cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Myotis capaccinii
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis capaccinii

description: Myotis capaccinii (Bonaparte, 1837). Fauna Ital., 1, fasc. 20. TYPE LOCALITY: Italy, Sicily. DISTRIBUTION: Mediterranean zone and islands of Europe and N.W. Africa; S. Asia Minor; Israel; S. Iraq; S. Iran; Uzbekistan (U.S. S. R.). COMMENT: See comment under macrodactylus. ISIS NUMBER: 5301405014014015001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 185, DOI: 10.5281/zenodo.7352990
Superconductivity in CeOBiS2 with cerium valence fluctuation
Creators: name: Nagao, Masanori
name: Miura, Akira
name: Ueta, Ikuo
name: Watauchi, Satoshi
name: Tanaka, Isao
Publisher: name: arXiv
Year: 2016
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Resistivities of single-crystalline as well as poly-crystalline samples of CeOBiS2 without fluorine doping were measured at temperatures down to 0.13 K, and were compared with those of poly-crystalline LaOBiS2 and PrOBiS2. Both poly-crystalline and single-crystalline CeOBiS2 exhibited zero resistivity below 1.2 K while poly-crystalline LaOBiS2 and PrOBiS2 did not show zero resistivity down to 0.13 K. Superconducting transition temperature of CeOBiS2 was reduced by increasing the applied current density. The superconductivity of CeOBiS2 without chemical doping is likely triggered by the carriers induced by the valence fluctuation between Ce3+ and Ce4+.
description: 19 pages, 5 figures in Solid State Communications 2016
Myotis dasycneme
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis dasycneme

description: Myotis dasycneme (Boie, 1825). Isis Jena, p. 1200. TYPE LOCALITY: Denmark, Jutland, Dagbieg (near Wiborg). DISTRIBUTION: N.E. Europe and W. Siberia, west to E. France and Switzerland, east to Yenesei River, south to Austria and N.W. Kazakhstan (U.S. S.R.); single record from Manchuria. COMMENT: Probably includes surinamensis; see Carter and Dolan, 1978, Spec. Publ. Mus. Texas Tech Univ., 15:73. ISIS NUMBER: 5301405014014017001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
description: {"references": ["Carter, D. C., and P. G. Dolan. 1978. Catalog of type specimens of Neotropical bats in selected European museums. Special Publications, The Museum, Texas Tech University Press, 15: 1 - 136."]}
Myotis cobanensis Goodwin 1955
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis cobanensis

