cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Iris susiana Linnaeus 1753
Creators: name: Altinordu, Fahim
name: Crespo, Manuel B.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Asparagales
Iridaceae
Iris
Iris susiana

description: 1. Iris susiana Linnaeus (1753: 38)
 Type (lectotype, designated here):—Herb. Linnaeus No. 61.3 (LINN [photo!]).
 The protologue of Iris susiana (Linnaeus 1753: 38) consists of a diagnosis “ IRIS corollis barbatis, caule foliis longiore unifloro” with citations from earlier works (Linnaeus 1738: 18, van Royen 1740: 17), followed by one synonym from Bauhin (1623: 31, 1658: 579): “ Iris susiana, flore maximo ex albo nigricante”. Bauhin (1658: 579) provided an illustration (available at http://bibdigital.rjb.csic.es/ing/Libro.php?Libro=3057&Pagina=302) that can be considered original material. Except for this illustration, Jarvis (2007) cited as Linnaeus’s original material one specimen at LINN, Herb. Linn. No. 61.3 (LINN) (image available at: http://linnean-online.org/800/). This specimen bears Linnaeus’s annotation “1 susiana ”, where “1” explicitly refers to the number of the species account of Iris susiana in Species plantarum (Linnaeus 1753). The sheet bears also the abbreviation “ HU ” indicating that the plant was grown in the Uppsala botanical garden.
 Both original elements (the specimen from the Linnaean herbarium and the illustration from Bauhin) are definitely congruent with the traditional and current concept of Iris susiana, keeping in mind that this plant is only known in cultivation and its true origin is unknown (see e.g., Dykes 1912). The specimen Herb. Linnaeus no. 61.3 at LINN is better suited as lectotype of the concerned name, because any specimen is a potential source of additional characters (including molecular, chemical, and micromorphological data) that cannot be provided by an illustration. We therefore designate the specimen in the Linnaean herbarium (LINN) as the lectotype of Iris susiana.
description: Published as part of Altinordu, Fahim & Crespo, Manuel B., 2016, Nomenclatural type designation of four Linnaean names in Iris sensu lato (Iridaceae), pp. 296-300 in Phytotaxa 268 (4) on pages 296-297, DOI: 10.11646/phytotaxa.268.4.9, http://zenodo.org/record/13653621
Generalized geometry and non-symmetric gravity
Creators: name: Jurco, Branislav
name: Khoo, Fech Scen
name: Schupp, Peter
name: Vysoky, Jan
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Generalized geometry provides the framework for a systematic approach to non-symmetric metric gravity theory and naturally leads to an Einstein-Kalb-Ramond gravity theory with totally anti-symmetric contortion. The approach is related to the study of the low-energy effective closed string gravity actions.
description: 6 pages, Proceedings of the 14th Marcel Grossmann Meeting (Rome, July 12-18, 2015); v2: typos in eqns (14) and (15) corrected
Novel Diamond-Slurry Wire Sawing Process for Silicon Wafering
Creators: name: Zarepour, H.
name: Saptaji, K.
name: Subbiah, S.
name: Butler, D.L.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 773-775
description: The photovoltaic industry is shifting from loose SiC slurry-based sawing to fixed diamond-wire sawing
process to improve productivity in the wafering process. While the productivity has improved in sawing, the effect of
this process on the subsequent texturing process is still being studied. One of the known effects of the diamond wire
sawing on the sawn surface is that an amorphous layer of silicon is often seen. This amorphous layer can act as a
mask during the texturing step making it necessary to revise texturing recipes. Here we explore a wire sawing process
that uses loose diamnd slurry for the sawing action instead of the SiC slurry to avoid amorphous silicon formation.
The results of this study demonstrate that slurry-diamond wire sawing can yield a sawn surface without any
amorphous structure which is advantageous to the subsequent texturing process. This advantage not only avoids the
time-consuming etching process required to remove the amorphous layer formed in fixed-diamond abrasive wire
sawing , it is also capable of yielding surface roughness values suitable for desired reflectance which could prevent
additional post-process texturing.
Cost-effectiveness of recruitment and predictors of early withdrawal from a longitudinal interventional study
Creators: name: Garrett, Sinéad.
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.
Silicon Foil Fabrication at Fraunhofer ISE
Creators: name: Drießen, M.
name: Milenkovic, N.
name: Lösel, A.
name: Benick, J.
name: Janz, S.
name: Reber, S.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 747-752
description: Cost reduction is still a major goal in photovoltaic development. Silicon foils offer the possibility to
reduce silicon consumption and with this production costs while maintaining a high efficiency potential. In this work
silicon foils are fabricated by implementation of a release layer in a silicon substrate, reorganization of this layer and
epitaxial thickening prior to detachment. For the formation of the release layer two approaches are investigated,
hydrogen implantation and electrochemical etching of porous silicon. Hydrogen implanted layers reorganize during
heat treatment to layers with low amounts of small pores or with blisters depending on the implantation dose. The
overall amount of pores can be increased by applying several implantation processes. With the more often applied
electrochemically etched porous silicon as release layer the defect density in the foil deposited in a lab-type CVD
reactor could be reduced to (6 ± 2) x 103 cm-2 by optimization of the reorganization process. Effective carrier
lifetimes up to 56 μs are measured. Additionally, 5 x 5 cm2 foils deposited in a continuous CVD reactor are
presented.
