cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Acinopus picipes
Creators: name: Wrase, DW
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Acinopus
Acinopus picipes

description: Acinopus (s.str.) picipes (OLIVIER 1795)
J o r d a n: Maan: Petra, 12.XI.2004, K. Orszulik leg. (1♀, cWR).
A mostly common species, widely distributed from the Iberian Peninsula to the Near and Middle East (CATPAL 1: WRASE 2003: 368). Findings from Jordan were expected. First record for Jordan.
description: Published as part of Wrase, DW, 2009, New or interesting records of Carabid beetles from Europe, Madeira, northern Africa, Turkey, from the Near East, Iran, Iraq, Kuwait, and Pakistan, with nomenclatorial and taxonomic notes (Coleoptera, Carabidae, Bembidiini, Brachinini, Cyclosomini, Elaphrini, Harpalini, Lebiini, Nebriini, Platynini,, pp. 901-935 in Linzer biologische Beiträge 41 (1) on page 916, DOI: 10.5281/zenodo.5276330
Reduction of light shifts in Ramsey spectroscopy with a combined error signal
Creators: name: Shuker, M.
name: Pollock, J. W.
name: Boudot, R.
name: Yudin, V. I.
name: Taichenachev, A. V.
name: Kitching, J.
name: Donley, E. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Light-induced frequency shifts can be a key limiting contribution to the mid and long-term frequency instability in atomic clocks. In this letter, we demonstrate the experimental implementation of the combined error signal interrogation protocol to a cold-atom clock based on coherent population trapping (CPT) and Ramsey spectroscopy. The method uses a single error signal that results from the normalized combination of two error signals extracted from two Ramsey sequences of different dark periods. The single combined error signal is used to stabilize the atomic clock frequency. Compared to the standard Ramsey-CPT interrogation, this method reduces the clock frequency sensitivity to light-shift variations by more than one order of magnitude. This method can be applied in various kinds of Ramsey-based atomic clocks, sensors and instruments.
Additional file 1 of Promoting equality, diversity and inclusion in research and funding: reflections from a digital manufacturing research network
Creators: name: Fisher, Oliver J.
name: Fearnshaw, Debra
name: Watson, Nicholas J.
name: Green, Peter
name: Charnley, Fiona
name: McFarlane, Duncan
name: Sharples, Sarah
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1.
Exploring optimal institutional incentives for public cooperation
Creators: name: Wang, Shengxian
name: Chen, Xiaojie
name: Szolnoki, Attila
Publisher: name: arXiv
Year: 2019
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Computer Science and Game Theory (cs.GT)
subject: Optimization and Control (math.OC)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: Prosocial incentive can promote cooperation, but providing incentive is costly. Institutions in human society may prefer to use an incentive strategy which is able to promote cooperation at a reasonable cost. However, thus far few works have explored the optimal institutional incentives which minimize related cost for the benefit of public cooperation. In this work, in combination with optimal control theory we thus formulate two optimal control problems to explore the optimal incentive strategies for institutional reward and punishment respectively. By using the approach of Hamilton-Jacobi-Bellman equation for well-mixed populations, we theoretically obtain the optimal positive and negative incentive strategies with the minimal cumulative cost respectively. Additionally, we provide numerical examples to verify that the obtained optimal incentives allow the dynamical system to reach the desired destination at the lowest cumulative cost in comparison with other given incentive strategies. Furthermore, we find that the optimal punishing strategy is a cheaper way for obtaining an expected cooperation level when it is compared with the optimal rewarding strategy.
description: Communications in Nonlinear Science and Numerical Simulation, Volume 79, December 2019, Article 104914
Veigaia nemorensis
Creators: name: Nemati, A.
name: Gwiazdowicz, D. J.
name: Riahi, E.
name: Mohseni, M.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Veigaiidae
Veigaia
Veigaia nemorensis