description: Myotis cobanensis Goodwin, 1955. Am. Mus. Novit., 1744:2. TYPE LOCALITY: Guatemala, Alta Verapaz, Coban, 1305 m. DISTRIBUTION: C. Guatemala. COMMENT: Listed as a subspecies of velifer by Goodwin, 1955, Am. Mus. Novit., 1744:2; but see de la Torre, 1958, Proc. Biol. Soc. Wash., 71: 167-170; Hall, 1981: 197. Known only from the holotype.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
description: {"references": ["de la Torre, L. 1958. The status of the bat Myotis velifer cobanensis Goodwin. Proceedings of the Biological Society of Washington, 71: 167 - 170.", "Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
Local stability conditions and calibrating procedure for new car-following models used in driving simulators
Creators: name: Kurtc, Valentina
name: Anufriev, Igor
Publisher: name: arXiv
Year: 2016
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: The Intelligent Driver Model is studied and several drawbacks with respect to driving simulators are defined. We present two modifications of the IDM. The first one gives any predefined distance to the leading vehicle in a steady state. The second modification is a combination of the first one and the optimal velocity model. It takes into account drivers reaction time explicitly and is described by delay differential equation. This model always results in realistic vehicles accelerations what allows simulating real traffic collisions. Necessary and sufficient conditions are obtained, that guarantee a non-oscillating solution near the equilibrium for the vehicle platoon. We suggest the calibrating framework based on a numerical solution of the constrained optimization problem. Nonlinear constraints are generated by the numerical integration scheme. The suggested procedure incorporates the local stability conditions obtained and takes into account vehicle dynamics, drivers behavior and weather conditions.
description: 9 pages, 4 figures, contribution to the conference Traffic and Granular Flow '13 in Juelich. It is included in the Conference proceedings (Springer)
Magnetophonon oscillations of thermoelectric power and combined resonance in two-subband electron systems
Creators: name: Levin, A. D.
name: Gusev, G. M.
name: Raichev, O. E.
name: Bakarov, A. K.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: By measuring the thermoelectric effect in high-mobility quantum wells with two occupied subbands in perpendicular magnetic field, we detect magnetophonon oscillations due to interaction of electrons with acoustic phonons. These oscillations contain specific features identified as combined resonances caused by intersubband phonon-assisted transitions of electrons in the presence of Landau quantization. The quantum theory of phonon-drag magnetothermoelectric effect, generalized to the case of multi-subband occupation, describes our experimental findings.
description: 7 pages, 6 figures
Panchromatic Hubble Andromeda Treasury XVI. Star Cluster Formation Efficiency and the Clustered Fraction of Young Stars
Creators: name: Johnson, L. Clifton
name: Seth, Anil C.
name: Dalcanton, Julianne J.
name: Beerman, Lori C.
name: Fouesneau, Morgan
name: Lewis, Alexia R.
name: Weisz, Daniel R.
name: Williams, Benjamin F.
name: Bell, Eric F.
name: Dolphin, Andrew E.
name: Larsen, Søren S.
name: Sandstrom, Karin
name: Skillman, Evan D.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use the Panchromatic Hubble Andromeda Treasury (PHAT) survey dataset to perform spatially resolved measurements of star cluster formation efficiency ($Γ$), the fraction of stellar mass formed in long-lived star clusters. We use robust star formation history and cluster parameter constraints, obtained through color-magnitude diagram analysis of resolved stellar populations, to study Andromeda's cluster and field populations over the last $\sim$300 Myr. We measure $Γ$ of 4-8% for young, 10-100 Myr old populations in M31. We find that cluster formation efficiency varies systematically across the M31 disk, consistent with variations in mid-plane pressure. These $Γ$ measurements expand the range of well-studied galactic environments, providing precise constraints in an HI-dominated, low intensity star formation environment. Spatially resolved results from M31 are broadly consistent with previous trends observed on galaxy-integrated scales, where $Γ$ increases with increasing star formation rate surface density ($Σ_{\mathrm{SFR}}$). However, we can explain observed scatter in the relation and attain better agreement between observations and theoretical models if we account for environmental variations in gas depletion time ($τ_{\mathrm{dep}}$) when modeling $Γ$, accounting for the qualitative shift in star formation behavior when transitioning from a H$_2$-dominated to a HI-dominated interstellar medium. We also demonstrate that $Γ$ measurements in high $Σ_{\mathrm{SFR}}$ starburst systems are well-explained by $τ_{\mathrm{dep}}$-dependent fiducial $Γ$ models.
description: 26 pages, 13 figures, Accepted by ApJ
Myotis chiloensis
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis chiloensis

description: Myotis chiloensis (Waterhouse, 1840). Zool. Voy. H.M.S. "Beagle," Mammalia, p. 5. TYPE LOCALITY: Chile, Chiloe Isl., Islets on eastern side. DISTRIBUTION: C. and S. Chile. COMMENT: See LaVal, 1973, Bull. Los Ang. Cty. Mus. Nat. Hist. Sci. Soc., 15:43, 44, for restriction of the scope of this species. ISIS NUMBER: 5301405014014016001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 185, DOI: 10.5281/zenodo.7352990
Curriculum development, implementation and evaluation for first aid
Creators: name: Anker, Ron L.
Publisher: name: Monash University
Year: 2022

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Myotis chinensis
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis chinensis

description: Myotis chinensis (Tomes, 1857). Proc. Zool. Soc. Lond., 1857:52. TYPE LOCALITY: "Southern China ". DISTRIBUTION: Szechwan and Yunnan to Kiangsu (China); Hong Kong; N. Thailand. COMMENT: Included in myotis by Ellerman and Morrison-Scott, 1951:144; but also see Lekagul and McNeely, 1977:206.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
description: {"references": ["Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Lekagul, B., and J. A. McNeely. 1977. Mammals of Thailand. Association for the Conservation of Wildlife, Sahakarnbhat Co., Bangkok, 758 pp."]}
Two-step homogeneous geodesics in homogeneous spaces
Creators: name: Arvanitoyeorgos, Andreas
name: Souris, Nikolaos Panagiotis
Publisher: name: arXiv
Year: 2016
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C25, 53C30

