cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Spectral Gamma-ray Signatures of Cosmological Dark Matter Annihilation
Creators: name: Bergstrom, Lars
name: Edsjo, Joakim
name: Ullio, Piero
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose a new signature for weakly interacting massive particle (WIMP) dark matter, a spectral feature in the diffuse extragalactic gamma-ray radiation. This feature, a sudden drop of the gamma-ray intensity at an energy corresponding to the WIMP mass, comes from the asymmetric distortion of the line due to WIMP annihilation into two gamma-rays caused by the cosmological redshift. Unlike other proposed searches for a line signal, this method is not very sensitive to the exact dark matter density distribution in halos and subhalos. The only requirement is that the mass distribution of substructure on small scales follows approximately the Press-Schechter law, and that smaller halos are on the average denser than large halos, which is a generic outcome of N-body simulations of Cold Dark Matter, and which has observational support. The upcoming Gamma-ray Large Area Space Telescope (GLAST) will be eminently suited to search for these spectral features. For numerical examples, we use rates computed for supersymmetric particle dark matter, where a detectable signal is possible.
description: 4 pages, 1 figure. Matches the published version. Conclusions unchanged
Were Desert Kites Used Exclusively as Driven Hunting Structures? Unresolved Issues and Alternative Interpretations of the Evidence - Socio-economic and Biological Considerations (A Draft)
Creators: name: Svizzero, Serge
name: Tisdell, Clem
name: Svizzero, Serge
name: Tisdell, Clem
Publisher: name: Unknown
Year: 2017
Subjects: subject: Land Economics/Use
subject: desert kites
subject: drive structure
subject: Early Bronze Age
subject: ethology
subject: hunting strategies
subject: livestock domestication
subject: southwest Asia
subject: tended facilities
subject: wild ungulates
subject: zooarchaeology

description: Although much information has been gathered during the last decade (as a result of archaeological excavations and satellite imaging) many unresolved issues remain about desert kites. These include the precise function of these huge archaeological stone structures which are widely distributed throughout southwestern Asia. According to the common vision, kites were hunting structures used to drive and to mass-kill large herds of wild ungulates. We qualify this view by analyzing the morphology of kites, the behavior of the targeted prey, and the logistical constraints associated with the mass-killing of ungulates. This leads us to conclude that as hunting structures, kites could also have been used for passively trapping animals. We believe it to be likely that kites were used (individually or collectively) for multiple purposes, which may have altered with the passage of time. An important use (at one stage in the existence of many kites) may have been for the mustering of livestock (especially sheep and goats), and for the capture of some wild or feral species of animals suitable for domestication. Some kites may also have been utilized for religious purposes or for cultural ceremonies.
3C 294 revisited: Deep Large Binocular Telescope AO NIR images and optical spectroscopy
Creators: name: Heidt, J.
name: Quirrenbach, A.
name: Hoyer, N.
name: Thompson, D.
name: Pramskiy, A.
name: Agapito, G.
name: Esposito, S.
name: Gredel, R.
name: Miller, D.
name: Pinna, E.
name: Puglisi, A.
name: Rossi, F.
name: Seifert, W.
name: Taylor, G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. High redshift radio galaxies are among the most massive galaxies at their redshift, are often found at the center of protoclusters of galaxies, and are expected to evolve into the present day massive central cluster galaxies. Thus they are a useful tool to explore structure formation in the young Universe. Aims. 3C~294 is a powerful FR II type radio galaxy at z = 1.786. Past studies have identified a clumpy structure, possibly indicative of a merging system, as well as tentative evidence that 3C~294 hosts a dual active galactic nucleus (AGN). Due to its proximity to a bright star, it has been subject to various adaptive optics imaging studies. Method. In order to distinguish between the various scenarios for 3C~294 we performed deep, high-resolution adaptive optics near-infrared imaging and optical spectroscopy of 3C~294 with the Large Binocular Telescope. Results. We resolve the 3C~294 system into three distinct components separated by a few tenths of an arcsecond on our images. One is compact, the other two are extended, and all appear to be non-stellar. The nature of each component is unclear. The two extended components could be a galaxy with an internal absorption feature, a galaxy merger, or two galaxies at different redshifts. We can now uniquely associate the radio source of 3C~294 with one of the extended components. Based on our spectroscopy, we determined a redshift of z = 1.784+-0.001, which is similar to the one previously cited. In addition we found a previously unreported emission line at $λ$6749.4 Å in our spectra. It is not clear that it originates from 3C~294. It could be the Ne [IV] doublet lambda 2424/2426 AA at z = 1.783, or belong to the compact component at a redshift of z ~ 4.56. We thus cannot unambiguously determine whether 3C~294 hosts a dual AGN or a projected pair of AGNs.
description: 9 pages, 4 figures, accepted for publication in A&A
Xenochodaeus Paulsen 2007, new genus
Creators: name: Paulsen, M. J.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Ochodaeidae
Xenochodaeus

description: Xenochodaeus Paulsen, new genus   (Fig. 3, 6-14)
description: Published as part of Paulsen, M. J., 2007, Nomenclatural changes in the Nearctic Ochodaeinae and description of two new genera (Coleoptera: Scarabaeoidea: Ochodaeidae), pp. 1-13 in Insecta Mundi 2007 (21) on page 3, DOI: 10.5281/zenodo.5352386
Ryphila cancellus
Creators: name: Naderloo, Reza
name: Türkay, Michael
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Leucosiidae
Ryphila
Ryphila cancellus

