cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The role of expertise in policy development: Towards a De-carbonized British road transport Infrastructure
Creators: name: Witting, Antje
Publisher: name: Freie Universität Berlin
Year: 2012
Subjects: subject: 300 Sozialwissenschaften::380 Handel, Kommunikation, Verkehr::388 Verkehr; Landverkehr
subject: 300 Sozialwissenschaften::330 Wirtschaft::333 Boden- und Energiewirtschaft

description: Boundedly rational policy specialists simultaneously interact, learn and adapt their behaviour and the rules that guide them. Collective structures and norms incrementally change along the way. The research presented in this paper further investigates the possibility of a reciprocal causal relationship between the emergence of policy specialists’ generic understanding of a decision situation and the development of collective structures from a realist perspective. Of particular interest is how expertise on techno-scientific and ecological issues enters into and influences this process. The Advocacy Coalition Framework (ACF) guides the investigation. The ACF describes the ways in which fundamental policy core beliefs concerning strategies to deliver ontological axioms could lead to conflict, coordination and collective action. Furthermore the ACF explains how perturbations external to the system, and learning processes within the system, might change how individuals with an interest in the policy area perceive a decision situation and possibly alter the relations between them. The empirical work in this investigation develops on Dudley and Richardson’s ACF-based study of British road transport policy. Their study described the links between policy-oriented learning and change towards a more sustainable approach to road transport in the 1990s. This investigation is a longitudinal, record-based, micro-level study into how policy specialists, who share a common interest in the case, exchanged, utilized and readjusted their expertise over the period between January 1988 and December 2011. Social network analysis was used to identify case relevant specialists and the relational structure between them. The method to transcribe their policy core beliefs from archival records follows Axelrod (1976). Citations made verbally during policy development were recorded, to map and closely examine cases in which one individual evidently influenced the expertise of another.
Deuterated Ammonia in Galactic Protostellar Cores
Creators: name: Shah, Ronak Y.
name: Wootten, H. Alwyn
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on a survey of \nh2d towards protostellar cores in low-mass star formation and quiescent regions in the Galaxy. Twenty-three out of thirty-two observed sources have significant ($\gsim 5σ$) \nh2d emission. Ion-molecule chemistry, which preferentially enhances deuterium in molecules above its cosmological value of \scnot{1.6}{-5} sufficiently explains these abundances. NH2D/NH3 ratios towards Class 0 sources yields information about the ``fossil remnants'' from the era prior to the onset of core collapse and star formation. We compare our observations with predictions of gas-phase chemical networks.
description: 16 Pages, 7 Figures, Accepted to Ap.J., to appear in the June 20, 2001 edition
Stenus sculptor Puthz 2008, nov.sp.
Creators: name: Puthz, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenus
Stenus sculptor

description: Stenus (s.str.) sculptor nov.sp.
T y p e n m a t e r i a l - Holotypus und 1 - Paratypus: U. S. A.: California: Siskiyou Co., 12 mi SE Somes Bar, 1100 feet, 2.VI.1996, litter near stream, L. Herman; 1 - Paratypus: Siskiyou Co., 5.8 mi NE Forks of Salman, 1100 feet, litter near strem, 1.VI.1996, L. Herman. - HT und 1 PT im AMNH, 1 PT in cP.
B e s c h r e i b u n g Schwarz, ziemlich glänzend, Kopf ziemlich grob und dicht punktiert, Pronotum stark uneben, ziemlich grob punktiert und mehrfach furchig skulptiert, Elytren grob-furchig skulptiert, Abdomen vorn wenig grob, hinten wenig fein, überall sehr dicht, aber nicht gedrängt-dicht, punktiert, auffällig goldglänzend, anliegend beborstet. Fühler schwarzbraun. An den Kiefertastern das 1. Glied und die Basis des 2. Gliedes gelb, der Rest gebräunt bis dunkelbraun. Schenkel schwarzbraun, Schienen und Tarsen dunkelbraun. Clypeus und Oberlippe schwarz, mässig dicht beborstet.
Länge: 4,0- 5,2 mm (Vorderkörperlänge: 2,2-2,3 mm).
PM des HT: HW: 39; FW: 23; PW: 33: PL: 33: EW: 47,3; EL: 42; SL: 34.
M ä n n c h e n: unbekannt.
W e i b c h e n: 8. Sternit breit abgerundet. Valvifer apikolateral spitz. 10. Tergit abgerundet. Keine sklerotisierte Spermatheka.
 D i s k u s s i o n: Diese neue Art ist die Schwesterart des S. sculptilis CASEY, von dem ich bisher 830 Stücke aus British Columbia, Washington, Idaho, Oregon und Kalifornien gesehen habe. Sie gleicht ihm in fast allen Punkten, fällt aber durch ihre kurzen, vergleichsweise schmalen Elytren deutlich aus einer Variationsbreite heraus (Abb. 71). Ihre Skulptur ist auch weniger dicht als bei den kalifornischen S. sculptilis (dessen Elytren manchmal wegen enger Furchen fast matt erscheinen), auch ist die Punktierung der Abdomenspitze weniger dicht, nicht so gedrängt und auch etwas feiner als bei kalifornischen S. sculptilis; hierin kommt die neue Art S. sculptilis -Exemplaren aus British Columbien nahe.
