cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1: of TET1-mediated DNA hydroxymethylation activates inhibitors of the Wnt/Î˛-catenin signaling pathway to suppress EMT in pancreatic tumor cells
Creators: name: Wu, Jian
name: Hongzhe Li
name: Minmin Shi
name: Youwei Zhu
name: Ma, Yang
name: Yiming Zhong
name: Xiong, Cheng
name: Chen, Hao
name: Chenghong Peng
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer

description: Table S1. Primers in this study (DOCX 18 kb) (DOCX 19 kb)
Mesanthura Barnard 1914
Creators: name: Kensley, B.
name: Schotte, M.
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Anthuridae
Mesanthura

description: Genus Mesanthura Barnard, 1914
 Mesanthura Barnard, 1914: 343 a; Poore and Lew Ton, 1986b: 90; MuÈller, 1993: 19.
 Diagnosis. Eyes present. Persistent species-speci®c dorsal pigment pattern present. Antennular ¯agellum of three articles. Antennal ¯agellum short, of few articles. Mandibular palp of three articles. Maxillipedal palp of three articles; endite very short or absent. Pereopod 1, propodus subchelate, expanded. Pereopods 4±7, carpus roughly triangular, with anterior margin shorter than posterior. Pleon short, pleonites fused. Telson with two basal statocysts.
 Remarks. Nine species of Mesanthura have been described from the Indian Ocean, separation of which, using clear key characters, is di cult due to lack of material and poor descriptions. Morphologically, aside from the dorsal colour pattern, species of Mesanthura are very similar. Table 2 attempts to provide some basis for distinguishing these species.
description: Published as part of Kensley, B. & Schotte, M., 2000, New species and records of anthuridean isopod crustaceans from the Indian Ocean, pp. 2057-2121 in Journal of Natural History 34 on page 2080
Tineobius (Tineobius) brachartonae Lucian Fusu & Antoni Ribes 2017, stat. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius brachartonae

description: 10. Tineobius (Tineobius) brachartonae (Gahan, 1927) stat. nov. [new subgeneric status]
Anastatoidea brachartonae Gahan, 1927: 13–15.
Holotype ♀, by original designation (USNM 29444, not examined). Type locality: Central Java.
Anastatoidea brachartonae – Ferrière 1936: 195 (catalogued, distribution). — Ferrière 1938: 48, 57 (keyed). — Risbec 1952: 67 (catalogued).
Tineobius brachartonae – Bouček 1988: 564.
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 12, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Olivine-Carbonate Mineralogy of the Jezero Crater Region
Creators: name: Brown, Adrian J.
name: Viviano, Christina E.
name: Goudge, Timothy A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: A well-preserved, ancient delta deposit, in combination with ample exposures of carbonate rich materials, make Jezero Crater in Nili Fossae a compelling astrobiological site. We use Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) observations to characterize the surface mineralogy of the crater and surrounding watershed. Previous studies have documented the occurrence of olivine and carbonates in the Nili Fossae region. We focus on correlations between these two well studied lithologies in the Jezero crater watershed. We map the position and shape of the olivine 1 μm absorption band and find that carbonates are only found in association with olivine which displays a 1 μm band shifted to long wavelengths. We then use THEMIS coverage of Nili Fossae and perform tests to investigate whether the long wavelength shifted olivine signature is correlated with high thermal inertia outcrops. We find no correlation between thermal inertia and the unique olivine signature. We discuss a range of formation scenarios, including the possibility that these olivine and carbonate associations are products of serpentinization reactions on early Mars. These lithologies provide an opportunity for deepening our understanding of early Mars, and, given their antiquity, may provide a framework to study the formation of valley networks, and the thermal history of the martian crust and interior from the early Noachian to today.
description: 15 figures, 2 tables
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration
Creators: name: Riess, Adam G.
name: Nugent, Peter E.
name: Schmidt, Brian P.
name: Tonry, John
name: Dickinson, Mark
name: Gilliland, Ronald L.
name: Thompson, Rodger I.
name: Budavari, Tamas
name: Casertano, Stefano
name: Evans, Aaron S.
name: Filippenko, Alexei V.
name: Livio, Mario
name: Sanders, David B.
name: Shapley, Alice E.
name: Spinrad, Hyron
name: Steidel, Charles C.
name: Stern, Daniel
name: Surace, Jason
name: Veilleux, Sylvain
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present photometric observations of an apparent Type Ia supernova (SN Ia) at a redshift of ~1.7, the farthest SN observed to date. SN 1997ff, was discovered in a repeat observation by the HST of the HDF-), and serendipitously monitored with NICMOS on HST throughout the GTO campaign. The SN type can be determined from the host galaxy type:an evolved, red elliptical lacking enough recent star formation to provide a significant population of core-collapse SNe. The class- ification is further supported by diagnostics available from the observed colors and temporal behavior of the SN, both of which match a typical SN Ia. The photo- metric record of the SN includes a dozen flux measurements in the I, J, and H bands spanning 35 days in the observed frame. The redshift derived from the SN photometry, z=1.7+/-0.1, is in excellent agreement with the redshift estimate of z=1.65+/-0.15 derived from the U_300,B_450,V_606,I_814,J_110,J_125,H_160, H_165,K_s photometry of the galaxy. Optical and near-infrared spectra of the host provide a very tentative spectroscopic redshift of 1.755. Fits to observations of the SN provide constraints for the redshift-distance relation of SNe~Ia and a powerful test of the current accelerating Universe hypothesis. The apparent SN brightness is consistent with that expected in the decelerating phase of the preferred cosmological model, Omega_M~1/3, Omega_Lambda~2/3. It is inconsistent with grey dust or simple luminosity evolution, candidate astro- physical effects which could mimic past evidence for an accelerating Universe from SNe Ia at z~0.5.We consider several sources of possible systematic error including lensing, SN misclassification, selection bias, and calibration errors. Currently, none of these effects appears likely to challenge our conclusions.
description: Accepted to the Astrophysical Journal 38 pages, 15 figures, Pretty version available at http://icarus.stsci.edu/~stefano/ariess.tar.gz
Additional file 4: of Resources to Guide Exercise Specialists Managing Adults with Diabetes
Creators: name: Turner, Grant
name: Quigg, Scott
name: Davoren, Peter
name: Basile, Renata
name: McAuley, Sybil
name: Coombes, Jeff
Publisher: name: figshare
Year: 2019
Subjects: subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Marine Biology
subject: Plant Biology
subject: 60506 Virology

