cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 6 of Transcriptomic analysis of α-linolenic acid content and biosynthesis in Paeonia ostii fruits and seeds
Creators: name: Yu, Shui-Yan
name: Zhang, Xiao
name: Huang, Liang-Bo
name: Lyu, Yu-Ping
name: Zhang, Ying
name: Yao, Zu-Jie
name: Zhang, Xiao-Xiao
name: Yuan, Jun-Hui
name: Hu, Yong-Hong
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 6: Figure S4. GO classification of differentially expressed genes. The number of DEGs is plotted along the x-axis; the GO terms is plotted along the y-axis. a T1 vs. T2 in the kernel. b T1 vs. T2 in the testa. c T1 vs. T2 in the pericarp.
title: The selective hydrogenation of alkynyl-substituted aromatic molecules over rhodium/silica
Creators: name: Gregory, Joseph William
Publisher: name: University of Glasgow
Year: 2019
Subjects: subject: alkynylaromatic, unsaturated, rhodium, rhodium/silica, hydrogenation, phenylacetylene, 1-phenyl-1-propyne, styrene, ethylbenzene, ethylcyclohexane, methylstyrene, propylbenzene, propylcyclohexane, competitive.

description: Kinetic studies involving phenylacetylene and 1-phenyl-1-propyne hydrogenation cascades over 2.5% w/w rhodium/silica were carried out to assess aspects of selectivity and catalytic behaviour. The reactions were performed over the temperature range 313 K – 343 K in the liquid phase using 2-propanol (IPA) as a solvent. Typically 0.1g of catalyst was used with 3 barg hydrogen pressure and 10 mmol of aromatic in a stirred tank reactor. Rate constants and activation energies for phenylacetylene, ethylbenzene, 1-phenyl-1-propyne and propylbenzene hydrogenation were calculated and, for molecules with analogous functionality, were found to increase with a decrease in the mass of the substituent. For the hydrogenation of 1-phenyl-1-propyne, the cis/trans ratio of β-methylstyrene was calculated and a kinetic isotope effect observed. The cis/trans ratio was typically at its greatest in the initial stages of the reaction and decreased with time. Increasing the temperature increased the cis/trans ratio, however this trend was reversed at higher temperatures, suggesting that there was a change in reaction pathway and meaning that the nature of the reaction was temperature-dependent. Competitive hydrogenation was carried out which showed that, in some instances, aromatic molecules with larger substituents can completely outcompete molecules with smaller substituents. This effect was reflected in an increased selectivity for alkylarenes with shorter-chain substituents when related alkylarenes with longer-chain substituents were present, for example the presence of propylbenzene in a reaction mixture improved ethylbenzene selectivity. Styrene selectivity during the hydrogenation cascade of phenylacetylene was monitored and found to be largely unaffected by altering the temperature and by changing the reactive hydrogen isotope, however an enhancement was made possible by competition with ethylbenzene and 1-phenyl-1-propyne. The majority of unsaturated functional groups assessed in this study appeared to undergo hydrogenation at the same active site of the catalyst, however kinetic results suggested the terminal alkyne group of phenylacetylene reacted at a different site. These kinetic results also provided evidence that subsurface hydrogen was the active hydrogen species in some of the hydrogenation processes observed. The findings of this study have further developed our understanding of the hydrogenation of alkynylaromatics.
On hyperspaces of knots and planar simple closed curves
Creators: name: Krupski, Paweł
name: Omiljanowski, Krzysztof
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Topology (math.GN)
subject: FOS: Mathematics
subject: 57K10 (Primary) 54B20, 54F45, 54H05 (Secondary)

description: We consider the Vietoris hyperspaces $\mathcal S(\mathbb R^n)$ of simple closed curves in $\mathbb R^n$, $n=2,3$, and their subspaces $\mathcal S_P(\mathbb R^2)$ of planar simple closed polygons, $\mathcal K_P$ of polygonal knots, and $\mathcal K_T$ of tame knots. We prove that all the hyperspaces are strongly locally contractible, arcwise connected, infinite-dimensional Cantor manifolds, and $\mathcal S(\mathbb R^2)$ and $\mathcal K_T$ are strongly infinite-dimensional Cantor manifolds. Moreover, $\mathcal S_P(\mathbb R^2)$ and $\mathcal K_P$ are $σ$-compact, strongly countable-dimensional absolute neighborhood retracts.
Hyperfine structure of S-states in muonic ions of lithium, beryllium and boron
Creators: name: Dorokhov, A. E.
name: Krutov, A. A.
name: Martynenko, A. P.
name: Martynenko, F. A.
name: Sukhorukova, O. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We make precise calculation of hyperfine structure of $S$-states in muonic ions of lithium, beryllium and boron in quantum electrodynamics. Corrections of orders $α^5$ and $α^6$ due to the vacuum polarization, nuclear structure and recoil in first and second orders of perturbation theory are taken into account. We obtain estimates of the total values of hyperfine splittings which can be used for a comparison with future experimental data.
description: 22 pages, 8 figures
Pheidole Aeberlii Forel, 1894, n. spec.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1894
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole

description: Pheidole Aeberlii, n. spec.
