cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Artoadenus dius OPITZ 2015, nov. sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Artoadenus
Artoadenus dius

description: Artoadenus dius OPITZ nov. sp. (Figs 64, 113, 114, 147, 175)
Holotype: ♂. Panama, Pnma. Prov. K 8-13 El Llano-Carti Rd, 10-13 May 1996, Wappes Huether, & Morris (FSCA). Paratypes: Three specimens. Panamá: Panamá: 7-11 km El Llano / Carti Rd., 7-V-1999, Morris / Wappes (JEWC, 1); Canal Zone: Barro Colorado Island, 3- VIII-1978, R.B. & L.S. Kimsey (UCDC, 1). Venezuela: Tachira: La Morita, 8-14-IV-72, A. D’Ascoli, A. Montague, J. Salcedo (WFBM, 1).
Diagnosis: The metatibial glandular pit is prominent in the males of Artoadenus and Platynoptera. But, specimens of A. dius have subsecuriform terminal palpomeres, whereas Platynoptera specimens have securiform terminal palpomeres.
Description: Size: Length 12.0 mm; width 6.0 mm. Form: As in Fig. 147. Color: Cranium bicolorous, upper frons and region behind eyes black, remainder flavotestaceous; pronotum mostly flavotestaceous, disc with two lateral black lines; mesoscutellum flavotestaceous; elytral disc mostly flavotestaceous, posterior third black. Head: Antennal capitulum very long (Fig. 64), each capitular antennomere longer than combined length of scape, pedicel, and funicle; antennal carina very prominent; EW/FW 20/20. Thorax: Pronotal anterior margin not projected at middle; side margin of disc slightly rounded in posterior third; PW/PL 100/85; elytra moderately flared; EL/EW 180/55. Abdomen: Male pygidium not incised at distal margin; aedeagus as in Figs. 113, 114.
Variation: Size: length 12.0-15.0 mm; width 6.0-8.0 mm. The elytral disc may be entirely flavotestaceous, or mostly black with the basal margin and middle fascia flavotestaceous.
Natural history: Specimens were collected during April, May, and August. The specimen from Venezuela was collected at 300 m.
Distribution (Fig. 175): Known from Panamá and Venezuela.
Etymology: The trivial name dius (= between) is a Greek adjective. I refer to the superficial similarities among specimens of Artoadenus, Platynoptera, and Tarandocerus.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on pages 1526-1527, DOI: 10.5281/zenodo.5282503
Artoadenus regina OPITZ 2015, nov. sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Artoadenus
Artoadenus regina

description: Artoadenus regina OPITZ nov. sp.
(Figs 65, 115, 116, 148, 175)
Holotype: ♂. Guyane (Régina) (French Guiana), Montagne de Kaw Pk., 37.5, 5.XII.2004, J. A. Cerda. A second label reads: á vue en forět (FSCA). Paratypes: Two specimens. Guyana, Regina, Kaw Mountain Park, 2-IX-1999, J. A. Cerda (WOPC, 1); idem, 10-X-2001, J. A. Cerda (WOPC, 1).
Diagnosis: The elytral color pattern, as depicted in Fig. 148, will distinguish the members of this species from congeners.
Description: Size: Length 10.0 mm; width 4.0 mm. Form: As in Fig. 148. Color: Cranium bicolorous, cranial venter and region behind eyes flavotestaceous, remainder black; pronotum mostly black, sides flavotestaceous; mesoscutellum brown; elytral disc mostly black, with flavotestaceous fascia. Head: Antennal capitulum very long (Fig. 65), each capitular antennomeres longer than combined length of funicle; antennal carina very prominent; EW/FW 18/18. Thorax: Pronotal anterior margin not projected at middle; side margin of disc slightly rounded; PW/PL 60/55; elytra moderately flared; EL/EW 230/50. Abdomen: Male pygidium not incised at distal margin; aedeagus as in Figs. 115, 116.
Variation: Size: length 10.0-12.0 mm; width 4.0-5.0 mm. The pronotal disc may show a narrow flavotestaceous line that may extend to the cranial vertex.
Natural history: Specimens were collected during October, November, and December.
Distribution (Fig. 175): Known from French Guiana.
Etymology: The trivial name regina constitutes a noun in apposition and refers to the type locality.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on page 1527, DOI: 10.5281/zenodo.5282503
TeV Gamma-Ray Observations of the Perseus and Abell 2029 Galaxy Clusters
Creators: name: Perkins, J. S.
name: Badran, H. M.
name: Blaylock, G.
name: Bradbury, S. M.
name: Cogan, P.
name: Chow, Y. C. K.
name: Cui, W.
name: Daniel, M. K.
name: Falcone, A. D.
name: Fegan, S. J.
name: Finley, J. P.
name: Fortin, P.
name: Fortson, L. F.
name: Gillanders, G. H.
name: Gutierrez, K. J.
name: Grube, J.
name: Hall, J.
name: Hanna, D.
name: Holder, J.
name: Horan, D.
name: Hughes, S. B.
name: Kenny, G. E.
name: Kertzman, M.
name: Kieda, D. B.
name: Kildea, J.
name: Kosack, K.
name: Krawczynski, H.
name: Krennrich, F.
name: Lang, M. J.
