... LUMAM . ... ABOUT LOMO . ... Home Products Microscopes Lumam RPO-11T . ... High-performance plan achromats specially designed for fluorescence observations: 20 x 0.45, 40 x 0.65 (spring-loaded), 40 x 0.65 NCG (spring-loaded), 40 x 0.65 NCG Phase (spring-loaded), . ... LOMO America, Inc. will repair or replace the defective microscope covered by this warranty free of charge if it is returned, postage prepaid, to LOMO America’s Service Center in Prospect Heights, Illinois in its original package. ...

... Tonight's Sky . ... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . ... Moon . ... The Magazine . ... Observing . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... In the exact center . ... Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

... The DiFX correlator has a capability to process many phase centers within a primary beam in one pass. ... SCHED supports the multiple phase center mode by providing the details of all the desired phase centers to use for a given pointing center in the output .v2d file, which is used in correlator setup. ... When using this capability, the user should specify the size of the FFTs to do on each baseband channel before spliting the data for each phase center. ...

Testing Mount Stability Alex Rea adr34@cam.ac.uk Cavendish Lab oratory, University of Cambridge FTT Brainstorm Meeting Monday 16th May 2011 Alex Rea (Cavendish Labs, Cambridge) Testing Mount Stability 16th May 2011 1 / 21 Goal Alex Rea (Cavendish Labs, Cambridge) Testing Mount Stability 16th May 2011 2 / 21 Goal Want to discover if the mounts designed meet the stringent stability requirement that we have placed on them. ... The tests for these two cases will almost certainly be different. ...

Next: NICMOS/HST H-band (F160W) Images Up: NICMOS Science Previous: HST NICMOS Observations of . ... Observations of P . ... The NICMOS team has devised a comprehensive program of observations of the Galactic Center. ... Data in hand give a first look at variability and a detailed look at the search for the tip of the main sequence will be discussed where NICMOS has demonstrated adequate sensitivity and photometric precision to identify likely O8-B1 stars at the Galactic Center. ...

. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .

Procedure to Remove or Mount Plate in Cartridge . ... Data cartridge ; Location : stored on racks inside elevator bay, plugging station, or mapping station; Appearance : approx 4.5' dia X 3' thick., fiber optic wire interior, plate top, protected sides, top, and bottom; nine total; 320 lbs. each. ... Small hand tools ; Location : free-standing red tool boxes; Appearance : as described in procedure. ... Using a red colored "T" handle wrench, tighten a bolt until it is flush with the ring upper surface. ...

... This is usually defined as the direction pointing toward the center of the primary body. ... NODE: The place where the plane of one orbit crosses the plane of another. ... ORBITAL PLANE: The flat surface that would result if every point on the orbit of a body was connected to the center of its primary. ... PENUMBRA: The edge of the primary body's shadow. ... PERIOD : The time required for one body to orbit the primary body. ... PROBE: A vessel designed to pass and observe an astronomical object. ...

... Bauman Moscow State Technical University Edu . Branch of Shemyakin' 'Ovchinnikov Institution of Bioorganic Chemistry PU . Budker Institute of Nuclear Physics Novosibirsk . ... Favorsky Irkutsk Institute of Chemistry of SB RAS Irkutsk . ... General Physics Institute RAS . Geological Institute RAS . ... The Physics Department of Moscow State University . The Department of Chemistry, Moscow State University . ... List of Universities/Academies/Institutes and Search for graduated people . ...

... Р?С?С?С?Р?Р?Р?Р?РеС?Р?С?Р?РеР? ... Launched on February 17, 1996, the Near Earth Asteroid Rendezvous (NEAR) mission is to be the first of NASA's Discovery missions, a series of small-scale spacecraft designed to proceed from development to flight in under three years for a cost of less than $150 million. ... The ultimate goal of the mission is to rendezvous with and achieve orbit around the near Earth asteroid 433 Eros in February, 1999, and study the asteroid for approximately one year. ...