First Sagittarius A* Event Horizon Telescope results. II. EHT and multiwavelength observations, data processing, and calibration

We present Event Horizon Telescope (EHT) 1.3 mm measurements of the radio source located at the position of the supermassive black hole Sagittarius A* (Sgr A*), collected during the 2017 April 5–11 campaign. The observations were carried out with eight facilities at six locations across the globe. Novel calibration methods are employed to account for Sgr A*'s flux variability. The majority of the 1.3 mm emission arises from horizon scales, where intrinsic structural source variability is detected on timescales of minutes to hours. The effects of interstellar scattering on the image and its variability are found to be subdominant to intrinsic source structure. The calibrated visibility amplitudes, particularly the locations of the visibility minima, are broadly consistent with a blurred ring with a diameter of ∼50 μas, as determined in later works in this series. Contemporaneous multiwavelength monitoring of Sgr A* was performed at 22, 43, and 86 GHz and at near-infrared and X-ray wavelengths. Several X-ray flares from Sgr A* are detected by Chandra, one at low significance jointly with Swift on 2017 April 7 and the other at higher significance jointly with NuSTAR on 2017 April 11. The brighter April 11 flare is not observed simultaneously by the EHT but is followed by a significant increase in millimeter flux variability immediately after the X-ray outburst, indicating a likely connection in the emission physics near the event horizon. We compare Sgr A*'s broadband flux during the EHT campaign to its historical spectral energy distribution and find that both the quiescent emission and flare emission are consistent with its long-term behavior.http://iopscience.iop.org/2041-8205Physic

First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration

We present Event Horizon Telescope (EHT) 1.3 mm measurements of the radio source located at the position of the supermassive black hole Sagittarius A* (Sgr A*), collected during the 2017 April 5–11 campaign. The observations were carried out with eight facilities at six locations across the globe. Novel calibration methods are employed to account for Sgr A*'s flux variability. The majority of the 1.3 mm emission arises from horizon scales, where intrinsic structural source variability is detected on timescales of minutes to hours. The effects of interstellar scattering on the image and its variability are found to be subdominant to intrinsic source structure. The calibrated visibility amplitudes, particularly the locations of the visibility minima, are broadly consistent with a blurred ring with a diameter of ∼50 μas, as determined in later works in this series. Contemporaneous multiwavelength monitoring of Sgr A* was performed at 22, 43, and 86 GHz and at near-infrared and X-ray wavelengths. Several X-ray flares from Sgr A* are detected by Chandra, one at low significance jointly with Swift on 2017 April 7 and the other at higher significance jointly with NuSTAR on 2017 April 11. The brighter April 11 flare is not observed simultaneously by the EHT but is followed by a significant increase in millimeter flux variability immediately after the X-ray outburst, indicating a likely connection in the emission physics near the event horizon. We compare Sgr A*’s broadband flux during the EHT campaign to its historical spectral energy distribution and find that both the quiescent emission and flare emission are consistent with its long-term behavior

Dynamic of autochthonous malaria transmission in the Atlantic Forest: analysis of variation in Anopheles cruzii (Diptera: Culicidae) acrodendrophilic behavior and development of a mathematical model for zoonotic transmission

