cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Globiceps (Kelidocoris) fulvicollis Jakovlev 1877
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Globiceps
Globiceps fulvicollis

description: Globiceps (Kelidocoris) fulvicollis Jakovlev, 1877
 Material examined. Many specimens: GILAN: Deylaman, 16.-20.vii.1996; Deylaman – Barasar, 23.vii.1996; Masuleh, 3.vii.1996; Rustam Abad – Salan Sar, 6-8.vi.2001. ARDABIL: 20-50 km E of Khalkhal, 1.-21.vii.1996, 27.vi.2002; Khalkhal – Kivi, 22.vii.-4.viii.1996, 27.vi.-9.vii.2002; Majareh – Khalkhal, 22.vii.1996. GOLESTAN: Golestan N.P., Tangegol, 23.-24.v.2001, E. Heiss lgt.
 Comments. On deciduous trees in mountain forests. West-Palaearctic. New for Iran.
 All Iranian specimens are dark-coloured, belonging to the form cruciatus Reuter, 1897, which was regarded as a synonym of G. fulvicollis by KERZHNER (1964: 740). Since no intermediate forms were found, the form could be a subspecies of G. fulvicollis.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 37, DOI: 10.5281/zenodo.5328235
Complete and Simultaneous Spectral Observations of the Black-Hole X-ray Nova XTE J1118+480
Creators: name: McClintock, J. E.
name: Haswell, C. A.
name: Garcia, M. R.
name: Drake, J. J.
name: Hynes, R. I.
name: Marshall, H. L.
name: Muno, M. P.
name: Chaty, S.
name: Garnavich, P. M.
name: Groot, P. J.
name: Lewin, W. H. G.
name: Mauche, C. W.
name: Miller, J. M.
name: Pooley, G. G.
name: Shrader, C. R.
name: Vrtilek, S. D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The X-ray nova XTE J1118+480 suffers minimal extinction (b = 62 degrees) and therefore represents an outstanding opportunity for multiwavelength studies. Hynes et al. (2000) conducted the first such study, which was centered on 2000 April 8 using UKIRT, EUVE, HST and RXTE. On 2000 April 18, the Chandra X-ray Observatory obtained data coincident with a second set of observations using all of these same observatories. A 30 ks grating observation using Chandra yielded a spectrum with high resolution and sensitivity covering the range 0.24-7 keV. Our near-simultaneous observations cover approximately 80% of the electromagnetic spectrum from the infrared to hard X-rays. The UV/X-ray spectrum of XTE J1118+480 consists of two principal components. The first of these is an approximately 24 eV thermal component which is due to an accretion disk with a large inner disk radius: > 35 Schwarzschild radii. The second is a quasi power-law component that was recorded with complete spectral coverage from 0.4-160 keV. A model for this two-component spectrum is presented in a companion paper by Esin et al. (2001).
description: 19 pages, 4 figures, resubmitted to ApJ on March 2, 2001
Malacocoris chlorizans
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Malacocoris
Malacocoris chlorizans

description: Malacocoris chlorizans (Panzer, 1794)
 Material examined. GILAN: Damashk, 3 specimens, 30.vii.1996; Darreh Dasht, 2 specimens, 25.v.-20.vi.1995, 18.- 21.viii.1998; Dasht-e-Veel, 1 specimen, 20.-25.viii.1998; Manjil, 1 specimen, 15.-17.ix.2000; Rasht, 2 specimens, vi.-viii.1996; Sang Rud, 1 specimen, 30.vi.-1.vii.2003. ZANJAN: Jilan Keshe, 1 specimen, 9.-13.x.2000. TEHRAN: Evin near Tehran, several specimens, 14.-18.vii.1995; near Karadj, several specimens, 12.-14.vii.2002; Shahrestenak, 1 specimen, 10.-12.vii.1995.
 Comments. On Fraxinus. West-Palaearctic, also known from the Khorasan province in Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 37, DOI: 10.5281/zenodo.5328235
Flaring Up All Over -- Radio Activity in Rapidly-Rotating Late-Type M and L Dwarfs
Creators: name: Berger, E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Very Large Array observations of twelve late M and L dwarfs in the Solar neighborhood. The observed sources were chosen to cover a wide range of physical characteristics - spectral type, rotation, age, binarity, and X-ray and Hαactivity - to determine the role of these properties in the production of radio emission, and hence magnetic fields. Three of the twelve sources, TVLM513-46546, 2MASS J0036159+182110, and BRI0021-0214, were observed to flare and also exhibit persistent emission, indicating that magnetic activity is not quenched at the bottom of the main sequence. The radio emission extends to spectral type L3.5, and there is no apparent decrease in the ratio of flaring luminosities to bolometric luminosities between M8-L3.5. Moreover, contrary to the significant drop in persistent Hαactivity beyond spectral type M7, the persistent radio activity appears to steadily increase between M3-L3.5. Similarly, the radio emission from BRI0021-0214 violates the phenomenological relations between the radio and X-ray luminosities of coronally active stars, hinting that radio and X-ray activity are also uncorrelated at the bottom of the main sequence. The radio active sources that have measured rotational velocities are rapid rotators, Vsin(i)>30 km/sec, while the upper limits on radio activity in slowly-rotating late M dwarfs (Vsin(i)<10 km/sec) are lower than these detections. These observations provide tantalizing evidence that rapidly-rotating late M and L dwarfs are more likely to be radio active. This possible correlation is puzzling given that the observed radio emission requires sustained magnetic fields of 10-1000 G and densities of 10^12 cm^-3, indicating that the active sources should have slowed down considerably due to magnetic braking.
description: Accepted to ApJ; Two new figures; Minor text revisions
Study of the energy variation in many-body open quantum systems: role of interactions in the weak and strong coupling regimes
Creators: name: Talarico, N. W.
name: Maniscalco, S.
name: Gullo, N. Lo
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We derive an expression for the rate of change of the energy of an interacting many-body system connected to macroscopic leads. We show that the energy variation is the sum of contributions from each different lead. Unlike the charge current each of this contribution can differ from the rate of change of the energy of the lead. We demonstrate that the discrepancy between the two is due to the direct exchange of energy among the considered lead and all other leads. We conclude that the microscopic mechanism behind it are virtual processes via the interacting central region. We also speculate on what are the implications of our findings in the calculation of the thermal conductance of an interacting system.
description: Published version: 11 pages, 4 figures
Hyparrhenia nyassae Stapf
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyparrhenia
Hyparrhenia nyassae