 Ich möchte nicht ausschliessen, dass sich S. sculptilis möglicherweise als polytypische Spezies entpuppt (nördliche/ südliche Rassen); die hier beschriebenen Tiere fallen aber so deutlich aus dem bisher bekannten Matetrial heraus, dass man sie als eigene Art ansehen muss.
 E t y m o l o g i e: Ich nenne diese neue Art " sculptor " = Bildhauer, um einerseits ihre Nähe zu S. sculptilis zu signalisieren, andererseits um ihre kunstvoll skulptierten Elytren zu bezeichnen.
description: Published as part of Puthz, V., 2008, Stenus LATREILLE und die segenreiche Himmelstochter (Coleoptera, Staphylinidae), pp. 137-230 in Linzer biologische Beiträge 40 (1) on pages 158-159, DOI: 10.5281/zenodo.5426801
An unusually massive stellar black hole in the Galaxy
Creators: name: Greiner, J.
name: Cuby, J. G.
name: McCaughrean, M. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Here we report a measurement of the orbital period and mass function of GRS 1915+105 which allow us to deduce a mass of 14 +- 4 solar masses for its black hole. This large mass provides a challenge for black hole formation scenarios in binaries, since black holes with masses above 5-7 solar masses are hard to explain. Also, the mass estimate allows us to understand the unique X-ray variability of GRS 1915+105 as being due to instabilities of a radiation-pressure dominated disk radiating near the Eddington limit. Finally, several models are constrained which relate observable X-ray properties to the spin of black holes in microquasars. Once further calibrated, these relations may soon turn into a valuable tool to study relativistic effects in strong gravitational fields.
description: appeared in Nature 414, p. 522 (Nov. 29, 2001)
Wormaldia ladiel Malicky 2012, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Philopotamidae
Wormaldia
Wormaldia ladiel

description: Wormaldia ladiel nov.sp.
 Heller bis dunkler braun, Flügel mit dunklen Adern. Vorderflügelmitte mit einigen weissen Punkten, Gabel 4 im Vorderflügel fehlt. VFL 4-4,5 mm. KA (Tafel 8): 8. Tergit mit gewelltem Kaudalrand, darunter eine grosse, rundliche Höhlung. 9. Segment mit einem grossen Vorsprung oberhalb der Mitte des Vorderrandes. OA lang und schlank, etwas kürzer als das 10. Segment, das in DA basal breit und dann allmählich verschmälert ist, in LA schlank mit einem subdistalen dorsalen Höcker. UA lang und schlank, 2. Glied in LA stumpf zugespitzt, in VA gerade. PA mit einem kurzen starken Skleriten und einem, langen, dünnen Dorn innen, Ähnliche Arten sind W. amalek MALICKY 2009 aus Laos, W. dolophion SCHMID 1991 aus Indien und W. triacanthophora SUN 1998 aus Zhejiang, bei denen aber das subdistale Häkchen am Segment 10 fehlt und die Sklerite im PA im einzelnen verschieden sind.
Holotypus und 1 Paratypus und 1 vermutlich dazugehöriges: China, Jiangxi, Jinggang Shan, Baiyinhu env., 800m, 26°36‘N, 114°11‘E, 23.- 29.4.2011, leg. M. Fikáček & J. Hájek, NMP.
description: Published as part of Malicky, H., 2012, Neue asiatische Köcherfliegen aus neuen Ausbeuten (Insecta, Trichoptera), pp. 1263-1310 in Linzer biologische Beiträge 44 (2) on page 1271, DOI: 10.5281/zenodo.5329501
Exploring the Gamma Ray Horizon with the next generation of Gamma Ray Telescopes. Part 1: Theoretical predictions
Creators: name: Blanch, O.
name: Martinez, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The physics potential of the next generation of Gamma Ray Telescopes in exploring the Gamma Ray Horizon is discussed. It is shown that the reduction in the Gamma Ray detection threshold might open the window to use precise determinations of the Gamma Ray Horizon as a function of the redshift to either put strong constraints on the Extragalactic Background Light modeling or to obtain relevant independent constraints in some fundamental cosmological parameters.
description: Updated contents, 19 pages, 8 figures
Tidal resonance in extreme mass-ratio inspirals
Creators: name: Bonga, Béatrice
name: Yang, Huan
name: Hughes, Scott A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We describe a new class of resonances for extreme mass-ratio inspirals (EMRIs): tidal resonances, induced by the tidal field of nearby stars or stellar-mass black holes. A tidal resonance can be viewed as a general relativistic extension of the Kozai-Lidov resonances in Newtonian systems, and is distinct from the transient resonance already known for EMRI systems. Tidal resonances will generically occur for EMRIs. By probing their influence on the phase of an EMRI waveform, we can learn about the tidal environmental of the EMRI system, albeit at the cost of a more complicated waveform model. Observations by LISA of EMRI systems therefore have the potential to provide information about the distribution of stellar-mass objects near their host galactic-center black holes.
description: 5 pages; v2: matches version published in PRL
Stenopsyche sidon Malicky 2012, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Stenopsychidae
Stenopsyche
Stenopsyche sidon

description: Stenopsyche sidon nov.sp.
