawiser, Eric
name: Wolfe, Arthur M.
name: Prochaska, Jason X.
name: Lanzetta, Kenneth M.
name: Yahata, Noriaki
name: Quirrenbach, Andreas
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the first observations of the clustering environment of damped Lyman alpha absorption systems at z=4. Color selection and photometric redshifts were used to select 44 candidate Lyman-break galaxies brighter than I_AB=25.5 from deep BRI images of the 35 sq. arcmin field containing the quasar BR 0951-04. Multislit spectroscopy of 35 candidate galaxies was performed and 8 of these candidates have been confirmed as z>3.5 Lyman-break galaxies. With only BRI photometry, the photometric redshifts are quite accurate for the spectroscopically confirmed galaxies but have a high rate of misclassification due to color degeneracies between Lyman-break galaxies and low-redshift ellipticals. Both of the z>3.5 galaxies found within 15'' of the quasar line-of-sight appear to be causing absorption systems in the quasar spectrum. We use a battery of statistical tests to look for clustering in the redshift histogram of the z>3.5 galaxies but do not find measurable clustering of these Lyman-break galaxies with the damped Lyman alpha absorbers. With a larger sample of galaxies, our method should determine the cross-correlation between these objects, which probes the bias and hence the mass of the damped Lyman alpha absorbers.
description: submitted to ApJ, revised version in response to referee's comments, one conclusion changed, 9 pages including 3 color figures
Applying Probabilistic Programming to Affective Computing
Creators: name: Ong, Desmond C.
name: Soh, Harold
name: Zaki, Jamil
name: Goodman, Noah D.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Affective Computing is a rapidly growing field spurred by advancements in artificial intelligence, but often, held back by the inability to translate psychological theories of emotion into tractable computational models. To address this, we propose a probabilistic programming approach to affective computing, which models psychological-grounded theories as generative models of emotion, and implements them as stochastic, executable computer programs. We first review probabilistic approaches that integrate reasoning about emotions with reasoning about other latent mental states (e.g., beliefs, desires) in context. Recently-developed probabilistic programming languages offer several key desidarata over previous approaches, such as: (i) flexibility in representing emotions and emotional processes; (ii) modularity and compositionality; (iii) integration with deep learning libraries that facilitate efficient inference and learning from large, naturalistic data; and (iv) ease of adoption. Furthermore, using a probabilistic programming framework allows a standardized platform for theory-building and experimentation: Competing theories (e.g., of appraisal or other emotional processes) can be easily compared via modular substitution of code followed by model comparison. To jumpstart adoption, we illustrate our points with executable code that researchers can easily modify for their own models. We end with a discussion of applications and future directions of the probabilistic programming approach.
description: Accepted by IEEE Transactions on Affective Computing. 12 pages, 6 figures
Badioglobus tapanti Short, 2004, new species
Creators: name: Short, Andrew Edward Z.
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Hydrophilidae
Badioglobus
Badioglobus tapanti