Hipposideros cervinus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros cervinus

description: Hipposideros cervinus (Gould, 1863). Mamm. Austr., 3: pl. 34. TYPE LOCALITY: Australia, Queensland, Cape York. DISTRIBUTION: W Malaysia, Sumatra, and the Philippines to Vanuatu (= New Hebrides) and NE Australia. SYNONYMS: batchianensis, celebensis, labuanensis, misoriensis, schneideri. COMMENTS: Considered distinct from galeritus (in which it was formerly included) by Jenkins and Hill (1981).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 171, DOI: 10.5281/zenodo.7353060
description: {"references": ["Jenkins, P. D., and J. E. Hill. 1981. The status of Hipposideros galeritus Cantor, 1846 and Hipposideros cervinus (Gould, 1854) (Chiroptera: Hipposideridae). Bulletin of the British Museum (Natural History), Zoology Series, 415: 279 - 294."]}
Reducing Wafer Surface Saw Damage with Diamond Wire Sawing Technology
Creators: name: Bätzner, D.L.
name: Heiber, J.
name: Lanz, M.
name: Heiniger, C.
name: Debrot, F.
name: Kramer, R.
name: Andreetta, L.
name: Lachenal, D.
name: Frammelsberger, W.
name: Legradic, B.
name: Meixenberger, J.
name: Papet, P.
name: Strahm, B.
name: Wahli, G.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 760-763
description: When processing wafers to solar cells, the surface damage introduced by wafer sawing is
typically removed in the first steps of cell processing. This saw damage removal (SDR) becomes even more
important for cell concepts that need a high surface passivation quality, e.g., the heterojunction solar cells such
as Meyer Burger’s HJT cells that yield Vocs in the range of 740 mV with surface recombination velocities
around 1 cm/s [1,2].
Such surface passivation properties can be used as a sensitive tool to determine the depth of the saw damage
caused by wafer sawing. The advantages of wafering mono crystalline silicon using diamond wires has already
been demonstrated [3] and finds now increasing application amongst commercial wafer suppliers [4]. Mono
crystalline silicon is increasingly wafered with diamond wire sawing. This has not only a cost advantage for the
wafering but allows reducing the saw damage depth considerably. Moving from slurry wafering to diamond wire
wafering will reduce the saw damage depth typically by 20% - 30%. However, by optimising the sawing
parameters for diamond wire wafering, the damage depth can be further reduced up to 50% compared to
traditional slurry wafering. The overall yield can be higher when less saw damage has to be removed, which
becomes especially important when moving towards thinner wafers. It also implies further cost savings on the
cell processing side.
UV and H$α$ HST observations of 6 GASP jellyfish galaxies
Creators: name: Gullieuszik, Marco
name: Giunchi, Eric
name: Poggianti, Bianca M.
name: Moretti, Alessia
name: Scarlata, Claudia
name: Calzetti, Daniela
name: Werle, Ariel
name: Zanella, Anita
name: Radovich, Mario
name: Bellhouse, Callum
name: Bettoni, Daniela
name: Franchetto, Andrea
name: Fritz, Jacopo
name: Jaffé, Yara L.
name: McGee, Sean
name: Mingozzi, Matilde
name: Omizzolo, Alessando
name: Tonnesen, Stephanie
name: Verheijen, Marc
name: Vulcani, Benedetta
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Star-forming, H$α$-emitting clumps are found embedded in the gaseous tails of galaxies undergoing intense ram-pressure stripping in galaxy clusters, so-called jellyfish galaxies. These clumps offer a unique opportunity to study star formation under extreme conditions, in the absence of an underlying disk and embedded within the hot intracluster medium. Yet, a comprehensive, high spatial resolution study of these systems is missing. We obtained UVIS/HST data to observe the first statistical sample of clumps in the tails and disks of six jellyfish galaxies from the GASP survey; we used a combination of broad-band filters and a narrow-band Hα filter. HST observations are needed to study the sizes, stellar masses and ages of the clumps and their clustering hierarchy. These observations will be used to study the clump scaling relations, the universality of the star formation process and verify whether a disk is irrelevant, as hinted by jellyfish galaxy results. This paper presents the observations, data reduction strategy, and some general results based on the preliminary data analysis: the UVIS high spatial resolution gives an unprecedented sharp view of the complex structure of the inner regions of the galaxies and of the substructures in the galaxy disks; we found clear signatures of stripping in regions very close in projection to the galactic disk; the star-forming regions in the stripped tails are extremely bright and compact while we did not detect a significant number of star-forming clumps outside those detected by MUSE. The paper finally presents the development plan for the project.
description: 17 pages, 7 figures. Accepted for publication in ApJ
Betti numbers in three dimensional minimal model program
Creators: name: Chen, Hsin-Ku
Publisher: name: arXiv
Year: 2016
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: Let $X$ be a smooth projective threefold. We prove that, among the process of minimal model program, the variance of the third Betti number can be bounded by some integer depends only on the Picard number of $X$.