description: Hyparrhenia nyassae (Rendle) Stapf in D.Oliver & auct. suc. (eds.), Fl. Trop. Afr. 9: 313 (1919).
 Distribution: Trop. & S. Africa, Madagascar, Indo-China
 Specimens: MOSHI Kilema, Robson, T.O. 180 (K); Kirua, Haarer, A.E. 1684 (K); Kirua, Haarer, A.E. 1699 (K); Marangu, Archbold, M.E. 395 (K); Marangu, Geilinger, W. 4718 (K); Marangu, Schlieben, H.J. 4635 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 230, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Perinatal versus adult loss of ULK1 and ULK2 distinctly influences cardiac autophagy and function
Creators: name: Harris, Matthew P.
name: Zhang, Quan J.
name: Cochran, Cole T.
name: Ponce, Jessica
name: Alexander, Sean
name: Kronemberger, Ana
name: Fuqua, Jordan D.
name: Zhang, Yuan
name: Fattal, Ranan
name: Harper, Tyler
name: Murry, Matthew L.
name: Grueter, Chad E.
name: Abel, E. Dale
name: Lira, Vitor A.
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Developmental Biology

description: Impairments in macroautophagy/autophagy, which degrades dysfunctional organelles as well as long-lived and aggregate proteins, are associated with several cardiomyopathies; however, the regulation of cardiac autophagy remains insufficiently understood. In this regard, ULK1 and ULK2 are thought to play primarily redundant roles in autophagy initiation, but whether their function is developmentally determined, potentially having an impact on cardiac integrity and function remains unknown. Here, we demonstrate that perinatal loss of ULK1 or ULK2 in cardiomyocytes (cU1-KO and cU2-KO mice, respectively) enhances basal autophagy without altering autophagy machinery content while preserving cardiac function. This increased basal autophagy is dependent on the remaining ULK protein given that perinatal loss of both ULK1 and ULK2 in cU1/2-DKO mice impaired autophagy causing age-related cardiomyopathy and reduced survival. Conversely, adult loss of cardiac ULK1, but not of ULK2 (i.e., icU1-KO and icU2-KO mice, respectively), led to a rapidly developing cardiomyopathy, heart failure and early death. icU1-KO mice had impaired autophagy with robust deficits in mitochondrial respiration and ATP synthesis. Trehalose ameliorated autophagy impairments in icU1-KO hearts but did not delay cardiac dysfunction suggesting that ULK1 plays other critical, autophagy-independent, functions in the adult heart. Collectively, these results indicate that cardiac ULK1 and ULK2 are functionally redundant in the developing heart, while ULK1 assumes a more unique, prominent role in the adult heart. Abbreviations: ATG4: autophagy related 4, cysteine peptidase; ATG5: autophagy related 5; ATG7: autophagy related 7; ATG9: autophagy related 9; ATG13: autophagy related 13; CYCS: Cytochrome C; DNM1L, dynamin 1-like; MAP1LC3A: microtubule-associated protein 1 light chain 3 alpha; MAP1LC3B: microtubule-associated protein 1 light chain 3 beta; MFN1: mitofusin 1; MFN2: mitofusin 2; MT-CO1: mitochondrially encoded cytochrome c oxidase I; MYH: myosin, heavy polypeptide; NBR1: NBR1 autophagy cargo receptor; NDUFA9: NADH:ubiquinone oxidoreductase subunit A9; OPA1: OPA1, mitochondrial dynamin like GTPase; PPARGC1A, peroxisome proliferator activated receptor, gamma, coactivator 1 alpha; SDHA: succinate dehydrogenase complex, subunit A, flavoprotein (Fp); SQSTM1: sequestosome 1; ULK1: unc-51 like kinase 1; ULK2: unc-51 like kinase 2; UQCRC1: ubiquinol-cytochrome c reductase core protein 1
Νους ποιητικός - Νους παθητικός
Creators: name: Γέρου, Θεόφραστος
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Orthotylus (Melanotrichus) minutus Jakovlev 1877
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Orthotylus
Orthotylus minutus