[[soldier]]. Lg. 6 mm. Kopf fast oval, etwas laenger als breit, mit stark convexen Seiten, hinten und vorne verengt, hinten tief und eng eingeschnitten. Mandibeln glaenzend mit stark gestreifter Basalhaelfte. Clypeus gekielt, vorne in der Mitte nur schwach ausgerandet. Stirnrinne bis zum Hinterhaupteinschnitt fortgesetzt. Stirnleisten kurz; keine Rinne fuer den Schaft. Derselbe reicht kaum ueber die Mitte der Entfernung vom Fuehlergelenk zur Hinterhauptsecke. Augen vor dem vorderen Drittel. Pronotum ohne deutliche Hoecker. Mesonotum mit einem Querwulst. Basalflaeche des Metanotum mit, einer mittleren Laengsrinne und zwei schmalen, ziemlich kurzen, an der Spitze, ganz stumpf gerundeten Dornen, die etwa 2 / 3 so lang sind wie ihr Zwischenraum. Basalflaeche so lang wie die abschuessige. Erstes Stielchenglied lang gestielt, mit oben scharfrandigem, nicht ausgerandetem Knoten. Zweites Glied so lang als breit, seitlich gerundet.
Kopf grob laengsgestreift, dazwischen fein genetzt; der hintere Viertel glatt und glaenzend. Pronotum und Metanotum quergerunzelt; Thoraxseiten laengsgerunzelt; Mesonotum theilweise glatt. Zweites Stielchenglied und Basis des Abdomens sehr dicht und fein laengsgestreift und dazwischen punktirt-genetzt. Der Rest glatt und glaenzend. Koerper massig und fein, gelblich abstehend, Schienen und Schaefte nur sehr schief, fast ganz anliegend behaart.
Roetblichbraun (gelblichbraeunlich, weil noch nicht ausgefaerbt); Abdomen, Schaefte und Schenkel dunkelbraun.
[[worker]]. Lg. 3,2 — 3,3 mm. Kopf hinter den Augen ziemlich stark verengt, doch durchaus nicht halsartig. Mesonotum mit einem Quereindruck. Metanotum mit zwei Doernchen. Stielchenglieder eng und laenglich. Fuehler und Beine lang, schief abstehend behaart. Stirnleisten sehr lang und parallel, reichen bis zur Hoehe der Mitte des Auges.
Glatt und glaenzend; Thorax, mit Ausnahme der Pronotumscheibe, fein punktirt-genetzt und matt. Wangen gerunzelt.
Braun; Thorax roethlichbraun; Fuehler, Mandibeln und Beine gelblichbraun.
[[male]] Lg. 5,2 — 5,4 mm. Gelblichbraun; Kopf und Abdomen dunkler braun. Fuehler und Beine blassgelblich. Kopf matt, punktirt-genetzt und groeber gerunzelt. Mesonotum schimmernd, genetzt und laengsgerunzelt. Metanotum mit zwei Beulen. Fluegel - ziemlich hell, mit gelben Adern und Randmal.
Oberer Senegal, durch Herrn Emil Aeberli aus Zuerich erhalten.
description: Published as part of Forel, A., 1894, Abessinische und andere afrikanische Ameisen, gesammelt von Herrn Ingenieur Alfred Ilg, von Herrn Dr. Liengme, von Herrn Pfarrer Missionar P. Berthoud, Herrn Dr. Arth. Müller, etc., pp. 64-100 in Mitteilungen der Schweizerischen Entomologischen Gesellschaft 9 on pages 91-92, DOI: 10.5281/zenodo.14259
Fig. A.4. Two parallel magmatic belts with contrasting isotopic characteristics from southern Tibet to Myanmar: Zircon U–Pb and Hf isotopic constraints
Creators: name: Te-Hsien Lin
name: A.H.G. Mitchell
name: Sun-Lin Chung
name: Tan, Xi-Bin
name: Jui-Ting Tang
name: Thura Oo
name: Wu, Fu-Yuan
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. A.4. U–Pb concordia diagrams of magmatic zircons of the studied samples from the Popa–Loimye Arc.
Effect of finite disk-thickness on swing amplification of non-axisymmetric perturbations in a sheared galactic disk
Creators: name: Ghosh, Soumavo
name: Jog, Chanda J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A typical galactic disk is observed to have a finite thickness. Here, we present the study of the physical effect of introduction of finite thickness on the generation of small-scale spiral arms by swing amplification in a differentially rotating galactic disk. The galactic disk is modelled first as a one-fluid system, and then as a gravitationally-coupled two-fluid (stars and gas) system where each fluid is taken as isothermal, and corotating with each other. We derived the equations governing the evolution of growth of the non-axisymmetric perturbations in a sheared frame of reference while incorporating the effect of finite thickness of a galactic disk. We found that the finite thickness of a galactic disk has a generic trend of suppressing the growth of the non-axisymmetric perturbations via swing amplification. Moreover, even the observed range of disk-thickness values (~ 300-500 pc) can lead to a complete suppression of swing amplification for Q ~ 1.7, whereas for an infinitesimally-thin disk, the corresponding critical value is Q ~ 2. For a two-fluid (stars and gas) system, the net amplification is shown to be set by the mutual interplay of the effect of interstellar gas in promoting the spiral features and the effect of finite thickness in preventing the spiral arms. The coexistence of these two opposite effects is shown to be capable of giving rise to diverse and complex dynamical behaviour.
description: 13 pages, 8 figures, accepted for publication in A&A
One-dimensional model potentials optimized for the calculation of the HHG spectrum
Creators: name: Sallai, Krisztina
name: Hack, Szabolcs
name: Majorosi, Szilárd
name: Czirják, Attila
Publisher: name: arXiv
Year: 2024
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Based on the favourable properties of previously used one-dimensional (1D) atomic model potentials, we introduce a novel 1D atomic model potential for the 1D simulation of the quantum dynamics of a single active electron atom driven by a strong, linearly polarized near-infrared laser pulse. By comparing numerical simulation results of typical strong-field physics scenarios in 1D and 3D, we show that this novel 1D model potential gives single atom HHG spectra with impressively increased accuracy for the most frequently used driving laser pulse parameters.
