... SPICE System Documentation . Comprehensive set of SPICE System documentation including tutorials, subroutines and data formats descriptions, etc. Other related home pages: . Navigation and Ancillary Information Facility at JPL . MARS-96 Space Mission . ... Please, forward comments and questions about information on this page and all descending NAIF and M96 SPICE implementation pages to NAIF group at IKI . naif@arc.iki.rssi.ru . ...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . Australia Telescope Compact Array . ... CSIRO, Australia's national science agency, operates a number of world-class radio astronomy observatories that are collectively known as the Australia Telescope National Facility or ATNF. ... CSIRO also manages the Murchison Radio-astronomy Observatory, where the Square Kilometre Array telescope infrastructure in Australia is to be centred. ...

... Partly based on observations performed with radio telescopes of IAA RAS (Federal State Budget Scientific Organization Institue of Applied Astronomy of Russian Academy of Sciences). c . ... Partly based on observations with the 100-m telescope of the MPIfR (Max-Planck-Institute for Radio Astronomy) at Effelsberg . ... NRAO facilities . The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. ...

... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...

... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How do I combine the individual 3-D cubes into a final mosaic? ... Observing Facilities . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... If the individual cubes come from a single offset sequence, the easiest is to use the ESO.SEQ.CUMOFFSETX/Y keywords in the...

Form W-8BEN (Rev. December 2000) Department of the Treasury Internal Revenue Service Cer tificate of Foreign Status of Beneficial Owner for United States Tax Withholding Section references are to the Internal Revenue Code. See separate instructions. ... The beneficial owner is not an individual, is claiming treaty benefits for dividends received from a foreign corporation or interest from a U.S. trade or business of a foreign corporation, and meets qualified resident status (see instructions). ...

... Site Fire . ... Medical . ... If an emergency occurs, contact the Site Operations Manager or any staff member; they know the area and services available to APO. ... APO fire protection has individual panels in each building that have a local alarm and are also monitored by an outside alarm monitoring company. ... Fire response is provided by the Sunspot Volunteer Fire Department (SVFD) through the Otero County Sheriff s Office Dispatch Center. 911 is the Emergency phone number for all emergencies. ...

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

. Chairs . Teachers . Postgraduate Students . Undergraduate Students . Courses . Head: A.M.Cherepaschuk . Vice-Head: A.C.Rastorguev . Webmaster: Yuri V. Pakhomov . pakhomov@sai.msu.su

... How much energy is there in a 20 mph wind? . 20 mph wind =10 m/s .0006 * 10 3 = .0006 * 1000 = .6 KILO watts per square meter . ... In your back yard the average wind speed is 10 mph which yields 100 watts per square meter. ... 4 3 = 64 if a 10 mph wind gives you 100 watts per square meter then a 40 mph wind gives you 64 times more power per square meter 6400 watts per square meter . total power = 6400 watts per square meter * 2 square meters = 12800 watts = 12.8 Kilowatts this is a lot! ...

... What this work needs is a good space telescope to get high resolution images of these galaxies, and some really big ground-based telescopes equipped with low resolution, multi-object spectrographs, to measure their redshifts. ... Rumor has it that some low individuals, jealous at your great success, are claiming that you have missed most of the galaxies in the early universe: that these galaxies are too red or too dusty for the Ly-limit technique to detect. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . ... Flights Chronology . ... ISS Russian Segment . ... History of flights . ... Investigation of human neuroendocrine and immune responses in and after a space flight aboard the ISS. ... Making measurements of the radiation dose as a result of the ionizing space radiation onboard the ISS Russian Segment using the "Pille-ISS" flight dosimeter. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

... Samara State Aerospace University Research Grants and support . Project Designing a range of gas-turbine engines on the basis of a high energy efficiency gas generator in cooperation with Kuznetsov plc within the framework of implementing the Russian Federation Government Order of 09.04.2010 No.218 Measures of state support of the development of cooperation between higher educational institutions and organizations implementing complex projects on high-technology production design . ...

... Armagh Observatory astronomers report the publication of the first stunning celestial images obtained with the 11-metre multi-national Southern African Large Telescope (SALT) . ... Exactly five years after groundbreaking, the SALT project has released its first colour images, marking the achievement of 'first light' and the successful debut of full operation for SALTICAM, a $600,000 digital camera designed and built for SALT at the South African Astronomical Observatory (SAAO) . ...

... Annual Meeting . Past Meetings . ... Four individual complimentary national conference registrations . ... Prominent logo on ASP website conference page . Prominent logo in annual national conference program book . Complimentary full page ad in annual national conference program book . Prominent logo on signage at annual national conference . ... Complimentary half page ad in annual national conference program book . Prominent logo on signage at the annual national conference . ...

Optico-physical department is one of the oldest scientific teams of the Space Research Institute of the Russian Academy of Sciences. The Department's main activity is space research of the Earth and other Solar System's bodies in the visible and near-IR bands. ... The new generation star tracker BOKZ-MF with a built-in gyro as well as the TV system for navigation and observations (TSNN) have been developed for the "Phobos-Grunt" mission planned for 2011. New! ...

Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...

. Other related sites: . Back to Space and Atmospheric Science Department Homepage . Last updated on: March 7, 2003

... The useable imaging area of the OM CCD detector is 256 by 256 physical (detector) pixels. Individual photon events are centroided to one eighth of a physical CCD detector pixel by the OM electronics. The resulting OM imaging area is therefore 2048 by 2048 pixels. However, the centroiding algorithm distributes the photons unevenly within each physical CCD pixel, corresponding to 8 by 8 unbinned image pixels or a single mod-8 tile, as though the pixels are smaller near the edge of the tile. ...

... Finally, the individual observations themselves are reduced, using the parameters from the extinction solution. ... That is, the extinction solution can in principle produce results if we observe extinction star 1 only in passband A and star 2 in passband B on night 1, and star 1 only in passband B and star 2 in passband A on night 2. ... Even if the passbands are linked by color terms in the extinction, the solution is possible, because we do obtain mean colors for each star. ...