description: Orthotylus (Melanotrichus) minutus Jakovlev, 1877
 Material examined. Many specimens: GILAN: 10 km W of Asalem, 5.-7.vii.2002; Dasht-e-Veel, 6.-8.vi.2002; Parudbar, 28.-30.vii.2003; Sang Rud, 30.vi.-1.vii.2003. ARDABIL: Ganjgeh, 9.-10.viii.2002; near Khalkhal, 9.-11.viii.1998; Kivi, 9.-11.viii.2002. ZANJAN: Mamalan, 4.-6.vii.2002; Mamalan – Abbar, 20.-21.vii.2002. MAZANDARAN: Hassan Abad, 15.-16.vii.2002. GOLESTAN: Gilankesh, 5.-6.vii.2004; Gonbad – Baksht-e-Haft, 14.-15.vii.2003, 4.-5.vii.2004; Inche Borun, Alagol, 4.-5.vii.2004.
 Comments. On Chenopodiaceae. Pontomediterranean, extending to eastern Siberia.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 38, DOI: 10.5281/zenodo.5328235
A multiwavelength strategy for identifying celestial gamma-ray sources
Creators: name: Caraveo, P. A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The vast majority of the high-energy gamma-ray sources discovered by EGRET are still unidentified. Percentages range from 50% at high galactic latitudes, where blazars are responsible for almost all identified sources, to more than 90% near the galactic plane, where isolated neutron stars appear to be the only certified class of sources of high energy gamma-rays. In spite of all the efforts devoted to the identification problem, the only success story, so far, appears to be the chase for Geminga, where X-rays led the way to eventual optical identification. Similar searches are now starting to produce encouraging results, although none has reached, as yet, a certified identification.
description: PDF, 8 pages, 2 figures. Invited talk at the "Gamma 2001" Symposium, April 4-6 Baltimore, Maryland. To be published by AIP
Thermodynamic modelling and optimization of oxy-reforming and oxy-steam reforming of biogas by RSM
Creators: name: Özcan, Merve Doğan
name: Özcan, Orhan
name: Ayşe Nilgün Akın
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology

description: In this study, a comparative thermodynamic equilibrium calculation of biogas oxy-reforming and oxy-steam reforming processes to produce syngas has been conducted by Aspen Plus simulation software. The effects of temperature (600–800°C), pressure (1−20 atm), and inlet O2/CH4 (0−1.0), H2O/CH4 (0−3.0), and CO2/CH4 (0.3−1.0) mole ratios on the equilibrium compositions of products were determined. The operation of the process was optimized using Gibbs free energy minimization method and statistical approach: response surface methodology (RSM). Optimum operating conditions CH4/CO2/O2 = 1:0.51:0.12 at 788°C and 1 atm for oxy-reforming and CH4/CO2/H2O/O2 = 1:0.63:0.19:0.07 at 780°C and 1 atm for oxy-steam reforming were obtained to reach maximum H2 yield, CH4 and CO2 conversions by minimizing carbon selectivity to produce syngas for methanol production.
The W-function applied to the age of Globular Clusters
Creators: name: Rengel, Miriam
name: Bruzual, Gustavo
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a statistical approach for estimating the age of Globular Clusters by measurement of the likelihood between the observed cluster sequences in the Colour--Magnitude Diagram and the synthetic cluster sequences computed from stellar evolutionary models. In the conventional isochrone fitting procedure, the age is estimated in a subjective way. Here, we calculate the degree of likelihood by applying a modern statistical estimator, the Saha estimator {\it W}, and the interval of confidence from $χ^{2}$ statistics. We apply this approach to sets of three different evolutionary models. Each of these sets consists of different chemical abundances, ages, input physics, etc. Based on our approach, we estimate the age of NGC 6397, M92 and M3. With a confidence level of 99%, we find that the best estimate of the age is 14.0 Gyr within the range of 13.8 to 14.4 Gyr for NGC 6397, 14.75 Gyr within the range of 14.50 to 15.40 Gyr for M92, and 16.0 Gyr within the range of 15.9 to 16.3 Gyr for M3.
description: 4 pages, 2 figures, latex, macro included. To appear in ESO Astrophysics Symposia 'Extragalactic Globular Cluster Systems', ed. by M. Kissler-Patig, 2002
Orphan GRB radio afterglows: Candidates and constraints on beaming
Creators: name: Levinson, Amir
name: Ofek, Eran
name: Waxman, Eli
name: Gal-Yam, Avishay
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The number of orphan radio afterglows associated with gamma-ray bursts (GRBs) that should be detected by a flux limited radio survey, is calculated. It is shown that for jetted GRBs this number is smaller for smaller jet opening angle (theta), contrary to naive expectation. For a beaming factor f_b^{-1}=(theta^2/2)^{-1} = 500, roughly the value inferred by Frail et al. (2001) from analysis of afterglow light curves, we predict that between several hundreds to several thousands orphan radio afterglows should be detectable (over all sky) above 1 mJy at GHz frequencies at any given time. This orphan population is dominated by sources lying at distances of a few hundred Mpc, and having an age of ~1 yr. A search for point-like radio transients with flux densities greater than 6 mJy was conducted using the FIRST and NVSS surveys, yielding a list of 25 orphan candidates. We argue that most of the candidates are unlikely to be radio supernovae. However, the possibility that they are radio loud AGNs cannot be ruled out without further observations. Our analysis sets an upper limit for the all sky number of radio orphans, which corresponds to a lower limit f_b^{-1}>10 on the beaming factor. Rejection of all candidates found in our search would imply f_b^{-1}>100. This, and the fact that some candidates may indeed be radio afterglows, strongly motivate further observations of these transients.
description: 18 pages, including 2 figures
Density-constraint Time-dependent Hartree-Fock-Bogoliubov method
Creators: name: Scamps, G.
name: Hashimoto, Y.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Background: The Density-constraint Time-dependent Hartree-Fock method is currently the tool of choice to predict fusion cross-sections. However, it does not include pairing correlations, which have been found recently to play an important role. Purpose: To describe the fusion cross-section with a method that includes the superfluidity and to understand the impact of pairing on both the fusion barrier and cross-section. Method: The density-constraint method is tested first on the following reactions without pairing, $^{16}$O+$^{16}$O and $^{40}$Ca+$^{40}$Ca. A new method is developed, the Density-constraint Time-dependent Hartree-Fock-Bogoliubov method. Using the Gogny-TDHFB code, it is applied to the reactions $^{20}$O+$^{20}$O and $^{44}$Ca+$^{44}$Ca. Results: The Gogny approach for systems without pairing reproduces the experimental data well. The DC-TDHFB method is coherent with the TDHFB fusion threshold. The effect of the phase-lock mechanism is shown for those reactions. Conclusions: The DC-TDHFB method is a useful new tool to determine the fusion potential between superfluid systems and to deduce their fusion cross-sections.
description: 8 pages, 11 figures
Το πρόβλημα των καθόλου και η θέση του στην ύστερη φιλοσοφία του Wittgenstein
Creators: name: Κωβαίος, Κωστής Μ.
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Hyparrhenia papillipes Andersson ex Stapf 1919
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyparrhenia
Hyparrhenia papillipes