description: Ryphila cancellus (Herbst, 1783)
 Persian Gulf. Saudi Arabia (Basson et al. 1977; Galil 2009), UAE (Hornby 1997; Apel 2001), Iran (Stephensen 1946; present study).
 Iran. Hormozgan Province: Qeshm I. (four stations along the south coast), Bostano, Moghdan (Parsian). Bushehr Province: Kabgan, Ghaleh-Heydar.
 General distribution. Indo-West Pacific: East Africa, Madagascar, southern Oman (Dhofar), Persian Gulf, Gulf of Oman, Pakistan, India, Mergui Archipelago, Malay Archipelago, Burma, Thailand, Borneo, Sumatra, Australia (Western Australia).
 Habitat. Sandy beach.
 Remarks. Ryphila cancellus is the type species of the recently introduced genus Ryphila Galil, 2009. This species is the commonest one of the family along the Iranian coast occurring on the low-intertidal sandy beaches.
description: Published as part of Naderloo, Reza & Türkay, Michael, 2012, Decapod crustaceans of the littoral and shallow sublittoral Iranian coast of the Persian Gulf: Faunistics, Biodiversity and Zoogeography 3374, pp. 1-67 in Zootaxa 3374 (1) on pages 32-33, DOI: 10.11646/zootaxa.3374.1.1, http://zenodo.org/record/5253502
Tracking the evolution of galaxy populations over the last 8 Gyr with VIPERS
Creators: name: Haines, Christopher
Publisher: name: Zenodo
Year: 2021

description: The VIMOS Public Extragalactic Redshift Survey (VIPERS) is an ESO Large Programme that obtained spectra for ~100K galaxies at redshifts 0.5-1.2 across a 24deg2 survey region. This dataset has enabled us to reveal the development of the bimodal galaxy distribution in the D4000-M* plane over the last 8 Gyr, track the evolutions and extents of the red sequence and blue-cloud populations in unprecedented detail, and explore the relationships between star-formation history and galaxy structure. The large volume covered and high sampling rate of VIPERS makes it a unique resource for studying the most massive galaxies (log M*>11) in the Universe, and we highlight the dramatic collapse in the number density of massive star-forming (D4000<1.55) galaxies after z~0.8 and the parallel rise in the numbers of low-density massive passive galaxies.
The Explosive Yields Produced by the First Generation of Core Collapse Supernovae and the Chemical Composition of Extremely Metal Poor Stars
Creators: name: Chieffi, Alessandro
name: Limongi, Marco
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a detailed comparison between an extended set of elemental abundances observed in some of the most metal poor stars presently known and the ejecta produced by a generation of primordial core collapse supernovae. We used five stars which form our initial database and define a "template" ultra metal poor star which is then compared to the theoretical predictions. Our main findings are as follows: a) the fit to [Si/Mg] and [Ca/Mg] of these very metal poor stars seems to favor the presence of a rather large C abundance at the end of the central He burning; in a classical scenario in which the border of the convective core is strictly determined by the Schwarzschild criterion, such a large C abundance would imply a rather low C12(alpha,gamma)O16 reaction rate; b) a low C abundance left by the central He burning would imply a low [Al/Mg] (
description: 30 pages, 8 figures, 8 tables. Accepted for publication on ApJ
The Probabilistic Value-Added Catalog for the DESI Bright Galaxy Survey
Creators: name: Hahn, Changhoon
Publisher: name: Zenodo
Year: 2021

description: Over the next five years, the Bright Galaxy Survey (BGS) of the Dark Energy Spectroscopic Instrument (DESI) will measure the spectra of 10 million galaxies out to z~0.5. The PRObabilistic Value-Added BGS (PROVABGS) will provide posteriors on the physical properties (e.g. M*, SFR, metallicity) for each of these galaxies and produce the most statistically powerful magnitude-limited sample for galaxy studies. In this talk, I will present the target selection and design of the DESI BGS. I will also present the methods used to construct the PROVABGS, such as neural network emulators for stellar population synthesis, which enables tractable sampling of 10 million posteriors. Lastly, I will discuss the potential of PROVABGS to advance galaxy science.
The magnetic state of Yb in Kondo-lattice YbNi2B2C
Creators: name: Boothroyd, A. T.
name: Barratt, J. P.
name: Bonville, P.
name: Canfield, P. C.
name: Murani, A.
name: Wildes, A. R.
name: Bewley, R. I.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report neutron scattering experiments performed to investigate the dynamic magnetic properties of the Kondo-lattice compound YbNi2B2C. The spectrum of magnetic excitations is found to be broad, extending up to at least 150 meV, and contains inelastic peaks centred near 18 meV and 43 meV. At low energies we observe quasielastic scattering with a width Gamma = 2.1 meV. The results suggest a Yb3+ ground state with predominantly localized 4f electrons subject to (i) a crystalline electric field (CEF) potential, and (ii) a Kondo interaction, which at low temperatures is about an order of magnitude smaller than the CEF interaction. From an analysis of the dynamic magnetic response we conclude that the crystalline electric field acting on the Yb ions has a similar anisotropy to that in other RNi2B2C compounds, but is uniformly enhanced by almost a factor of 2. The static and dynamic magnetic properties of YbNi2B2C are found to be reconciled quite well by means of an approximation scheme to the Anderson impurity model, and this procedure also indicates that the effective Kondo interaction varies with temperature due to the crystal field splitting. We discuss the nature of the correlated-electron ground state of YbNi2B2C based on these and other experimental results, and suggest that this compound might be close to a quantum critical point on the non-magnetic side.
description: Revised version to be published in Phys Rev B
Ochodaeus Dejean. Nikolajev 1995
Creators: name: Paulsen, M. J.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Ochodaeidae
Ochodaeus