A Malária autóctone de Mata Atlântica é caracterizada por baixa incidência de casos com pouca ou nenhuma manifestação clínica e baixa parasitemia, tendo como principal agente etiológico o Plasmodium vivax (ou plasmódios muito semelhantes a este). O principal mosquito envolvido na transmissão é o Anopheles (Kerteszia) cruzii, cujas formas imaturas se desenvolvem na água acumulada nas imbricações das folhas de bromélias, vegetal muito abundante neste bioma. As formas adultas de An. cruzii tendem a viver e se alimentar com maior frequência na copa das árvores, comportamento conhecido como acrodendrofilia, no entanto, em diversas situações esta espécie tem sido observada em elevada densidade no estrato inferior da floresta. Evidências sugerem que a malária possa ser transmitida de forma zoonótica nestas áreas, uma vez que primatas das famílias Atelidae e Cebidae são encontrados portando plasmódios muito próximos geneticamente aos que infectam humanos e An. cruzii pode se alimentar do sangue de ambos os hospedeiros. O presente estudo teve como objetivo investigar a influência da composição e configuração da paisagem sobre as variações na abundância e no comportamento acrodendrófilo de An. cruzii e como estas variações atuam sobre a dinâmica de transmissão de malária na Mata Atlântica, considerando um cenário de transmissão zoonótica. Coletas entomológicas mensais foram conduzidas no período de março de 2015 a abril de 2017 em duas unidades de conservação situadas no município de São Paulo, ambas com histórico de malária autóctone. Em cada área foram selecionados pontos de coleta com diferentes graus de interferência antrópica e os mosquitos foram coletados utilizando armadilhas do tipo CDC e Shannon. Métricas de composição e configuração da paisagem foram mensuradas para cada ponto de estudo e modelos estatísticos foram utilizados para avaliar a relação entre estas métricas e variações na abundância e acrodendrofilia de An. cruzii. Foi proposto um modelo matemático de transmissão zoonótica que permitiu observar, por meio de simulações, como a dinâmica de transmissão da malária é influenciada por variações na abundância e acrodendrofilia do vetor. Os resultados obtidos sugerem que a perda de vegetação natural e aumento das áreas de borda levam a uma redução na abundância de An. cruzii mas favorecem uma maior atividade desta espécie próximo ao solo. As análises baseadas no modelo teórico corroboram com observações anteriores, apontando que as variações na acrodendrofilia do vetor podem ter um papel importante na dinâmica de transmissão de plasmódios entre símios e humanos na Mata Atlântica. Em condições nas quais An. cruzii tende a se alimentar quase exclusivamente na copa das árvores ou quase exclusivamente próximo ao solo a transmissão zoonótica parece não se sustentar, ainda que a abundância do vetor seja elevada. De outra forma, condições nas quais An. cruzii se desloque com maior frequência entre os estratos copa e solo tendem a favorecer a transmissão zoonótica, sendo que quanto maior o deslocamento menor é a abundância relativa do vetor necessária para que um símio infectado gere mais do que um caso novo na população de humanos suscetível ou vice-versa.The autochthonous Malaria of the Atlantic Forest is characterized by a low incidence of cases with little or no clinical manifestation and low charge of parasites in the blood stream, being Plasmodium vivax (or plasmodiums very similar to it) the main etiologic agent. The main mosquito involved in transmission is the Anopheles (Kerteszia) cruzii, whose immature forms develop in the water held in bromeliads, which are very abundant plants in this biome. The adult forms of An. cruzii prefer to live and feed on the treetops, a behavior known as acrodendrophily, however, in several situations this species has been observed in high density near the ground of the forest. Some evidences suggest that malaria can be transmitted zoonotically in these areas, since monkeys of Atelidae and Cebidae families are found carrying plasmodiums very close to those that infect humans and An. cruzii can feed on the blood of both hosts. This study aimed to investigate the influence of the landscape composition and configuration on the variations in the abundance and acrodendrophic behavior of An. cruzii and how these variations affect the dynamics of malaria transmission in the Atlantic Forest, considering a zoonotic transmission scenario. Monthly entomological collections were conducted from March 2015 to April 2017 in two conservation units located in the municipality of São Paulo, Brazil, where human and simian malaria occurs. In each area, collection points with different degrees of anthropic intervention were selected and mosquitoes were collected using CDC and Shannon traps. Metrics of landscape composition and configuration were measured for each study point and generalized linear models were used to evaluate the relationship between these metrics and variations in abundance and acrodendrophily of An. cruzii. It was proposed a mathematical model of zoonotic transmission that allowed to observe, through simulations, how the dynamics of malaria transmission is influenced by variations in the abundance and acrodendrophily of the vector. The results suggest that loss of natural vegetation and increase in edge effect lead to a reduction in the abundance of An. cruzii but favor a higher activity of this species near the ground level. The analyzes based on the theoretical model corroborate previous observations, pointing out that the variations in the acrodendrophily of the vector may play an important role in the dynamics of plasmodium transmission between monkeys and humans in the Atlantic Forest. In situations in which An. cruzii seeks to feed almost exclusively on the treetops or in situations where it feeds almost exclusively near the ground, the zoonotic transmission does not seem to occur, even in situations of high abundance of the vector. Otherwise, conditions in which An. cruzii moves more frequently between canopy and ground level tend to favor zoonotic transmission, and the more vertical movement occurs, the lower is the needed relative abundance of the vector for an infected monkey to generate more than a new case in the susceptible human population or vice versa