description: Veigaia nemorensis (Koch, 1839)
 Recorded in Kermanshah (34°18’51"N, 47°3’54"E) (Rijab) from soil (Babakfard et al., 2008); from Gachsaran (30°22’7"N, 50°48’24"E, H: 1279 m) (Kohgiloyeh Va Boir Ahmad province) in soils of rape seed and corn farms (Moradian et al., 2011); from the Homayjan region (30°14’33"N, 51°59’22"E, H: 2184 m) (Sepidan county) and Fars province (29°37’32"N, 52°31’8"E, H: 1810 m) from soils under apple trees (Maneshi et al., 2012).
New Records include reports from soil in Esfahan (32°39’37"N, 51°41’22"E, H: 1608 m), Shahrekord (32°19’39"N, 50°51’35"E, H: 2206 m), Baghmalek (31°31’22"N, 49°53’8"E, H: 707 m)(Khuzestan province), Ghaletol (31°37’55"N, 49°53’20"E, H: 885 m), and Izeh (31°49’52"N, 49°52’9"E, H: 845 m), coll., A. Nemati, 2011 and 2012.
description: Published as part of Nemati, A., Gwiazdowicz, D. J., Riahi, E. & Mohseni, M., 2013, Catalogue Of Mesostigmatid Mites Of Iran. Part 4: Parasitidae, Veigaiidae And Zerconidae, pp. 263-271 in Acarologia 53 (3) on page 267, DOI: 10.1051/acarologia/20132094, http://zenodo.org/record/5393444
Gamma-Ray Burst in a Molecular Cloud: Destruction of Dust and H2, and Emergent Spectrum
Creators: name: Draine, B. T.
name: Hao, Lei
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A gamma ray burst with strong optical-UV emission occuring in a molecular cloud will photodissociate H2, photoionize H2, H, and He, and destroy dust grains. We model these processes, including time-dependent radiative transfer in both continuum radiation and the resonance lines of H2. The UV will pump H2 into vibrationally-excited levels. We calculate the absorption spectrum imprinted on radiation from the GRB at various times. In addition to the strong absorption lines of H2(v=0) at lambda < 1110 Angstrom, due to cold ambient gas, we find that radiation reaching us from the GRB and its afterglow will show strong absorption lines due to vibrationally-excited H2 at 1110 < lambda < 1705 Angstrom. These absorption lines, if observed, would provide unequivocal evidence for association of the GRB with molecular gas. Low-resolution spectra will exhibit conspicuous features due to clustering of individual lines; a list of the strongest such absorption features is given for spectral resolution R approx 350 characteristic of the grism on the Swift UV-Optical Telescope.
description: submitted to ApJ, 27 pages, 11 figures, Latex
The 2001 Superoutburst of WZ Sagittae
Creators: name: Patterson, J.
name: Masi, G.
name: Richmond, M.
name: Martin, B.
name: Beshore, E.
name: Skillman, D.
name: Kemp, J.
name: Vanmunster, T.
name: Rea, R.
name: Allen, W.
name: Davis, S.
name: Davis, T.
name: Henden, A.
name: Starkey, D.
name: Foote, J.
name: Oksanen, A.
name: Cook, L.
name: Fried, R.
name: Husar, D.
name: Novak, R.
name: Campbell, T.
name: Robertson, J.
name: Krajci, T.
name: Pavlenko, E.
name: Mirabal, N.
name: Niarchos, P.
name: Brettman, O.
name: Walker, S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a worldwide campaign to observe WZ Sagittae during its 2001 superoutburst. After a 23-year slumber at V=15.5, the star rose within 2 days to a peak brightness of 8.2, and showed a main eruption lasting 25 days. The return to quiescence was punctuated by 12 small eruptions, of ~1 mag amplitude and 2 day recurrence time; these "echo outbursts" are of uncertain origin, but somewhat resemble the normal outbursts of dwarf novae. After 52 days, the star began a slow decline to quiescence. Periodic waves in the light curve closely followed the pattern seen in the 1978 superoutburst: a strong orbital signal dominated the first 12 days, followed by a powerful /common superhump/ at 0.05721(5) d, 0.92(8)% longer than P_orb. The latter endured for at least 90 days, although probably mutating into a "late" superhump with a slightly longer mean period [0.05736(5) d]. The superhump appeared to follow familiar rules for such phenomena in dwarf novae, with components given by linear combinations of two basic frequencies: the orbital frequency omega_o and an unseen low frequency Omega, believed to represent the accretion disk's apsidal precession. Long time series reveal an intricate fine structure, with ~20 incommensurate frequencies. Essentially all components occurred at a frequency n(omega_o)-m(Omega), with m=1, ..., n. But during its first week, the common superhump showed primary components at n (omega_o)-Omega, for n=1, 2, 3, 4, 5, 6, 7, 8, 9 (i.e., m=1 consistently); a month later, the dominant power shifted to components with m=n-1. This may arise from a shift in the disk's spiral-arm pattern, likely to be the underlying cause of superhumps. The great majority of frequency components ... . (etc., abstract continues)
description: PDF, 54 pages, 4 tables, 21 figures, 1 appendix; accepted, in press, to appear July 2002, PASP; more info at http://cba.phys.columbia.edu/
The Metadata Game
Creators: name: Habermann, Ted
Publisher: name: Zenodo
Year: 2019
Subjects: metadata training
FAIR Principles
collaborative games
metadata game
data management
libraries
repositories

description: A collaborative table-top game designed to help diverse teams work together to create complete metadata repositories. This introductory version is built around the general and high-level FAIR Principles. Other versions can be created around more specific community recommendations or needs.
Singularity formation in the Yang-Mills flow
Creators: name: Weinkove, Ben
Publisher: name: arXiv
Year: 2002
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics

description: This paper studies rapidly forming singularities in the Yang-Mills flow. It is shown that a sequence of blow-ups near the singular point converges, modulo the gauge group, to a homothetically shrinking soliton with non-zero curvature. The proof uses Hamilton's monotonicity formula. Examples of homothetically shrinking solitons are given in the case of trivial bundles over R^n for dimensions 5 through 9.
description: 13 pages. Final version, to appear in Calculus of Variations
Extraction of higher-order nonlinear electronic response to strong field excitation in solids using high harmonic generation
Creators: name: Han, Seunghwoi
name: Ortmann, Lisa
name: Kim, Hyunwoong
name: Kim, Yong Woo
name: Oka, Takashi
name: Chacon, Alexis
name: Doran, Brent
name: Ciappina, Marcelo
name: Lewenstein, Maciej
name: Kim, Seung-Woo
name: Kim, Seungchul
name: Landsman, Alexandra S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: State-of-the-art experiments employ strong ultrafast optical fields to study the nonlinear response of electrons in solids on an attosecond time-scale. Notably, a recent experiment retrieved a 3rd order nonlinear susceptibility by comparing the nonlinear response induced by a strong laser field to a linear response induced by the otherwise identical weak field. In parallel, experiments have demonstrated high harmonic generation (HHG) in solids, a highly nonlinear process that until recently had only been observed in gases. The highly nonlinear nature of HHG has the potential to extract even higher order nonlinear susceptibility terms, and thereby characterize the entire response of the electronic system to strong field excitation. However, up till now, such characterization has been elusive due to a lack of direct correspondence between high harmonics and nonlinear susceptibilities. Here, we demonstrate a regime where such correspondence can be clearly made, extracting nonlinear susceptibilities (7th, 9th, and 11th) from sapphire of the same order as the measured high harmonics. The extracted high order susceptibilities show angular-resolved periodicities arising from variation in the band structure with crystal orientation. Nonlinear susceptibilities are key to ultrafast lightwave driven optoelectronics, allowing petahertz scaling manipulation of the signal. Our results open a door to multi-channel signal processing, controlled by laser polarization.
Additional file 1: of An assessment of awareness of mental health conditions and its association with socio-demographic characteristics: a cross-sectional study in a rural district in Bangladesh
Creators: name: Uddin, Mohammed
name: Bhar, Sunil
name: Fakir M Islam
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Associations of socio-demographic characteristics with the combined awareness score of common MHCs items. (DOCX 18 kb)
Additional file 8: of Beneficial effects of curtailing immune susceptibility in an Alzheimerâ s disease model
Creators: name: Benedetto, Giulia Di
name: Burgaletto, Chiara
name: Carta, Anna
name: Saccone, Salvatore
name: Lempereur, Laurence
name: Mulas, Giovanna
name: Loreto, Carla
name: Bernardini, Renato
name: Cantarella, Giuseppina
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 60506 Virology
subject: Computational Biology

description: Table S1. List of all antibodies used, with respective working dilutions for either WB or IHF, as well as Companies of origin and catalog number specification. (PDF 290 kb)
Amenability and the bicrossed product construction
Creators: name: Desmedt, P.
name: Quaegebeur, J.
name: Vaes, S.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Quantum Algebra (math.QA)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics

description: We study stability properties of amenable locally compact quantum groups under the bicrossed product construction. We obtain as our main result an equivalence between amenability of the bicrossed product and amenability of the matched quantum groups used as building ingredients of the bicrossed product. Finally, we give examples of non-amenable locally compact quantum groups obtained by a bicrossed product construction.
description: 19 pages LaTeX
Veigaia planicola
Creators: name: Nemati, A.
name: Gwiazdowicz, D. J.
name: Riahi, E.
name: Mohseni, M.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Veigaiidae
Veigaia
Veigaia planicola

description: Veigaia planicola (Belese, 1892)
 Recorded in Esfahan (32°39’37"N, 51°41’22"E, H: 1608 m), Kermanshah (34°18’51"N, 47°3’54"E) (Rijab), and Tehran (35°42’2"N, 51°21’20"E, H: 1200 m) from soil (Babakfard et al., 2008; Jalaeian et al., 2004; Kamali et al., 2004); from Salmas region (West Azarbaijan province) in apple orchard soil (Alizadeh and Shirdel, 2012).
New Record from soil in Shahrekord (32°19’39"N, 50°51’35"E, H: 2206 m), coll., A. Nemati, 2011 and 2012.
 Kamali et al. (2001) reported V. serrata Willmann, 1936 from soils in E. Azarbaijan (38°4’36"N, 46°17’5"E, H: 1386 m), but this species has been considered as a junior synonym of V. planicola.
 Two unidentified species of this genus were recorded from cow manure in Kerman (30°16’39"N, 57°3’53"E, H: 1763 m) (Arjomandi et al., 2011) and from cotton field soil in Ardebil (48°31’33"N, 37°37’08"E, H: 1500 m) (Kamali et al., 2001).
description: Published as part of Nemati, A., Gwiazdowicz, D. J., Riahi, E. & Mohseni, M., 2013, Catalogue Of Mesostigmatid Mites Of Iran. Part 4: Parasitidae, Veigaiidae And Zerconidae, pp. 263-271 in Acarologia 53 (3) on page 268, DOI: 10.1051/acarologia/20132094, http://zenodo.org/record/5393444
Feeding Management of Dairy Animals
Creators: name: Manoj Sharma1, Nadeem Shah2* and Aditi Gupta3
Publisher: name: The Science world a Monthly e magazine
Year: 2024