name: LeBohec, S.
name: Maier, G.
name: Moriarty, P.
name: Ong, R. A.
name: Pohl, M.
name: Ragan, K.
name: Rebillot, P. F.
name: Sembroski, G. H.
name: Steele, D.
name: Swordy, S. P.
name: Valcarcel, L.
name: Vassiliev, V. V.
name: Wakely, S. P.
name: Weekes, T. C.
name: Williams, D. A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Galaxy clusters might be sources of TeV gamma rays emitted by high-energy protons and electrons accelerated by large scale structure formation shocks, galactic winds, or active galactic nuclei. Furthermore, gamma rays may be produced in dark matter particle annihilation processes at the cluster cores. We report on observations of the galaxy clusters Perseus and Abell 2029 using the 10 m Whipple Cherenkov telescope during the 2003-2004 and 2004-2005 observing seasons. We apply a two-dimensional analysis technique to scrutinize the clusters for TeV emission. In this paper we first determine flux upper limits on TeV gamma-ray emission from point sources within the clusters. Second, we derive upper limits on the extended cluster emission. We subsequently compare the flux upper limits with EGRET upper limits at 100 MeV and theoretical models. Assuming that the gamma-ray surface brightness profile mimics that of the thermal X-ray emission and that the spectrum of cluster cosmic rays extends all the way from thermal energies to multi-TeV energies with a differential spectral index of -2.1, our results imply that the cosmic ray proton energy density is less than 7.9% of the thermal energy density for the Perseus cluster.
description: Accepted for publication in the Astrophysical Journal
Double-peaked Lyman-$α$ emission at z=6.803: a reionisation-era galaxy self-ionising its local HII bubble
Creators: name: Meyer, Romain A.
name: Laporte, Nicolas
name: Ellis, Richard S.
name: Verhamme, Anne
name: Garel, Thibault
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the discovery of a double-peaked Lyman-alpha profile in a galaxy at $z=6.803$, A370p\_z1, in the parallel Frontier Field of Abell 370. The velocity separation between the blue and red peaks of the Lyman-$α$ profile ($Δv=101_{-19}^{+38} (\pm48)\,\text{km s}^{-1}$) suggests an extremely high escape fraction of ionising photons $> 59(51)\% (2σ)$. The spectral energy distribution indicates a young ($50$ Myr), star-forming ($12\pm 6 \, \rm{M}_\odot \rm{yr}^{-1}$) galaxy with an IRAC excess implying strong [OIII]+H$β$ emission. On the basis of the high escape fraction measured, we demonstrate that A370p\_z1 was solely capable of creating an ionised bubble sufficiently large to account for the blue component of its Lyman-alpha profile. We discuss whether A370p\_z1 may be representative of a larger population of luminous $z\simeq7$ double-peaked Lyman-alpha emitting sources with high escape fractions that self-ionised their surroundings without contributions from associated UV-fainter sources.
description: Accepted for publication in MNRAS. 7 pages, 4 figures, 3 tables
Artoadenus similus OPITZ 2015, nov.sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Artoadenus
Artoadenus similus

description: Artoadenus similus OPITZ, nov.sp.
(Figs. 82, 133, 134, 149, 174)
Holotype: ♂. México: Jalisco, Puerto Los Mazos, 9 mi NW Autlan, VIII-28-1970, M. S. & J. S. Wasbauer (WFBM).
Diagnosis: This is the only member of Artoadenus that is distributed in Middle America.
Description: Size: Length 14.0 mm; width 6.0 mm. Form: As in Fig. 149. Color: Cranium mostly black, vertex with small flavotestaceous streak; pronotum mostly flavotestaceous, disc with two paralateral black streaks; mesoscutellum flavotestaceous; elytra bicolorous, humeral margin brown, disc mostly black, with wide flavotestaceous fascia. Head: Antennal capitulum long (Fig. 82), each capitular antennomere longer than combined length of funicular antennomeres; antennal carina very prominent; EW/FW 23/25. Thorax: Pronotal anterior margin not projected at middle, side margin of disc parallel in anterior two-thirds; PW/PL 92/87; elytral disc strongly explanate at sides, carina not present; EL/EW 390/120. Abdomen: Male pygidium not incised at distal margin; aedeagus (Figs. 133, 134); phallic apex very large.
Natural history: The holotype was collected in August.
Distribution (Fig. 174): Known only from the type locality.
Etymology: The trivial name similus stems from similis (= like), is a Latin adjective. I refer to the shared superficial similarity between the members of this species and congeners.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on pages 1528-1529, DOI: 10.5281/zenodo.5282503
Representations of Generalized a$_r$ Statistics and Eigenstates of Jacobson Generators
Creators: name: Daoud, Mohammed
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We investigate a generalization of $A_r$ statistics discussed recently in the literature. The explicit complete set of state vectors for the $A_r$ statistics system is given. We consider a Bargmann or an analytic function description of the Fock space corresponding to $A_r$ statistics of bosonic kind. This brings, in a natural way, the so-called Gazeau-Klauder coherent states defined as eigenstates of the Jacobson annihilation operators. The minimization of Robertson uncertainty relation is also considered.
