Meningitis Associated With B. Proteus.

Wilson, W. James

doi:10.1016/s0140-6736(00)75681-9

Cited by 38 publications

(55 citation statements)

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“…The total number of galaxies in the DR2 for each morphology type is written on each bar. Error bars are computed from the binomial errors of the associated DR2 number counts (Wilson 1927). The morphological distribution of the DR2 sample is similar to that of the mother sample.…”

Section: Observing Strategy and Setup Overviewmentioning

confidence: 99%

CALIFA, the Calar Alto Legacy Integral Field Area survey

García-Benito

Zibetti

Sánchez

et al. 2015

A&A

188

136

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This paper describes the Second Public Data Release (DR2) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. The data for 200 objects are made public, including the 100 galaxies of the First Public Data Release (DR1). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5 m telescope at the Calar Alto observatory. Two different spectral setups are available for each galaxy, (i) a lowresolution V500 setup covering the wavelength range 3745-7500 Å with a spectral resolution of 6.0 Å (FWHM); and (ii) a medium-resolution V1200 setup covering the wavelength range 3650-4840 Å with a spectral resolution of 2.3 Å (FWHM). The sample covers a redshift range between 0.005 and 0.03, with a wide range of properties in the color-magnitude diagram, stellar mass, ionization conditions, and morphological types. All the cubes in the data release were reduced with the latest pipeline, which includes improved spectrophotometric calibration, spatial registration, and spatial resolution. The spectrophotometric calibration is better than 6% and the median spatial resolution is 2. 4. In total, the second data release contains over 1.5 million spectra.

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Section: Observing Strategy and Setup Overviewmentioning

confidence: 99%

CALIFA, the Calar Alto Legacy Integral Field Area survey

García-Benito

Zibetti

Sánchez

et al. 2015

A&A

188

136

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show abstract

“…As shown in the figure, the difference in average fraction of nucleating polymorph between the two reference series 1 and 2 is small. Statistically no difference can be established, using 95% confidence limits calculated by the Wilson equation 44 without correction for continuity. Since the same applies to the average nucleation temperatures of both polymorphs, it appears that by employing a superheating temperature of 10 °C for 6 hours, a reference state is created where at least the effect of the dissolved polymorph has disappeared.…”

Section: Influence Of Solution Pre-treatment On the Nucleating Polymorphmentioning

confidence: 99%

Influence of Solution Thermal and Structural History on the Nucleation of m-Hydroxybenzoic Acid Polymorphs

Nordström

Svärd

Malmberg

et al. 2012

Crystal Growth & Design

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The influence of solution pre-treatment on primary nucleation of m-hydroxybenzoic acid has been investigated through 550 cooling crystallization experiments. The metastable zone width has been determined at constant cooling rate and the time and temperature of the preceding superheating step have been varied. m-Hydroxybenzoic acid has two polymorphs and the influence of the polymorph used to prepare the solutions has also been investigated. There is an overall tendency in the experiments for the solution to exhibit a larger metastable zone width if it is superheated for a longer time and at a higher temperature, but under the investigated conditions this tendency is not very strong. The results show that the metastable form II preferentially crystallizes in all experiments and in particular when the solution has been more strongly superheated for several hours. However, when the time and/or the temperature of superheating is reduced there is an increasing tendency to obtain the stable form I. This is most clearly found for solutions prepared by dissolving form I. When the solutions are prepared by dissolution of form II, this tendency is weaker in what appears to be a systematic way. It is hypothesized that, unless the solution is strongly superheated for several hours, it will contain for a significant period of time clusters of solute molecules which can retain some degree of structure from the dissolved crystal. This leads to "memory" effects in the solution which may influence subsequent nucleation. The work includes a comprehensive review of previous published work on the influence of thermal history on nucleation in solutions and melts.

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“…The error bars are obtained with the Wilson (1927) formula. 11 Both versions of MAGGIE lead to fragmentation of typically 15%, even when realistic errors on galaxy luminosities and stellar masses are considered.…”

Section: Fragmentationmentioning

confidence: 99%

maggie: Models and Algorithms for Galaxy Groups, Interlopers and Environment

Duarte¹,

Mamon²

2015

Mon. Not. R. Astron. Soc.

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Combining our knowledge of halo structure and internal kinematics from cosmological dark matter simulations and the distribution of halo interlopers in projected phase space measured in cosmological galaxy simulations, we develop MAGGIE, a prior-and halo-based, probabilistic, abundance matching (AM) grouping algorithm for doubly complete subsamples (in distance and luminosity) of flux-limited samples. We test MAGGIE-L and MAGGIE-M (in which group masses are derived from AM applied to the group luminosities and stellar masses, respectively) on groups of at least three galaxies extracted from a mock Sloan Digital Sky Survey Legacy redshift survey, incorporating realistic observational errors on galaxy luminosities and stellar masses. In comparison with the optimal Friends-of-Friends (FoF) group finder, groups extracted with MAGGIE are much less likely to be secondary fragments of true groups; in primary fragments, its galaxy memberships (relative to the virial sphere of the realspace group) are much more complete and usually more reliable, and its masses are much less biased and usually with less scatter, as are its group luminosities and stellar masses (computed in MAGGIE using the membership probabilities as weights). FoF outperforms MAGGIE only for high-mass clusters: for the reliability of the galaxy population and the dispersion of its total mass. In comparison with our implementation of the Yang et al. group finder, MAG-GIE reaches much higher completeness and slightly lower group fragmentation and dispersion on group total masses, luminosities and stellar masses, but slightly greater bias in the latter two and lower reliabilities. MAGGIE should therefore lead to sharper trends of environmental effects on galaxies and more accurate mass/orbit modelling.

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Meningitis Associated With B. Proteus.

Cited by 38 publications

References 0 publications

CALIFA, the Calar Alto Legacy Integral Field Area survey

CALIFA, the Calar Alto Legacy Integral Field Area survey

Influence of Solution Thermal and Structural History on the Nucleation of m-Hydroxybenzoic Acid Polymorphs

maggie: Models and Algorithms for Galaxy Groups, Interlopers and Environment

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