SiD Tracking using VXD Nick Sinev, University of Oregon Plan Motivation Track reconstruction algorithm Performance for single tracks Does it have any limits ? With backgrounds To do Motivation Tracking in SiD is a challenge, especially pattern recognition. ... Limitations caused by reconstruction speed consideration In the presence of high number of background hits, number of 3-point combinations used as track seed became enormous if we consider all combinations. ...

... A Close Up or Martian Soil . ... Credit: Mars Exploration Rover Mission , JPL , NASA Explanation: Make your background the closest image of Mars yet. The Spirit Rover currently rolling on Mars has taken the highest resolution image to date of another planet. ... As more images come in and as the Spirit Rover continues to explore Mars, more information about the unusual floor of Gusev Crater are likely to emerge. ... Публикации с ключевыми словами: Mars - Spirit rover - Марс . ... Вид на Марс . ...

... Meta Index / Home Page / Description / Soft flare rejection for . The EPIC-pn fast timing mode was designed so that a time resolution of 0.029 milliseconds can be achieved. ... Below this energy the data is affected by so-called soft flares which are caused by stack overflows generated by high energy particles. These so-called soft flares have sharp rise (from 0 counts/sec to several thousand counts/sec in 0.10-0.15 sec) then decaying back 0 counts/sec slightly slower in about 0.3-0.4 sec). ...

... Classes . ... casa::MSValidIds . ... MSValidIds (const MeasurementSet &ms) . ... antenna1 ( uInt rownr) const . ... antenna2 ( uInt rownr) const . ... dataDescId ( uInt rownr) const . ... fieldId ( uInt rownr) const . ... observationId ( uInt rownr) const . ... processorId ( uInt rownr) const . ... stateId ( uInt rownr) const . ... polarizationId ( uInt rownr) const . The polarizationId comes from the DATA_DESCRIPTION subtable, so dataDescId must first be valid in order for this to also be valid. ...

... Both sets of objective transmission gratings consist of hundreds of co-aligned facets mounted to supporting structures on 4 annuli (one for each of the four co-aligned mirror pairs) to intercept the x rays exiting the HRMA. ... The two sets of transmission gratings, attached to the mounting structure are shown in Figure . ... An individual facet has 0.43-m-thick gold grating bars with 50% filling factor and 9920- period, resulting in 1.15-/mm dispersion. The HRC-S is the primary LETG readout. ...

... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...

OptInt PmWiki . ... The above top-level requirements are being flowed down to a set of derived requirements by means of brainstorming sessions and appropriate analysis/simulations. A matrix developed by CAH, MF and ADR attempts to identify all derived requirements and can be used to check if we have captured them all: [[Attach:derived-requirements matrix-v1.pdf | Derived Requirements Matrix]] . ... The derived requirements are being written up in the document: [[Attach:derived_merged.pdf | ...

Next: Acknowledgments Up: HST Image Restoration with Previous: Results . ... To the desirable characteristics of the FMAPE algorithm, this development adds the capability of different degrees of smoothing in different regions of the image. This implies a variation in resolution in the restoration, allowing high resolution in high S/N regions and lower resolution with lower artifacts in poor S/N regions . ...

The Library of Medium Resolution Spectra . HyperLeda home | Documentation | ... The library is divided into different archive corresponding to the different datasets. ... They are stored as tar files. ... cumulus . ... The archive will be divided in subdirectories in order to avoid problems with some unix commands which have a limitation in the size of the argument or number of files. ... The file name is the file number in this dataset The file naming convention has the form: LYYMMOBSj/nnnn . ...

... Using the DRAO Synthesis Telescope (Landecker et al. 2000), the Canadian Galactic Plane Survey ( CGPS ; Taylor et al. 2002) has captured a multitude of HISA features, the majority of which are invisible in prior surveys at lower resolution. ... Since the HISA gas temperature must be less than the background brightness temperature, all the H I shown in this poster has T ~ 100 K. Figure 1 provides panoramic views of the cold H I visible as HISA in the CGPS. ... GIFs: HISA + CO | HISA only | ...