description: 10 pages, to appear in MPLA (2006)
Optical Hall response in spin-orbit coupled metals: Comparative study of magnetic cluster monopole, quadrupole, and toroidal orders
Creators: name: Sato, Tatsuki
name: Umimoto, Yuma
name: Sugita, Yusuke
name: Kato, Yasuyuki
name: Motome, Yukitoshi
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The optical Hall response is theoretically studied for spin-orbit coupled metals with ferroic orders of cluster-type magnetic multipoles. We find that different magnetic multipoles give rise to distinct spectra in the optical Hall conductivity. In the cases of monopole and quadrupole orders, the optical Hall response appears predominantly in high- and low-energy regions, which correspond to the energy scales of electron correlation and kinetic energy, respectively, while the response is dispersed and rather weak in the case of toroidal order. By decomposing the spectra into different interband contributions, we reveal selection rules stemming from the interplay between the antisymmetric spin-orbit coupling and the underlying multipoles. Our results suggest that the optical Hall measurement is useful to detect and distinguish the cluster-type magnetic multipole orders.
description: 10 pages, 10 figures
A Generating Function for all Semi-Magic Squares and the Volume of the Birkhoff Polytope
Creators: name: De Loera, Jesus A.
name: Liu, Fu
name: Yoshida, Ruriko
Publisher: name: arXiv
Year: 2007
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 52C07; 52B20

description: We present a multivariate generating function for all n x n nonnegative integral matrices with all row and column sums equal to a positive integer t, the so called semi-magic squares. As a consequence we obtain formulas for all coefficients of the Ehrhart polynomial of the polytope B_n of n x n doubly-stochastic matrices, also known as the Birkhoff polytope. In particular we derive formulas for the volumes of B_n and any of its faces.
description: 24 pages, 1 figure. To appear in Journal of Algebraic Combinatorics
Aspitonis alarutinis OPITZ 2015, nov.sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Lycidae
Aspitonis
Aspitonis alarutinis

description: Aspitonis alarutinis OPITZ, nov.sp.
(Figs. 66, 93-95, 117, 118, 150, 173)
Holotype: ♀. Costa Rica, Puntarenas, Monteverde, Feb 21 1987, E. Giesbert (FSCA).
Diagnosis: The elytral disc is bright red. This characteristic will distinguish the members of this species from congeners.
Description: Size: Length 8.0 mm; width 2.5 mm. Form: As in Fig. 150. Color: Cranium black, clypeus testaceous; pronotum mostly red, upper sides and short line at midbase testaceous; mesoscutellum black; elytra bright red. Head: Antennal capitulum very long (Fig. 66), each capitular antennomere longer than combined length of scape, pedicel, and funicle (Fig. 93); antennal carina very prominent; EW/FW 11/17. Thorax: Pronotal anterior margin not projected at middle, side margin of disc with welldeveloped tubercle; PW/PL 48/45; elytral disc strongly deflexed at sides, elytral carina faintly visible; EL/EW 190/35. Abdomen: Male pygidium incised distally; aedeagus (Figs. 117, 118) slightly sclerotized; tegminal lobes acuminate.
Natural history: The holotype was collected during February.
Distribution (Fig. 173): Known only from the type locality.
Etymology: The specific epithet alarutinis is a Latin compound name derived from ala (= wing) and rutilus (= red). I refer to the red coloration of the elytra.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on page 1530, DOI: 10.5281/zenodo.5282503
Scattering of polarized laser light by an atomic gas in free space: a QSDE approach
Creators: name: Bouten, Luc
name: Stockton, John K.
name: Sarma, Gopal
name: Mabuchi, Hideo
Publisher: name: arXiv
Year: 2007
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We propose a model, based on a quantum stochastic differential equation (QSDE), to describe the scattering of polarized laser light by an atomic gas. The gauge terms in the QSDE account for the direct scattering of the laser light into different field channels. Once the model has been set, we can rigorously derive quantum filtering equations for balanced polarimetry and homodyne detection experiments, study the statistics of output processes and investigate a strong driving, weak coupling limit.
description: 9 pages, 2 figures
Predicting marital instability: an empirical test of competing models
Creators: name: Bartolic-Zlomislic, Silvia
Publisher: name: University of British Columbia
Year: 2009

description: There has been substantial empirical. research and theoretical modelling on the determinants of marital instability. However, the predominant theoretical models, largely based on field theory and social exchange, are ambiguous. Due to this ambiguity, there remains an ongoing debate in the literature as to the utility of these models. In addition, there are few empirical tests of these models, while existing tests are limited by poor measures and sample restrictiveness. Furthermore, the models are largely developed from research with samples restricted to short marital durations, consequently, limiting the utility of these models on marriages of longer duration. Five models based on Levinger's (1965, 1976) conceptualisation of marital attractions, alternatives, and barriers and Lewis and Spanier's (1979) theory of marital quality and marital stability are developed. Four sets of tests are conducted using the National Survey of Families and Households data set (waves 1 and 2), a national, stratified, multi-stage area probability sample consisting of over 13,000 cases in the United States'. First, a series of logistic regression analyses are run to determine if marital quality has a significant effect on marital stability, a notion based on little empirical evidence. Second, five models are compared to determine which of five competing explanations best fits the data. Third, the best fitting model is retested with the addition of control variables. Fourth, the resulting model is retested on younger and older marriage cohorts. Marital quality is found to have a significant effect on marital stability. Results of the model comparisons provide support for an additive curvilinear model where marital quality, alternatives, and barriers all have independent effects on marital stability. This provides support for Lewis and Spanier's (1979) marital typology With the addition of controls, the model remains significant. However, the additional significance of duration and commitment suggest that cohort and duration effects may be occurring. The model is effective in predicting marital stability for the younger marriage cohort but did not apply to the older marriage cohort. These results suggest a theoretical implication. Time oriented theories need to be examined as possible explanations for marital stability, especially for older marriage cohorts.
