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1. Adaptive filtering from the wavelet transform
Next: Hierarchical adaptive filtering Up: Noise reduction from Previous: Hierarchical Wiener filtering . In the preceding algorithm we have assumed the properties of the signal and the noise to be stationary. The wavelet transform was first used to obtain an algorithm which is faster than classical Wiener Filtering. ... Knowing the noise distribution, we can determine the statistically significant level at each scale of the measured wavelet coefficients. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node344.html -- 7.0 Кб -- 23.02.1996
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2. Observing with VISTA
Home . ... Observing . Exposure Time Calculator (ETC) . Survey processing . ... ESO - Public Surveys . near IR surveys . ... Exposure Time Calculator . ... Survey Area Definition Tool . Recommended values for Detector Integration Time (DIT) . ... Detector Properties . ... Filter properties . ... ESO ][ VISTA Home ] ...
[ Сохраненная копия ]  Ссылки http://www.vista.ac.uk/observing/index.html -- 8.0 Кб -- 24.10.2012
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3. GPI IFS Data Handbook GPI Data Pipeline 1.0 documentation
... GPI Data Pipeline 1.0 documentation . ... GPI IFS Data Handbook . ... GPI IFS Detector Properties . ... This document describes the GPI Integral Field Spectrograph (IFS), the properties of its output data, including various systematics and noise sources that one may encounter, and how these data should be calibrated. Its goal is to summarize in one place all the properties of GPI data that a new user should be familiar with to usefully work with the data. ... Field of View and Lenslet Geometry . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~mperrin/software/gpidata/ifs/index.html -- 12.0 Кб -- 14.02.2014
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4. Database of Optical Properties -- Level: database
Optical characteristics of non-spherical scatterers . ... A list of reviews (under preparation) and links to the databases of Hovenier's and Gustafson's groups on the visible/infrared and microwave light scattering experiments, respectively. ... Light scattering codes . ... Benchmarks in optical properties . Tables of different light scattering characteristics carefully calculated by different codes (methods). Dependence of optical properties on scatterer parameters . ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/1-dbase.html -- 5.9 Кб -- 19.11.2010
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5. Mail Filters
... This appendix tells you how you can use JavaScript to filter your incoming mail and news when you use Netscape Messenger. ... Write a JavaScript function to serve as a filter and put it in your filters file. This function takes one argument, a message object, and can make changes to that message. ... News Filters . ... This file contains the JavaScript functions that perform the mail filtering. ... For news filters it is a News Message object and for mail filters it is a Mail Message object. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientguide/mail.htm -- 18.2 Кб -- 07.10.1999
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6. Stellarium: MeteorMgr Class Reference
Stellarium 0.12.3 . ... Classes . ... ClassљList . ... MeteorMgr Class Reference . Simulates a meteor shower. ... intљ . getZHR (void) . ... setFlagShow (bool b) . ... getFlagShow (void) const . ... MeteorMgr (int zhr, int maxv) . ... virtual voidљ . ... virtual boolљ . ... the initial value of the maximum meteor velocity. virtual void MeteorMgr::draw . ... Get the current zenith hourly rate. virtual void MeteorMgr::init . ... Set the zenith hourly rate. virtual void MeteorMgr::update . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classMeteorMgr.html -- 30.9 Кб -- 28.02.2014
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7. Suppression of detector noise at low energies
... While there is practically no detector noise present at energies above , X-ray data below are considerably contaminated by noise events, which become more and more dominant towards the lowest transmitted energies (Fig. ... Investigations of 40 hours of in-orbit calibration data with the filter wheel closed, taken over a period of more than two years, showed that the noise properties vary with position and energy, but are fairly stable in time for most areas on the detector. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/epreject/node5.html -- 10.4 Кб -- 01.07.2008
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8. casacore: casa::HDF5HidProperty Class Reference
... Classes . Files . ... casa . casa::HDF5HidProperty . ... A class representing an HDF5 property hid. ... HDF5HidProperty ( hid_t hid) . ... operator= ( hid_t hid) . ... Get the hid. operator hid_t () const . ... hid_t casa::HDF5HidProperty::getHid . ... casa::HDF5HidProperty::operator hid_t . ... Convert automatically to hid_t. Definition at line 73 of file HDF5HidMeta.h . ... hid_t casa::HDF5HidProperty::itsHid [private] . ... Referenced by getHid() , operator hid_t() , and operator=() . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/classcasa_1_1HDF5HidProperty.html -- 20.7 Кб -- 14.02.2011
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9. ChaMP Initial Data Release - X-ray
... champ name : Source ID in the format explained in the Definitions section. ra : RA in decimal degrees. ... pos_error : Source count extraction radius in arcseconds. netB : net counts in B-band. See Definitions section. error_netB : error of net counts in B-band. see Definitions section. netS : S-band net counts, defined analogously to netB . ... See Definitions section. C21 : X-ray color. ... C32 : X-ray color. See Definitions section. rateB : B-band count rate in ksec. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/CHAMP/IMAGES_DATA/XRAY/index.html -- 4.6 Кб -- 02.10.2012
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