1,513 research outputs found
Probing the Geometry of Supernovae with Spectropolarimetry
We present results from a spectropolarimetric survey of young supernovae
completed at the Keck Observatory, including at least one example from each of
the major supernova types: Ia (1997dt), Ib (1998T, 1997dq), Ib/c-pec (1997ef),
IIn (1997eg), and II-P (1997ds). All objects show evidence for intrinsic
polarization, suggesting that asphericity may be a common feature in young
supernova atmospheres.Comment: 4 pages, 2 figures. To appear in the Proceedings of the 10th Annual
October Astrophysics Conference in Maryland: Cosmic Explosion
Editorial
This is the second special issue to be developed from the international conference ‘At the Crossroads: New Directions in Teacher Education’, held at Canterbury Christ Church University in July 2012, which brought together over 200 scholars from 16 countries. As well as a range of methodological approaches to research in teacher education, represented in the studies published in the previous special issue (Vol. 6 issue 1, March 2014), many of the conference papers focussed on the development of innovative practice in initial teacher education. The five papers presented here, which have been updated for this special issue, illustrate some of these exciting initiatives
Editorial
Editorial special issue 1, Methodological approaches to researching teacher education: The idea for this special issue of TEAN developed from the international conference ‘At the Crossroads: New Directions in Teacher Education’, held at Canterbury Christ Church University in July 2012, which brought together over 200 scholars from 16 countries. It was striking that a sizeable number of papers focussed on specific methodologies used in researching teacher education, representing a growing interest in this area. The six articles published here, originally presented at the conference, represent just some of the different and innovative methodological approaches being used in current studies
Exploring the Structure of Distant Galaxies with Adaptive Optics on the Keck-II Telescope
We report on the first observation of cosmologically distant field galaxies
with an high order Adaptive Optics (AO) system on an 8-10 meter class
telescope. Two galaxies were observed at 1.6 microns at an angular resolution
as high as 50 milliarcsec using the AO system on the Keck-II telescope. Radial
profiles of both objects are consistent with those of local spiral galaxies and
are decomposed into a classic exponential disk and a central bulge. A
star-forming cluster or companion galaxy as well as a compact core are detected
in one of the galaxies at a redshift of 0.37+/-0.05. We discuss possible
explanations for the core including a small bulge, a nuclear starburst, or an
active nucleus. The same galaxy shows a peak disk surface brightness that is
brighter than local disks of comparable size. These observations demonstrate
the power of AO to reveal details of the morphology of distant faint galaxies
and to explore galaxy evolution.Comment: 5 pages, Latex, 3 figures. Accepted for publication in P.A.S.
Spectroscopy of High-Redshift Supernovae from the ESSENCE Project: The First Four Years
We present the results of spectroscopic observations from the ESSENCE
high-redshift supernova (SN) survey during its first four years of operation.
This sample includes spectra of all SNe Ia whose light curves were presented by
Miknaitis et al. (2007) and used in the cosmological analyses of Davis et al.
(2007) and Wood-Vasey et al. (2007). The sample represents 273 hours of
spectroscopic observations with 6.5 - 10-m-class telescopes of objects detected
and selected for spectroscopy by the ESSENCE team. We present 174 spectra of
156 objects. Combining this sample with that of Matheson et al. (2005), we have
a total sample of 329 spectra of 274 objects. From this, we are able to
spectroscopically classify 118 Type Ia SNe. As the survey has matured, the
efficiency of classifying SNe Ia has remained constant while we have observed
both higher-redshift SNe Ia and SNe Ia farther from maximum brightness.
Examining the subsample of SNe Ia with host-galaxy redshifts shows that
redshifts derived from only the SN Ia spectra are consistent with redshifts
found from host-galaxy spectra. Moreover, the phases derived from only the SN
Ia spectra are consistent with those derived from light-curve fits. By
comparing our spectra to local templates, we find that the rate of objects
similar to the overluminous SN 1991T and the underluminous SN 1991bg in our
sample are consistent with that of the local sample. We do note, however, that
we detect no object spectroscopically or photometrically similar to SN 1991bg.
Although systematic effects could reduce the high-redshift rate we expect based
on the low-redshift surveys, it is possible that SN 1991bg-like SNe Ia are less
prevalent at high redshift.Comment: 21 pages, 17 figures, accepted to A
Characteristic velocities of stripped-envelope core-collapse supernova cores
The velocity of the inner ejecta of stripped-envelope core-collapse
supernovae (CC-SNe) is studied by means of an analysis of their nebular
spectra. Stripped-envelope CC-SNe are the result of the explosion of bare cores
of massive stars ( M), and their late-time spectra are
typically dominated by a strong [O {\sc i}] 6300, 6363 emission
line produced by the innermost, slow-moving ejecta which are not visible at
earlier times as they are located below the photosphere. A characteristic
velocity of the inner ejecta is obtained for a sample of 56 stripped-envelope
CC-SNe of different spectral types (IIb, Ib, Ic) using direct measurements of
the line width as well as spectral fitting. For most SNe, this value shows a
small scatter around 4500 km s. Observations ( days) of
stripped-envelope CC-SNe have revealed a subclass of very energetic SNe, termed
broad-lined SNe (BL-SNe) or hypernovae, which are characterised by broad
absorption lines in the early-time spectra, indicative of outer ejecta moving
at very high velocity (). SNe identified as BL in the early phase
show large variations of core velocities at late phases, with some having much
higher and some having similar velocities with respect to regular CC-SNe. This
might indicate asphericity of the inner ejecta of BL-SNe, a possibility we
investigate using synthetic three-dimensional nebular spectra.Comment: 14 pages, 10 figures, MNRAS accepte
On the economic impact of international sport events: microevidence from survey data at the EURO 2008
Using firm-level data for more than 700 Swiss hotels and restaurants, we evaluate the economic impact of the EURO 2008 soccer championship in Switzerland. Although aggregated macrodata do not reveal any sizable economic impact, we report an overall negative effect based on the surveyed companies. Notably the reported effects of the individual firms are very heterogeneous. For instance, hotels in cities benefitted from the tournament as they were able to raise prices and thereby increase sales. Looking at the long-run impact only a small fraction of companies do believe in a positive effect. Interestingly, this outlook does not depend on realized sales, but on the guest structure. © 2014 © 2014 Taylor & Francis
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