cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A Search for Lyman alpha Emitters at Redshift 3.7
Creators: name: Fujita, Shinobu S.
name: Ajiki, Masaru
name: Shioya, Yasuhiro
name: Nagao, Tohru
name: Murayama, Takashi
name: Taniguchi, Yoshiaki
name: Okamura, Sadanori
name: Ouchi, Masami
name: Shimasaku, Kazuhiro
name: Doi, Mamoru
name: Furusawa, Hisanori
name: Hamabe, Masaru
name: Kimura, Masahiko
name: Komiyama, Yutaka
name: Miyazaki, Masayuki
name: Miyazaki, Satoshi
name: Nakata, Fumiaki
name: Sekiguchi, Maki
name: Yagi, Masafumi
name: Yasuda, Naoki
name: Matsuda, Yuichi
name: Tamura, Hajime
name: Hayashino, Tomoki
name: Kodaira, Keiichi
name: Karoji, Hiroshi
name: Yamada, Toru
name: Ohta, Kouji
name: Umemura, Masayuki
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a survey for emission-line objects based on optical intermediate-band ($λ_{\rm c}$ = 5736 Å~ and $Δλ$ = 280 Å) and broad-band ($B$, $V$, $R$, and $i^\prime$) observations of the Subaru/XMM-Newton Deep Field on the 8.2 m Subaru telescope with the Subaru Prime Focus Camera, Suprime-Cam. All the data were obtained during the guaranteed time observations of the Suprime-Cam instrument. The intermediate-band image covered a sky area with 10\minpoint62 $\times 12\minpoint40 \approx 132$ arcmin$^2$ in the Subaru/XMM-Newton Deep Field (Ouchi et al.). Using this image, we have found 23 emission-line sources whose observed emission-line equivalent widths are greater than 250 Å. Their optical multicolor properties indicate that six emission-line sources are Ly$α$ emitters at $z \approx$ 3.7 ($Δz \approx 0.22$). They are either intense starburst galaxies or active galactic nuclei like quasars at $z \approx$ 3.7. Two more emission-line sources may also be Ly$α$ emitters at $z \approx$ 3.7 although their multicolor properties are marginal. Among the remaining 15 emission-line objects, eight objects appear strong emission-line galaxies at lower redshift; e.g., [O {\sc ii}] $λ$3727 emitters at $z \approx 0.54$, H$β$ at $z \approx 0.18$, or [O {\sc iii}]$λ$5007 emitters at $z \approx 0.15$. The remaining seven objects are unclassified because they are too faint to be detected in broad-band images. We discuss observational properties of these strong emission-line sources. In particular, our data allow us to estimate the star formation density at $z \approx 3.7$ for the first time.
description: Accepted for publication in AJ;14 pages, 26 figures (all figures are JPEG file)
On the "initial" Angular Momentum of Galaxies
Creators: name: Abel, Tom
name: Croft, Rupert C.
name: Hernquist, Lars
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Spherical density profiles and specific angular momentum profiles of Dark Matter halos found in cosmological N-body simulations have been measured extensively. The distribution of the total angular momentum of dark matter halos is also used routinely in semi-analytic modeling of the formation of disk galaxies. However, it is unclear whether the initial (i.e. at the time the halo is assembled) angular momentum distributions of baryons is related to the dark matter at all. Theoretical models for ellipticities in weak lensing studies often rely on an assumed correlation of the angular momentum vectors of dark matter and gas in galaxies. Both of these assumptions are shown to be in reasonable agreement with high resolution cosmological smoothed particle hydrodynamical simulations that follow the dark matter as long as only adiabatic gas physics are included. However, we argue that in more realistic models of galaxy formation one expects pressure forces to play a significant role at turn--around. Consequently the torquing force on DM and baryons will be uncorrelated and their respective angular momenta are not expected to align. An SPH simulation with ad-hoc feedback is presented that illustrates these effects. Massive low redshift elliptical galaxies may be a notable exception where "light may trace mass".
description: 4 latex pages (uses sprocl.sty), 1 eps figure. To appear in the proceedings of "The Shapes of Galaxies and Their Halos", Yale, May 2001
Multi-critical Behavior in Topological Phase Transitions
Creators: name: Rufo, S.
name: Lopes, Nei
name: Continentino, Mucio A.
name: R, Griffith M. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Topological phase transitions can be described by the theory of critical phenomena and identified by critical exponents that define their universality classes. This is a consequence of the existence of a diverging length at the transition that has been identified as the penetration depth of the surface modes in the non-trivial topological phase. In this paper, we characterize different universality classes of topological transitions by determining their correlation length exponents directly from numerical calculations of the penetration length of the edge modes as a function of the distance to the topological transition. We consider generalizations of the topological non-trivial Su-Schrieefer-Heeger (SSH) model, for the case of next nearest neighbors hopping and in the presence of a synthetic potential. The latter allows the system to transit between two universality classes with different correlation length and dynamic critical exponents. It presents a multi-critical point in its phase diagram since the behavior of the Berry connection depends on the path it is approached. We compare our results with those obtained from a scaling approach to the Berry connection.
description: 1) Improvements in figures 2 and 3. 2) To compare our results with previous works, we added a little sentence in the final of the page 10
Euphorbiaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae

