cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Revised TESS Input Catalog and Candidate Target List
Creators: name: Stassun, Keivan G.
name: Oelkers, Ryan J.
name: Paegert, Martin
name: Torres, Guillermo
name: Pepper, Joshua
name: De Lee, Nathan
name: Collins, Kevin
name: Latham, David W.
name: Muirhead, Philip S.
name: Chittidi, Jay
name: Rojas-Ayala, Barbara
name: Fleming, Scott W.
name: Rose, Mark E.
name: Tenenbaum, Peter
name: Ting, Eric B.
name: Kane, Stephen R.
name: Barclay, Thomas
name: Bean, Jacob L.
name: Brassuer, C. E.
name: Charbonneau, David
name: Lissauer, Jack J.
name: Mann, Andrew W.
name: McLean, Brian
name: Mulally, Susan
name: Narita, Norio
name: Plavchan, Peter
name: Ricker, George R.
name: Sasselov, Dimitar
name: Seager, S.
name: Sharma, Sanjib
name: Shiao, Bernie
name: Sozzetti, Alessandro
name: Stello, Dennis
name: Vanderspek, Roland
name: Wallace, Geoff
name: Winn, Joshua N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We describe the catalogs assembled and the algorithms used to populate the revised TESS Input Catalog (TIC), based on the incorporation of the Gaia second data release. We also describe a revised ranking system for prioritizing stars for 2-minute cadence observations, and assemble a revised Candidate Target List (CTL) using that ranking. The TIC is available on the Mikulski Archive for Space Telescopes (MAST) server, and an enhanced CTL is available through the Filtergraph data visualization portal system at the URL http://filtergraph.vanderbilt.edu/tess_ctl.
description: 30 pages, 16 figures, submitted to AAS Journals; provided to the community in advance of publication in conjunction with public release of the TIC/CTL on 28 May 2019
Enaysma splendens Delucchi 1954
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Enaysma
Enaysma splendens

description: Enaysma splendens Delucchi (Eulophidae)
 Enaysma splendens Delucchi, 1954a: 2. Lectotype m, Germany: Bayern, MuÈnchen, hereby validated, selected by Hansson (VD [examined]).
 Material. LECTOTYPE m (cr, right hind leg lacking beyond trochanter, gaster glued beside rest of body) labelled`198; MuÈnchen 23.II.52; su Alnus incana; ex Lithoc. stringulatella HW. V. Delucchi leg.; Enaysma splendens n. V. Delucchi det.; m; TYPE [red]’.
PARALECTOTYPES, VD: 1 m, 1 l(cr). One slide (sc) with female ¯agellum and left male antenna of paralectotypes.
 Remarks. Delucchi mentioned two females, one male but did not specify a type. Specimens subsequently remounted from micro-pins by Hansson. The number`198’ on the slide is misleading, since it refers to the lectotype which does not lack any antenna. The female ¯agellum is likely to belong to the female paralectotype which is numbered`196’ and lacks the head. Two slides (sc) with data not mentioned by Delucchi (ex L. messaniella), and one slide (sc) with the species name only, are not considered as part of the type series.
 Status. Achrysocharoides splendens (Delucchi) (Yoshimoto, 1977: 928).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 75, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Uteopsis Dendy & Row 1913
Creators: name: Borojevic, Radovan
name: Boury-Esnault, Nicole
name: Vacelet, Jean
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Calcarea
Leucosolenida
Jenkinidae
Uteopsis

description: Genus Uteopsis Dendy & Row, 1913
 TYPE SPECIES. — Ute argentea Poléjaeff, 1883 by monotypy.
DIAGNOSIS. — Jenkinidae with a syconoid organization. The cortex is thick and is supported by giant longitudinal diactines. The choanoskeleton is reduced to the unpaired actines of the subatrial spicules and smaller distal radial diactines.
DESCRIPTION
 Uteopsis is well-described and illustrated by Poléjaeff (1883). It is characterized by an inarticulate choanoskeleton and a thick cortex composed of giant longitudinal diactines and triactines.
description: Published as part of Borojevic, Radovan, Boury-Esnault, Nicole & Vacelet, Jean, 2000, A revision of the supraspecific classification of the subclass Calcaronea (Porifera, class Calcarea), pp. 203-263 in Zoosystema 22 (2) on page 233, DOI: 10.5281/zenodo.5392175
Grantilla Row 1909
Creators: name: Borojevic, Radovan
name: Boury-Esnault, Nicole
name: Vacelet, Jean
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Calcarea
Leucosolenida
Heteropiidae
Grantilla

description: Genus Grantilla Row, 1909
 TYPE SPECIES. — Grantilla quadriradiata Row, 1909 by monotypy.
DIAGNOSIS. — Heteropiidae with a syconoid organization. The skeleton of the tubes is inarticulate, composed of subatrial triactines, and subcortical pseudosagittal triactines and tetractines.
DESCRIPTION
 The vast majority of Heteropiidae have only pseudosagittal triactines in the subcortical skeleton. The genus Grantilla has been proposed for the single species G. quadriradiata Row, 1909, with pseudosagittal tetractines. Other morphological characteristics are quite similar to Sycettusa.
description: Published as part of Borojevic, Radovan, Boury-Esnault, Nicole & Vacelet, Jean, 2000, A revision of the supraspecific classification of the subclass Calcaronea (Porifera, class Calcarea), pp. 203-263 in Zoosystema 22 (2) on page 236, DOI: 10.5281/zenodo.5392175
Re-visiting Cyclone Nargis of Myanmar: vulnerability, resiliency and the dynamics of recovery in the Ayeyarwady Delta
Creators: name: Zaw, Myint
Publisher: name: The Australian National University
Year: 2017
Subjects: Cyclone Nargis, hazard and disaster, vulnerability, early warning system, emergency, post disaster recovery