description: Effective feeding management is crucial for maximizing milk production and maintaining the health of dairy animals. It involves formulating well-balanced diets, considering factors such as age, weight, and lactation stage. Regular monitoring of feed quality, nutritional content, and available pasture ensures optimal nutrition. Strategic feeding plans may be employed, adjusting rations based on individual needs. Incorporating supplements like vitamins and minerals further supports animal well-being. Additionally, proper water supply is integral to digestion and milk production. Overall, meticulous feeding management contributes to higher milk yields, improved reproductive performance, and enhanced profitability in dairy farming while promoting the longevity and welfare of the animals.
Deuterated molecules as a probe of ionization fraction in dense interstellar clouds
Creators: name: Caselli, Paola
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Deuterium fractionation in molecular ions, in particular HCO+, has been extensively used to estimate the degree of ionization in molecular clouds. This paper reviews recent work on ionization degree in homogeneous clouds. We will show that the N(DCO+)/N(HCO+) column density ratio furnishes a measurement of x(e) only in regions where CO is not significantly depleted, thus in the outer skirts of dense cloud cores. To probe x(e) deep inside the clouds, one has to gauge deuterium enhancement in molecular ions with parent species not affected by depletion (e.g. N2H+), and rely on chemical models which take into account the cloud density structure. Unlike N(DCO+)/N(HCO+), the N(N2D+)/N(N2H+) column density ratio is predicted to considerably increase with core evolution (and/or the amount of CO depletion), reaching large values (> 0.2) in cloud cores on the verge of forming a star.
description: 25 pages, 5 figures, accepted for publication in the special issue on "Deuterium in The Universe" of Planetary and Space Science
Additional file 2: of Exploring adultsâ experiences of sedentary behaviour and participation in non-workplace interventions designed to reduce sedentary behaviour: a thematic synthesis of qualitative studies
Creators: name: G. Rawlings
name: R. Williams
name: D. Clarke
name: C. English
name: C. Fitzsimons
name: I. Holloway
name: R. Lawton
name: G. Mead
name: A. Patel
name: A. Forster
Publisher: name: figshare
Year: 2019
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 60506 Virology

description: Excluded workplace-based studies (DOC 56 kb)
Direct Detection of Galactic Halo Dark Matter
Creators: name: Oppenheimer, B. R.
name: Hambly, N. C.
name: Digby, A. P.
name: Hodgkin, S. T.
name: Saumon, D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Milky Way Galaxy contains a large, spherical component which is believed to harbor a substantial amount of unseen matter. Recent observations indirectly suggest that as much as half of this ``dark matter'' may be in the form of old, very cool white dwarfs, the remnants of an ancient population of stars as old as the Galaxy itself. We conducted a survey to find faint, cool white dwarfs with large space velocities, indicative of their membership in the Galaxy's spherical halo component. The survey reveals a substantial, directly observed population of old white dwarfs, too faint to be seen in previous surveys. This newly discovered population accounts for at least 2% of the halo dark matter. It provides a natural explanation for the indirect observations, and represents a direct detection of Galactic halo dark matter.
description: 13 pages, 4 figures, 1 table. Note added after Science Express online publication: This text reflects the correction of a few typographical errors in the online version of the table. It also includes the new constraint on the calculation of d_max which accounts for the fact that the survey could not have detected stars with proper motions below 0.33 arcseconds per year. Published online at ScienceExpress www.sciencemag.org 22 March 2001; 10.1126/science.1059954; To appear in Science 27 April 2001
Quantum Robots Can Fly; Play Games: An IBM Quantum Experience
Creators: name: Mahanti, Soumik
name: Das, Santanu
name: Behera, Bikash K.
name: Panigrahi, Prasanta K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum Robot is an excellent future application that can be achieved with the help of a quantum computer. As a practical example, quantum controlled Braitenberg vehicles proposed by Raghuvanshi et al. [Proceedings of the 37th International Symposium on Multiple-Valued Logic (2007)] is a mobile quantum system and hence acts as a quantum robot. Braitenberg vehicles are simple circuit robots which can experience natural behaviours like fear, aggression and love etc. These robots can be controlled by quantum circuits incorporating quantum principles such as entanglement and superposition. Complex behaviours can be mimicked by a quantum circuit that can be implemented in a quantum robot. Here we investigate the scheme of Raghuvanshi et al. and propose a new quantum circuit to make the quantum robot fly. We demonstrate one of its application in playing a game. The quantum robot we present here shows the behaviour of `fear' and its movement is deterministic in nature. This phenomenon can be successfully modelled in a game, where it can always avoid accident. The proposed quantum circuit is designed in IBM quantum experience describing the above protocol.
description: 11 pages, 7 figures
Harpalus (Cephalophonus) cephalotes subsp. somcheticus SCHAUBERGER 1933
Creators: name: Wrase, DW
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Harpalus
Harpalus cephalotes
Harpalus (cephalophonus) cephalotes ssp. somcheticus schauberger 1933

description: Harpalus (Cephalophonus) cephalotes ssp. somcheticus SCHAUBERGER 1933
I r a n: Lorestan: Aligudarz, Ghalikuh, 2300 m, 30./ 31.VI.1990, Hashemi & Ebrahimi leg. (13, HMIM).
This subspecies is known from arid areas of SW-Transcaucasus area (SW-Armenia) and E-Turkey (KATAEV 2006: 142), hence above mentioned finding was expected. First record for Iran.
description: Published as part of Wrase, DW, 2009, New or interesting records of Carabid beetles from Europe, Madeira, northern Africa, Turkey, from the Near East, Iran, Iraq, Kuwait, and Pakistan, with nomenclatorial and taxonomic notes (Coleoptera, Carabidae, Bembidiini, Brachinini, Cyclosomini, Elaphrini, Harpalini, Lebiini, Nebriini, Platynini,, pp. 901-935 in Linzer biologische Beiträge 41 (1) on page 916, DOI: 10.5281/zenodo.5276330
Additional file 2 of MegaLMM: Mega-scale linear mixed models for genomic predictions with thousands of traits
Creators: name: Runcie, Daniel E.
name: Qu, Jiayi
name: Cheng, Hao
name: Crawford, Lorin
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Statistics
subject: FOS: Mathematics