description: Ochodaeus Dejean 1821: 56
 Remarks. Ochodaeus consists of approximately 60 Old World species, with 28 species in the Palearctic region (López-Colón et al. 2006), some of which are not members of that genus based on propygidial structure. Nikolajev (2005) recently created the genus Notochodaeus (type species = O. maculatus Waterhouse) based on the presence of a propygidial sulcus and differences in the metasternum and wing venation, although this is not reflected in the Palearctic catalog (López-Colón et al. 2006). Similarly, I have not seen any New World species that should remain in Ochodaeus.
 In North America, the only taxa (other than Codocera gnatho) with an unmodified propygidium are O. sparsus LeConte and O. mandibularis Linell, and these appear to be conspecific. LeConte (1868) described O. sparsus from Cañon Blanco, NM. Linell (1896) subsequently described O. mandibularis from Winslow, AZ, comparing his new species with N. frontalis (LeConte) without mentioning O. sparsus. Both O. sparsus and O. mandibularis were considered valid by Fall (1909), and the species were distinguished by a “somewhat difficult mental character” and placement of the frontal horn, both of which might differ with size. Almost all specimens in collections were previously determined as O. mandibularis, and the name O. sparsus has become more or less disused. The holotype of O. sparsus (MCZ) is conspecific with the species currently treated as O. mandibularis. Although the type of O. mandibularis could not be located at the USNM (D. Furth, personal communication), there appears to be only one taxon present and O. mandibularis Linell is therefore a junior synonym of O. sparsus.
 Although O. sparsus lacks a propygidial sulcus or tubercles, it has little else in common with Palearctic Ochodaeus, the type species of which is O. chrysomeloides (Schrank). Ochodaeus sparsus is the only species of Nearctic ochodaeid examined in which the head is declivous behind the eyes, and the anterior marginal bead of the pronotum is correspondingly thickened and produced to contact the head; in the other Nearctic ochodaeids examined and O. chrysomeloides the anterior margin of the pronotum is simply convex. The stridulatory peg of the abdomen (see Fig. 4) is lacking in O. sparsus, and the antennal club has only nine antennomeres, not ten as in the type species of Ochodaeus. Due to these differences together with a complete lack of shared, derived characters that would unite it with Old World taxa, it is inappropriate to leave this species in the genus Ochodaeus, and a new genus is created for it.
description: Published as part of Paulsen, M. J., 2007, Nomenclatural changes in the Nearctic Ochodaeinae and description of two new genera (Coleoptera: Scarabaeoidea: Ochodaeidae), pp. 1-13 in Insecta Mundi 2007 (21) on pages 8-9, DOI: 10.5281/zenodo.5352386
Elamena sindensis Alcock 1900
Creators: name: Naderloo, Reza
name: Türkay, Michael
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Hymenosomatidae
Elamena
Elamena sindensis

description: Elamena sindensis Alcock, 1900
 Persian Gulf. Kuwait (Chopra & Das 1930), Saudi Arabia (Basson et al. 1977; Apel 2001), Iran (Stephensen 1946; present study).
 Iran. Hormozgan Province: Qeshm I. (two stations along the south coast). Bushehr Province: Khalij-Nayband (Haleh).
 General distribution. Northwestern Indian Ocean: Persian Gulf, Gulf of Oman, Pakistan, India (Bombay), Sri Lanka.
 Habitat. Rocky/cobble intertidal, found attached to algae or sea weeds.
 Remarks. Elamena sindensis is the only species of the family Hymenosomatidae occurring along the intertidal region of the Persian Gulf. Chopra & Das (1930) described another species of the family, Neorhynchoplax kempi (Chopra & Das, 1930), from Shat al-Arab freshwater marshes in Iraq, about 70 miles off the sea.
description: Published as part of Naderloo, Reza & Türkay, Michael, 2012, Decapod crustaceans of the littoral and shallow sublittoral Iranian coast of the Persian Gulf: Faunistics, Biodiversity and Zoogeography 3374, pp. 1-67 in Zootaxa 3374 (1) on page 33, DOI: 10.11646/zootaxa.3374.1.1, http://zenodo.org/record/5253502
Modified Archimedes' principle predicts rising and sinking of intruders in sheared granular flows
Creators: name: Jing, Lu
name: Ottino, Julio M.
name: Lueptow, Richard M.
name: Umbanhowar, Paul B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We computationally determine the force on single spherical intruder particles in sheared granular flows as a function of particle size, particle density, shear rate, overburden pressure, and gravitational acceleration. The force scales similarly to, but deviates from, the buoyancy force predicted by Archimedes' principle. The deviation depends only on the intruder to bed particle size ratio, but not the density ratio or flow conditions. We propose a simple force model that successfully predicts whether intruders rise or sink, knowing only the size and density ratios, for a variety of flow configurations in physical experiments.
Cut-and-Paste Dataset Generation for Balancing Domain Gaps in Object Instance Detection
Creators: name: Yun, Woo-han
name: Kim, Taewoo
name: Lee, Jaeyeon
name: Kim, Jaehong
name: Kim, Junmo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Robotics (cs.RO)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Training an object instance detector where only a few training object images are available is a challenging task. One solution is a cut-and-paste method that generates a training dataset by cutting object areas out of training images and pasting them onto other background images. A detector trained on a dataset generated with a cut-and-paste method suffers from the conventional domain shift problem, which stems from a discrepancy between the source domain (generated training dataset) and the target domain (real test dataset). Though state-of-the-art domain adaptation methods are able to reduce this gap, it is limited because they do not consider the difference of domain gaps of foreground and background. In this study, we present that the conventional domain gap can be divided into two sub-domain gaps for foreground and background. Then, we show that the original cut-and-paste approach suffers from a new domain gap problem, an unbalanced domain gaps, because it has two separate source domains for foreground and background, unlike the conventional domain shift problem. Then, we introduce an advanced cut-and-paste method to balance the unbalanced domain gaps by diversifying the foreground with GAN (generative adversarial network)-generated seed images and simplifying the background using image processing techniques. Experimental results show that our method is effective for balancing domain gaps and improving the accuracy of object instance detection in a cluttered indoor environment using only a few seed images. Furthermore, we show that balancing domain gaps can improve the detection accuracy of state-of-the-art domain adaptation methods.
description: 12 pages, 7 figures
Regularity of finite-dimensional realizations for Evolution Equations
Creators: name: Filipovic, Damir
name: Teichmann, Josef
Publisher: name: arXiv
Year: 2001
Subjects: subject: Functional Analysis (math.FA)
subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 60H15, 46A04, 53C12