The Latency Validation of the Optical Link for the ATLAS Liquid Argon Calorimeter Phase-I Trigger Upgrade
Creators: name: Deng, Binwei
name: Xiao, Le
name: Zhao, Xiandong
name: Baker, Emily
name: Gong, Datao
name: Guo, Di
name: He, Huiqin
name: Hou, Suen
name: Liu, Chonghan
name: Liu, Tiankuan
name: Sun, Quan
name: Thomas, James
name: Wang, Jian
name: Xiang, Annie C.
name: Yang, Dongxu
name: Ye, Jingbo
name: Zhou, Wei
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Two optical data link data transmission Application Specific Integrated Circuits (ASICs), the baseline and its backup, have been designed for the ATLAS Liquid Argon (LAr) Calorimeter Phase-I trigger upgrade. The latency of each ASIC and that of its corresponding receiver implemented in a back-end Field-Programmable Gate Array (FPGA) are critical specifications. In this paper, we present the latency measurements and simulation of two ASICs. The measurement results indicate that both ASICs achieve their design goals and meet the latency specifications. The consistency between the simulation and measurements validates the ASIC latency characterization.
Tensorial Structure of the LQG graviton propagator
Creators: name: Alesci, Emanuele
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We review the construction of the tensorial structure of the graviton propagator in the context of loop quantum gravity and spinfoam formalism. The main result of this analysis is that applying the same strategy used to compute the diagonal terms, the Barrett-Crane vertex is unable to yield the correct propagator in the long distance limit. The problem is in the intertwiner-independence of the Barrett-Crane vertex. We also review the asymptotic behavior of an alternative vertex that is able to give the correct propagator.
description: 4 pages,; to appear in the proceedings of the II Stueckelberg Workshop, Int.J.Mod.Phys.A
Aspitonis chiapas OPITZ 2015, nov.sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Lycidae
Aspitonis
Aspitonis chiapas

description: Aspitonis chiapas Opitz, nov.sp.
(Figs. 119, 120, 151, 173)
Holotype: ♂. 16 mi. E. Teopisca, Chis. Mex. V.14, 1969, H. Howden (CMNC).
Diagnosis: The elytral disc is completely black. This characteristic will distinguish the members of this species from congeners.
Description: Size: Length 5.5 mm; width 1.8 mm. Form: As in Fig. 151. Color: Cranium black, lower frons and clypeus yellow; pronotum mostly black, upper sides reddish; mesoscutellum black; elytra black. Head: Antennal capitulum not available; antennal carina very prominent; EW/FW 10/13. Thorax: Pronotal anterior margin not projected at middle, side margin without tubercle; form elongate; PW/PL 30/35; elytral disc strongly deflexed at sides, elytral carina absent; EL/EW 140/30. Abdomen: Male pygidium not incised distally; aedeagus (Figs. 119, 120) slightly sclerotized; tegminal lobes acuminate and fimbriate.
Natural history: The holotype was collected in May.
Distribution (Fig. 173): Known only from the type locality.
Etymology: The specific epithet chiapas is a noun in apposition and refers to the type locality.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on page 1530, DOI: 10.5281/zenodo.5282503
Magnetism of Sigma-Phase Fe68V32 Compound
Creators: name: Konieczny, Piotr
name: Dubiel, Stanisław M.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The magnetic phase diagram in the H-T coordinates has been determined for σ-Fe68V32 from the ZFC/FC magnetization measurements. The re-entrant character of magnetism, going from paramagnetic through ferromagnetic to spin-glass (SG) states, has been evidenced. The SG phase is magnetically heterogeneous, because two sub phases can be identified i.e. with the strong (SG-SI) and the weak (SG-WI) irreversibility. The ireversibility, T_irr and the crossover, T_cros, temperatures were quantitatively analysed using the mean-field theory and ϕ_irr=1.6(2) and ϕ_cros=0.91(9) values were obtained. A qualitative agreement with the Gabay-Toulouse model was reached. The isothermal magnetization measurements point to a soft magnetic behaviour of the studied sample. The γ critical exponent was determined with the Kouvel-Fisher approach yielding the value of γ=1.0(1) in line with the mean-field theory.
description: 10 pages, 6 Figures and 19 References
Topological phonons in oxide perovskites controlled by light
Creators: name: Peng, Bo
name: Hu, Yuchen
name: Murakami, Shuichi
name: Zhang, Tiantian
name: Monserrat, Bartomeu
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Perovskite oxides exhibit a rich variety of structural phases hosting different physical phenomena that generate multiple technological applications. We find that topological phonons, i.e., nodal rings, nodal lines, and Weyl points, are ubiquitous in oxide perovskites in terms of structures (tetragonal, orthorhombic, and rhombohedral), compounds (BaTiO3, PbTiO3, and SrTiO3), and external conditions (photoexcitation, strain, and temperature). In particular, in the tetragonal phase of these compounds, all types of topological phonons can simultaneously emerge when stabilized by photoexcitation, whereas the tetragonal phase stabilized by thermal fluctuations only hosts a more limited set of topological phonon states. Additionally, we find that the photoexcited carrier concentration can be used to tune the topological phonon states and induce topological transitions even without associated structural phase changes. Overall, we propose oxide perovskites as a versatile platform in which to study topological phonons and their manipulation with light.
description: 26 pages, 5 figures
D5.1: 5G Security Test Cases
Creators: name: Osorio, Diana P. M.
