... PmWiki . ... The files in this directory include: . README.txt An introductory document pmwiki.php The main PmWiki script local/ Configuration scripts (local configuration files) cookbook/ Recipes (add-ons) from the Cookbook docs/ Brief documentation, sample configuration scripts pub/ Publicly accessible files pub/css/ Extra CSS stylesheet files [1] pub/guiedit/ pub/skins/ Layout templates for custom look and feel scripts/ Scripts that are part of PmWiki wikilib.d/ Bundled default PmWiki pages . ...

... Science Users Information > Science and Technical Meetings > Conferences 1998 > eso-osa98 . ... The European Southern Observatory and the Optical Society of America are cosponsoring for the second time a topical meeting on Adaptive Optics. ... The meeting will cover the full range of topics from astronomical observational results and techniques, to foreseen breakthroughs in astrophysics due to new generation systems, from data reduction techniques, to AO system engineering and developments. ...

... GPI Data Pipeline 1.0 documentation . ... Installing Compiled Executables for use with the IDL Runtime . ... If you do not have an IDL license, the GPI Data Reduction Pipeline is distributed as compiled code along with the IDL runtime. ... gpi_pipeline_1.0_runtime_macosx.zip - GPI pipeline compiled code plus IDL runtime for Mac OS X . gpi_pipeline_1.0_runtime_linux.zip - GPI pipeline compiled code plus IDL runtime for Linux . ... unix% idl -rt=/path/to/executables/gpi_launch_pipeline.sav . ...

Welcome to the 10C Survey website! ... The first 10C Survey results from an area of 27 sq. degrees complete to 1 mJy and 12 sq. degrees complete to 0.5 mJy have now been released. ... The first results from the survey, which is the deepest extragalactic radio source survey of any significant extent (> 0.2 sq. degrees) above 1.4 GHz, including the deep 15.7-GHz source count are contained in AMI Consortium: Davies et al. ... For each field, deep and shallow areas have been defined. ...

... Obtaining the software . ... a. Decide on the root directory where your software is going to go.... /home/friday , for example. b. In your .cshrc file, define . ... home/friday/]lib . ... after make ) an object code library ../pack/qub/libqub.a . ... Then a common section of code, found in ../pack/make_library supplies all the necessary targets: . ... remove The conservative way to build this library is to cd /home/friday/pack/qub; make; make install; make clean . ... cd /home/friday/pack; make . ...

The Arcetri Catalog contains measures and bibliographic data for all known H2O maser sources north of declination = -30 degrees (to be observable with the Medicina radiotelescope). ... This database is fully described in Cesaroni et al. ... A statistical analysis on the atlas has been carried (Palagi et al 1993). R. Cesaroni, F. Palagi, M. Felli, M. Catarzi, G. Comoretto, S. Di Franco, C. Giovanardi, F. Palla: A Catalogue of H2O maser sources north of delta=-30 , Astronomy and Astrophysics Suppl., ...

... To install PINTofALE: 0. If all you need are the IDL procedures, download and unpack http://hea-www.harvard.edu/PINTofALE/PoA_pro_current.tar.gz and add the location to IDL's !PATH. ... Assuming that PINTofALE will be installed in the directory /foo/bar/, type cd /foo/bar/ gunzip -c PoA_current.tar.gz | ... One possible method is to include the following (or equivalent) in your $HOME/.cshrc setenv PINTofALE /foo/bar/PINTofALE if ( $?IDL_PATH ) setenv IDL_PATH +$PINTofALE/pro\:${IDL_PATH} if (! ...

... Using the Proc Filesystem Interface . ... You can use the /proc filesystem interface to obtain run-time information about the driver, any installed NVIDIA graphics cards, and the AGP status. This information is contained in several files in /proc/driver/nvidia . proc/driver/nvidia/version . ... Information about the installed AGP card's AGP capabilities. /proc/driver/nvidia/agp/host-bridge . Information about the host bridge (model and AGP capabilities). /proc/driver/nvidia/agp/status . ...