Key Areas of Cattle Care and Management Survey
Creators: name: Cheng, Ting-Yu
name: Wilson, Devon
name: Brooks, Cecilia
name: Pempek, Jessica
name: George, Kelly
name: LeBlanc, Stephen
name: Cobo-Angel
name: Renaud, David
name: Habing, Gregory
Publisher: name: Zenodo
Year: 2022
Subjects: Veterinary science
Basic human values
Schwartz's value survey
Social science

description: This is supplementary data for a paper to be submitted titled, "Basic human values of dairy producers in Canada and the U.S.: A cross-sectional survey study." The survey aims to describe the herd and dairy farmer demographics and values of participants from five states of the U.S. (Florida, Michigan, Ohio, Vermont, Wisconsin), along with their male and female calf care practices.
Investigation of the Development of the Microcrack Structure in Scratch Tests with Single Diamond Particles on Monocrystalline Silicon Wafers
Creators: name: Würzner, S.
name: Buchwald, R.
name: Retsch, S.
name: Möller, H.J.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 742-746
description: This paper studies the development of the damage structure by scratching single particle tips over a
surface, which is the basic mechanism, when sawing wafers with diamond coated wires. The process has been investigated
on single scratches, which are produced by a newly developed scratch technique under defined conditions
comparable to a real sawing process. The tests have been performed with single diamond particles on
monocrystalline silicon wafers. The surface structure and the resulting microcrack systems have been investigated
by means of optical confocal microscopy, with scanning electron microscope and by Raman spectroscopy. Details
of the shape, depth and distribution of the cracks have been obtained by cross section preparations. The results
are discussed in view of the impact on diamond wire sawing.
Functional independence in elderly Australians
Creators: name: Mead, Valerie Ann.
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.
Note on "Diffusive quantum criticality in three-dimensional disordered Dirac semimetals"
Creators: name: Roy, Bitan
name: Sarma, S. Das
Publisher: name: arXiv
Year: 2016
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We correct erroneous conclusions from Ref.[1] regarding the values of various critical exponents, calculated to the two-loop order, and argue that $ε$-expansion near two spatial dimension, with $ε=d-2$ may not be reliable to address the critical properties of disorder driven Dirac semimetal-metal quantum phase transition in $d=3$.
description: 2 Pages, 1 Figure: Erratum accepted for publication in Phys. Rev. B
Hipposideros cineraceus Blyth 1853
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros cineraceus

description: Hipposideros cineraceus Blyth, 1853. J. Asiat. Soc. Bengal, 22:410. TYPE LOCALITY: Pakistan, Punjab, Salt Range, near Pind Dadan Khan. DISTRIBUTION: Pakistan to Vietnam and Borneo; adjacent small islands; probably the Philippines. SYNONYMS: durgadasi, micropus, wrighti?. COMMENTS: Includes durgadasi; but see Khajuria (1982:288). Probably includes wrighti, see Hill and Francis (1984:308).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on pages 171-172, DOI: 10.5281/zenodo.7353060
description: {"references": ["Khajuria, H. 1982. External genitalia and bacula of some central Indian Microchiroptera. Saugetierkundliche Mitteilungen, 30: 287 - 295.", "Hill, J. E., and C. M. Francis. 1984. New bats (Mammalia: Chiroptera) and new records of bats from Borneo and Malaya. Bulletin of the British Museum (Natural History), Zoology Series, 47: 303 - 329."]}
Hipposideros commersoni
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros commersoni

description: Hipposideros commersoni (E. Geoffroy, 1813). Ann. Mus. Hist. Nat. Paris, 20:263. TYPE LOCALITY: Madagascar, Fort Dauphin. DISTRIBUTION: Gambia to Ethiopia, south to Namibia, Botswana, Transvaal (South Africa) and Mozambique; Madagascar; adjacent small islands, including Saô Thomé. SYNONYMS: gambiensis, gigas, marungensis, mostellum, niangarae, thomensis, viegasi, vittata.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
Vortex dynamics and shear layer instability in high intensity cyclotrons
Creators: name: Cerfon, Antoine J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We show that the space charge dynamics of high intensity beams in the plane perpendicular to the magnetic field in cyclotrons is described by the two-dimensional Euler equations for an incompressible fluid. This analogy with fluid dynamics gives a unified and intuitive framework to explain the beam spiraling and beam break up behavior observed in experiments and in simulations. In particular, we demonstrate that beam break up is the result of a classical instability occurring in fluids subject to a sheared flow. We give scaling laws for the instability and predict the nonlinear evolution of beams subject to it. Our work suggests that cyclotrons may be uniquely suited for the experimental study of shear layers and vortex distributions that are not achievable in Penning-Malmberg traps.