Publisher: name: Zenodo
Year: 2021

description: This deliverable presents the set of test cases selected for validation on the INSPIRE-5Gplus project. This set of test cases were selected by performing an exhaustive requirements elicitation of 5G security use cases defined in WP2, stemming from the new and enhanced 5G security and trust/liability enablers developed in WP3 and WP4. Herein, we perform an initial description on the requirements, key performance indicators and relationship of the test cases to the High-Level Architecture being developed in WP2. Finally, the capabilities and enhancements required for the envisioned testing environment for the integration and experimentation of the 5G security test cases is also presented.
A broadband spectroscopic search for CO line emission in HDF850.1: the brightest submillimetre object in the Hubble Deep Field North
Creators: name: Wagg, J.
name: Hughes, D. H.
name: Aretxaga, I.
name: Chapin, E. L.
name: Dunlop, J. S.
name: Gaztanaga, E.
name: Devlin, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using the 100-m Green Bank Telescope, we have conducted a cm-wavelength search for CO J=1-0 line emission towards the high-redshift, far-infrared luminous object, HDF850.1 over the redshift interval 3.3nu(obs)>18.0 GHz), making HDF850.1 a potential occupent of the `high-redshift tail' of submm selected galaxies. We have also conducted a search for CO J=2-1 line emission over the narrower redshift range, 3.9
description: accepted for publication in MNRAS
Extragalactic MeV gamma-ray emission from cocoons of young radio galaxies
Creators: name: Kino, M.
name: Kawakatu, N.
name: Ito, H.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Strong $γ$-ray emission from cocoons of young radio galaxies is newly predicted. Considering the process of adiabatic injection of the shock dissipation energy and mass of the relativistic jet in active nuclei (AGNs) into the cocoon, while assuming thermalizing electron plasma interactions, we find that the thermal electron temperature of the cocoon is typically predicted in $\sim$MeV, which is determined only by the bulk Lorentz factor of the relativistic jet. Together with the time-dependent dynamics of the cocoon expansion, we find that young cocoons can yield thermal bremsstrahlung emissions at energies $\sim$ MeV.
description: 5pages, 1figure, MNRAS accepted
The connection between entropy and the absorption spectra of Schwarzschild black holes for light and massless scalar fields
Creators: name: Mendoza, S.
name: Hernandez, X.
name: Rendon, P. L.
name: Lopez-Monsalvo, C. S.
name: Velasco-Segura, R.
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present heuristic arguments suggesting that if EM waves with wavelengths somewhat larger than the Schwarzschild radius of a black hole were fully absorbed by it, the second law of thermodynamics would be violated, under the Bekenstein interpretation of the area of a black hole as a measure of its entropy. Thus, entropy considerations make the well known fact that large wavelengths are only marginally absorbed by black holes, a natural consequence of thermodynamics. We also study numerically the ingoing radial propagation of a scalar field wave in a Schwarzschild metric, relaxing the standard assumption which leads to the eikonal equation, that the wave has zero spatial extent. We find that if these waves have wavelengths larger that the Schwarzschild radius, they are very substantially reflected, fully to numerical accuracy. Interestingly, this critical wavelength approximately coincides with the one derived from entropy considerations of the EM field, and is consistent with well known limit results of scattering in the Schwarzschild metric. The propagation speed is also calculated and seen to differ from the value $c$, for wavelengths larger than $R_{s}$, in the vicinity of $R_{s}$. As in all classical wave phenomena, whenever the wavelength is larger or comparable to the physical size of elements in the system, in this case changes in the metric, the zero extent 'particle' description fails, and the wave nature becomes apparent.
description: 14 Pages, 4 figures. Accepted for publication in the Journal Entropy
The All-Sky SignAl Short-Spacing INterferometer (ASSASSIN) I: Global sky measurements with the Engineering Development Array-2
Creators: name: McKinley, B.
name: Trott, C. M.
name: Sokolowski, M.
name: Wayth, R. B.
name: Sutinjo, A.
name: Patra, N.