description: Hyparrhenia papillipes (Hochst. ex A.Rich.) Andersson ex Stapf in D.Oliver & auct. suc. (eds.), Fl. Trop. Afr. 9: 347
 (1919).
 Distribution: Ethiopia to E. Trop. Africa, SW. Arabian Pen., Madagascar
 Specimens: MOSHI Engare Nairobi, Greenway, P.J. 6701 (K, NH); Kirua, Haarer, A.E. 1695 (K); Lake Chala, Hemp, A. 5668 (UBT); Sanya Juu, Hemp, A. 1935 (UBT).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 230, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Merging Timescales and Merger Rates of Star Clusters in Dense Star Cluster Complexes
Creators: name: Fellhauer, M.
name: Baumgardt, H.
name: Kroupa, P.
name: Spurzem, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Interacting galaxies like the famous Antennae (NGC 4038/4039) or Stephan's Quintet (HCG 92) show considerable star forming activity in their tidal arms. High resolution images (e.g. from HST-observations) indicate that these regions consist of up to hundreds of massive stellar clusters or tidal dwarf galaxies (TDG). In this paper we want to investigate the future fate of these clusters of massive star clusters (in this work called super-clusters). We simulate compact super-clusters in the tidal field of a host-galaxy and investigate the influence of orbital and internal parameters on the rate and timescale of the merging process. We show that it is possible that such configurations merge and build a dwarf galaxy, which could be an important mechanism of how long-lived dwarf satellite galaxies form. A detailed study of the merger object will appear in a follow-up paper.
description: 22 pages, 11 figures, Cel. Mech. and Dyn. Astron., accepted; minor changes to previous version, conclusions remain unchanged
Patterned Probes for High Precision 4D-STEM Bragg Measurements
Creators: name: Zeltmann, Steven E
name: Müller, Alexander
name: Bustillo, Karen C
name: Savitzky, Benjamin
name: Hughes, Lauren
name: Minor, Andrew M
name: Ophus, Colin
Publisher: name: arXiv
Year: 2019
Subjects: subject: Applied Physics (physics.app-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Nanoscale strain mapping by four-dimensional scanning transmission electron microscopy (4D-STEM) relies on determining the precise locations of Bragg-scattered electrons in a sequence of diffraction patterns, a task which is complicated by dynamical scattering, inelastic scattering, and shot noise. These features hinder accurate automated computational detection and position measurement of the diffracted disks, limiting the precision of measurements of local deformation. Here, we investigate the use of patterned probes to improve the precision of strain mapping. We imprint a "bullseye" pattern onto the probe, by using a binary mask in the probe-forming aperture, to improve the robustness of the peak finding algorithm to intensity modulations inside the diffracted disks. We show that this imprinting leads to substantially improved strain-mapping precision at the expense of a slight decrease in spatial resolution. In experiments on an unstrained silicon reference sample, we observe an improvement in strain measurement precision from 2.7% of the reciprocal lattice vectors with standard probes to 0.3% using bullseye probes for a thin sample, and an improvement from 4.7% to 0.8% for a thick sample. We also use multislice simulations to explore how sample thickness and electron dose limit the attainable accuracy and precision for 4D-STEM strain measurements.
description: 29 pages, 7 figures; revision 1
Photodissociation regions and star formation in the Carina Nebula
Creators: name: Rathborne, J. M.
name: Burton, M. G.
name: Brooks, K. J.
name: Cohen, M.
name: Ashley, M. C. B.
name: Storey, J. W. V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained wide-field thermal infrared (IR) images of the Carina Nebula, using the SPIREX/Abu telescope at the South Pole. Emission from poly-cyclic aromatic hydrocarbons (PAHs) at 3.29um, a tracer of photodissociation regions (PDRs), reveals many interesting well defined clumps and diffuse regions throughout the complex. Near-IR images (1--2um), along with images from the Midcourse Space Experiment (MSX) satellite (8--21um) were incorporated to study the interactions between the young stars and the surrounding molecular cloud in more detail. Two new PAH emission clumps have been identified in the Keyhole Nebula and were mapped in 12CO(2--1) and (1--0) using the SEST. Analysis of their physical properties reveals they are dense molecular clumps, externally heated with PDRs on their surfaces and supported by external pressure in a similar manner to the other clumps in the region. A previously identified externally heated globule containing IRAS 10430-5931 in the southern molecular cloud, shows strong 3.29-, 8- and 21-um emission, the spectral energy distribution (SED) revealing the location of an ultra-compact (UC) HII region. The northern part of the nebula is complicated, with PAH emission inter-mixed with mid-IR dust continuum emission. Several point sources are located here and through a two-component black-body fit to their SEDs, we have identified 3 possible UC HII regions as well as a young star surrounded by a circumstellar disc. This implies that star formation in this region is on-going and not halted by the intense radiation from the surrounding young massive stars.
description: 14 pages, 12 figures. Accepted by MNRAS. Higher resolution figures available at http://www.phys.unsw.edu.au/~jmr/papers.html
Το αρχείο Δημητρίου Γ. Μοστράτου
Creators: name: Παπακώστας, Γιάννης
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Σεμινάρια σχολικών συμβούλων για τα "Φιλοσοφικά Κείμενα" στο γυμνάσιο
Creators: name: Κατσιμάνης, Κυριάκος Σ.
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Η διδασκαλία της φιλοσοφίας: θεωρητικές απόψεις και πρακτικές κατευθύνσεις
Creators: name: Βαρδάκης, Μάρκος
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Additional file 1 of A novel chalcone derivative has antitumor activity in melanoma by inducing DNA damage through the upregulation of ROS products
Creators: name: Li, Keke
name: Zhao, Shuang
name: Long, Jing
name: Su, Juan
name: Wu, Lisha
name: Tao, Juan
name: Zhou, Jianda
name: Zhang, JiangLin
name: Chen, Xiang
name: Peng, Cong
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 1. Additional figures.
Κείμενα για τον Δημόκριτο (Από το Α' Διεθνές Συνέδριο για τον Δημόκριτο)
Creators: name: Πανέρης, Ιωάννης
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Orthotylus (Orthotylus) eleagni Jakovlev 1881
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Orthotylus
Orthotylus eleagni

description: Orthotylus (Orthotylus) eleagni Jakovlev, 1881
 Material examined. ARDABIL: Firuzabad, 6 specimens, 9.viii.2002; Majareh – Kolur, several specimens, 21.vii.1995. TEHRAN: near Firuzkuh, 1 specimen, 18.-19.vii.2003; Shahrestenak, numerous specimens, 10.-12.vii.1995.
 Comments. On Eleagnus angustifolius. Known from Ukraine, Middle Asia and Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 38, DOI: 10.5281/zenodo.5328235
Ελληνική Ανθρωπιστική Εταιρεία, "Αρετής μνήμη". Αφιέρωμα εις μνήμη του Κωνσταντίνου Ι. Βουρβέρη
Creators: name: Τζαβάρας, Γιάννης
Publisher: name: Ελληνική Φιλοσοφική Επιθεώρηση
Year: 2012
Subjects: philosophy