description: Type 1 Diabetes. (PDF 49 kb)
A single fast radio burst localized to a massive galaxy at cosmological distance
Creators: name: Bannister, K. W.
name: Deller, A. T.
name: Phillips, C.
name: Macquart, J. -P.
name: Prochaska, J. X.
name: Tejos, N.
name: Ryder, S. D.
name: Sadler, E. M.
name: Shannon, R. M.
name: Simha, S.
name: Day, C. K.
name: McQuinn, M.
name: North-Hickey, F. O.
name: Bhandari, S.
name: Arcus, W. R.
name: Bennert, V. N.
name: Burchett, J.
name: Bouwhuis, M.
name: Dodson, R.
name: Ekers, R. D.
name: Farah, W.
name: Flynn, C.
name: James, C. W.
name: Kerr, M.
name: Lenc, E.
name: Mahony, E. K.
name: O'Meara, J.
name: Osłowski, S.
name: Qiu, H.
name: Treu, T.
name: U, V.
name: Bateman, T. J.
name: Bock, D. C. -J.
name: Bolton, R. J.
name: Brown, A.
name: Bunton, J. D.
name: Chippendale, A. P.
name: Cooray, F. R.
name: Cornwell, T.
name: Gupta, N.
name: Hayman, D. B.
name: Kesteven, M.
name: Koribalski, B. S.
name: MacLeod, A.
name: McClure-Griffiths, N. M.
name: Neuhold, S.
name: Norris, R. P.
name: Pilawa, M. A.
name: Qiao, R. -Y.
name: Reynolds, J.
name: Roxby, D. N.
name: Shimwell, T. W.
name: Voronkov, M. A.
name: Wilson, C. D.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Fast Radio Bursts (FRBs) are brief radio emissions from distant astronomical sources. Some are known to repeat, but most are single bursts. Non-repeating FRB observations have had insufficient positional accuracy to localize them to an individual host galaxy. We report the interferometric localization of the single pulse FRB 180924 to a position 4 kpc from the center of a luminous galaxy at redshift 0.3214. The burst has not been observed to repeat. The properties of the burst and its host are markedly different from the only other accurately localized FRB source. The integrated electron column density along the line of sight closely matches models of the intergalactic medium, indicating that some FRBs are clean probes of the baryonic component of the cosmic web.
description: Published online in Science 27 June 2019
Tineobius (Tineobius) capensis Lucian Fusu & Antoni Ribes 2017, comb. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius capensis

description: 11. Tineobius (Tineobius) capensis (Ferrière, 1938) comb. nov.
Anastatoidea capensis Ferrière, 1938: 53–54, 58.
Syntypes ♀ (BMNH 5.945, examined by LF). Type locality: South Africa: Pondoland, Fort St. John.
Anastatoïdea capensis – Risbec 1952: 67, 68 (keyed, distribution).
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 12, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Amiota hesongensis Xu & Chen 2013, SP. NOV.
Creators: name: Zhao, Feng
name: Xu, Xiaoyang
name: Jiang, Jianjun
name: He, Xiaofang
name: Chen, Hongwei
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Drosophilidae
Amiota
Amiota hesongensis