name: T., J. Nambissan
name: Ung, D. C. X.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Aiming to fill a crucial gap in our observational knowledge of the early Universe, experiments around the world continue to attempt to verify the claimed detection of the redshifted 21-cm signal from Cosmic Dawn by the EDGES experiment. This sky-averaged or 'global' signal from neutral hydrogen should be detectable at low radio frequencies (50-200 MHz), but is difficult to measure due to bright foreground emission and difficulties in reaching the required levels of instrumental-calibration precision. In this paper we outline our progress toward using a novel new method to measure the global redshifted 21-cm signal. Motivated by the need to use alternative methods with very different systematic errors to EDGES for an independent result, we employ an array of closely-spaced antennas to measure the global sky signal interferometrically, rather than using the conventional approach with a single antenna. We use simulations to demonstrate our newly-developed methods and show that, for an idealised instrument, a 21-cm signal could theoretically be extracted from the visibilities of an array of closely-spaced dipoles. We verify that our signal-extraction methods work on real data using observations made with a Square Kilometre-Array-like prototype; the Engineering Development Array-2. Finally, we use the lessons learned in both our simulations and observations to lay out a clear plan for future work, which will ultimately lead to a new global redshifted 21-cm instrument: the All-Sky SignAl Short-Spacing INterferometer (ASSASSIN).
description: 18 pages, 13 figures
Aspitonis graminis OPITZ 2015, nov. sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Lycidae
Aspitonis
Aspitonis graminis

description: Aspitonis graminis OPITZ nov. sp.
(Figs. 67, 152, 173)
Holotype: ♀. Panama: Chiriquí: Bambito, 1585 m, 7 Jan. 1988, MacDonald & Shiefer (MEMU). Paratypes: One specimen. Panamá: Chiriquí: Bambito, 1585 m, 7-I-1988, MacDonald & Shiefer (WOPC).
Diagnosis: The elytral disc is mostly flavotestaceous. This characteristic will distinguish the members of this species from congeners.
Description: Size: Length 5.5 mm; width 1.6 mm. Form: As in Fig. 152. Color: Cranium mostly black, lower frons and venter flavotestaceous; pronotum mostly flavotestaceous, upper sides and short line at midbase black; mesoscutellum black; elytral disc mostly flavotestaceous, epipleural and sutural margins partly dark brown. Head: Antennal capitulum very long (Fig. 67), each capitular antennomere as long as combined length of scape, pedicel, and funicle; antennal carina very prominent; EW/FW 10/12. Thorax: Pronotal anterior margin not projected at middle, side margin of disc with welldeveloped tubercle; PW/PL 33/30; elytral disc strongly deflexed at sides, with 3 faintly developed carina; EL/EW 130/20. Abdomen: Female pygidium not incised at distal margin.
Variation: Size: length 7.0-8.5 mm; width 1.6-2.0.0 mm.
Natural history: Specimens were collected from the type locality during January, at 1585 m.
Distribution (Fig. 173): Known only from western Panamá.
Etymology: The specific epithet graminis (= grass) is a Latin noun. I refer to the straw-colored elytra.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on pages 1531-1532, DOI: 10.5281/zenodo.5282503
Kinematics and stellar populations of the dwarf elliptical galaxy IC 3653
Creators: name: Chilingarian, Igor
name: Prugniel, Philippe
name: Sil'chenko, Olga
name: Afanasiev, Victor
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first 3D observations of a diffuse elliptical galaxy (dE). The good quality data (S/N up to 40) reveal the kinematical signature of an embedded stellar disc, reminiscent of what is commonly observed in elliptical galaxies, though similarity of their origins is questionable. Colour map built from HST ACS images confirms the presence of this disc. Its characteristic scale (about 3 arcsec = 250 pc) is about a half of galaxy's effective radius, and its metallicity is 0.1-0.2 dex larger than the underlying population. Fitting the spectra with synthetic single stellar populations (SSP) we found an SSP-equivalent age of 5 Gyr and nearly solar metallicity [Fe/H]=-0.06 dex. We checked that these determinations are consistent with those based on Lick indices, but have smaller error bars. The kinematical discovery of a stellar disc in dE gives additional support to an evolutionary link from dwarf irregular galaxies due to stripping of the gas against the intra-cluster medium.
description: 15 pages, 10 figures, accepted to MNRAS
Coffee Lecture Slides: Datendokumentation
Creators: name: Gerlach, Roman
name: Schröter, Annett
name: Lang, Kevin
Publisher: name: Zenodo
Year: 2021
Subjects: datendokumentation
data documentation
tkfdm
research data
forschungsdaten

description: English: Coffee Lecture Slides: Datendokumentation - Die Basis hoher Datenqualität! (Coffee Lecture 24.02.2021, only in German available) In this Coffee Lecture we will start with the question why good data documentation is so important for the reusability of data. However, the central topic of the event will be the different forms of data documentation and how they can help to improve data quality. The event will provide practical advice on which methods and tools exist to facilitate the creation of documentation and how high quality of documentation can be achieved. Video: Link ------------------------------------------------------ Deutsch: Datendokumentation - Die Basis hoher Datenqualität! (Coffee Lecture 24.02.2021) In dieser Coffee Lecture starten wir mit der Frage, warum eine gute Datendokumentation so wichtig ist für die Nachnutzbarkeit von Daten. Das zentrale Thema der Veranstaltung werden jedoch die verschiedenen Formen der Datendokumentation sein und wie diese dazu beitragen können, die Datenqualität zu verbessern. Die Veranstaltung soll praktische Hinweise geben, welche Methoden und Tools existieren um die Erstellung einer Dokumentation zu erleichtern und wie eine hohe Qualität der Dokumentation erreicht werden kann. Video: Link
Electronic Books Primer: Acquisition, Access and Processing
Creators: name: Lowe, Randall
name: Williams, Virginia
Publisher: name: Maryland Shared Open Access Repository
Year: 2011

description: Original document was revised October 2011. Proprietary pricing information has been redacted in the white paper.
description: Beginning with a brief history and context, this white paper addresses issues related to electronic books at Frostburg State University including: acquisition models, selection, access and discovery, and processing.
