2,197 research outputs found
Assessing the Value of Time Travel Savings – A Feasibility Study on Humberside.
It is expected that the opening of the Humber Bridge
will cause major changes to travel patterns around Humberside;
given the level of tolls as currently stated, many travellers
will face decisions involving a trade-off between travel time,
money outlay on tolls or fares and money outlay on private
vehicle running costs; this either in the context of
destination choice, mode choice or route choice.
This report sets out the conclusions of a preliminary
study of the feasibility of inferring values of travel time
savings from observations made on the outcomes of these
decisions. Methods based on aggregate data of destination
choice are found t o be inefficient; a disaggregate mode
choice study i s recommended, subject to caveats on sample size
Photometric Response Functions of the SDSS Imager
The monochromatic illumination system is constructed to carry out in situ
measurements of the response function of the mosaicked CCD imager used in the
Sloan Digital Sky Survey (SDSS). The system is outlined and the results of the
measurements, mostly during the first 6 years of the SDSS, are described. We
present the reference response functions for the five colour passbands derived
from these measurements, and discuss column to column variations and variations
in time, and also their effects on photometry. We also discuss the effect
arising from various, slightly different response functions of the associated
detector systems that were used to give SDSS photometry. We show that the
calibration procedures of SDSS remove these variations reasonably well with the
resulting final errors from variant response functions being unlikely to be
larger than 0.01 mag for g, r, i, and z bands over the entire duration of the
survey. The considerable aging effect is uncovered in the u band, the response
function showing a 30% decrease in the throughput in the short wavelength side
during the survey years, which potentially causes a systematic error in
photometry. The aging effect is consistent with variation of the instrumental
sensitivity in u-band, which is calibrated out. The expected colour variation
is consistent with measured colour variation in the catalog of repeated
photometry. The colour variation is delta (u-g) ~ 0.01 for most stars, and at
most delta (u-g) ~ 0.02 mag for those with extreme colours. We verified in the
final catalogue that no systematic variations in excess of 0.01 mag are
detected in the photometry which can be ascribed to aging and/or seasonal
effects except for the secular u-g colour variation for stars with extreme
colours.Comment: 54 pages, 18 figures, 7 tables, accepted for publication in A
The velocity peaks in the cold dark matter spectrum on Earth
The cold dark matter spectrum on earth is expected to have peaks in velocity
space. We obtain estimates for the sizes and locations of these peaks. To this
end we have generalized the secondary infall model of galactic halo formation
to include angular momentum of the dark matter particles. This new model is
still spherically symmetric and it has self-similar solutions. Our results are
relevant to direct dark matter search experiments.Comment: 12 pages including 1 table and 4 figures, LaTeX, REVTEX 3.0 versio
On the link between rotation, chromospheric activity and Li abundance in subgiant stars
The connection rotation-CaII emission flux-lithium abundance is analyzed for
a sample of bona fide subgiant stars, with evolutionary status determined from
HIPPARCOS trigonometric parallax measurements and from the Toulouse-Geneva
code.Comment: 9 pages, 8 figure
Monte Carlo study of the hull distribution for the q=1 Brauer model
We study a special case of the Brauer model in which every path of the model
has weight q=1. The model has been studied before as a solvable lattice model
and can be viewed as a Lorentz lattice gas. The paths of the model are also
called self-avoiding trails. We consider the model in a triangle with boundary
conditions such that one of the trails must cross the triangle from a corner to
the opposite side. Motivated by similarities between this model, SLE(6) and
critical percolation, we investigate the distribution of the hull generated by
this trail (the set of points on or surrounded by the trail) up to the hitting
time of the side of the triangle opposite the starting point. Our Monte Carlo
results are consistent with the hypothesis that for system size tending to
infinity, the hull distribution is the same as that of a Brownian motion with
perpendicular reflection on the boundary.Comment: 21 pages, 9 figure
VLT + UVES Spectroscopy of the Low-Ionization Intrinsic Absorber in SDSS J001130.56+005550.7
We analyse high-resolution VLT+UVES spectra of the low-ionization intrinsic
absorber observed in the BAL QSO SDSS J001130.56+005550.7. Two narrow
absorption systems at velocities -600 km/s and -22000 km/s are detected. The
low-velocity system is part of the broad absorption line (BAL), while the
high-velocity one is well detached. While most narrow absorption components are
only detected in the high-ionization species, the lowest velocity component is
detected in both high- and low-ionization species, including in the excited
SiII* and CII* lines. From the analysis of doublet lines, we find that the