Neutrino Oscillations v.s. Leptogenesis in SO(10) Models
Creators: name: Nezri, Emmanuel
name: Orloff, Jean
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the link between neutrino oscillations and leptogenesis in the minimal framework assuming an SO(10) see-saw mechanism with 3 families. Dirac neutrino masses being fixed, the solar and atmospheric data then generically induce a large mass-hierarchy and a small mixing between the lightest right-handed neutrinos, which fails to produce sufficient lepton asymmetry by 5 orders of magnitudes at least. This failure can be attenuated for a very specific value of the mixing sin^2(2θ_{e3})=0.1, which interestingly lies at the boundary of the CHOOZ exclusion region, but will be accessible to future long baseline experiments.
description: 23 pages, 8 eps figures, JHEP3 format; more accurate effect of dilution reduces previous results, inclusion of all phases, added references
Pheidole liengmei Forel, 1894, n. spec.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1894
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole
Pheidole liengmei

description: Pheidole Liengmei, n. spec.
[[worker]]. Lg. 3,7 — 4 mm. Der Ph. longispinosa For. r. scabrata aus Madagascar sehr nahestehend, aber der Clypeus ist scharf laengsgekielt. Kopf viereckig, schwach gerundet, etwas breiter als lang, mit geradem Hinterrand; die Augen stehen etwas vor der Mitte der Kopfraender; der Fuehlerschaft ueberragt nur sehr wenig den Hinterkopf; die viel schmaeleren Mandibeln sind grob laengsgestreift und zerstreut punktirt. Das Metanotum ist etwas kuerzer und breiter; die Basalflaeche von einer schwachen Leiste gerandet. Die Dornen sind an der Basis kraeftiger, aber etwas kuerzer als die Basalflaeche und nur wenig laenger als die Breite der Basalflaeche; sie sind auch etwas mehr nach hinten gerichtet. Erstes Stielchenglied ebenfalls sehr lang gestielt, aber oben etwas ausgerandet und au den Vorderecken weniger erweitert. Zweites Stielchenglied viel kleiner, etwas breiter als lang, mit zwei kurzen, kleinen seitlichen Kegeln. Schenkel in der Mitte weniger verdickt. Pronotumhoecker etwas hoeher und mehr vorspringend.
Hinterleib vorne dicht genetzt und schwach glaenzend, hinten, sowie die Beine, glatt und glaenzend. Der ganze uebrige Koerper dicht punktirt-genetzt und matt, mit lockeren, groeberen Laengsrunzeln auf dem Kopf und dem Thorax.
Koerper sparsam und fein abstehend, Schaefte und Schienen nur lang und nicht ganz angepresst anliegend gelblich behaart. Am Koerper fast keine anliegenden Haare.
Roethlichbraun; Abdomen mehr kastanienbraun.
Delagoa (Dr. Liengme). Durch die Sculptur, die Groesse und die langen, starken Metanotumdornen von allen anderen afrikanischen Arten leicht zu unterscheiden. Ein [[soldier]], den ich zuerst zu diesen [[worker]] stellen zu koennen glaubte, gehoert, wie mir mein Freund; Prof. Emery, versichert, zu der folgenden Art, die er beschreiben wird.
description: Published as part of Forel, A., 1894, Abessinische und andere afrikanische Ameisen, gesammelt von Herrn Ingenieur Alfred Ilg, von Herrn Dr. Liengme, von Herrn Pfarrer Missionar P. Berthoud, Herrn Dr. Arth. Müller, etc., pp. 64-100 in Mitteilungen der Schweizerischen Entomologischen Gesellschaft 9 on pages 93-94, DOI: 10.5281/zenodo.14259
Neural State Classification for Hybrid Systems
Creators: name: Phan, Dung
name: Paoletti, Nicola
name: Zhang, Timothy
name: Grosu, Radu
name: Smolka, Scott A.
name: Stoller, Scott D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: We introduce the State Classification Problem (SCP) for hybrid systems, and present Neural State Classification (NSC) as an efficient solution technique. SCP generalizes the model checking problem as it entails classifying each state $s$ of a hybrid automaton as either positive or negative, depending on whether or not $s$ satisfies a given time-bounded reachability specification. This is an interesting problem in its own right, which NSC solves using machine-learning techniques, Deep Neural Networks in particular. State classifiers produced by NSC tend to be very efficient (run in constant time and space), but may be subject to classification errors. To quantify and mitigate such errors, our approach comprises: i) techniques for certifying, with statistical guarantees, that an NSC classifier meets given accuracy levels; ii) tuning techniques, including a novel technique based on adversarial sampling, that can virtually eliminate false negatives (positive states classified as negative), thereby making the classifier more conservative. We have applied NSC to six nonlinear hybrid system benchmarks, achieving an accuracy of 99.25% to 99.98%, and a false-negative rate of 0.0033 to 0, which we further reduced to 0.0015 to 0 after tuning the classifier. We believe that this level of accuracy is acceptable in many practical applications, and that these results demonstrate the promise of the NSC approach.
description: ATVA2018 extended version
Pheidole crassinoda Emery
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1894
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole
Pheidole crassinoda

description: Pheidole crassinoda Emery i. litt.