description: Badioglobus tapanti, new species
(Figs. 1–4)
 Type Locality. Costa Rica, Cartago Province, Tapanti National Park.
 Descripton. Length 6.7–7.5 mm. Dorsum and venter reddish brown. Punctation on clypeus dense, moderately impressed; distance between punctures 1.0–1.5 3 width of one puncture; punctation of pronotum and elytra less impressed and slightly less dense. Aedeagus (Fig. 1) with parameres and median lobe equal in length; parameres flattened laterally; tips of parameres curved ventrally in lateral view. See generic diagnosis for additional characters.
 Biology and Distribution. Broadly distributed in Costa Rica. Specimens were collected at lights, litter samples, and malaise traps. Immature stages unknown.
 Material Examined. HOLOTYPE. Male. ‘‘Quebrada Segunda, P. N. Tapanti/ 1,230 m, Prov. Cart., COSTA/ RICA. May 1993. G. Mora./ L-N-194000, 560000,’’ ‘‘ Holotype / Badioglobus / tapanti/ A. E. Z. Short’’ (INBIO). PARATYPES. (41). COSTA RICA: Cartago Province, Tapanti National Park, Quebrada Segunda, G. Morra, alt. 1,250 m. Various Dates: May 1992 (AEZS, 1; CNCC, 1; INBIO, 1), June 1992 (AEZS, 1; USNM 1; INBIO, 1), July 1992 (AEZS, 1; CNCC, 1; INBIO, 4), Aug. 1992 (CUIC, 2; USNM, 1; INBIO, 4), Sept. 1992 (INBIO, 2), Oct. 1992, (INBIO, 1), Mar. 1993 (INBIO, 2), May 1993 (CNIC, 1; INBIO, 1), Oct. 1993 (USNM, 2; NHMV, 1; INBIO, 2); Cartago Province, Grano de Oro, Chirripo, Turrialba, P. Campos, alt. 1,120 m, Sept. 1992 (NHMV, 1; INBIO, 1). Guanacaste Province: Rio San Lorenzo, C. Alvarado, alt. 1,050 m, Jul. 1991 (INBIO, 1). Alajuela Province: Rio San Lorencito, Res. For. San Ramon, 5 km N. Col. Palmarena, alt. 900 m, Mar. 1990 (INBIO, 1); San Ramon, Alberto Branes station, Rio San Lorencito, C. Rojas, alt. 800 m, 30 June 1999 (INBIO, 1); San Ramon, Alberto Branes station, Rio San Lorencito, E. Ulate & A. Mora, alt. 850 m, 30 June–5 July 1999 (INBIO, 1); Volcan Tenorio N. P., Upala, Bijagua, Sand Heliconias, A. Lopez, 17 Aug–17 Sept. 2000 (INBIO, 1); Guanacaste N. P., San Ramon Sta., alt, 620 m, 10–21 June, 1994 (INBIO, 1); Upala Bijagua, Heliconias Sta., A. Lopez, 680 m, 16 Sept. 2001 (INBIO, 1); Upala, Alb. Heliconias, Send. Heliconias, alt. 700 m, A. Lopez, 3 Aug. 2000 (AEZS, 1).
 Etymology. Named after its type locality, Tapanti National Park.
description: Published as part of Short, Andrew Edward Z., 2004, A New Genus and Species of Sphaeridiinae from Costa Rica (Coleoptera: Hydrophilidae), pp. 534-537 in The Coleopterists Bulletin 58 (4) on page 536, DOI: 10.1649/375, http://zenodo.org/record/10104209
Self-similar evolution of wind-blown bubbles with mass loading by hydrodynamic ablation
Creators: name: Pittard, J. M.
name: Hartquist, T. W.
name: Dyson, J. E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present similarity solutions for adiabatic bubbles that are blown by winds having time independent mechanical luminosities and that are each mass-loaded by the hydrodynamic ablation of distributed clumps. The mass loading is `switched-on' at a specified radius (with free-expansion of the wind interior to this point) and injects mass at a rate per unit volume proportional to M^delta r^lambda where delta = 4/3 (1) if the flow is subsonic (supersonic) with respect to the clumps. In the limit of negligible mass loading a similarity solution found by Dyson (1973) for expansion into a smooth ambient medium is recovered. The presence of mass loading heats the flow, which leads to a reduction in the Mach number of the supersonic freely-expanding flow, and weaker jump conditions across the inner shock. In solutions with large mass loading, it is possible for the wind to connect directly to the contact discontinuity without first passing through an inner shock. For a solution that gives the mass of swept-up ambient gas to be less than the sum of the masses of the wind and ablated material, lambda < -2. Maximum possible values for the ratio of ablated mass to wind mass occur when mass loading starts very close to the bubble center and when the flow is supersonic with respect to the clumps over the entire bubble radius. The maximum temperature in the bubble often occurs near the onset of mass loading, and in some cases can be many times greater than the post-inner-shock temperature. Our solutions are relevant to eg stellar wind-blown bubbles, galactic winds, etc. This work complements Pittard et al (2001) where it was assumed that clumps were evaporated through conductive energy transport.
description: 13 pages, 7 figures, to be published in A&A
Moraceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Moraceae

description: Moraceae.
Ficus ovata Vahl.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 160, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Gigacuma Kurian 1951
Creators: name: Haye, Pilar A.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Cumacea
Bodotriidae
Gigacuma