description: In 2008, Cyclone Nargis devastated the low-lying Ayeyarwady Delta and more than 150,000 people died during the storm. It was the worst natural disaster in Myanmar’s history and globally it was one of the deadliest cyclones of all time. This thesis assesses the implications of Cyclone Nargis for the human security of delta communities in the past and the future. Using Cyclone Nargis as the focus event, the research investigates multiple dimensions of pre-existing vulnerability, strengths and weaknesses in the early warning and emergency response systems, and the dynamics of post-impact recovery. It argues that the roots of vulnerability and resilience were situated in the history of the national political regime in place at the time of the cyclone. The research is based on community narratives collected in 45 villages from three different marginal zones of the Ayeyarwady Delta. This study argues that disaster risk reduction and the promotion of human security in the Delta requires the expansion of community-based processes focusing on building community resilience and the better utilization of locally relevant physical assets for improved safety. These lessons from Cyclone Nargis should be incorporated into the national DRR framework. More broadly, beyond Myanmar this place-based study of rural communities should inform the connected issues of development, governance and disaster risk reduction.
Enaysma zwoelferi Delucchi 1954
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Enaysma
Enaysma zwoelferi

description: Enaysma zwoelferi Delucchi (Eulophidae)
 Enaysma zwoÈlferi Delucchi, 1954a: 2. Holotype m, Germany: Bayern, Oberpfalz, Nittenau (VD [examined]).
 Material. HOLOTYPE m (mp, left antenna and right pedicel with ¯agellum lacking) labelled`238; ex. Lithoc. salicicolella Sirc. V. Delucchi leg.; Nittenau (Oberpfalz) 13.IIÐ 10.III.52; su Salix aurita; m; TYPE [red]; Enaysma zwoÈlferi nov. V. Delucchi det.’. One slide (sc) labelled`231/238 (m) m lanten. E. zwoÈlferi m (Typus)’ with left antenna of holotype only, antenna of the male paratype labelled`231’ missing.
PARATYPES, VD: 1 m, 5 ll(mp) with data as speci®ed by Delucchi, considered as part of the type series. One slide (scx) with left antenna of a paratype female.
 Remarks. A further male (mp) with same data as paratypes in Delucchi’s collection was not mentioned by him and is therefore not considered as part of the type series.
 Status. Achrysocharoides zwoelferi (Delucchi) (BoucÏek and Graham, 1978: 232).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on pages 75-76, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
The Rigged Hilbert Space of the Free Hamiltonian
Creators: name: de la Madrid, R.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We explicitly construct the Rigged Hilbert Space (RHS) of the free Hamiltonian $H_0$. The construction of the RHS of $H_0$ provides yet another opportunity to see that when continuous spectrum is present, the solutions of the Schrodinger equation lie in a RHS rather than just in a Hilbert space.
description: 18 pages. Invited, refereed contribution to the Jaca proceedings; v2: minor, cosmetic changes
Additional file 1 of Genetic aetiology of primary adrenal insufficiency in Chinese children
Creators: name: Chang, Zhuo
name: Lu, Wei
name: Zhao, Zhuhui
name: Xi, Li
name: Li, Xiaojing
name: Ye, Rong
name: Ni, Jinwen
name: Pei, Zhou
name: Zhang, Miaoying
name: Cheng, Ruoqian
name: Zheng, Zhangqian
name: Sun, Chengjun
name: Wu, Jing
name: Luo, Feihong
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1: Fig. S1. Diagnostic algorithm for PAI patients. For a patient with primary adrenal insufficiency, a high serum level of 17-OHP suggests CAH, and he or she was subjected to CYP21A2 sequencing and MLPA. Children with normal or lower 17-OHP levels accompanied by developmental delay, intellectual disability or congenital anomalies underwent Array-GCH examination. WES was performed for the remaining patients.
Entedon erdoesi Delucchi 2001
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Entedon
Entedon erdoesi