Delagoa (Dr. Liengme).
description: Published as part of Forel, A., 1894, Abessinische und andere afrikanische Ameisen, gesammelt von Herrn Ingenieur Alfred Ilg, von Herrn Dr. Liengme, von Herrn Pfarrer Missionar P. Berthoud, Herrn Dr. Arth. Müller, etc., pp. 64-100 in Mitteilungen der Schweizerischen Entomologischen Gesellschaft 9 on page 94, DOI: 10.5281/zenodo.14259
Motivations of Educators for Participating in NITARP, an Authentic Astronomy Research Experience Professional Development Program
Creators: name: Rebull, L. M.
name: Roberts, T.
name: Laurence, W.
name: Fitzgerald, M.
name: French, D.
name: Gorjian, V.
name: Squires, G. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics Education (physics.ed-ph)
subject: FOS: Physical sciences

description: The NASA/IPAC Teacher Archive Research Program (NITARP) partners small groups of educators with a research astronomer for a year-long authentic research project. This program aligns well with the characteristics of high-quality professional development (PD) programs and has worked with a total of 103 educators since 2005. In this paper, surveys were explored that were obtained from 74 different educators, at up to four waypoints during the course of 13 months, incorporating data from the class of 2010 through the class of 2017. This paper investigates how participating teachers describe their motivations for participating in NITARP as evidenced in these feedback forms. Analysis of self-reported data allows a mapping onto a continuum ranging from more inward-focused to more outward-focused; there is a shift from more inward-focused responses to more outward-focused responses. This insight into teacher motivations has implications for how the educators might be supported during their year with the program. This work provides a new way of parameterizing why educators participate in PD programs that require a considerable investment of time. NITARP, since it has many qualities of successful PD, serves as a model for similar PD programs in other STEM subjects. Likewise, the analysis method might also be useful to similarly evaluate other PD programs.
description: Accepted by PRPER for the Focused Collection on Astronomy Education Research
Universal collective Larmor-Silin mode emerging in magnetized correlated Dirac fermions
Creators: name: Chen, Chuang
name: Da Liao, Yuan
name: Zhou, Chengkang
name: Pan, Gaopei
name: Meng, Zi Yang
name: Qi, Yang
Publisher: name: arXiv
Year: 2024
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Employing large-scale quantum Monte Carlo simulations, we find that in the magnetized interacting Dirac fermion model there emerges a universal collective Larmor-Silin spin wave mode in the transverse dynamical spin susceptibility. Such mode purely originates from the interaction among Dirac fermions and distinguishes itself from the usual particle-hole continuum with finite lifetime and clear dispersion, both at small and large momenta in a large portion of the Brillouin zone. Our unbiased numerical results offer the dynamic signature of this collective excitation in interacting Dirac fermion systems, and provide experimental guidance for inelastic neutron scattering, electron spin resonance, and other spectroscopic approaches in the investigation of such universal collective modes in quantum Moire materials, topological insulators, and quantum spin liquid materials under magnetic field, with quintessential interaction nature beyond the commonly assumed noninteracting Dirac fermion or spinon approximations.
description: 12 pages, 6 figures
Fig. A.5. Two parallel magmatic belts with contrasting isotopic characteristics from southern Tibet to Myanmar: Zircon U–Pb and Hf isotopic constraints
Creators: name: Te-Hsien Lin
name: A.H.G. Mitchell
name: Sun-Lin Chung
name: Tan, Xi-Bin
name: Jui-Ting Tang
name: Thura Oo
name: Wu, Fu-Yuan
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. A.5. Plots of εNd (T) values vs. initial Sr isotope ratios for the samples from Myanmar. For comparison, the data of the Tengchong block from Liu et al. (2009), Monywa and Popa volcanos from Yang (2008), and the eastern Transhimalayan batholith, SE Tibet from Lin et al. (2012) are also shown.
Measuring the spectral running from cosmic microwave background and primordial black holes
Creators: name: Li, Jun
name: Huang, Qing-Guo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We constrain the spectral running by combining cosmic microwave background (CMB) data, baryon acoustic oscillation (BAO) data and the constraint from primordial black holes (PBHs). We find that the constraint from PBHs has a significant impact on the running of running of scalar spectral index, and a power-law scalar power spectrum without running is consistent with observational data once the constraint from PBHs is taken into account. In addition, from the constraints on the slow-roll parameters, the derived tensor spectral index in the single-field slow-roll inflation model is quite small, namely $|n_t|\lesssim 9.3\times 10^{-3}$ which will be very difficult to be measured by CMB data only in the future, and the absolute value of derived running of tensor spectral index is not larger than $2.1\times 10^{-4}$ at 95% confidence level.
description: 5 pages, 3 figures
Greybody factor for the BTZ black hole and a 5D black hole
Creators: name: Lee, H. W.
name: Myung, Y. S.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the 5D black holes in the type IIB superstring theory compactified on $S^1 \times T^4$. Far from horizon, we have flat space-time. Near horizon, we have $AdS_3(BTZ black hole) \times S^3 \times T^4$. We calculate the greybody factor of a minimally coupled scalar by replacing the original geometry($M_5 \times S^1 \times T^4$) by $AdS_3 \times S^3 \times T^4$. In the low-energy scattering, it turns out that the result agrees with the greybody factor of the 5D black hole (or D1 + D5 branes)in the dilute gas approximation. This confirms that the $AdS$-theory($AdS_3 \times S^3 \times T^4$) contains the essential information about the bulk 5D black holes.