narrow absorption lines at the low-velocity end of the BAL trough are
completely saturated but do not reach zero flux, their profiles being dominated
by a velocity-dependent covering factor. The covering factor is significantly
smaller for MgII than for SiIV and NV, which demonstrates the intrinsic nature
of absorber. From the analysis of the excited SiII* and CII* lines in the
lowest velocity component, we find an electron density ~ 1000 cm^{-3}. Assuming
photoionization equilibrium, we derive a distance ~ 20 kpc between the
low-ionization region and the quasar core. The correspondence in velocity of
the high- and low-ionization features suggests that all these species must be
closely associated, hence formed at the same distance of ~ 20 kpc, much higher
than the distance usually assumed for BAL absorbers.Comment: Accepted for publication in A&
A value hierarchy for inclusive design of heart valve implants in regenerative medicine
Aim: This paper investigates the conditions for inclusive design of regenerative medicine interventions from a bioethical perspective, taking regenerative valve implants as a showcase. Methods: A value hierarchy is construed to translate the value of justice into norms and design requirements for inclusive design of regenerative valve implants. Results: Three norms are proposed and translated into design requirements: regenerative valve implants should be designed to promote equal opportunity to good health for all potential users; equal respect for all potential users should be shown; and the implants should be designed to be accessible to everyone in need. Conclusion: The norms and design requirements help to design regenerative valve implants that are appropriate, respectful and available for everyone in need.</p
Elliptical Galaxies with Emission Lines from the Sloan Digital Sky Survey
We present the results of 11 elliptical galaxies with strong nebular emission
lines during our study of star formation history along the Hubble sequence.
After removing the dilution from the underlying old stellar populations by use
of stellar population synthesis model, we derive the accurate fluxes of all
emission lines for these objects, which are later classified with emission line
ratios into one Seyfert 2, six LINERs and four HII galaxies. We also identify
one HII galaxy (A1216+04) as a hitherto unknown Wolf-Rayet galaxy from the
presence of the Wolf-Rayet broad bump at 4650 \AA. We propose that the
star-forming activities in elliptical galaxies are triggered by either
galaxy-galaxy interaction or the merging of a small satellite/a massive star
cluster, as already suggested by recent numerical simulations
HI Selected Galaxies in the Sloan Digital Sky Survey II: The Colors of Gas-Rich Galaxies
We utilize color information for an HI-selected sample of 195 galaxies to
explore the star formation histories and physical conditions that produce the
observed colors. We show that the HI selection creates a significant offset
towards bluer colors that can be explained by enhanced recent bursts of star
formation. There is also no obvious color bimodality, because the HI selection
restricts the sample to bluer, actively star forming systems, diminishing the
importance of the red sequence. Rising star formation rates are still required
to explain the colors of galaxies bluer than g-r < 0.3. We also demonstrate
that the colors of the bluest galaxies in our sample are dominated by emission
lines and that stellar population synthesis models alone (without emission
lines) are not adequate for reproducing many of the galaxy colors. These
emission lines produce large changes in the r-i colors but leave the g-r color
largely unchanged. In addition, we find an increase in the dispersion of galaxy
colors at low masses that may be the result of a change in the star formation
process in low-mass galaxies.Comment: 12 pages, 16 figures, published in AJ (138, 796); replaced Figure 16
with higher resolution versio
Building the Galactic halo from globular clusters: evidence from chemically unusual red giants
We present a spectroscopic search for halo field stars that originally formed
in globular clusters. Using moderate-resolution SDSS-III/SEGUE-2 spectra of 561
red giants with typical halo metallicities (-1.8 < [Fe/H] < -1.0), we identify
16 stars, 3% of the sample, with CN and CH bandstrength behavior indicating
depleted carbon and enhanced nitrogen abundances relative to the rest of the
data set. Since globular clusters are the only environment known in which stars
form with this pattern of atypical light-element abundances, we claim that
these stars are second-generation globular cluster stars that have been lost to
the halo field via normal cluster mass-loss processes. Extrapolating from
theoretical models of two-generation globular cluster formation, this result
suggests that globular clusters contributed significant numbers of stars to the
construction of the Galactic halo: we calculate that a minimum of 17% of the
present-day mass of the stellar halo was originally formed in globular
clusters. The ratio of CN-strong to CN-normal stars drops with Galactocentric
distance, suggesting that the inner-halo population may be the primary
repository of these stars.Comment: 9 pages including 8 figures, A&A accepte
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