description: Entedon erdoesi Delucchi (Eulophidae)
 Entedon (Chlorentedon) erdoÈsi Delucchi, 1954b: 97. Lectotype m, Switzerland: Schwyz, Sihlsee, hereby validated, selected by Askew (VD [examined]).
 Material. LECTOTYPE m (mp, left wings lacking) labelled`Sihlsee 18.V.52 V. Delucchi leg.; ENTEDON erdoÈsi n. sp. V. Delucchi det.; TYPE [red]’ (body illustrated, 1954b: 98, ®gure 1).
PARALECTOTYPES, VD: 2 mm, 10 ll(mp), labelled as follows: 1 l` Sihlsee 18.V.52 V. Delucchi leg.; Entedon erdoÈsi n. sp. V. Delucchi det.; TYPE [red]’ and 2 mm, 9 ll` Sihlsee 18.V.52 V. Delucchi leg.’. One slide (sc) labelled`39; ENTEDON erdoÈsi Del. DIS Antennae ml ’ with left antennae (1954b: 100, ®gures 2a, 2b) of a male and a female paralectotype and one slide (sc) labelled`40; ENTEDON erdoÈsi Del. Ala DIS’ with left fore wing (1954b: 100, ®gures 2c, 2d) of a female.
 Remarks. Delucchi described both sexes and stated`Type in meiner Sammlung.’ but did not specify the number of specimens he had. Unfortunately, both the lectotype and one female paralectotyp e lack the left wings. Because the two specimens are extremely similar in this respect it cannot be established with certainty to which specimen the slide with the wing belongs.
 Status. Junior synonym of Entedon metatarsalis Thomson syn. n. (Askew, in litt.).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 76, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Measuring the Size of Quasar Broad-Line Clouds Through Time Delay Light-Curve Anomalies of Gravitational Lenses
Creators: name: Wyithe, Stuart
name: Loeb, Abraham
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Intensive monitoring campaigns have recently attempted to measure the time delays between multiple images of gravitational lenses. Some of the resulting light-curves show puzzling low-level, rapid variability which is unique to individual images, superimposed on top of (and concurrent with) longer time-scale intrinsic quasar variations which repeat in all images. We demonstrate that both the amplitude and variability time-scale of the rapid light-curve anomalies, as well as the correlation observed between intrinsic and microlensed variability, are naturally explained by stellar microlensing of a smooth accretion disk which is occulted by optically-thick broad-line clouds. The rapid time-scale is caused by the high velocities of the clouds (~5x10^3 km/s), and the low amplitude results from the large number of clouds covering the magnified or demagnified parts of the disk. The observed amplitudes of variations in specific lenses implies that the number of broad-line clouds that cover ~10% of the quasar sky is ~10^5 per 4 pi steradian. This is comparable to the expected number of broad line clouds in models where the clouds originate from bloated stars.
description: 19 pages, 9 figures. Submitted to ApJ
Urban land tenure and administration in Papua New Guinea
Creators: name: Haynes, C. E. P
Publisher: name: The Australian National University
Year: 1990
Subjects: subject: Land tenure Papua New Guinea
subject: Land use, Urban Papua New Guinea

description: The colonial administration in Papua New Guinea considered custom and customary land tenure to be anachronistic institutions which were to be eventually replaced by western forms of law and land tenure. Whereas customary land tenure had to be tolerated in rural areas, there was no such pressure operating in urban areas which were the creation of the colonial state and remained 'European enclaves' until the 1960s. Urban development took place only on state land; this entailed the purchase of customary land for the establishment and expansion of towns and the drawing of urban boundaries so as to exclude existing neighbouring villages on customary land. Torrens registered state leases were granted over this land. With the approach to Independence in the early 1970s and the re-assertion of traditional values, it was expected that customary law and customary land tenure would play a more important role in national development. The Eight Aims which were adopted at the end of 1972 seemed to ensure this. However customary law and customary land tenure were subordinated to state law and controls in the new urban land tenure regime which the Commission of Inquiry into Land Matters (CILM) devised for an Independent Papua New Guinea. The CILM considered that the development goals of the new nation state required that state law and state institutions be used exclusively in developing urban land. In keeping with this, the CILM called for the nationalisation of all remaining customary land in urban and peri-urban areas. This thesis argues that arguments which led the CILM to recommend the abolition of all customary land tenure in urban areas were misconceived, and that it placed too much reliance on state law and institutions to achieve an efficient and just urban land tenure system. The urban land laws, administrative procedures and institutional structures which have so far obtained in urban areas in Papua New Guinea have failed to advance the national development goals which were adopted at Independence, and have led to substantial inefficiencies and inequities. Changes are necessary, both to the state system and to custom, to promote a more efficient and equitable urban land tenure system.
Clausius inequality versus quantum coherence
Creators: name: Soltanmanesh, Ali
name: Shafiee, Afshin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this study, we model a harmonic oscillator that enters an interferometer partially coupled to a thermal bath of oscillatory fields by employing a Brownian-type Lindblad master equation. More specifically, we investigate the dynamics and the variations of the thermodynamic quantities of the system at different temperatures. We recognize that although the system can remain coherent during its interaction with the thermal bath in the low-temperature limit, the system's entropy production violates the Clausius inequality. Furthermore, we argue that the system's coherence is the source of this violation, rather than the entanglement degree of system-environment, as reported in previous studies.
DDO Photometry of M71: Carbon and Nitrogen Patterns Among Evolving Giants
Creators: name: Briley, M. M.
name: Smith, G. H.
name: Claver, C. F.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present V, B-V, and DDO C(41-42) and C(42-45) photometry for a sample of 75 red giants down to M_V = +2 in the relatively metal-rich Galactic globular cluster M71. The C(41-42) colors reveal a bimodal distribution of CN band strengths generally anticorrelated with CH band strength as measured by the C(42-45) color. Both DDO colors agree well with those found in 47 Tucanae -- a nearby globular cluster of similar metallicity -- and suggest nearly identical C and N abundance patterns among the giants of both clusters. A comparison with synthetic DDO colors demonstrates that little change in surface C or N abundance is required to match the colors of the M71 giants over the entire luminosity range observed. Apparently like 47 Tuc (a cluster of much greater mass and central concentration), M71 exhibits an abundance pattern which cannot be solely the result of internal mixing.
description: To appear in the Astronomical Journal, November 2001. 17 Pages, 5 Figures
Reseña: La sala de máquinas de la Constitución
Creators: name: Nieto Olvera, Pedro David
Publisher: name: Zenodo
Year: 2023
Subjects: subject: constitucionalismo
subject: derecho
subject: America latina
subject: Constitución
subject: Law
subject: FOS: Law