Aspitonis undulicornis OPITZ 2015, nov. sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Lycidae
Aspitonis
Aspitonis undulicornis

description: Aspitonis undulicornis OPITZ nov. sp.
(Figs. 68, 121, 122, 153, 174)
Holotype: ♂. Mexico, Chis. Hwy. 190, 10 mi. SE San Cristobal de las Casas, 7400'. A second label reads: 25 May 1983, C.W. & L. O’Brien 7 G.B. Marshall (FSCA).
Diagnosis: The pronotum is mostly red and is without the midbasal dark line. This characteristic will distinguish the members of this species from congeners.
Description: Size: Length 5.5 mm; width 1.5 mm. Form: As in Fig.153. Color: Cranium mostly red, region near antennal base and behind eyes narrowly black; pronotum mostly red, lower sides black; mesoscutellum yellow; elytral disc red. Head: Antennal capitulum very long (Fig. 68), each capitular antennomere as long as combined length of scape, pedicel, and funicle; antennal carina very prominent; EW/FW 9/15. Thorax: Pronotal anterior margin not projected at middle, side margin of disc with shallow tubercle; PW/PL 34/34; elytral disc strongly deflexed at sides, carina not present; EL/EW 138/28. Abdomen: Male pygidium not incised at distal margin; aedeagus as in Figs. 121, 122.
Natural history: The holotype was collected during May, at 2256 m.
Distribution (Fig. 174): Known only from southeastern México.
Etymology: The specific epithet undulicornis is a Latin compound name derived from unda (= wave) and cornu (= horn). I refer to the undulation of the anterior margin of antennomere 9.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on page 1532, DOI: 10.5281/zenodo.5282503
Gaia Early Data Release 3 -- Catalogue validation
Creators: name: Fabricius, C.
name: Luri, X.
name: Arenou, F.
name: Babusiaux, C.
name: Helmi, A.
name: Muraveva, T.
name: Reylé, C.
name: Spoto, F.
name: Vallenari, A.
name: Antoja, T.
name: Balbinot, E.
name: Barache, C.
name: Bauchet, N.
name: Bragaglia, A.
name: Busonero, D.
name: Cantat-Gaudin, T.
name: Carrasco, J. M.
name: Diakité, S.
name: Fabrizio, M.
name: Figueras, F.
name: Garcia-Gutierrez, A.
name: Garofalo, A.
name: Jordi, C.
name: Kervella, P.
name: Khanna, S.
name: Leclerc, N.
name: Licata, E.
name: Lambert, S.
name: Marrese, P. M.
name: Masip, A.
name: Ramos, P.
name: Robichon, N.
name: Robin, A. C.
name: Romero-Gómez, M.
name: Rubele, S.
name: Weiler, M.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The third Gaia data release is published in two stages. The early part, Gaia EDR3, gives very precise astrometric and photometric properties for nearly two billion sources together with seven million radial velocities from Gaia DR2. The full release, Gaia DR3, will add radial velocities, spectra, light curves, and astrophysical parameters for a large subset of the sources, as well as orbits for solar system objects. Before the publication of the catalogue, many different data items have undergone dedicated validation processes. The goal of this paper is to describe the validation results in terms of completeness, accuracy, and precision for the Gaia EDR3 data and to provide recommendations for the use of the catalogue data. The validation processes include a systematic analysis of the catalogue contents to detect anomalies, either individual errors or statistical properties, using statistical analysis and comparisons to the previous release as well as to external data and to models. Gaia EDR3 represents a major step forward, compared to Gaia DR2, in terms of precision, accuracy, and completeness for both astrometry and photometry. We provide recommendations for dealing with issues related to the parallax zero point, negative parallaxes, photometry for faint sources, and the quality indicators.
description: This paper is part of the Astronomy&Astrophysics special issue on Gaia Early Data Release 3
Scalar-tensor cosmological simulations
Creators: name: Rodriguez-Meza, M. A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present $N$-body cosmlogical simulations in the framework of the Newtonian limit of scalar-tensor theories of gravity. The scalar field is described by a modified Helmholtz equation with a source that is coupled to the standard Poisson equation of Newtonian gravity. The effective gravitational force is given by two contributions: the standard Newtonian potential plus a Yukawa potential stemming from massive scalar fields. In particular, we consider simulations of $Λ$CDM models and compute the density and velocity profiles of the most massive groups found at z=0.
description: 6 pages, 6 figures. Recent Developments in Gravitation and Experimental Physics: 3rd Mexican Meeting of Mathematical and Experimental Physics. Edited by A. Macias, C. Laemmerzahl, and A. Camacho. (American Institute of Physics, 2008). Pag. 302
Isoforma biguttula OPITZ 2015, nov. sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Isoforma
Isoforma biguttula

description: Isoforma biguttula OPITZ nov. sp.