description: Euphorbiaceae.
Acalypha ornata Hochst.ex A.Rich., Clutia abyssinica Jaub.& Spach, Croton macrostachyus Hochst. ex Delile, Phyllanthus niruri L., Synadenium grantii Hook. f., Tragia brevipes Pax.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 159, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Ichneumon pillichi KISS 1929
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Ichneumon
Ichneumon pillichi

description: Ichneumon pillichi KISS 1929
 Ichneumon pillichi KISS 1929: 97 f. – Holotypus (): "Simontornya (Kert), 1909.VII.6. Pillich.", "Hungaria" (in Ungarn) und Determinationsetiketten, Budapest
 G ü l t i g e r N a m e Spilothyrateles punctus (GRAVENHORST 1829) (Hilpert det.) (syn.nov.).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 778, DOI: 10.5281/zenodo.5429664
Derula delagrangei Puton 1892
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Derula
Derula delagrangei

description: Derula delagrangei Puton, 1892
 Material examined. FARS: Tang-e-Bostanak, 1650 m a.s.l., 1 specimen, 8.–9.vi.1996.
 Comments. In mountain steppes. Anatolian, known from the Asian part of Turkey and Iran.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 85, DOI: 10.5281/zenodo.5330439
A Transition to the Soft State in GRS 1758-258
Creators: name: Smith, D. M.
name: Heindl, W. A.
name: Markwardt, C. B.
name: Swank, J. H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Near the end of 2001 February, the black-hole candidate (BHC) GRS 1758-258 made an abrupt transition from a standard hard (low) state to a soft state. Unlike Cyg X-1 and other BHCs, whose luminosity increases during this transition, GRS 1758-258 was dimmer after the transition. We present observations with the Proportional Counter Array on the Rossi X-ray Timing Explorer and interpret the phenomenon in the context of a ``dynamical'' soft state model. Using this model we predicted that mass transfer from the companion had ceased, and that the luminosity should decay on a timescale of a few weeks. The most recent data support this prediction, being consistent with a decay time of 34 dy. The current state is consistent with the ``off'' state of GRS 1758-258 reported by GRANAT/Sigma in 1991-1992.
description: 13 pages, 5 figures, accepted for publication in The Astrophysical Journal Letters Accepted version has only minor changes, plus extra data showing more of the decay
MOESM2 of Association between cardiovascular autonomic neuropathy and left ventricular hypertrophy in young patients with congenital generalized lipodystrophy
Creators: name: Ponte, Clarisse
name: Fernandes, Virgínia
name: Liberato, Christiane
name: Montenegro, Ana
name: Batista, Lívia
name: Gurgel, Maria
name: Karbage, Lia Azevedo
name: Vasconcelos, Izabella
name: D’Alva, Catarina
name: Júnior, Renan Montenegro
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2. Clinical, biochemical and CAN parameters in patients with congenital generalized lipodystrophy and healthy individuals (n = 30).
Extended Magnetic Dome Induced by Low Pressures in Superconducting FeSe$_\mathrm{1\text{-}x}$S$_\mathrm{x}$
Creators: name: Holenstein, S.
name: Stahl, J.
name: Shermadini, Z.
name: Simutis, G.
name: Grinenko, V.
name: Chareev, D. A.
name: Khasanov, R.
name: Orain, J. -C.
name: Amato, A.
name: Klauss, H. -H.
name: Morenzoni, E.
name: Johrendt, D.
name: Luetkens, H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report muon spin rotation ($μ$SR) and magnetization measurements under pressure on Fe$_{1+δ}$Se$_\mathrm{1\text{-}x}$S$_\mathrm{x}$ with x $\approx 0.11$.Above $p\approx0.6$ GPa we find microscopic coexistence of superconductivity with an extended dome of long range magnetic order that spans a pressure range between previously reported separated magnetic phases. The magnetism initially competes on an atomic scale with the coexisting superconductivity leading to a local maximum and minimum of the superconducting $T_\mathrm{c}(p)$. The maximum of $T_\mathrm{c}$ corresponds to the onset of magnetism while the minimum coincides with the pressure of strongest competition. A shift of the maximum of $T_\mathrm{c}(p)$ for a series of single crystals with x up to 0.14 roughly extrapolates to a putative magnetic and superconducting state at ambient pressure for x $\geq0.2$.
description: 10 pages, 6 figures, including supplemental material
Additional file 1 of Retinal microvasculature dysfunction is associated with Alzheimer’s disease and mild cognitive impairment
Creators: name: Chua, Jacqueline
name: Hu, Qinglan
name: Ke, Mengyuan
name: Tan, Bingyao
name: Hong, Jimmy
name: Yao, Xinwen
name: Hilal, Saima
name: Venketasubramanian, Narayanaswamy
name: Garhöfer, Gerhard
name: Cheung, Carol Y.
name: Wong, Tien Yin
name: Chen, Christopher Li-Hsian
name: Schmetterer, Leopold
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Mental Health