description: A pesar de las muchas reformas constitucionales realizadas en América Latina en las últimas décadas, las constituciones lationamericanas han sido desatendidas por el pensamiento académico y político, que tampoco mostró mayor interés por la riquísima tradición constitucional que, a lo largo de doscientos años, se fue conformando en la región. En esta obra, Roberto Gargarella, uno de los más prestigiosos constitucionalistas de la actualidad, cubre ampliamente ese vacío con un minucioso estudio de la evolución de los textos fundamentales de las naciones latinoamericanas, estableciendo continuidades y rupturas, semejanzas y diferencias, influencias cruzadas y contradictorias.
Investigating `dark' energy in the solar corona using forward modeling of MHD waves
Creators: name: Pant, Vaibhav
name: Magyar, Norbert
name: Van Doorsselaere, Tom
name: Morton, Richard J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: It is now well established that the Alfvénic waves are ubiquitous in the solar corona. However, the Alfvénic wave energy estimated from the Doppler velocity measurements in the corona was found to be four orders of magnitude less than that estimated from non-thermal line widths. McIntosh & De Pontieu (2012) suggested that this discrepancy in energy might be due to the line-of-sight (LOS) superposition of the several oscillating structures, which can lead to an underestimation of the Alfvénic wave amplitudes and energies. McIntosh & De Pontieu (2012) termed this coronal `dark' or `hidden' energy. However, their simulations required the use of an additional, unknown source of Alfvénic wave energy to provide agreement with measurements of the coronal non-thermal line widths. In this study, we investigate the requirement of this unknown source of additional `dark' energy in the solar corona using gravitationally stratified 3D magnetohydrodynamic (MHD) simulations of propagating waves. We excite the transverse MHD waves and generate synthetic observations for the Fe XIII emission line. We establish that the LOS superposition greatly reduces the Doppler velocity amplitudes and increases the non-thermal line widths. Importantly, our model generates the observed wedge-shaped correlation between Doppler velocities and non-thermal line widths. We find that the observed wave energy is only 0.2-1\% of the true wave energy which explains 2-3 orders of magnitude of the energy discrepancy. We conclusively establish that the true wave energies are hidden in the non-thermal line widths. Hence, our results rule out the requirement for an additional `dark' energy in the solar corona.
description: Accepted for publication in Astrophysical Journal (ApJ). 20 pages, 10 figures
Coalgebraic Formal Curve Spectra and the Annular Tower
Creators: name: Peterson, Eric C.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics

description: We import into homotopy theory the algebro-geometric construction of the cotangent space of a geometric point on a scheme. Specializing to the category of spectra local to a Morava $K$-theory of height $d$, we show that this can be used to produce a choice-free model of the determinantal sphere as well as an efficient Picard-graded cellular decomposition of $K(\mathbb Z_p, d+1)$. Coupling these ideas to work of Westerland, we give a "Snaith's theorem" for the Iwasawa extension of the $K(d)$-local sphere.
description: Submitted as author's 2015 PhD thesis, submitted for journal publication in 2017, only realized in 2019 that it wasn't available on the arXiv
Grantessa Lendenfeld 1885
Creators: name: Borojevic, Radovan
name: Boury-Esnault, Nicole
name: Vacelet, Jean
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Calcarea
Leucosolenida
Heteropiidae
Grantessa

description: Genus Grantessa Lendenfeld, 1885
 TYPE SPECIES. — Grantessa sacca Lendenfeld, 1885 by monotypy.
 DIAGNOSIS. — Heteropiidae with a syconoid organization and an articulate choanoskeleton. A thin cortex is formed by triactines but lacks longitudinal large diactines. The distal part of the radial tubes is frequently decorated by tufts of radially arranged diactines, indicating a close relationship to the genus Syconessa.
DESCRIPTION
 We include in the genus Grantessa s.s. the syconoid Heteropiidae with articulate choanoskeletons (Fig. 32). We consider that they are derived from sponges similar to Syconessa, in which the increase of radial tubes had generated the articulate choanoskeleton. Grantessa are common in warm seas, and often grow as large arborescent or bushy cormus.
description: Published as part of Borojevic, Radovan, Boury-Esnault, Nicole & Vacelet, Jean, 2000, A revision of the supraspecific classification of the subclass Calcaronea (Porifera, class Calcarea), pp. 203-263 in Zoosystema 22 (2) on page 236, DOI: 10.5281/zenodo.5392175
Epilampsis coxalis Delucchi 1956
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Epilampsis
Epilampsis coxalis