description: some discussions are added, 15 Pages, No figure, RevTeX
Quantum Circuit Reconstruction from Power Side-Channel Attacks on Quantum Computer Controllers
Creators: name: Erata, Ferhat
name: Xu, Chuanqi
name: Piskac, Ruzica
name: Szefer, Jakub
Publisher: name: arXiv
Year: 2024
Subjects: subject: Cryptography and Security (cs.CR)
subject: Emerging Technologies (cs.ET)
subject: FOS: Computer and information sciences

description: The interest in quantum computing has grown rapidly in recent years, and with it grows the importance of securing quantum circuits. A novel type of threat to quantum circuits that dedicated attackers could launch are power trace attacks. To address this threat, this paper presents first formalization and demonstration of using power traces to unlock and steal quantum circuit secrets. With access to power traces, attackers can recover information about the control pulses sent to quantum computers. From the control pulses, the gate level description of the circuits, and eventually the secret algorithms can be reverse engineered. This work demonstrates how and what information could be recovered. This work uses algebraic reconstruction from power traces to realize two new types of single trace attacks: per-channel and total power attacks. The former attack relies on per-channel measurements to perform a brute-force attack to reconstruct the quantum circuits. The latter attack performs a single-trace attack using Mixed-Integer Linear Programming optimization. Through the use of algebraic reconstruction, this work demonstrates that quantum circuit secrets can be stolen with high accuracy. Evaluation on 32 real benchmark quantum circuits shows that our technique is highly effective at reconstructing quantum circuits. The findings not only show the veracity of the potential attacks, but also the need to develop new means to protect quantum circuits from power trace attacks. Throughout this work real control pulse information from real quantum computers is used to demonstrate potential attacks based on simulation of collection of power traces.
description: IACR Transactions on Cryptographic Hardware and Embedded Systems, 2024(2), 735-768
Spectral analysis of SXP59.0 during its 2017 outburst and properties of the soft excess in X-ray binary pulsars
Creators: name: La Palombara, N.
name: Esposito, P.
name: Pintore, F.
name: Sidoli, L.
name: Mereghetti, S.
name: Tiengo, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report the results provided by the XMM-Newton observation of the X-ray binary pulsar SXP59.0 during its most recent outburst in April 2017. The source was detected at $f_{\rm X}$(0.2-12 keV) = 8$\times 10^{-11}$ erg cm$^{-2}$ s$^{-1}$, one of its highest flux levels reported to date. The measured pulse period was $P_{\rm spin}$ = 58.949(1) s, very similar to the periods measured in most of the previous observations. The pulsed emission was clearly detected over the whole energy range between 0.2 and 12 keV, but the pulse profile is energy dependent and the pulsed fraction increases as the energy increases. Although the time-averaged EPIC spectrum is dominated by a power-law component (with photon index $Γ= 0.76 \pm 0.01$), the data show an evident soft excess, which can be described with the sum of a black-body and a hot thermal plasma component (with temperatures $kT_{\rm BB} = 171^{+11}_{-14}$ eV and $kT_{\rm APEC} = 1.09^{+0.16}_{-0.09}$ keV, respectively). Moreover, the EPIC and RGS spectra show narrow emission lines due to N, O, Ne, Mg, and Fe. The phase-resolved spectral analysis of the EPIC data shows that the flux of the black-body component varies with the pulse phase, while the plasma component is almost constant. We show that the black-body component can be attributed to the reprocessing of the primary emission by the optically thick material at the inner edge of the accretion disc, while the hot plasma component is due to a diffuse gas far from the accretion region and the narrow emission lines of the RGS spectrum are most probably due to photoionized matter around the accreting source.
description: 11 pages, 9 figures, 5 tables. Accepted for publication by Astronomy and Astrophysics
Fig. A.2. Two parallel magmatic belts with contrasting isotopic characteristics from southern Tibet to Myanmar: Zircon U–Pb and Hf isotopic constraints
Creators: name: Te-Hsien Lin
name: A.H.G. Mitchell
name: Sun-Lin Chung
name: Tan, Xi-Bin
name: Jui-Ting Tang
name: Thura Oo
name: Wu, Fu-Yuan
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. A.2. U–Pb concordia diagrams of magmatic zircons of the studied samples from the east part of the Dianxi Batholith in China.
Additional file 7 of Transcriptomic analysis of α-linolenic acid content and biosynthesis in Paeonia ostii fruits and seeds
Creators: name: Yu, Shui-Yan
name: Zhang, Xiao
name: Huang, Liang-Bo
name: Lyu, Yu-Ping
name: Zhang, Ying
name: Yao, Zu-Jie
name: Zhang, Xiao-Xiao
name: Yuan, Jun-Hui
name: Hu, Yong-Hong
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Plant Biology

description: Additional file 7: Figure S5. KEGG pathways enriched in the genes differentially expressed in the developing kernel at various time points. The enrichment factor is plotted on the x-axis; pathway names are shown on the y-axis. The color of each dot reflects the Qvalue, while the size of the dot represents the number of DEGs. a T1 vs. T3. b T1 vs. T4. c T1 vs. T5. d T1 vs. T6.
Pheidole mayri Forel, 1894, n. spec.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1894
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole
Pheidole mayri

description: Pheidole Mayri, n. spec.