description: We show that a continuous local semiflow of $C^k$-maps on a finite-dimensional $C^k$-manifold M can be embedded into a local $C^k$-flow on M under some weak (necessary) assumptions. This result is applied to an open problem in [fil/tei:01]. We prove that finite-dimensional realizations for interest rate models are highly regular objects, namely given by submanifolds M of $D(A^{\infty})$, where A is the generator of a strongly continuous semigroup.
Polyonyx loimicola Sankolli 1965
Creators: name: Naderloo, Reza
name: Türkay, Michael
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Porcellanidae
Polyonyx
Polyonyx loimicola

description: Polyonyx loimicola Sankolli, 1965
 Persian Gulf. First Persian Gulf record.
 Iran. Hormozgan Province: Qeshm I. (Dargahan, Kuweii).
 General distribution. Northwestern Indian Ocean: Persian Gulf, Pakistan, India.
 Habitat. Muddy-sand intertidal.
 Remarks. Sankolli (1965) described P. loimicola from India. Tirmizi et al. (1989) recorded it from Pakistan in Guadr Bay in the vicinity of Iranian border. In the present study, this rare species was found buried in the sandy/ muddy substrate mixed with shell fragments, which is the typical habitat of the thalassinid shrimps of Upogebia carinicauda in the Persian Gulf.
description: Published as part of Naderloo, Reza & Türkay, Michael, 2012, Decapod crustaceans of the littoral and shallow sublittoral Iranian coast of the Persian Gulf: Faunistics, Biodiversity and Zoogeography 3374, pp. 1-67 in Zootaxa 3374 (1) on page 22, DOI: 10.11646/zootaxa.3374.1.1, http://zenodo.org/record/5253502
Additional file 1 of Optimal care for the management of older people non-weight bearing after lower limb fracture: a consensus study
Creators: name: Aloraibi, S.
name: J. Gladman
name: D. Godfrey
name: V. Booth
name: K. Robinson
name: E. Lunt
name: A. Caswell
name: M. Kerr
name: B. Ollivere
name: A. L. Gordon
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Biotechnology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1.
Clibanarius signatus Heller 1861
Creators: name: Naderloo, Reza
name: Türkay, Michael
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Diogenidae
Clibanarius
Clibanarius signatus

description: Clibanarius signatus Heller, 1861
 Persian Gulf. Saudi Arabia (Apel 2001), UAE (Nobili 1906a; Titgen 1982; Hornby 1977; Apel 2001), Iran (Apel 2001; Moradmand 2007; present study).
 Iran. During the present study this was the most common species of the rocky shores along entire Iranian coast.
 General distribution. Northwestern Indian Ocean: Red Sea, Gulf of Aden, Socotra, southern Oman (Dhofar), Persian Gulf, Gulf of Oman, Pakistan.
 Habitat. Rocky/cobble intertidal.
 Remarks. This is the most common species within the intertidal zone of the Persian Gulf, and along the Iranian coast as well. Clibanarius signatus is one of the taxonomically well known species of the genus.
description: Published as part of Naderloo, Reza & Türkay, Michael, 2012, Decapod crustaceans of the littoral and shallow sublittoral Iranian coast of the Persian Gulf: Faunistics, Biodiversity and Zoogeography 3374, pp. 1-67 in Zootaxa 3374 (1) on page 25, DOI: 10.11646/zootaxa.3374.1.1, http://zenodo.org/record/5253502
Transitionless phonon assisted photon-qubit quantum state transfer in a hybrid optomechanical system
Creators: name: Saha, Arindam
name: Sarma, Amarendra K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Quantum state transfer is crucial for quantum information processing and quantum computation. Here, we propose a hybrid optomechanical system capable of coupling a qubit, an optical mode and a mechanical oscillator. The displacement of the mechanical oscillator,due to radiation pressure, induces spatial variation in the cavity field, which in turn couples the qubit with phonon mode. This allows state transfer between the cavity mode and the qubit without an actual interaction between them. We present a scheme for the transitionless quantum state transfer based on the transitionless quantum driving algorithm allowing us to achieve perfect state transfer.
Petrolisthes leptocheles
Creators: name: Naderloo, Reza
name: Türkay, Michael
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Porcellanidae
Petrolisthes
Petrolisthes leptocheles