description: AMIOTA HESONGENSIS XU & CHEN SP. NOV. (FIG. 3)
 Specimens examined: Holotype male (SCAU 110042) and four male paratypes (SCAU 121256–121259), China, Hesong, Menghai, Xishuangbanna, Yunnan, 1900 m a.s.l, 6–9 April 2011, J.M. Lu, Z.F. Shao, Y.R. Su, and S.J. Yan.
 Etymology: Pertaining to the type locality.
 Diagnosis: This species is similar to A. sinuata in the shape of the distal part of the paramere, but can be distinguished by the following characters. In A. sinuata, the distal part of the paramere is slightly longer than the basal part, which is basally not narrowed in lateral view (Fig. 1C in Chen & Toda, 1998b).
 Description: Male. Thorax brownish yellow, with dark-brown patches and stripes; pleura brownish; scutellum yellow, brown on margin. Abdominal tergites black; first to third yellow, medially. Male terminalia: epandrium pubescent except for anterior margin, with about ten setae near posterior margin on each side of the body (Fig. 3A). Surstylus with several setae and about nine prensisetae (Fig. 3B). Vertical lobe of gonopod broad, arched, slightly sclerotized (Fig. 3C). Paramere with a row of ~12 sensilla submedially to apically (Fig. 3C). Aedeagal apodeme longer than wide (Fig. 3C). Female: unknown.
 Measurements: BL = 2.80 mm in the holotype (range in four male paratypes: 2.78–2.85 mm), THL = 1.30 mm (1.20–1.35 mm), WL = 2.38 mm (2.22–2.40 mm), WW = 1.00 mm (0.90–1.00 mm), arb = 5/3 (5/3), avd = 0.85 (0.85–0.95), adf = 2.10 (2.00–2.10), flw = 2.00 (1.90–2.00), FW/HW = 0.35 (0.35), ch/o = 0.07 (0.07), prorb = 0.90 (0.90–1.00), rcorb = 0.65 (0.65–0.70), orbito = 2.30 (2.30–2.40), vb = 0.35 (0.35–0.40), dcl = 0.55 (0.50–0.60), sctl = 1.20 (1.20–1.30), sterno = 0.90 (0.85–0.95), dcp = 0.25 (0.25–0.28), sctlp = 1.00 (1.00), C = 1.23 (1.14–1.42), 4c = 2.10 (1.85–2.30), 4v = 2.85 (2.40–2.85), 5x = 1.50 (1.44–1.80), ac = 6.00 (4.11– 5.75), M = 0.90 (0.64–0.83), C3F = 0.83 (0.76–0.81).
 Distribution: China (Yunnan).
description: Published as part of Zhao, Feng, Xu, Xiaoyang, Jiang, Jianjun, He, Xiaofang & Chen, Hongwei, 2013, Molecular phylogenetic analysis of the Amiota apodemata and Amiota sinuata species groups (Diptera: Drosophilidae), with descriptions of four new species, pp. 849-858 in Zoological Journal of the Linnean Society 168 (4) on pages 853-854, DOI: 10.1111/zoj.12043, http://zenodo.org/record/5285870
Képességfejlesztő játékok az IPOO-modell aspektusából: a fejlesztésbe integrált diagnosztika lehetősége
Creators: name: Mező, Ferenc
name: Mező, Katalin
name: Mező, Lilla Dóra
Publisher: name: Debreceni Egyetem
Year: 2018

description: Különleges Bánásmód, vol. 4. issue 2. ISSN 2498-5368
Panathura Barnard 1925
Creators: name: Kensley, B.
name: Schotte, M.
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Expanathuridae
Panathura

description: Panathura Barnard, 1925
 Panathura Barnard, 1925:143; Kensley, 1982:159.
 Diagnosis. Body pigmented or not. Pleonites 1±5 free, articulating; pleonites 5 and 6 usually longer than preceding pleonites; pleonite 6 with posterior margin dorsally distinct. Eyes present. Mandible with molar blunt; palp of three articles. Maxillipedal endite distally rounded, reaching to palp article 3; palp with ®ve articles, suture between articles 1 and 2. Pereopods 1±3 diOEerentiated from posterior pereopods, propodus somewhat swollen, palm with few mesial setae. Pereopod 2 and 3 with robust distal seta. Pereopod 7, propodus with row of serrate setae anterodistally. Pleopod 1 exopod operculiform, endopod contributing somewhat in proximal region. Uropodal exopod lacking serrate lateral lobe.
Male: Rostrum stronger than in female. Eyes enlarged. Antennular ¯agellum of seven or more articles. Pereopods more elongate than in female; pereopod 1 propodus with increased number of setae on palm. Pleopod 2 appendix masculina as long or longer than rami.
description: Published as part of Kensley, B. & Schotte, M., 2000, New species and records of anthuridean isopod crustaceans from the Indian Ocean, pp. 2057-2121 in Journal of Natural History 34 on page 2083
Origin of the Hard X-ray Emission from the Galactic Plane
Creators: name: Ebisawa, Ken
name: Maeda, Yoshitomo
name: Kaneda, Hidehiro
name: Yamauchi, Shigeo
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Galactic plane is a strong hard x-ray emitter and the emission forms a narrow continuous ridge. The currently known hard x-ray sources are far too few to explain the ridge x-ray emission, and the fundamental question as to whether the ridge emission is ultimately resolved into numerous dimmer discrete sources or truly diffuse emission has not yet been settled. In order to obtain a decisive answer, using the Chandra x-ray observatory, we have carried out the deepest hard x-ray survey of a Galactic plane region which is devoid of known x-ray point sources. We have detected at least 36 new hard x-ray point sources in addition to strong diffuse emission within a 17' x 17' field of view. The surface density of the point sources is comparable to that at high Galactic latitudes after the effects of Galactic absorption are considered. Therefore, most of these point sources are probably extragalactic, presumably active galaxies seen through the Galactic disk. The Galactic ridge hard x-ray emission is diffuse, which indicates omnipresence of the hot plasma along the Galactic plane whose energy density is more than one order of magnitude higher than any other substances in the interstellar space.
description: three figures (two of them jpg files)
Multiplicity one theorem for $(\mathrm{GL}_{n+1},\mathrm{GL}_n)$ over a local field of positive characteristic
Creators: name: Mezer, Dor
Publisher: name: arXiv
Year: 2019
Subjects: subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 22E50 (Primary) 20G05, 20G25, 46F10 (Secondary)