description: We study geodesics of the form $γ(t)=π(\exp(tX)\exp(tY))$, $X,Y\in \fr{g}=\operatorname{Lie}(G)$, in homogeneous spaces $G/K$, where $π:G\rightarrow G/K$ is the natural projection. These curves naturally generalise homogeneous geodesics, that is orbits of one-parameter subgroups of $G$ (i.e. $γ(t)=π(\exp (tX))$, $X\in \fr{g}$). We obtain sufficient conditions on a homogeneous space implying the existence of such geodesics for $X,Y\in \fr{m}=T_o(G/K)$. We use these conditions to obtain examples of Riemannian homogeneous spaces $G/K$ so that all geodesics of $G/K$ are of the above form. These include total spaces of homogeneous Riemannian submersions endowed with one parameter families of fiber bundle metrics, Lie groups endowed with special one parameter families of left-invariant metrics, generalised Wallach spaces, generalized flag manifolds, and $k$-symmetric spaces with $k$-even, equipped with certain one-parameter families of invariant metrics.
description: 18 pages
Nucleon structure functions in noncommutative space-time
Creators: name: Rafiei, Ali
name: Rezaei, Zahra
name: Mirjalili, Abolfazl
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the context of noncommutative space-time, we investigate the nucleon structure functions which plays an important role to identify the internal structure of nucleons. We use the corrected vertices and employ new vertices that appear in two approaches of noncommutativity and calculate the proton structure functions in terms of noncommutative tensor θ_{μν}. To check our result, we plot the nucleon structure function (NSF), F_2(x), and compare it with experimental data and the result coming out from the GRV, GJR and CT10 parametrization models. We show that new vertex which is arising the noncommutativity correction will lead us to better consistency between theoretical result and experimental data for NSF. This consistency would be better at small values of x-Bjorken variable. To indicate and confirm the validity of our calculations, we also act conversely and obtain an lower bound for the numerical values of Λ_{NC} scale which are corresponding to the recent reports.
description: 28 pages, 5 figuree
Myotis daubentoni
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis daubentoni

description: Myotis daubentoni (Kuhl, 1819). Ann. Wetterau Ges. Naturk., 4(2): 195. TYPE LOCALITY: Germany, Hessen, Hanau. DISTRIBUTION: Europe and S. Siberia, east to Kamtschatka, Vladivostok, Sakhalin (U.S. S.R.); Korea; Manchuria, E., S. China (SW); Britain and Ireland; S. Scandinavia; Assam (India). COMMENT: Includes laniger; see Ellerman and Morrison-Scott, 1951:147. ISIS NUMBER: 5301405014014018001 as M. daubentoni. 5301405014014035001 as M. laniger.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
description: {"references": ["Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp."]}
Spatially Resolved Spectroscopy of Sub-mm Galaxies at z~2
Creators: name: Olivares, V.
name: Treister, E.
name: Privon, G. C.
name: Alaghband-Zadeh, S.
name: Casey, Caitlin M.
name: Schawinski, K.
name: Kurczynski, P.
name: Gawiser, E.
name: Nagar, N.
name: Chapman, S.
name: Bauer, F. E.
name: Sanders, D.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present near-infrared integral-field spectroscopic observations targeting H$α$ in eight sub-millimeter galaxies (SMGs) at $z$=1.3-2.5 using VLT/SINFONI, obtaining significant detections for six of them. The star formation rates derived from the H$α$ emission are $\sim$100 M$_\odot$yr$^{-1}$, which account for only $\sim$ 20-30\% of the infrared-derived values, thus suggesting that these systems are very dusty. Two of these systems present [NII]/H$α$ ratios indicative of the presence of an Active Galactic Nucleus (AGN). We mapped the spatial distribution and kinematics of the star forming regions in these galaxies on kpc-scales. In general, the H$α$ morphologies tend to be highly irregular and/or clumpy, showing spatial extents of $\sim$3-11~kpc. We find evidence for significant spatial offsets, of $\sim$0.1-0.4$"$ or 1.2-3.4 kpc, between the H$α$ and the continuum emission in three of the sources. Performing a kinemetry analysis we conclude that the majority of the sample is not consistent with disk-like rotation-dominated kinematics. Instead, they tend to show irregular and/or clumpy and turbulent velocity and velocity dispersion fields. This can be interpreted as evidence for scenario in which these extreme star formation episodes are triggered by galaxy-galaxy interactions and major mergers. In contrast to recent results for SMGs, these sources appear to follow the same relations between gas and star forming rate densities as less luminous and/or normal star forming galaxies.
description: Astrophysical Journal, accepted. 17 page in emulateapj format, 6 figures
Myotis dryas K. Andersen 1907
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis dryas

