... 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...

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• Main research and development work completed in 2012 and ready for

HUBBLE SPACE TELESCOPE DAILY REPORT #982 PERIOD COVERED: 0800 EST Daily Status Report as of 272/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed GHRS/2 3859 (Nighttime Measurements of Nitric Oxide - Continuation of 2544) The High Resolution Spectrograph was used to make observations of the bright B class star HD037128. ... 3.0 ACTIVITIES SCHEDULED FOR NEXT REPORTING PERIOD: 3.1 Complete Four Sets of WFC 5075 (WF/PC Cycle 3 Calibration: (WFC Flats Wide. ...

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• http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_03_28_94
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_01_22_93
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_01_26_94

The process of determining the number and characteristics of sources in astronomical images is so fundamental to a large range of astronomical problems that it is perhaps surprising that no standard procedure has ever been defined that has well understood properties with a high degree of statistical rigour on completeness and reliability. ... In this analysis we present results from testing such algorithms as implemented in the SExtractor, Selavy (Duchamp), and sfind tools on simulated data. ...

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• Molecular gas
• PPTA Dashboard | Projects
• Australia Telescope National Facility

OptInt PmWiki . ... Tech Meet 2 . ... Page History | ... PmWiki . ... Return to Tech Meet 2 ( Edit ) . ... 1 pixel independent of pixel scale (avoids aliasing of high frequencies in speckled image) . ... ADR & CAH: Optical image quality tolerancing of OAP-based layout . ... ADR & CAH: Layout and tolerancing of lens-based optical system . ... ADR & CAH: Use tolerancing results to assign image quality and stability budgets by component . ... ADR & CAH: Think about how to apportion image quality budget . ...

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• OptInt PmWiki : Tech Meet 2
• OptInt PmWiki : Tech Meet 4 | History
• OptInt PmWiki : Tech Meet 4

... The ROSAT Consortium (the Max-Planck-Institut fuer extraterrestrische Physik, the Goddard Space Flight Center, the Smithsonian Astrophysical Observatory, Leicester University, and the Astrophysikalisches Institut Potsdam) announces the release of the completed source catalogs of all ROSAT pointed observations. ... Detailed information about the catalog and methods of access to the catalog and data products can be obtained from the ROSAT Results Archive web pages in Germany, in the US, and in the UK:...

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• SAO RSDC Home Page - RRA - PSPC
• The AstroStat Slog incompleteness
• The AstroStat Slog light curve

To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...

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... Science . ... Science Users Information > Science Publications > Science Announcements > Stellar End Products: The Low Mass - High Mass Connection . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... ESO Data Access Policy . ... The aim of the meeting is to bring together observers and theorists from the low and high mass stellar communities with the goals of exploring the commonalities of evolved star mass loss. ...

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• ESO - Science Announcements
• ESO - 8th VLTI Summer School: High angular resolution in astrophysics: optical
• ESO - Circumstellar Dynamics at High Resolution

. Note: This material is from a 1994(!) Talk about CCDs - the physics remains the same, only the detector size has increased since then. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• U of O High Energy Physics Seminars
• Astronomy HyperText Book: Fusion Sequences in Stars
• University of Oregon Center for High Energy Physics - Group Talks, Papers, and

Next: Mission Operations Data Transfer . ... VLBI Tape Management . VLBI Tapes . ... When: As soon as the correlator is satisfied with the correlator output. back to top . ... What: Each correlator will maintain a data base including the status of all VLBI tapes under its control. ... The correlators will distribute tapes to mission elements based on the Observation Summary File produced by the RSOG ( Observation Summary File ) to ensure each element has enough tapes to support SVLBI observations. ...

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• MEMORANDUM

... AGES Precursor Observations · Targeted the M74 ( NGC 628) group · Noise falls as t (to 200s) AGES Precursor Observations · Targeted the M74 ( NGC 628) group · Noise falls as t (to 200s) AGES Precursor Observations · Targeted the M74 ( NGC 628) group · Noise falls as t (to 200s) · Detected 5 galaxies in the group KDG 010 dw0137+1540 UGC 1171 AGES Precursor ...

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• http://www.naic.edu/vscience/schedule/tpfiles/KovalevtagV3003tp.pdf
• GALFA - H I Projects
• AGES - the Arecibo Galaxy Environment Survey

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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... The distinguishing characteristic of VIMOS is its very high multiplex capability: in MOS mode up to 800 spectra can be acquired simultaneously, while the Integral Field Unit produces 6400 spectra to obtain integral field spectroscopy of an area approximately 1 1 arcmin in size. ... Figure 1: A block diagram scheme of the DRS spectral extraction process . ... The extraction itself is carried out following two different procedures for MOS and IFU observations. ...

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• The PROS Big Picture: A High-Level Representation of a Software System
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... 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 ...

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• Hardware sector, archive 2001
• Hardware sector, archive 1997
• Metagalaxy scientific results 2003

... NASA Astronaut (former) . ... Graduated from East Detroit High School, Eastpointe, Michigan, in 1973; received a bachelor of science degree in bioscience from the U.S . Naval Academy in 1977; a doctorate in medicine from Wayne State University in 1981; a master of science degree in systems management from University of Southern California in 1988; a master of public health degree in health policy from the ... Top graduate, Naval Flight Surgeon Training and Naval Safety Officer's School. ...

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• Astronaut Bio: Eugene A. Cernan
• Astronaut Bio: Stephen G. Bowen (2/2013)
• Astronaut Bio: Steven L. Smith (12/2013)

Solar High Resolution Studies . ... Solar Group . ... High Resolution Studies . Small Scale Activity . ... High resolution observations at different heights in the solar atmosphere have emphasized that there is no such thing as a "quiet" Sun (e.g. Schrijver et al., ... This, and the temporal coincidence of other signatures, supports the idea that microflares are indeed just miniature flares, but that one needs a very high resolution in order to observe them (Cauzzi et al., 2003, in preparation) . ...

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• High-resolution Herschel spectroscopy reveals the proto-planetary disk around
• A local window on galaxy formation with ALMA
• Observing capabilities

Next: J.E. Chambers, Research Astronomer Up: Research Previous: Research Contents . ... Solar Variability and Climate . Other Activities . ... Applied to data of flares on Gliese866 he was able to estimate the area of hydrogen emitting flare regions as 1-13% of the stellar surface. ... As partners in the project, Armagh Observatory has been asked to contribute to the selection process in exchange for priority access to the data which will eventually flow from the satellite. ...

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• Doppler Imaging and Flare Activity on HR1099
• ULTRACAM Observations of Subdwarf B Stars
• Armagh Observatory

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? ...

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... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2000 November 25 . A High Energy Fleet . Courtesy: MSFC Historical Archive , NASA . Explanation: Like a fleet of futuristic starcruisers, NASA's highly successful series of High Energy Astrophysical Observatory (HEAO) spacecraft appear poised over planet Earth. ... Archive | ... About APOD | ... NASA Technical Rep.: ...

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• APOD: May 25, 1997 - A High Energy Fleet
• APOD: May 24, 1998 - A High Energy Fleet
• APOD: 2005 October 5 - An Annular Solar Eclipse at High Resolution

... In this activity, students will observe that the faintest stars which they can see in the sky are affected by many things: the adaptation of their eyes to the dark, the presence of clouds or haze, the time of year, and the presence of light pollution. General Information . ... After completing this activity, students should have a better understanding of the practical processes for dealing with the light pollution problem and with other environmental and societal issues. << previous page | ...

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• ASP: Contents, Spring 2010
• ASP: Using Multicultural Dimensions to Teach Astronomy
• ASP: Astronomy Behind the Headlines