description: Ελληνική Φιλοσοφική Επιθεώρηση, Vol 1, No 2 (1984)
Hyparrhenia pilgeriana C. E. Hubb., Bull. Misc. Inform. Kew 1928
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyparrhenia
Hyparrhenia pilgeriana

description: Hyparrhenia pilgeriana C.E.Hubb., Bull. Misc. Inform. Kew 1928: 39 (1928).
 Distribution: Ethiopia to KwaZulu-Natal
 Specimens: MOSHI Fau (near Mashame), Haarer, A.E. 1048 (K); Kirua, Haarer, A.E. 1683 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 230, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Are some breaks in GRB afterglows caused by their spectra?
Creators: name: Wei, D. M.
name: Lu, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Sharp breaks have been observed in the afterglow light curves of several GRBs; this is generally explained by the jet model. However, there are still some uncertainties concerning this interpretation due to the unclear hydrodynamics of jet sideways expansion. Here we propose an alternative explanation to these observed breaks. If we assume that the multiwavelength spectra of GRB afterglows are not made of exact power law segments but their slope changes smoothly, i.e. $dβ/d logν<0$, where $β$ is the spectral index, we find that this fact can very nicely explain the afterglow light curves showing breaks. Therefore we suggest that some breaks in the afterglow light curves may be caused by their curved spectra. The main feature of this interpretation is that the break time is dependent on the observed frequency, while the jet model produces achromatic breaks in the light curves. In addition, it is very important to know the position of the characteristic frequency $ν_{c}$ in the multiwavelength spectrum at the time of the break, since it is a further discriminant between our model and the jet model. We find that although the optical light curves of seven GRB afterglows can be well fitted by the model we propose, in fact only one of them (i.e. GRB000926) can be explained in this framework, since for other ones the characteristic frequency $ν_{c}$ is either above the optical after the break or below the optical before the break.
description: Latex, revised version accepted by A&A
On the Geometry of Extended Self-Similar Solutions of the Airy Shallow Water Equations
Creators: name: Camassa, Roberto
name: Falqui, Gregorio
name: Ortenzi, Giovanni
name: Pedroni, Marco
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: Self-similar solutions of the so called Airy equations, equivalent to the dispersionless nonlinear Schrödinger equation written in Madelung coordinates, are found and studied from the point of view of complete integrability and of their role in the recurrence relation from a bi-Hamiltonian structure for the equations. This class of solutions reduces the PDEs to a finite ODE system which admits several conserved quantities, which allow to construct explicit solutions by quadratures and provide the bi-Hamiltonian formulation for the reduced ODEs.
Orthotylus (Orthotylus) marginalis Reuter 1883
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Orthotylus
Orthotylus marginalis

description: Orthotylus (Orthotylus) marginalis Reuter, 1883
 Material examined. TEHRAN: Shahrestenak, 5 specimens, 10.-12.vii.1995.
 Comments. On deciduous trees such as Alnus, Fraxinus and Salix. Euro-Siberian. New for Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 38, DOI: 10.5281/zenodo.5328235
Modeling the observations of GRB 180720B: From radio to sub-TeV gamma-rays
Creators: name: Fraija, N.
name: Dichiara, S.
name: Pedreira, A. C. Caligula do E. S.
name: Galvan-Gamez, A.
name: Becerra, R. L.
name: Montalvo, A.
name: Montero, J.
name: Kamenetskaia, B. Betancourt
name: Zhang, B. B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Early and late multiwavelength observations play an important role in determining the nature of the progenitor, circumburst medium, physical processes and emitting regions associated to the spectral and temporal features of bursts. GRB 180720B is a long and powerful burst detected by a large number of observatories in multiwavelenths that range from radio bands to sub-TeV gamma-rays. The simultaneous multiwavelength observations were presented over multiple periods of time beginning just after the trigger time and extending for more than 30 days. The temporal and spectral analysis of Fermi LAT observations suggests that it presents similar characteristics to other bursts detected by this instrument. Coupled with X-ray and optical observations, the standard external-shock model in a homogeneous medium is favored by this analysis. The X-ray flare is consistent with the synchrotron self-Compton (SSC) model from the reverse-shock region evolving in a thin shell and long-lived LAT, X-ray and optical data with the standard synchrotron forward-shock model. The best-fit parameters derived with the Markov chain Monte Carlo simulations indicate that the outflow is endowed with magnetic fields and that the radio observations are in the self-absorption regime. The SSC forward-shock model with our parameters can explain the LAT photons beyond the synchrotron limit as well as the emission recently reported by the HESS Collaboration.
description: 18 pages, 9 figures. Minor changes. Accepted for publication in ApJ
Hyparrhenia quarrei Robyns, Fl. Agrost.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyparrhenia
Hyparrhenia quarrei