description: Let $\mathbb{F}$ be a non-archimedean local field of positive characteristic different from 2. We consider distributions on $\mathrm{GL}(n+1,\mathbb{F})$ which are invariant under the adjoint action of $\mathrm{GL}(n,\mathbb{F})$. We prove that any such distribution is invariant with respect to transposition. This implies that the restriction to $\mathrm{GL}(n,\mathbb{F})$ of any irreducible smooth representation of $\mathrm{GL}(n+1,\mathbb{F})$ is multiplicity free.
description: This article draws heavily from arXiv:0707.2363 by other author
3D eclipse mapping in AM Herculis systems - `Genetically modified fireflies'
Creators: name: Ramsay, Pasi J. Hakala Mark Cropper Gavin
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In order to map the 3-dimensional location and shape of the emission originating within the accretion stream in AM Her systems, we have investigated the possibilities of relaxing the hitherto-applied constraint of a predetermined stream trajectory in modelling the eclipse profiles. We use emission points which can be located anywhere in the Roche lobe of the primary, together with a regularisation term which favours any curved stream structure, connected at the secondary and white dwarf primary. Our results show that, given suitable regularisation constraints, such inversion is feasible. We investigate the effect of removing the regularisation term, and also the sensitivity of the fit to input parameters such as inclination.
description: 10 pages, accepted for publication in MNRAS
Tineobius (Tineobius) citri Ashmead 1896, stat. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius citri

description: 12. Tineobius (Tineobius) citri Ashmead, 1896 stat. nov. [new subgeneric status]
Tineobius citri Ashmead, 1896: 15.
Holotype ♀, unique specimen (USNM 3465, not examined). Type locality: Australia, New South Wales, Paramatta.
Tineobius citri – Bouček 1988: 565, fgs 1004, 1005 (distribution, redescription).
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 12, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Amiota reikae Zhao & Xu & Jiang & He & Chen 2013, SP. NOV.
Creators: name: Zhao, Feng
name: Xu, Xiaoyang
name: Jiang, Jianjun
name: He, Xiaofang
name: Chen, Hongwei
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Drosophilidae
Amiota
Amiota reikae

description: AMIOTA REIKAE XU & CHEN SP. NOV. (FIG. 1)
 Specimens examined: Holotype male (SCAU 121071) and five male paratypes (SCAU 121072–121076), China, Mengla, Xishuangbanna, Yunnan, 600 m a.s.l., 17, 18 April 2007, HW Chen and JJ Gao.
 Etymology: Patronym, in honor of Ms Lihua Wang (SCAU), who helped Hongwei Chen in the study of drosophlids.
 Diagnosis: This species is similar to A. apodemata in the male terminalia, can be distinguished from the latter by having the paramere broad, slightly bifurcated dorsad, with a strongly sclerotized, arcuate process basally (pr; Fig. 1C, D).
 Description: Only the important characters are listed here; see Chen & Toda (1998a) for the rest (common to the apodemata group). Male terminalia: epandrium not constricted mid-dorsally, with about nine setae near posterior to ventral margins on each side of the body (Fig. 1A). Surstylus lacking pubescence, with finger-like process at posteroventral corner, about seven prensisetae on distal margin, and a few stout, spine-like setae on inner surface (Fig. 1B). Hypandrium narrowly separated into two lateral arches at middle of anterior portion (Fig. 1C, D). Gonopods sclerotized and slender (Fig. 1D). Parameres subbasally fused to each other, with numerous pits along outer margins (Fig. 1C, D). Aedeagus single, somewhat sclerotized, spoon-shaped lobe, basally fused to apodeme (Fig. 1C, D). Aedeagal apodeme nearly straight (Fig. 1C, D). Female: unknown.
 Measurements: Body length, BL = 2.46 mm in the holotype (range in five male paratypes: 2.44–2.60 mm), THL = 1.32 mm (1.20–1.36 mm), WL = 2.28 mm (2.00– 2.32 mm), WW = 1.04 mm (0.92–1.08 mm), arb = 5/3 (4/3–5/3), avd = 0.89 (0.71–0.90), adf = 2.25 (1.40– 2.20), flw = 2.75 (2.00–2.40), FW/HW = 0.44 (0.36– 0.51), ch/o = 0.12 (0.07–0.15), prorb = 0.92 (0.69–0.91), rcorb = 0.83 (0.64–0.77), orbito = 1.60 (1.60–2.30), vb = 0.50 (0.38–0.43), dc1 = 0.41 (0.38–0.52), presct1 = 0.45 (0.38–0.50), sct1 = 1.28 (1.21–1.38), sterno = 0.79 (0.64–0.86), dcp = 0.25 (0.22–0.29), sct1p = 0.89 (0.88– 1.33), C = 1.43 (1.32–1.77), 4c = 1.76 (1.61–1.76), 4v = 2.89 (2.35–2.67), 5x = 1.75 (1.38–1.88), ac = 5.00 (5.00– 7.25), M = 0.82 (0.60–0.76), C3F = 0.81 (0.73–0.84).
 Distribution: China (Yunnan).
description: Published as part of Zhao, Feng, Xu, Xiaoyang, Jiang, Jianjun, He, Xiaofang & Chen, Hongwei, 2013, Molecular phylogenetic analysis of the Amiota apodemata and Amiota sinuata species groups (Diptera: Drosophilidae), with descriptions of four new species, pp. 849-858 in Zoological Journal of the Linnean Society 168 (4) on pages 851-852, DOI: 10.1111/zoj.12043, http://zenodo.org/record/5285870
Comparative analysis of active and passive recreational consumption habits of disabled children living in the Northern Great Plain region
Creators: name: Laoues-Czimbalmos, Nóra
name: Müller, Anetta
name: Bába, Éva
Publisher: name: Debreceni Egyetem
Year: 2019