description: Additional file 1: Supplementary information: Figure S1. Identification of study participants. Of the 165 participants, we excluded participants who were unable to complete OCTA scanning due to fatigue (n = 15), poor scan quality (n = 53), and presence of eye diseases (n = 7). Among the 90 participants included for the analysis, 24 were Alzheimer’s disease (AD) participants, 37 were mild cognitive impairment (MCI) participants, and 29 were controls. Figure S2. Receiver operating characteristic curves and corresponding AUCs for the top 3 parameters for discriminating AD/MCI from controls as compared to MTA scores ≥ 2. FD = fractal dimension; MTA = medial temporal atrophy; and VD = vessel density. Table S1. Multivariate analysis of OCTA metrics with MMSE scores Table S2. Multivariate analysis of OCTA metrics with presence of medial temporal atrophy (MTA) Table S3. Multivariate analysis of OCTA metrics with global cortical atrophy (GCA) Table S4. Multivariate analysis of OCTA metrics with white matter hyperintensities (WMH). Table S5. Diagnostic performance for cognitive status in decreasing order of the most relevant parameters.
Optical Detection of a Variable Millisecond Pulsar Companion in 47 Tucanae
Creators: name: Edmonds, Peter D.
name: Gilliland, Ronald L.
name: Heinke, Craig O.
name: Grindlay, Jonathan E.
name: Camilo, Fernando
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using results from radio and X-ray observations of millisecond pulsars in 47 Tucanae, and extensive HST U, V, I imaging of the globular cluster core, we have derived a common astrometric solution good to < 0.1". A close positional coincidence is found for 47 Tuc U, a 4.3 ms pulsar in a 0.429 day orbit, detected in radio and X-rays, with an m_V = 20.9 blue star. Analysis of extensive time series data for this optical candidate shows a 0.004 magnitude semi-amplitude variation at the period and phase expected from the radio ephemeris, and the optical variations are spatially coincident with the candidate. This provides secure optical detection of the white dwarf companion to the millisecond pulsar, the first such detection in a globular cluster, allowing for comparisons to recent models for such companions with dependencies on mass and age.
description: 8 pages, 3 figures, accepted in ApJ Letters. Revised content of discussion section
Additional file 1: of Plasmacytoid dendritic cells orchestrate innate and adaptive anti-tumor immunity induced by oncolytic coxsackievirus A21
Creators: name: MĂźller, Louise
name: Holmes, Matthew
name: Michael, Joanne
name: Scott, Gina
name: West, Emma J.
name: Scott, Karen
name: Parrish, Christopher
name: Hall, Kathryn
name: StĂ¤Ble, Sina
name: Jennings, Victoria
name: Cullen, Matthew
name: McConnell, Stewart
name: Langton, Catherine
name: Tidswell, Emma
name: Shafren, Darren
name: Samson, Adel
name: Harrington, Kevin
name: Pandha, Hardev
name: Ralph, Christy
name: Kelly, Richard
name: Cook, Gordon
name: Melcher, Alan
name: Errington-Mais, Fiona
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Table S1. Details of flow cytometry antibodies used in the study. (DOCX 15 kb)
Ichneumon ridibundus var. albicollis KISS 1924
Creators: name: Horstmann, K.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Ichneumonidae
Ichneumon
Ichneumon ridibundus
Ichneumon ridibundus gravenhorst var. albicollis kiss 1924

description: Ichneumon ridibundus GRAVENHORST var. albicollis KISS 1924
 Ichneumon ridibundus GRAVENHORST var. albicollis KISS 1924: 41 – praeocc. durch Ichneumon albicollis WESMAEL 1857 – Holotypus (): "Maros-Gombás Dr. Szilády" (= Gimbas/ Rumänien), "907.V.20" (Unterseite des Ortsetiketts) und Determinationsetikett, Budapest. Dem Typus fehlen beide Vorderflügel und ein Hinterflügel, dazu beide Hintertarsenspitzen.
 G ü l t i g e r N a m e Baranisobas lateritius (BERTHOUMIEU 1904) (Selfa det.) (syn.nov.).
description: Published as part of Horstmann, K., 2008, Typenrevisionen der von Kiss beschriebenen Taxa der Ichneumonidae. II. Ichneumoninae (Hymenoptera, Ichneumonidae), pp. 771-784 in Linzer biologische Beiträge 40 (1) on page 779, DOI: 10.5281/zenodo.5429664
MOESM1 of Association between cardiovascular autonomic neuropathy and left ventricular hypertrophy in young patients with congenital generalized lipodystrophy
Creators: name: Ponte, Clarisse
name: Fernandes, Virgínia
name: Liberato, Christiane
name: Montenegro, Ana
name: Batista, Lívia
name: Gurgel, Maria
name: Karbage, Lia Azevedo
name: Vasconcelos, Izabella
name: D’Alva, Catarina
name: Júnior, Renan Montenegro
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy
subject: Computational Biology