description: Additional file 2 Review history.
Phenomemology of a Realistic Accelerating Universe Using Tracker Fields
Creators: name: Johri, Vinod B.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a realistic scenario of tracking of scalar fields with varying equation of state. The astrophysical constraints on the evolution of scalar fields in the physical universe are discussed. The nucleosynthesis and the galaxy formation constraints have been used to put limits on $Ω_ϕ$ and estimate $ε$ during cosmic evolution. Interpolation techniques have been applied to estimate $ε\simeq0.772$ at the present epoch. The epoch of transition from matter to quintessence dominated era and consequent onset of acceleration in cosmic expansion is calculated and taking the lower limit $Ω_n^0 = 0.2$ as estimated from $SN_e I_a$ data, it is shown that the supernova observations beyond redshift $z=1$ would reveal deceleration in cosmic expansion.
description: 10 pages, 4 figures, latex
Additional file 7: of Beneficial effects of curtailing immune susceptibility in an Alzheimerâ s disease model
Creators: name: Benedetto, Giulia Di
name: Burgaletto, Chiara
name: Carta, Anna
name: Saccone, Salvatore
name: Lempereur, Laurence
name: Mulas, Giovanna
name: Loreto, Carla
name: Bernardini, Renato
name: Cantarella, Giuseppina
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology

description: Figure S7. Negative controls for Fig. 8, panel b (phosphorylated Tau protein expression). Negative controls are reported in all panels marked with acronyms of secondary antibodies labeled with, Alexa Fluor 488. (PDF 491 kb)
Intersection multiplicities over Gorenstein rings
Creators: name: Miller, Claudia M.
name: Singh, Anurag K.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 14C17; 13H15; 14C15; 14C40

description: We construct a complex of free-modules over a Gorenstein ring R of dimension five, for which the Euler characteristic and Dutta multiplicity are different. This complex is the resolution of an R-module of finite length and finite projective dimension. As a consequence, the ring R has a nonzero Todd class tau_3(R) and a bounded free complex whose local Chern character does not vanish on this class. In the course of our work, we construct a module N of finite length and finite projective dimension over the hypersurface A=K[u,v,w,x,y,z]/(ux+vy+wz), such that the Serre intersection multiplicity of the modules N and A/(u,v,w)A is -2.
Harpalus fuscicornis MENETRIES 1832
Creators: name: Wrase, DW
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Harpalus
Harpalus fuscicornis

description: Harpalus (s.str.) fuscicornis MÉNÉTRIÉS 1832
I r a n: Māzandarān: Chalus env., VI 1998, Chr. Reuter leg. (233, cREUT, cWR). Hasan Keif, Kerla Dasht, 600 m, 7.V.2002, D. Gianasso leg. (13, MRSNT).
A widely distributed species, recorded from N-Africa and Spain to Middle Asia (CATPAL 1: KATAEV & WRASE: 376). First records for Iran.
description: Published as part of Wrase, DW, 2009, New or interesting records of Carabid beetles from Europe, Madeira, northern Africa, Turkey, from the Near East, Iran, Iraq, Kuwait, and Pakistan, with nomenclatorial and taxonomic notes (Coleoptera, Carabidae, Bembidiini, Brachinini, Cyclosomini, Elaphrini, Harpalini, Lebiini, Nebriini, Platynini,, pp. 901-935 in Linzer biologische Beiträge 41 (1) on page 917, DOI: 10.5281/zenodo.5276330
SomaliREN Annual Report 2023 Highlights
Creators: name: Siyad, Ahmed Dahir
Publisher: name: SORER
Year: 2024
Subjects: AnnualReport
FinancialReport
TechnicalReport
SecretariatOffice

description: This presentation is a highlight of the annual report which reflects on the accomplishments of SomaliREN over the past year,  it highlights progress and initiatives outlined in the Annual Report for 2023. Among the notable achievements in the past year is the finalization of our new five-year strategy plan, which will guide SomaliREN’s endeavors from 2023 to 2028. Grounded in SomaliREN’s shared mission and values, this strategy plan sets forth ambitious goals and key initiatives aimed at advancing education, research, and innovation for our member institutions.

