Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory

The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth's crust. Tau leptons from nu(tau) charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January 2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of nu(tau) at EeV energies. Assuming an E(nu)(-2) differential energy spectrum the limit set at 90% C. L. is E(nu)(2)dN(nu tau)/dE(nu) < 1: 3 x 10(-7) GeV cm(-2) s(-1) sr(-1) in the energy range 2 x 10(17) eV< E(nu) < 2 x 10(19) eV.

Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming nu(tau) may interact in the Earth's crust and produce a tau lepton by means of charged-current interactions. The tau lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by tau decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is detailed. Systematic uncertainties in the exposure from the detector, the analysis, and the involved physics are discussed. No tau neutrino candidates have been found. For neutrinos in the energy range 2x10(17) eV < E(nu)< 2x10(19) eV, assuming a diffuse spectrum of the form E(nu)(-2), data collected between 1 January 2004 and 30 April 2008 yield a 90% confidence-level upper limit of E(nu)(2)dN(nu tau)/dE(nu)< 9x10(-8) GeV cm(-2) s(-1) sr(-1).

Ireland and Northern Ireland's Population Health Observatory (INIsPHO)

Ireland and Northern Ireland's Population Health Observatory (INIsPHO) is housed in  The Institute of Public Health in Ireland (IPH) and is part of the Association of Public Health Observatories (APHO). The Observatory supports those working to improve health and reduce health inequalities by producing, disseminating and supporting the use of relevant health knowledge and strengthening the research and information infrastructure on the island of Ireland.

The Public Health Observatory Handbook of Health Inequalities Measurement (2005)

This SEPHO handbook primarily focuses on the measurement and interpretation of health inequalities. Written by Roy Carr-Hill and Paul Chalmers-Dixon of York University, it provides a comprehensive collection of material for those concerned to document and understand health inequalities.

London Health Observatory - Inequalities Reports

Inequality reports from the London Health Observatory from 1996 to 2010.

A Novel Autonomous Observation Platform for Multi-Disciplinary Investigations at the Cape Verde Ocean Observatory (CVOO)

In order to investigate the spatial and temporal variability (daily, seasonal and inter-annual) of CO2 and O2 air-sea fluxes and their underlying processes, a dense network of observations is required. For this purpose, the Cape Verde Ocean Observatory (CVOO) provides a unique infrastructure. Information thus obtained also links biological productivity and atmospheric composition. To expand these capabilities, a novel “virtual mooring” approach for high resolution measurements, based on a modified NEMO profiling float, is pursued. This Profiling Float was equipped with O2 and pCO2 sensors for the first time, in order to collect daily depth profiles (0-200 m) in the vicinity of the ocean site. Data access and remote control is provided through Iridium satellite telemetry. Recalibrations and redeployments are carried out every 1-3 month. First, we present the new developed instrument and the innovative in situ and real-time approach behind. Second, we show the inter-disciplinary scientific objectives which will benefit from this approach as a result of the intensive partnership between IFM-GEOMAR and INDP during the last years.

Proposed gravitational wave observatory based on solid elastic spheres

Spherical gravitational wave (GW) detectors offer a wealth of so far unexplored possibilities to detect gravitational radiation. We find that a sphere can be used as a powerful testbed for any metric theory of gravity, not only general relativity as considered so far, by making use of a deconvolution procedure for all the electric components of the Riemann tensor. We also find that the spheres cross section is large at two frequencies, and advantageous at higher frequencies in the sense that a single antenna constitutes a real xylophone in its own. Proposed GW networks will greatly benefit from this. The main features of a two large sphere observatory are reported.

[Voyage en Italie : 1824-1830]. , Panoplia Manuscrit grec du Vatican XII[e] Siècle. St François d'Assise. XIII[e] Siècle : [sept motifs : cinq personnages (trois hommes nimbés, une Vierge à l'enfant et un personnage non identifé), une croix, détail ornemental d'un arc] : [dessin] / h. L. [Henri Labrouste]

Référence bibliographique : Weigert, 614

[Voyage en Italie : 1824-1830]. , [Musée du Vatican, détail d'une composition ornementale] : [un motif] : [dessin] / [Henri Labrouste]

Référence bibliographique : Weigert, 619

[Voyage en Italie : 1824-1830]. , [Bas-relief, cippe, deux urnes funéraires] au Musée du Vatican : [quatre motifs] : [dessin] / h. L. [Henri Labrouste]

Référence bibliographique : Weigert, 618

[Voyage en Italie : 1824-1830]. , [Cuve de bain en basalte, socle à motifs de griffons, motif de palmette] au Musée du Vatican : [trois motifs] : [dessin] / h. L. [Henri Labrouste]

Référence bibliographique : Weigert, 617