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http://astro.uni-altai.ru/~aw/stellarium/api/classTelescopeClient.html.

1. Stellarium: BigStarCatalogExtension::StarWrapper< Star > Class Template
... BigStarCatalogExtension::StarWrapper< Star > Class Template Reference . StarWrapper (const SpecialZoneArray < Star > *a, const SpecialZoneData < Star > *z, const Star *s) . ... getJ2000EquatorialPos (const StelCore *core) const . ... getVMagnitude (const StelCore *core, bool withExtinction=false) const . ... getSelectPriority (const StelCore *core) const . ... getInfoString (const StelCore *core, const InfoStringGroup &flags) const . ... getEquinoxEquatorialPos (const StelCore *core) const . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classBigStarCatalogExtension_1_1StarWrapper.html -- 41.7 Кб -- 28.02.2014
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2. lsst.coordConv: coordConv::ObsCoordSys Class Reference
lsst.coordConv љ unknown . ... coordConv::ObsCoordSys Class Reference . ... ObsCoordSys (double date=0) . ... clone (double date) const . ... taiFromDate (double date) const . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom (double &toDir, double &scaleChange, CoordSys const &fromCoordSys, Coord const &fromCoord, double fromDir, Site const &site, double tai=0) const . ... virtual coordConv::ObsCoordSys::~ObsCoordSys . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/coordConv/html/classcoord_conv_1_1_obs_coord_sys.html -- 43.2 Кб -- 07.05.2015
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3. casacore: casa::ROMSObservationColumns Class Reference
... casa::ROMSObservationColumns . ... Definition at line 80 of file MSObsColumns.h . ... Definition at line 111 of file MSObsColumns.h . ... Definition at line 100 of file MSObsColumns.h . ... Definition at line 101 of file MSObsColumns.h . ... Definition at line 102 of file MSObsColumns.h . ... Definition at line 103 of file MSObsColumns.h . ... Definition at line 106 of file MSObsColumns.h . ... Definition at line 104 of file MSObsColumns.h . ... Definition at line 128 of file MSObsColumns.h . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/classcasa_1_1ROMSObservationColumns.html -- 57.2 Кб -- 14.02.2011
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4. Apertures
Optical Filters . The WFPC2 camera configuration and filter set require a substantial number of apertures for full utilization of its capabilities. ... An additional set of aperture names have been defined for use with the WFPC2 filters which require partial rotations. ... The pixel coordinates of these apertures will be reviewed on a regular basis to reflect changes in CCD and filter cosmetics. ... The aperture name is generally the same as the (rotated) filter name. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/wfpc2/W2_31.html -- 5.1 Кб -- 24.07.1996
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5. Actor Prolog User Guide. Residents.
In Actor Prolog a resident is a special mechanism that helps processes to inspect state of other processes. A resident observes the state of a specified (target) process and if the state of the process changes (for instance, after message handling) it proves a specified predicate of the process. ... Work of the resident. ... Any change of the list of target processes or arguments of resident function results in activation of the resident and repeated collection of information in the target worlds. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/Lab144/start/e_reside.html -- 14.6 Кб -- 24.09.2007
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6. –А observer : V–їnus, Spica et des –їtoiles filantes | Ciel et Espace
... Ciel Espace, le magazine qui vous guide toujours plus loin . ... des actualit–їs . ... les plus belles images de l'Univers d–їcrypt–їes pour vous . ... Accueil –А observer : V–їnus, Spica et des –їtoiles filantes . ... Surveillez aussi les –їtoiles filantes . Lorsque le ciel devient sombre, il se peut que quelques m–їt–їores z–Rbrent le ciel, car c'est actuellement le pic d'activit–ї de l'essaim d'–їtoiles filantes des Aurigides . ... 08/08/2013 - Les Nuits des –їtoiles 2013 : cвАЩest parti ! ...
[ Сохраненная копия ]  Ссылки http://www.cieletespace.fr/node/5836 -- 29.9 Кб -- 09.04.2016
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7. ON/OFF (Position Switching)
... The procedure simply observes ON your source for x minutes and then takes a `blank sky' observation OFF your source for the same amount of time and tracking the same azimuth and zenith angle range. ... Typically, observing times are kept to within 5 minutes (with 5 minutes as the most efficient, and therefore default, choice). ... If your scans are for 5 minutes or less, your wait time should be set to 1 minute (the default setting). ... A 5 minute ON/OFF + 10s CAL takes 11.3 minutes. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/spectral_line/handbook_old/node9.html -- 6.0 Кб -- 31.05.2001
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8. ESO - Observing conditions: definitions
... Science Users Information > Observing with ESO Telescopes > Phase 2 Preparation > Observing conditions . ... Service Mode Philosophy . ... The following definitions of the observing conditions are common between Phase 1 preparation and Phase 2 preparation, as well as between Service Mode and Visitor Mode observations. ... There are additional Service Mode Policies and Service Mode Guidelines regarding the observing conditions. ... Seeing (Phase 1) and Image quality (Phase2) constraints . ... Moon . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/observing/phase2_p95/ObsConditions.html -- 31.6 Кб -- 10.04.2016
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9. Calculating the Position and Velocity Components of HST
... The HST uses an onboard model of its orbit to perform in real-time various control functions relating to spacecraft operations and observation support. ... New coefficients for the ephemeris are updated every other day, and are archived as FITS keywords for each HST observation data set. Using these coefficients,an observer can perform a variety of calibration and characterization calculations relating to the orbital position and velocity of the telescope. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/aket.html -- 12.3 Кб -- 03.11.2000
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10. Star formation
... Unbiased surveies of star-forming regions; evolutionary processes in star formation; IMF; determination of evolutionary tracers . ... Light elements; mixing in stars . ... Spectroscopy of low-mass stars in SFRs/associations: cluster formation, triggered SF, SFHs, accretion properties . ... Influence of cooling e and magnetic field on the formation of primordial stars . ... This email address is being protected from spambots. You need JavaScript enabled to view it. ... 39 0552752 251 . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/research/star-formation -- 38.1 Кб -- 09.04.2016
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11. Order Definition
... The first of the equations defines the position of the spectral orders, m , in the raw image, while the second equation gives, for each order, the dispersion relation in one dimension. ... where the coefficients are computed using least squares techniques on a grid , i.e. sample number and line number of points located within the spectral orders of the image. These points in the grid are found automatically by an order--following algorithm, normally using the FLAT or STD image. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94N