In addition to the development of the strategy plan, SomaliREN has made significant strides in advancing connectivity, capacity building, and innovation throughout the year. SomaliREN, in collaboration with Hormuud Telecom, successfully upgraded the fiber infrastructure for several member institutions’ campuses, enhancing connectivity performance and enabling seamless collaboration and knowledge exchange. Furthermore, Direct Engineering Assistance program has provided tailored support to address the unique needs and challenges faced by SomaliREN members, ensuring optimal performance and reliability of their network infrastructure. SomaliREN’s commitment to driving innovation through the delivery of cutting-edge services and resources for higher education and research institutions remains unwavering, as we continue to empower our members with the tools and support they need to excel in their academic and research endeavors.
description: As we look ahead to the future, SomaliREN remains steadfast in its commitment to advancing connectivity and innovation across the Somali regions. We recognize that the digital landscape is constantly evolving, and we are committed to staying at the forefront of these changes to ensure that our members have access to the tools and resources they need to succeed.
MOESM1 of Renal temperature reduction progressively favors mitochondrial ROS production over respiration in hypothermic kidney preservation
Creators: name: Hendriks, Koen
name: BrĂźggenwirth, Isabel
name: Maassen, Hanno
name: Gerding, Albert
name: Bakker, Barbara
name: Porte, Robert
name: Henning, Robert
name: Leuvenink, Henri
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Marine Biology
subject: Inorganic Chemistry
subject: Computational Biology

description: Additional file 1: Figure S1. A: Live kidney oxygen and temperature registration during whole kidney perfusion at different temperatures. B: Live kidney flow registration during whole kidney perfusion at different temperatures. Figure S2. Oxygen consumption versus temperature in whole kidney perfusion. Data shown for up and downwards temperature curve. The Q10 line was fitted using the R package respirometry. Figure S3. A: Amplex Red assay verification, RFU levels at different concentrations H2O2, at different temperatures over time. B: Full membrane for the western blot on MnSOD. Arrow at 25Â kDa. C: Full membrane for the western blot on B-actin. Arrow at 50Â kDa.
Additional file 1: of Exploring adultsâ experiences of sedentary behaviour and participation in non-workplace interventions designed to reduce sedentary behaviour: a thematic synthesis of qualitative studies
Creators: name: G. Rawlings
name: R. Williams
name: D. Clarke
name: C. English
name: C. Fitzsimons
name: I. Holloway
name: R. Lawton
name: G. Mead
name: A. Patel
name: A. Forster
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: 111714 Mental Health
subject: FOS: Health sciences

description: Example search strategy (MEDLINE) (DOC 25 kb)
Evidence for Orbital Decay of RX J1914.4+2456: Gravitational Radiation and the Nature of the X-ray Emission
Creators: name: Strohmayer, Tod E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: RX J1914.4+2456 is a candidate double-degenerate binary (AM CVn) with a putative 569 s orbital period. If this identification is correct, then it has one of the shortest binary orbital periods known, and gravitational radiation should drive the orbital evolution and mass transfer if the binary is semi-detached. Here we report the results of a coherent timing study of the archival ROSAT and ASCA data for RX J1914.4+2456. We performed a phase coherent timing analysis using all five ROSAT observations spanning a 4.6 year period. We demonstrate that all the data can be phase connected, and we show evidence that the 1.756 mHz orbital frequency is increasing at a rate of 8 +- 3 e-18 Hz/s, consistent with the expected loss of angular momentum from the binary system via gravitational radiation. In addition to providing evidence for the emission of gravitational waves, our measurement of the orbital decay constrains models for the X-ray emission and the nature of the secondary. If stable mass accretion drives the X-ray flux, then orbital decay is inconsistent with a degenerate donor. A helium burning dwarf is compatible if indeed such systems can have periods as short as that of RX J1914.4+2456, an open theoretical question. Our measurement is consistent with the unipolar induction model of Wu et al. which does not require accretion to drive the X-ray flux. We discuss how future timing measurements of RX J1914.4+2456 (and systems like it) with for example, Chandra and XMM-Newton, can provide a unique probe of the interaction between mass loss and gravitational radiation. We also discuss the importance of such measurements in the context of gravitational wave detection from space, such as is expected in the future with the LISA mission.
description: AASTeX, 23 pages, 6 figures. Updated and revised version accepted for publication in the Astrophysical Journal
Dynamic Input for Deep Reinforcement Learning in Autonomous Driving
Creators: name: Hügle, Maria
name: Kalweit, Gabriel
name: Mirchevska, Branka
name: Werling, Moritz
name: Boedecker, Joschka
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Robotics (cs.RO)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: In many real-world decision making problems, reaching an optimal decision requires taking into account a variable number of objects around the agent. Autonomous driving is a domain in which this is especially relevant, since the number of cars surrounding the agent varies considerably over time and affects the optimal action to be taken. Classical methods that process object lists can deal with this requirement. However, to take advantage of recent high-performing methods based on deep reinforcement learning in modular pipelines, special architectures are necessary. For these, a number of options exist, but a thorough comparison of the different possibilities is missing. In this paper, we elaborate limitations of fully-connected neural networks and other established approaches like convolutional and recurrent neural networks in the context of reinforcement learning problems that have to deal with variable sized inputs. We employ the structure of Deep Sets in off-policy reinforcement learning for high-level decision making, highlight their capabilities to alleviate these limitations, and show that Deep Sets not only yield the best overall performance but also offer better generalization to unseen situations than the other approaches.
description: Accepted at IROS 2019
X-Ray Probes of Cosmic Star-Formation History
Creators: name: Ghosh, Pranab
name: White, Nicholas E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the imprints left by a cosmological evolution of the star formation rate (SFR) on the evolution of X-ray luminosities Lx of normal galaxies, using the scheme proposed by White and Ghosh (1998, WG98), wherein the evolution of Lx of a galaxy is driven by the evolution of its X-ray binary population. As indicated in WG98, the profile of Lx with redshift can both serve as a diagnostic probe of the SFR profile and constrain evolutionary models for X-ray binaries. We report here the first calculation of the expected evolution of X-ray luminosities of galaxies, updating the WG98 work by using a suite of more recently developed SFR profiles that span the currently plausible range. The first Chandra deep imaging results on Lx are beginning to probe the SFR profile of bright spirals: the early results are consistent with predictions based on current SFR models. Using these new SFR profiles, the resolution of the ``birthrate problem'' of low-mass X-ray binaries (LMXBs) and recycled, millisecond pulsars (WG98) in terms of an evolving global SFR is more complete. We discuss the possible impact of the variations in the SFR profile of individual galaxies and galaxy-types.
description: 16 pages, 2 Figures, Accepted for publication in ApJ Letters
Harpalus picipennis
Creators: name: Wrase, DW
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Harpalus
Harpalus picipennis