description: Myotis dryas K. Andersen, 1907. Ann. Mus. Civ. Stor. Nat. Genova, 3: 33. TYPE LOCALITY: India, Andaman Isis., South Andaman Isl., Port Blair. DISTRIBUTION: Andaman Isis. COMMENT: Listed as a subspecies of adversus by Ellerman and Morrison-Scott, 1951:149; but also see Hill, 1976, J. Bombay Nat. Hist. Soc., 73:436.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
description: {"references": ["Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Hill, J. E. 1976. Bats referred to Hesperoptenus Peters, 1869 (Chiroptera: Vespertilionidae) with the description of a new subgenus. Bulletin of the British Museum (Natural History), Zoology Series, 30: 1 - 28."]}
Ensemble master equation for a trapped-atom clock with one- and two-body losses
Creators: name: Ivannikov, Valentin
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: An ensemble density matrix model that includes one- and two-body losses is derived for a trapped-atom clock. A trapped-atom clock is mainly affected by one- and two-body losses, generally giving nonexponential decays of populations; nevertheless, three-body recombination is also quantitatively analyzed to demonstrate the boundaries of its practical relevance. The importance of one-body losses is highlighted without which population trapping behavior would be observed. The model is written with decay constants expressed through experimental parameters. It can complement, e.g., the ISRE (identical spin rotation effect) model to improve its predictions: ISRE dramatically increases the ensemble coherence time, hence it enables one to observe the influence of two-body losses on the interferometry contrast envelope. The presented model is useful for Ramsey interferometry and is ready for immediate experimental verification in existing systems.
The Neutral Excitations in the Gaffnian State
Creators: name: Kang, Byungmin
name: Moore, Joel E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study a model fractional quantum Hall (FQH) wavefunction called the Gaffnian state, which is believed to represent a gapless, strongly correlated state that is very different from conventional metals. To understand this exotic gapless state better, we provide a representation based on work of Halperin in which the pairing structure of the Gaffnian state becomes more explicit. We employ the single-mode approximation introduced by Girvin, MacDonald, and Platzman (GMP), here extended to three-body interactions, in order to treat a neutral collective exitation mode in order to clarify the physical origin of the gaplessness of the Gaffnian state. We discuss approaches to extract systematically the relevant physics in the long-distance, large-electron-number limit of FQH states using numerical calculations with relatively few electrons. In an appendix, we provide second quantized expressions for many-body Haldane pseudopotentials in various geometries including the plane, sphere, cylinder, and the torus based on the proper definition of the relative angular momentum.
description: 8 pages + 16 pages of appendices, 4 figures
Modeling the source of GW150914 with targeted numerical-relativity simulations
Creators: name: Lovelace, Geoffrey
name: Lousto, Carlos O.
name: Healy, James
name: Scheel, Mark A.
name: Garcia, Alyssa
name: O'Shaughnessy, Richard
name: Boyle, Michael
name: Campanelli, Manuela
name: Hemberger, Daniel A.
name: Kidder, Lawrence E.
name: Pfeiffer, Harald P.
name: Szilagyi, Bela
name: Teukolsky, Saul A.
name: Zlochower, Yosef
Publisher: name: arXiv
Year: 2016
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In fall of 2015, the two LIGO detectors measured the gravitational wave signal GW150914, which originated from a pair of merging black holes. In the final 0.2 seconds (about 8 gravitational-wave cycles) before the amplitude reached its maximum, the observed signal swept up in amplitude and frequency, from 35 Hz to 150 Hz. The theoretical gravitational-wave signal for merging black holes, as predicted by general relativity, can be computed only by full numerical relativity, because analytic approximations fail near the time of merger. Moreover, the nearly-equal masses, moderate spins, and small number of orbits of GW150914 are especially straightforward and efficient to simulate with modern numerical-relativity codes. In this paper, we report the modeling of GW150914 with numerical-relativity simulations, using black-hole masses and spins consistent with those inferred from LIGO's measurement. In particular, we employ two independent numerical-relativity codes that use completely different analytical and numerical methods to model the same merging black holes and to compute the emitted gravitational waveform; we find excellent agreement between the waveforms produced by the two independent codes. These results demonstrate the validity, impact, and potential of current and future studies using rapid-response, targeted numerical-relativity simulations for better understanding gravitational-wave observations.