[[soldier]]. Lg. 4,4 — 4,8 mm. Mandibeln und Clypeus wie bei der vorigen. Kopf nur wenig oder kaum laenger als breit, breiter hinten als vorne, hinten breit und tief eingeschnitten, etwa wie bei rhombinoda, der diese Art sehr aehnlich sieht. Die stark divergirenden Stirnleisten setzen sich bis zum hinteren Drittel des Kopfes fort und lassen nach aussen eine Rinne fuer den Fuehlerschaft, der ebenfalls den hinteren Drittel des Kopfes erreicht. In allen Theilen der Ph. rhombinoda gleich, auch bezueglich Sculptur, Farbe und Behaarung, aber das Metanotum hat zwei ziemlich lange, duenne Dornen, die 2 / 3 so lang als ihr Zwischenraum und etwas nach innen gebogen sind. Das erste Stielchenglied ist aeusserst kurz, breiter als lang (laenger als breit bei rhombinoda), vorne mit stumpfen Ecken (scharfen bei rhombinoda), unten vorne mit einem langen lamellenartigen, etwas durchscheinenden Zahn (ohne Zahn und sehr duenn bei rhombinoda). Zweites Stielchenglied wie bei rhombinoda geformt, sehr breit und gerundet, mit durchsichtigem hinteren Theil des Seitenrandes, aber viel breiter als lang und unten mit einem Zaehnchen (kaum breiter als lang und ohne Zahn unten bei rhombinoda). Basalhaelfte des ersten Hinterleibssegmentes wenig glaenzend, fein genetzt und weitlaeufig laengsgestreift.
[[worker]]. Lg. 2,5 — 2,7 mm. Etwas gedrungener als rhombinoda. Kopf mit deutlicherem Hinterrand (mehr gerundet bei rhombinoda): Metanodum ganz unbewehrt (mit zwei spitzen Zaehnen bei rhombinoda). Sonst gleich, namentlich auch das grosse zweite Stielchenglied.
Aus einer aus Senegal stammenden Passiflorenfrucht entnommen, worin eine Masse [[soldier]] und [[worker]] lebendig mit ihren Larven enthalten waren. Die Frucht war soeben aus Senegal in Paris angekommen, als ich daselbst war und mir die Ameisen lebendig von Herrn J. Kuenckel gegeben wurden: Die Aehnlichkeit und Verwandtschaft mit der indischen Form ist so auffallend, dass ich die Frage aufwerfen muss, ob es nicht eine indische Art ist, die im Dampfschiff eingenistet war und dortselbst erst in die Passiflorafrucht Einzug hielt.
description: Published as part of Forel, A., 1894, Abessinische und andere afrikanische Ameisen, gesammelt von Herrn Ingenieur Alfred Ilg, von Herrn Dr. Liengme, von Herrn Pfarrer Missionar P. Berthoud, Herrn Dr. Arth. Müller, etc., pp. 64-100 in Mitteilungen der Schweizerischen Entomologischen Gesellschaft 9 on page 91, DOI: 10.5281/zenodo.14259
Monomorium venustum Smith
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1894
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Monomorium
Monomorium venustum

description: Monomorium venustum Smith.
Suebabessinien (Hg).
description: Published as part of Forel, A., 1894, Abessinische und andere afrikanische Ameisen, gesammelt von Herrn Ingenieur Alfred Ilg, von Herrn Dr. Liengme, von Herrn Pfarrer Missionar P. Berthoud, Herrn Dr. Arth. Müller, etc., pp. 64-100 in Mitteilungen der Schweizerischen Entomologischen Gesellschaft 9 on page 88, DOI: 10.5281/zenodo.14259
Galaxies at z=4 and the Formation of Population II
Creators: name: Trager, S. C.
name: Faber, S. M.
name: Dressler, A.
name: Oemler, A.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of four high-redshift objects (3.3 < z < 4) observed behind the rich cluster CL0939+4713 (Abell 851). One object (DG 433) has a redshift of z=3.3453; the other three objects have redshifts of z\approx 4: A0 at z=3.9819, DG 353 and P1/P2 at z=3.9822. It is possible that all four objects are being lensed in some way by the cluster, DG 433 being weakly sheared, A0 being strongly sheared, and DG 353 and P1/P2 being an image pair of a common source object; detailed modelling of the cluster potential will be necessary to confirm this hypothesis. The weakness of common stellar wind features like N V and especially C IV in the spectra of these objects argues for sub-solar metallicities, at least as low as the SMC. DG 353 and DG 433, which have ground-based colors, are moderately dusty [E_{int}(B-V) < 0.15], similar to other z>3 galaxies. Star formation rates range from 2.5 (7.8) h^{-2} to 22. (78.) h^{-2} M_{\odot}/yr, for q_0=0.5 (0.05), depending on assumptions about gravitational lensing and extinction, also typical of other z>3 galaxies. These objects are tenatively identified as the low-metallicity proto-spheroid clumps that will merge to form the Population II components of today's spheroids.
description: 16 pages, including 2 PostScript figures. Needs aaspp4.sty (included). Accepted for publication in the Astrophysical Journal
Connected correlator of 1/2 BPS Wilson loops in $\mathcal{N}=4$ SYM
Creators: name: Okuyama, Kazumi
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the connected correlator of 1/2 BPS winding Wilson loops in $\mathcal{N}=4$ $U(N)$ super Yang-Mills theory, where those Wilson loops are on top of each other along the same circle. We find the exact finite $N$ expression of the connected correlator of such Wilson loops. We show that the $1/N$ expansion of this exact result is reproduced from the topological recursion of Gaussian matrix model. We also study the exact finite $N$ expression of the generating function of 1/2 BPS Wilson loops in the symmetric representation.