Study of diversity patterns of mosquitoes (Diptera: Culicidae) in urban parks in the city of São Paulo

Na medida em que o homem altera processos ecológicos e pressiona os ambientes naturais, cresce também o risco de contato com agentes patogênicos provenientes desses meios, muitos dos quais podem ser veiculados por mosquitos. A cidade de São Paulo possui uma centena de parques públicos que preservam remanescentes da flora e fauna e são utilizados pela população como espaços de lazer. Pouco se sabe sobre os padrões de diversidade de culicídeos que habitam estas áreas e tal ausência de dados inviabiliza predições e inferências sobre processos ecológicos atuantes ou riscos epidemiológicos inerentes. Este trabalho teve como objetivo descrever e analisar os padrões de diversidade das assembleias de culicídeos em parques urbanos da cidade. Mosquitos adultos e Imaturos foram coletados entre 2011/2012 e 2012/2013 em dez parques urbanos da cidade: Alfredo Volpi, Anhanguera, Burle Marx, Carmo, Chico Mendes, Ibirapuera, Piqueri, Previdência, Santo Dias e Sangrilá. Ao todo foram realizadas doze coletas em cada parque ao longo de um ano. Após identificação das espécies foram calculados riqueza, abundância e índices de diversidade por coleta em cada parque. Testes estatísticos foram aplicados para verificar diferenças significantes entre os parques e períodos do ano em relação aos parâmetros de diversidade mensurados. Verificou-se a similaridade na composição de espécies para os parques e tipos de criadouros e foram testadas associações entre parâmetros ambientais em relação à diversidade alfa e beta. Ao longo do estudo foram coletadas 81 espécies/táxons nos dez parques pesquisados. As espécies mais comuns e abundantes foram Ae. albopictus, Ae. scapularis, Ae. fluviatilis, Cx. quinquefasciatus e Cx. nigripalpus, todas de interesse epidemiológico. O Anhanguera apresentou a maior riqueza e o Shangrilá a maior diversidade. Ibirapuera e Alfredo Volpi apresentaram a menor riqueza e diversidade respectivamente. As assembleias mostraram variações nos padrões de diversidade na comparação entre os meses mais quentes e chuvosos em relação aos meses mais frios e secos. Foi demonstrado que diferenças ambientais entre os parques podem influenciar a riqueza e composição de espécies. O Processo de seleção mostrou ser um importante fator-chave na formação dos padrões de riqueza e composição de culicídeos dos parques. Aparentemente, a perda de espécies pode promover uma homogeneização na composição de culicídeos ao longo dos parques, onde poucas espécies resilientes permanecem no ambiente e destas a maioria apresenta importância médico-epidemiológica. O contato entre mosquitos vetores, animais reservatórios e a população que utiliza os parques pode promover epizootias e o estabelecimento de ciclos de transmissão em nosso meio, recomenda-se constante vigilância epidemiológica.Human activities and population growth leads to fragmentation and isolation of natural environments, triggering key alterations on organisms diversity in these locations. To the extent that man interferes with ecological processes and natural environments, increases the risk of contact with pathogens from those places, many of which can be transmitted by mosquitoes. The city of Sao Paulo has a hundred public parks that preserve remnants of flora and fauna and are used by the population as recreational spaces. Little is known about culicid diversity patterns whitin these areas and this lack of data precludes predictions and inferences about ecological processes and risks of vector-borne diseases. This study aimed to describe and analyze the diversity patterns of culicids assemblages in urban parks of the city. Immature and adult mosquitoes were collected between 2011/2012 and 2012/2013 in ten urban parks: Alfredo Volpi, Anhanguera, Burle Marx, Carmo, Chico Mendes, Ibirapuera, Piqueri, Previdência, Santo Dias and Sangrila. Altogether twelve samplings were performed at each park throughout a year. After species identification were calculated richness, abundance and Shannon e Simpson index for each park and replica. Statistical tests were applied to verify significant differences between parks and seasons of the year in relation to diversity parameters. Similarity were calculated for species composition between parks and type of breeding sites and associations between environmental parameters were tested for alpha and beta diversity. Over the study 81 species / taxa were collected in all the ten parks surveyed. The most common and abundant species were Ae. albopictus, Ae. scapularis, Ae. fluviatilis, Cx. quinquefasciatus and Cx. nigripalpus, epidemiologically important vectors. The Anhanguera was the richest park in species and the Shangrilá park showed the highest diversity. Ibirapuera and Alfredo Volpi showed the lowest richness and diversity respectively. The assemblages showed variations in the comparison between the warmer and rainier months compared to colder and drier ones. We found that environmental differences between parks can influence the species richness and composition. The Selection process proved to be an important key factor in shaping patterns of richness and culicids composition in parks of the city. Apparently, the decrease in the amount of species can promote a homogenization in culicids composition over urban parks, where few resilient species remain in the environment and the majority of these have medical and epidemiological importance. The interaction between vector mosquitoes, reservoirs and people can promote epizootic events and the establishment of transmission cycles in urban environments, it is recommended constant epidemiological surveillance

