... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Risks Comparable to NEOs . ... The Increasing Rate of Discovery of Asteroids . ... Comet and Asteroid Collision Probabilities . ... Extreme albedo comets and the impact hazard (PDF Format) . ... Asteroid Impact Animations . ... Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids - 2002 . ... The Spaceguard Survey Report, 1992 (PDF) . Tsunami from Asteroid/Comet Impacts . ...

... A file upload element on an HTML form. ... JavaScript 1.1: added type property . ... The HTML INPUT tag, with "file" as the value of the TYPE attribute. For a given form, the JavaScript runtime engine creates appropriate FileUpload objects and puts these objects in the elements array of the corresponding Form object. ... form . ... For all FileUpload objects, the value of the type property is "file" . ... Use the value property to obtain the file name that the user typed into a FileUpload object. ...

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...

... CentralProcessor 0.11 documentation . ... The Central Processor Manager is the local monitoring and control agent for the Central Processor sub-system. ... At the moment the Central Processor Manager only controls the acquisition phase; that is, it only controls the ingest pipeline. ... In addition to the CP manager specific parameters, any parameters that begin with ice_properties are passed directly to the ICE Communicator during initialisation. ... string . ... Central Processor Manager . ...

. XMM-Newton Science Analysis System . dssetlabel (daltools-1.9) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . Mand . Type . Default . Constraints . label . yes . String . The label to assign to the object . object . yes . String . Fully qualified column, table, attribute or array name . Parameter . Mand . Type . Default . Constraints . XMM-Newton SOC/SSC -- 2008-07-02

... ALTER FULLTEXT .. OWNER -- change the owner of a full-text object . ALTER FULLTEXT { PARSER|DICTIONARY|CONFIGURATION } name OWNER TO newowner ; . ... The new owner of the full-text object. ... Then we change owner of the new dictionary. ... CREATE SCHEMA test; =# CREATE FULLTEXT DICTIONARY test.synonym LIKE pg_catalog."synonym"; =# SHOW search_path; search_path ---------------- "$user",public =# SET search_path TO test,public; =# ALTER FULLTEXT DICTIONARY synonym OWNER TO megera; . ...

... This effect is visible in Figure 4.3 which shows a logarithmic stretch of the image resulting from a 100s exposure on a star of V magnitude 2.6 through filter F502N in the PC. Extreme overexposure of the Loral CCDs is not believed to cause any permanent effects, and therefore the WFPC2 does not have a bright object limit. ... Several other artifacts that are common in saturated stellar images are also obvious in Figure 4.3 . ... Figure 4.3: Saturated Stellar Image Showing Horizontal Smearing. ...

There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...

... NED Home . ... Redshift: Between 0.150000 and 0.270000 . Include ALL Object Type: QSO Radio . ... Number of Essential Note) RA DEC Type km/s z Qual arcmin Refs Notes Phot Posn Vel/z Assoc Images 1 30000 0.228000 0.0 26 0 8 3 0 0 Retrieve 2 30000 0.181000 0.0 5 0 4 1 0 0 Retrieve 3 30000 0.171000 0.0 67 1 1 0 0 0 Retrieve 4 30000 0.260000 0.0 90 1 16 5 0 0 Retrieve 5 30000 0.163009 0.0 170 10 5 4 3 0 Retrieve 6 30000 0.245000 0.0 27 1 1 2 1 0 Retrieve 7 30000 ...

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

... The used with LSS CCD camera (1994,*) was designed in the Laboratory of Spectroscopy and Photometry of Extragalactic Objects of SAO RAS on the base of CCD chip ISD015A ("Electron", St-Petersburg). The cryostat of CCD camera was produced in VNIIT. CCD camera authors: Gudkin (VNIIT), V.L.Afanasiev and S.V.Drabek (SAO) . A cryostated Charge Coupled Device (CCD) parameters: . ... ADU . ... 0 - 8191 ADU . ... Back to LSS main page. Back to Laboratory Home Page . ...

... 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. ...

... Doug's Home Page . ... The output was created using version 1.00 of the module, using the PDL support , together with the S-Lang library from CIAO 3.2 . ... Set up everything in S-Lang code and execute it from Perl # use strict; use Inline 'SLang'; # access the fit results from Perl # print Now in perl \n ; my $res = get_par ( ptest ); print Fit results:\n ; foreach my $par ( @{$res} ) { printf parameter : %-15s , $$par{name}; if ( $$par{ frozen } ) { printf [ ...

Pulkovo NEO Page . ... EPOS Software Package . ... EPOS ( E phemeris P rogram for O bjects of the S olar system) is the Windows PC application for study and ephemeris support of observations of the Solar system objects. ... It controls the part of common data and transfers the control to one of the programs that solve the restricted set of tasks. ... So with the EPOS software package one can calculate the accurate ephemerides for many objects and get the quick illustration of their motion as well. ...

... Classes . ... gTime Class Reference . This class implements time calculations. ... gTime (double ai_jDays=0) . ... gTime (const gTime &timeSrc) . ... Set the time value of the time object to the julian day of year, day. ... operator= (const gTime &timeSrc) . ... Returns the time GMT value in Julian days. ... Returns the time_t value of the gTime Object. ... Returns a gTime object setted with the actual machine time. ... gTime Object assigned with real machine time. double gTime::getGmtTm . ...

Starburst models, May 2006 R.Siebenmorgen and E. Kr"ugel, AA submm., astroph/0606444 Spatially integrated SEDs are computed for starbursts at a distance of 50 Mpc. Free model parameter are the radius, total luminosity, visual extinction (measured from center to surface) and as secondary parameter the luminosity ratio of hots spots to total. Models are sorted in directories named by the applied radius of the nucleus. ... Each file in the subdirectories contain a particular SED model. ...

... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...

Общая Астрономическая Конференция > Практика > Астрономический наблюдательно-информационный портал > Хвостатые гостьи (все о кометах) > C/2014 E2 (Jacques) _ CK14E020 _ S002692 object - комета в созвездии Орла (Aquila) .. ... Просмотр полной версии : C/2014 E2 (Jacques) _ CK14E020 _ S002692 object - комета в созвездии Орла (Aquila) .. ... C/2014 E2 (Jacques) _ CK14E020 _ S002692 object - самая яркая комета летнего неба в созвездии Кассиопеи (Cassiopeia (http://www.starlab.ru/showthread.php?t=20402))! ...

... Space flight . ... Zero Gravity . ... Characteristics of a Complex Flight: . ... Characteristics of the Reduced Gravity (Lunar Gravitation): . ... Characteristics of the Reduced Gravity (Martian Gravitation): . ... Services / Zero Gravity: General description Technical description Flight parameters Photo gallery Price . ...