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Selected AbstractsEvaluation of Ssp I polymerase chain reaction assay in the detection of Wuchereria bancrofti infection in field-collected Culex quinquefasciatus and its application in the transmission studies of lymphatic filariasisJOURNAL OF APPLIED ENTOMOLOGY, Issue 7-8 2002S. L. Hoti The evaluation of the assay was carried out using pools of vector mosquitoes collected from areas under filariasis survey and control trial projects, in comparison with the standard dissection and microscopy technique. In the filariasis survey area the infection rate as determined by the dissection and microscopy technique was 0.89% whereas it was 1.7% by PCR assay. In the Bacillus sphaericus trial area the infection rates as assessed by the conventional technique were 6.6 and 4.5% in the treated and check areas, respectively, whereas those obtained by the PCR assay were 4.7 to 2.2%. Although the infection rates determined by the PCR assay are slightly higher or lower than the rates obtained by the conventional technique, the difference was not statistically significant (P=0.451 for filariasis survey area, and P=0.203 and 0.161 for B. sphaericus trial area). When the pool size of Cx. quinquefasciatus was increased to 50 the sensitivity of the PCR was affected. The changes in infection rates as influenced by the antifilarial chemotherapy were similar when determined by PCR assay and the standard method. The major advantage of the PCR assay over the conventional technique is that thousands of mosquitoes can be processed within a short duration and this attribute has potential application in rapid assessment of disease prevalence and monitoring of the transmission dynamics. [source] Historical and contemporary distributions of carnivores in forests of the Sierra Nevada, California, USAJOURNAL OF BIOGEOGRAPHY, Issue 8 2005William J. Zielinski Abstract Aim, Mammalian carnivores are considered particularly sensitive indicators of environmental change. Information on the distribution of carnivores from the early 1900s provides a unique opportunity to evaluate changes in their distributions over a 75-year period during which the influence of human uses of forest resources in California greatly increased. We present information on the distributions of forest carnivores in the context of two of the most significant changes in the Sierra Nevada during this period: the expansion of human settlement and the reduction in mature forests by timber harvest. Methods, We compare the historical and contemporary distributions of 10 taxa of mesocarnivores in the conifer forests of the Sierra Nevada and southern Cascade Range by contrasting the distribution of museum and fur harvest records from the early 1900s with the distribution of detections from baited track-plate and camera surveys conducted from 1996 to 2002. A total of 344 sample units (6 track plates and 1 camera each) were distributed systematically across c. 3,000,000 ha area over a 7-year period. Results, Two species, the wolverine (Gulo gulo) and the red fox (Vulpes vulpes), present in the historical record for our survey area, were not detected during the contemporary surveys. The distributions of 3 species (fisher [Martespennanti], American marten [M. americana], and Virginia opossum [Didelphisvirginiana]) have substantially changed since the early 1900s. The distributions of fishers and martens, mature-forest specialists, appeared to have decreased in the northern Sierra Nevada and southern Cascade region. A reputed gap in the current distribution of fishers was confirmed. We report for the first time evidence that the distribution of martens has become fragmented in the southern Cascades and northern Sierra Nevada. The opossum, an introduced marsupial, expanded its distribution in the Sierra Nevada significantly since it was introduced to the south-central coast region of California in the 1930s. There did not appear to be any changes in the distributions of the species that were considered habitat generalists: gray fox (Urocyon cinereoargenteus), striped skunk (Mephitis mephitis), western spotted skunk (Spilogale gracilis), or black bear (Ursus americanus). Detections of raccoons (Procyon lotor) and badgers (Taxidea taxus) were too rare to evaluate. Contemporary surveys indicated that weasels (M. frenata and M. erminea) were distributed throughout the study area, but historical data were not available for comparison. Main conclusions, Two species, the wolverine and Sierra Nevada red fox, were not detected in contemporary surveys and may be extirpated or in extremely low densities in the regions sampled. The distributions of the mature forest specialists (marten and fisher) appear to have changed more than the distributions of the forest generalists. This is most likely due to a combination of loss of mature forest habitat, residential development and the latent effects of commercial trapping. Biological characteristics of individual species, in combination with the effect of human activities, appear to have combined to affect the current distributions of carnivores in the Sierra Nevada. Periodic resampling of the distributions of carnivores in California, via remote detection methods, is an efficient means for monitoring the status of their populations. [source] Elephants caught in the middle: impacts of war, fences and people on elephant distribution and abundance in the Caprivi Strip, NamibiaAFRICAN JOURNAL OF ECOLOGY, Issue 2 2009Michael J. Chase Abstract We conducted wet [26 March,4 April 2003 (Apr03)] and dry [1,8 November 2005 (Nov05)] season aerial surveys of African elephants (Loxodonta africana Blumenbach) in the Caprivi Strip, Namibia to provide an updated status report on elephant numbers and distribution and assist with a historical analysis of elephant distribution and abundance in the Caprivi Strip. During the wet season when water was available in seasonal pans, elephants were widely distributed throughout the survey area. In contrast, during the dry season, a majority of elephant herds occurred within 30 km of the perennial Kwando, Linyanti and Okavango rivers and few herds occurred within the West Caprivi Game Reserve where water in the seasonal pans was limited. We estimated 5318 elephants for the 7731-km2 survey area (0.71 elephants km,2) for the Apr03 wet season survey and 6474 elephants for the 8597-km2 survey area (0.75 elephants km,2) for the Nov05 dry season survey. Based on our aerial surveys and reports of elephant numbers and distribution from historical aerial surveys and telemetry studies, civil war, veterinary fences and human activities appear to have effected changes in African elephant abundance, distribution and movements in the Caprivi Strip, Namibia since 1988 when the first comprehensive aerial surveys were conducted. Résumé En saison des pluies (avril 2003) et en saison sèche (novembre 2005), nous avons réalisé des contrôles aériens des éléphants africains (Loxodonta africana Blumenbach) dans la Bande de Caprivi, en Namibie, pour pouvoir fournir un rapport actualisé sur le statut du nombre et de la distribution des éléphants, et aider une analyse de longue durée de la distribution et de l'abondance des éléphants dans la Bande de Caprivi. Pendant la saison des pluies, lorsque l'eau était disponible dans les « pans » saisonniers, les éléphants étaient largement distribués dans toute la zone étudiée. Par contre, en saison sèche, la grande majorité des troupeaux d'éléphants se trouvaient dans les 30 km des rivières permanentes Kwando, Linyanti et Okavango, et peu de troupeaux se trouvaient dans la West Caprivi Game Reserve, où l'eau était limitée dans les pans saisonniers. Nous avons estimé le nombre d'éléphants à 5 318 dans les 7 731 km² de la zone étudiée (0,71 éléphant km,²) pour l'étude faite en saison des pluies d'avril 2003, et à 6 474 éléphants dans les 8 597 km²étudiés (0,75 éléphant km,²) pendant la saison sèche de novembre 2005. En se basant sur nos contrôles aériens et sur des rapports concernant le nombre et la distribution des éléphants provenant de contrôles aériens et d'études télémétriques anciens, il s'avère que la guerre civile, les barrières vétérinaires et les activités humaines ont provoqué des changements de l'abondance, de la distribution et des déplacements des éléphants dans la Bande de Caprivi depuis 1988, date où les premiers contrôles aériens complets ont été effectués. [source] Holocene sedimentation in the Skagerrak interpreted from chirp sonar and core data,JOURNAL OF QUATERNARY SCIENCE, Issue 1 2005Richard Gyllencreutz Abstract High-resolution chirp sonar profiling in the northeastern Skagerrak shows acoustically stratified sediments draping a rough-surfaced substratum. A 32 metre long sediment core retrieved from the survey area encompasses the entire Holocene and latest Pleistocene. The uppermost seismo-acoustic units in the chirp profiles represent Holocene marine sediments. The lowermost unit is interpreted as ice-proximal glacial-marine sediments rapidly deposited during the last deglaciation. The end of ice-proximal sedimentation is marked by a strong reflector, interpreted to have been formed during latest Pleistocene time as a consequence of rapid ice retreat and drastically lowered sedimentation rate. The subsequent distal glacial-marine sediments were deposited with initially high sedimentation rates caused by an isostatic rebound-associated sea-level fall. Based on correlation between the core and the chirp sonar profiles using measured sediment physical properties and AMS 14C dating, we propose a revised position for the Pleistocene/Holocene boundary in the seismo-acoustic stratigraphy of the investigated area. Copyright © 2005 John Wiley & Sons, Ltd. [source] An unbiased pilot survey for Galactic water masersMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Issue 4 2010J. L. Caswell ABSTRACT The Australia Telescope Compact Array has been used in a fast surveying mode to study the 22-GHz transition of water in two small sample regions of the southern Galactic plane. The observations allow an unbiased search for water masers, including any that may have no association with masers from other molecules (or indeed, no association with any other detectable celestial object). Positions with arcsecond accuracy were obtained from the original survey data for detected sources, and these were re-observed at an epoch more than two years later. Variability of the spectra between the epochs was considerable: our total of 32 masers comprises 24 detected at both epochs, two detected at only the first epoch and six detected at only the follow-up epoch. The success of our surveying mode shows it to be a practical strategy for the difficult task of extending unbiased water maser surveys to a large portion of the Galactic plane. Our results show quantitatively the effect of variability on the completeness of surveys conducted at a single epoch. Most of our maser detections are new discoveries. Only four had previously been detected (in searches towards interesting targets in the survey area). The high density of water masers from our unbiased survey supports earlier suggestions that