Composition and diversity of mosquitoes (Diptera: Culicidae) in urban parks in the South region of the city of São Paulo, Brazil

Abstract Many parks in the city of São Paulo contain remnants of Atlantic Forest. Of the 30 municipal parks in the South of the city, we investigated two in this study (Santo Dias Park and Shangrilá Park) in order to survey their mosquito fauna and investigate the presence of potential bioindicators of environmental conditions and vectors of human pathogens. Mosquitoes were collected monthly between March 2011 and February 2012 using aspirators, Shannon and CDC traps for adult mosquitoes and larval dippers and suction samplers for immature forms. Sampling effort was evaluated by plotting a species accumulation curve, and total richness was estimated using the first-order jackknife. To compare the diversity between the two parks Shannon and Simpson diversity indexes were calculated. Species similarity was compared by the Sorensen similarity index. In all, 8,850 specimens were sampled in both parks. Collections in Santo Dias Park yielded 1,577 adult mosquitoes and 658 immature individuals distributed in seven genera (Aedes, Anopheles, Culex, Limatus, Mansonia, Toxorhynchites and Wyeomyia) and 27 taxonomic units. Among the adult mosquitoes collected, Culex nigripalpus .and Aedes fluviatilis were the most abundant, while the most abundant immature forms were Cx. imitator, Wy. davisi, Wy. galvaoi and Ae. albopictus. Collections in Shangrilá Park yielded 4,952 adult specimens and 1,663 immature forms distributed in eight genera (Aedes, Anopheles, Culex, Limatus, Mansonia, Toxorhynchites, Uranotaenia and Wyeomyia) and 36 taxonomic units. Species accumulation curves in both parks were close to the asymptote, and the total richness estimate was close to the observed richness. Although the observed species richness was higher in the Shangrilá Park, there was no statistically significant difference between the diversity indexes measured. Regarding species composition, the two sites shared 16 species, including those of epidemiological importance such as Culex nigripalpus, Cx. quinquefasciatus, Aedes albopictus and Ae. aegypti. As some of the mosquito taxa found are bioindicators of environmental conditions and have epidemiological potential to carry pathogens, we recommend that urban parks should be included in official mosquito surveillance programs, and regular surveys carried out to detect circulating arboviruses

First M87 Event Horizon Telescope Results. II. Array and Instrumentation

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of similar to 1.3 mm, EHT angular resolution (lambda/D) is similar to 25 mu as, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of the EHT, detail the technology and instrumentation that enable observations, and provide measures of its performance. Meeting the EHT science objectives has required several key developments that have facilitated the robust extension of the VLBI technique to EHT observing wavelengths and the production of instrumentation that can be deployed on a heterogeneous array of existing telescopes and facilities. To meet sensitivity requirements, high-bandwidth digital systems were developed that process data at rates of 64. gigabit s(-1), exceeding those of currently operating cm-wavelength VLBI arrays by more than an order of magnitude. Associated improvements include the development of phasing systems at array facilities, new receiver installation at several sites, and the deployment of hydrogen maser frequency standards to ensure coherent data capture across the array. These efforts led to the coordination and execution of the first Global EHT observations in 2017 April, and to event-horizon-scale imaging of the supermassive black hole candidate in M87

Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

3C 279 is an archetypal blazar with a prominent radio jet that show broadband flux density variability across the entire electromagnetic spectrum. We use an ultra-high angular resolution technique - global Very Long Baseline Interferometry (VLBI) at 1.3 mm (230 GHz) - to resolve the innermost jet of 3C 279 in order to study its fine-scale morphology close to the jet base where highly variable gamma -ray emission is thought to originate, according to various models. The source was observed during four days in April 2017 with the Event Horizon Telescope at 230 GHz, including the phased Atacama Large Millimeter/submillimeter Array (ALMA), at an angular resolution of similar to 20 mu as (at a redshift of z=0.536 this corresponds to similar to 0.13 pc similar to 1700 Schwarzschild radii with a black hole mass M-BH=8x10(8) M-circle dot). Imaging and model-fitting techniques were applied to the data to parameterize the fine-scale source structure and its variation. We find a multicomponent inner jet morphology with the northernmost component elongated perpendicular to the direction of the jet, as imaged at longer wavelengths. The elongated nuclear structure is consistent on all four observing days and across different imaging methods and model-fitting techniques, and therefore appears robust. Owing to its compactness and brightness, we associate the northern nuclear structure as the VLBI "core". This morphology can be interpreted as either a broad resolved jet base or a spatially bent jet. We also find significant day-to-day variations in the closure phases, which appear most pronounced on the triangles with the longest baselines. Our analysis shows that this variation is related to a systematic change of the source structure. Two inner jet components move non-radially at apparent speeds of similar to 15 c and similar to 20 c (similar to 1.3 and similar to 1.7 mu as day(-1), respectively), which more strongly supports the scenario of traveling shocks or instabilities in a bent, possibly rotating jet. The observed apparent speeds are also coincident with the 3C 279 large-scale jet kinematics observed at longer (cm) wavelengths, suggesting no significant jet acceleration between the 1.3 mm core and the outer jet. The intrinsic brightness temperature of the jet components are less than or similar to 10(10) K, a magnitude or more lower than typical values seen at >= 7 mm wavelengths. The low brightness temperature and morphological complexity suggest that the core region of 3C 279 becomes optically thin at short (mm) wavelengths

3C 279 Event Horizon Telescope imaging

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution.' (bibcode: 2020A&A...640A..69K

First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

Abstract We present the first Event Horizon Telescope (EHT) observations of Sagittarius A* (Sgr A*), the Galactic center source associated with a supermassive black hole. These observations were conducted in 2017 using a global interferometric array of eight telescopes operating at a wavelength of λ = 1.3 mm. The EHT data resolve a compact emission region with intrahour variability. A variety of imaging and modeling analyses all support an image that is dominated by a bright, thick ring with a diameter of 51.8 ± 2.3 μas (68% credible interval). The ring has modest azimuthal brightness asymmetry and a comparatively dim interior. Using a large suite of numerical simulations, we demonstrate that the EHT images of Sgr A* are consistent with the expected appearance of a Kerr black hole with mass ∼4 × 106 M ⊙, which is inferred to exist at this location based on previous infrared observations of individual stellar orbits, as well as maser proper-motion studies. Our model comparisons disfavor scenarios where the black hole is viewed at high inclination (i &gt; 50°), as well as nonspinning black holes and those with retrograde accretion disks. Our results provide direct evidence for the presence of a supermassive black hole at the center of the Milky Way, and for the first time we connect the predictions from dynamical measurements of stellar orbits on scales of 103–105 gravitational radii to event-horizon-scale images and variability. Furthermore, a comparison with the EHT results for the supermassive black hole M87* shows consistency with the predictions of general relativity spanning over three orders of magnitude in central mass.</jats:p