description: Különleges Bánásmód, vol. 5. issue 1. ISSN 2498-5368
Resolving the Topological Classification of Bismuth with Topological Defects
Creators: name: Nayak, Abhay Kumar
name: Reiner, Jonathan
name: Queiroz, Raquel
name: Fu, Huixia
name: Shekhar, Chandra
name: Yan, Binghai
name: Felser, Claudia
name: Avraham, Nurit
name: Beidenkopf, Haim
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Bulk boundary correspondence in topological materials allows to study their bulk topology through the investigation of their topological boundary modes. However, for classes that share similar boundary phenomenology, the growing diversity of topological phases may lead to ambiguity in the topological classification of materials. Such is the current status of bulk bismuth. While some theoretical models indicate that bismuth possesses a trivial topological nature, other theoretical and experimental studies suggest non-trivial topological classifications such as a strong or a higher order topological insulator, both of which hosts helical modes on their boundaries. Here we use a novel approach to resolve the topological classification of bismuth by spectroscopically mapping the response of its boundary modes to a topological defect in the form of a screw dislocation (SD). We find that the edge mode extends over a wide energy range, and withstands crystallographic irregularities, without showing any signs of backscattering. It seems to bind to the bulk SD, as expected for a topological insulator (TI) with non-vanishing weak indices. We argue that the small scale of the bulk energy gap, at the time reversal symmetric momentum $L$, positions bismuth within the critical region of a topological phase transition to a strong TI with non-vanishing weak indices. We show that the observed boundary modes are approximately helical already on the $\mathbb{Z}_2$ trivial side of the topological phase transition. This work opens the door for further possibilities to examine the response of topological phases to crystallographic topological defects, and to uniquely explore their associated bulk boundary phenomena.
Abundances in the Uranium-Rich Star CS 31082-001
Creators: name: Qian, Y. -Z.
name: Wasserburg, G. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent discovery by Cayrel et al. of U in CS 31082-001 along with Os and Ir at greatly enhanced abundances but with [Fe/H]=-2.9 strongly reinforces the argument that there are at least two kinds of SNII sources for r-nuclei. One source is the high-frequency H events responsible for heavy r-nuclei (A>135) but not Fe. The H-yields calculated from data on other ultra-metal-poor stars and the sun provide a template for quantitatively predicting the abundances of all other r-elements. In CS 31082-001 these should show a significant deficiency at A<135 relative to the solar r-pattern. It is proposed that CS 31082-001 should have had a companion that exploded as an SNII H event. If the binary survived the explosion, this star should now have a compact companion, most likely a stellar-mass black hole. Comparison of abundance data with predicted values and a search for a compact companion should provide a stringent test of the proposed r-process model. The U-Th age determined by Cayrel et al. for CS 31082-001 is, to within substantial uncertainties, in accord with the r-process age determined from solar system data. The time gap between Big Bang and onset of normal star formation only allows r-process chronometers to provide a lower limit on the age of the universe.
description: 5 pages, 1 figure
Additional file 1: of Role of KRAS in regulating normal human airway basal cell differentiation
Creators: name: Ogawa, Fumihiro
name: Walters, Matthew
name: Afrah Shafquat
name: OâBeirne, Sarah
name: Kaner, Robert
name: Mezey, Jason
name: Haijun Zhang
name: Leopold, Philip
name: Crystal, Ronald
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: Computational Biology

description: Figure S1. Effect of constitutive KRAS activity on expression of SOX family tran-scription factors and NOTCH pathway genes. (PDF 239 kb)
A Convolutional Decoder for Point Clouds using Adaptive Instance Normalization
Creators: name: Lim, Isaak
name: Ibing, Moritz
name: Kobbelt, Leif
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Graphics (cs.GR)
subject: FOS: Computer and information sciences