they are the most populous maser species, and one of the most sensitive and reliable tracers of massive young stellar objects , newly forming massive young stars. The spectra of nine masers show high-velocity emission, and they show a striking preponderance of blueshifted high-velocity features. This is compatible with such blueshifts being a characteristic of populations dominated by masers at the earliest evolutionary stage of star formation, in some cases prior to the onset of methanol masers. Amongst the high-velocity emission sources there are two new examples where blueshifted high-velocity outflows dominate the total emission; these substantially increase the previously known meagre population of five such objects and suggest that they may be surprisingly abundant. [source] Error analysis in cross-correlation of sky maps: application to the Integrated Sachs,Wolfe detectionMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Issue 4 2007Anna Cabré ABSTRACT Constraining cosmological parameters from measurements of the Integrated Sachs,Wolfe effect requires developing robust and accurate methods for computing statistical errors in the cross-correlation between maps. This paper presents a detailed comparison of such error estimation applied to the case of cross-correlation of cosmic microwave background (CMB) and large-scale structure data. We compare theoretical models for error estimation with Monte Carlo simulations where both the galaxy and the CMB maps vary around a fiducial autocorrelation and cross-correlation model which agrees well with the current concordance , cold dark matter cosmology. Our analysis compares estimators both in harmonic and configuration (or real) space, quantifies the accuracy of the error analysis and discusses the impact of partial sky survey area and the choice of input fiducial model on dark energy constraints. We show that purely analytic approaches yield accurate errors even in surveys that cover only 10 per cent of the sky and that parameter constraints strongly depend on the fiducial model employed. Alternatively, we discuss the advantages and limitations of error estimators that can be directly applied to data. In particular, we show that errors and covariances from the jackknife method agree well with the theoretical approaches and simulations. We also introduce a novel method in real space that is computationally efficient and can be applied to real data and realistic survey geometries. Finally, we present a number of new findings and prescriptions that can be useful for analysis of real data and forecasts, and present a critical summary of the analyses done to date. [source] Universal fitting formulae for baryon oscillation surveysMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, Issue 1 2006Chris Blake ABSTRACT The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be used as a standard ruler to constrain cosmological parameters and dark energy models. In this paper we present simple analytical fitting formulae for the accuracy with which the preferred scale may be determined in the tangential and radial directions by future spectroscopic and photometric galaxy redshift surveys. We express these accuracies as a function of survey parameters such as the central redshift, volume, galaxy number density and (where applicable) photometric redshift error. These fitting formulae should greatly increase the efficiency of optimizing future surveys, which requires analysis of a potentially vast number of survey configurations and cosmological models. The formulae are calibrated using a grid of Monte Carlo simulations, which are analysed by dividing out the overall shape of the power spectrum before fitting a simple decaying sinusoid to the oscillations. The fitting formulae reproduce the simulation results with a fractional scatter of 7 per cent (10 per cent) in the tangential (radial) directions over a wide range of input parameters. We also indicate how sparse-sampling strategies may enhance the effective survey area if the sampling scale is much smaller than the projected baryon oscillation scale. [source] Geo,tectonic Position of Tin Polymetallic Mineralization Zone in the Southern Da Hinggan Mountains Area, Inner Mongolia, China: An Introduction to This Special IssueRESOURCE GEOLOGY, Issue 4 2001Shihua SUN Abstract: As a part of the main activities of Japan-China technical cooperation project, a test survey area, approximately 5,000 km2, was established for the implement of its geological and geochemical research program. A major mineralization zone called Huanggang,Ganzhuermiao,Wulanhaote Sn-Cu polymetallic mineralization zone is recognized in the southern Da Hinggan Mountains area. The southern half of this zone is known as the sole Sn-mineralization zone in North China. The survey area lies in this prominent zone. As the most of the papers presented in this issue have concerns to the geology and mineralization in this survey area, this report was prepared to introduce geo-tectonic situation of the Sn-Cu polymetallic mineralization zone in the Inner Mongolia orogenic belt. The belt is divided into four tectonic facies (from NW to SE); I: Wuliyasitai volcano-plutonic zone, II: Hegenshan ophiolite mélange zone, III: Sunitezuoqi volcano-plutonic zone, IV: Wenduermiao ophiolite mélange zone. The subject Sn-Cu polymetallic mineralization zone is situated in the southeastern part of the Sunitezuoqi magmatic zone. About this Sunitezuoqi magmatic zone, three geo-tectonic characteristics are pointed out. In late Carboniferous to early Permian period, subduction of Hegenshan