description: GIGACUMA KURIAN, 1951
 Type species: Gigacuma halei Kurian, 1951
 Body: Carapace shorter than abdomen and peraeon; abdomen longer than carapace and peraeon together.
 Cephalothorax: From dorsal view the carapace may be laterally compressed anteriorly. Pseudorostral lappets may extend beyond frontal lobe towards midline but do not meet (or partially meet leaving a suture between them). Antennal notch as a depression or as a subacute incision. Anterolateral corner bluntly rounded or with subacute tooth. Frontal lobe 1/5 or less of the carapace length; as wide as long; anteriorly linguiform; with ocular pigment and eye lenses.
Antenna 1 with basal article of the peduncle straight; same length or shorter than the other two articles together. Main flagellum bi-articulated; may have two aesthetascs in distal-most article and/or a group of aesthetascs on proximal article. Accessory flagellum bi-articulated; with brush of setae. Antenna 2 in males reaching end of pleon; with sensory setae on anterior margin of article 4. Antenna 2 in females with three articles.
Maxilliped 3 basis straight or arcuate; extended dorso-distally over ischium beyond the articulation of the ischium and merus. Ischium shorter or same size as merus. Merus expanded laterally. Carpus oviform; equal to or shorter than propodus and dactylus together. Propodus distally widened; with a brush of setae.
 Peraeon: First peraeonite visible only above lateral midline. Peraeonite 2 may have ventrolateral expansion overriding peraeonite 1 and/or carapace or not overriding other somites. Peraeonite 3 extended backwards overriding peraeonite 4 or forward and backwards overriding peraeonites 2 and 4. Peraeonite 4 with ventrolateral expansion overriding peraeonite 5.
Females and males with fully developed exopods on peraeopods 1 and 2. Peraeopod 1 with basis arcuate, with row of setae, slightly projected ventrally; brush (3 or more) of long setae on the propodus (setae longer than carpus); carpus shorter than propodus. Peraeopod 2 with ischium; dactylus longer than propodus. Peraeopod 4 with ischium.
 Pleon: Pleonite 6 longer than wide; longer than or as long as peduncle of uropod. Wide portion of distal end of pleonite 6 slightly extended past the insertion of the uropods and apex rounded.
Uropod endopod bi-articulated; proximal article shorter than distal one. Uropod exopod with proximal article shorter than distal one. Peduncle of uropods slightly longer than rami; rami approximately same length. Males with five pairs of pleopods. Pleopodal endopod without process.
 Species included:
 1. G. halei Kurian, 1951
 Distribution: Indo-West Pacific from 7 to 27 m.
description: Published as part of Haye, Pilar A., 2007, Systematics of the genera of Bodotriidae (Crustacea: Cumacea), pp. 1-58 in Zoological Journal of the Linnean Society 151 (1) on page 27, DOI: 10.1111/j.1096-3642.2007.00322.x, http://zenodo.org/record/5428051
Portraying Double Higgs at the Large Hadron Collider
Creators: name: Kim, Jeong Han
name: Kim, Minho
name: Kong, Kyoungchul
name: Matchev, Konstantin T.
name: Park, Myeonghun
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We examine the discovery potential for double Higgs production at the high luminosity LHC in the final state with two $b$-tagged jets, two leptons and missing transverse momentum. Although this dilepton final state has been considered a difficult channel due to the large backgrounds, we argue that it is possible to obtain sizable signal significance, by adopting a deep learning framework making full use of the relevant kinematics along with the jet images from the Higgs decay. For the relevant number of signal events we obtain a substantial increase in signal sensitivity over existing analyses. We discuss relative improvements at each stage and the correlations among the different input variables for the neutral network. The proposed method can be easily generalized to the semi-leptonic channel of double Higgs production, as well as to other processes with similar final states.
description: 37 pages. Matched to published version. Revisions in section 1, 2. Replaced figures. Added references. Conclusions unchanged
DID JESUS STUDY VEDANTA?
Creators: name: Dr. Alan Wenham-Prosser DProf., MA.
Publisher: name: Zenodo
Year: 2018
Subjects: Vedanta
Jesus teachings
Eurocentricism
Upanishads

description: A study which seeks to unravel the many centuries of false ways of the jumbled Christian ideas. And to show that Jesus lived at a time and in a land where it was known that a higher culture existed in India. And to show that his teaching is proof that he went there to get instruction on the mysteries of the real purpose of human life.
Osmundaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Osmundales
Osmundaceae

description: Osmundaceae.
Osmunda regalis L.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 160, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Letter from Alice R. Appenzeller to William Elliot Griffis, December 29, 1912
Creators: name: Appenzeller, Alice R.
Publisher: name: No Publisher Supplied
Year: 1912

description: Extends Christmas salutations, and thanks Griffis for the present (rose and silver star). Provides details of Christmas festivities; Henry, Mary, and Ida (sick) all home, college day at Wellesley Club of S.E. PA. Inquires about Katherine. Describes her plans to travel to Providence.
Goliathini Hope 1831
Creators: name: Nogueira, Guillermo
name: Morón, Miguel-Angel
name: Fierros-López, Hugo-Eduardo
name: Navarrete-Heredia, José-Luis
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae

description: Larvae of Goliathini  Few larvae of Goliathini from the world are described. Consequently, it is difficult to get a set of diagnostic characters that aid in distinguishing the larvae of the tribe Goliathini from the larvae of other Cetoniinae. But as a preliminary introduction, based on Oberholzer (1959), Jerath and Unny (1965), Ritcher (1966), Lumaret (1985), Donaldson (1987) and Morón and Arce (2002), we propose the following combination of characters as the diagnosis for the larvae of Goliathini: Frons with 1 posterior frontal seta at each side. Labrum symmetrical, anterior border trilobed. Clithra present. Plegmata absent. Scissorial area of right mandible with 2–4 teeth. Scissorial area of right mandible with 3–4 teeth. Mala with 1 terminal uncus, well-developed, conical, and 2–3 subterminal unci closely fused. Maxillary stridulatory area consisting of a row of 5–8 curved teeth with anteriorly projecting points. Ocelli present, vaguely defined or absent. Last antennal segment with 2–10 dorsal sensory spots. Tarsungulus cylindrical, rounded apically, bearing 6–15 setae, or with falcate process bearing 2–6 setae. Dorsa of abdominal segments 9 and 10 fused. Respiratory plate of spiracle of 8th abdominal segment slightly smaller than preceeding respiratory plates, or as large as these. Raster with or without longitudinal palidia, if present, each monostichous palidium with 7–38 pali.
description: Published as part of Nogueira, Guillermo, Morón, Miguel-Angel, Fierros-López, Hugo-Eduardo & Navarrete-Heredia, José-Luis, 2004, The Immature Stages of Neoscelis Dohrni (Westwood) (Coleoptera: Scarabaeidae: Cetoniinae: Goliathini) with Notes on Adult Behavior, pp. 171-183 in The Coleopterists Bulletin 58 (2) on page 172, DOI: 10.1649/604, http://zenodo.org/record/10104282
Massive star formation in 100,000 years from turbulent and pressurized molecular clouds
Creators: name: McKee, Christopher F.
name: Tan, Jonathan C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Massive stars (with mass m_* > 8 solar masses) are fundamental to the evolution of galaxies, because they produce heavy elements, inject energy into the interstellar medium, and possibly regulate the star formation rate. The individual star formation time, t_*f, determines the accretion rate of the star; the value of the former quantity is currently uncertain by many orders of magnitude, leading to other astrophysical questions. For example, the variation of t_*f with stellar mass dictates whether massive stars can form simultaneously with low-mass stars in clusters. Here we show that t_*f is determined by conditions in the star's natal cloud, and is typically ~10^5 yr. The corresponding mass accretion rate depends on the pressure within the cloud - which we relate to the gas surface density - and on both the instantaneous and final stellar masses. Characteristic accretion rates are sufficient to overcome radiation pressure from ~100 solar mass protostars, while simultaneously driving intense bipolar gas outflows. The weak dependence of t_*f on the final mass of the star allows high- and low-mass star formation to occur nearly simultaneously in clusters.
description: 9 pages plus 2 figures, Nature, 416, 59 (7th March 2002)
On cross-correlogram IRF's estimators of two-output systems in spaces of continuous functions
Creators: name: Blazhievska, Irina
name: Zaiats, Vladimir
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 60F17, 60G10, 60G17

description: In this paper, single input--double output linear time-invariant systems are studied. Both components of system's impulse response function (IRF) are supposed to be real-valued and square-integrable. One component is unknown while the second one is controlled. The problem is to estimate the unknown component after observations of the other component. We apply cross-correlating of the outputs given that the input is a standard Wiener process. Weak asymptotic normality of appropriately centred estimators in spaces of continuous functions is proved. This enables us to construct confidence intervals in these spaces. Our results employ techniques related to Gaussian processes and bilinear forms of Gaussian processes.
description: 25 pages, 11 Postscript figures
P=W Phenomena
Creators: name: Harder, Andrew
name: Katzarkov, Ludmil
name: Przyjalkowski, Victor
Publisher: name: arXiv
Year: 2019
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: In this paper, we describe recent work towards the mirror P=W conjecture, which relates the weight filtration on a cohomology of a log Calabi--Yau manifold to the perverse Leray filtration on the cohomology of the homological mirror dual log Calabi--Yau manifold, taken with respect to the affinization map. This conjecture extends the classical relationship between Hodge numbers of mirror dual compact Calabi--Yau manifolds, incorporating tools and ideas which appear in the fascinating and groundbreaking works of de Cataldo, Hausel, and Migliorini, and de Cataldo and Migliorini. We give a broad overview of the motivation for this conjecture, recent results towards it, and describe how this result might arise from the SYZ formulation of mirror symmetry. This interpretation of the mirror P=W conjecture provides a possible bridge between the mirror P=W conjecture and the well-known P=W conjecture in nonabelian Hodge theory.
description: 11 pages
Spectroscopic Signatures of Convection in the Spectrum of Procyon. Fundamental Parameters and Iron Abundance
Creators: name: Prieto, Carlos Allende
name: Asplund, Martin
name: Lopez, Ramon J. Garcia
name: Lambert, David L.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have observed the spectrum of Procyon A (F5IV) from 4559 to 5780 A with a S/N of ~ 1e3 and a resolving power of 2e5. We have measured the line bisectors and relative line shifts of a large number of Fe I and Fe II lines, comparing them to those found in the Sun. A three-dimensional(3D) hydrodynamical model atmosphere has been computed and is tested against observations. The model reproduces in detail most of the features observed, although we identify some room for improvement. At all levels, the comparison of the 3D time-dependent calculations with the observed spectral lines shows a much better agreement than for classical homogeneous models, making it possible to refine previous estimates of the iron abundance, the projected rotational velocity, the limb-darkening, and the systemic velocity of the Procyon binary system. The difference between the iron abundance determined with the 3D model and its 1D counterpart is
description: 30 pages, 19 figures; uses emulateapj.sty (included); to appear in ApJ (Feb 2002)
Penicillilactone A, a novel antibacterial 7-membered lactone derivative from the sponge-associated fungus Penicillium sp. LS54
Creators: name: Liu, Yong
name: Ding, Lijian
name: Fang, Fang
name: He, Shan
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biochemistry
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Plant Biology