description: 16 pages; v2:reference added
A Multi-wavelength Study of the Galactic Point Sources in the MeerKAT Galactic Plane Survey with Gaia DR3
Creators: name: Egbo, Okwudili Daniel
Publisher: name: Zenodo
Year: 2024

description: The MeerKAT Galactic Plane Survey is a radio continuum survey conducted in the L band (~1.4 GHz) in the Galactic plane, covering a wide range of galactic longitudes, spanning from 0 to 60 degrees and 250 to 360 degrees and mostly within a latitude range of |b| <= 1.5 degrees. The survey resulted in the detection of approximately 5 x 10^5 sources. In this study, we present our analysis of the Galactic sources by cross-matching the radio point sources with the Gaia Data Release 3 (DR3) catalog using a Bayesian cross-match approach. To refine our sample and mitigate spurious and extragalactic counterparts, we imposed a selection criterion based on GAIA parallax over error, focusing on sources with a parallax measurement accuracy of at least 10. This restriction reduced our initial association sample size to approximately 3000 sources. Leveraging the Gaia extinction measurements along the line of sight and the reddening parameter, we applied extinction corrections to the magnitudes and dereddened the colors of the selected sources. Utilizing the dereddened colors and extinction-corrected magnitudes, we constructed a color-magnitude diagram (CMD). The CMD analysis revealed a diverse population of stellar objects, ranging from massive OB stars, white dwarfs, RS CVn binaries, high-mass X-ray binaries (HMXB), YSOs and dMe flare stars. Additionally, we conducted spectroscopic observations of some of the young stars using the Mokodi instrument on the 1-m Lesedi telescope at SAAO. These observations revealed the presence of H-alpha emission, a characteristic emission associated with coronally and chromospherically active radio stars. Our findings provide valuable insights into the radio stellar populations within the Galactic plane, showcasing the diverse range of stellar objects detected in the MeerKAT Galactic Plane Survey. This study highlights the power of cross-matching radio surveys with multi-wavelength datasets, enabling comprehensive characterisation of Galactic sources and advancing our understanding of stellar evolution in our galaxy.
Pheidole megacephala subsp. punctulata Mayr
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1894
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Pheidole
Pheidole megacephala
Pheidole megacephala f., r. punctulata mayr

description: Pheidole megacephala F., r. punctulata Mayr.
Delagoa (Dr. Liengme).
description: Published as part of Forel, A., 1894, Abessinische und andere afrikanische Ameisen, gesammelt von Herrn Ingenieur Alfred Ilg, von Herrn Dr. Liengme, von Herrn Pfarrer Missionar P. Berthoud, Herrn Dr. Arth. Müller, etc., pp. 64-100 in Mitteilungen der Schweizerischen Entomologischen Gesellschaft 9 on page 94, DOI: 10.5281/zenodo.14259
Dilepton Production in Elementary Processes on the Nucleon
Creators: name: Mosel, U.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study elementary processes for production of dileptons from nucleons, either through NN bremsstrahlung or through photon-induced reactions. We emphasize the dependence of the expected cross-sections on the electromagnetic formfactor of the nucleon in the time-like regime and point out that the mentioned reactions can provide important information on the validity of vector meson dominance for the nucleon. We also study the off-shell dependence of the formfactors.
description: Figures available from author by fax
Fig. A.1. Two parallel magmatic belts with contrasting isotopic characteristics from southern Tibet to Myanmar: Zircon U–Pb and Hf isotopic constraints
Creators: name: Te-Hsien Lin
name: A.H.G. Mitchell
name: Sun-Lin Chung
name: Tan, Xi-Bin
name: Jui-Ting Tang
name: Thura Oo
name: Wu, Fu-Yuan
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. A.1. (A) Regional setting of the studied area in Yunnan and Myanmar, and adjacent areas showing locations of (B) and (C), which are sketch geological map showing the distribution of major batholiths in Yunnan and Myanmar, respectively (modified from Mitchell et al., 2012; Lin et al., 2009; Xu et al., 2012). JS, Jinshajiang suture; BNS, Bangong–Nujiang suture; YTS, Yarlu–Tsangpo suture; PMZ, Paung Laung–Mawchi zone; IBR, Indo–Burman Ranges; Tagaung–Myitkyina; Tagaung–Myitkyina belt.
Constraints on Gamma-ray Emission from the Galactic Plane at 300 TeV
Creators: name: Borione, A.
name: Catanese, M. A.
name: Chantell, M. C.
name: Covault, C. E.
name: Cronin, J. W.
name: Fick, B. E.
name: Fortson, L. F.
name: Fowler, J.
name: Glasmacher, M. A. K.
name: Green, K. D.
name: Kieda, D. B.
name: Matthews, J.
name: Newport, B. J.
name: Nitz, D.
name: Ong, R. A.
name: Oser, S.
name: Sinclair, D.
name: van der Velde, J. C.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe a new search for diffuse ultrahigh energy gamma-ray emission associated with molecular clouds in the galactic disk. The Chicago Air Shower Array (CASA), operating in coincidence with the Michigan muon array (MIA), has recorded over 2.2 x 10^{9} air showers from April 4, 1990 to October 7, 1995. We search for gamma rays based upon the muon content of air showers arriving from the direction of the galactic plane. We find no significant evidence for diffuse gamma-ray emission, and we set an upper limit on the ratio of gamma rays to normal hadronic cosmic rays at less than 2.4 x 10^{-5} at 310 TeV (90% confidence limit) from the galactic plane region: (50 degrees < l < 200 degrees); -5 degrees < b < 5 degrees). This limit places a strong constraint on models for emission from molecular clouds in the galaxy. We rule out significant spectral hardening in the outer galaxy, and conclude that emission from the plane at these energies is likely to be dominated by the decay of neutral pions resulting from cosmic rays interactions with passive target gas molecules.