description: Automatic synthesis of high quality 3D shapes is an ongoing and challenging area of research. While several data-driven methods have been proposed that make use of neural networks to generate 3D shapes, none of them reach the level of quality that deep learning synthesis approaches for images provide. In this work we present a method for a convolutional point cloud decoder/generator that makes use of recent advances in the domain of image synthesis. Namely, we use Adaptive Instance Normalization and offer an intuition on why it can improve training. Furthermore, we propose extensions to the minimization of the commonly used Chamfer distance for auto-encoding point clouds. In addition, we show that careful sampling is important both for the input geometry and in our point cloud generation process to improve results. The results are evaluated in an auto-encoding setup to offer both qualitative and quantitative analysis. The proposed decoder is validated by an extensive ablation study and is able to outperform current state of the art results in a number of experiments. We show the applicability of our method in the fields of point cloud upsampling, single view reconstruction, and shape synthesis.
description: Symposium on Geometry Processing 2019
Leptanthura Sars 1899
Creators: name: Kensley, B.
name: Schotte, M.
Publisher: name: Zenodo
Year: 2000
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Anthuridae
Leptanthura

description: Genus Leptanthura Sars, 1899
 Leptanthura Sars, 1899: 47; Poore, 1978: 136; Poore, 1980: 61; Poore, 1981: 76.
 Diagnosis. Eyes usually lacking. Antennular ¯agellum of three to four articles. Antennal ¯agellum of four to ®ve articles. Mandibular palp of three articles. Maxillipedal endite obsolete. Pereopod 1 subchelate, propodus ināted. Pereopods 2 and 3 subchelate, propodi not as ināted as in pereopod 1. Pereopods 4±7 with carpi triangular, lacking free anterior margin. Pleopod 1 exopod operculiform. Pleonites short, free. Telson thin, often dorsally concave, with single basal statocyst.
description: Published as part of Kensley, B. & Schotte, M., 2000, New species and records of anthuridean isopod crustaceans from the Indian Ocean, pp. 2057-2121 in Journal of Natural History 34 on page 2106
Additional file 2: of Towards a definition of male partner involvement in the prevention of mother-to-child transmission of HIV in Uganda: a pragmatic grounded theory approach
Creators: name: Muwanguzi, Patience
name: Nassuna, Louise
name: Voss, Joachim
name: Joanita Kigozi
name: Muganzi, Alex
name: Ngabirano, Tom
name: Sewankambo, Nelson
name: Damalie Nakanjako
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Coding tree for male partner involvement in PMTCT (DOCX 18 kb)
Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
Creators: name: Sanz-Requena, J. F.
name: Perez-Hoyos, S.
name: Sanchez-Lavega, A.
name: del Rio-Gaztelurrutia, T.
name: Irwin, P. G. J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: In this paper we present a study of the vertical haze and cloud structure over a triple vortex in Saturn's atmosphere in the planetographic latitude range 55N-69N (del Rio- Gaztelurrutia et al. , 2018) using HST/WFC3 multispectral imaging. The observations were taken during 29-30 June and 1 July 2015 at ten different filters covering spectral range from the 225 nm to 937 nm, including the deep methane band at 889 nm. Absolute reflectivity measurements of this region at all wavelengths and under a number of illumination and observation geometries are fitted with the values produced by a radiative transfer model. Most of the reflectivity variations in this wavelength range can be attributed to changes in the tropospheric haze. The anticyclones are optically thicker ($τ\sim$ 25 vs $\sim$ 10), more vertically extended ($\sim$ 3 gas scale heights vs $\sim$ 2) and their bases are located deeper in the atmosphere (550 mbar vs 500 mbar) than the cyclone.
description: 36 pages, 16 figures
Tineobius (Tineobius) columbi Lucian Fusu & Antoni Ribes 2017, stat. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius columbi

description: 13. Tineobius (Tineobius) columbi (Girault, 1923) stat. nov. [new subgeneric status]
Metapelma columbi Girault, 1923: 96 –97.
Holotype ♀, unique specimen (QMBA T.4215, not examined). Type locality: Australia, Queensland, Kuranda.
Metapelma columbi – Dahms 1983: 189 (type information).
Anastatoidea columbi – Gahan 1927: 15 (keyed). — Ferrière 1936: 195 (catalogued). — Ferrière 1938: 45, 57 (keyed, distribution).
Anastatoïdea colombi – Risbec 1952: 67 (misspelling).
Tineobius columbi – Bouček 1988: 565.
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 12, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
The case of PSR J1911-5958A in the outskirts of NGC 6752: signature of a black hole binary in the cluster core?
Creators: name: Colpi, Monica
name: Possenti, Andrea
name: Gualandris, Alessia
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have investigated different scenarios for the origin of the binary millisecond pulsar PSR J1911-5958A in NGC 6752, the most distant pulsar discovered from the core of a globular cluster to date. The hypothesis that it results from a truly primordial binary born in the halo calls for accretion-induced collapse and negligible recoil speed at the moment of neutron star formation. Scattering or exchange interactions off cluster stars are not consistent with both the observed orbital period and its offset position. We show that a binary system of two black holes with (unequal) masses in the range of 3-100 solar masses can live in NGC 6752 until present time and can have propelled PSR J1911-5958A into an eccentric peripheral orbit during the last ~1 Gyr.
description: Accepted by ApJ Letter. 5 pages, 1 figure, 1 table
The Soap Bubble Theorem and a $p$-Laplacian overdetermined problem
Creators: name: Colasuonno, Francesca
name: Ferrari, Fausto
Publisher: name: arXiv
Year: 2019
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35J92, 35B06, 35N25, 53A10, 35A23

