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http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt.pdf.

1. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Кб -- 15.12.2015
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2. ISIS: An Interactive Spectral Interpretation System for High Resolution X-Ray
... The Interactive Spectral Interpretation System (ISIS) is designed to facilitate the interpretation and analysis of high resolution X-ray spectra like those obtained using the grating spectrographs on Chandra and XMM and the microcalorimeter on Astro-E. It is being developed as an interactive tool for studying the physics of X-ray spectrum formation, supporting measurement and identification of spectral features, and interaction with a database of atomic structure parameters and plasma emission...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P2-39/ -- 13.2 Кб -- 11.10.2000
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3. http://www.stsci.edu/ftp/instrument_news/FOS/pub/fos_isr101.ps
... Straylight V 15 = Observations of HD144858 An example of the excess flux due to straylight can be seen in figure 1a,b where the observation of 16 CYG B are compared to a reference spectrum of a G2V star. The extra flux detected by the diode array is readily apparent. ... Predicting the Amount of Straylight Spectra from the BPGS spectra library were used as the data to construct the graphs of the amount of straylight as a function of spectral type. ...
[ Текст ]  Ссылки http://www.stsci.edu/ftp/instrument_news/FOS/pub/fos_isr101.ps -- 53.6 Кб -- 26.10.1994
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4. AGES Database Search
... All the parameters provided in this database have been obtained using the the MIRIAD ( Sault et al. 1995 ) task MBSPECT . MBSPECT makes a spectrum of the velocity (or frequency) axis of a cube. The spectrum is beam-weighted, over the width specified, for the other image axes. ... Robust parameters are calculated by using an algorithm which minimises the mean absolute deviation of the flux-weighted velocities. mask= This specifies the x-axis ranges to be excluded from any continuum fit. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~ages/public/glossary.shtml -- 10.0 Кб -- 10.04.2016
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5. Pulkovo Database of Observations of Planets and Their Satellites
Pulkovo Database of Observations of Planets and Their Satellites . Select object, time interval and type of observations . ... First year (optional) . Last year (optional) . ... satellite relative to planet . satellite relative to another satellite . ... Select database . ...
[ Сохраненная копия ]  Ссылки http://www.puldb.ru/db/sdb.php -- 7.1 Кб -- 09.04.2016
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6. Main research and development work completed in 2009 and ready for
... Space Research Institute . ... Main research and development work completed in 2009 and ready for implementation . ... Development of the Northern Eurasia land cover map based on medium spatial resolution satellite data. ... The research and development has been completed of the first in Russia and in the whole world high-speed digital streams decoder for space and satellite channels with extremely high noise levels. ... Main research and development work completed in 2008 and ready for...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/eng/niokr2009.htm -- 7.7 Кб -- 18.07.2011
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/eng/niokr2009.htm -- 7.7 Кб -- 18.07.2011
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7. Data bases of Natural Satellites. Documentation. Structure
Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/DocStructe.htm -- 11.4 Кб -- 18.05.2009
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8. ChaMPlane data_archive_.html
... Fields Observed . ... Data Archive . ... Complete Optical and X-ray data for all ChaMPlane fields are available through the DS9 VO interface . ... functionality of DS9 is available to manipulate the results in addition to those provided by the "Champlane tools" You can select images, compare . ... our region of interest has been selected by drawing a red square region on the image. at bottom left the high res optical image of that selected region, and on the right is the X-ray image. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChaMPlane/virtual_obs.html -- 10.9 Кб -- 01.10.2012
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9. http://xmm.vilspa.esa.es/sas/6.5.0/doc/esrcselect.ps.gz
... The task accepts two sources lists: the observation source list and the exposure source list. ... List of selected sources. This le contains a table, called SRCLIST, with the following columns: Name Type Description SRC NUM Integer Source ID from observation source list RA Double RA from exposure source list DEC Double Declination from expoure source list RATE Real Count rate from observation source list COUNTS Real Number of source counts, from exposure source ...