description: One novel 7-membered lactone derivative, penicillilactone A (1), together with two known compounds, rugulosin A (2) and rugulosin (3) were isolated from the sponge-derived fungus Penicillium sp. LS54. Their structures were elucidated on the basis of spectroscopic analysis and comparison with literature data. Remarkably, penicillilactone A (1) is the first natural product containing a 7-membered lactone ring fused with a furan core. Penicillilactone A (1) exhibited moderate antibacterial activity against aquatic pathogen Vibrio harveyi with an MIC value of 8 μg/mL.
Coupling parameters and the form of the potential via Noether symmetry
Creators: name: Sanyal, A. K.
name: Rubano, C.
name: Piedipalumbo, E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We explore the conditions for the existence of Noether symmetries in the dynamics of FRW metric, non minimally coupled with a scalar field, in the most general situation, and with nonzero spatial curvature. When such symmetries are present we find general exact solution for the Einstein equations. We also show that non Noether symmetries can be found. Finally,we present an extension of the procedure to the Kantowski- Sachs metric which is particularly interesting in the case of degenerate Lagrangian.
description: 13 pages, no figures
Hypocuma Jones 1973
Creators: name: Haye, Pilar A.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Cumacea
Bodotriidae
Hypocuma

description: HYPOCUMA JONES, 1973
 Type species: Hypocuma serratifrons Jones, 1973
 Body: Carapace shorter than abdomen and longer than peraeon; abdomen longer than carapace and peraeon together.
 Cephalothorax: From dorsal view the carapace appears laterally compressed anteriorly. Carapace with mid-dorsal ridge or mid-dorsal serration. Pseudorostral lappets extend beyond frontal lobe and meet in midline. Antennal notch not distinct. Anterolateral corner bluntly rounded. Frontal lobe from 1/4 of carapace length; as wide as long or wider than long; not extended; without ocular pigment or eye lenses.
Antenna 1 with basal article of the peduncle arcuate or straight; longer than the other two articles together or as long as the other two articles together. Main flagellum uni-, bi- or tri-articulated; with second article longer than third; with two aesthetascs in distal-most article. Accessory flagellum uni- or bi-articulated. Antenna 2 in males with sensory setae on anterior margin of article four. Antenna 2 in females with five articles.
Maxilliped 3 basis geniculate or arcuate; not projected over ischium. Ischium shorter than merus. Merus extended dorso-distally over carpus. Carpus may be oviform; equal to or shorter than propodus and dactylus together. Propodus may be oviform.
 Peraeon: First peraeonite well exposed. Peraeonite 2 narrow or proportional to other peraeonites; with ventrolateral expansion overriding peraeonite 1 and/or carapace or peraeonite 3. Peraeonite 3 extended forward overriding peraeonite 2 or backwards overriding peraeonite 4. Peraeonite 4 with ventrolateral expansion overriding peraeonite 3, peraeonite 5 or peraeonites 3 and 5.
Females and males with fully developed exopods on peraeopods 1–3. Females with reduced exopods on peraeopod 4, while males have them fully developed. Peraeopod 1 with basis arcuate; carpus same size as propodus. Peraeopod 2, ischium present; dactylus longer than propodus. Peraeopod 4 with ischium.
 Pleon: Pleonite 6 longer than wide; shorter than peduncle of uropod. Wide portion of distal end of pleonite 6 strongly extended past the insertion of the uropods; apex rounded.
Uropod endopod bi-articulated; proximal article longer than distal one. Uropod exopod with proximal article shorter than distal one. Peduncle of uropods slightly longer than rami; exopod longer than endopod. Males with five pairs of pleopods. Pleopodal endopod with well developed process.
 Species included:
 1. H. dentatum Day, 1975
 2. H. serratifrons Jones, 1973
 Distribution: Heterocuma dentatum is found off the southern point of South Africa at 400 m, while Heterocuma serratifrons is found in the North Atlantic at depths between 1000 and 5000 m.
description: Published as part of Haye, Pilar A., 2007, Systematics of the genera of Bodotriidae (Crustacea: Cumacea), pp. 1-58 in Zoological Journal of the Linnean Society 151 (1) on page 28, DOI: 10.1111/j.1096-3642.2007.00322.x, http://zenodo.org/record/5428051
title: Muddy Waters: A Molecular Approach to Clarifying Freshwater Mussel Diversity in Australia
Creators: name: Fawcett, James
Publisher: name: Griffith University
Year: 2009
Subjects: subject: Freshwater mussels
subject: Invertebrate protection
subject: Mussel taxonomy
subject: Australian mussel diversity
subject: Lake Eyre
subject: Gulf of Carpentaria Rivers