description: We consider the $p$-Laplacian equation $-Δ_p u=1$ for $1
description: 18 pages, 0 figures
Lax representation for the systems of S.Kowalevskaya type
Creators: name: Perelomov, A. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We descibe a number of dynamical systems that are generalizations of S. Kowalevskaya system and admit the Lax representation.
description: 4 pages
Reevaluating the species status of the southern ghost pipe, Monotropa brittonii (Ericaceae)
Creators: name: Keesling, Ashley
name: Freudenstein, John
name: Broe, Michael
Publisher: name: Zenodo
Year: 2021
Subjects: Florida
Host specificity
mycoheterotrophy
species delimitation.

description: Relationships among members of Ericaceae subfamily Monotropoideae have been notoriously difficult to resolve due to convergent evolution in these parasitic plants. All species in this subfamily are fully mycoheterotrophic, meaning they obtain nutrients by parasitizing fungi rather than through photosynthesis. Here, we examine relationships and host specificity in one of the most widespread species in this subfamily, Monotropa uniflora L. We use several lines of evidence to investigate whether there is support for recognizing a segregate, M. brittonii Small, as distinct. Based on molecular and morphological analysis of Monotropa collected throughout their range in the United States, we find two distinct lineages, one of which corresponds morphologically and geographically to Small's M. brittonii. We identified several morphological characters that differ between the two species. We also observed a high degree of fungal host specificity in M. brittonii, which appear to parasitize almost exclusively Lactifluus subgenus Lactariopsis section Albati. Additionally, M. brittonii were primarily collected from Florida scrub, which are xeric, shrub-dominated habitats that differ substantially from the mesic forests where M. uniflora typically occur. Based on these molecular, morphological, and ecological differences, we support recognition of M. brittonii as distinct from M. uniflora.
Additional file 1: of Towards a definition of male partner involvement in the prevention of mother-to-child transmission of HIV in Uganda: a pragmatic grounded theory approach
Creators: name: Muwanguzi, Patience
name: Nassuna, Louise
name: Voss, Joachim
name: Joanita Kigozi
name: Muganzi, Alex
name: Ngabirano, Tom
name: Sewankambo, Nelson
name: Damalie Nakanjako
Publisher: name: figshare
Year: 2019
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Focus Group Discussion guide (DOCX 20 kb)
Tineobius (Tineobius) crassipes
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius crassipes

description: 14. Tineobius (Tineobius) crassipes (Yoshimoto & Ishii,1965)
Anastatus crassipes Yoshimoto & Ishii, 1965: 156–158.
Holotype ♀, by original designation (BPBM 3581, not examined). Type locality: Caroline Island group: Palau Island, Koror.
Tineobius (Tineobius) crassipes – Gibson et al. 2012: 56.
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 12, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Cold Gas Kinematics in an L* Spiral Galaxy at z=0.437: The Nature of Damped Lyman-alpha Absorbers
Creators: name: Briggs, F. H.
name: de Bruyn, A. G.
name: Vermeulen, R. C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Westerbork Radio Synthesis Telescope observations of the redshifted 21cm line absorber against the z_em = 0.871 double lobed quasar 3C196 show that the intervening absorber is an L approximately equal L* spiral galaxy (3C196-G1) and that the absorbing layer of cold gas extends to radii of at least 30 h_50^-1 kpc. The new data solve several long standing puzzles about this system by (1) discovering a second 21cm absorption feature, corresponding to absorption against the NE lobe of the background radio source and (2) spatially ``resolving'' the two absorption features to isolate the absorption along the two lines of sight to the opposing radio lobes. These findings resolve the disagreement in redshift between the UV metal and 21cm lines, and as well as demonstrating that the neutral layer does absorb both lobes of the background radio source. Simple kinematic models with an inclined, rotating gas disk match the observed 21cm profile and are also compatible with both the redshift and velocity spread of the absorption measured in UV resonance lines along a third, independent line of sight to the quasar nucleus and with the lack of 21cm absorption in as earlier VLBI experiment that was sensitive to opacity against the hot spot in the northern lobe. The inferred rotation speed and luminosity for the galaxy are compatible with the z approximately 0 Tully-Fisher Relation. This system illustrates well how 21cm absorption against extended background radio sources is a powerful tool in determining the nature of the damped Lyman-alpha class of QSO absorption line system.
description: 9 pages, accepted at A&A
Additional file 2: of The efficacy of polyglycolic acid felt reinforcement in preventing postoperative pancreatic fistula after pancreaticojejunostomy in patients with main pancreatic duct less than 3â mm in diameter and soft pancreas undergoing pancreatoduodenectomy (PLANET-PJ trial): study protocol for a multicentre randomized phase III trial in Japan and Korea
Creators: name: Shibuya, Kazuto
name: Jang, Jin-Young
name: Satoi, Sohei
name: Sho, Masayuki
name: Yamada, Suguru
name: Kawai, Manabu
name: Hongbeom Kim
name: Kim, Song
name: Heo, Jin
name: Yoo-Seok Yoon
name: Park, Joon
name: Hwang, Ho
name: Isaku Yoshioka
name: Shimokawa, Toshio
name: Yamaue, Hiroki
name: Fujii, Tsutomu
Publisher: name: figshare
Year: 2019
Subjects: subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: SPIRIT 2013 Checklist: Recommended items to address in a clinical trial protocol and related documents (DOC 123 kb)
Symplectic tomography of nonlinear coherent states of a trapped ion
Creators: name: Man'ko, O. V.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Squeezed and rotated quadrature of an ion in a Paul trap is discussed in connection with reconstructing its quantum state using symplectic-tomography method. Marginal distributions of the quadrature for squeezed and correlated states and for nonlinear coherent states of a trapped ion are obtained and the density matrices in the Fock basis are expressed explicitly in terms of these marginal distributions.
Poecilimon luschani Ramme 1933
Creators: name: Boztepe, Zehra
name: Kaya, Sarp
name: Çiplak, Battal
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Poecilimon
Poecilimon luschani