... Like the Lynxx and the ST-4, this camera has a preferred orientation with the telescope (see figure 4). ... Before taking images, the camera and the telescope have to be calibrated. ... This is the normal CCD camera image mode. The second method is the track and accumulate mode. In this mode, the camera takes several short images, and then adds them together to give an image that is comparable to the same total time image as taken by the grab function. ...

TIRGO has three standard instruments, most of them developed and build in­house: ARNICA, a portable 256x256 NICMOS3 camera for wide field imaging and fast fotometry. ... Common fields of study at TIRGO are: Comets; Lunar occultations; Regions of star formation; Interstellar medium; Galaxy morphology; Galaxy nuclei; Forming galaxies; QSO and Seyfert galaxies. ...

... Contacts: Evgeny A. Loupian, Dr. Sci., e-mail: evgeny@smis.iki.rssi.ru Sergey A. Bartalev, Dr. Sci., e-mail: bartalev@smis.iki.rssi.ru Web interface for burnt area mapping using Landsat data Stellar Tracker In 2013 IKI RAN together with the NPK "Electrooptics" completed the phase of the five-year research on studying the ways to build a stellar inertial navigation system (SINS) for aviation applications. ... Fig. 1 shows the SINS layout created on the basis of the astronomical camera. ... Fig.1. ...

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2004 January 18 . A Close-Up of Martian Soil . Credit: Mars Exploration Rover Mission , JPL , NASA . Explanation: Make your background the closest image of Mars yet. The Spirit Rover currently rolling on Mars has taken the highest resolution image to date of another planet. ... About APOD | ... NASA Official: Jay Norris. ...

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

of the RadioAstron Teleconference 4 . ... The agenda of the teleconference and the list of participants are attached as an Appendix A to the Minutes. The main intents of the teleconference were to discuss the results of Pushchino tests, to develop actions in order to overcome the problem of aging of 6-cm and 18-cm receivers and to understand situation with NASA support for the project. ... Andreyanov informed the participants about the procedure and main results of Pushchino tests. ...

June 11-13, 2007 S.P.Korolev RSC Energia – MCC-M, . ... On June 10, 2007 the International Space Station (ISS) received another manned vehicle. In addition to Soyuz TMA-10 crew rescue vehicle attached to the station, the US Space Shuttle Atlantis mated to the ISS. ... The onboard crew conducted video imagery of the vehicle external surface. The crew commander Fyodor Yurchikhin (test-cosmonaut, S.P. Korolev RSC Energia) conducted photo imagery of several phases of this process. ...

... Spectrometer and CCD camera attached to the 2 metre "Karl-Zeiss-Jena" telescope of the Observatory on peak Terskol (3100 m, Northern Caucasus). ... The accessible spectral range is ~3500 - ~10200 AA. The CCD camera and the data handling system, developed at SAO, consist of front-illuminated CCD device of 1024x1024 pixels (pixel size 16x16 mkm) inside a dewar, an electronic controller-interface and a IBM PC computer. ... R=45 000 (~90 spectral orders, ~3500 - ~10200 AA registered simultaneously) . ...

... About ISSP . RAS members working in ISSP . ... A set of technological processes is developed in the Institute of Solid State Physics RAS for manufacturing of scintillation elements for radiation detectors with high space resolution. ... тАв€а a technology of direct forming of scintillation elements with necessary profiles and dimensions by means of external pressure in pressing tools with corresponding geometry. ... Scientific Secretary WWW: www.issp.ac.ru . ...

... AstroAsciiData is a Python module to handle ASCII tables. ... The idea to develop this Python module emerged from the fact that ASCII tables continue to be one of the most popular and widely used data exchange formats in astronomy and probably science in general. ... To load this ASCII table, go into Python, load the AstroAsciiData module and read in the table with: . ... demo = asciidata.open('webexa.txt') . ... Users who only want to work with ASCII tables neeed no further python modules. ...