. Full screen versions . Number - magnitude counts . Number - redshift counts . | Front page | . | << - Redshift wedge | Completeness estimates - >> | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

. Number . Task . Pri . Author . Created By Tool . Created On . Modified On . Completed . Modified By . Assigned To . Link To . Magic . Description

... The MIDAS release 94NOV is the 9th official release of portable MIDAS. A number of new applications have been added to this version. ... It enhances the line editing capabilities of MIDAS, like a history stack of commands, Emacs or Vi editing functions, command and filename completion functions, and a communication channel to the MIDAS GUI Xhelp for a help-on-line function . ... For a more complete list of all updates/additions use the MIDAS command HELP [NEWS] after having installed this release. ...

... Readability |Check number: 1 | Description: Header existence for each |Evaluation (always/often/sometimes/| |source file and for each method, class, |never) : | ... Description: Naming conventions existence |Evaluation (always/often/sometimes/| |(variables start with lowercase, then |never) : | ... limited and commented |(always/often/sometimes/ | ... Description: Error message are formated : when an|Evaluation | error or an exception is raised, report the |(always/often/sometimes/ | ...

<entry> <id><?=$link?>?id=<?=$number?>&amp;db=<?=$db?></id> <author><?=$author?></author> <issued><?=$dbtime?></issued> <modified><?=$dbtime?></modified> <link rel="alternate" type="text/html" href="<?=$link?>?id=<?=$number?>&amp;db=<?=$db?>" /> <title><![CDATA[<?=$title?>]]></title> <content type="text/html" mode="escaped"><![CDATA[<?=$abstract?>]]></content> </entry>

. Assumed Source Spectra (2-10 keV): . Normal AGN: a x = 0.5, N H = 3 10 20 cm -2 . Absorbed AGN: a x = 0.5, N H = 3 10 23 cm -2 . An explanation of and further information on these predictions can be found here . Sky Area vs. flux limit (0.5 - 3.5 keV) . Sky Area vs. flux limit (2 - 10 keV) . Home | Science Goals | Survey Strategy | Publications | Images & Data | Education/Outreach | Internal Page (password access only) . Date Last Modified: 22 April 2002 . Contact: Webmaster .

snap_comp . ... Module snap_comp.py . ... Modules . ... get_completed_visits (prop_id) . Return the number of completed visits in the input proposal. get_total_visits (prop_id) . Return the total number of active visits in the input proposal. get_unique (prop_id, users =True ) . Return either the number of unique users (if users is True) or the number . of unique archive requests (if users is False) to access the data. run (*args) . ... A single argument is allowed, the cycle. ...

This document lists, in reverse chronological order, changes made to Tempo since version 11.000 . ... Added binary model BTJ which allow jumps in Keplerian binary parameters at specified times. ... To override default max number of TOAs or parameters use -m or -l, e.g., "tempo 0833.a -m 200000" for up to 200000 TOAs. ... Added NTOA (number of toas) and TRES (residual) to output xxx.par. ... Added output of calculated binary parameters to parameter file. ... TASC parameter allowed for binary model BT. ...

Numbering Procedures for APO 2.5m and 3.5m Drawings and Engineering/Drafting Documents . ... Document part numbers are to consist of a 7 character long "base numbe,r" which is coded to provide information about the part's intended first use. The part number becomes complete and unique only with the addition of a revision number. ... Example of a "base number": 25CSA01 . ... PART NUMBER CONVENTION . ... For Example: . ... R = "Revision" . ... Questions contact Larry Carey/University of Washington ...

Search engine provided by WebGlimpse . String to search for: . ... Return only files modified within the last days. Maximum number of files returned: 10 50 100 1000 . Maximum number of matches per file returned: 10 30 50 500 . Maximum number of characters output per file: . ... sorted by author . sorted by date . sorted by subject . ...

Hot subdwarfs are hots stars with masses somewhat less than that of the Sun. ... They are known as sdB stars because their spectra are dominated by hydrogen lines. ... Normally, a red giant will switch on core helium burning without losingthe layers of hydrogen around the helium core. sdOB stars are related to sdB stars, possibly being the sdB stars which have completed core helium burning and are evolving to become white dwarfs. ... Such stars are known as PG1159 stars and DO white dwarfs. ...