description: Hyparrhenia quarrei Robyns, Fl. Agrost. Congo Belge 1: 171 (1929).
 Distribution: Nigeria to Eritrea and S. Africa, SW. Arabian Pen.
 Specimens: MOSHI Marangu, Hitchcock, A.S. 24598 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 230, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Discovery of a Population of HI Clouds in the Galactic Halo
Creators: name: Lockman, Felix J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A population of discrete HI clouds in the halo of the inner Galaxy has been discovered in 21cm observations made with the Green Bank Telescope. The halo clouds are seen up to 1.5 kpc from the Galactic plane at many longitudes. Their velocities follow Galactic rotation. A group of clouds chosen for detailed study are found to have, in the median, a peak NHI of 2x10^19, a diameter of a few tens of pc, a density of a few tenths cm^-3, and a mass in HI of 50 solar masses. Some halo clouds have narrow lines implying that their temperature must be <1000 K; some have a core-halo spectral structure. As much as half of the mass of the neutral halo may reside in these discrete clouds. They may have been formed in a Galactic fountain and are now returning to the disk.
description: Accepted for publication in ApJ(Letters). The 12 pages include 3 figures
Synthesis of new substituted imidazo[1,2-a]pyridinylpropenenitriles through sequential one-pot Suzuki–Miyaura/Knoevenagel reactions in aqueous medium
Creators: name: Saléha Bakhta
name: Kabri, Youssef
name: Crozet, Maxime D.
name: Bellara Nedjar-Kolli
name: Vanelle, Patrice
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Plant Biology

description: A series of imidazo[1,2-a]pyridinylpropenenitriles were synthesized via consecutive one-pot Suzuki–Miyaura and Knoevenagel reactions in water/ethanol mixture between imidazo[1,2-a]pyridine-2-carbaldehydes, arylboronic acids and malononitrile, methyl cyanoacetate or ethyl cyanoacetate. This environmental friendly procedure tolerates a wide range of boronic acids and affords a new substituted imidazo[1,2-a]pyridinyl propenenitriles in good yields under microwave irradiation.
Hyparrhenia rufa Stapf
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyparrhenia
Hyparrhenia rufa

description: Hyparrhenia rufa (Nees) Stapf in D.Oliver & auct. suc. (eds.), Fl. Trop. Afr. 9: 304 (1919).
 Distribution: Trop. & S. Africa, W. Indian Ocean, SC. China to Indo-China
 Specimens: MOSHI Himo, Elisante, F. PM23 (K); Kiboroloni, Hemp, A. 711 (UBT); Kidia, Hemp, A. 34 (UBT); Nanga stream, Bigger, M. 2107 (K); s. loc., Johnston, H.H. s.n. (K); s. loc., Volkens, G. 353 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 230, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
The Ionized Gas and Nuclear Environment in NGC 3783. I. Time-Averaged 900 ks Chandra Grating Spectroscopy
Creators: name: Kaspi, S.
name: Brandt, W. N.
name: George, I. M.
name: Netzer, H.
name: Crenshaw, D. M.
name: Gabel, J. R.
name: Hamann, F. W.
name: Kaiser, M. E.
name: Koratkar, A.
name: Kraemer, S. B.
name: Kriss, G. A.
name: Mathur, S.
name: Mushotzky, R. F.
name: Nandra, K.
name: Peterson, B. M.
name: Shields, J. C.
name: Turner, T. J.
name: Zheng, W.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from a 900 ks exposure of NGC 3783 with the High-Energy Transmission Grating Spectrometer on board the Chandra X-ray Observatory. The resulting X-ray spectrum has the best combination of signal-to-noise and resolution ever obtained for an AGN. This spectrum reveals absorption lines from H-like and He-like ions of N, O, Ne, Mg, Al, Si, and S. There are also possible absorption lines from H-like and He-like Ar and Ca. We also identify inner-shell absorption from lower-ionization ions such as Si_VII-Si_XII and S_XII-S_XIV. The iron absorption spectrum is very rich; L-shell lines of Fe_XVII-Fe_XXIV are detected, strong complex of M-shell lines, and probable resonance lines from Fe_XXV. The absorption lines are blueshifted relative to the systemic velocity by a mean velocity of -590+-150 km/s. We resolve many of the absorption lines, and their mean FWHM is 820+-280 km/s. We do not find correlations between the velocity shifts or the FWHMs with the ionization potentials of the ions. Most absorption lines show asymmetry, having more extended blue wings than red wings. In O_VII we have resolved this asymmetry to be from an additional absorption system at ~ -1300 km/s. The two X-ray absorption systems are consistent in velocity shift and FWHM with the ones identified in the UV lines of C IV, N V, and H I. Equivalent width measurements for all lines are given and column densities are calculated for several ions. We resolve the narrow Fe_Kαline at 6398.2+-3.3 eV to have a FWHM of 1720+-360 km/s, which suggests that this narrow line may be emitted from the outer part of the broad line region or the inner part of the torus. We also detect a `Compton shoulder' redward of the narrow Fe_Kαline which indicates that it arises in cold, Compton-thick gas.
description: 19 pages, 12 figures (2 in color), emulateapj5, accepted for publication in The Astrophysical Journal Supplements
Hyparrhenia schimperi Stapf
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyparrhenia
Hyparrhenia schimperi

