9,105 research outputs found
Product identification techniques used as training aids for analytical chemists
Laboratory staff assistants are trained to use data and observations of routine product analyses performed by experienced analytical chemists when analyzing compounds for potential toxic hazards. Commercial products are used as examples in teaching the analytical approach to unknowns
Reasons to Ban? The Anti-Burqa Movement in Western Europe
Originally published at http://www.mmg.mpg.de/en/publications/working-papers/2012/
'Our Working Papers are refereed and may be downloaded from this site by individuals, for their own use, subject to the ordinary rules governing the fair use of professional scholarship. Working Papers may be cited without seeking prior permission from the author.
First gravitational lensing mass estimate of a damped Lyman-alpha galaxy at z=2.2
We present the first lensing total mass estimate of a galaxy, at redshift
2.207, that acts as a gravitational deflector and damped Lyman-alpha absorber
on the background QSO SDSS J1135-0010, at redshift 2.888. The remarkably small
projected distance, or impact parameter, between the lens and the source has
been estimated to be 0.8 +/- 0.1 kpc in a recent work. By exploiting the Sloan
Digital Sky Survey database, we establish a likely lensing magnification signal
in the photometry of the QSO. This is determined to be 2.2 mag brighter (or 8
times more luminous) than the median QSO at comparable redshifts. We describe
the total mass distribution of the lens galaxy with a one-component singular
isothermal sphere model and contrast the values of the observed and
model-predicted magnification factors. For the former, we use conservatively
the photometric data of the 95% of the available distant QSO population. We
estimate that the values of the lens effective velocity dispersion and
two-dimensional total mass, projected within a cylinder with radius equal to
the impact parameter, are included between 60 and 170 km/s and 2.1 x 10^9 and
1.8 x 10^10 M_Sun, respectively. We conclude by remarking that analyses of this
kind are crucial to exploring the relation between the luminous and dark matter
components of galaxies in the high-redshift Universe.Comment: 5 pages, 3 figures, accepted by MNRA
Detection of GRB signals with Fluorescence Detectors
Gamma Ray Bursts are being searched in many ground based experiments
detecting the high energy component (GeV TeV energy range) of the photon
bursts. In this paper, Fluorescence Detectors are considered as possible
candidate devices for these searches. It is shown that the GRB photons induce
fluorescence emission of UV photons on a wide range of their spectrum. The
induced fluorescence flux is dominated by GRB photons from 0.1 to about 100 MeV
and, once the extinction through the atmosphere is taken into account, it is
distributed over a wide angular region. This flux can be detected through a
monitor of the diffuse photon flux, provided that its maximum value exceeds a
threshold value, that is primarily determined by the sky brightness above the
detector. The feasibility of this search and the expected rates are discussed
on the basis of the current GRB observations and the existing fluorescence
detectors.Comment: 16 pages 9 eps figure
Numerical simulations challenged on the prediction of massive subhalo abundance in galaxy clusters: the case of Abell 2142
In this Letter we compare the abundance of member galaxies of a rich, nearby
() galaxy cluster, Abell 2142, with that of halos of comparable virial
mass extracted from sets of state-of-the-art numerical simulations, both
collisionless at different resolutions and with the inclusion of baryonic
physics in the form of cooling, star formation, and feedback by active galactic
nuclei. We also use two semi-analytical models to account for the presence of
orphan galaxies. The photometric and spectroscopic information, taken from the
Sloan Digital Sky Survey Data Release 12 (SDSS DR12) database, allows us to
estimate the stellar velocity dispersion of member galaxies of Abell 2142. This
quantity is used as proxy for the total mass of secure cluster members and is
properly compared with that of subhalos in simulations. We find that simulated
halos have a statistically significant ( sigma confidence level)
smaller amount of massive (circular velocity above )
subhalos, even before accounting for the possible incompleteness of
observations. These results corroborate the findings from a recent strong
lensing study of the Hubble Frontier Fields galaxy cluster MACS J0416
\citep{grillo2015} and suggest that the observed difference is already present
at the level of dark matter (DM) subhalos and is not solved by introducing
baryonic physics. A deeper understanding of this discrepancy between
observations and simulations will provide valuable insights into the impact of
the physical properties of DM particles and the effect of baryons on the
formation and evolution of cosmological structures.Comment: 8 pages, 2 figures. Modified to match the version published in ApJ
The frozen state in the liquid phase of side-chain liquid-crystal polymers
International audienceQuenched isotropic melts of side-chain liquid-crystal polymers reveal surprisingly an anisotropic polymer conformation. This small-angle neutron-scattering (SANS) result is consistent with the identification of a macroscopic, solidlike response in the isotropic phase. Both experiments (rheology and SANS) indicate that the polymer system appears frozen on millimeter length scales and at the time scales of the observation. This result implies that the flow behavior is not the terminal behavior and that cross-links or entanglements are not a necessary condition to provide elasticity in melts
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