description: 8 pages, 3 figures
Influence of Crystal Dislocations on Brick and Wafer Shape
Creators: name: Heiber, J.
name: Hunziker, B.
name: Boeckli, S.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 757-759
description: It is well known, that defects in the silicon crystal have a large impact on the electrical quality of
silicon and thus on the solar cell performance. In most of the studies mainly the effects of different imperfections
within the silicon lattice e.g. dislocations, impurities and precipitates on the solar cell processing were investigated. In
contrast, the influence of these defects on preceding processes like squaring and wafering was less studied. In this
work, we investigate the impact of dislocations (slip lines) on these two processes. Neither for mechanical machining
nor for cell processing crystal imperfections are acceptable. Thus, an ingot qualifier has been developed to identify
slip lines on as grown ingots with minority carrier lifetime measurements. This method allows determining the
cropping positions to eliminate low quality material as early as possible in the manufacturing process.
Willingness to pay : a study to evaluate travellers' value of health interventions to decrease the risk of Hepatitis A
Creators: name: Watts, Caroline.
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.
Investigation of the Impact of Ingot Temperature and Silicon Debris on the Generation of Saw Marks in Multi-Wire Sawing
Creators: name: Retsch, S.
name: Fuchs, M.
name: Schumann, M.
name: Möller, H.J.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 738-741
description: The standard technique for sawing silicon wafers for solar cells is the multi-wire sawing technique with
abrasive SiC slurries. The current industrial development is to reduce cost mainly by increasing the throughput, while
maintaining a high surface quality. A production limiting problem is the local appearance of deep groves in parts of the
wafer surface for higher sawing velocities. This phenomenon, generally denoted as saw marks, can affect many wafers in
a batch and reduces the yield. In a previous study a physical explanation of this phenomenon has been given. It is based
on the observation that changes of the SiC particle size distribution along the sawing channel are responsible for the
occurrence of saw marks. Such a change can be caused by viscosity changes due to the temperature increase and/or the
accumulation of smaller particles in the slurry from particle breakage and silicon debris. In this paper experimental results
are presented, which support the impact of temperature and fine grained silicon debris. It is shown how one can simply
modify a wire saw to cool the ingot, particular on the wire exit side.
Hipposideros coronatus
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros coronatus

description: Hipposideros coronatus (Peters, 1871). Monatsb. K. Preuss. Akad. Wiss. Berlin, 1871:327. TYPE LOCALITY: Philippines, Mindanao, Surigao, Mainit. DISTRIBUTION: NE Mindanao (Philippines).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
Fragility of spectral flow for topological phases in non-Wigner-Dyson classes
Creators: name: Altland, Alexander
name: Brouwer, Piet W
name: Dieplinger, Johannes
name: Foster, Matthew S
name: Moreno-Gonzalez, Mateo
name: Trifunovic, Luka
Publisher: name: Universität Regensburg
Year: 2023
Subjects: subject: 530 Physik

description: Topological insulators and superconductors support extended surface states protected against the otherwise localizing effects of static disorder. Specifically, in the Wigner-Dyson insulators belonging to the symmetry classes A, AI, and AII, a band of extended surface states is continuously connected to a likewise extended set of bulk states forming a ``bridge'' between different surfaces via the mechanism of spectral flow. In this work we show that this principle becomes \emph{fragile} in the majority of non-Wigner-Dyson topological superconductors and chiral topological insulators. In these systems, there is precisely one point with granted extended states, the center of the band, E=0. Away from it, states are spatially localized, or can be made so by the addition of spatially local potentials. Considering the three-dimensional insulator in class AIII and winding number ν=1 as a paradigmatic case study, we discuss the physical principles behind this phenomenon, and its methodological and applied consequences. In particular, we show that low-energy Dirac approximations in the description of surface states can be treacherous in that they tend to conceal the localizability phenomenon. We also identify markers defined in terms of Berry curvature as measures for the degree of state localization in lattice models, and back our analytical predictions by extensive numerical simulations. A main conclusion of this work is that the surface phenomenology of non-Wigner-Dyson topological insulators is a lot richer than that of their Wigner-Dyson siblings, extreme limits being spectrum wide quantum critical delocalization of all states vs. full localization except at the E=0 critical point. As part of our study we identify possible experimental signatures distinguishing between these different alternatives in transport or tunnel spectroscopy.
