1,486 research outputs found
The National Virtual Observatory
As a scientific discipline, Astronomy is rather unique. We only have one
laboratory, the Universe, and we cannot, of course, change the initial
conditions and study the resulting effects. On top of this, acquiring
Astronomical data has historically been a very labor-intensive effort. As a
result, data has traditionally been preserved for posterity. With recent
technological advances, however, the rate at which we acquire new data has
grown exponentially, which has generated a Data Tsunami, whose wave train
threatens to overwhelm the field. In this conference proceedings, we present
and define the concept of virtual observatories, which we feel is the only
logical answer to this dilemma.Comment: 5 pages, uses newpasp.sty (included), to appear in "Extragalactic Gas
at Low Redshfit", ASP Conf. Series, J. S. Mulchaey and J. T. Stocke (eds.
Nachhaltigkeitskriterien als essentieller Bestandteil einer novellierten EU-Öko-Basisverordnung
The main goal of this study was to develop sustainability criteria for the advancement of the EU-Eco-Regulations. To achieve this, the authors analyzed 8 international certification schemes for sustainable aspects which could be transferred to existing regulations. By doing so it was possible to abstract 10 sustainability criteria and in the prozess evaluate their value for future developments of the EU-Eco-Regulations.
Sustainability of agricultural systems is of the utmost importance for future development of mankind itself. Since ecological agriculture is the most sustainable System we have that works on a large scale (cf. Pick 2009), it is reasonable to suggest that the outline we use for this kind of agriculture – producing best quality with fewest external inputs – is true for sustainable agriculture itself. This work proofed this conjecture to be true.
So although the here found sustainability criteria are only partly adopted in the ad-vancement of the EU-Eco-Regulations it can be said that sustainable agriculture of any kind should involve the criteria found in this work
Nebraska Trapping
Fur bearers and trapping played an important role in the exploration and development of Nebraska. The harvest of our fur-bearer resource is part of every Nebraskan\u27s heritage. Wise use of the resource and consideration for other people\u27s property and personal rights can insure that trapping will remain a part of the heritage of future generations. The purpose of this publication is to help insure this heritage ... through the educational process. Knowledge of and respect for the resource, as well as consideration for other people, are the keys to perpetuating trapping as an outdoor activity. While primarily designed to assist the young or novice trapper, this manual should benefit veterans as well. Contrary to popular belief, you can teach an old dog new tricks. Trapping is a biologically sound and legitimate use of a renewable natural resource. In fact, it is our primary means of managing fur-bearer populations, and management is essential to the health and well-being of all wildlife species. Significant problems develop for both the wildlife and man when management is not practiced and numbers are allowed to exceed what the habitat or environment will support.
An Open Letter to Trappers • Trapping ... Yesterday, Today and Tomorrow • Pre-Season Preparation • Muskrat • Mink • Beaver • Raccoon • Opossum • Coyote • Fox • Skunk • Badger • Weasel • Releasing an Unwanted Catch • After the Catch • Trapping Summary • Trapper\u27s Cree
Massive Datasets in Astronomy
Astronomy has a long history of acquiring, systematizing, and interpreting
large quantities of data. Starting from the earliest sky atlases through the
first major photographic sky surveys of the 20th century, this tradition is
continuing today, and at an ever increasing rate.
Like many other fields, astronomy has become a very data-rich science, driven
by the advances in telescope, detector, and computer technology. Numerous large
digital sky surveys and archives already exist, with information content
measured in multiple Terabytes, and even larger, multi-Petabyte data sets are
on the horizon. Systematic observations of the sky, over a range of
wavelengths, are becoming the primary source of astronomical data. Numerical
simulations are also producing comparable volumes of information. Data mining
promises to both make the scientific utilization of these data sets more
effective and more complete, and to open completely new avenues of astronomical
research.
Technological problems range from the issues of database design and
federation, to data mining and advanced visualization, leading to a new toolkit
for astronomical research. This is similar to challenges encountered in other
data-intensive fields today.