description: POECILIMON LUSCHANI RAMME, 1933
 Poecilimon luschani Ramme, 1933: 539–540.
 All populations in the southern part of the group’s range constitute a single species with three different morphological units. Each of these units is considered as a subspecies. Of these morphounits, two correspond to the existing species P. luschani and P. birandi. Based on priority, P. luschani is retained as the species name and P. birandi is treated as a subspecies of P. luschani. The third morphounit is named as a new subspecies (Figs 1, 86). In two recent studies the entire Antalya + Mug˘la range was considered as a single species under the name of P. birandi (Çıplak et al., 2008; Kaya et al., 2012b). These records correspond to three subspecies of P. luschani.
description: Published as part of Boztepe, Zehra, Kaya, Sarp & Çiplak, Battal, 2013, Integrated systematics of the Poecilimon luschani species group (Orthoptera, Tettigoniidae): radiation as a chain of populations in a small heterogeneous area, pp. 43-69 in Zoological Journal of the Linnean Society 169 (1) on page 63, DOI: 10.1111/zoj.12058, http://zenodo.org/record/5287680
Quasinormal modes for quarkonium in a plasma with magnetic fields
Creators: name: Braga, Nelson R. F.
name: Ferreira, Luiz F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Heavy vector mesons detected after a heavy ion collision are important sources of information about the quark gluon plasma. The fraction of such particles that survive the plasma phase and reach the detectors is related to the dissociation degree inside the thermal medium. A consistent picture for the thermal behavior of charmonium and bottomonium quasi-states in a thermal medium was obtained recently using a holographic bottom up model. This model captures the heavy flavour spectroscopy of masses and decay constants in the vacuum (zero temperature) and is consistently extended to finite temperature. The spectral functions that emerge provide a description of the dissociation process in terms of the broadening of the quasi-state peaks with temperature. The holographic approach makes it possible to determine also the quasinormal modes. They are gravity solutions representing the quasi-particle states in the thermal medium, with complex frequencies related to the thermal mass and width. The quasinormal modes for charmonium and bottomonium have been studied very recently and a consistent description of the dissociation process was found. An additional factor can affect the dissociation process: strong magnetic fields are expected to be present when the plasma is formed by non-central heavy ion collisions. So, it is important to understand the effect of such fields on the heavy meson dissociation scenario. Here we extend the holographic determination of quasinormal modes for the case when magnetic fields are present. The real and imaginary parts of the mode frequencies are determined for different values of background $e B$ field. The associated dispersion relations for heavy quarks moving inside the plasma are also investigated for both $ c \bar c$ and $ b \bar b \, $.
description: 20 pages, 2 tables, 10 figures
The Star Formation History of LGS 3
Creators: name: Miller, B. W.
name: Dolphin, A. E.
name: Lee, M. G.
name: Kim, S. C.
name: Hodge, P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have determined the distance and star formation history of the Local Group dwarf galaxy LGS 3 from deep Hubble Space Telescope WFPC2 observations. LGS 3 is intriguing because ground-based observations showed that, while its stellar population is dominated by old, metal-poor stars, there is a handful of young, blue stars. Also, the presence of HI gas makes this a possible ``transition object'' between dwarf spheroidal and dwarf irregular galaxies. The HST data are deep enough to detect the horizontal branch and young main sequence for the first time. A new distance of D=620+/-20 kpc has been measured from the positions of the TRGB, the red clump, and the horizontal branch. The mean metallicity of the stars older than 8 Gyr is Fe/H = -1.5 +/- 0.3. The most recent generation of stars has Fe/H ~ -1. For the first few Gyr the global star formation rate was several times higher than the historical average and has been fairly constant since then. However, we do see significant changes in stellar populations and star formation history with radial position in the galaxy. Most of the young stars are found in the central 63 pc (21''), where the star formation rate has been relatively constant, while the outer parts have had a declining star formation rate.
description: To appear in The Astrophysical Journal, 26 pages, 14 figures, uses AASTeX