description: Epilampsis coxalis Delucchi (Eulophidae)
 Epilampsis coxalis Delucchi, 1956b: 74. Holotype m, Switzerland: Canton ZuÈrich (VD [examined]).
 Material. HOLOTYPE m (mp, left antenna lacking) labelled`l 15; ex Lithocolletis sp. (cram. od. querc.) V. Delucchi leg.; Zurich [sic], Wintergeneration, leg. Dr H. Pschorn; EPILAMPSIS coxalis n. sp. V. Delucchi det.; HOLOTYPE [red]’. One slide (sc) labelled`24; EPILAMPSIS coxalisn. sp. (ex quercif.-cramar.) antenne m Kt. ZuÈrich. leg. Pschorn-Walcher DIS’ with left antenna (1956b: 67, ®gure 11) of holotype.
PARATYPES, VD: 1 m (mp).
 Status. Junior synonym of Chrysocharis laomedon (Walker) (Hansson, 1985: 71).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on pages 76-77, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Heteropia Carter 1886
Creators: name: Borojevic, Radovan
name: Boury-Esnault, Nicole
name: Vacelet, Jean
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Calcarea
Leucosolenida
Heteropiidae
Heteropia

description: Genus Heteropia Carter, 1886
 TYPE SPECIES. — Aphroceras ramosa Carter, 1886 by monotypy.
DIAGNOSIS. — Heteropiidae with a syconoid organization, an articulate choanoskeleton, and where the cortical skeleton consists of longitudinal large diactines, with occasionally tangential triactines and perpendicular small diactines.
DESCRIPTION
 Heteropia in the family Heteropiidae corresponds to the same grade of skeletal complexity than Ute in the family Grantiidae.
description: Published as part of Borojevic, Radovan, Boury-Esnault, Nicole & Vacelet, Jean, 2000, A revision of the supraspecific classification of the subclass Calcaronea (Porifera, class Calcarea), pp. 203-263 in Zoosystema 22 (2) on page 236, DOI: 10.5281/zenodo.5392175
Predictions for the frequency and orbital radii of massive extrasolar planets
Creators: name: Armitage, Philip J.
name: Livio, Mario
name: Lubow, S. H.
name: Pringle, J. E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the migration of massive extrasolar planets due to gravitational interaction with a viscous protoplanetary disc. We show that a model in which planets form at 5 AU at a constant rate, before migrating, leads to a predicted distribution of planets that is a steeply rising function of log (a), where a is the orbital radius. Between 1 AU and 3 AU, the expected number of planets per logarithmic interval in orbital radius roughly doubles. We demonstrate that, once selection effects are accounted for, this is consistent with current data, and then extrapolate the observed planet fraction to masses and radii that are inaccessible to current observations. In total, about 15 percent of stars targeted by existing radial velocity searches are predicted to possess planets with masses 0.3 M_Jupiter < M_p sin (i) < 10 M_Jupiter, and radii 0.1 AU < a < 5 AU. A third of these planets (around 5 percent of the target stars) lie at the radii most amenable to detection via microlensing. A further 5-10 percent of stars could have planets at radii of 5 AU < a < 8 AU that have migrated outwards. We discuss the probability of forming a system (akin to the Solar System) in which significant radial migration of the most massive planet does not occur. About 10-15 percent of systems with a surviving massive planet are estimated to fall into this class. Finally, we note that a smaller fraction of low mass planets than high mass planets is expected to survive without being consumed by the star. The initial mass function for planets is thus predicted to rise more steeply towards small masses than the observed mass function.
description: MNRAS, in press
Fine vortex structure and flow transition to the geostrophic regime in rotating Rayleigh-Bénard convection
Creators: name: Shi, Jun-Qiang
name: Lu, Hao-Yuan
name: Ding, Shan-Shan
name: Zhong, Jin-Qiang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We present spatial-resolved measurements of the columnar vortex structures in rotating Rayleigh-Bénard convection. The scaled radial profiles of the azimuthal velocity $u_ϕ(r)$ and vertical vorticity $ω(r)$ of the vortices are analyzed and compared with the predictions of the asymptotic theory. The results reveal that the asymptotic theory predicts accurately $u_ϕ(r)$ and $ω(r)$ in the geostrophic convection regime, but extension of the theory in the weak rotation regime is needed to interpret the rotation-dependence of the experimental data. Our measurements of the mean velocity, vorticity of the vortices, and the strength of the vortex shield structure all indicate a flow transition from weekly rotating convection to geostrophic convection. Results of the parameter values for the transition are in agreement with the scaling relationship obtained from previous heat-transfer measurements.
Topological states of matter and noncommutative geometry
Creators: name: Bourne, Christopher
Publisher: name: The Australian National University
Year: 2015
Subjects: Noncommutative geometry
KK-theory
topological insulators
topological phases