oceanic crust occurred, which accelerated volcano-plutonic activities and brought about basic to intermediate volcanic rocks of tholeiitic to calc-alkaline series represented by Dashizhai Group in the Sunitezuoqi magmatic zone. Late Jurassic to early Cretaceous acidic rocks representing the most culminated volcanism and plutonism in Mesozoic era in the Da Hinggan Moutains area are distributed very extensively in and around the Sn-Cu polymetallic mineralization zone. The Proterozoic metamorphic basement rocks called Xilinhaote complex are distributed close to the mineralized area in the Sunitezuoqi magmatic zone. Although the real mineralization was known associated with Mesozoic acidic to intermediate volcano-plutonic activities, it is thought that the lower Permian Dashizhai volcanic rocks and pre-Cambrian basement rocks might have played certain significant role in the process respectively of extraction of elements and formation of the magma favorable for such mineralization in the Sunitezuoqi magmatic zone. It would be necessary to give further considerations to these three geological units in relation to the Sn-Cu polymetallic mineralization. [source] Finding the most variable stars in the Orion Belt with the All Sky Automated SurveyASTRONOMISCHE NACHRICHTEN, Issue 3 2010J.A. Caballero Abstract We look for high-amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS-3 Photometric V -band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and IRAS catalogues, proper motions, and the Aladin sky atlas to obtain a list of the most variable stars in a survey area of side 5° centred on the bright star Alnilam (, Ori) in the centre of the Orion Belt. We identify 32 highly variable stars, of which 16 had not been reported to vary before. They are mostly variable young stars and candidates (16) and background giants (8), but there are also field cataclysmic variables, contact binaries, and eclipsing binary candidates. Of the young stars, which typically are active Herbig Ae/Be and T Tauri stars with H, emission and infrared flux excess, we discover four new variables and confirm the variability status of another two. Some of them belong to the well known , Orionis cluster. Besides, six of the eight giants are new variables, and three are new periodic variables (© 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim) [source] Sediment quality in near coastal waters of the Gulf of Mexico: Influence of Hurricane Katrina,ENVIRONMENTAL TOXICOLOGY & CHEMISTRY, Issue 7 2010John M. Macauley Abstract The results of the present study represent a synoptic analysis of sediment quality in coastal waters of Lake Pontchartrain and Mississippi Sound two months after the landfall of Hurricane Katrina. Posthurricane conditions were compared to prehurricane (2000,2004) conditions, for sediment quality data. There were no exceedances of effects range median (ERM) sediment quality guideline values for chemical contaminants in any of the sediment samples collected from the Lake Pontchartrain or the Mississippi Sound study areas following the hurricane. Lower threshold effects range low (ERL) values were exceeded for As, Cd, and Ni at several stations in both survey areas, similar to levels of contamination observed prior to the hurricane. The comparison of sediment quality indicators before and after the hurricane suggests considerable stability of these systems with respect to short-term ecological impacts. Although other studies have shown storm-related changes could be detected (e.g., effects on benthic communities associated with shifts in salinity), there were no indications of widespread sediment contamination. Environ. Toxicol. Chem. 2010;29:1403,1408. © 2010 SETAC [source] Magnetic survey in the investigation of sociopolitical change at a Late Bronze age fortress settlement in northwestern ArmeniaARCHAEOLOGICAL PROSPECTION, Issue 1 2010Ian Lindsay Abstract The construction of large stone fortresses across much of northern Armenia during the Late Bronze Age (ca. 1500,1150 BC) represented a shift away from centuries of nomadic pastoralism, and also marked a profound transformation in the constitution of political authority and how social orders were mediated through the built environment. To date, however, little archaeological attention has been given to Late Bronze Age (LBA) settlements located outside the fortress citadels, partly due to the difficulty in detecting them from the surface. In this report we highlight results and observations from a magnetic gradiometry survey in northwestern Armenia where we test the hypothesis that an extensive LBA domestic complex existed at the base of the fortified hill at the site of Tsaghkahovit. The study surveyed four grids in the settlement area at the base of fortress. Three test units were excavated in three of the four survey areas to test selected anomalies. Two of the test units confirmed the presence of subsurface LBA deposits, including basalt stone walls, burned features, and a storage pit, appearing in the data as large dipoles. The spatial configurations of buildings revealed by the gradiometry surveys elucidate the extent of the Tsaghkahovit settlement and the formal differentiation of domestic and institutional spaces as new architectural traditions emerge during the Middle to Late Bronze Age transition. However, targeted subsurface tests also hint at the ephemeral nature of the domestic constructions suggesting the retention of mobility among subject populations under the authority of settled fortress elites. Copyright © 2009 John Wiley & Sons, Ltd. [source] | |||||||||||||||||||