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... ApJ Intro paper Appendix . ... Chandra Survey . ... The ChaMPlane survey is being conducted at the Harvard-Smithsonian Center for Astrophysics. ... Dominance of Magnetic Catalysmic Variables in the Resolved Galactic Ridge X-ray Emission of the Limiting Window . ... Spectroscopic Follow-up of X-Ray Sources in the ChaMPlane Survey: Identification of a New Cataclysmic Variable . ... 2012, ApJ 748, 32 ( astro-ph/1112.0606 ) . The ChaMPlane bright X-ray sources - Galactic longitudes l=2-358 deg . ...

... To select this, type 'use PALFA;' h. To list the tables in the database, type 'show tables;'. ... 2) Tables in the PALFA database : To print the fields contained in each of these tables , follow the steps in 1) for connecting to the database and then type 'describe **tablename**;' where **tablename** is one of the following: atnfshort: This contains the pulsars in the ATNF catalog, with a reduced number of parameters for each pulsar. candidates: This table will contain the candidates ...

... Field size . Object name . ... Map size . ... Field size: the approximate size of the map in the Y direction. ... Galaxies: . ... Galaxies, which size exceeds some value depending on the field and map sizes, are displayed with their real positional angles and sizes by 25m isophote. ... In the "tools" fields there are links to the several famous AVO (Astrophysical Virtual Observatory) resources: NED and Simbad databases and DSS2 (Palomar Digitized Sky Survey) images of the corresponding sky area. ...

... very large . no limits in x,m . ... x, m, alpha . ... no limits in x,m,alpha . As a first approximation when one wants to learn possible effects of nonsphericity of scatterers. seldom . ... very large / large . ... Study of shape effects since spheroids with different semiaxis ratio present a set of 2D shapes from needles to disks (incl. spheres) . ... Study of complex shape effects. seldom . ... Possible study of 3D shape effects. ... Possible study of shape and structure effects. ...

... 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. Efficient data mining in the X-ray sky background John Cunniffe, Evert J.A. Meurs Dunsink Observatory, Castleknock, Dublin 15, Ireland Aaron Golden IT Centre, NUI Galway, University Road, Galway, Ireland Abstract. Abstract: The calculation of flux upper limits in the sourcefree ("background") regions of photon-limited images is complicated by instrumental and statistical modeling and requires non-trivial computational effort. ... 2004). ...

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... We estimate that the energies so obtained are accurate to +/- 2000 cm-1. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % P.R.Young and E.Landi 1999 . ... contains the spline fits to the scaled proton collision strengths. ...

... 150Trushkin Verkhodanov We present results of cross-identifications of the objects from two large catalogs, IRAS-Point Source and Texas, in the database CATS. ... In the 511 ITA sources, already identified with different sources in the initial IRAS catalog, galaxies and Milky Way radio sources dominated. ... However radio catalogs at the higher frequencies than those of the Texas catalog, which are more sensitive to extended objects radiation, are needed for cross-identification with the IRAS...

... Table 32.2 summarizes the nominal initial accuracies for different kinds of acquisitions. ... FOS Target Acquisition Calibration Accuracies . ... ACQ . ... Blind Pointing . ... In summary, the pointing accuracy limitations of FOS target acquisition methods are: . ... ACQ/PEAK: . ... This was the value achieved by all FOS externally pointed calibration observations obtained after July 1, 1992 and was the ultimate limiting positional accuracy of FOS photocathode granularity and sensitivity calibration...

... Perform a search for the words 'database' or 'query'. ... SELECT *, headline(line, to_tsquery('database | query')), rank(ts_vec, to_tsquery('database | ... query') ORDER BY rank(ts_vec, to_tsquery('database | ... 44 line | documents could be stored in file system), database and query engine. ts_vec | ... documents could be stored in file system), database and query engine. rank | ... tsearch2 as a storage, while database engine is used as a query executor ts_vec | ...