Search results for " lace"

showing 10 items of 39 documents

Scent of Jasmine Attracts Alien Invaders and Records on Citizen Science Platforms: Multiple Introductions of the Invasive Lacebug Corythauma ayyari (…

2020

Simple Summary The distribution of the lacebug Corythauma ayyari, a pest species associated to jasmine plants, has been updated using collections and citizen-science data. The path of introduction of this species in Italy has been inferred with molecular analysis. The results revealed an extent of occurrence in Italy wider than was previously known and the evidence of multiple introduction events. The work shows that citizen science can represent a further tool within the early warning information system for alien species introduction. Abstract The jasmine lacebug Corythauma ayyari is a pest of cultivated and ornamental plants mainly associated to Jasminum spp. This invasive insect is nativ…

0106 biological sciencesJasminumSpecies distributionBiodiversityDistribution (economics)Alienoccurrence010603 evolutionary biology01 natural sciencesMediterranean BasinTingidaeArticlelacebugtingidcitizen scienceornamental plantslcsh:ScienceCladealien invasive species<i>Jasminum</i>alien invasive species; citizen science; occurrence; <i>Jasminum</i>; lacebug; ornamental plants; tingidbiologybusiness.industryEcology010604 marine biology & hydrobiologyHeteropterabiology.organism_classificationInsect Sciencelcsh:QbusinessInsects
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FT-IR spectroscopy : A powerful tool for studying the inter- and intraspecific biodiversity of cultivable non-Saccharomyces yeasts isolated from grap…

2016

International audience; The efficiency of the FT-IR technique for studying the inter- and intra biodiversity of cultivable non-Saccharomyces yeasts (NS) present in different must samples was examined. In first, the capacity of the technique FF-IR to study the global diversity of a given sample was compared to the pyrosequencing method, used as a reference technique. Seven different genera (Aureobasidium, Candida, Cryptococcus, Hanseniaspora, Issatchenkia, Metschnikowia and Pichia) were identified by FT-IR and also by pyrosequencing. Thirty-eight other genera were identified by pyrosequencing, but together they represented less than 6% of the average total population of 6 musts. Among the sp…

0301 basic medicineIdentification[ SDV.AEN ] Life Sciences [q-bio]/Food and NutritionBiodiversityWineHanseniasporaSaccharomycesMicrobial ecology[ SDV.MP ] Life Sciences [q-bio]/Microbiology and ParasitologyYeastsSpectroscopy Fourier Transform InfraredVitisDNA FungalMycological Typing TechniquesPhylogenyCandidaIntragenomic variationbiologySp-nov.Pyrolysis mass-spectrometryPyrosequencingBiodiversityCandida zemplininaYeast in winemaking[SDV.MP]Life Sciences [q-bio]/Microbiology and ParasitologyFT-IR spectroscopyMetschnikowiaAlcoholic fermentationMicrobiology (medical)food.ingredientWine yeast030106 microbiologyMicrobiologyIntraspecific competitionCandida-zemplininaSaccharomyces03 medical and health sciencesfoodBotanyRNA Ribosomal 18SMolecular BiologyBase SequenceComputational BiologySequence Analysis DNAbiology.organism_classificationGreen lacewingsStrain typingPyrosequencingTransform-infrared-spectroscopy[SDV.AEN]Life Sciences [q-bio]/Food and NutritionBotrytis-affected wine
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Long-term monitoring of mrk 501 for its very high energy γ emission and a flare in 2011 october

2012

"As one of the brightest active blazars in both X-ray and very high energy γ -ray bands, Mrk 501, is very useful for" "physics associated with jets from active galactic nuclei. The ARGO-YBJ experiment has monitored Mrk 501 for γ - rays above 0.3 TeV since 2007 November. The largest flare since 2005 was observed from 2011 October and lasted until about 2012 April. In this paper, a detailed analysis of this event is reported. During the brightest γ -ray flaring episodes from 2011 October 17 to November 22, an excess of the event rate over 6σ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the γ -ray flux above 1 TeV by a factor of 6.6 ± 2.2 from its steady…

Active galactic nucleusactive" ["galaxies]Astrophysics::High Energy Astrophysical PhenomenaFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencesBlazar010303 astronomy & astrophysicsPhysicsindividual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermal [BL Lacertae objects]" "general" ["gamma rays]010308 nuclear & particles physicsBL Lacertae objects: individual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermalSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsQuasarGalaxyindividual (Markarian 501)" ["BL Lacertae objects]13. Climate actionSpace and Planetary ScienceSpectral energy distributionFlare
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REM near-IR and optical multiband observations of PKS 2155-304 in 2005 : Erratum