Körper gelblich bis bräunlich, Vorder- und Mitteltibien gelblich mit je zwei dunklen breiten Binden, 1. Glied der Mittelbeine mit einer solchen. Hinterbeine ganz gelblich, Antennen braun und schwach geringelt. Hinterflügel fahl hellbräunlich, Vorderflügel mit einem charakteristischen Muster laut Zeichnung (Tafel 21). VFL 20-25 mm. KA (Tafel 6): 9. Segment in LA ziemlich breit. 10. Segment ziemlich lang, in DA rechteckig und basal etwas bauchig, seine Seitenteile sind sehr gross, fast ebenso lang, breit und leicht sichelförmig gekrümmt und mit je einem subbasalen Vorsprung. UA in VA gerade und distal schräg abgestutzt. Die Dorsaläste sind s-förmig gebogen und distal leicht hakig. Die genauen Formen sind der Zeichnung zu entnehmen. Andere Arten mit so geformtem 10. Segment sind mir nicht bekannt.
Holotypus: China, Shaanxi, Qin Ling Mts., S von Xian, 5.9.200 6, leg. Kyselak, CM. 15 Paratypen: China, Shaanxi, Tai Bei Shan, 1300-1500m, 33°35‘N, 107°43‘E, 20.8.- 4.9.1998, leg. Murzin & Siniaiev, MNB.
description: Published as part of Malicky, H., 2012, Neue asiatische Köcherfliegen aus neuen Ausbeuten (Insecta, Trichoptera), pp. 1263-1310 in Linzer biologische Beiträge 44 (2) on pages 1272-1273, DOI: 10.5281/zenodo.5329501
Thermodynamics of Weakly Measured Quantum Systems
Creators: name: Alonso, Jose Joaquin
name: Lutz, Eric
name: Romito, Alessandro
Publisher: name: Freie Universität Berlin
Year: 2016
Subjects: subject: 500 Naturwissenschaften und Mathematik::530 Physik

description: We consider continuously monitored quantum systems and introduce definitions of work and heat along individual quantum trajectories that are valid for coherent superposition of energy eigenstates. We use these quantities to extend the first and second laws of stochastic thermodynamics to the quantum domain. We illustrate our results with the case of a weakly measured driven two-level system and show how to distinguish between quantum work and heat contributions. We finally employ quantum feedback control to suppress detector backaction and determine the work statistics.
Additional file 3: of Africaâ s challenged ENT services: highlighting challenges in Zambia
Creators: name: Lufunda Lukama
name: Kalinda, Chester
name: Aldous, Colleen
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: STROBE checklist. Checklist used in writing the manuscript. (DOCX 18 kb)
Joint User and Data Detection in Grant-Free NOMA with Attention-based BiLSTM Network
Creators: name: Khan, Saud
name: Durrani, Salman
name: Shahab, Muhammad Basit
name: Johnson, Sarah J.
name: Camtepe, Seyit
Publisher: name: arXiv
Year: 2022
Subjects: subject: Signal Processing (eess.SP)
subject: Machine Learning (cs.LG)
subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: We consider the multi-user detection (MUD) problem in uplink grant-free non-orthogonal multiple access (NOMA), where the access point has to identify the total number and correct identity of the active Internet of Things (IoT) devices and decode their transmitted data. We assume that IoT devices use complex spreading sequences and transmit information in a random-access manner following the burst-sparsity model, where some IoT devices transmit their data in multiple adjacent time slots with a high probability, while others transmit only once during a frame. Exploiting the temporal correlation, we propose an attention-based bidirectional long short-term memory (BiLSTM) network to solve the MUD problem. The BiLSTM network creates a pattern of the device activation history using forward and reverse pass LSTMs, whereas the attention mechanism provides essential context to the device activation points. By doing so, a hierarchical pathway is followed for detecting active devices in a grant-free scenario. Then, by utilising the complex spreading sequences, blind data detection for the estimated active devices is performed. The proposed framework does not require prior knowledge of device sparsity levels and channels for performing MUD. The results show that the proposed network achieves better performance compared to existing benchmark schemes.
Fast Spiking of a Mott VO2-Carbon Nanotube Composite Device
Creators: name: Bohaichuk, Stephanie M.
name: Kumar, Suhas
name: Pitner, Greg
name: McClellan, Connor J.
name: Jeong, Jaewoo
name: Samant, Mahesh G.
name: Wong, H-. S. Philip
name: Parkin, Stuart S. P.
name: Williams, R. Stanley
name: Pop, Eric
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The recent surge of interest in brain-inspired computing and power-efficient electronics has dramatically bolstered development of computation and communication using neuron-like spiking signals. Devices that can produce rapid and energy-efficient spiking could significantly advance these applications. Here we demonstrate DC-current or voltage-driven periodic spiking with sub-20 ns pulse widths from a single device composed of a thin VO2 film with a metallic carbon nanotube as a nanoscale heater. Compared with VO2-only devices, adding the nanotube heater dramatically decreases the transient duration and pulse energy, and increases the spiking frequency, by up to three orders of magnitude. This is caused by heating and cooling of the VO2 across its insulator-metal transition being localized to a nanoscale conduction channel in an otherwise bulk medium. This result provides an important component of energy-efficient neuromorphic computing systems, and a lithography-free technique for power-scaling of electronic devices that operate via bulk mechanisms.