(Figs 24-26, 69, 123, 124, 154, 175)
Holotype: ♂. Teffe (Ega), Amazonas (Brazil), M. De Mathan, 1 st Trimester, 1879 (MNHN).
Diagnosis: The holotype has the black elytral macula extended to the anterior third of the elytral disc. No other available specimens of this genus have this characteristic. Also, only in the available specimen of this species is the cranium entirely testaceous.
Description: Size: Length 9.0 mm; width 4.0 mm. Form: As in Fig. 154. Color: Cranium flavotestaceous; pronotum flavotestaceous; elytral disc mostly black, basal third flavotestaceous. Head: Antennal capitulum very long (Fig. 69), each capitular antennomere longer than funicle; antennal carina very prominent; EW/FW 15/30. Thorax: Pronotal anterior margin linear, not projected at middle; side margins of disc rounded at middle; PW/PL 70/50; elytra conspicuously flared, discal carinae faintly developed; EL/EW 245/125. Abdomen: Male pygidium not incised at distal margin; aedeagus (Figs. 123, 124) short; tegminal lobes uncinate; phallobasic rod long and broad.
Distribution (Fig. 175): Known only from the type locality.
Etymology: The trivial name biguttula is a Latin adjective derived from the prefix bi- (= two) and gutta (= spot). I refer to the two black spots on the elytral disc.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on page 1536, DOI: 10.5281/zenodo.5282503
Holographic melting and related properties of mesons in a quark gluon plasma
Creators: name: Peeters, Kasper
name: Sonnenschein, Jacob
name: Zamaklar, Marija
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyse mesons at finite temperature in a chiral, confining string dual. The temperature dependence of low-spin as well as high-spin meson masses is shown to exhibit a pattern familiar from the lattice. Furthermore, we find the dissociation temperature of mesons as a function of their spin, showing that at a fixed quark mass, mesons with larger spins dissociate at lower temperatures. The Goldstone bosons associated with chiral symmetry breaking are shown to disappear above the chiral symmetry restoration temperature. Finally, we show that holographic consideration imply that large-spin mesons do not experience drag effects when moving through the quark gluon plasma. They do, however, have a maximum velocity for fixed spin, beyond which they dissociate.
description: 25 pages, 23 figures; v2: emphasised dependence of interquark distance on velocity, added plot, added references; v3: error in section V corrected, conclusions unchanged
Isoforma fritilla OPITZ 2015, nov. sp.
Creators: name: Opitz, Weston
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Cleridae
Isoforma
Isoforma fritilla

description: Isoforma fritilla OPITZ nov. sp.
(Figs 70, 155, 175)
Holotype: ♀. Piste de Belizon pk 12, 1 Marz 1987, Guyane (French Guiana), piégeage lumineux, Henri Cevaer (FSCA).
Diagnosis: The holotype has two testaceous fascias on the elytral disc. To date, this is unique in the genus.
Description: Size: Length 15.0 mm; width 7.0 mm. Form: As in Fig. 155. Color: Cranium mostly testaceous, epicranium and venter brown; pronotum mostly black, upper sides of disc testaceous; elytral disc mostly black, with basal and medial testaceous fasciae. Head: Antennal capitulum very long (Fig. 70), each capitular antennomere longer than funicle; antennal carina very prominent; EW/FW 25/35. Thorax: Pronotal anterior margin linear, not projected at middle; side margins of disc rounded at middle; PW/PL 108/85; elytra conspicuously flared; discal carinae faintly developed; EL/EW 400/110. Abdomen: Female pygidium not incised at distal margin.
Natural history: The holotype was collected in March.
Distribution (Fig. 175): Known only from the type locality.
Etymology: The trivial name fritilla is a Latin adjective derived from fritillus (= spotted). I refer to the black macula on the elytral disc.
description: Published as part of Opitz, Weston, 2015, Systematics of the checkered beetle subfamily Platynopterinae SPINOLA (Coleoptera Cleridae), pp. 1513-1572 in Linzer biologische Beiträge 47 (2) on page 1537, DOI: 10.5281/zenodo.5282503
LOCx2-130, a low-power, low-latency, 2 x 4.8-Gbps serializer ASIC for detector front-end readout
Creators: name: Xiao, Le
name: Sun, Quan
name: Gong, Datao
name: Baker, Emily
name: Deng, Binwei
name: Guo, Di
name: He, Huiqin
name: Hou, Suen
name: Liu, Chonghan
name: Liu, Tiankuan
name: Thomas, James
name: Wang, Jian
name: Xiang, Annie C.
name: Yang, Dongxu
name: Ye, Jingbo
name: Zhao, Xiandong
name: Zhou, Wei
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: In this paper, we present the design and test results of LOCx2-130, a low-power, low-latency, dual-channel transmitter ASIC for detector front-end readout. LOCx2-130 has two channels of encoders and serializers, and each channel operates at 4.8 Gbps. LOCx2-130 can interface with three types of ADCs, an ASIC ADC and two COTS ADCs. LOCx2-130 is fabricated in a commercial 130-nm CMOS technology and is packaged in a 100-pin QFN package. LOCx2-130 consumes 440 mW and achieves a latency of less than 40.7 ns.
description: 16 pages, 14 figures