2007

Fernandez Soto, Alberto, Alberto.Fernandez@uv.es

Active galaxies ; BL Lacertae objects ; Individual ; PKS 2155-30 ; Errata ; AddendaAddendaErrataActive galaxiesBL Lacertae objectsIndividualPKS 2155-30UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaUNESCO::ASTRONOMÍA Y ASTROFÍSICA:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Data from: Effects of undergrowth removal and edge proximity on ground beetles and vascular plants in urban boreal forests

2019

Urban forests are regularly managed for human safety and aesthetic reasons, but they are crucial habitat for many species. Removals of undergrowth occur commonly in these forests, yet the ecological consequences of these operations are poorly understood. We sampled ground beetles (Coleoptera, Carabidae) and vascular plants along 20-m edge gradients in Finnish urban forests, in five stands treated 0.5−2.5 years earlier with undergrowth removal and in five untreated stands. We hypothesized that undergrowth removal and edge proximity would benefit opportunistic and open-habitat species, whereas shady-habitat species would be affected negatively. (1) Regarding carabids, diversity and evenness i…

Agrostis capillarisRichnessDryopteris filix-masMilium effusumNardus strictaRubus idaeusVaccinium myrtillusLeistus terminatusCarex canescensLinnaea borealisOxalis acetocellaLuzula luzuloidesParis quadrifoliaLonicera xylosteumPterostichus nigerGeranium sylvaticumCalamagrostis arundinaceusmedicine and health carePatrobus assimilisTaraxacum spFragaria vescaArtemisia vulgarisPterostichus diligensCalathus micropterusPterostichus oblongopunctatusCalathus melanocephalusPhleum pretenseDeschampsia flexuosaHypericum maculatumViola rivinianaPterostichus melanariusLife SciencesPterostichus nigritaActaea spicataUrtica dioicaMelampyrum pretenseEquisetum pretenseFestuca ovinaSorbus aucupariaRubus saxatilisAnisodactylus binotatusMedicineMelica nutansCarabidaeAmara lunicollisAnthriscus sylvestrisLuzula pilosaTrechus secalisPterostichus strenuousCarabus hortensisHarpalus tardusedge effectGalium albumVeronica officinalisBadister lacertosusAlchemilla spQuaternaryCychrus caraboidesDryopteris carthusianaMaianthemum bifoliumPatrobus atrorufusTrechus rivularisNotiophilus biguttatusGeum urbanumundergrowthVaccinium vitis-idaeaMelampyrum sylvaticumGymnocarpium dryopterisDeschampsia cespitosaLoricera pilicornisCarex acutaAmara communisRanunculus repensConvallaria majalisAthyrium filix-feminaRibes rubrumHoloceneCirsium arvensePoa chaixiiAegopodium podagrariaTrientalis europaeaLeistus ferrugineusEquisetum sylvaticumRanunculus acrisEpilobium montanumAcer platanoidesScrophularia nodosaHarpalus laevipesUrtica urensCarabus nemoralisHieracium sylvaticaCampanula rotundifoliaSynuchus vivalisEpilobium angustifoliumVeronica chamaedrys
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Absolute kinematics of radio-source components in the complete S5 polar cap sample: IV. Proper motions of the radio cores over a decade and spectral …

2016

We have carried out a high-precision astrometric analysis of two very-long-baseline-interferometry (VLBI) epochs of observation of the 13 extragalactic radio sources in the complete S5 polar cap sample. The VLBI epochs span a time baseline of ten years and enable us to achieve precisions in the proper motions of the source cores up to a few micro-arcseconds per year. The observations were performed at 14.4 GHz and 43.1 GHz, and enable us to estimate the frequency core-shifts in a subset of sources, for which the spectral-index distributions can be computed. We study the source-position stability by analysing the changes in the relative positions of fiducial source points (the jet cores) ove…

AstrofísicaActive galactic nucleusAstrometriaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematics01 natural sciencesStability (probability)Radio continuum: generalBinary black hole0103 physical sciencesVery-long-baseline interferometry010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsJet (fluid)general [Radio continuum]general [BL Lacertae objects]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsgeneral [Quasars]BL Lacertae objects: generalAstrometryAstrometryAstrophysics - Astrophysics of GalaxiesQuasars: generalGravitational lensSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]Astrophysics - Instrumentation and Methods for Astrophysics
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Discovery of off-axis jet structure of TeV blazar Mrk 501 with mm-VLBI

2016

Context. High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal tool for probing the structure at the base of extragalactic jets in detail. The TeV blazar Mrk 501 is one of the best targets among BL Lac objects for studying the nature of off-axis jet structures because it shows different jet position angles at different scales. Aims. The aim of this study is to investigate the properties of the off-axis jet structure through high-resolution mm-VLBI images at the jet base and physical parameters such as kinematics, flux densities, and spectral indices. Methods. We performed Very Long Baseline Array (VLBA) observations over six epochs from 2012 February to 201…

