268 research outputs found
The 8th Habit from Effectiveness to Greatness
The 8th Habit shows how to solve such common dilemmas as :
- People want peace of mind and good relationships, but also want to keep their listyle and habits.
- Relationships are built on trust, but most people think more in terms of “me”- my wants, my needs, my rights.
- Management wants more for less; employees want more of “what’s in it for me” for less time and effort.
- Businesses are run by the economic rules of the marketplace; organizations are run by the cultural rules of the workplace.
- Society operates by its dominant social values, mut must live the the consequences of the inviolable operation of natural laws and principles
Covey’s new book will transform the way we think about ourselves and our purpose in life, about our organizations, and about humankind. Just as The 7 Habits of Highly Effective People helped us focus on effectiveness, The 8th Habit shows us the way to greatness
Creating Vertical Strategic Alliances: Theory and Cases from Canada's Agri-Food Sector
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Evidence for Grain Growth in Molecular Clouds: A Bayesian Examination of the Extinction Law in Perseus
We investigate the shape of the extinction law in two square fields of the Perseus molecular cloud complex. We combine deep red-optical (r, i and z band) observations obtained using Megacam on the MMT with UKIRT (United Kingdom Infrared Telescope) Infrared Deep Sky Survey near-infrared (J, H and K band) data to measure the colours of background stars. We develop a new hierarchical Bayesian statistical model, including measurement error, intrinsic colour variation, spectral type and dust reddening, to simultaneously infer parameters for individual stars and characteristics of the population. We implement an efficient Markov chain Monte Carlo algorithm utilizing generalized Gibbs sampling to compute coherent probabilistic inferences. We find a strong correlation between the extinction and the slope of the extinction law (parametrized by . Because the majority of the extinction towards our stars comes from the Perseus molecular cloud, we interpret this correlation as evidence of grain growth at moderate optical depths. The extinction law changes from the ‘diffuse’ value of to the 'dense cloud' value of as the column density rises from to 10 mag. This relationship is similar for the two regions in our study, despite their different physical conditions, suggesting that dust grain growth is a fairly universal process.Astronom
Young stars in the time domain
Variability is a defining characteristic of young stellar systems, and optical variability has been heavily studied to select and characterize the photospheric properties of young stars. In recent years, multi-epoch observations sampling a wider range of wavelengths and time-scales have revealed a wealth of time-variable phenomena at work during the star formation process. This splinter session was convened to summarize recent progress in providing improved coverage and understanding of time-variable processes in young stars and circumstellar disks. We begin by summarizing results from several multi-epoch Spitzer campaigns, which have demonstrated that many young stellar objects evidence significant mid-IR variability. While some of these variations can be attributed to processes in the stellar photosphere, others appear to trace short time-scale changes in the circumstellar disk which can be successfully modeled with axisymmetric or non-axisymmetric structures. We also review recent studies probing variability at shorter wavelengths that provide evidence for high frequency pulsations associated with accretion outbursts, correlated optical/X-ray variability in Classical T Tauri stars, and magnetic reversals in young solar analogs
TOI-150: A transiting hot Jupiter in the TESS southern CVZ
We report the detection of a hot Jupiter ($M_{p}=1.75_{-0.17}^{+0.14}\
M_{J}R_{p}=1.38\pm0.04\ R_{J}\log
g=4.152^{+0.030}_{-0.043}\beta=-79.59^{\circ}$). We confirm the
planetary nature of the candidate TOI-150.01 using radial velocity observations
from the APOGEE-2 South spectrograph and the Carnegie Planet Finder
Spectrograph, ground-based photometric observations from the robotic
Three-hundred MilliMeter Telescope at Las Campanas Observatory, and Gaia
distance estimates. Large-scale spectroscopic surveys, such as APOGEE/APOGEE-2,
now have sufficient radial velocity precision to directly confirm the signature
of giant exoplanets, making such data sets valuable tools in the TESS era.