description: This thesis examines topological states of matter from the perspective of noncommutative geometry and KK-theory. Examples of such topological states of matter include the quantum Hall e ect and topological insulators. For the quantum Hall e ect, we consider a continuous model and show that the Hall conductance can be expressed in terms of the index pairing of the Fermi projection of a disordered Hamiltonian with a spectral triple encoding the geometry of the sample's momentum space. The presence of a magnetic eld means that noncommutative algebras and methods must be employed. Higher dimensional analogues of the quantum Hall system are also considered, where the index pairing produces the `higher-dimensional Chern numbers' in the continuous setting. Next we consider a discrete quantum Hall system with an edge. We show that topological properties of observables concentrated at the boundary can be linked to invariants from a boundary-free model via the Kasparov product. Hence we obtain the bulk-edge correspondence of the quantum Hall e ect in the language of KK-theory. Finally we consider topological insulators, which come from imposing (possibly anti-linear) symmetries on condensed-matter systems and studying the invariants that are protected by these symmetries. We show how symmetry data can be linked to classes in real or complex KK-theory. Finally we prove the bulk-edge correspondence for topological insulator systems by linking bulk and edge systems using the Kasparov product in KKO-theory.
Non-Reciprocal and Collimated Surface Plasmons in Drift-biased Graphene Metasurfaces
Creators: name: Correas-Serrano, D.
name: Gomez-Diaz, J. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We explore the unusual non-reciprocal and diffraction-less properties of surface plasmon polaritons propagating in drift-biased graphene-based metasurfaces. We show that applying a drift-current on a graphene sheet leads to extremely asymmetric in-plane modal dispersions from terahertz to infrared frequencies, associated with plasmons with low-loss (high-loss and ultra-high confinement) traveling along (against) the bias. Strikingly, truly unidirectional wave propagation is prevented by the intrinsic nonlocal response of a graphene, a mechanism that shapes the energy flow over the surface. We also show that highly-directive hyperbolic plasmons completely immune to backscattering propagate obliquely along the drift in nanostructured graphene. Finally, we discuss how spin-orbit interactions can be exploited in this platform to efficiently launch collimated plasmons along a single direction while maintaining giant non-reciprocal responses. Our findings open a new paradigm to excite, collimate, steer, and process surface plasmons over a broad frequency band.
Epilampsis deciduae Delucchi
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Epilampsis
Epilampsis deciduae

description: Epilampsis deciduae Delucchi (Eulophidae)
 Epilampsis deciduae Delucchi, 1954a: 3. Holotype m, Germany: Rhein, Gernsheimer Wald (VD [examined]).
 Material. HOLOTYPE m (mp) labelled`ex Tischeria decidua Wck. V. Delucchi leg.; su Quercus; 10.IV.52; 262; m; EPILAMPSIS deciduae n. V. Delucchi det. 54; TYPE [red]’.
PARATYPES, VD: 1 m, 2 ll(mp) with data as speci®ed by Delucchi, considered as part of the type series. One slide (sc) with right antenna of a paratype male.
 Remarks. One of the females mentioned by Delucchi is in fact a male.
 Status. Junior synonym of Chrysocharis nautius (Walker) (Hansson, 1985: 66).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 77, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Coupled spheroid and black-hole formation, and the multifrequency detectability of active galactic nuclei and submillimetre sources
Creators: name: Archibald, E. N.
name: Dunlop, J. S.
name: Jimenez, R.
name: Friaca, A. C. S.
name: McLure, R. J.
name: Hughes, D. H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use a simple model of spheroid formation to explore the relationship between the creation of stars and dust in a massive proto galaxy and the growth of its central black hole. This model predicts that sub-mm luminosity peaks after only ~ 0.2 Gyr. However, without a very massive seed black hole, Eddington-limited growth means that a black hole mass of 10^9 solar masses, and hence very luminous AGN activity, cannot be produced until > 0.5 Gyr after the formation of the first massive stars in the halo. The model thus predicts a time-lag between the peak of sub-mm luminosity and AGN luminosity in a massive proto-elliptical of a few times 10^8 years. For a formation redshift z = 5, this means that powerful AGN activity is delayed until z = 3.5, by which time star formation in the host is 90% complete, and sub-mm luminosity has declined to ~ 25% of its peak value. This provides a natural explanation for why successful sub-mm detections of luminous radio galaxies are largely confined to z > 2.5. Conversely the model also predicts that while all high-redshift luminous sub-mm-selected sources should contain an active (and growing) black hole, the typical luminosity of the AGN in such objects is ~1000 times smaller than that of the most powerful AGN. This is consistent with the almost complete failure to detect sub-mm selected galaxies with existing X-ray surveys. Finally the model yields a black-hole:spheroid mass ratio which evolves rapidly in the first Gyr, but asymptotes to ~ 0.001-0.003 in agreement with results at low redshift. This ratio arises not because the AGN terminates star formation, but because fueling of the massive black hole is linked to the total mass of gas available for star formation in the host.
description: Revised version accepted for publication in MNRAS. 10 pages with 8 figures
Amphoriscus Haeckel 1870
Creators: name: Borojevic, Radovan
name: Boury-Esnault, Nicole
name: Vacelet, Jean
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Porifera
Calcarea
Leucosolenida
Amphoriscidae
Amphoriscus