Kinematic differences between multiple populations in Galactic globular clusters
Creators: name: Martens, Sven
name: Kamann, Sebastian
name: Dreizler, Stefan
name: Göttgens, Fabian
name: Husser, Tim-Oliver
name: Latour, Marilyn
name: Balakina, Elena
name: Krajnović, Davor
name: Pechetti, Renuka
name: Weilbacher, Peter M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The formation process of multiple populations in globular clusters is still up for debate. Kinematic differences between the populations are particularly interesting in this respect, because they allow us to distinguish between single-epoch formation scenarios and multi-epoch formation scenarios. We analyze the kinematics of 25 globular clusters and aim to find kinematic differences between multiple populations to constrain their formation process. We split red-giant branch (RGB) stars in each cluster into three populations (P1, P2, P3) for the type-II clusters and two populations (P1 and P2) otherwise using Hubble photometry. We derive the rotation and dispersion profiles for each cluster and its populations by using all stars with radial velocity measurements obtained from MUSE spectroscopy. Based on these profiles, we calculate the rotation strength in terms of ordered-over-random motion $\left(v/σ\right)_\mathrm{HL}$ evaluated at the half-light radius of the cluster. We detect rotation in all but four clusters. For NGC~104, NGC~1851, NGC~2808, NGC~5286, NGC~5904, NGC~6093, NGC~6388, NGC~6541, NGC~7078 and NGC~7089 we also detect rotation for P1 and/or P2 stars. For NGC~2808, NGC~6093 and NGC~7078 we find differences in $\left(v/σ\right)_\mathrm{HL}$ between P1 and P2 that are larger than $1σ$. Whereas we find that P2 rotates faster than P1 for NGC~6093 and NGC~7078, the opposite is true for NGC~2808. However, even for these three clusters, the differences are still of low significance. We find that the strength of rotation of a cluster generally scales with its median relaxation time. For P1 and P2, the corresponding relation is very weak at best. We observe no correlation between the difference in rotation strength between P1 and P2 and cluster relaxation time. The MUSE stellar radial velocities that this analysis is based on are made publicly available.
Hipposideros corynophyllus Hill 1985
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros corynophyllus

description: Hipposideros corynophyllus Hill, 1985. Mammalia, 49:527. TYPE LOCALITY: Papua New Guinea, W Sepik, 3 km ENE Telephomin, 1800 m. DISTRIBUTION: C New Guinea.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
Breakage Root Cause Analysis in as-Cut Monocrystalline Silicon Wafers
Creators: name: Klute, C.
name: Kaule, F.
name: Schoenfelder, S.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 753-756
description: Breakage of silicon wafers during manufacturing is an important issue in the processing of silicon solar
cells. By reducing critical loadings with sensitive handling steps and improvement of manufacturing processes, the
failure probability of wafers during production was reduced in the last years. Still, it is necessary to find and
understand the reasons leading to breakage of silicon wafers. In this work, the subsurface damage is investigated in
detail as the main factor for breakage of slurry based multi wire sawn wafers by use of fractographic analysis. The
fracture origins, which lead to wafer breakage are identified and interpreted on as-cut monocrystalline wafers in
bending tests. Typical origins of breakage are presented which were identified as half-penny shape cracks most likely
resulting from indentation processes of SiC grain during wire sawing.
Tidally perturbed g-mode pulsations in a sample of close eclipsing binaries
Creators: name: Van Reeth, T.
name: Johnston, C.
name: Southworth, J.
name: Fuller, J.
name: Bowman, D. M.
name: Poniatowski, L.
name: Van Beeck, J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Thanks to the high-precision photometry from space missions such as Kepler and TESS, tidal perturbations and tilting of pulsations have been detected in more than a dozen binary systems. However, only two of these were g-mode pulsators. Aims. We aim to detect tidally perturbed g modes in additional binary systems and characterise them observationally. Methods. We perform a custom data reduction of the available Kepler and TESS photometry of a well-studied sample of 35 binary systems with gamma Doradus pulsators. For each target, we model the binary signal using a sum of 100 sine waves, with frequencies at orbital harmonics, and measure significant pulsation frequencies by iteratively prewhitening the residual light curve. Pulsations are labelled as tidally perturbed g modes if they are part of both period-spacing patterns and orbital-frequency-spaced multiplets. After visual inspection and confirmation, the properties of these targets and g modes are characterised. Results. We detect tidally perturbed g-mode pulsations for five short-period binaries that are circularised and (almost) synchronously rotating: KIC3228863, KIC3341457, KIC4947528, KIC9108579, and KIC12785282. Tidally perturbed g modes that occur within the same star and have the same mode identification (k,m), are found to have near-identical relative amplitude and phase modulations, which are within their respective 1-sigma uncertainties also identical for the Kepler and TESS photometric passbands. By contrast, pulsations with different mode identification (k,m) are found to exhibit different modulations. Moreover, the observed amplitude and phase modulations are correlated, indicating that the binary tides primarily distort g-mode amplitudes on the stellar surface. The phase modulations are then primarily a geometric effect of the integration of the stellar flux over the visible stellar surface. (abbreviated)
description: 21 pages, 33 figures, 2 tables. Accepted for publication in Astronomy and Astrophysics on 17 January 2023
Hipposideros coxi Shelford 1901
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros coxi

description: Hipposideros coxi Shelford, 1901. Ann. Mag. Nat. Hist., ser. 7, 8:113. TYPE LOCALITY: Malaysia, Sarawak, Mt. Penrisen, 4,200 ft. (1,280 m). DISTRIBUTION: Sarawak (Borneo, Malaysian part).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
Uncertainties in asteroseismic grid-based estimates of the ages of halo stars
Creators: name: Moser, S.