description: Petrolisthes leptocheles (Heller, 1861)
 Persian Gulf. Iran (Heller 1961; Haig 1966; Apel 2001; present study).
 Iran. Hormozgan Province: Qeshm I. (12 stations around the island), Mahtabi, Moghdan. Bushehr Province: Dayyer, Bandargah, Bushehr (Jofreh).
 General distribution. Northwestern Indian Ocean: Somalia, Red Sea, Gulf of Aden, southern Oman (Dhofar), Persian Gulf, Gulf of Oman, Pakistan.
 Habitat. Rocky/cobble intertidal.
 Remarks. This is one of the most common species of porcellanid crabs in rocky habitats along the Iranian coast. Interestingly, this species has still not been recorded from the Arabian coast. Apel (2001) did not find it neither at the Saudi Arabian and nor the UAE coasts in his extensive sampling.
description: Published as part of Naderloo, Reza & Türkay, Michael, 2012, Decapod crustaceans of the littoral and shallow sublittoral Iranian coast of the Persian Gulf: Faunistics, Biodiversity and Zoogeography 3374, pp. 1-67 in Zootaxa 3374 (1) on page 21, DOI: 10.11646/zootaxa.3374.1.1, http://zenodo.org/record/5253502
Hedychridium maculiventre subsp. raucum * Linsenmaier 1997
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium maculiventre
Hedychridium maculiventre raucum linsenmaier, 1997

description: Hedychridium maculiventre raucum Linsenmaier, 1997
(Fig. 41A–41F)
Hedychridium (Hedychridium) maculiventre raucum Linsenmaier, 1997: 258 (descr., sculpturatum group), 289 (fig. 40).
Hedychridium scutellare palestinense Balthasar, 1953: Arens 2010: 407 (synonymised).
Type locality. Turkey: “ Turkey, ♂ Type (Holotypus), ♀ Allotype und 2 ♂ Paratypen Konya 22. VI.69, leg. und Coll. m. Paratypen: 2 ♂ Konya, Alti Napa 18. VII.72, Schmidt; 1♂ Konya Madensch 23.6.84, Schmidt; 1♂ Hakkari Sat Dag 1700 m 8. VII.83, Schacht; - Coll. m.”.
Holotype, ♂: Turkey Konya 22.VI.69 leg. Linsenmaier // ♂ Type Hedychridium Ab. maculiventre raucum Linsenmaier det. 1995 // Hedychridium ♂ scutellare palestinense Balth. W. Arens 2005 // 467 // NML _ ENT GBIF _ Chr0011475 (ex type-collection).
Allotype, ♀: Turkey Denizli 3.VII.69 leg. Linsenmaier // ♀ Allotype Hedychridium Ab. maculiventre raucum Linsenmaier det. 1995 // Hedychridium ♀ scutellare palestinense W. Arens 2005 // NML _ ENT GBIF _ Chr0011476 (ex type-collection).
Paratypes, 2♂: Konya As. Türk. Alti Napa Barai 18.VII.1972 leg. Jos. Schmidt // ♂ Paratype Hedychridium Ab. maculiventre raucum Linsenmaier det. 1995 // Hedychridium ♂ scutellare palestinense Balth. W. Arens 2005 // NML _ ENT GBIF _ Chr0011451, Chr0011452; 2♂: Turkey Konya 24.VI.69 leg. Linsenmaier // ♂ Paratypen Hedychridium Ab. maculiventre raucum Linsenmaier det. 1995 // Hedychridium ♂ scutellare palestinense W. Arens 2005 // NML _ ENT GBIF _ Chr0011453; 1♂: Tk Madenşehir Konya 23.VI.84 1300m Warncke // ♂ Paratype Hedychridium Ab. maculiventre raucum Linsenmaier det. 1995// Hedychridium ♂ scutellare palestinense Balth. W. Arens 2005 // NML _ ENT GBIF _ Chr0011454; 1♂: Türkey, Pr. Hakkari Sat Dag. Varegŏs SW Yüksekova 1700m 4.– 8.8.1983 leg. W. Schacht // ♂ Paratype Hedychridium Ab. maculiventre raucum Linsenmaier det. 1995// Hedychridium ♂ scutellare palestinense Balth. W. Arens 2005 // NML _ ENT GBIF _ Chr0011455.
Remarks. According to the original description, the allotype locality is Konya and not Denizli. We consider this a case of lapsus calami. Arens (2010) synonymised H. maculiventre raucum with H. palestinense Balthasar, 1953.
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on pages 40-41, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Hard X-ray emission from the galaxy cluster A3667
Creators: name: Fusco-Femiano, R.
name: Fiume, D. Dal
name: Orlandini, M.
name: Brunetti, G.
name: Feretti, L.
name: Giovannini, G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the results of a long BeppoSAX observation of Abell 3667, one of the most spectacular galaxy cluster in the southern sky. A clear detection of hard X-ray radiation up to ~ 35 keV is reported, while a hard excess above the thermal gas emission is present at a marginal level that should be considered as an upper limit to the presence of nonthermal radiation. The strong hard excesses reported by BeppoSAX in Coma and A2256 and the only marginal detection of nonthermal emission in A3667 can be explained in the framework of the inverse Compton model. We argue that the nonthermal X-ray detections in the PDS energy range are related to the radio index structure of halos and relics present in the observed clusters of galaxie.
description: 15 pages, 1 figure, ApJL in press
Synthetic parity-time symmetry breaking in a single microcavity
Creators: name: Zhang, Fangxing
name: Feng, Yaming
name: Ge, Li
name: Wan, Wenjie
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Non-Hermitian systems based on parity-time (PT) symmetry reveal rich physics beyond the Hermitian regime. So far, realizations of PT-symmetric systems have been limited to the spatial domain. Here we theoretically and experimentally demonstrate PT symmetry in a synthetic spectral dimension induced by nonlinear Brillouin scattering in a single optical microcavity, where electromagnetically induced transparency or absorption in two spectral resonances provides the optical gain and loss to observe a phase transition between two symmetry regimes. This scheme provides a new paradigm towards the investigation of non-Hermitian physics in a synthetic photonic dimension for all-optical signal processing and quantum information science.
description: 11 pages, 3 figures
Cucochodaeus Paulsen 2007, new genus
Creators: name: Paulsen, M. J.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Ochodaeidae
Cucochodaeus