Astrofísicaactive [Galaxies]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxContext (language use)galaxies [Radio continuum]Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio continuum: galaxiesindividual: Markarian 501 [BL Lacertae objects]0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsVery Long Baseline Array0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Spectral indexBL Lacertae objects: individual: Markarian 501 galaxies: active galaxies: jets radio continuum: galaxiesAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsGalaxies: activeAstrophysics - Astrophysics of GalaxiesBL Lacertae objects: individual: Markarian 501Galaxies: jetsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astronomiajets [Galaxies]MillimeterAstrophysics - High Energy Astrophysical PhenomenaAstronomy &amp; Astrophysics
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Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

2010

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (4300 m a.s.l., Tibet, China), we monitored the source at gamma ray energies E &gt; 0.3 TeV during the whole year. The observed flux was variable, with the strongest flares in March and June, in correlation with X-ray enhanced activity. While during specific episodes the TeV flux could be several times larger than the Crab Nebula one, the average emission from day 41 to 180 was almost twice the Crab level, with an integral flux of (3.6 +-0.6) 10^-1…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsBL Lacertae objectSettore FIS/05 - Astronomia E AstrofisicaExtended Air showersSettore FIS/05 - Astronomia e Astrofisicageneral" ["gamma rays]BlazarBL Lacertae objects; Markarian 421; gamma rays; Extended Air showersCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexindividual (Markarian 421)" ["BL Lacertae objects]Markarian 421Settore FIS/01 - Fisica SperimentaleGamma rayindividual (Markarian 421) - gamma rays: observations [BL Lacertae objects]Astronomy and AstrophysicsAir showerCrab NebulaSpace and Planetary Sciencegamma rayIntergalactic travelAstrophysics - High Energy Astrophysical Phenomena
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Relativistic beaming and gamma-ray brightness of blazars

2009

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA images from the MOJAVE program with millimetre-wavelength flux density monitoring data from Metsahovi Radio Observatory, we estimate the jet Doppler factors, Lorentz factors, and viewing angles for a sample of 62 blazars. We study the trends in these quantities between the sources which were detected in gamma-rays by the Fermi Large Area Telescope (LAT) during its first three months of science operations and those which were not detected. The LAT-detected blaz…

BrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenajets [galaxies]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionTelescopesymbols.namesakeRelativistic beaminglawquasars: general0103 physical sciencesBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physicsGamma rayAstronomy and Astrophysicsgalaxies: jetsViewing angle:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Lorentz factorSpace and Planetary Scienceactive [galaxies]BL Lacertae objectssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAstrophysics - High Energy Astrophysical Phenomenagalaxies: active; ; ; BL Lacertae objects : generalFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Sub specie æternitatis: the role of the ruin and the ancient in the process of architectural renewal between metamorphosis and resurgence

2022

Composing new works of architecture inspired by vestiges from antiquity or archaeology. The reflections and the case study which will be proposed, pertaining to a recent design experiment for the archaeological area and Antiquarium of Tyndaris, are dedicated to this theme. Over and above any charm exerted by such places, by landscapes in which the ruins appear identical in substance and which sometimes manifest themselves as “sub specie æternitatis”, there are reasons linked to the very profession of architect and to the gashes in the crucible of controversies around the role of history in its contentious relationship with architectural design. That apart, the aporias revealed by Michel Fou…

Entro questa concezione della storia o meglio di una metodologia per la storia che "tenda all'archeologia in quanto descrizione intrinseca del monumento" le opere e i progetti di architettura appaiono come i protagonisti di un'azione drammatica incentrata sull'opposizione tra la permanenza della "struttura" e il fremito del mutamento. Quel fremito che nell'età dell'Umanesimo aveva animato le menti degli architetti affrontando allo stesso modo i campi della filologia e dell'architettura studiando i monumenti antichi come testi allo scopo di "generare nuove forme e dare così vita a una nuova classica tradizione".Settore ICAR/14 - Composizione Architettonica E Urbanain sintesi alle trasformazioni che valgono come fondazione e rinnovamento delle fondazioni stesse.&nbspdi Tindari che si proporranno. Al di là e oltre la suggestione esercitata dai luoghi da paesaggi cui i ruderi appaiono consustanziali e che si manifestano talora "sub specie aeternitatis" vi sono motivi legati al mestiere stesso di architetto e alle lacerazioni vissute nel crogiolo delle polemiche intorno al ruolo della storia nel suo controverso rapporto con il progetto di architettura. Del resto le aporie svelate da Michel Foucault mettendo in discussione quello che si era proposto come progetto di una storia globale avevano dato rilievo alla discontinuità alle fratture alle soglieComporre nuova architettura in rapporto con le vestigia dell'antichità o in ambito archeologico. A questo tema sono dedicate le riflessioni e il caso studio relativo alla recente esperienza progettuale per l’area archeologica e l’Antiquarium&nbsp
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