description: Additional file 1. Cardiovascular autonomic reflex tests.
Kinematics of diffuse elliptical galaxies
Creators: name: Prugniel, Philippe
name: Simien, Francois
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: New observations show that most of the flattened diffuse elliptical (dE) galaxies are essentially isotropic rotators. This supports the idea that dEs have evolved from fast rotating dIrr systems or late-type spirals after their gas was expelled by SN-driven winds and stripped by ram pressure against the intergalactic medium.
description: To be published in "The Evolution of Galaxies. III. From Simple Approaches to Self-Consistent Models", G. Hensler, Edt
Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
Creators: name: Ma, Xiangcheng
name: Grudić, Michael Y.
name: Quataert, Eliot
name: Hopkins, Philip F.
name: Faucher-Giguère, Claude-André
name: Boylan-Kolchin, Michael
name: Wetzel, Andrew
name: Kim, Ji-hoon
name: Murray, Norman
name: Kereš, Dušan
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: We report the formation of bound star clusters in a sample of high-resolution cosmological zoom-in simulations of z>5 galaxies from the FIRE project. We find that bound clusters preferentially form in high-pressure clouds with gas surface densities over 10^4 Msun pc^-2, where the cloud-scale star formation efficiency is near unity and young stars born in these regions are gravitationally bound at birth. These high-pressure clouds are compressed by feedback-driven winds and/or collisions of smaller clouds/gas streams in highly gas-rich, turbulent environments. The newly formed clusters follow a power-law mass function of dN/dM~M^-2. The cluster formation efficiency is similar across galaxies with stellar masses of ~10^7-10^10 Msun at z>5. The age spread of cluster stars is typically a few Myrs and increases with cluster mass. The metallicity dispersion of cluster members is ~0.08 dex in [Z/H] and does not depend on cluster mass significantly. Our findings support the scenario that present-day old globular clusters (GCs) were formed during relatively normal star formation in high-redshift galaxies. Simulations with a stricter/looser star formation model form a factor of a few more/fewer bound clusters per stellar mass formed, while the shape of the mass function is unchanged. Simulations with a lower local star formation efficiency form more stars in bound clusters. The simulated clusters are larger than observed GCs due to finite resolution. Our simulations are among the first cosmological simulations that form bound clusters self-consistently in a wide range of high-redshift galaxies.
description: 18 pages, 17 figures, accepted to MNRAS, high-quality images and/or animations for Figs 3,4,5,8,9 are available at http://www.tapir.caltech.edu/~xchma/HiZFIRE/globular/
The Fundamental Properties of Early-type Galaxies in the Coma Cluster
Creators: name: Moore, Stephen A. W.
name: Lucey, J. R.
name: Kuntschner, H.
name: Davies, R. L.
name: Colless, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a high quality spectral study of early-type galaxies within the Coma Cluster core. Stellar population analysis using Lick/IDS indices to break the age/metallicity degeneracy are presented, probing their formation history and properties. A clear metallicity trend and a dominant single age population are found.
description: 4 pages, 3 figures, from the conference proceedings of "The Evolution of Galaxies: I - Observational Clues" held in Granada, Spain on 23-27 May 2000
Graphosoma (Graphosoma) semipunctatum
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Graphosoma
Graphosoma semipunctatum

description: Graphosoma (Graphosoma) semipunctatum (Fabricius, 1775)
 Material examined. FARS: Zarqan Bamon National Park, 1650 m a.s.l., 3 specimens of f. wilsoni A. White, 1839, 13.–14.vi.1996.
 Comments. In mountain steppes. Holomediterranean, extending to Middle East and Central Asia.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 86, DOI: 10.5281/zenodo.5330439
Fabaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Fabales
Fabaceae

description: Fabaceae.
Crotalaria aculeata De Wild., Crotalaria lachnophora A.Rich., Crotalaria ononoides Benth., Crotalaria sp., Desmodium salicifolium (Poir.) DC., Desmodium setigerum (E.Mey.) Benth. ex Harv., Desmodium triflorum (L.) DC., Desmodium velutinum (Willd.) DC., Eriosema chrysadenium Taub., Eriosema rhodesicum R.E.Fr., Eriosema stanerianum Hauman, Indigofera emarginella Steud. ex A.Rich., Indigofera homblei Baker f. & Martin, Indigofera paracapitata J.B.Gillett, Indigofera rhynchocarpa Welw. ex Baker, Indigofera spicata Forssk., Indigofera zenkeri Harms ex Baker f., Rhynchosia sublobata (Schumach. & Thonn.) Meikle, Tephrosia linearis (Willd.) Pers., Teramnus labialis (L.f.) Spreng., Vigna luteola (Jacq.) Benth., Vigna parkeri Baker.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 159, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Testing Modified Gravity with Wide Binaries in GAIA DR2
Creators: name: Pittordis, Charalambos
name: Sutherland, Will
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Several recent studies have shown that very wide binary stars can potentially provide an interesting test for modified-gravity theories which attempt to emulate dark matter; these systems should be almost Newtonian according to standard dark-matter theories, while the predictions for MOND-like theories are distinctly different, if the various observational issues can be overcome. Here we explore an observational application of the test from the recent GAIA DR2 data release: we select a large sample of $\sim 24,000$ candidate wide binary stars with distance $< 200$ parsec and magnitudes $G < 16$ from GAIA DR2, and estimated component masses using a main-sequence mass-luminosity relation. We then compare the frequency distribution of pairwise relative projected velocity (relative to circular-orbit value) as a function of projected separation; these distributions show a clear peak at a value close to Newtonian expectations, along with a long `tail' which extends to much larger velocity ratios; the `tail' is considerably more numerous than in control samples constructed from DR2 with randomised positions, so its origin is unclear. Comparing the velocity histograms with simulated data, we conclude that MOND-like theories without an external field effect are strongly inconsistent with the observed data since they predict a peak-shift in clear disagreement with the data; testing MOND-like theories with an external field effect is not decisive at present, but has good prospects to become decisive in future with improved modelling or understanding of the high-velocity tail, and additional spectroscopic data.
description: Latex, 14 pages, 13 figures. v2: accepted by MNRAS, 05 Jul 2019; 3 figures added, conclusions unchanged
Epidose: Contact tracing for all
Creators: name: Spinellis, Diomidis
Publisher: name: Zenodo
Year: 2020
Subjects: exposure notification
epidemic dosimeter
contact tracing
COVID-19