Overlap renormalization group transformations for disordered systems
Creators: name: Bachtis, Dimitrios
Publisher: name: arXiv
Year: 2023
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: We establish a renormalization group approach which is implemented on the degrees of freedom defined by the overlap of two replicas to determine the critical fixed point and to extract four critical exponents for the phase transition of the three-dimensional Edwards-Anderson model. In addition, we couple the overlap order parameter to a fictitious field and introduce it within the two-replica Hamiltonian of the system to study its explicit symmetry-breaking with the renormalization group. Overlap transformations do not require a renormalization of the random couplings of a system to extract the critical exponents associated with the relevant variables of the renormalization group. We conclude by discussing the applicability of such transformations in the study of any phase transition which is fully characterized by an overlap order parameter.
Additional file 1: of The reproducibility of psychiatric evaluations of work disability: two reliability and agreement studies
Creators: name: Kunz, Regina
name: Allmen, David
name: Marelli, Renato
name: Hoffmann-Richter, Ulrike
name: Joerg Jeger
name: Mager, Ralph
name: Colomb, Etienne
name: Schaad, Heinz
name: Bachmann, Monica
name: Vogel, Nicole
name: Busse, Jason
name: Eichhorn, Martin
name: BĂ¤Nziger, Oskar
name: Zumbrunn, Thomas
name: Boer, Wout
name: Fischer, Katrin
Publisher: name: figshare
Year: 2019
Subjects: subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Planned design versus actual conduct of the studies. Comparison of the design for the RELY study as planned with the actual conduct of the studies as RELY 1 and RELY 2. *SIMâ =â Swiss Insurance Medicine, professional society of medical experts (DOCX 15 kb)
Additional file 2: of Africaâ s challenged ENT services: highlighting challenges in Zambia
Creators: name: Lufunda Lukama
name: Kalinda, Chester
name: Aldous, Colleen
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Description of terms. Terms applicable to the Zambian health care system at the time the study was conducted. (DOCX 17 kb)
The Cosmic Radio and Infrared Backgrounds Connection
Creators: name: Dwek, Eli
name: Barker, Michael K.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use the radio-infrared (IR) flux correlation bet ween star-forming galaxies in the local universe to derive a simple analytical expression between the intensity of the IR background and the brightness t emperature of the radio background. This relation i s insensitive to the star formation history of the galaxies that produce the cosmic IR background (CIB). We use the observed CIB intensity to constrain t he cosmic star formation history, and the relation between the CIB and the cosmic radio background (CR B) to constrain the relative contribution of star-f orming galaxies to the CRB. Current limits on the C IB intensity predict a 178 MHz brightness temperature of ~18+-9 K, about half of the 37+-8 K inferred for an isotropic radio component. This suggests that s tar-forming galaxies and AGN contribute about equal ly to the CRB intensity at that frequency.
description: Accepted for publication in the ApJ (14 pages + 3 embedded figures)
Stenus (Hemistenus) ochropus KIESENWETTER 1858
Creators: name: Puthz, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenus
Stenus ochropus

description: Stenus (Hemistenus) ochropus KIESENWETTER 1858
 Stenus ochropus KIESENWETTER 1858: 125; HERMAN 2001: 2310 ff.
 Stenus cres PUTHZ 1971a: 3 fig. syn.nov.
 Im Laufe der letzten dreissig Jahre habe ich umfangreiches Material von S. ochropus untersucht, darunter zahlreiche Stücke von Kreta: der Umriss des vorderen Medianlobus, seitlich meist leicht konkav ausgebuchtet, variiert deutlich, und auch die Bedornung der Beine schwankt zwischen "deutlich vorhanden" und "fehlend". S. cres wird deshalb in die Variationsbreite des S. ochropus gestellt.
description: Published as part of Puthz, V., 2008, Stenus LATREILLE und die segenreiche Himmelstochter (Coleoptera, Staphylinidae), pp. 137-230 in Linzer biologische Beiträge 40 (1) on page 161, DOI: 10.5281/zenodo.5426801
Stenopsyche camor Malicky 2012, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Stenopsychidae
Stenopsyche
Stenopsyche camor

description: Stenopsyche camor nov.sp.
 Das Belegstück ist nicht gut erhalten, aber die Vorderflügel scheinen eine relativ einheitliche helle Sprenkelung zu haben. VFL ca. 24 mm. KA (Tafel 6): 9. Segment in LA schmal, der Vorsprung der Kaudalkante ist lang und spitz, die OA sind relativ breit. 10. Segment sehr kurz, aus einem Paar ovaler Lappen bestehend, dazwischen distal eingeschnitten, und lateral an der Basis mit je einem kleinen Häkchen. UA in VA schmal und bei gerader Innenkante und gebogener Aussenkante zugespitzt, ihre Dorsaläste laut Zeichnung geschwungen. Ähnlich ist S. arvadit MALICKY 2008 aus Taiwan, bei der aber das 10. Segment und die Dorsaläste der UA in DA andere Proportionen haben.