These advances are now being organized through a concept of the Virtual
Observatories, federations of data archives and services representing a new
information infrastructure for astronomy of the 21st century. In this article,
we provide an overview of some of the major datasets in astronomy, discuss
different techniques used for archiving data, and conclude with a discussion of
the future of massive datasets in astronomy.Comment: 46 Pages, 21 Figures, Invited Review for the Handbook of Massive
Datasets, editors J. Abello, P. Pardalos, and M. Resende. Due to space
limitations this version has low resolution figures. For full resolution
review see http://www.astro.caltech.edu/~rb/publications/hmds.ps.g
yourSky: rapid desktop access to custom astronomical image mosaics
The yourSky custom astronomical image mosaicking software has a Web portal architecture that allows access via ordinary desktop computers with low bandwidth network connections to high performance and highly customizable mosaicking software deployed in a high performance computing and communications environment. The emphasis is on custom access to image mosaics constructed from terabytes of raw image data stored in remote archives. In this context, custom access refers to new technology that enables on the fly mosaicking to meet user-specified criteria for region of the sky to be mosaicked, datasets to be used, resolution, coordinate system, projection, data type and image format. The yourSky server is a fully automated end-to-end system that handles all aspects of the mosaic construction. This includes management of mosaic requests, determining which input images are required to fulfill each request, management of a data cache for both input image plates and output mosaics, retrieval of input image plates from massive remote archives, image mosaic construction on a multiprocessor system, and making the result accessible to the user on the desktop. The URL for yourSky is http://yourSky.jpl.nasa.gov
VOFilter, Bridging Virtual Observatory and Industrial Office Applications
VOFilter is an XML based filter developed by the Chinese Virtual Observatory
project to transform tabular data files from VOTable format into OpenDocument
format. VOTable is an XML format defined for the exchange of tabular data in
the context of the Virtual Observatory (VO). It is the first Proposed
Recommendation defined by International Virtual Observatory Alliance, and has
obtained wide support from both the VO community and many Astronomy projects.
OpenOffice.org is a mature, open source, front office applications suite with
the advantage of native support of industrial standard OpenDocument XML file
format. Using the VOFilter, VOTable files can be loaded in OpenOffice.org Calc,
a spreadsheet application, and then displayed and analyzed as other spreadsheet
files. Here, the VOFilter acts as a connector, bridging the coming VO with
current industrial office applications. Virtual Observatory and technical
background of the VOFilter are introduced. Its workflow, installation and usage
are presented. Existing problems and limitations are also discussed together
with the future development plans.Comment: Accepted for publication in ChJAA (9 pages, 2 figures, 185KB
Clustering of adverse health and educational outcomes in adolescence following early childhood disadvantage: population-based retrospective UK cohort study
Background: Disadvantage in early childhood (ages 0–5 years) is associated with worse health and educational outcomes in adolescence. Evidence on the clustering of these adverse outcomes by household income is scarce in the generation of adolescents born since the turn of the millennium. We aimed to describe the association between household income in early childhood and physical health, psychological distress, smoking behaviour, obesity, and educational outcomes at age 17 years, including the patterning and clustering of these five outcomes by income quintiles. Methods: In this population-based, retrospective cohort study, we used data from the Millennium Cohort Study in which individuals born in the UK between Sept 1, 2000, and Jan 1, 2002, were followed up. We collected data on five adverse health and social outcomes in adolescents aged 17 years known to limit life chances: psychological distress, self-assessed ill health, smoking, obesity, and poor educational achievement. We compared how single and multiple outcomes were distributed across early childhood quintile groups of income, as an indicator of disadvantage, and modelled the potential effect of three income-shifting scenarios in early childhood for reducing adverse outcomes in adolescence. Findings: We included 15 245 adolescents aged 17 years, 7788 (51·1%) of whom were male and 7457 (48·9%) of whom were female. Adolescents in the lowest income quintile group in childhood were 12·7 (95% CI 6·4–25·1) times more likely than those in the highest quintile group to have four or five adverse adolescent outcomes, with poor educational achievement (risk ratio [RR] 4·6, 95% CI 4·2–5·0) and smoking (3·6, 3·0–4·2), showing the largest single risk ratios. Shifting up to the