description: 11 pages, 3 figures, submitted to Classical and Quantum Gravity
Probing seismic solar analogues through observations with the NASA Kepler space telescope and HERMES high-resolution spectrograph
Creators: name: Beck, P. G.
name: Salabert, D.
name: García, R. A.
name: Nascimento,, J. do
name: Duarte, T. S. S.
name: Mathis, S.
name: Regulo, C.
name: Ballot, J.
name: Egeland, R.
name: Castro, M.
name: Pérez-Herńandez, F.
name: Creevey, O.
name: Tkachenko, A.
name: van Reeth, T.
name: Bigot, L.
name: Corsaro, E.
name: Metcalfe, T.
name: Mathur, S.
name: Palle, P. L.
name: Prieto, C. Allende
name: Montes, D.
name: Johnston, C.
name: Andersen, M. F.
name: van Winckel, H.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Stars similar to the Sun, known as solar analogues, provide an excellent opportunity to study the preceding and following evolutionary phases of our host star. The unprecedented quality of photometric data collected by the \Kepler NASA mission allows us to characterise solar-like stars through asteroseismology and study diagnostics of stellar evolution, such as variation of magnetic activity, rotation and the surface lithium abundance. In this project, presented in a series of papers by Salabert et al. (2016a,b) and Beck et al (2016a,b), we investigate the link between stellar activity, rotation, lithium abundance and oscillations in a group of 18 solar-analogue stars through space photometry, obtained with the NASA Kepler space telescope and from currently 50+ hours of ground-based, high-resolution spectroscopy with the Hermes instrument. In these proceedings, we first discuss the selection of the stars in the sample, observations and calibrations and then summarise the main results of the project. By investigating the chromospheric and photospheric activity of the solar analogues in this sample, it was shown that for a large fraction of these stars the measured activity levels are compatible to levels of the 11-year solar activity cycle 23. A clear correlation between the lithium abundance and surface rotation was found for rotation periods shorter than the solar value. Comparing the lithium abundance measured in the solar analogues to evolutionary models with the Toulouse-Geneva Evolutionary Code (TGEC), we found that the solar models calibrated to the Sun also correctly describe the set of solar/stellar analogs showing that they share the same internal mixing physics. Finally, the star KIC 3241581 and KIC 10644353 are discussed in more detail.
description: Proceedings of "The 19th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun"; 8 pages, 4 Figures
Intrinsic optical fibre sensing based on integrated mode division multiplexing
Creators: name: Ross-Adams, Andrew J.
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: This study addresses a significant deficiency; the absence of integrated solutions to real-time fiber integrity monitoring and intrusion detection. An optimized solution to this problem which is both practical and scalable is highly coveted. Our approach to providing such a solution is to use the femtosecond laser direct-write (FLDW) process for the fabrication of novel optical waveguide circuits and the creation of an integrated hybrid-wavelength optical fiber sensing platform based on spatial mode-division multiplexing which is capable of operating across standard single-mode fiber as used in the telecommunications industry.The development of integrated, parametric implementations of optical spatial-division multiplexing and fiber sensing mechanisms is a key step towards maturation of the photonics industry. This thesis reports on the design, simulation and fabrication of integrated optical code division multiplexers capable of performing higher order mode sensing in industry standard G.652 single-mode optical fiber. The efficacy of this sensing platform was verified via the demonstration of a novel, intrinsic optical fiber torsion sensor based on intra-modal cross-talk, capable of augmenting existing fiber integrity monitoring techniques. Further-more, the successful application of this technique to single-mode fiber unlocks the potentialfor exploiting optical fiber telecoms infrastructure for large scale distributed sensing.
Myotis emarginatus
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis emarginatus