Holotypus: China, Shaanxi, Daba Shan, 15 km S Shou-Man vill., 32°08‘N, 108°37‘E, 25.5.- 14.6.200 0, leg. Siniaiev & Plutenko, MNB.
description: Published as part of Malicky, H., 2012, Neue asiatische Köcherfliegen aus neuen Ausbeuten (Insecta, Trichoptera), pp. 1263-1310 in Linzer biologische Beiträge 44 (2) on page 1273, DOI: 10.5281/zenodo.5329501
Machine learning applications for the study of AGN physical properties using photometric observations
Creators: name: Mechbal, Sarah
name: Ackermann, Markus
name: Kowalski, Marek
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate the physical nature of active galactic nuclei (AGNs) using machine learning (ML) tools. We show that the redshift, $z$, bolometric luminosity, $L_{\rm Bol}$, central mass of the supermassive black hole (SMBH), $M_{\rm BH}$, Eddington ratio, $λ_{\rm Edd}$, and AGN class (obscured or unobscured) can be reconstructed through multi-wavelength photometric observations only. We trained a random forest regressor (RFR) ML-model on 7616 spectroscopically observed AGNs from the SPIDERS-AGN survey, which had previously been cross-matched with soft X-ray observations (from ROSAT or XMM), WISE mid-infrared photometry, and optical photometry from SDSS \textit{ugriz} filters. We built a catalog of 21050 AGNs that were subsequently reconstructed with the trained RFR; for 9687 sources, we found archival redshift measurements. All AGNs were classified as either type 1 or type 2 using a random forest classifier (RFC) algorithm on a subset of known sources. All known photometric measurement uncertainties were incorporated via a simulation-based approach. We present the reconstructed catalog of 21050 AGNs with redshifts ranging from $ 0 < z < 2.5$. We determined $z$ estimations for 11363 new sources, with both accuracy and outlier rates within 2%. The distinction between type 1 or type 2 AGNs could be identified with respective efficiencies of 94% and 89%. The estimated obscuration level, a proxy for AGN classification, of all sources is given in the dataset. The $L_{\rm Bol}$, $M_{\rm BH}$, and $λ_{\rm Edd}$ values are given for 21050 new sources with their estimated error. These results have been made publicly available. The release of this catalog will advance AGN studies by presenting key parameters of the accretion history of 6 dex in luminosity over a wide range of $z$.
description: 20 pages, 24 figures, accepted by A&A
The tidal effects on the lithium abundance of binary systems with giant component
Creators: name: Costa, J. M.
name: da Silva, L.
name: Nascimento, J. D. do
name: De Medeiros, J. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analise the behavior of lithium abundance as a function of effective temperature, projected rotational velocity, orbital period and eccentricity for a sample of 68 binary systems with giant component and orbital period ranging from about 10 to 6400 days. For these binary systems the Li abundances show a gradual decrease with temperature, paralleling the well established result for single giants. We have also observed a dependence of lithium content on rotation. Binary systems with moderate to high rotation present also moderate to high Li content. This study shows also that synchronized binary systems with giant component seems to retain more of their original lithium than the unsynchronized systems. For orbital periods lower than 100 to 250 days, typically the period of synchronization for this kind of binary systems, lithium depleted stars seems to be unusual. The suggestion is made that there is an 'inhibited zone' in which synchronized binary systems with giant component having lithium abundance lower than a threshold level should be unusual.
description: 6 pages, 3 Postscript figures, uses: aa.cls, psfig.sty
A short introduction to the Lindblad Master Equation
Creators: name: Manzano, Daniel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The theory of open quantum system is one of the most essential tools for the development of quantum technologies. Furthermore, the Lindblad (or Gorini-Kossakowski-Sudarshan-Lindblad) Master Equation plays a key role as it is the most general generator of Markovian dynamics in quantum systems. In this paper, we present this equation together with its derivation and methods of resolution. The presentation tries to be as self-contained and straightforward as possible to be useful to readers with no previous knowledge of this field.
description: Pedagogical paper, aimed to people which knowledge about quantum mechanics but not previous background about quantum master equations
Neural-network-designed three-qubit gates robust against charge noise and crosstalk in silicon
Creators: name: Kanaar, David W.
name: Kestner, J. P.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Spin qubits in semiconductor quantum dots are a promising platform for quantum computing, however scaling to large systems is hampered by crosstalk and charge noise. Crosstalk here refers to the unwanted off-resonant rotation of idle qubits during the resonant rotation of the target qubit. For a three-qubit system with crosstalk and charge noise, it is difficult to analytically create gate protocols that produce three-qubit gates, such as the Toffoli gate, directly in a single shot instead of through the composition of two-qubit gates. Therefore, we numerically optimize a physics-informed neural network to produce theoretically robust shaped pulses that generate a Toffoli-equivalent gate. Additionally, robust $\fracπ{2}$ $X$ and CZ gates are also presented in this work to create a universal set of gates robust against charge noise. The robust pulses maintain an infidelity of $10^{-3}$ for average quasistatic fluctuations in the voltage of up to a few mV instead of tenths of mV for non-robust pulses.
description: 7 pages, 7 figures
Lowest order QED radiative effects in polarized SIDIS
Creators: name: Akushevich, Igor
name: Ilyichev, Alexander
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The explicit exact analytical expressions for the lowest-order radiative corrections to the semi-inclusive deep inelastic scattering of the polarized particles are obtained in the most compact, covariant form convenient for the numerical analysis. The infrared divergence from the real photon emission is extracted and cancelled using the Bardin-Shumeiko approach. The contribution of the exclusive radiative tail is presented.The analytic results obtained within the ultrarelativistic approximation are also show.
description: 17 pages, 1 figure
Plectrocnemia alheniel Malicky 2012, nov.sp.
Creators: name: Malicky, H.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Trichoptera
Polycentropodidae
Plectrocnemia
Plectrocnemia alheniel

description: Plectrocnemia alheniel nov.sp.