name: Valle, G.
name: Dell'Omodarme, M.
name: Degl'Innocenti, S.
name: Moroni, P. G. Prada
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: [...] The aim of this paper is to study the precision and theoretical biases in the age determinations of halo stars adopting both asteroseismic and classic observational constraints. [...] We adopt the well-tested SCEPtER pipeline, covering evolutionary phases up to the red giant branch (RGB). The fitting grids contain stars with mass in the range of [0.7; 1.0] $M_{\odot}$ and metallicity [Fe/H] from -2.5 to -0.5. We investigate several scenarios characterised by different adopted observational uncertainties. We also assess the impact of systematic discrepancies between the recovery grid models and target stars by computing several synthetic grids of stellar models with perturbed input physics. In our reference scenario, we recover ages for stars in the main sequence (MS) or subgiant branch (SGB) with a typical 10\%--20\% precision, while we recover those of RGB stars with a precision of about 60\%. However, adopting tighter constraints on asteroseismic parameters, the age precision in RGB improved to 20\%, while few modifications occur in the other analysed evolutionary phases. A systematic discrepancies between grid models and target stars shows that a mismatch in the mixing-length parameter value leads to significant bias in the age estimations for MS stars (about 10\%), but this bias is smaller for SGB and RGB stars. Neglecting the microscopic diffusion effect in the recovery grid leads to a typical 40\% bias in age estimates for stars on the MS. Finally, we applied the technique to stars in globular clusters. We find a precision in age estimates of around 20\% for MS stars and up to 40\% for RGB stars, greater than those obtained with classical methods. We demonstrate the method on stars of the cluster M4, obtaining a cluster age of $11.9 \pm 1.5$ Gyr and a mass at the turn-of off $0.86 \pm 0.04$ $M_{\odot}$, which are in good agreement with literature results.
description: Accepted for publication in A&A. Abstract abridged
Hipposideros crumeniferus Lesueur and Petit 1807
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros crumeniferus

description: Hipposideros crumeniferus Lesueur and Petit, 1807. In Peron, Voyage Decouv. Terres Australes, Atlas, pl. 35. TYPE LOCALITY: Indonesia, Timor. DISTRIBUTION: Timor (Indonesia). COMMENTS: Based on plate only; not certainly determinable; see Laurie and Hill (1954:56) and Hill (1963t>:23).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
description: {"references": ["Laurie, E. M. O., and J. E. Hill. 1954. List of land mammals of New Guinea, Celebes and adjacent islands 1758 - 1952. British Museum (Natural History) Publications, London, 175 pp."]}
Holography on Non-Orientable Surfaces
Creators: name: Maloney, Alexander
name: Ross, Simon F.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider the holographic computation of two dimensional conformal field theory partition functions on non-orientable surfaces. We classify the three dimensional geometries that give bulk saddle point contributions to the partition function, and find that there are fewer saddles than in the orientable case. For example, for the Klein bottle there is a single smooth saddle and a single additional saddle with an orbifold singularity. We argue that one must generally include singular bulk saddle points in order to reproduce the CFT results. We also discuss loop corrections to these partition functions for the Klein bottle.
description: 26 pages, 1 figure
Feedstock Recharging During Directional Solidification of Silicon Ingots for PV Applications
Creators: name: Beier, M.
name: Trempa, M.
name: Seebeck, J.
name: Reimann, C.
name: Wellmann, P.
name: Gründig-Wendrock, B.
name: Friedrich, J.
name: Dadzis, K.
name: Sylla, L.
name: Richter, T.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 717-721
description: Directional solidification (DS) is a well-established crystallization technology to produce
polycrystalline or quasi-mono crystalline silicon ingots for photovoltaic applications. Before the crystallization
process the silica crucible is charged with irregular shaped silicon feedstock typically resulting in a filling degree of
50 to 60%. Hence, the grown silicon ingot is only about the half of the available crucible height or volume,
respectively. The upper part of the crucible cannot be used for crystallization which means considerable yield losses.