description: This presentation describes an open source software and hardware reference implementation for an epidemic dosimeter. Just as a radiation dosimeter measures dose uptake of external ionizing radiation, the epidemic dosimeter tracks potential exposure to viruses or bacteria associated with an epidemic. The dosimeter measures a person's exposure to an epidemic, such as COVID-19, based on exposure to contacts that have been tested positive. The epidemic dosimeter is designed to be widely accessible and to safeguard privacy. Specifically, it is designed to run on the $10 open-hardware Raspberry Pi Zero-W computer, with a minimal user interface, comprising LED indicators regarding operation and exposure risk and a physical interlock switch to allow the release of contact data. The software is based on the DP3T contact tracing "unlinkable" design and corresponding reference implementation code, gratefully acknowledging the team's amazing work. The presentation was made at the 2020 EOSC Use Case meeting. Epidose is partly funded through the EOSC Secretariat. EOSCsecretariat.eu has received funding from the European Union's Horizon Programme call H2020-INFRAEOSC-05-2018-2019, grant Agreement number 831644.
MOESM2 of Population pharmacokinetics, exposure-safety, and immunogenicity of atezolizumab in pediatric and young adult patients with cancer
Creators: name: Shemesh, Colby
name: Chanu, Pascal
name: Jamsen, Kris
name: Wada, Russ
name: Rossato, Gianluca
name: Donaldson, Francis
name: Garg, Amit
name: Winter, Helen
name: Ruppel, Jane
name: Wang, Xin
name: Bruno, Rene
name: Jin, Jin
name: Girish, Sandhya
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Mental Health
subject: Virology

description: Additional file 2: Figure S2. Scatterplot of random effects of (A) clearance and (B) volume of distribution parameters by body surface area in pediatric patients. Solid circles represent estimates in 69 patients receiving 15 mg/kg intravenous atezolizumab q3w. The blue line represents a loess trend. Abbreviations: BSA body surface area, CL clearance, q3w every 3 weeks, V1 volume of the central compartment.
The Reddest Quasars II. A gravitationally-lensed FeLoBAL quasar
Creators: name: Lacy, M.
name: Gregg, M.
name: Becker, R. H.
name: White, R. L.
name: Glikman, E.
name: Helfand, D.
name: Winn, J. N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of a z=2.65 low-ionization iron broad absorption line quasar, FIRST J100424.9+122922, which is gravitationally-lensed by a galaxy at z~0.95. The object was discovered as part of a program to find very red quasars by matching the FIRST radio survey with the 2-MASS near-infrared survey. J100424.9+122922 is the second lensed system to be found in this program, suggesting that many gravitational lenses are probably missed from conventional optical quasar surveys. We have made a simple lens model and a rough estimate of the reddening in the immediate environment of the quasar which suggests that the quasar is intrinsically very luminous and is accreting at close to the Eddington limit of its ~10^9 M_sun black hole. The lensing galaxy has a small amount of dust which is responsible for some excess reddening observed in the fainter image of the quasar, but is otherwise a fairly typical massive elliptical galaxy. We model the selection effects working against the detection of red quasars in both lensed and unlensed samples. We show that these selection effects are very effective at removing even lightly-reddened high redshift quasars from magnitude-limited samples, whether they are lensed or not. This suggests that the red quasar population in general could be very large, and in particular the class of iron broad absorption line quasars of which J100424.9+122922 is a member may be much larger than their rarity in magnitude-limited samples would suggest.
description: 20 pages, 8 figures (3 color), accepted by AJ
Leprosoma stali Douglas & Scott 1868
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Leprosoma
Leprosoma stali