Körper fahlgelb bis braun, Flügel fahlbraun mit einigen kleinen weissen Flecken, VFL 6 mm. KA (Tafel 8): 9. Segment eckig, basal mit weit nach vorne ausladendem Seitenlappen. 10. Segment kurz und breit, häutig, mit einem Paar runder Seitenlappen. OA klein, oval, schräg nach oben gerichtet. Von der Basis der OA entspringt ein Paar dünner Stäbe, die zuerst nach innen und dann nach hinten gerichtet sind und im Endteil eine gerunzelte Oberfläche haben. UA in LA rundlich, mit gerader, leicht gewellter Kaudalkante und einem spitzen Vorsprung an ihrem Vertralende und einem dicken Innenfinger. Die Form der UA in VA ist aus der Zeichnung zu entnehmen. PA gross und dick, mit einem Paar dünner spitzer Stäbe dorsal, die parallel laufen und ungefähr bis 2/3 des PA reichen. Ich kenne keine ähnliche Art.
Holotypus und 1 Paratypus: Laos, Attapeu prov., Annam Highlands, Dong Amphan NBCA, Nong Fa crater lake, 1160m, 15°05‘N, 107°25‘E, 30.4.- 6.5.2010, leg. J. Hájek, NMP.
description: Published as part of Malicky, H., 2012, Neue asiatische Köcherfliegen aus neuen Ausbeuten (Insecta, Trichoptera), pp. 1263-1310 in Linzer biologische Beiträge 44 (2) on page 1273, DOI: 10.5281/zenodo.5329501
Evidence for the evolutionary sequence of blazars: different types of accretion flows in BL Lac objects
Creators: name: Cao, Xinwu
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The limits on the mass of the black hole in 23 BL Lac objects are obtained from their luminosities of the broad emission line Hβon the assumption that broad emission lines are emitted from clouds ionized by the radiation of the accretion disk surrounding a black hole. The distribution of line luminosity L_{Hβ} of all these BL Lac objects suggests a bimodal nature, although this cannot be statistically proven on the basis of the present, rather small sample. We found that standard thin disks are probably in the sources with L_{Hβ}>10^{41} erg s^{-1}. The central black holes in these sources have masses of 10^{8-10} M_\odot, if the matter is accreting at the rate of 0.025 {\dot M}_{\rm Edd}. For the sources with L_{Hβ}<10^{41} erg s^{-1}, the accretion flows have transited from standard thin disk type to the ADAF type. The lower limits on the mass of the black hole in these sources are in the range of 1.66-24.5\times 10^{8} M_\odot. The results support the evolutionary sequence of blazars: FSRQ\to LBL\to HBL.
description: 5 pages, accepted for publication in ApJ Letters
Stenus (Hemistenus) paschtun Puthz 2008, nov.sp.
Creators: name: Puthz, V.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Staphylinidae
Stenus
Stenus paschtun

description: Stenus (Hemistenus) paschtun nov.sp.
T y p e n m a t e r i a l - Holotypus und 1 - Paratypus: Afghanistan: Umgebung Kabul, 27.V.1952, J. Klapperich; 1 - Paratypus: Tangi Saidan bei Kabul, 27.V.1952, J. Klapperich. - HT und 1 PT im NHMW, 1 PT in cP.
B e s c h r e i b u n g Makropter, schwarz mit Messingeinschlag, stark glänzend, Vorderkörper grob und dicht, Abdomen vorn grob (auf der Tergitvorderhälfte) bis fein (Tergithinterhälfte), hinten fein und weitläufig bis sehr weitläufig punktiert; Beborstung sehr auffällig, lang, glänzend, anliegend. Paraglossen oval. Fühler rötlichgelb, die Keule etwas verdunkelt. Kiefertaster gelb, das 3. Glied wenig dunkler. Beine gelblichbraun, apikale zwei Fünftel der Mittel- und der Hinterschenkel, ziemlich scharf abgesetzt, braun. Hintertarsen fast fünf Sechstel schienenlang (29: 37), ihr 1. Glied so lang wie die drei folgenden zusammengenommen, doppelt so lang wie das Klauenglied; das 4. Glied ist einfach, nicht gelappt! Clypeus schwarz, Oberlippe dunkelbraun, ziemlich dicht beborstet.
Länge: 3,6-4,6 mm (Vorderkörperlänge: 2,0- 2,1 mm).
PM des HT: HW: 37,5; FW: 18,5; PW: 26; PL: 27; EW: 38; EL: 38,5; SL: 33.
M ä n n c h e n: Beine ohne Auszeichnungen. 7. Sternit vor dem Hinterrand median feiner als an den Seiten punktiert und beborstet. 8. Sternit mit breit-dreieckiger Ausrandung etwa im hinteren Zwanzigstel. 9. Sternit apikolateral mit spitzem Zahn. 10. Tergit abgerundet. A e d o e a g u s (Abb. 40), der Medianlobus vorn nach konkavem Bogen in eine mässig breit abgerundete, häutige Spitze verengt, Ausstülpspange mit spitzen Seitenhaken, Innensack breittubig; Parameren fast so lang wie der Medianlobus, apikal mit zahlreichen langen Borsten.
W e i b c h e n: unbekannt.