description: Myotis emarginatus (E. Geoffroy, 1806). Ann. Mus. Hist. Nat. Paris, 8: 198. TYPE LOCALITY: France, Ardennes, Givet, Charlemont. DISTRIBUTION: S. Europe, north to Netherlands and S. Poland, Crimea, Caucasus, Kopet Dag, east to Uzbekistan (U.S. S.R.) and E. Iran; Israel; Morocco; Algeria; Tunisia; Lebanon; Afghanistan. ISIS NUMBER: 5301405014014021001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
Inferring the interplanetary dust properties from remote observations and simulations
Creators: name: Lasue, Jeremie
name: Levasseur-Regourd, Anny-Chantal
name: Fray, Nicolas
name: Cottin, Hervé
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Since in situ studies and interplanetary dust collections only provide a spatially limited amount of information about the interplanetary dust properties, it is of major importance to complete these studies with properties inferred from remote observations of light scattered and emitted, with interpretation through simulations. Physical properties of the interplanetary dust in the near-ecliptic symmetry surface, such as the local polarization, temperature and composition, together with their heliocentric variations, may be derived from scattered and emitted light observations, giving clues to the respective contribution of the particles sources. A model of light scattering by a cloud of solid particles constituted by spheroidal grains and aggregates thereof is used to interpret the local light scattering data. Equilibrium temperature of the same particles allows us to interpret the temperature heliocentric variations. A good fit of the local polarization phase curve, $P_α$, near 1.5~AU from the Sun is obtained for a mixture of silicates and more absorbing organics material ($\approx$40 % in mass) and for a realistic size distribution typical of the interplanetary dust in the 0.2 to 200 micrometre size range. The contribution of dust particles of cometary origin is at least 20% in mass. The same size distribution of particles gives a solar distance, $R$, dependence of the temperature in $R^{-0.45}$ different than the typical black body behavior. The heliocentric dependence of $P_{α=90°}$ is interpreted as a progressive disappearance of solid organics (such as HCN polymers or amorphous carbon) towards the Sun.
description: 10 pages, 9 figures, 1 table
Femtosecond laser-written integrated components for future all-fibre mid-infrared laser systems
Creators: name: Bharathan, Gayathri
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Lasers emitting at mid-infrared (mid-IR) wavelengths in the 2.5-5 µm range are essential for various applications as this spectral region coincides with the vibrational-rotational absorption lines of many important atmospheric gases and liquid water. Fibre lasers are an efficient way to generate light at mid-IR wavelengths. However, mid-IR fibre laser technology is still in its infancy, mainly due to the non-existence of fibre coupled optical components to create all-fibre cavities, which severely limits their practical applications. This thesis investigates the feasibility of using a femtosecond laser to fabricate integrated components such as fibre Bragg gratings (FBGs), couplers and splitters which can add a new perspective for mid-IR all-fibre lasers. We report the development of a widely tunable (37 nm) all-fibre mid-IR laser based on a mechanically robust FBG which was inscribed through the polymer coating of a double clad fluoride fibre by focusing femtosecond laser pulses into the core of the fibre without the use of a phase mask. In a further step, the possibility of using on-chip optical couplers inscribed in fluoride and chalcogenide glasses is also investigated to pave the way for the realization of compact and robust mid-IR fibre laser systems for real-world applications in spectroscopy and medicine.
Rule Extraction Algorithm for Deep Neural Networks: A Review
Creators: name: Hailesilassie, Tameru
Publisher: name: arXiv
Year: 2016
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Despite the highest classification accuracy in wide varieties of application areas, artificial neural network has one disadvantage. The way this Network comes to a decision is not easily comprehensible. The lack of explanation ability reduces the acceptability of neural network in data mining and decision system. This drawback is the reason why researchers have proposed many rule extraction algorithms to solve the problem. Recently, Deep Neural Network (DNN) is achieving a profound result over the standard neural network for classification and recognition problems. It is a hot machine learning area proven both useful and innovative. This paper has thoroughly reviewed various rule extraction algorithms, considering the classification scheme: decompositional, pedagogical, and eclectics. It also presents the evaluation of these algorithms based on the neural network structure with which the algorithm is intended to work. The main contribution of this review is to show that there is a limited study of rule extraction algorithm from DNN.
description: 6 pages,2 figures,IEEE Publication format, Keywords- Artificial neural network; Deep neural network; Rule extraction; Decompositional; Pedagogical; Eclectic
Randall-Sundrum brane-world in modified gravity
Creators: name: Nakada, Hiroshi
name: Ketov, Sergei V.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We modify Randall-Sundrum model of brane-world (with two branes) by adding the scalar curvature squared term in five dimensions. We find that it does not destabilize Randall-Sundrum solution to the hierarchy problem of the Standard Model in particle physics.
description: 9 pages, 3 figures, LaTeX2e
Myotis evotis
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis evotis