description: Cucochodaeus Paulsen, new genus   (Fig. 1)
description: Published as part of Paulsen, M. J., 2007, Nomenclatural changes in the Nearctic Ochodaeinae and description of two new genera (Coleoptera: Scarabaeoidea: Ochodaeidae), pp. 1-13 in Insecta Mundi 2007 (21) on page 9, DOI: 10.5281/zenodo.5352386
Robust standard errors for panel regressions with cross–sectional dependence
Creators: name: Hoechle, Daniel
name: Hoechle, Daniel
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: xtscc
subject: robust standard errors
subject: nonparametric covariance estimation

description: I present a new Stata program, xtscc, that estimates pooled ordinary least-squares/weighted least-squares regression and fixed-effects (within) regression models with Driscoll and Kraay (Review of Economics and Statistics 80: 549–560) standard errors. By running Monte Carlo simulations, I compare the finite-sample properties of the cross-sectional dependence–consistent Driscoll–Kraay estimator with the properties of other, more commonly used covariance matrix estimators that do not account for cross-sectional dependence. The results indicate that Driscoll–Kraay standard errors are well calibrated when cross-sectional dependence is present. However, erroneously ignoring cross-sectional correlation in the estimation of panel models can lead to severely biased statistical results. I illustrate the xtscc program by considering an application from empirical nance. Thereby, I also propose a Hausman-type test for fixed effects that is robust to general forms of cross-sectional and temporal dependence.
BUDDI-MaNGA: a statistical spectroscopic survey of galaxy bulges and discs
Creators: name: Johnston, Evelyn
name: Häußler, Boris
Publisher: name: Zenodo
Year: 2021

description: As a galaxy evolves, its morphology typically changes. The processes that trigger these transformations affect their bulge and disc in different ways, leaving characteristic imprints on their stellar populations. Extracting the clean spectra of these components through traditional techniques is tricky due to the superposition of the light from other structures. But, the introduction of IFU surveys of nearby galaxies provides the combined spatial and spectral information for these galaxies. We have developed BUDDI to use this spatial information to cleanly separate the spectra from the bulges and discs, and applied it to the MaNGA DR16 sample of galaxies to extract their independent SFHs. To date, this is by far the largest sample of bulge and disc spectra extracted from IFU datacubes through light profile modelling, and we will use it to study how galaxies evolve and the role of their individual structures. I will present the sample and technique, and will highlight our initial results
Estimating parameters of dichotomous and ordinal item response models with gllamm
Creators: name: Zheng, Xiaohui
name: Rabe-Hesketh, Sophia
name: Zheng, Xiaohui
name: Rabe-Hesketh, Sophia
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: gllamm
subject: gllapred
subject: latent variables
subject: Rasch model
subject: partial-credit model
subject: rating scale model
subject: latent regression
subject: generalized linear latent and mixed model
subject: adaptive quadrature
subject: item response theory

description: Item response theory models are measurement models for categorical responses. Traditionally, the models are used in educational testing, where responses to test items can be viewed as indirect measures of latent ability. The test items are scored either dichotomously (correct–incorrect) or by using an ordinal scale (a grade from poor to excellent). Item response models also apply equally for measurement of other latent traits. Here we describe the one- and two-parameter logit models for dichotomous items, the partial-credit and rating scale models for ordinal items, and an extension of these models where the latent variable is regressed on explanatory variables. We show how these models can be expressed as generalized linear latent and mixed models and fitted by using the user-written command gllamm.
Additional file 1 of Use of an evidence-based health portal to improve teaching and learning in primary care: a mixed methods evaluation
Creators: name: Costa, José Roberto Bittencourt
name: Luiz Anastacio Alves
name: Alberto, Anael Viana Pinto
name: De Souza, Cristina Alves Magalhães
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 1.
The Chemical Yields Produced by Zero Metal Massive Stars
Creators: name: Limongi, Marco
name: Chieffi, Alessandro
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this review we compare the three existing sets of theoretical yields of zero metal massive stars available in the literature. We also show how each of these three different sets of yields fits the element abundance ratios observed in the extremely metal poor star CD 38245. We find that, at present, no theoretical set of yields of zero metal massive stars is able to satisfactorily reproduce the elemental ratios [X/Fe] of this star.
description: 19 pages, 7 figures, 6 tables
Simulation-based sensitivity analysis for matching estimators
Creators: name: Nannicini, Tommaso
name: Nannicini, Tommaso
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: sensatt
subject: sensitivity analysis
subject: matching
subject: propensity score
subject: program evaluation