description: Hyparrhenia schimperi (Hochst. ex A.Rich.) Andersson ex Stapf in D.Oliver & auct. suc. (eds.), Fl. Trop. Afr. 9: 341
 (1919).
 Distribution: Ethiopia to S. Africa, Madagascar
 Specimens: MOSHI Marangu, Volkens, G. 534 (K); Moshi, Haarer, A.E. 736 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 230, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Discrete Modified Projection Methods for Urysohn Integral Equations with Green's Function Type Kernels
Creators: name: Kulkarni, Rekha P.
name: Rakshit, Gobinda
Publisher: name: arXiv
Year: 2019
Subjects: subject: Functional Analysis (math.FA)
subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 45G10, 65J15, 65R20

description: In the present paper we consider discrete versions of the modified projection methods for solving a Urysohn integral equation with a kernel of the type of Green's function. For $r \geq 0,$ a space of piecewise polynomials of degree $\leq r $ with respect to an uniform partition is chosen to be the approximating space. We define a discrete orthogonal projection onto this space and replace the Urysohn integral operator by a Nyström approximation. The order of convergence which we obtain for the discrete version indicates the choice of numerical quadrature which preserves the orders of convergence in the continuous modified projection methods. Numerical results are given for a specific example.
description: This is the the same paper with the arXiv identifier 1904.07895, but the shortened version. A bit change in the title also
Orthotylus (Orthotylus) nassatus
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Orthotylus
Orthotylus nassatus

description: Orthotylus (Orthotylus) nassatus (Fabricius, 1787)
 Material examined. GILAN: Sang Rud, 3 specimens, 30.vi.-1.vii.2003. ARDABIL: Khalkhal – Kivi, 5 specimens, 4.viii.1996, 7.-9.vii.2002; Majareh – Kolur, 2 specimens, 21.vii.1996. ZANJAN: Gilankesh 15 km NW of Gilvan, 1 specimen, 26.-27.vi.2004.
 Comments. On deciduous trees such as Salix, Fraxinus, Quercus and Tilia. West-Palaearctic. New for Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 38, DOI: 10.5281/zenodo.5328235
Additional file 4: of Intratumor heterogeneity comparison among different subtypes of non-small-cell lung cancer through multi-region tissue and matched ctDNA sequencing
Creators: name: Zhang, Yaxiong
name: Chang, Lianpeng
name: Yang, Yunpeng
name: Fang, Wenfeng
name: Guan, Yanfang
name: Wu, Aiwei
name: Hong, Shaodong
name: Zhou, Huaqiang
name: Chen, Gang
name: Chen, Xi
name: Zhao, Shen
name: Zheng, Qiufan
name: Pan, Hui
name: Zhang, Lanjun
name: Long, Hao
name: Yang, Haoxian
name: Wang, Xin
name: Wen, Zhesheng
name: Wang, Junye
name: Yang, Hong
name: Xia, Xuefeng
name: Zhao, Yuanyuan
name: Hou, Xue
name: Ma, Yuxiang
name: Zhou, Ting
name: Zhang, Zhonghan
name: Zhan, Jianhua
name: Huang, Yan
name: Zhao, Hongyun
name: Zhou, Ningning
name: Yi, Xin
name: Zhang, Li
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Figure S2. The consistency of mutation numbers, ITH and phylogenetic trees between panel sequencing and WES in 4 randomly selected patients. (A) mutation numbers, (B) ITH, (C) phylogenetic trees. Abbreviations: ITH intratumor heterogeneity, WES wholeexome sequencing. (PDF 259 kb)
Hyperthelia dissoluta Clayton, Kew Bull.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Hyperthelia
Hyperthelia dissoluta

description: Hyperthelia dissoluta (Nees ex Steud.) Clayton, Kew Bull. 20: 441 (1966).
 Distribution: Trop. & S. Africa, Madagascar
 Specimens: MOSHI Kirua, Haarer, A.E. 1698 (K); Lake Chala, Hemp, A. 679 (UBT); Lake Chala, Hemp, A. 679_neu (UBT); Lume River, Hemp, A. 3955 (UBT).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on pages 230-231, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Measuring the non-Gorenstein locus of Hibi rings and normal affine semigroup rings
Creators: name: Herzog, Jürgen
name: Mohammadi, Fatemeh
name: Page, Janet
Publisher: name: arXiv
Year: 2019
Subjects: subject: Commutative Algebra (math.AC)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: The trace of the canonical module of a Cohen-Macaulay ring describes its non-Gorenstein locus. We study the trace of the canonical module of a Segre product of algebras, and we apply our results to compute the non-Gorenstein locus of toric rings. We provide several sufficient and necessary conditions for Hibi rings and normal semigroup rings to be Gorenstein on the punctured spectrum.