5,165 research outputs found
The Dark Side of Performance Appraisals: A Study of University Librarians Across the U.S.
Performance appraisals are conducted regularly in professional organizations as a means to evaluate employee performance and overall company effectiveness. Employees and employers alike dread appraisal time; appraisals are often time consuming, tedious, and yield minimal positive results. Previous research has shown that employee perceptions of performance appraisals are important to consider when determining their overall effectiveness. In order to build new systems that could be viewed more positively by managers and employees, a deeper examination into the issues of performance appraisals, especially from the manager’s perspective, is needed. Our study looks at data gathered from a survey given to academic library directors, prompting them to evaluate the purposefulness of their current performance appraisal systems. Embedded in this survey is an open-ended response question, asking directors their perceptions of the PA system in their library. Our study seeks to determine if we can use text analytics create a better understanding of manager’s reactions and perceptions of PA systems and formats. We believe that the data gathered from the textual analysis will provide incremental validity into manager perceptions of performance appraisals and further insight into how organizations can improve their own processes
Faraday Rotation of Extended Emission as a Probe of the Large-Scale Galactic Magnetic Field
The Galactic magnetic field is an integral constituent of the interstellar
medium (ISM), and knowledge of its structure is crucial to understanding
Galactic dynamics. The Rotation Measures (RM) of extragalactic (EG) sources
have been the basis of comprehensive Galactic magnetic field models. Polarised
extended emission (XE) is also seen along lines of sight through the Galactic
disk, and also displays the effects of Faraday rotation. Our aim is to
investigate and understand the relationship between EG and XE RMs near the
Galactic plane, and to determine how the XE RMs, a hitherto unused resource,
can be used as a probe of the large-scale Galactic magnetic field. We used
polarisation data from the Canadian Galactic Plane Survey (CGPS), observed near
1420 MHz with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis
Telescope. We calculated RMs from a linear fit to the polarisation angles as a
function of wavelength squared in four frequency channels, for both the EG
sources and the XE. Across the CGPS area, , the RMs of the XE closely track the RMs of the EG
sources, with XE RMs about half the value of EG-source RMs. The exceptions are
places where large local HII complexes heavily depolarise more distant
emission. We conclude that there is valuable information in the XE RM dataset.
The factor of 2 between the two types of RM values is close to that expected
from a Burn slab model of the ISM. This result indicates that, at least in the
outer Galaxy, the EG and XE sources are likely probing similar depths, and that
the Faraday rotating medium and the synchrotron emitting medium have similar
variation with galactocentric distance.Comment: Accepted to Galaxies, March 22, 201
Baby-Led Weaning: The Evidence to Date
Purpose of ReviewInfants are traditionally introduced to solid foods using spoon-feeding of specially prepared infant foods.Recent FindingsHowever, over the last 10–15 years, an alternative approach termed ‘baby-led weaning’ has grown in popularity. This approach involves allowing infants to self-feed family foods, encouraging the infant to set the pace and intake of the meal. Proponents of the approach believe it promotes healthy eating behaviour and weight gain trajectories, and evidence is starting to build surrounding the method. This review brings together all empirical evidence to date examining behaviours associated with the approach, its outcomes and confounding factors.SummaryOverall, although there is limited evidence suggesting that a baby-led approach may encourage positive outcomes, limitations of the data leave these conclusions weak. Further research is needed, particularly to explore pathways to impact and understand the approach in different contexts and populations
Velocity Dispersion of Dissolving OB Associations Affected by External Pressure of Formation Environment
This paper presents a possible way to understand dissolution of OB
associations (or groups). Assuming rapid escape of parental cloud gas from
associations, we show that the shadow of the formation environment for
associations can be partially imprinted on the velocity dispersion at their
dissolution. This conclusion is not surprising as long as associations are
formed in a multiphase interstellar medium, because the external pressure
should suppress expansion caused by the internal motion of the parental clouds.
Our model predicts a few km s as the internal velocity dispersion.
Observationally, the internal velocity dispersion is km s which
is smaller than our prediction. This suggests that the dissipation of internal
energy happens before the formation of OB associations.Comment: 6 pages. AJ accepte
A low-density hot Jupiter in a near-aligned, 4.5-day orbit around a = 10.8, F5V star
We report the independent discovery and characterisation of a hot Jupiter in
a 4.5-d, transiting orbit around the star TYC 7282-1298-1 ( = 10.8, F5V).