description: Myotis evotis (H. Allen, 1864). Smithson. Misc. Coll., 7:48. TYPE LOCALITY: U.S.A., California, Monterey. DISTRIBUTION: S. British Columbia, S. Alberta, S. Saskatchewan (Canada) to W. New Mexico and S. California (U.S.A.); Baja California (Mexico). COMMENT: See Genoways and Jones, 1969, Southwest. Nat., 14:1. This species is in need of revision (BVR). ISIS NUMBER: 5301405014014022001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
Case study of new product development in a multinational technology manufacturing company collaborating online across offices in Europe and Asia
Creators: name: Chan, CL
Publisher: name: CQUniversity
Year: 2024
Subjects: classificationCode: 350602
subject: Consumer-oriented product or service development

description: "A multi-year case study examined new product development (NPD) processes in a multinational corporation (MNC) that spanned three continental regions: Europe, Asia-Pacific and USA. The MNC designs and produces display/monitoring systems used by the military, news broadcasters, the TV entertainment industry, and movie producers. NPD was known to be risky with a high failure rate, as cited in the existing literature, and recently observed at the case study MNC"--Abstract.
The host galaxies and possible progenitors of fast radio bursts
Creators: name: Marnoch, Lachlan
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Fast radio bursts (FRBs) are millisecond-scale radio pulses from extragalactic sources, the origin of which remains mysterious. This is partially because of the difficulty in localising FRBs to host galaxies, previously achieved only with the repeating source FRB 121102. Now, the Commensal Real-time ASKAP Fast Transients (CRAFT) survey has traced several FRBs to their hosts. These localisations provide the opportunity to study the host galaxies at a range of wavelengths, which will shed light on FRB source environments, and, in the future, the nature of their progenitors. This work focuses on optical follow-up of CRAFT fast radio bursts using Very Large Telescope imaging. Photometric measurements of five host galaxies are performed, and their nature discussed. Four FRB hosts are examined, using the method of direct subtraction of two epochs, for supernova-like optical counterparts to the FRBs. None are identified. Limits are placed on the brightness of any associated transients, and a Monte Carlo approach is used to estimate the probability of a supernova associated with each FRB going undetected. It is found that Type Ia and IIn supernovae are unlikely to accompany all FRBs. Implications for FRB progenitor models are discussed.
Myotis elegans Hall 1962
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis elegans

description: Myotis elegans Hall, 1962. Univ. Kans. Publ. Mus. Nat. Hist., 14: 163 -164. TYPE LOCALITY: Mexico, Veracruz, 12.5 mi. (20 km) N. Tihuatlan. DISTRIBUTION: San Luis Potosi (Mexico) to Costa Rica. ISIS NUMBER: 5301405014014020001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
Myotis dominicensis Miller 1902
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis dominicensis

description: Myotis dominicensis Miller, 1902. Proc. Biol. Soc. Wash., 15: 243. TYPE LOCALITY: Dominica (Lesser Antilles). DISTRIBUTION: N. Lesser Antilles. COMMENT: Listed as a subspecies of nigricans by Hall and Kelson, 1959:176, but see LaVal, 1973, Bull. Los Ang. Cty. Mus. Nat. Hist. Sei. Soc., 15: 16, 17; Hall, 1981:200.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 186, DOI: 10.5281/zenodo.7352990
description: {"references": ["Hall, E. R., and K. R. Kelson. 1959. The mammals of North America. Ronald Press Co., New York, 1: 1 - 546; 2: 547 - 1083 + 79.", "Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
Galactoseismology in the GAIA Era
Creators: name: Chakrabarti, Sukanya
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The GAIA satellite will provide unprecedented phase-space information for our Galaxy and enable a new era of Galactic dynamics. We may soon see successful realizations of Galactoseismology, i.e., inferring the characteristics of the Galactic potential and sub-structure from a dynamical analysis of observed perturbations in the gas or stellar disk of the Milky Way. Here, we argue that to maximally take advantage of the GAIA data and other complementary surveys, it is necessary to build comprehensive models for both the stars and the gas. We outline several key morphological puzzles of the Galactic disk and proposed solutions that may soon be tested.
description: 3 pages, 1 figure, proceedings for Galaxy Outskirts conference
Interview with Tony Correia
Creators: name: HIV In My Day
Publisher: name: University of Victoria Libraries
Year: 2021
Subjects: Correia, Tony
Stigma & Discrimination
Caregiving
Death & Loss
Gay Community

description: An interview with Tony Correia as part of the HIV in My Day Oral History project. Interviewer: Ben Klassen. Location: Vancouver (Momentum).
Myotis fortidens Miller and Allen 1928
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis fortidens

description: Myotis fortidens Miller and Allen, 1928. Bull. U.S. Nat. Mus., 144:54. TYPE LOCALITY: Mexico, Tabasco, Teapa. DISTRIBUTION: Sonora (Mexico) to Guatemala. W. Texas (U.S. A.) (NS). ISIS NUMBER: 5301405014014024001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 187, DOI: 10.5281/zenodo.7352990
EFFECTS OF INLET CONDITIONS, TURBINE DESIGN, AND NON-FLAT TOPOGRAPHY ON THE WAKE OF SCALED-DOWN WIND TURBINES
Creators: name: Alvarado, Diego Andres Siguenza
Publisher: name: Purdue University Graduate School
Year: 2023
Subjects: Mechanical engineering not elsewhere classified
Turbulent flows