One approach to overcome this problem is the recharging of new silicon feedstock (solid or liquid state) into the melt
during crystallization.
In this work the effects of the recharging processes on the crystal growth behavior and the material properties were
investigated. At the beginning the immersion behavior of the silicon feedstock into the silicon melt was simulated by
model experiments where polyethylene granules were dropped into water. Afterwards some growth experiments in a
modified G1-DS-furnace were carried out. The recharging process was done with 10 kg of different feedstock types
leading to a 60% increase of ingot height from 130 to 210 mm. After crystallization the grain structure and the
specific resistivity of the silicon ingots were investigated. The results show that the contact of the recharged feedstock
particles with the solid liquid interface has necessarily to be avoided to grow high quality silicon ingots by this
technology. Additionally it could be demonstrated that recharging of undoped feedstock during the crystallization
process has the potential to flat the resistivity gradient over the ingot height.
Hipposideros curtus G. M. Allen 1921
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros curtus

description: Hipposideros curtus G. M. Allen, 1921. Rev. Zool. Afr., 9:194. TYPE LOCALITY: Cameroon, Sakbayeme. DISTRIBUTION: Cameroon, Bioko, perhaps Nigeria. SYNONYMS: sandersoni. COMMENTS: Includes sandersoni; see Hill (1963b:60).
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
description: {"references": ["Hill, J. E. 1963 b. A revision of the genus Hipposideros. Bulletin of the British Museum (Natural History), Zoology Series, 11: 1 - 129."]}
Modeling the Wiresawing Yield from SiC Shape Measurements
Creators: name: Wang, X.
name: Lin, L.-T.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 735-737
description: Multi-wire sawing using loose Silicon Carbide (SiC) abrasives powder is still the main technology for
the wafering of multicrystalline silicon nowadays. To control the quality of SiC powder is of great importance to the
wafering industry that employing this process. A number of investigations had been published to analysis and model
the behavior of SiC in the wiresaw process. However, there is still a lack of quantitative relation of the SiC inspection
data to the wiresaw yield. There is no SiC incoming inspection criterion has been reported to have a consistent relation
with the yield data to the authors’ knowledge. A model was proposed in this study to correlate the shape measurement
data from the SYSMEX FPIA 3000 to the yield of wiresaw process. The model is based on a series of assumptions that
relate the silicon material removal mechanisms to a state-of-the-art particle shape analysis method. More than 50
thousand plant wiresaw data were gathered to tune and verify the model. The model was found to be able to set a
consistent incoming inspection specification for the SiC abrasive particles. At the same time, the model can be used as
a tool for optimizing the wiresaw process.
Bombardment of CO ice by cosmic rays: I. Experimental insights into the microphysics of molecule destruction and sputtering
Creators: name: Ivlev, Alexei V.
name: Giuliano, Barbara M.
name: Juhász, Zoltán
name: Herczku, Péter
name: Sulik, Béla
name: Mifsud, Duncan V.
name: Kovács, Sándor T. S.
name: Rahul, K. K.
name: Rácz, Richárd
name: Biri, Sándor
name: Rajta, István
name: Vajda, István
name: Mason, Nigel J.
name: Ioppolo, Sergio
name: Caselli, Paola
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present a dedicated experimental study of microscopic mechanisms controlling radiolysis and sputtering of astrophysical ices due to their bombardment by cosmic ray ions. Such ions are slowed down due to inelastic collisions with bound electrons, resulting in ionization and excitation of ice molecules. In experiments on CO ice irradiation, we show that the relative contribution of these two mechanisms of energy loss to molecule destruction and sputtering can be probed by selecting ion energies near the peak of the electronic stopping power. We have observed a significant asymmetry, both in the destruction cross section and the sputtering yield, for pairs of ion energies corresponding to same values of the stopping power on either side of the peak. This implies that the stopping power does not solely control these processes, as usually assumed in the literature. Our results suggest that electronic excitations represent a significantly more efficient channel for radiolysis and, possibly, also for sputtering of CO ice. We also show that the charge state of incident ions as well as the rate for CO$^+$ production in the ice have negligible effect on these processes.
description: Accepted for publication in ApJ
Oxidation of Pressed Sintered Silicon Substrate for Integrated Solar Cell
Creators: name: Boye, Y.
name: Sun, G.
name: Chancerel, F.
name: Sow, A.
name: Brette, J.-B.
name: Petit, A.
name: Millon, E.
name: Straboni, A.