description: Leprosoma stali Douglas & Scott, 1868
 Material examined. FARS: 15 km E Sa’adatshahr, 1680 m a.s.l., 1 specimen, 6.–7.vi.1996.
 Comments. In mountain steppes. Syrio-Anatolian. Recorded from Egypt, Asian part of Turkey, Cyprus, Israel, Syria, Iraq, Iran, Armenia, and Azerbaijan (GAPON 2008).
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 86, DOI: 10.5281/zenodo.5330439
Couples and Technology - Wave 2 Addendum
Creators: name: Human, Lauren
name: Heyman, Jennifer
Publisher: name: OSF Registries
Year: 2020
Subjects: subject: Personality and Social Contexts
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: Lauren J. Human

description: After posting the associated preregistration for Wave 2 analyses (https://osf.io/n97q6) but before running analyses on Wave 2 data, we realized an error with our original Wave 1 R code wherein some of the columns indicated to convert the data from a wide to a long format were incorrect. Specifically, for the unstructured interaction, participants’ ratings of their partner’s affect were not being compared to the partner’s self-reported affect, but instead were being compared to participants’ meta-ratings of how they believe their partner was viewing them.

After fixing this error in the R code, the results of our Wave 1 analyses changed such that the significant main effect of cell phone condition (present vs. absent) on normative empathic accuracy became marginal. That is, those who had their phones with them during the interactions saw their partners with marginally greater levels of normative empathic accuracy compared to those who did not have their phones with them during the interactions. In addition, the significant mediation analyses also became marginal, such that the indirect effect from cell phone condition to relationship perceptions via normative empathic accuracy was marginal. The significant positive association between normative empathic accuracy and relationship perceptions remained significant.

In light of this, we plan to run the originally-planned preregistered analyses examining the main effect of cell phone condition on empathic accuracy, the association between empathic accuracy and relationship perceptions, and the mediation of cell phone condition influencing relationship perceptions via empathic accuracy on the combined Wave 1 and Wave 2 datasets in order to maximize power. This plan to use the combined Wave 1 and Wave 2 datasets was originally preregistered as a secondary analysis.
Translocation of Nitrate in Rice Rhizosphere and Total Nitrogen Uptake Improvement under Interactive Effect of Water and Nitrogen Supply
Creators: name: Rushimisha, Iranzi Emile
name: Wang, Weimu
name: Li, Yongtao
name: Li, Xiaojing
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Space Science
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Plant Biology

description: Nitrogen, an essential macronutrient for rice (Oryza sativa L), mineral forms are extremely prone to leaching. In this study, pot experiment in a greenhouse was utilized to investigate the coupling effect of irrigation (W) and fertilizer (N) on nitrate (NO3-N) translocation in the soil-water-plant system, Total Nitrogen (TN) uptake. Three N levels (Low, Medium, High: N1, N2, N3) rated 25, 120, and 250 mg/kg similarly three W levels (Low, Medium, High: W1, W2, W3) 70%-80%, 80%-90% and 100% of field capacity (θf) +0.5 cm submergence depth were applied. Nine treatments (W1N1:T1, W1N2:T2, W1N3:T3, W2N1:T4, W2N2:T5, W2N3:T6, W3N1:T7, W3N2:T8 and W3N3:T9) with four replicates. To understand NO3-N distribution, six soil layers (1 cm width each) per treatment were generated making it 54 in total. T6 (69.2%) revealed the highest increment in NO3-N content followed by T7 (44.2%) and T8 (39%) compared to T1. Generally, Middle layers (3rd-4th) had the least NO3-N content compared to shallow (1st-2nd) and bottom (5th-6th) layers. Concerning TN, the highest was found in T3(63%), T2(45%) and T6(41.5%) and T7(-26%) with the highest decrement. Interacting W and N significantly affected means of NO3-N, TN, moisture content, and root shoot ratio (R/S) at 5% probability level. Results of this study suggested that proper W and N combination result in high rhizosphere NO3-N accumulation in shallow layers leading to high nitrogen uptake by plant thus N leaching reduction.
Epidose: Ιχνηλάτηση επαφών για όλους
Creators: name: Spinellis, Diomidis
Publisher: name: Zenodo
Year: 2020
Subjects: contact tracing
exposure notification
COVID-19
epidemic dosimeter