description: This work is a five-article-based collection of published and to-be-published research articles that explore a novel combination of inlet conditions, wind turbine design, and non-flat topography by performing scaled-down experiments in a wind tunnel.
Myotis goudoti
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis goudoti

description: Myotis goudoti (A. Smith, 1834). S. Afr. Quart. J., 2: 244. TYPE LOCALITY: Madagascar. DISTRIBUTION: Madagascar; Anjouan Isl. (Comoro Isis.). ISIS NUMBER: 5301405014014026001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 187, DOI: 10.5281/zenodo.7352990
Sensitivity of the Fe K-alpha Compton shoulder to the geometry and variability of the X-ray illumination of cosmic objects
Creators: name: Odaka, Hirokazu
name: Yoneda, Hiroki
name: Takahashi, Tadayuki
name: Fabian, Andrew
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In an X-ray reflection spectrum, a tail-like spectral feature generated via Compton down-scattering, known as a Compton shoulder (CS), appears at the low-energy side of the iron K$α$ line. Despite its great diagnostic potential, its use as a spectral probe of the reflector has been seriously limited due to observational difficulties and modelling complexities. We revisit the basic nature of the CS by systematic investigation into its dependence on spatial and temporal parameters. The calculations are performed by Monte-Carlo simulations for sphere and slab geometries. The dependence is obtained in a two-dimensional space of column density and metal abundance, demonstrating that the CS solves parameter degeneration between them which was seen in conventional spectral analysis using photoelectric absorption and fluorescence lines. Unlike the iron line, the CS does not suffer from any observational dependence on the spectral hardness. The CS profile is highly dependent on the inclination angle of the slab geometry unless the slab is Compton-thick, and the time evolution of the CS is shown to be useful to constrain temporal information on the source if the intrinsic radiation is variable. We also discuss how atomic binding of the scattering electrons in cold matter blurs the CS profile, finding that the effect is practically similar to thermal broadening in a plasma with a moderate temperature of $\sim$5 eV. Spectral diagnostics using the CS is demonstrated with grating data of X-ray binary GX 301$-$2, and will be available in future with high-resolution spectra of active galactic nuclei obtained by microcalorimeters.
description: 16 pages, 20 figures, accepted for publication in MNRAS
Myotis findleyi Bogan 1978
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Vespertilionidae
Myotis
Myotis findleyi

description: Myotis findleyi Bogan, 1978. J. Mammal., 59: 524. TYPE LOCALITY: Mexico, Nayarit, Très Marias Isis., Maria Magdalena Isl. DISTRIBUTION: Très Marias Isis. COMMENT: Very close to and possibly conspecific with nigricans (KFK).
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Chiroptera, pp. 111-215 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 187, DOI: 10.5281/zenodo.7352990
A comparison of immigration growth and fertility growth as alternative solutions to Australia's ageing population problem
Creators: name: Reeve, Rebecca
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: The combined effects of the post World War Two 'baby boomers' approaching retirement age and a decreasing fertility rate is predicted to cause Australia's worker ratio to increase from 2011. This raises the policy issue of how future tax revenue can be generated to finance the increase in social expenditure necessary to support theincreasing number of dependents. This paper explores fertility growth and immigration growth as alternative policy options to increase the size of the future labour force. Inaddition to exploring the impacts on employment of these alternative policies, theimpact on various other economic variables is investigated. -- The increase in skilled immigration under recent immigration policy changes is found to improve employment outcomes for recently arrived new-immigrants relative to thosewho arrived prior to the policy changes. A logit analysis of the second Longitudinal Survey of Immigration to Australia data reveals that the probability of employment forless-skilled immigrants is significantly related to post-secondary education, Australian qualifications and English language skills. The future employment rate of new immigrants is predicted to increase as less-skilled immigrants who invest in educationpost-arrival enter the labour force. -- Forecasts generated using the Murphy Model (MM2) for various demographic scenarios reveal that gradually increasing immigration levels from 2010 produces a more favourable worker ratio than alternative scenarios. Economic forecasts at 2011 indicate that, in addition to increasing the worker ratio, gradually increasing immigration impacts positively on other economic indicators. Gradually increasing immigration increases labour productivity, is non-inflationary, increases per capita consumption, reduces the income gap, and increases income for the pre-immigration population. Unemployment is marginally increased in the medium-term, as is the ratio of the current account deficit to GDP. However, as productivity and GDP increase overtime, unemployment and the ratio of the current account deficit to GDP are expected to decrease.