description: Historically, when the terms “conservation, threatened, endangered or extinct” were used, it was in reference to vertebrate animal species. Funding for conservation and policy implementation for protection of invertebrates has historically been difficult, even though 95% of all animal species are invertebrates and are an important component of many ecosystems. Human impact on the earth has influenced the natural population structure of many organisms, through habitat destruction, fragmentation and degradation. Issues that affect population structure and dispersal are heightened when that species is confined to a specific range or habitat. This is especially paramount for aquatic organisms with the slightest change in weather pattern, damage to riparian zones or the stream environment, or alteration to stream engineering and water flow resulting in significant impacts to the stream biota. Freshwater mussels are organisms that have been found to be seriously affected by changes to stream conditions. Because mussels filter the water column, they are generally the first group of animals to react if contaminants enter a system and as a result freshwater mussels are considered by many scientific and government agencies worldwide as key indicator species for stream health assessments. Freshwater mussel conservation is a relatively unexplored field within Australia and little is known about mussel recruitment and patterns of population connectivity. Mussel taxonomy in Australia is based entirely on shell morphology, although local environmental conditions have been shown to have significant effects on shell morphology. Therefore, basing taxonomy purely on shell morphological characteristics may not to be systematically meaningful. Before effective conservation measures can be implemented within Australia, clarification of contemporary mussel diversity is required.
Polygonaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae

description: Polygonaceae.
Rumex usambarensis (Dammer) Dammer.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 160, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
CII-data.xlsx
Creators: name: Yu, Yue
Publisher: name: figshare
Year: 2019
Subjects: subject: Hydrology
subject: 40608 Surfacewater Hydrology
subject: FOS: Earth and related environmental sciences

description: CII is a dimensionless structural variable to predict canopy water storage capacity. This data can be used to validate the potential of CII to predict canopy water storage capacity, as well as used to compare with other structural variables.
Poaceae Barnhart 1895
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae

description: Poaceae.
Hyparrhenia cymbaria (L.) Stapf, Hyparrhenia newtonii (Hack.) Stapf, Hyparrhenia rufa (Nees) Stapf, Loudetia kagerensis (K.Schum.) C.E.Hubb. ex Hutch., Oplismenus compositus (L.) P.Beauv., Pennisetum polystachion (L.) Schult., Setaria kagerensis Mez, Setaria pumila (Poir.) Roem. & Schult., Urelytrum digitatum K.Schum.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 160, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Neoscelis Schoch 1897
Creators: name: Nogueira, Guillermo
name: Morón, Miguel-Angel
name: Fierros-López, Hugo-Eduardo
name: Navarrete-Heredia, José-Luis
Publisher: name: Zenodo
Year: 2004
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cetoniidae
Neoscelis

description: Larvae of Neoscelis Schoch, 1897
 The larval description of Neoscelis dohrni (Westwood) that follows is the first for the genus. Larvae of Neoscelis appear to be most similar morphologically to those of African species of Chlorocala Kirby (¼ Smaragdesthes Kraatz). The known larva of Neoscelis have the ocelli weakly defined, haptomeral region with 17 heli in a transverse row, last antennal segment with 3 dorsal sensory spots, tarsungulus bearing 9–11 setae, and each palidium consisting of a row of 10–11 pali. Larvae of Chlorocala have the last antennal segment with 9 sensory spots, tarsungulus bearing 14–15 setae, and each palidium consisting of a row of 12–13 pali.
 The genus Neoscelis consist of two species that are found from south of Sonora to central Guerrero in western Mexico (Morón and Ratcliffe 1984; Morón et al. 1997). Adults of Neoscelis dohrni are active during August to November, flying in oak forests and deciduous tropical forests, as well as in old orchads or unused crop lands located between 1,000 to 1,700 m altitude, where they have been collected with rotting fruit traps and directly on host plants: Nicotiana glauca Graham (Solanaceae) and Quercus resinosa Liebmann, Q. magnoliaefolia Née (Fagaceae), Verbesina greenmanii Urban (Asteraceae), Caesalpinia pulcherrima (Linne´)Sw., and Acacia pennatula (Schl.and Cham.) Stand. (Leguminosae). Other species of Cetoniinae feeding in the same host were Cotinis mutabilis (Gory and Percheron), Hologymnetis cinerea (Gory and Percheron), Euphoria biguttata Gory and Percheron, E. leucographa Gory and Percheron and, rarely Ischnoscelis hoepfneri (Gory and Percheron). The larvae of N. dohrni feed in rich organic soil.
description: Published as part of Nogueira, Guillermo, Morón, Miguel-Angel, Fierros-López, Hugo-Eduardo & Navarrete-Heredia, José-Luis, 2004, The Immature Stages of Neoscelis Dohrni (Westwood) (Coleoptera: Scarabaeidae: Cetoniinae: Goliathini) with Notes on Adult Behavior, pp. 171-183 in The Coleopterists Bulletin 58 (2) on page 174, DOI: 10.1649/604, http://zenodo.org/record/10104282
Critically Examining the "Neural Hype": Weak Baselines and the Additivity of Effectiveness Gains from Neural Ranking Models
Creators: name: Yang, Wei
name: Lu, Kuang
name: Yang, Peilin
name: Lin, Jimmy
Publisher: name: arXiv
Year: 2019
Subjects: subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: Is neural IR mostly hype? In a recent SIGIR Forum article, Lin expressed skepticism that neural ranking models were actually improving ad hoc retrieval effectiveness in limited data scenarios. He provided anecdotal evidence that authors of neural IR papers demonstrate "wins" by comparing against weak baselines. This paper provides a rigorous evaluation of those claims in two ways: First, we conducted a meta-analysis of papers that have reported experimental results on the TREC Robust04 test collection. We do not find evidence of an upward trend in effectiveness over time. In fact, the best reported results are from a decade ago and no recent neural approach comes close. Second, we applied five recent neural models to rerank the strong baselines that Lin used to make his arguments. A significant improvement was observed for one of the models, demonstrating additivity in gains. While there appears to be merit to neural IR approaches, at least some of the gains reported in the literature appear illusory.
description: Published in the Proceedings of the 42nd Annual International ACM SIGIR Conference on Research and Development in Information Retrieval (SIGIR 2019)
Some aspects of Shang administration : a survey based solely on the evidence available in the oracle bone texts
Creators: name: Chou, Hung-Hsiang
Publisher: name: The Australian National University
Year: 1968
Subjects: subject: Oracle bones
subject: China History Shang dynasty, 1766-1122 B.C
subject: China Politics and government 1766-1122 B.C