description: This article presents a Stata program (sensatt) that implements the sensitivity analysis for matching estimators proposed by Ichino, Mealli, and Nannicini (Journal of Applied Econometrics, forthcoming). The analysis simulates a potential confounder to assess the robustness of the estimated treatment effects with respect to deviations from the conditional independence assumption. The program uses the commands for propensity-score matching (att* ) developed by Becker and Ichino (Stata Journal 2: 358–377). I give an example by using the National Supported Work demonstration, widely known in the program evaluation literature.
Supplementary methods and Figure to 'Diabetes is associated with genotypically drug-resistant tuberculosis'.docx
Creators: name: Ruesen, Carolien
name: Chaidir, Chaidir
name: Ugarte-Gil, Cesar
name: Ingen, Jakko Van
name: Critchley, Julia
name: Hill, Philip C.
name: Ruslami, Rovina
name: Santoso, Prayudi
name: Huynen, Martijn A.
name: Dockrell, Hazel M.
name: Moore, David
name: Alisjahbana, Bachti
name: Crevel, Reinout Van
Publisher: name: figshare
Year: 2019
Subjects: subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplementary methods and Figure to 'Diabetes is associated with genotypically drug-resistant tuberculosis'.
Profile likelihood for estimation and confidence intervals
Creators: name: Royston, Patrick
name: Royston, Patrick
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: pllf
subject: profile likelihood
subject: confidence interval
subject: nonnormality
subject: nonlinear model

description: Normal-based confidence intervals for a parameter of interest are inaccurate when the sampling distribution of the estimate is nonnormal. The technique known as profile likelihood can produce confidence intervals with better coverage. It may be used when the model includes only the variable of interest or several other variables in addition. Profile-likelihood confidence intervals are particularly useful in nonlinear models. The command pllf computes and plots the maximum likelihood estimate and profile likelihood–based confidence interval for one parameter in a wide variety of regression models.
Hedychridium luteipenne Lins. Linsenmaier 1968
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium luteipenne

description: Hedychridium luteipenne Linsenmaier, 1968
(Fig. 40A–40E)
Hedychridium (Hedychridium) luteipenne Linsenmaier, 1968: 22 (descr., luteipenne group); 1999: 55 (key, diagn., modestum group), 69 (figs 89, 90).
Type locality. Egypt: “Ägypten, ♂ Type von Kairo (Dahschour), V.58, leg. Pulawski, in Coll. m., ♂ Paratype, Fayum, in Coll Nadig”.
Holotype, ♂: Egypte Dahschour Rég. du Caire 8.V.1958 leg. W.J. Puławski // ♂ Type Hedychridium Ab. luteipenne Lins. Linsenmaier det. 1963 // 211 // NML _ ENT GBIF _ Chr0008113 (ex type-collection).
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on pages 39-40, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207
Fitting mixed logit models by using maximum simulated likelihood
Creators: name: Hole, Arne Risa
name: Hole, Arne Risa
Publisher: name: Unknown
Year: 2007
Subjects: subject: Research Methods/ Statistical Methods
subject: mixlogit
subject: mixlpred
subject: mixlcov
subject: mixed logit
subject: maximum simulated likelihood

description: This article describes the mixlogit Stata command for fitting mixed logit models by using maximum simulated likelihood.
Additional file 3: of Investigation into the underlying regulatory mechanisms shaping inflorescence architecture in Chenopodium quinoa
Creators: name: Wu, Qi
name: Bai, Xue
name: Zhao, Wei
name: Shi, Xiaodong
name: Xiang, Dabing
name: Wan, Yan
name: Wu, Xiaoyong
name: Sun, Yanxia
name: Zhao, Jianglin
name: Peng, Lianxin
name: Zhao, Gang
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Computational Biology

description: Table S1. Statistic of the expressed genes at each stage. (DOCX 19 kb)
Neochodaeus Nikolajev 1995
Creators: name: Paulsen, M. J.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Ochodaeidae
Neochodaeus

description: Neochodaeus Nikolajev, 1995: 77
 Neochodaeus frontalis (LeConte, 1863: 76) (Ochodaeus).
 Ochodaeus complex LeConte, 1868: 51, synonym.
 Neochodaeus praesidii (Bates, 1887: 106) (Ochodaeus).
 Neochodaeus repandus (Fall, 1909: 36) (Ochodaeus), new combination.
 Neochodaeus striatus (LeConte, 1854: 222) (Ochodaeus), new combination.
description: Published as part of Paulsen, M. J., 2007, Nomenclatural changes in the Nearctic Ochodaeinae and description of two new genera (Coleoptera: Scarabaeoidea: Ochodaeidae), pp. 1-13 in Insecta Mundi 2007 (21) on page 11, DOI: 10.5281/zenodo.5352386
Spectroscopic Surveys and HI in Deep Fields
Creators: name: Holwerda, Benne
Publisher: name: Zenodo
Year: 2021