The planet has been pursued by the NGTS team as NGTS-2b and by ourselves as
WASP-179b. We characterised the system using a combination of photometry from
WASP-South and TRAPPIST-South, and spectra from CORALIE (around the orbit) and
HARPS (through the transit). We find the planet's orbit to be nearly aligned
with its star's spin. From a detection of the Rossiter-McLaughlin effect, we
measure a projected stellar obliquity of . From
line-profile tomography of the same spectra, we measure . We find the planet to have a low density ( = 0.67
0.09 , = 1.54 0.06 ), which, along
with its moderately bright host star, makes it a good target for transmission
spectroscopy. We find a lower stellar mass ( = )
than reported by the NGTS team ( = ), though the
difference is only .Comment: Submitted to AJ. 9 pages, 6 figures, 5 table
Information sharing and credit : firm-level evidence from transition countries
We investigate whether information sharing among banks has affected credit market performance in the transition countries of Eastern Europe and the former Soviet Union, using a large sample of firm-level data. Our estimates show that information sharing is associated with improved availability and lower cost of credit to firms. This correlation is stronger for opaque firms than transparent ones and stronger in countries with weak legal environments than in those with strong legal environments. In cross-sectional estimates, we control for variation in country-level aggregate variables that may affect credit, by examining the differential impact of information sharing across firm types. In panel estimates, we also control for the presence of unobserved heterogeneity at the firm level, as well as for changes in macroeconomic variables and the legal environment
Magnetic topology and surface differential rotation on the K1 subgiant of the RS CVn system HR 1099
We present here spectropolarimetric observations of the RS CVn system HR 1099
(V711 Tau) secured from 1998 February to 2002 January with the
spectropolarimeter MuSiCoS at the Telescope Bernard Lyot (Observatoire du Pic
du Midi, France). We apply Zeeman-Doppler Imaging and reconstruct brightness
and magnetic surface topologies of the K1 primary subgiant of the system, at
five different epochs. We confirm the presence of large, axisymmetric regions
where the magnetic field is mainly azimuthal, providing further support to the
hypothesis that dynamo processes may be distributed throughout the whole
convective zone in this star. We study the short-term evolution of surface
structures from a comparison of our images with observations secured at
close-by epochs by Donati et al. (2003) at the Anglo-Australian Telescope. We
conclude that the small-scale brightness and magnetic patterns undergo major
changes within a timescale of 4 to 6 weeks, while the largest structures remain
stable over several years. We report the detection of a weak surface
differential rotation (both from brightness and magnetic tracers) indicating
that the equator rotates faster than the pole with a difference in rotation
rate between the pole and the equator about 4 times smaller than that of the
Sun. This result suggests that tidal forces also impact the global dynamic
equilibrium of convective zones in cool active stars.Comment: accepted by MNRA
Methylated DNA Immunoprecipitation
The identification of DNA methylation patterns is a common procedure in the study of epigenetics, as methylation is known to have significant effects on gene expression, and is involved with normal development as well as disease 1-4. Thus, the ability to discriminate between methylated DNA and non-methylated DNA is essential for generating methylation profiles for such studies. Methylated DNA immunoprecipitation (MeDIP) is an efficient technique for the extraction of methylated DNA from a sample of interest 5-7. A sample of as little as 200 ng of DNA is sufficient for the antibody, or immunoprecipitation (IP), reaction. DNA is sonicated into fragments ranging in size from 300-1000 bp, and is divided into immunoprecipitated (IP) and input (IN) portions. IP DNA is subsequently heat denatured and then incubated with anti-5'mC, allowing the monoclonal antibody to bind methylated DNA. After this, magnetic beads containing a secondary antibody with affinity for the primary antibody are added, and incubated. These bead-linked antibodies will bind the monoclonal antibody used in the first step. DNA bound to the antibody complex (methylated DNA) is separated from the rest of the DNA by using a magnet to pull the complexes out of solution. Several washes using IP buffer are then performed to remove the unbound, non-methylated DNA. The methylated DNA/antibody complexes are then digested with Proteinase K to digest the antibodies leaving only the methylated DNA intact. The enriched DNA is purified by phenol:chloroform extraction to remove the protein matter and then precipitated and resuspended in water for later use. PCR techniques can be used to validate the efficiency of the MeDIP procedure by analyzing the amplification products of IP and IN DNA for regions known to lack and known to contain methylated sequences. The purified methylated DNA can then be used for locus-specific (PCR) or genome-wide (microarray and sequencing) methylation studies, and is particularly useful when applied in conjunction with other research tools such as gene expression profiling and array comparative genome hybridization (CGH) 8. Further investigation into DNA methylation will lead to the discovery of new epigenetic targets, which in turn, may be useful in developing new therapeutic or prognostic research tools for diseases such as cancer that are characterized by aberrantly methylated DNA 2, 4, 9-11
WASP-157b, a Transiting Hot Jupiter Observed with K2
We announce the discovery of the transiting hot Jupiter WASP-157b in a 3.95-d
orbit around a V = 12.9 G2 main-sequence star. This moderately inflated planet
has a Saturn-like density with a mass of M and a
radius of R. We do not detect any rotational or
phase-curve modulations, nor the secondary eclipse, with conservative
semi-amplitude upper limits of 250 and 20 ppm, respectively.Comment: 6 pages, 5 figures and 4 tables. Accepted for publication in PAS
WASP-189b: an ultra-hot Jupiter transiting the bright A star HR 5599 in a polar orbit
We report the discovery of WASP-189b: an ultra-hot Jupiter in a 2.72-d
transiting orbit around the A star WASP-189 (HR 5599). We detected
periodic dimmings in the star's lightcurve, first with the WASP-South survey
facility then with the TRAPPIST-South telescope. We confirmed that a planet is
the cause of those dimmings via line-profile tomography and radial-velocity
measurements using the HARPS and CORALIE spectrographs. Those reveal WASP-189b
to be an ultra-hot Jupiter ( = 2.13 0.28 ;
= 1.374 0.082 ) in a polar orbit (; ) around a rapidly rotating
A6IV-V star ( = 8000 100 K; 100
km\, s). We calculate a predicted equilibrium temperature of = 2641 34 K, assuming zero albedo and efficient redistribution,
which is the third hottest for the known exoplanets. WASP-189 is the brightest
known host of a transiting hot Jupiter and the third-brightest known host of
any transiting exoplanet. We note that of the eight hot-Jupiter systems with
7000 K, seven have strongly misaligned orbits, and two of the
three systems with 8000 K have polar orbits (the third is
aligned).Comment: Submitted to MNRAS. 10 pages, 9 figures, 3 table
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