description: This presentation describes an open source software and hardware reference implementation for an epidemic dosimeter. Just as a radiation dosimeter measures dose uptake of external ionizing radiation, the epidemic dosimeter tracks potential exposure to viruses or bacteria associated with an epidemic. The dosimeter measures a person's exposure to an epidemic, such as COVID-19, based on exposure to contacts that have been tested positive. The epidemic dosimeter is designed to be widely accessible and to safeguard privacy. Specifically, it is designed to run on the $10 open-hardware Raspberry Pi Zero-W computer, with a minimal user interface, comprising LED indicators regarding operation and exposure risk and a physical interlock switch to allow the release of contact data. The software is based on the DP3T contact tracing "unlinkable" design and corresponding reference implementation code, gratefully acknowledging the team's amazing work. The presentation was made at the 2021 Free and Open Source Software Communities Meeting (FOSSCOMM 2021). Epidose is partly funded through the EOSC Secretariat. EOSCsecretariat.eu has received funding from the European Union's Horizon Programme call H2020-INFRAEOSC-05-2018-2019, grant Agreement number 831644.
Additional file 7: of Adipose tissue protects against sepsis-induced muscle weakness in mice: from lipolysis to ketones
Creators: name: ChloĂŤ Goossens
name: Weckx, Ruben
name: Derde, Sarah
name: Dufour, Thomas
name: Perre, Sarah Vander
name: Pauwels, Lies
name: Thiessen, Steven
name: Veldhoven, Paul Van
name: Berghe, Greet Van Den
name: Langouche, Lies
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Supplemental Material and Methods. (DOCX 83 kb)
Photometry and membership for low mass stars in the young open cluster NGC 2516
Creators: name: Jeffries, R. D.
name: Thurston, M. R.
name: Hambly, N. C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a 0.86 square degree CCD photometric survey of the open cluster NGC 2516, which has an age of about 150 Myr and may have a much lower metallicity than the similarly-aged Pleiades. We select a preliminary catalogue of 1254 low mass (between 0.2 and 2.0M_{sun}) cluster candidates, of which about 70--80 percent are expected to be genuine. The mass function is metallicity dependent, but consistent with a Salpeter-like law (dN/dlog M ~ M^{-alpha}, alpha=+1.47+/-0.11 or alpha=+1.67+/-0.11 for solar and half-solar metallicities) between 0.7 and 3.0M_{sun}. At lower masses (between 0.3 and 0.7M_{sun}) there is a sharp fall in the mass function, with alpha=-0.75+/-0.20 (solar metallicity) or alpha=-0.49+/-0.13 (half-solar metallicity), which seems inconsistent with the much flatter mass functions seen in the Pleiades and field populations. We explain this by demonstrating that mass segregation has been at work in NGC 2516 -- more than half the cluster low mass stars are expected to lie outside out survey. The mass of NGC 2516 stars with mass greater than 0.3M_{sun} inside our survey is 950-1200M_{sun}, depending on metallicity and what corrections are applied for unresolved binarity. Correcting for mass segregation increases this to ~1240-1560M_{sun}, about twice the total mass of the Pleiades.
description: 27 pages, accepted for Astronomy & Astrophysics
title: Sharing the 'Self' Online: A multi-method investigation into young adults' self-disclosure motivations on social network sites
Creators: name: O'Donnell, Karlee J
Publisher: name: Griffith University
Year: 2023
Subjects: subject: social media
subject: young adult development
subject: relationships
subject: self-disclosure

description: This thesis investigates self-disclosure on social network sites (SNSs), with a specific focus on what drives young adults to share their thoughts, feelings, and experiences (i.e., self-disclose) online and the impacts of these disclosures on adjustment. Young adulthood is a distinct life period where young people navigate important developmental tasks such as establishing meaningful and intimate relationships and consolidating one’s sense of self. Self-disclosure is integral to navigating these tasks as it provides young adults with the means to learn about, connect with, and stay up to date with important others, as well as express and present aspects of the self. For contemporary young adults, SNSs are a popular platform for self-disclosure that offers convenient access to a network of others with whom to share their disclosures. Previous research has established that disclosing on SNSs is intrinsically rewarding for young adults (Towner et al., 2022; Van Gool et al., 2015; Varnali & Toker, 2015) and is typically driven by social validation, self-expression, and relationship development goals (Bazarova & Choi, 2014; Williamson et al., 2017). Although this research has provided insight into self-disclosure on SNSs, there is still much to learn about young adults SNS self-disclosure motivations. In this thesis, a multi-method approach across three empirical studies was employed to understand young adults’ own perceptions of what drives them to disclose on SNSs, the role of self-disclosure motivations in outcomes associated with SNS use, and whether young adults’ self-disclosure motivations are satisfied by their daily SNS use. [...]
Opportunities and Challenges of Standard Model Production Cross Section Measurements at 8 TeV using CMS Open Data
Creators: name: Apyan, Aram
name: Cuozzo, William
name: Klute, Markus
name: Saito, Yoshihiro
name: Schott, Matthias
name: Sintayehu, Bereket
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The CMS Open Data project offers new opportunities to measure cross sections of standard model (SM) processes which have not been probed so far. In this work, we evaluate the challenges and the opportunities of the CMS Open Data project in the view of cross-section measurements. In particular, we reevaluate SM cross sections of the production of W bosons, Z bosons, top-quark pairs and WZ dibosons in several decay channels at a center of mass energy of 8 TeV with a corresponding integrated luminosity of 1.8 fb-1. Those cross sections have been previously measured by the ATLAS and CMS collaborations and hence can be used to validate our analysis and calibration strategy. This gives an indication to which precision also new, so far unmeasured cross sections can be determined using CMS Open Data by scientists, who are not a member of the LHC collaborations and hence lack detailed knowledge on experimental and detector related effects and their handling.
description: 22 pages, 9 figures. arXiv admin note: text overlap with arXiv:1904.11195
Additional file 1: of PULSE-I - Is rePetitive Upper Limb SEnsory stimulation early after stroke feasible and acceptable? A stratified single-blinded randomised controlled feasibility study
Creators: name: Kausik Chatterjee
name: Stockley, Rachel
name: Lane, Steven
name: Watkins, Caroline
name: Cottrell, Katy
name: Ankers, Brenda
name: Davies, Sioned
name: Morris, Mary
name: Fallon, Nick
name: Nurmikko, Turo
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: PULSE feedback questionnaire for participants and their carers. (DOCX 27 kb)
EOSC Landscape Moving from Static Picture to Living - The work by INFRAEOSC5 projects
Creators: name: Tanlongo, Federica
Publisher: name: Zenodo
Year: 2021
Subjects: EOSC, Lansdcape, KPIs, INFRAEOSC5