 D i s k u s s i o n: Diese neue Art gehört in die Gruppe des S. glacialis Heer und stellt hier – neben S. pakistanicus PUTHZ – deren östlichsten Verteter. In ihrer Gruppe fällt sie wegen ihrer langen, glänzenden Beborstung sehr auf. Abgesehen von ihrem Aedoeagus unterscheidet sie sich von S. pakistanicus durch weniger gedrängte Stirnpunktierung, quadratische Elytren und viel feinere, viel weitläufigere Punktierung des Abdomens, von S. armeniacus PUTHZ durch viel gröbere Punktierung, vor allem des Vorderkörpers, von S. limicola KORGE durch geringere Grösse und viel dichtere Punktierung des Vorderkörpers.
E t y m o l o g i e: Um ihre Herkunft zu signalisieren, wähle ich für diese neue Art den Namen der häufigsten Volksgruppe Afghanistans.
description: Published as part of Puthz, V., 2008, Stenus LATREILLE und die segenreiche Himmelstochter (Coleoptera, Staphylinidae), pp. 137-230 in Linzer biologische Beiträge 40 (1) on page 172, DOI: 10.5281/zenodo.5426801
Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
Creators: name: Blondin, John M.
name: Mezzacappa, Anthony
name: DeMarino, Christine
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the stability of standing, spherical accretion shocks. Accretion shocks arise in core collapse supernovae (the focus of this paper), star formation, and accreting white dwarfs and neutron stars. We present a simple analytic model and use time-dependent hydrodynamics simulations to show that this solution is stable to radial perturbations. In two dimensions we show that small perturbations to a spherical shock front can lead to rapid growth of turbulence behind the shock, driven by the injection of vorticity from the now non-spherical shock. We discuss the ramifications this instability may have for the supernova mechanism.
description: 21 pages, 13 figures; to be published in The Astrophysical Journal
Multiparameter Discrete Morse Theory
Creators: name: Brouillette, Guillaume
name: Allili, Madjid
name: Kaczynski, Tomasz
Publisher: name: arXiv
Year: 2022
Subjects: subject: Geometric Topology (math.GT)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 57Q05 (Primary) 37B30, 52C99, 57Q10 (Secondary)

description: The main objective of this paper is to extend Morse-Forman theory to vector-valued functions. This is mostly motivated by the need to develop new tools and methods to compute multiparameter persistence. To generalize the theory, in addition to adapting the main definitions and results of Forman to this vectorial setting, we use concepts of combinatorial topological dynamics studied in recent years. This approach proves to be successful in the following ways. First, we establish a result which is more general than that of Forman regarding the sublevel sets of a multidimensional discrete Morse function. Second, we find a way to induce a Morse decomposition in critical components from the critical points of such a function. Finally, we deduce a set of Morse equation and inequalities specific to the multiparameter setting.
description: 39 pages, 19 figures
title: Identification, Characterisation and Expression of PRSV-P Resistance Genes in Carica and Vasconcellea
Creators: name: Mohd Razali, Razean Haireen
Publisher: name: Griffith University
Year: 2013
Subjects: subject: Papaya (Carica papaya L.)
subject: Carica
subject: Vasconcellea
subject: Papaya Ringspot Virus

description: Papaya (Carica papaya L.) is one of the major tropical fruit crops worldwide; however, commercial and local production is reduced by several diseases and pests. Papaya Ringspot Virus type P (PRSV-P) is a serious disease of Carica papaya, and all known varieties of papaya are susceptible. Vasconcellea parviflora is a PRSV-P susceptible species. Researchers have identified PRSV-P resistant genes in Vasconcellea spp., which were formerly included in the genus Carica. Of the 21 Vasconcellea species, only one, Vasconcellea pubescens sometimes called Vasconcellea cundinamarcensis, has been consistently reported worldwide to be resistant or immune to PRSV-P for more than 60 years.
High-resolution radio observations of Seyfert galaxies in the extended 12-micron sample - II. The properties of compact radio components
Creators: name: Thean, Andy
name: Pedlar, Alan
name: Kukula, Marek J.
name: Baum, Stefi A.
name: O'Dea, Christopher P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the properties of compact nuclear radio components in Seyfert galaxies from the extended 12-micron AGN sample of Rush et al.(1993). Our main results can be summarised as follows. Type 1 and type 2 Seyferts produce compact radio components which are indistinguishable in strength and aspect, indicating that their central engines are alike as proposed by the unification model. Infrared IRAS fluxes are more closely correlated with low-resolution radio fluxes than high-resolution radio fluxes, suggesting that they are dominated by kiloparsec-scale, extra-nuclear emission regions; extra-nuclear emission may be stronger in type 2 Seyferts. Early-type Seyfert galaxies tend to have stronger nuclear radio emission than late-type Seyfert galaxies. V-shaped extended emission-line regions, indicative of `ionisation cones', are usually found in sources with large, collimated radio outflows. Hidden broad lines are most likely to be found in sources with powerful nuclear radio sources. Type 1 and type 2 Seyferts selected by their IRAS 12-micron flux densities have well matched properties.
Additional file 3 of Mitophagy promotes sorafenib resistance through hypoxia-inducible ATAD3A dependent Axis
Creators: name: Wu, Hong
name: Wang, Tao
name: Liu, Yiqiang
name: Li, Xin
name: Xu, Senlin
name: Wu, Changtao
name: Zou, Hongbo
name: Cao, Mianfu
name: Jin, Guoxiang
name: Lang, Jinyi
name: Wang, Bin
name: Liu, Baohua
name: Luo, Xiaolin
name: Xu, Chuan
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 3. Sequences of the primers used for qRT-PCR.