description: Harpalus (s.str.) picipennis (DUFTSCHMID 1812)
G r e e c e: Macedonía: Kavála: Stavroupoli env., 20.IV.2005, O. Hillert leg. (1♀, cWR).
Known on the Balkan Peninsula from Albania, Bosnia-Herzegovina, Bulgaria, und Yugoslavia, so its finding in Greece was expected. First record for Greece.
description: Published as part of Wrase, DW, 2009, New or interesting records of Carabid beetles from Europe, Madeira, northern Africa, Turkey, from the Near East, Iran, Iraq, Kuwait, and Pakistan, with nomenclatorial and taxonomic notes (Coleoptera, Carabidae, Bembidiini, Brachinini, Cyclosomini, Elaphrini, Harpalini, Lebiini, Nebriini, Platynini,, pp. 901-935 in Linzer biologische Beiträge 41 (1) on page 917, DOI: 10.5281/zenodo.5276330
Todd classes of affine cones of Grassmannians
Creators: name: Kurano, Kazuhiko
name: Singh, Anurag K.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 14C17; 13H15; 14C15; 14C40

description: A local ring R is said to be a Roberts ring if tau_R([R]) = [Spec R]_dim R, where tau_R is the Riemann-Roch map for Spec R. Such rings satisfy a vanishing theorem for the Serre intersection multiplicity, as was established by Paul Roberts in his proof of the Serre vanishing conjecture. It is known that complete intersections are Roberts rings, and the first author proved that a determinantal ring is a Roberts ring precisely if it is complete intersection. Let A_d(n) denote the affine cone of the Grassmannian G_d(n) under the Plucker embedding. We determine which of the rings A_d(n) are Roberts rings.
Probing Magnetism in Insulating Cr2Ge2Te6 by Induced Anomalous Hall Effect in Pt
Creators: name: Lohmann, Mark
name: Su, Tang
name: Niu, Ben
name: Hou, Yusheng
name: Alghamdi, Mohammed
name: Aldosary, Mohammed
name: Xing, Wenyu
name: Zhong, Jiangnan
name: Jia, Shuang
name: Han, Wei
name: Wu, Ruqian
name: Cui, Yong-Tao
name: Shi, Jing
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Two-dimensional ferromagnet Cr2Ge2Te6 (CGT) is so resistive below its Curie temperature that probing its magnetism by electrical transport becomes extremely difficult. By forming heterostructures with Pt, however, we observe clear anomalous Hall effect (AHE) in 5 nm thick Pt deposited on thin (< 50 nm) exfoliated flakes of CGT. The AHE hysteresis loops persist to ~ 60 K, which matches well to the Curie temperature of CGT obtained from the bulk magnetization measurements. The slanted AHE loops with a narrow opening indicate magnetic domain formation, which is confirmed by low-temperature magnetic force microscopy (MFM) imaging. These results clearly demonstrate that CGT imprints its magnetization in the AHE signal of the Pt layer. Density functional theory calculations of CGT/Pt heterostructures suggest that the induced ferromagnetism in Pt may be primarily responsible for the observed AHE. Our results establish a powerful way of investigating magnetism in 2D insulating ferromagnets which can potentially work for monolayer devices.
SwSt 1: an O-rich planetary nebula around a C-rich central star
Creators: name: De Marco, O.
name: Crowther, P. A.
name: Barlow, M. J.
name: Clayton, G. C.
name: deKoter, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The hydrogen-deficient carbon-rich [WCL] type central star HD167362 and its oxygen-rich planetary nebula (PN) SwSt~1 are investigated. The nebular chemistry might indicate a recent origin for the carbon-rich stellar spectrum. Its stellar and nebular properties might therefore provide further understanding of the origin of the [WCL] central star class. The UV-IR stellar spectra are modelled with state of the codes and show ~40kK central star with a wind and a C/O~3, indicative of efficient third dredge-up. The synthetic stellar flux distribution is used to model the high density, compact PN, which has a solar C/O ratio, is still enshrouded by 1200K and 230K dust shells and, reported here for the first time, in molecular hydrogen. Although it appears that the change in C/O ratio has been recent, the published spectroscopy since 1895 has been re-examined and no clear spectral change is seen. If an event occurred that has turned it into a hydrogen-deficient central star, it did not happen in the last 100 years.
description: 31 pages, 19 figures (some are gif files), MNRAS in press
Additional file 5: of Beneficial effects of curtailing immune susceptibility in an Alzheimerâ s disease model
Creators: name: Benedetto, Giulia Di
name: Burgaletto, Chiara
name: Carta, Anna
name: Saccone, Salvatore
name: Lempereur, Laurence
name: Mulas, Giovanna
name: Loreto, Carla
name: Bernardini, Renato
name: Cantarella, Giuseppina
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Hematology

