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After the first few quasars were found, many others were discovered and observed Some quasars had been photographed previously, but in the photographs they had been dismissed as ordinary stars In one case, when several photographs having been taken over a period of decades were examined, it was found that large changes in brightness had occurred within periods of a few months This implied that the quasar is a fraction of a light-year in diameter However, if its red shift is a correct indicator of its distance, its energy output is many times that of a normal galaxy! Quasars are concentrated, as well as intense, sources of energy When observed with radio telescopes having high resolution less than 1 second of arc in some cases some quasars still appear as point sources This is also true of the nuclei of certain radio galaxies Optically, many of the quasars look like point sources of light, and therefore, they resemble stars, until the extreme magnification and resolving power of the Hubble Space Telescope (HST) is put to work on them Then some quasars show evidence of glowing matter around a central, intense core Some quasars can be resolved into components by radio telescopes, but this requires the use of multiple antennas and a baseline of hundreds or even thousands of kilometers Antennas in diverse locations on Earth are linked by satellite communications systems, and their outputs are combined by computer programs in order to accomplish this This provides the equivalent resolving power of an antenna much larger than any single structure that could be constructed The angular resolution goes down to less

Once the changes are captured, ODI can use a publish-and-subscribe model for propagating changes to the destination database in real time or near real-time (based on the capture method) The CDC Knowledge Module support for non-Oracle sources and their specific versions needs to be consulted prior to deciding on using ODI

ASP.NET is configured to protect files with the extension .sitemap so they cannot be seen by a browser.

than 0001 second of arc With such sophisticated apparatus, radio galaxies and quasars have been probed in detail

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Third-party tools exist in the market and are capable of migrating database schemas, database stored objects, and server-side scripts from non-Oracle systems to Oracle The effectiveness of these tools needs to be investigated thoroughly against your database environment A tool should be evaluated for its support for the source database type, the object types it can automatically migrate, and its automated conversion rates You should remember that each database environment is different, and the success and automated conversion rates of these tools from one successful migration cannot be generalized, since you might not get the same results in your environment as have been achieved in other scenarios Using advertised conversion rates and success stories as a guideline might help, but cannot be taken as accurate estimates and applied as-is to your migration project The best way to get an insight into the effectiveness of the tool is to perform a proof of concept with the vendor on a sample representation of your environment and observe the results There are third-party vendors that provide end-to-end migration services that encompass the use of automated tools along with manual migration services These vendors utilize the best on-shore and off-shore implementation models (sometimes referred to as best shore) to considerably lower the cost of manual migrations This book does not discuss third-party service providers or third-party migration tools

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Once the site map file is in place, you need to identify it to the master page. This is done by dragging a SiteMapDataSource control from the Data section of the Toolbox onto the master page. By default, the SiteMapDataSource control will look for and use the file named Web.sitemap. It doesn t matter where you place this SiteMapDataSource control, as long as it is somewhere between the <form> and </form> tags in Source view. The SiteMapDataSource will be visible in Design view but will not appear when the web site is run. The Design view should look something like Figure 6-20.

This section will highlight the important methods and steps currently in use for migrating Oracle Databases residing on non-Exadata platforms to the Oracle Database 11g Release 2 on the Database Machine These methods will be discussed at a high level; for detailed step-by-step instructions, refer to the Oracle Database documentation and the My Oracle Support portal

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