description: Although this survey is particularly concerned with aspects of administration in Shang times and is essentially historical in scope, it has nevertheless become considerably involved with problems of presentation, not the least of which is the rendering in English both the content of the oracular texts and notes on individual characters and phrases. It is the first attempt in English or in any other Western language substantial number of oracle bone texts in translation. Accordingly, the first problem - which has been found an especially difficult one - concerns the transcription of the archaic graph into a modern character equivalent or into a modern character form. To the Chinese or Japanese reader this is not regarded as a particularly important matter, but once it becomes necessary to render archaic text into an entirely different language, transcription becomes an unexpectedly significant matter - of this there will be more to discuss shortly. Secondly, meanings must be carefully investigated and especial care taken when they are to be expressed in an alien language - when writing in his own language a Chinese and also a Japanese, can sometimes side-step a problem because there exists an intrinsic element of a partial understanding - an emotional assessment - but one which perhaps does not always really amount to an actual understanding. Only when the precision required in translation arises do we come to appreciate that the problem has unconsciously been side-stepped. For one who has, at one stage or another during the compilation of this survey, had to reconsider various long accepted view-points then to revise a longcherished understanding of them, it has necessitated considerable readjustment in interpretation.
Constrained Simulations of the Real Universe: the Local Supercluster
Creators: name: Klypin, Anatoly
name: Hoffman, Yehuda
name: Kravtsov, Andrey
name: Gottloeber, Stefan
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present cosmological simulations which closely mimic the real Universe within 100Mpc of the Local Group. The simulations, called Constrained Simulations, reproduce the large-scale density field with major nearby structures, including the Local Group, the Coma and Virgo clusters, the Great Attractor, the Perseus-Pices, and the Local Supercluster, in approximately correct locations. The MARK III survey of peculiar velocities of the observed structures inside 80Mpc/h sphere is used to constrain the initial conditions. Fourier modes on scales larger then 5Mpc/h are dominated by the constraints, while small scale waves are random. The main aim of this paper is the structure of the Local Supercluster (LSC; 30Mpc/h around the Virgo cluster) and the Local Group environment. We find that at the current epoch most of the mass (7.5e14Msun/h) of the LSC is located in a filament roughly centered on the Virgo cluster and extending over 40Mpc/h. The simulated Local Group (LG) is located in an adjacent smaller filament, which is not a part of the main body of the LSC, and has a peculiar velocity of 250kms toward the Virgo cluster. The peculiar velocity field in the LSC region is complicated and is drastically different from the field assumed in the Virgocentric infall models. The peculiar velocity flow in the vicinity of the LG in the simulation is ``cold'': the peculiar line-of-sight velocity dispersion within 7Mpc/h of the LG is less than 60km/s, comparable to the observed velocity dispersion of nearby galaxies.
description: 22 pages, 9 figures, submitted to ApJ, high resolution version is available at http://astro.nmsu.edu/~aklypin/HOFFMAN
Disclosing the true nature of the Sy 2 galaxy NGC 3281: one more Compton-thick source
Creators: name: Vignali, C.
name: Comastri, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the BeppoSAX broad-band X-ray spectrum of the Seyfert 2 galaxy NGC 3281. The source high-energy spectrum is characterized by the nuclear transmitted component, with an absorbing column density of about 2 10^24 cm^-2, while the MECS spectrum is reflection-dominated, with a prominent (EW about 0.5-1.2 keV) iron K_alpha emission line. The source is detected at only the 5 sigma significance level in the LECS band, because of the strong obscuration which hampers at low energies the direct view of the active nucleus harbored in NGC 3281. BeppoSAX results are consistent with the scenario where NGC 3281 is inclined more than 60 degrees with respect to the line-of-sight. Combining the N_H value obtained from the present X-ray analysis with the A_V measurement, a N_H/A_V about 50 times the Galactic value is derived.
description: 7 pages, 5 figures included, accepted for publication by Astronomy & Astrophysics
The analysis of red giant branch photometry in galaxies
Creators: name: Frayn, C. M.
name: Gilmore, G. F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an analysis of the many possible methods for simulating and analysing colour-magnitude diagrams, with application to studies of the field halo stellar populations of resolved galaxies. Special consideration is made to the analysis of stars on the Red Giant branch (RGB), and methods for obtaining metallicity distributions for old populations based on analysis of evolved sections of the Colour Magnitude Diagram (CMD). These tools are designed to provide a reliable and accurate method for the analysis of resolved Population II stars in the haloes of nearby galaxies. In particular, we introduce a Perpendicular Distance method for calculating most likely source isochrones for stars in our input dataset. This method is shown to have several advantages over a more traditional approach considering the isochrone as a set of finely-spaced Gaussian probability distributions. We also consider methods by which the obtained metallicity distribution might be most efficiently optimised and especially evaluate the difficulties involved in avoiding sub-optimal local maxima in the likelihood maximisation procedure.
description: 16 pages, 15 postscript figures
Additional file 1 of Accurate long-read de novo assembly evaluation with Inspector
Creators: name: Chen, Yu
name: Zhang, Yixin
name: Wang, Amy Y.
name: Gao, Min
name: Chong, Zechen
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Additional file 1: Supplementary Fig. S1-S20.
Overseas Chinese affairs of the People's Republic of China
Creators: name: Fitzgerald, Stephen
Publisher: name: The Australian National University
Year: 1969
Subjects: subject: Chinese Foreign countries
subject: China Foreign relations