second lowest, middle, and highest income groups would reduce multiple adolescent adversities by 4·9% (95% CI –23·8 to 33·6), 32·3% (–2·7 to 67·3), and 83·9% (47·2 to 120·7), respectively. Adjusting for parental education and single parent status moderately attenuated these estimates. Interpretation: Early childhood disadvantage is more strongly correlated with multiple adolescent adversities than any of the five single adverse outcomes. However, shifting children from the lowest income quintile group to the next lowest group is ineffective. Tackling multiple adolescent adversities requires managing early childhood disadvantage across the social gradient, with income redistribution as a central element of coordinated cross-sectoral action. Funding: UK Prevention Research Partnership
Clustering of adverse health and educational outcomes in adolescence following early childhood disadvantage: population-based retrospective UK cohort study
BACKGROUND: Disadvantage in early childhood (ages 0-5 years) is associated with worse health and educational outcomes in adolescence. Evidence on the clustering of these adverse outcomes by household income is scarce in the generation of adolescents born since the turn of the millennium. We aimed to describe the association between household income in early childhood and physical health, psychological distress, smoking behaviour, obesity, and educational outcomes at age 17 years, including the patterning and clustering of these five outcomes by income quintiles. METHODS: In this population-based, retrospective cohort study, we used data from the Millennium Cohort Study in which individuals born in the UK between Sept 1, 2000, and Jan 1, 2002, were followed up. We collected data on five adverse health and social outcomes in adolescents aged 17 years known to limit life chances: psychological distress, self-assessed ill health, smoking, obesity, and poor educational achievement. We compared how single and multiple outcomes were distributed across early childhood quintile groups of income, as an indicator of disadvantage, and modelled the potential effect of three income-shifting scenarios in early childhood for reducing adverse outcomes in adolescence. FINDINGS: We included 15 245 adolescents aged 17 years, 7788 (51·1%) of whom were male and 7457 (48·9%) of whom were female. Adolescents in the lowest income quintile group in childhood were 12·7 (95% CI 6·4-25·1) times more likely than those in the highest quintile group to have four or five adverse adolescent outcomes, with poor educational achievement (risk ratio [RR] 4·6, 95% CI 4·2-5·0) and smoking (3·6, 3·0-4·2), showing the largest single risk ratios. Shifting up to the second lowest, middle, and highest income groups would reduce multiple adolescent adversities by 4·9% (95% CI -23·8 to 33·6), 32·3% (-2·7 to 67·3), and 83·9% (47·2 to 120·7), respectively. Adjusting for parental education and single parent status moderately attenuated these estimates. INTERPRETATION: Early childhood disadvantage is more strongly correlated with multiple adolescent adversities than any of the five single adverse outcomes. However, shifting children from the lowest income quintile group to the next lowest group is ineffective. Tackling multiple adolescent adversities requires managing early childhood disadvantage across the social gradient, with income redistribution as a central element of coordinated cross-sectoral action
Peculiar Broad Absorption Line Quasars found in DPOSS
With the recent release of large (i.e., > hundred million objects),
well-calibrated photometric surveys, such as DPOSS, 2MASS, and SDSS,
spectroscopic identification of important targets is no longer a simple issue.
In order to enhance the returns from a spectroscopic survey, candidate sources
are often preferentially selected to be of interest, such as brown dwarfs or
high redshift quasars. This approach, while useful for targeted projects, risks
missing new or unusual species. We have, as a result, taken the alternative
path of spectroscopically identifying interesting sources with the sole
criterion being that they are in low density areas of the g - r and r - i
color-space defined by the DPOSS survey. In this paper, we present three
peculiar broad absorption line quasars that were discovered during this
spectroscopic survey, demonstrating the efficacy of this approach. PSS
J0052+2405 is an Iron LoBAL quasar at a redshift z = 2.4512 with very broad
absorption from many species. PSS J0141+3334 is a reddened LoBAL quasar at z =
3.005 with no obvious emission lines. PSS J1537+1227 is a Iron LoBAL at a
redshift of z = 1.212 with strong narrow Mgii and Feii emission. Follow-up high
resolution spectroscopy of these three quasars promises to improve our
understanding of BAL quasars. The sensitivity of particular parameter spaces,
in this case a two-color space, to the redshift of these three sources is
dramatic, raising questions about traditional techniques of defining quasar
populations for statistical analysis.Comment: 27 pages, 13 figures, Accepted to the Astronomical Journa
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