Continual monitoring of TOI-150 by TESS can reveal additional planets and
subsequent observations can provide insights into planetary system
architectures involving a hot Jupiter around a star about halfway through its
main-sequence life.Comment: 13 pages, 3 figures, 2 tables, accepted to ApJ
Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey
The Survey Science Centre of the XMM-Newton satellite released the first
incremental version of the 2XMM catalogue in August 2008 . With more than
220,000 X-ray sources, the 2XMMi was at that time the largest catalogue of
X-ray sources ever published and thus constitutes an unprecedented resource for
studying the high-energy properties of various classes of X-ray emitters such
as AGN and stars. The advent of the 7th release of the Sloan Digital Sky Survey
offers the opportunity to cross-match two major surveys and extend the spectral
energy distribution of many 2XMMi sources towards the optical bands. We here
present a cross-matching algorithm based on the classical likelihood ratio
estimator. The method developed has the advantage of providing true
probabilities of identifications without resorting to Monte-Carlo simulations.
Over 30,000 2XMMi sources have SDSS counterparts with individual probabilities
of identification higher than 90%. Using spectroscopic identifications from the
SDSS DR7 catalogue supplemented by extraction from other catalogues, we build
an identified sample from which the way the various classes of X-ray emitters
gather in the multi dimensional parameter space can be analysed. We investigate
two scientific use cases. In the first example we show how these
multi-wavelength data can be used to search for new QSO2s. Although no specific
range of observed properties allows us to identify Compton Thick QSO2s, we show
that the prospects are much better for Compton Thin AGN2 and discuss several
possible multi-parameter selection strategies. In a second example, we confirm
the hardening of the mean X-ray spectrum with increasing X-ray luminosity on a
sample of over 500 X-ray active stars and reveal that on average X-ray active M
stars display bluer colour indexes than less active ones (abridged).Comment: Accepted for publication in A&A. The corresponding fits file can be
downloaded from the XCat-DB home page (http://xcatdb.u-strasbg.fr/) (tools
and data). The file also contains line information for all SDSS spectroscopic
entries matching a 2XMM source. Results from the cross-correlation with the
2XMM DR3 are also available at the same location. 22 pages and 14 figure
Sloan Digital Sky Survey Imaging of Low Galactic Latitude Fields: Technical Summary and Data Release
The Sloan Digital Sky Survey (SDSS) mosaic camera and telescope have obtained
five-band optical-wavelength imaging near the Galactic plane outside of the
nominal survey boundaries. These additional data were obtained during
commissioning and subsequent testing of the SDSS observing system, and they
provide unique wide-area imaging data in regions of high obscuration and star
formation, including numerous young stellar objects, Herbig-Haro objects and
young star clusters. Because these data are outside the Survey regions in the
Galactic caps, they are not part of the standard SDSS data releases. This paper
presents imaging data for 832 square degrees of sky (including repeats), in the
star-forming regions of Orion, Taurus, and Cygnus. About 470 square degrees are
now released to the public, with the remainder to follow at the time of SDSS
Data Release 4. The public data in Orion include the star-forming region NGC
2068/NGC 2071/HH24 and a large part of Barnard's loop.Comment: 31 pages, 9 figures (3 missing to save space), accepted by AJ, in
press, see http://photo.astro.princeton.edu/oriondatarelease for data and
paper with all figure
LSST Science Book, Version 2.0
A survey that can cover the sky in optical bands over wide fields to faint
magnitudes with a fast cadence will enable many of the exciting science
opportunities of the next decade. The Large Synoptic Survey Telescope (LSST)
will have an effective aperture of 6.7 meters and an imaging camera with field
of view of 9.6 deg^2, and will be devoted to a ten-year imaging survey over
20,000 deg^2 south of +15 deg. Each pointing will be imaged 2000 times with
fifteen second exposures in six broad bands from 0.35 to 1.1 microns, to a
total point-source depth of r~27.5. The LSST Science Book describes the basic
parameters of the LSST hardware, software, and observing plans. The book
discusses educational and outreach opportunities, then goes on to describe a
broad range of science that LSST will revolutionize: mapping the inner and
outer Solar System, stellar populations in the Milky Way and nearby galaxies,
the structure of the Milky Way disk and halo and other objects in the Local
Volume, transient and variable objects both at low and high redshift, and the
properties of normal and active galaxies at low and high redshift. It then
turns to far-field cosmological topics, exploring properties of supernovae to
z~1, strong and weak lensing, the large-scale distribution of galaxies and
baryon oscillations, and how these different probes may be combined to
constrain cosmological models and the physics of dark energy.Comment: 596 pages. Also available at full resolution at
http://www.lsst.org/lsst/sciboo
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