description: Figure S5. Co-localization of CD3 and FoxP3 in the human AD brain. Immunofluorescence in representative samples for both molecules was detected in immune cells in the hippocampus of AD patients, whereas it was absent in the brain of healthy individuals (merge column; DAPIâ =â nuclear staining). Negative controls are reported in all panels marked with acronyms of secondary antibodies labeled with, respectively, Texas Red (TR) and Fluorescein isothiocyanate (FITC). (PDF 842 kb)
RR Lyrae pulsational temperature scales: On the consistency between different empirical relations
Creators: name: De Santis, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper, by assuming as correct equilibrium temperatures of RRab Lyrae variables those defined from Carney, Storm & Jones (1992, CSJ), we show that temperatures derived from (B-V) colour (mean colour over the pulsational cycle calculated on the magnitude scale) by Bessel, Castelli & Plez 1998 (BCP) transformations, are consistent with CSJ equilibrium temperatures within a probable error of $δ\log T_e = \pm 0.003$. As a consequence it is shown that the pulsational temperature scale, temperature-period-blue amplitude ($T_{eff}=f(P,A_B)$), provided by De Santis (1996, DS96) by (B-V) colour of about 70 stars of Lub's sample, is a suitable relation, reddening and metallicity free, to calculate equilibrium temperatures for RRab variables. This relation is independent from variable mass and luminosity within a large range of period-shift from the mean period-amplitude relation valid for the Lub's sample of variables. On the contrary, it is also shown that a temperature-amplitude-metallicity relation is strictly dependent from the period-amplitude relation of the sample used for calibrating it: we prove this means that it is dependent from both mass and luminosity variations of variables.
description: 6 pages, 5 postscript figures, accepted for publication on MNRAS
Additional file 6: of Beneficial effects of curtailing immune susceptibility in an Alzheimerâ s disease model
Creators: name: Benedetto, Giulia Di
name: Burgaletto, Chiara
name: Carta, Anna
name: Saccone, Salvatore
name: Lempereur, Laurence
name: Mulas, Giovanna
name: Loreto, Carla
name: Bernardini, Renato
name: Cantarella, Giuseppina
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Figure S6. Negative controls for Fig. 8, panel a (AÎ˛1â 42 expression). Negative controls are reported in all panels marked with acronyms of secondary antibodies labeled with, respectively, Texas Red (TR) (PDF 455 kb)
Harpalus polyglyptus SCHAUM 1862
Creators: name: Wrase, DW
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Carabidae
Harpalus
Harpalus polyglyptus

description: Harpalus (s.str.) polyglyptus SCHAUM 1862
G r e e c e Ipiros: Ioánnina: Ioánnina 21.IV.1993, J. Macek leg. (13, cW). - Stereá Ellas: Etolía Akarnanía: Kilisura env., 5 km S Agrínio, 14.-15.V.2006, L. Kašpar leg. (1♀, cKASP).
Described from "Corfu" (Kérkyra), this species, endemic to Greece, is seemingly rare in collections, up to now there are records from the Ionian Isles and from the Greek mainland (see also APFELBECK 1904: 189).
description: Published as part of Wrase, DW, 2009, New or interesting records of Carabid beetles from Europe, Madeira, northern Africa, Turkey, from the Near East, Iran, Iraq, Kuwait, and Pakistan, with nomenclatorial and taxonomic notes (Coleoptera, Carabidae, Bembidiini, Brachinini, Cyclosomini, Elaphrini, Harpalini, Lebiini, Nebriini, Platynini,, pp. 901-935 in Linzer biologische Beiträge 41 (1) on page 918, DOI: 10.5281/zenodo.5276330
Detection of the 2175ÅExtinction Feature at z=0.83
Creators: name: Motta, V.
name: Mediavilla, E.
name: Munoz, J. A.
name: Falco, E.
name: Kochanek, C. S.
name: Arribas, S.
name: Garcia-Lorenzo, B.
name: Oscoz, A.
name: Serra-Ricart, M.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We determine the extinction curve in the z_l=0.83 lens galaxy of the gravitational lens SBS0909+532 from the wavelength dependence of the flux ratio between the lensed quasar images (z_s=1.38) from 3400 to 9200Å. It is the first measurement of an extinction curve at a cosmological distance of comparable quality to those obtained within the Galaxy. The extinction curve has a strong 2175Åfeature, a noteworthy fact because it has been weak or non-existent in most estimates of extinction curves outside the Galaxy. The extinction curve is fitted well by a standard $R_V=2.1\pm0.9$ Galactic extinction curve. If we assume standard Galactic extinction laws, the estimated dust redshift of $z=0.88\pm0.02$ is in good agreement with the spectroscopic redshift of the lens galaxy. The widespread assumption that SMC extinction curves are more appropriate models for cosmological dust may be incorrect.
description: 17 pages, 5 figures. ApJ Accepted (Apr 4)