... Bojan Nikolic web pages (r. 329) . ... The is the main page for code for Bayesian analysis of radio spectra and similar observational data. ... Nested Sampling in R & analysis of spectra . ... Paper I: Method . ... Observed radio spectra often consist of few measurements (typically 3?10) with significant errors against which it is tempting to try to fit a number of different models. ... page. ... Analysis of (radio) spectra . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

... CB3 0HA, U.K. The UCDs (Unified Content Descriptors) were first developed in the ESO/CDS data mining project, to describe precisely the contents of the individual fields (columns) of tables available from a data center. ... We present different applications of UCDs: selection of catalogues, based on their content; identification of catalogues having similar fields; automated data conversion allowing direct comparison of data in cross-identifications. ... a definition of the corresponding UCD; . ...

Open Systems Handbook: A Guide to Building Open Systems . ... This book is designed to provide interested individuals and organizations with an overview of open systems and the work being done to achieve them. ... This section is organized using a descriptive model of an open systems environment developed by the IEEE PI 003.0 Working Group, which is developing the Guide to POSIX-based Open System Architecture. ... Standards for open systems 13 . Chapter 3: The open systems environment (OSE) 15 . ...

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...

Stars are the fundamental building blocks of galaxies. ... Comparison between observations and models of evolving stellar populations helps understand the star formation process, triggering mechanisms, influence of the environment, the chemical history, and processes in the interstellar gas. Our research concentrates on galaxies with active current star formation. Many of these objects show signatures of violent high-mass star formation, a phenomenon often called `starburst'. ...

... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Late Stages of Stellar Evolution . Welcome to the home page of the Late Stages of Stellar Evolution" We are a research group which operates within the Astrophysics Group of the Australia Telescope National Facility. ... To investigate the late stages of stellar evolution and in particular the role of stellar mass-loss in the evolution of asymptotic giant branch stars, proto-planetary nebulae and extremely massive stars. ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

... Evolution of the coalescence rate of double neutron stars (NS) and neutron star - black hole (BH) binaries are computed for model galaxies with different star formation rates. Assuming gamma-ray bursts (GRB) to originate from NS+NS or NS+BH merging in distant galaxies, theoretical - distributions for gamma-ray bursts (GRB) are calculated for the first time taking the computed merging rates into account. ... Effect of sources evolution on - distribution and -test. ...

... Hopkins: The Phoenix Deep Survey at 1.4 GHz . ... For details of the Phoenix multiwavelength deep survey, refer to MNRAS 296, p839, 1998. ... We present the first results from the Phoenix Deep Survey, a multiwavelength survey of a 2 deg diameter region. Observations in the radio continuum at 1.4 GHz carried out with the Australia Telescope Compact Array are described. The catalogue of over 1000 radio sources compiled from these observations is analysed, and the source counts are presented. ...

XMM-Newton Science Analysis System . ... The current version of omcomb combines the four image segments generated by the full-frame low resolution mode into a single image, which the OM imaging chain task, OMICHAIN, can then process. ... A requirement therefore arose for a task in the OM imaging-chain to recombine the four full-frame low-resolution mode image segments into a single image, and since at the present time the OM slew-chain task is disabled, omcomb has been modified to perform this task. ...

... Download . Description . ... Utilities for building libraries and applications . ... f77 . Global COMMON referenced with f77 INCLUDE statement . ... f77/f90 . ... Tools for building a spectral atlas . ... f77/f90/make . ... Obtaining the software . ... Building subroutine libraries . ... Building spectrum . ... Detailed reports describing bugs in the download/installation procedure or in the software itself will be welcome and should be addressed to Simon Jeffery at the address below. ...

. Appl. Sci. Res. 51, 109-113, 1993. Jacques Lewalle, jlewalle@syr.edu

... The ANU 2.3m telescope building, the Anglo-AuтАж . Sidebar Left . ... Title: The ANU 2.3m telescope building, the Anglo-Australian Telescope dome and the ANU 24-inch telescope dome. ... NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. No use may be made of any of the images without Dr Shobbrook's written permission. ... The ANU 2.3m telescope building, the Anglo-Australian Telescope dome and the ANU 24-inch telescope dome. ...

... PINTofALE was originally developed to analyze spectroscopic data from optically-thin coronal plasmas, though much of the software is sufficiently general to be of use in a much wider range of astrophysical data analyses. ... Kashyap, V. \ Drake, J.J., 2000, BASI, 28, 475 . ... Kashyap, V.L., Lin, L., & Drake, J.J., 2004, AAS, 204, 73.11 . ... Kashyap, V. \ Drake, J.J., 2002, Stellar Coronae in the Era of Chandra and XMM-Newton, June 25-29, 2001, Noordwijk, Netherlands . ... Drake, J.J. \ Kashyap. ...

Electronic Catalogue of Comets "Halley" . ... In this paper we give a description of the Electronic Catalogue of Comets "Halley", which makes it possible to calculate the evolution of the orbits of comets, to visualize orbital motion, to determine the circumstances of a comet's close approach to planets within a given time interval, as well as a number of other opportunities. ...

... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...

Previous Next Table of Contents . The master location for the Plug-In source is at http://www.some.net/~user/gimp/source/plugin.tar.gz You should always be able to get the latest version from here. ... You should put a description of how to build th source here. For most plug-ins this will be the same bit of description, basically, since most plug-ins are single file source code that don't require any special libraries. If your Plug-In requires anything special, describe it here. ...

... Oleg V. Verkhodanov . ... The last few years have changed our view on the evolution of galaxies: the most distant galaxies (i.e. systems having stellar population) have been found at redshift z=6.68 (Chen H.-W., Lanzetta, K. M., Pascarelle, S. 1999, Nature, 398 , 586) and radio galaxy at z=5.19 (van Breugel W., De Breuck C., Stanford S. A., Stern D., Rottgering H., Miley G. 1999. astro-ph/9904272 ). ... Redshifts and age of stellar systems of distant radio galaxies from multicolour photometry data. ...

... AA(Max-Planck-Institut f r Radioastronomie, 53121 Bonn, Germany), AB(Max-Planck-Institut f r Radioastronomie, 53121 Bonn, Germany), AC(Max-Planck-Institut f r Radioastronomie, 53121 Bonn, Germany), AD(Special Astrophysical Observatory, Nizhnij Arkhyz, 357147, Russia), AE(Stockholm Observatory, 13336 Saltsj baden, Sweden) . ... 241B Structural and chemical changes during the AGB and post-AGB evolution are discussed with respect to two recent observational and theoretical findings. ... Abstract Text ....

... A correlation between metal abundance and orbital elements (the eccentricity and angular momentum) has been found for three semples of disk stars of our Galaxy with abundance derived from detailed analysis. The correlation indicates that metal abundance in the Galaxy kept increasing after the birth of old disk stars and that the Galaxy kept collapsing during the formation of its disk subsystems. ...