Publisher: name: WIP
Year: 2014
Subjects: WAFER-BASED SILICON SOLAR CELLS AND MATERIALS TECHNOLOGY
Silicon Feedstock, Crystallisation and Wafering

description: 29th European Photovoltaic Solar Energy Conference and Exhibition; 706-709
description: Wet thermal oxidation of porous pressed sintered silicon (PSSi) substrates obtained by sintering of
upgraded metallurgical (uMG) Si powder has been investigated for the integrated solar cell (i-Cell) technology. An i-
Cell consists of several small area sub-cells made from monocrystalline Si (mono-Si) thin film interconnected in
series on an oxidized insulating porous PSSi substrate on which local conductive zones have been realized for the
rear side electrical contact of each sub-cell. In this work we have demonstrated the influence of initial porosity, time
and temperature on oxidation rate and dielectric insulation of PSSi substrates. The oxidized PSSi substrates have been
characterized by their weight gain and the evolution of porosities. These changes were well correlated with their BET
(Brunauer–Emmett–Teller) specific surface area measurements. It has been shown that the oxidation kinetics of the
PSSi substrates is strongly influenced by the initial porosity of the substrates and the oxidation mainly occurs in the
core of the material. SEM (Scanning Electronic Microscopy) observations and EDS (Energy Dispersive x-ray
Spectroscopy) analysis have been used to evaluate the growth of the silicon dioxide through the pore channels and on
the silicon grains boundaries.
Hipposideros cyclops
Creators: name: Koopman, Karl F.
Publisher: name: Zenodo
Year: 1993
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Chiroptera
Hipposideridae
Hipposideros
Hipposideros cyclops

description: Hipposideros cyclops (Temminck, 1853). Esquisses Zool. sur la Côte de Guine, p. 75. TYPE LOCALITY: Ghana, Boutry River. DISTRIBUTION: Kenya and S Sudan to Senegal and Guinea-Bissau; Bioko. SYNONYMS: langi, micaceus.
description: Published as part of Karl F. Koopman, 1993, Order Chiroptera, pp. 137-241 in Mammal Species of the World (2 nd Edition), Washington and London :Smithsonian Institution Press on page 172, DOI: 10.5281/zenodo.7353060
J-NEP: 60-band photometry and photometric redshifts for the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
Creators: name: Hernán-Caballero, A.
name: Willmer, C. N. A.
name: Varela, J.
name: López-Sanjuan, C.
name: Marín-Franch, A.
name: Ramió, H. Vázquez
name: Civera, T.
name: Ederoclite, A.
name: Muniesa, D.
name: Cenarro, J.
name: Bonoli, S.
name: Dupke, R.
name: Lim, J.
name: Chaves-Montero, J.
name: Laur, J.
name: Hernández-Monteagudo, C.
name: Fernández-Ontiveros, J. A.
name: Fernández-Soto, A.
name: Díaz-García, L. A.
name: Delgado, R. M. González
name: Queiroz, C.
name: Vílchez, J. M.
name: Abramo, R.
name: Alcaniz, J.
name: Benítez, N.
name: Carneiro, S.
name: Cristóbal-Hornillos, D.
name: de Oliveira, C. Mendes
name: Moles, M.
name: Sodré, L.
name: Taylor, K.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The J-PAS survey will observe ~1/3 of the northern sky with a set of 56 narrow-band filters using the dedicated 2.55 m JST telescope at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera, in order to demonstrate the scientific potential of J-PAS, two small surveys were performed with the single-CCD Pathfinder camera: miniJPAS (~1 deg2 along the Extended Groth Strip), and J-NEP (~0.3 deg2 around the JWST North Ecliptic Pole Time Domain Field), including all 56 J-PAS filters as well as u, g, r, and i. J-NEP is ~0.5-1.0 magnitudes deeper than miniJPAS, providing photometry for 24,618 r-band detected sources and photometric redshifts (photo-z) for the 6,662 sources with r<23. In this paper we describe the photometry and photo-z of J-NEP and demonstrate a new method for the removal of systematic offsets in the photometry based on the median colours of galaxies, dubbed "galaxy locus recalibration". This method does not require spectroscopic observations except in a few reference pointings and, unlike previous methods, is applicable to the whole J-PAS survey. We use a spectroscopic sample of 787 galaxies to test the photo-z performance for J-NEP and in comparison to miniJPAS. We find that the deeper J-NEP observations result in a factor ~1.5-2 decrease in sigma_NMAD (a robust estimate of the standard deviation of the photo-z error) and the outlier rate relative to miniJPAS for r>21.5 sources, but no improvement in brighter ones. We find the same relation between sigma_NMAD and odds in J-NEP and miniJPAS, suggesting sigma_NMAD can be predicted for any set of J-PAS sources from their odds distribution alone, with no need for additional spectroscopy to calibrate the relation. We explore the causes for photo-z outliers and find that colour-space degeneracy at low S/N, photometry artifacts, source blending, and exotic spectra are the most important factors.
description: 16 pages, 25 figures, accepted for publication in Astronomy and Astrophysics