Index of mentions of St. Augustin\u27s Church and School in Newport Daily News, 1900-1940

List of mentions of the St. Augustin\u27s Church and St. Augustin\u27s School in the Newport Daily News, listed alphabetically by subject with date.https://digitalcommons.salve.edu/st-augustin/1001/thumbnail.jp

Index of mentions of St. Augustin\u27s Church and School in Newport Daily News, 1970-1999

List of mentions of the St. Augustin\u27s Church and St. Augustin\u27s School in the Newport Daily News, listed alphabetically by subject with date.https://digitalcommons.salve.edu/st-augustin/1003/thumbnail.jp

Chronological List of mentions of St. Augustin\u27s Church and School in Newport Daily News (1910-1995, 2007, 2013), with list of pastors, clergy, and teachers

List of mentions of the St. Augustin\u27s Church and St. Augustin\u27s School in the Newport Daily News, listed chronologically. Also included are a list of pastors, clergy, and teachers associated with the parish.https://digitalcommons.salve.edu/st-augustin/1005/thumbnail.jp

The Augustin Capacity and Center

For any channel, the existence of a unique Augustin mean is established for any positive order and probability mass function on the input set. The Augustin mean is shown to be the unique fixed point of an operator defined in terms of the order and the input distribution. The Augustin information is shown to be continuously differentiable in the order. For any channel and convex constraint set with finite Augustin capacity, the existence of a unique Augustin center and the associated van Erven-Harremoes bound are established. The Augustin-Legendre (A-L) information, capacity, center, and radius are introduced and the latter three are proved to be equal to the corresponding Renyi-Gallager quantities. The equality of the A-L capacity to the A-L radius for arbitrary channels and the existence of a unique A-L center for channels with finite A-L capacity are established. For all interior points of the feasible set of cost constraints, the cost constrained Augustin capacity and center are expressed in terms of the A-L capacity and center. Certain shift invariant families of probabilities and certain Gaussian channels are analyzed as examples.Comment: 59 page

Multiwavelength modelling the SED of supersoft X-ray sources. I. The method and examples

Radiation of supersoft X-ray sources (SSS) dominates both the supersof X-ray and the far-UV domain. A fraction of their radiation can be reprocessed into the thermal nebular emission, seen in the spectrum from the near-UV to longer wavelengths. In the case of symbiotic X-ray binaries (SyXBs) a strong contribution from their cool giants is indicated in the optical/near-IR. In this paper I introduce a method of multiwavelength modelling the spectral energy distribution (SED) of SSSs from the supersoft X-rays to the near-IR with the aim to determine the physical parameters of their composite spectra. The method is demonstrated on two extragalactic SSSs, the SyXB RX J0059.1-7505 (LIN 358) in the Small Magellanic Cloud (SMC), RX J0439.8-6809 in the Large Magellanic Cloud (LMC) and two Galactic SSSs, the classical nova RX J2030.5+5237 (V1974 Cyg) during its supersoft phase and the classical symbiotic star RX J1601.6+6648 (AG Dra) during its quiescent phase. The multiwavelength approach overcomes the problem of the mutual dependence between the temperature, luminosity and amount of absorption, which appears when only the X-ray data are fitted.Thus, the method provides an unambiguous solution. It was found that selection of the model (a blackbody or an atmospheric model) is not of crucial importance in fitting the global X-ray/IR SED. The multiwavelength modelling of the SED of SSSs is essential in determining their physical parameters.Comment: 15 pages, 11 figures, 2 tables, accepted for New Astronom