description: Overseas Chinese Affairs work is concerned with the 13 million Chinese who live outside China’s borders, and with some 11 million 'domestic Overseas Chinese', the dependants and relatives who reside in China, Since the Chinese abroad are not within the direct jurisdiction of the Chinese government, administration of external policy has to depend on various forms of communication, which are for the most part indirect, and of which the most important is the domestic Overseas Chinese. The administrative organisations for Overseas Chinese work are concerned primarily with the domestic Overseas Chinese, although the ultimate justification for the existence of the category of domestic Overseas Chinese is policy towards the Chinese abroad. The Chinese Communist Party's policies for domestic Overseas Chinese provide important indications of its intentions towards the Chinese abroad. The CCP's external policy since 19^9 reflects an evolving awareness of the problems and potential of the Overseas Chinese, if there has been an 'Overseas Chinese problem' in Southeast Asia, it has also been a problem to the CCP. In the first two years of its rule, the party appears to have believed that the Overseas Chinese could be exploited successfully in the pursuit of its political objectives in Southeast Asia. There were, however, few positive initiatives until the end of 1954. In the period from 1949 to 1954, the Chinese abroad were expected to support the party's internal reforms and foreign policies; domestic Overseas Chinese were allowed some privileges, and in most respects were made to conform with policies for the Chinese masses. External propaganda tended to echo the policies of the Kuomintang, overlaid with the language of communism and internationalism» Although there were few initiatives in the period, the party appears to have formed some opinions which were important in shaping the post — 1954 policy; In particular, the failure of the Malayan insurgency appears to have alerted the party to the possible limitations of Overseas Chinese revolution.
Observational Tests and Predictive Stellar Evolution
Creators: name: Young, P. A.
name: Mamajek, E. E.
name: Arnett, David
name: Liebert, James
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare eighteen binary systems with precisely determined radii and masses from 23 to 1.1 M_sol, and stellar evolution models produced with our newly revised code TYCHO. ``Overshooting'' and rotational mixing were suppressed in order to establish a baseline for isolating these and other hydrodynamic effects. Acceptable coeval fits are found for sixteen pairs without optimizing for heavy element or helium abundance. The precision of these tests is limited by the accuracies of the observed effective temperatures. High dispersion spectra and detailed atmospheric modeling should give more accurate effective temperatures and heavy element abundances. PV Cas, a peculiar early A system, EK Cep B, a known post-T Tauri star, and RS Cha, a member of a young OB association, are matched by pre-main sequence models. Predicted mass loss agrees with upper limits from IUE for CW Cep A and B. Relatively poor fits are obtained for binaries having at least one component in the mass range 1.7 < M/M_sol <2.6, whose evolution is sensitive to mixing. These discrepancies are robust and consistent with additional mixing in real stars. The predicted apsidal motion implies that massive star models are systematically less centrally condensed than the real stars. If these effects are due to overshooting, then the overshooting parameter alpha_OV increases with stellar mass. The apsidal motion constants are controlled by radiative opacity under conditions close to those directly measured in laser experiments, making this test more stringent than possible before.
description: 38 pages, 9 figures (color versions of figures 1,2,3,4, and 9 are available separately). Accepted for publication in the Astrophysical Journal