2,100 research outputs found

    Gravitational lens candidates in the E-CDFS

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    We report ten lens candidates in the E-CDFS from the GEMS survey. Nine of the systems are new detections and only one of the candidates is a known lens system. For the most promising five systems including the known lens system, we present results from preliminary lens mass modelling, which tests if the candidates are plausible lens systems. Photometric redshifts of the candidate lens galaxies are obtained from the COMBO-17 galaxy catalog. Stellar masses of the candidate lens galaxies within the Einstein radius are obtained by using the zz-band luminosity and the V−zV-z color-based stellar mass-to-light ratios. As expected, the lensing masses are found to be larger than the stellar masses of the candidate lens galaxies. These candidates have similar dark matter fractions as compared to lenses in SLACS and COSMOS. They also roughly follow the halo mass-stellar mass relation predicted by the subhalo abundance matching technique. One of the candidate lens galaxies qualifies as a LIRG and may not be a true lens because the arc-like feature in the system is likely to be an active region of star formation in the candidate lens galaxy. Amongst the five best candidates, one is a confirmed lens system, one is a likely lens system, two are less likely to be lenses and the status of one of the candidates is ambiguous. Spectroscopic follow-up of these systems is still required to confirm lensing and/or for more accurate determination of the lens masses and mass density profiles.Comment: 12 pages, 5 figures, 3 tables, ApJ accepte

    Diversity of Mosquitoes in Jalna urban, Maharashtra State, India

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    Present paper deals with the study of diversity of mosquitoes in Jalna urban of Maharashtra state in one year that is from June 2008 to May 2009. During a period of two years a total number of 1998 mosquitoes were collected and examined. Percentage density of different genera was found as Anopheles-64.71%; Aedes-19.61%; Culex-11.61% and Mansonia-4.05%

    Study of Ciliate Commensals from the Gills of Freshwater Bivalves (Molluscs: Bivalvia) of Jayakwadi Dam, Paithan, (M.S.), India

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    Samples of bivalve species viz. Lamillidens marginalis L. corrianus and Indonaia caeruleus were collected from the Jayekwadi dam. Three species of obligate commensalistic ciliates, Conchophthirus acuminatus, C. curtus and C. nikamentus n.sp. belonging to genus Conchophthirus were observed on the gills and mantle cavity of bivalve. Prevalence of the ciliate infection were reported for all three species of bivalves and Conchophthirus.  Correlation of infection intentisity with the length of shell in three species of bivalves were studied

    Percentage Prevalence of Eimerian Species Composition of Sheep and Goats from Beed District, Maharashtra

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    During the present study ten specimens of Eimeria from sheep and twelve species of Eimeria from goats were encountered. The relative prevalence of the sheep and goats are analysed

    Particle Detection by Evaporation from Superfluid Helium

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    We report the first experiments in which 5-MeV alpha particles are detected via evaporation from a bath of superfluid helium. The α excites phonons and rotons in the liquid helium, and these excitations are sufficiently energetic to evaporate helium atoms when they reach the free surface of the liquid. The approximate overall efficiency of this process has been determined, and we compare this with expectations. We have also been able to detect evaporation induced by a flux of γ’s from a 137Cs source

    SOME CHANGES REQUIRED TO INCREASE THE PUBLIC'S UTILIZATION OF PREVENTIVE DENTISTRY *

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    Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/65250/1/j.1752-7325.1968.tb03923.x.pd

    Removal of superfluid helium films from surfaces below 0.1 K

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    We have constructed an apparatus that is able to maintain a helium‐free surface at low temperature (T≀0.1 K) in a cell containing superfluid helium. We discuss the considerations involved in the design of this device, and describe tests that we have made to confirm that a film‐free surface has been produced

    Phonon amplification using evaporation and adsorption of helium

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    We report the results of experiments designed to investigate the feasibility of amplifying a phonon signal using the evaporation of helium from a superfluid film and its subsequent readsorption onto a helium-free surface. We envision a multistage amplifier in which helium is evaporated from a wafer with a helium film only on one side and then adsorbed onto the film-free surface of a similar wafer. The phonons created by the adsorption reach the film on the opposite side of the wafer and potentially desorb more helium than was evaporated by the first wafer. The amplification would come from the high ratio of the binding energy of a helium atom to a film-free surface relative to the binding energy to the liquid. A number of experiments are reported that investigate the efficiencies of the individual steps of the process. The gain per stage is found to be about 3 for high-energy densities in which multiphonon processes are possible. At low-energy densities, the energy deposited into a film-free wafer is found to be less than the original input energy, with the ratio of output to input energy 0.2. Since in applications requiring amplification the phonon density produced by the adsorption of helium on a wafer will be low, the configuration we have studied—phonons produced in silicon coated with a saturated He4 film—will not result in amplification. However, other configurations might improve the efficiency enough to make an amplifier possible

    Angular Distribution of Rotons Generated by Alpha Particles in Superfluid Helium: A Possible Tool for Low Energy Particle Detection

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    We report measurements of the distribution of rotons generated by α particles interacting in a bath of superfluid helium. The roton flux is found to be anisotropic; it is about 4 times larger transverse to the track direction than along it. This asymmetry may provide a powerful tool in particle and astrophysics experiments where sensitivity to low energy recoil track direction is important
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