336 research outputs found
Distant galaxy clusters in the COSMOS field found by HIROCS
We present the first high-redshift galaxy cluster candidate sample from the
HIROCS survey found in the COSMOS field. It results from a combination of
public COSMOS with proprietary H-band data on a 0.66 square degree part of the
COSMOS field and comprises 12 candidates in the redshift range 1.23 < z < 1.55.
We find an increasing fraction of blue cluster members with increasing
redshift. Many of the blue and even some of the reddest member galaxies exhibit
disturbed morphologies as well as signs of interaction.Comment: 5 pages, 5 figures, in print format, accepted for publication by A&A
Letter
Transmission of Dientamoeba fragilis: pinworm or cysts?
Recently, conflicting evidence has been published on the mode of transmission of the trichomonad Dientamoeba fragilis. Detection of D. fragilis DNA inside Enterobius vermicularis eggs agrees with the prediction of Dobell in 1940 that the eggs of a nematode act as a vector for transmission. However, the identification of a cyst stage of D. fragilis in the stool of rodents infected with a human isolate has also been reported, and this implies a life cycle similar to those of most other intestinal protistan parasites. Herein we discuss the recent data, identify gaps in the experimental evidence, and propose a method for determining which view of the life cycle of this organism is correct
Extending the first-order post-Newtonian scheme in multiple systems to the second-order contributions to light propagation
In this paper, we extend the first-order post-Newtonian scheme in multiple
systems presented by Damour-Soffel-Xu to the second-order contribution to light
propagation without changing the virtueof the scheme on the linear partial
differential equations of the potential and vector potential. The spatial
components of the metric are extended to second order level both in a global
coordinates () and a local coordinates (). The
equations of (or ) are obtained from the field equations.The
relationship between and are presented in this paper also. In
special case of the solar system (isotropic condition is applied ()), we obtain the solution of . Finally, a further extension
of the second-order contributions in the parametrized post-Newtonian formalism
is discussed.Comment: Latex2e; 6 pages PS fil
Radial velocities for the Hipparcos-Gaia Hundred-Thousand-Proper-Motion project
(abridged) The Hundred-Thousand-Proper-Motion (HTPM) project will determine
the proper motions of ~113500 stars using a 23-year baseline. The proper
motions will use the Hipparcos data, with epoch 1991.25, as first epoch and the
first intermediate-release Gaia astrometry, with epoch ~2014.5, as second
epoch. The expected HTPM proper-motion standard errors are 30-190 muas/yr,
depending on stellar magnitude. Depending on the characteristics of an object,
in particular its distance and velocity, its radial velocity can have a
significant impact on the determination of its proper motion. The impact of
this perspective acceleration is largest for fast-moving, nearby stars. Our
goal is to determine, for each star in the Hipparcos catalogue, the
radial-velocity standard error that is required to guarantee a negligible
contribution of perspective acceleration to the HTPM proper-motion precision.
We employ two evaluation criteria, both based on Monte-Carlo simulations, with
which we determine which stars need to be spectroscopically (re-)measured. Both
criteria take the Hipparcos measurement errors into account. For each star in
the Hipparcos catalogue, we determine the confidence level with which the
available radial velocity and its standard error, taken from the XHIP
compilation catalogue, are acceptable. We find that for 97 stars, the radial
velocities available in the literature are insufficiently precise for a 68.27%
confidence level. We also identify 109 stars for which radial velocities are
currently unknown yet need to be acquired to meet the 68.27% confidence level.
To satisfy the radial-velocity requirements coming from our study will be a
daunting task consuming a significant amount of spectroscopic telescope time.
Fortunately, the follow-up spectroscopy is not time-critical since the HTPM
proper motions can be corrected a posteriori once (improved) radial velocities
become available.Comment: Accepted in A&
The Luminosity Function Of Field Galaxies And Its Evolution Since z=1
We present the B-band luminosity function and comoving space and luminosity
densities for a sample of 2779 I-band selected field galaxies based on
multi-color data from the CADIS survey. The sample is complete down to I_815 =
22 without correction and with completeness correction extends to I_815=23.0.