description: Genus Amphoriscus Haeckel, 1870
 TYPE SPECIES. — Ute chrysalis Schmidt, 1864 by subsequent designation (Dendy & Row 1913).
DIAGNOSIS. — Amphoriscidae with a syconoid organization of the aquiferous system. Scattered spicules in the choanosome are always absent.
DESCRIPTION
 Amphoriscus is a well-characterized genus, and contains several species of solitary sponges with beautiful vitreous transparent walls. The genus is found in all the oceans.
 Dendy & Row (1913) kept the genus Syculmis Haeckel, 1872 for Amphoriscidae with a roottuft of diactines and anchoring tetractines. We had the opportunity to observe similar anchoring structures in the families Sycettidae and Jenkinidae, and we do not feel that this character calls for the creation of a special genus; we propose the inclusion of the sponge described as Syculmis synapta by Haeckel (1872), in the genus Amphoriscus.
description: Published as part of Borojevic, Radovan, Boury-Esnault, Nicole & Vacelet, Jean, 2000, A revision of the supraspecific classification of the subclass Calcaronea (Porifera, class Calcarea), pp. 203-263 in Zoosystema 22 (2) on page 238, DOI: 10.5281/zenodo.5392175
Generic Gaussian ideals
Creators: name: Corso, Alberto
name: Vasconcelos, Wolmer V.
name: Villarreal, Rafael
Publisher: name: arXiv
Year: 2002
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics

description: The content of a polynomial $f(t)$ is the ideal generated by its coefficients. Our aim here is to consider a beautiful formula of Dedekind-Mertens on the content of the product of two polynomials, to explain some of its features from the point of view of Cohen-Macaulay algebras and to apply it to obtain some Noether normalizations of certain toric rings. Furthermore, the structure of the primary decomposition of generic products is given and some extensions to joins of toric rings are considered.
description: 13 pages
Additional file 1: of Oral health of 12-year-old children in Quito, Ecuador: a population-based epidemiological survey
Creators: name: Michel-Crosato, Edgard
name: Raggio, Daniela
name: Coloma-Valverde, Alba
name: Edisson Lopez
name: Alvarez-Velasco, Patricia
name: Medina, Marco
name: Balseca, Mariela
name: Quezada-Conde, Maritza
name: Carrer, Fernanda Almeida
name: Romito, Giuseppe
name: Araujo, Maria
name: Biazevic, Maria
name: Braga, Mariana
name: Maristela Fratucci
name: Mendes, Fausto
name: Frias, Antonio
name: Pannuti, Claudio
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Computational Biology

description: STROBE checklist (PDF 140 kb)
Two families of elliptical plasma lenses
Creators: name: Er, Xinzhong
name: Rogers, Adam
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Plasma lensing is the refraction of low-frequency electromagnetic rays due to free electrons in the interstellar medium. Although the phenomenon has a distinct similarity to gravitational lensing, particularly in its mathematical description, plasma lensing introduces other additional features, such as wavelength dependence, radial rather than tangential image distortions, and strong demagnification of background sources. Axisymmetrical models of plasma lenses have been well-studied in the literature, but density distributions with more complicated shapes can provide new and exotic image configurations and increase the richness of the magnification properties. As a first step towards non-axisymmetrical distributions, we study two families of elliptical plasma lens, softened power-law and exponential plasma distributions. We perform numerical studies on each lens model, and present them over a parameter space. In addition to deriving elliptical plasma lens formulae, we also investigate the number of critical curves that the lens can produce by studying the lens parameter space, in particular the dependence on the lensing ellipticity. We find that the introduction of ellipticity into the plasma distribution can enhance the lensing effects as well as the complexity of the magnification map.
description: 14 pages, comments welcome
Partially Absorbed Comptonization Spectrum from the Nearly Edge-on Source X 1822-371
Creators: name: Iaria, R.
name: Di Salvo, T.
name: Burderi, L.
name: Robba, N. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a spectral analysis over the range 0.1-200 keV performed on the dipping source X 1822-371 observed by BeppoSAX. We find the best fit to the continuum using a partially covered Comptonization model, due to scattering off soft seed photons by electrons at a temperature of ~4.8 keV, without the presence of any soft blackbody emission. The equivalent hydrogen column obtained for the absorbed component is ~4.5 10^{22} cm^{-2}, an order of magnitude larger than the Galactic absorption for this source, and the covering fraction is ~71%. Because the inclination angle of X 1822-371 to the line of sight is ~85^\circ, this model gives a reasonable scenario for the source: the Comptonized spectrum could come from an extended accretion disk corona (ADC), probably the only region that can be directly observed due to the high inclination. The excess of matter producing the partial covering could be close to the equatorial plane of the system, above the outer disk, occulting the emission from the inner disk and the inner part of the ADC. An iron emission line is also present at ~6.5 keV with an equivalent width of ~150 eV. We argue that this strong iron line cannot be explained as reflection of the Comptonized spectrum by the accretion disk. It is probably produced in the ADC. An emission line at ~1.9 keV (with an equivalent width of ~54 eV) and an absorption edge at \~8.7 keV (with an optical depth of ~0.1) are also required to fit this spectrum. These features are probably produced by highly ionized iron (Fe XXIV) present in the outer part of the ADC, where the plasma density is \~10^{11}-10^{12} cm^{-3} and ionized plasma is present.
description: 15 pages, including 3 figures. Accepted by ApJ. Corrected typos and Figure 2
Gamma-rays from SS433: evidence for periodicity
Creators: name: Rasul, Kajwan
name: Chadwick, Paula M.
name: Graham, Jamie A.
name: Brown, Anthony M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In this paper we present our study of the gamma-ray emission from the microquasar SS433. Integrating over 9 years of Fermi-LAT \textsc{pass8} data, we detect SS433 with a significance of ~13$σ$ in the 200 to 500 MeV photon energy range, with evidence for an extension in the direction of the w1 X-ray `hotspot`. A temporal analysis reveals evidence for modulation of SS433's gamma-ray emission with the precession period of its relativistic jet. This suggests that at least some of SS433's gamma-ray emission originates close to the object rather than from the jet termination regions.
description: Accepted for publication in MNRAS, 6 pages, 4 figures
A Catalog of Candidate Intermediate-luminosity X-ray Objects
Creators: name: Colbert, E.
name: Ptak, A.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: ROSAT, and now Chandra, X-ray images allow studies of extranuclear X-ray point sources in galaxies other than our own. X-ray observations of normal galaxies with ROSAT and Chandra have revealed that off-nuclear, compact, Intermediate-luminosity (Lx[2-10 keV] >= 1e39 erg/s) X-ray Objects (IXOs, a.k.a. ULXs [Ultraluminous X-ray sources]) are quite common. Here we present a catalog and finding charts for 87 IXOs in 54 galaxies, derived from all of the ROSAT HRI imaging data for galaxies with cz <= 5000 km/s from the Third Reference Catalog of Bright Galaxies (RC3). We have defined the cutoff Lx for IXOs so that it is well above the Eddington luminosity of a 1.4 Msun black hole (10^38.3 erg/s), so as not to confuse IXOs with ``normal'' black hole X-ray binaries. This catalog is intended to provide a baseline for follow-up work with Chandra and XMM, and with space- and ground-based survey work at wavelengths other than X-ray. We demonstrate that elliptical galaxies with IXOs have a larger number of IXOs per galaxy than non-elliptical galaxies with IXOs, and note that they are not likely to be merely high-mass X-ray binaries with beamed X-ray emission, as may be the case for IXOs in starburst galaxies. Approximately half of the IXOs with multiple observations show X-ray variability, and many (19) of the IXOs have faint optical counterparts in DSS optical B-band images. Follow-up observations of these objects should be helpful in identifying their nature.
description: 29 pages, ApJS, accepted (catalog v2.0) (full resolution version of paper and future releases of catalog at http://www.xassist.org/ixocat_hri)
Epilampsis gunholdi Delucchi 1954
Creators: name: Baur, Hannes
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eulophidae
Epilampsis
Epilampsis gunholdi