description: Astrophysical Journal, submitted, 11 pages, AASTeX Latex, 3 Postscript figures
The dramatic technique of Jacinto Benavente
Creators: name: Woolsey, Arthur Wallace, 1906-
Publisher: name: The University of Texas at Austin
Year: 1945
Subjects: subject: Benavente, Jacinto, 1866-1954

description: From the time that I first read extensively in the theater of Jacinto Benavente this author has particularly appealed to me in the sweep of his works, the multiplicity of his themes and the variety of his forms and treatments. No previous study has been made of the purely technical aspects of his plays although there has been a great deal written on individual plays as well as concerning the subject matter, satire and treatment of women. This study has been limited to the technique of the author, although it has gone at times beyond the strictly mechanical features to include symbolism, psychological problems and the interés motif
To the Max: Reinventing Reward in Reinforcement Learning
Creators: name: Veviurko, Grigorii
name: Böhmer, Wendelin
name: de Weerdt, Mathijs
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: In reinforcement learning (RL), different reward functions can define the same optimal policy but result in drastically different learning performance. For some, the agent gets stuck with a suboptimal behavior, and for others, it solves the task efficiently. Choosing a good reward function is hence an extremely important yet challenging problem. In this paper, we explore an alternative approach for using rewards for learning. We introduce \textit{max-reward RL}, where an agent optimizes the maximum rather than the cumulative reward. Unlike earlier works, our approach works for deterministic and stochastic environments and can be easily combined with state-of-the-art RL algorithms. In the experiments, we study the performance of max-reward RL algorithms in two goal-reaching environments from Gymnasium-Robotics and demonstrate its benefits over standard RL. The code is available at https://github.com/veviurko/To-the-Max.
Additional file 2 of Modeling the natural history of ductal carcinoma in situ based on population data
Creators: name: Chootipongchaivat, Sarocha
name: van Ravesteyn, Nicolien T.
name: Li, Xiaoxue
name: Huang, Hui
name: Weedon-Fekjær, Harald
name: Ryser, Marc D.
name: Weaver, Donald L.
name: Burnside, Elizabeth S.
name: Heckman-Stoddard, Brandy M.
name: de Koning, Harry J.
name: Lee, Sandra J.
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Statistics
subject: FOS: Mathematics
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 2. Model E description.
Measurement of Pressure Gradients near the Interface in the Viscous Fingering Instability
Creators: name: Gowen, Savannah D.
name: Videbaek, Thomas E.
name: Nagel, Sidney R.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The viscous fingering instability, which forms when a less-viscous fluid invades a more-viscous one within a confined geometry, is an iconic system for studying pattern formation. For both miscible and immiscible fluid pairs the growth dynamics change after the initial instability onset and the global structures, typical of late-time growth, are governed by the viscosity ratio. Here we introduce an experimental technique to measure flow throughout the inner and outer fluids. This probes the existence of a new length scale associated with the local pressure gradients around the interface and allows us to compare our results to the predictions of a previously proposed model for late-time finger growth.
Next-to-leading Order Calculation of the Color-Octet 3S1 Gluon Fragmentation Function for Heavy Quarkonium
Creators: name: Braaten, Eric
name: Lee, Jungil
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The short-distance coefficients for the color-octet 3S1 term in the fragmentation function for a gluon to split into heavy quarkonium states is calculated to order alpha_s^2. The gauge-invariant definition of the fragmentation function by Collins and Soper is employed. Ultraviolet divergences are removed using the MS-bar renormalization procedure. The longitudinal term in the fragmentation function agrees with a previous calculation by Beneke and Rothstein. The next-to-leading order correction to the transverse term disagrees with a previous calculation.
description: 17 pages, 4 figures
Axion Cosmology with Early Matter Domination
Creators: name: Nelson, Ann E.
name: Xiao, Huangyu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The default assumption of early universe cosmology is that the postinflationary universe was radiation dominated until it was about 47000 years old. Direct evidence for the radiation dominated epoch extends back until nucleosynthesis, which began during the first second. However there are theoretical reasons to prefer a period of earlier matter domination, prior to nucleosynthesis, e.g. due to late decaying massive particles needed to explain baryogenesis. Axion cosmology is quantitatively affected by an early period of matter domination, with a different axion mass range preferred and greater inhomogeneity produced on small scales. In this work we show that such increased inhomogeneity can lead to the formation of axion miniclusters in axion parameter ranges that are different from those usually assumed. If the reheating temperature is below $58$ MeV, axion miniclusters can form even if the axion field is present during inflation and has been previously homogenized. The upper bound on the typical initial axion minicluster mass is raised from $10^{-10} M_{\odot}$ to $10^{-7} M_{\odot}$, where $M_{\odot}$ is a solar mass. These results may have consequences for indirect detection of axion miniclusters, and could conceivably probe the thermal history of the universe before nucleosynthesis.
description: 9 pages, 3 figures, refs added
Fig. A.6. Two parallel magmatic belts with contrasting isotopic characteristics from southern Tibet to Myanmar: Zircon U–Pb and Hf isotopic constraints
Creators: name: Te-Hsien Lin
name: A.H.G. Mitchell
name: Sun-Lin Chung
name: Tan, Xi-Bin
name: Jui-Ting Tang
name: Thura Oo
name: Wu, Fu-Yuan
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. A.6. Simplified diagram shows plausible correlation between the Gondwana related terranes.