description: The MeerKAT (64 x 13.5m dish radio interferometer) is South Africa's precursor instrument for the Square Kilometre Array (SKA), exploring dish design, instrumentation, and the characteristics of a Karoo desert site and is projected to be on sky in 2016. One of two top-priority, Key Projects is a single deep field, integrating for ~5000 hours total with the aim to detect neutral atomic hydrogen through its 21 cm line emission out to redshift unity and beyond. Key for maximizing science with LADUMA is additional spectroscopic information; to identify OH masers, as a prior for HI stacking, and for the star-formation and metallicity indicators. Stacking is especially useful to maximize HI science at high redshift but very large and accurate catalogs of optical redshifts are needed. The LADUMA target field (CDFS) is targeted by DEVILS, WAVES and MOONRISE. I will discuss future science and expected returns.
The Legacy of VIMOS in Exploring and Defining Proto-cluster Environments at High Redshift
Creators: name: Lemaux, Brian
Publisher: name: Zenodo
Year: 2021

description: The past decade has been witness to immense progress in the understanding of the early stages of cluster formation. During this time, samples of forming clusters at higher redshift, termed "proto-clusters" have begun to compete with lower-redshift samples both in number and in the homogeneity of the detection methods. I will focus on the legacy of VIMOS in exploring and observationally defining such regions in the universe. These achievements were primarily realized through the lens of large galaxy surveys such as VVDS, zCOSMOS, and VUDS with immense involvement from the PI of VIMOS, the late Prof. Olivier Le Fèvre. I will discuss these observations and the development of the methods for characterizing proto-clusters. Several case studies of a diverse set of massive proto-clusters will be presented and I will discuss the role of Keck/ DEIMOS in continuing the legacy of VIMOS. I will finally discuss constraints on relationship of star formation rate and galaxy density at these redshifts.
High Redshift Quasars and Star Formation in the Early Universe
Creators: name: Dietrich, M.
name: Appenzeller, I.
name: Vestergaard, M.
name: Wagner, S. J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In order to derive information on the star formation history in the early universe we observed 6 high-redshift (z=3.4) quasars in the near-infrared to measure the relative iron and \mgii emission strengths. A detailed comparison of the resulting spectra with those of low-redshift quasars show essentially the same FeII/MgII emission ratios and very similar continuum and line spectral properties, indicating a lack of evolution of the relative iron to magnesium abundance of the gas since z=3.4 in bright quasars. On the basis of current chemical evolution scenarios of galaxies, where magnesium is produced in massive stars ending in type II SNe, while iron is formed predominantly in SNe of type Ia with a delay of ~1 Gyr and assuming as cosmological parameters H_o = 72 km/s Mpc, Omega_M = 0.3, and Omega_Lambda = 0.7$, we conclude that major star formation activity in the host galaxies of our z=3.4 quasars must have started already at an epoch corresponding to z_f ~= 10, when the age of the universe was less than 0.5 Gyrs.
description: 29 pages, 5 figures, ApJ in press
Hedychridium maculiventre subsp. maculiventre maculiventre Linsenmaier 1959
Creators: name: Rosa, Paolo
name: Heim, René
name: Bernasconi, Marco Valerio
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Chrysididae
Hedychridium
Hedychridium maculiventre
Hedychridium maculiventre maculiventre linsenmaier, 1959b

description: Hedychridium maculiventre maculiventre Linsenmaier, 1959b
Hedychridium (Hedychridium) maculiventre Linsenmaier, 1959b: 235 (descr., sculpturatum group), nec Linsenmaier, 1959a: 63.
Hedychridium scutellare maculisternum Arens, 2011: 316, Replacement name for Hedychridium maculiventre Linsenmaier, 1959b, nom. praeocc., nec Linsenmaier, 1959a (roseum group).
Type locality. Croatia: “Jugoslawien, ♂ Type, ♀ Allotype Coll. m. (Dalmatien, Omis, VIII. 1952, leg. Verhoeff)”.
Holotype, ♂ and allotype, ♀ [glued on the same label]: Yugoslavia Omis (Dalm.) 12.–18.VIII.1952 PMF Verhoeff // Hedychridium Ab. maculiventre Lins. Linsenmaier det. 1959 // 74 // NML _ ENT GBIF _ Chr0011450 (ex type-collection).
Remarks. We (Arens and Rosa in Arens 2011) considered Hedychridium maculiventre Linsenmaier, 1959b a junior homonym of H. maculiventre Linsenmaier, 1959a (unnecessary replacement name for H. palestinense Balthasar, 1953) and Arens (2011) proposed the replacement name H. maculisternum pro H. maculiventre Linsenmaier, 1959b.
description: Published as part of Rosa, Paolo, Heim, René & Bernasconi, Marco Valerio, 2022, The Palaearctic types of Chrysididae (Insecta, Hymenoptera) deposited in the Linsenmaier collection. Part 2. Elampini: genus Hedychridium Abeille de Perrin, 1878, pp. 1-94 in Zootaxa 5090 (1) on page 41, DOI: 10.11646/zootaxa.5090.1.1, http://zenodo.org/record/5836207