description: The presentation introduces the why and how the INFRAEOSC5 landscape decided to approach the problem of defining and monitoring a set of living indicators to assess the level of EOSC-readiness at the country level. The work is still ongoing and will lead to the creation of a dashboard to collect the indicators and to test the workflows of information gathering with representatives of the national initiatives.
description: {"references": ["Arvola, Maijastiina, Beckmann, Volker, Budroni, Paolo, Castelli, Donatella, Cavalli, Valentino, Davidson, Joy, \u2026 Van Wezel, Jos. (2021, January 20). Second Working Proposal for Living Indicators to Monitor MS Progresses Towards EOSC Readiness. Zenodo. http://doi.org/10.5281/zenodo.4452799", "Directorate-General for Research and Innovation (European Commission) (2020), Country sheets analysis - Report from the EOSC Executive Board Working Group (WG) Landscape: ISBN 978-92-76-25379-2 DOI 10.2777/568900 Catalogue number KI-02-20-969-EN-N", "Directorate-General for Research and Innovation (European Commission) (2020), Landscape of EOSC-related infrastructures and initiatives, ISBN 978-92-76-25380-8\t DOI 10.2777/132181\t Catalogue number KI-02-20-971-EN-N"]}
Evidence for Accretion: High-Resolution X-ray Spectroscopy of the Classical T Tauri Star TW Hydrae
Creators: name: Kastner, Joel H.
name: Huenemoerder, David P.
name: Schulz, Norbert S.
name: Canizares, Claude R.
name: Weintraub, David A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present high resolution X-ray spectra of the X-ray bright classical T Tauri star, TW Hydrae, covering the wavelength range of 1.5-25 AA. The differential emission measure derived from fluxes of temperature-sensitive emission lines shows a plasma with a sharply peaked temperature distribution, peaking at log T = 6.5. Abundance anomalies are apparent, with iron very deficient relative to oxygen, while neon is enhanced relative to oxygen. Density-sensitive line ratios of Ne IX and O VII indicate densities near log n_e = 13. A flare with rapid (~1 ks) rise time was detected during our 48 ksec observation; however, based on analysis of the emission-line spectrum during quiescent and flaring states, the derived plasma parameters do not appear strongly time-dependent. The inferred plasma temperature distribution and densities are consistent with a model in which the bulk of the X-ray emission from TW Hya is generated via mass accretion from its circumstellar disk. Assuming accretion powers the X-ray emission, our results for log n_e suggest an accretion rate of ~10^{-8} M_sun yr^{-1}.
description: 14 pages, 6 figures; to appear in the Astrophysical Journal, March 1, 2002
Lamiaceae
Creators: name: Masharabu, Tatien
name: Bigendako, Marie Josée
name: Nzigidahera, Benoît
name: Mpawenayo, Balthazar
name: Lejoly, Jean
name: Bangirinama, Frédéric
name: Bogaert, Jan
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Lamiales
Lamiaceae

description: Lamiaceae.
Leucas calostachya Oliv., Solenostemon platostomoides (Robyns & Lebrun) Troupin.
description: Published as part of Masharabu, Tatien, Bigendako, Marie Josée, Nzigidahera, Benoît, Mpawenayo, Balthazar, Lejoly, Jean, Bangirinama, Frédéric & Bogaert, Jan, 2012, Vascular flora inventory and plant diversity of the Ruvubu National Park, Burundi, pp. 155-162 in Adansonia (3) (3) 34 (1) on page 159, DOI: 10.5252/a2012n1a17, http://zenodo.org/record/4599304
Leprosoma tuberculatum Jakovlev 1874
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Pentatomidae
Leprosoma
Leprosoma tuberculatum

description: Leprosoma tuberculatum Jakovlev, 1874
 Material examined. FARS: 15 km E Sa’adatshahr, 1680 m a.s.l., 1 specimen, 6.–7.vi.1996.
 Comments. In a mountain steppe on a shore of a salt lake with rich vegetation of Cyperus, Juncus, Phragmites, and grasses. Central Asiatic, extending from South Russia and Kazakhstan to the Middle East and China.
description: Published as part of Linnavuori, Rauno E., 2012, Studies on Pyrrhocoroidea, Coreoidea and Pentatomoidea of Khuzestan and the adjacent provinces in Iran (Hemiptera: Heteroptera), pp. 67-88 in Acta Entomologica Musei Nationalis Pragae 52 (1) on page 86, DOI: 10.5281/zenodo.5330439