By means of a new multi-color analysis the objects are classified according to
their spectral energy distributions (SEDs) and their redshifts are determined
with typical errors of delta z <= 0.03. We have split our sample into four
redshift bins between z=0.1 and z=1.04 and into three SED bins E-Sa,Sa-Sc and
starbursting (emission line) galaxies. The evolution of the luminosity function
is clearly differential with SED. The normalization phi* of luminosity function
for the E-Sa galaxies decreases towards higher redshift, and we find evidence
that the comoving galaxy space density decreases with redshift as well. In
contrast, we find phi* and the comoving space density increasing with redshift
for the Sa-Sc galaxies. For the starburst galaxies we find a steepening of the
luminosity function at the faint end and their comoving space density increases
with redshift.Comment: 15 pages, 14 figures, accepted by Astronomy&Astrophysic
Simulations of the Hyades
Context: Using the recent observational data of R\"oser et al. we present
-body simulations of the Hyades open cluster. Aims: We make an attempt to
determine initial conditions of the Hyades cluster at the time of its formation
in order to reproduce the present-day cumulative mass profile, stellar mass and
luminosity function (LF). Methods: We performed direct -body simulations of
the Hyades in an analytic Milky Way potential that account for stellar
evolution and include primordial binaries in a few models. Furthermore, we
applied a Kroupa (2001) IMF and used extensive ensemble-averaging. Results: We
find that evolved single-star King initial models with King parameters and initial particle numbers provide good fits to the
observational present-day cumulative mass profile within the Jacobi radius. The
best-fit King model has an initial mass of and an average mass
loss rate of . The K-band LFs of models and
observations show a reasonable agreement. Mass segregation is detected in both
observations and models. If 33% primordial binaries are included the initial
particle number is reduced by 5% as compared to the model without primordial
binaries. Conclusions: The present-day properties of the Hyades can be well
reproduced by a standard King or Plummer initial model when choosing
appropriate initial conditions. The degeneracy of good-fitting models can be
quite high due to the large dimension of the parameter space. More simulations
with different Roche-lobe filling factors and primordial binary fractions are
required to explore this degeneracy in more detail.Comment: 14 pages, 16+1 figures, hopefully final version, contains a note
added in proo
Skyline Tensile Forces in Cable Logging: Field Observations vs. Software Calculations
Skyline tensile forces have been shown to frequently exceed the recommended safety limits during ordinary cable logging operations. Several models for skyline engineering analyses have been proposed. Although skyline tensile forces assume a dynamic behaviour, practical solutions are based on a static approach without consideration of the dynamic nature of the cable systems. The aim of this study was to compare field data of skyline tensile forces with the static calculations derived by dedicated available software such as SkylineXL. To overcome the limitation of static calculation, this work also aimed to simulate the actual response of the tensile fluctuations measured in the real environment by mean of a finite element model (FEM). Field observations of skyline tensile forces included 103 work cycles, recorded over four different cable lines in standing skyline configuration. Payload estimations, carriages positions, and time study of the logging operations were also collected in the field. The ground profiles and the cable line geometries were analysed using digital elevation models. The field data were then used to simulate the work cycles in SkylineXL. The dynamic response of six fully-suspended loads in a single-span cable line was also simulated by a dedicated FEM built through ANSYS Âź. The observed data and the software calculations were then compared. SkylineXL resulted particularly reliable in the prediction of the actual tensile forces, with RMSE ranging between 7.5 and 13.5 KN, linked to an average CV(RMSE) of 7.24%. The reliability in predicting the peak tensile forces was lower, reporting CV(RMSE) of 10.12%, but still not likely resulting in a safety or performance problem. If properly set-up and used, thus, SkylineXL could be considered appropriate for operational and practical purposes. This work, however, showed that finite element models could be successfully used for detailed analysis and simulation of the skyline tensile forces, including the dynamic oscillations due to the motion of the carriage and payload along the cable line. Further developments of this technique could also lead to the physical simulation and analysis of the log-to-ground interaction and the investigation of the breakout force during lateral skidding
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