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... build and test receivers up to 40 - 350 GHz . ... Banham R., Valsecchi G., Lucci L., Pelosi G., Selleri S., Natale V., Nesti R., Tofani G. 2005, Microwave Journal 48, 112 Electroformed front-end at 100 GHz for Radioastronomical applications . Comoretto, G., D'Ambrosi, A., Nesti, R., Russo, A., Palagi, P. 2006, Arcetri Technical Report n. 4 A modular multichannel spectrometer - design study . ... Cresci, L., Lucci, L., Orfei A., Natale, V., Nesti, R., Panella, D., Pelosi, G., Rossi, L. 2006, Mem. ...

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The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

... Alien Life . ... During a mission planned to last a Martian year (nearly two of our years) after landing , Curiosity will use its instruments to investigate whether this area of Mars has ever enjoyed conditions suitable for life , especially the presence of liquid water.Lower layers of Aeolis Mons could reveal there was once a lake within Gale Crater long ago.But this is just the beginning of what ... Methane Not Detected by Curiosity Rover Does Not Rule Out Life on Mars . ... Astronotes...

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... 145, 1998 R. Albrecht, R. N. Hook and H. A. Bushouse, eds. Using Java for Astronomy: The Virtual Radio Interferometer Example N.P.F. McKay1 and D.J. McKay 1 Nuffield Radio Astronomy Laboratories, University of Manchester, Jodrel l Bank, Macclesfield, Cheshire SK11 9DL, UK Abstract. ... The use of the Java language is discussed, and the role of the language, within the astronomical software context, reviewed. ... The resulting program was called the Virtual Radio Interferometer2 (VRI). ...

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Find Similar Abstracts . ... 26, Jan. 1983, p. 77-83. ... CAUSTICS (OPTICS), COSMOLOGY, PARTICLE MOTION, GEOMETRICAL OPTICS, GRAVITATIONAL EFFECTS, UNIVERSE . ... The analogy between caustics in geometrical optics and the singularities that arise in irrotational flows in a cold collisionless medium is discussed. ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

... Новости астрономии и космонавтики (Модераторы: Karen , recarrion , LeMay ) ? Mars Science Laboratory - марсоход 'Curiosity' . ... Ответ #480 : 05.08.2012 [20:19:06] ? ... Ответ #481 : 05.08.2012 [20:26:36] ? ... Ответ #482 : 05.08.2012 [20:32:38] ? ... Ответ #483 : 05.08.2012 [20:46:36] ? Цитата: HansSibert от 05.08.2012 [20:10:11] А теперь раскажите поподробнее руководствуясь чем, был сделан такой вывод? ... Ответ #484 : 05.08.2012 [20:56:05] ? ... Ответ #485 : 05.08.2012 [20:57:28] ? ...

February 10, 2003 (Monday) Igor Tyukhov, Oregon Solar Radiation Monitoring Laboratory . February 17, 2003 (Monday) Osamu Yasuda, Tokyo Metropolitan University . February 20, 2003 (Thursday) Linear Collider Seminar . ... Fall 2002 . Fall 2001 . ... Fall 2000 . ... 3:00 pm, 472 Willamette Hall . ... The American Linear Collider Physics Group (ALCPG) has initiated a series of monthly seminars intended for a broad audience. ... This is the inaugural seminar. 1:00 pm, 472 Willamette Hall . ...

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... Using Java for Astronomy: The Virtual Radio Interferometer Example N.P.F. McKay 1 and D.J. McKay 1 Nu#eld Radio Astronomy Laboratories, University of Manchester, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, UK Abstract. ... The resulting program was called the Virtual Radio Interferometer 2 (VRI). ... Software development metrics for VRI Java Development Kit Version 1.0.2 Software classes 26 Java instructions 1565 Development time 80 hours Size of byte code 1.3 Mbyte 5. ...

... The zero point was derived in the following way: ffl Matching the OM repsonse using the measurements of BPM16274 and LBB227. ffl the zeropoints in U, B, V are set in a way that the simulations with the Vega spectrum (from ESO ftp server) matches the average brightness found in the literature which is (0.025, 0.03, 0.03) mag respectively. ffl In the UV filters the ESO Vega brightness is arbitrarily set to the U value, i.e. 0.025 mag ... The analysis comprised of the following steps: 1. ...