description: Epilampsis gunholdi Delucchi (Eulophidae)
 Epilampsis gunholdi Delucchi, 1954a: 4. Holotype m, Switzerland: Bern, Gurtenkulm (MHNG [examined]).
 Material. HOLOTYPE m (cp, right antenna and hind wings lacking) labelled` Berne Gurtenkulm 3.IV.1950 Schmidlin. 15; Ex Lithocolletis platanoidella [sic] s. Acer platanoides; EPILAMPSIS gunholdi n. V. Delucchi det. 54; TYPE [red]; m’.
PARATYPES, MHNG: 7 mm, 1 l(cp) with data as speci®ed by Delucchi, considered as part of the type series.
 Remarks. One female mentioned by Delucchi (`Gurtenkulm’) could not be located. The host of the holotype was quoted as`Lithocolletis joannisi LE MARCH.’.
 Status. Junior synonym of Chrysocharis nephereus (Walker) (BoucÏek, 1970: 97).
description: Published as part of Baur, Hannes, 2001, The Hymenoptera (Chalcidoidea, Ichneumonoidea, Platygastroidea) described by Vittorio Delucchi: an annotated catalogue, pp. 55-125 in Journal of Natural History 35 (1) on page 77, DOI: 10.1080/002229301447899, http://zenodo.org/record/5275865
Absence of magnetic thermal conductivity in the quantum spin liquid candidate EtMe3Sb[Pd(dmit)2]2 -- revisited
Creators: name: Ni, J. M.
name: Pan, B. L.
name: Huang, Y. Y.
name: Zeng, J. Y.
name: Yu, Y. J.
name: Cheng, E. J.
name: Wang, L. S.
name: Kato, R.
name: Li, S. Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We present the ultralow-temperature specific heat and thermal conductivity measurements on single crystals of triangular-lattice organic compound EtMe$_3$Sb[Pd(dmit)$_2$]$_2$, which has long been considered as a gapless quantum spin liquid candidate. In specific heat measurements, a finite linear term is observed, consistent with the previous work [S. Yamashita $et$ $al.$, Nat. Commun. {\bf 2}, 275 (2011)]. However, we do not observe a finite residual linear term in the thermal conductivity measurements, and the thermal conductivity does not change in a magnetic field of 6 Tesla. These results are in sharp contrast to previous thermal conductivity measurements on EtMe$_3$Sb[Pd(dmit)$_2$]$_2$ [M. Yamashita $et$ $al.$ Science {\bf 328}, 1246 (2010)], in which a huge residual linear term was observed and attributed to highly mobile gapless excitations, likely the spinons of a quantum spin liquid. In this context, the true ground state of EtMe$_3$Sb[Pd(dmit)$_2$]$_2$ has to be reconsidered.
description: 6 pages, 4 figures
Additional file 1: of Health-related quality of life in patients with rheumatoid arthritis
Creators: name: Wanruchada Katchamart
name: Pongthorn Narongroeknawin
name: Wanwisa Chanapai
name: Phakhamon Thaweeratthakul
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology

description: Table Supplement Relationship between the five domains of the EQ-5D and patient characteristics. (DOCX 54 kb)