Additional file 1: of Digital recording and documentation of endoscopic procedures: physiciansâ practice and perspectives
Creators: name: Peled-Raz, Maya
name: Willner, Nadav
name: Shteinberg, Dan
name: Or-Chen, Keren
name: Rainis, Tova
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Table S1. Study population - demographic data.Table S2. Differences in rankings of supporting DRD of endoscopic procedures, based on demographic data.Table S3. Model I - Non-significant mediation.Table S4. Model II - Non-significant mediation (DOCX 29 kb)
Moderate Temperature Clusters of Galaxies from the RDCS and the High Redshift Luminosity-Temperature Relation
Creators: name: Holden, B. P.
name: Stanford, S. A.
name: Squires, G. K.
name: Rosati, P.
name: Tozzi, P.
name: Eisenhardt, P.
name: Spinrad, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present our discovery observations and analysis of RDCS1317+2911, z = 0.805, and RDCS1350+6007, z= 0.804, two clusters of galaxies identified through X-ray emission in the ROSAT Deep Cluster Survey (RDCS). We find a temperature of 3.7 +1.5 -0.9 keV and a bolometric luminosity of 8.2e43 +1.7e43 -1.6e43 erg/s for RDCS1317+2911, and a temperature of 4.9 +1.3 -0.9 keV and a bolometric luminosity of 4.1e44 +0.5e44 -0.4e44 erg/s for RDCS1350+6007. Our weak lensing analysis of RDCS1350+6007 confirms the general shape of the inner density profile but predicts twice the mass of the model based on the X-ray profile. We combine the X-ray luminosities and temperatures for RDCS clusters of galaxies with such measurements of other clusters at high redshift (z>0.7) and fit the luminosity-temperature relation. We find no statistically significant evolution in the slope or zero-point of this relation at a median of z=0.83. This result is in agreement with models of intracluster medium evolution with significant pre-heating or high initial entropy values. We discuss how low temperature, high redshift clusters of galaxies will allow us to improve on this result and announce the discovery of two such objects, CXOU J0910.1+5419 and CXOU J1316.9+2914.
description: 33 pages, Latex 2e using the AASTEX v5 macros, with 13 figures. Figures number one and six are color jpegs. Abstract abridged. Error in Table 1 corrected
MOESM1 of Economic burden of diabetes in Brazil in 2014
Creators: name: Bahia, Luciana
name: Rosa, Michelle
name: Denizar Araujo
name: Correia, Marcelo
name: Rosa, Roger
name: Duncan, Bruce
name: Toscano, Cristiana
Publisher: name: figshare
Year: 2019
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Marine Biology
subject: Science Policy

description: Additional file 1: Table S1. State level diabetes prevalence and population estimates in adults (20+ years). SUS. Brazil. 2014. Table S2. DM and related conditions and relative risks.
Stellar population gradients in Seyfert 2 galaxies. Northern sample
Creators: name: Raimann, D.
name: Storchi-Bergmann, T.
name: Delgado, R. M. Gonzalez
name: Fernandes, R. Cid
name: Heckman, T.
name: Leitherer, C.
name: Schmitt, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use high signal-to-noise ratio long-slit spectra in the 3600-4700A range of the twenty brightest northern Seyfert 2 galaxies to study the variation of the stellar population properties as a function of distance from the nucleus. In order to characterize the stellar population and other continuum sources (e.g. featureless continuum FC) we have measured equivalent widths Ws of six absorption features, four continuum colours and their radial variations, and performed spectral population synthesis as a function of distance from the nucleus. About half the sample has CaIIK and G-band W values smaller at the nucleus than at 1 kpc from it, due to a younger population and/or FC. The stellar population synthesis shows that, while at the nucleus, 75% of the galaxies present contribution > 20% of ages younger or equal than 100Myr and/or of a FC, this proportion decreases to 45% at 3 kpc. In particular, 55% of the galaxies have contribution > 10% of the 3 Myr/FC component (a degenerate component in which one cannot separate what is due to a FC or to a 3 Myr stellar population) at the nucleus, but only 25% of them have this contribution at 3 kpc. As reference, the stellar population of 10 non-Seyfert galaxies, spanning the Hubble types of the Seyfert (from S0 to Sc) was also studied. A comparison between the stellar population of the Seyferts and that of the non-Seyferts shows systematic differences: the contribution of ages younger than 1 Gyr is in most cases larger in the Seyfert galaxies than in non-Seyferts, not only at the nucleus but up to 1 kpc from it.
description: 23 pages, 18 figures, MNRAS in press
Decadal climate variability: mechanisms and impacts
Creators: name: Gastineau, Guillaume
Publisher: name: Zenodo
Year: 2019

description: HDR thesis defense. Paris, January 18th 2019. Jury: P. Bouruet-Aubertot, M. Kageyama, R. Sutton, M. Déqué, G. Rivière, D. Swingedouw
Additional file 1: of Africaâ s challenged ENT services: highlighting challenges in Zambia
Creators: name: Lufunda Lukama
name: Kalinda, Chester
name: Aldous, Colleen
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Data collection tool. Hospital Respondents Questionnaire. Includes Respondents information, written consent and description of terms. (DOC 465 kb)