... This possibility is certainly helpful in case you did not obtain separate bias calibration frames or in case you want to determine the bias offset for each science frame individually. ... Table: CCD keywords for overscan fitting . ... In case of a zero order fit the correction is a simple constant. ... After every interactive has been completed the command will ask you if you want to fit the next frame interactively as well, or if you want to apply the overscan correction to all subsequent frames. ...

... In this example we will use /usr/local/data/catalogue for the location of all original catalogues, and /usr/local/scisim-x.y.z for the installation directory of SciSim . ... The installer has to specify their full path in the csim_config section of / usr / local / scisim-x.y.z /config/ scisim .cfg : gsc_regions / usr / local / scisim-x.y.z / data / catalogue /gsc.regions tic_ data / usr / local / scisim-x.y.z / data / catalogue /TICcat.dat wga_ data / usr / local / scisim-x.y.z / data / ...

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

... PUL2 catalog contains original absolute proper motions of 59646 stars in 149 fields with galaxies. ... Mean errors of relative proper motions in PUL2 catalog is 5.5 mas/year. ... The external mean error of one relative proper motion of a bright star of PUL2 catalog is 9 mas/year for both of coordinates. ... After issue of UCAC2 catalog, we decided to improve accuracy of proper motions, using Pul-3 coordinates (of 1950s) as the first epoch, and UCAC2 coordinates as the second epoch. ...

... 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. User provided reduced data, catalogues and atlases in the ISO Data Archive Alberto Salama, Inaki Ortiz, Christophe Arviset, John Dowson, Pedro ~ ґ ario, Cґcile Gry, Jose Hernґndez, Rosario Lorente, Jean Garcia-L e a Matagne, Pedro Osuna, Jesus Salgado, Eva Verdugo ISO Data Centre, RSSD, ESA VILSPA, PO BOX 50727, 28080 Madrid, Spain Abstract. ... The ISO Data Archive (IDA) has been enhanced to host these new products. ...

User has possibility to start running the application being in any item of ephemeris menu. To do this click on Run button at the bottom of Ephemerides dialog box. The Calculation progress dialog box allows one to keep track of run. ... After inspecting them the calculations can be continued by selecting Ephemerides item in menu bar and then Continue item in drop-down box. For information about current task select Ephemerides item in menu bar and then Task Info item in drop-down box. ...

... Limit of star magnitude. If you want to obtain best results, you should use reference stars not more dimly than limiting star magnitude of your telescope. Limiting star magnitude depends on time of an exposition also.) This value should be set as " maximum of star magnitude " in a dialog box " Extraction from catalogue". To find darkest stars in the frame, make the following: . ... Two star magnitudes (m1, m2 in two photometric systems) will be outputted in the window "Information". ...

... 1) Our CAS system will store the catalogues. ... Each catalogue should contain one or more tables. 2) The names of the catalogues should be unique, as well as the the names of tables of the SAME catalogue. ... 4) All the metadata about the CAS system, its tables, catalogues should reside in separate schema (currently "cas_metadata"). 1) The main system table of CAS is the table "catalog_list". ... short info (column "info") . ... 2) The second system table of CAS is the table "table_list". ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The ionogram catalogue is divided into the data file and the key file. ... The station codes database consists of the data file and two key files. ... This database consists of the data file and the key file. ... The antenna DB consists of two interrelated databases. ... The data file contains the following information: antenna type, antenna name, antenna parameters names, measurement units, and ranges of parameters. ...

Observational data on solar activity is a basement for investigation of processes that take place on the Sun and interplanetary space, with data of long-term observations being of special importance. ... Subsection "Sunspot groups" is the catalogue of all sunspot groups that were observed in the given year. ... For every day of observation of the group the area of the group, the area of the largest spot (both areas - in millionths of solar hemisphere) and number of spots in the group are presented. ...

The bisque directory contains software for communicating with Software Bisque's Paramount ME. mks === This protocol is a native linux application. ... The protocol has been tested only with the Paramount ME's serial interface. ... It should be possible to switch back and forth between these applications. tsx === This protocol communicates with TheSkyX Professional (TSX) through its Orchestrate scripting program. ... At this time TSX and Orchestrate are available for Windows and Mac OSX, but not Linux. ...

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...