... The distributed control software for the prototype delay line consists of the following components: . Delay Line Software Libraries [DFB, JSY] . ... Trolley Software [EBS] . ... The above components communciate with each other using the protocol defined in Network Message Protocols and Log File Format . The prototype software should conform to the agreed Coding Standards . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIDelayLine/DelayLinePrototypeSoftware) ...
... The FITS conversion commands INTAPE and OUTTAPE can both access FITS files on disk or directly on tape devices. Thus, it is in principle possible to use general system utilities to transfer the FITS files between disk and tape. ... In order to save disk space, it may be desirable to compress the files. ... Use OUTTAPE to write file to disk in FITS format. Compress FITS file on disk e.g. compress . Use system utility to save compressed file on tape e.g. tar . ... File naming . ...
... This page is being developed by D.Semenov within the project "Optics and dynamics of cometary dust" supported by the "Universities of Russia - Fundamental Researches" research grant program of the Russian federal goverment. books . ... Polarimetry & Photometry of comet C/1996 B2 Hyakutake , by N.N.Kisilev, Icarus , 133 , 286-292, 1998. ... Narrowband Photometry of comet P/Halley: Variations with Hel. distance, season, and solar phase angle , by David G.Schleicher, Icarus , 132 , 397-417, 1998. ...
Welcome from the Staff ARC 3.5-m Telescope Sloan Foundation 2.5-m Telescope Astrophysical Research Consortium New Mexico State University 1.0-m Telescope ARC Small Aperture 0.5-m Telescope Celebration 400th Anniversary of the Telescope http://www.eso.org/public/events/iya2009/ The Apache Point Observatory is privately owned and supported by the Astrophysical Research Consortium, whose mission is to operate the ... NMSU operates the observatory site for the Consortium. ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/ARCprogress/041009OHphotos/Program.pdf -- 449.9 Кб -- 07.05.2009 Похожие документы
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SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 2 / number of data axes NAXIS1 = 1138 / length of data axis 1 NAXIS2 = 1114 / length of data axis 2 TELESCOP= 'UT1 ' PI-COI = 'C. Cesarsky' / Name of PI and COI ORIGIN = 'ESO/EIS ' / Data processed by RA = 53.0917713808546 / RA (J2000) at start (deg). ... RADECSYS= 'FK5 ' / Coordinate reference frame. ... TOT-IMAG= 125 / Total number of images. ... MOSTILES= 21 / Total number of tiles in MOSAICID. ...
Truebloodb,g, K. Zelayab Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43221 USA; bNational Optical Astronomy Observatory, 950 North Cherry Street, Tucson AZ 85719 USA; cCerro Tololo Inter-American Observatory, Casilla 603, La Serena ... USA ABSTRACT We describe the design, construction and measured performance of the Kitt Peak Ohio State Multi-Object Spectrograph ( KOSMOS ) for the 4-m Mayall ... Optical layout for KOSMOS and COSMOS. ...
... Среди этих проблем: расширение существующей опорной системы ICRF на слабые звезды, исследование инерциальности системы ICRF, проблема связи радио и оптической систем координат, уточнение теорий движения тел Солнечной системы, исследование динамики двойных и кратных звезд. ... Наша лаборатория единственная в России и одна из немногих в мире, которая имеет столь длительные ряды наблюдений ( 30-40 лет) различных объектов Солнечной системы. ... Обновлена и расширена программа наблюдений двойных звезд. ...
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Instructions for Uploading Images and Video Related to the Columbia Accident . For anyone who has recorded video or taken photos that they believe may be of aid in the investigation of the Space Shuttle Columbia accident, NASA has established a special location on the Web where Internet users may upload their media files to be reviewed by NASA. ... Image file: johndoe_020203_0415pm.jpg . ... If you have any problems uploading your files, please e-mail Mike Koester . ...
Dynamic Shack-Hartmann System RAPID V. G. Orlov, V. V. Voitsekhovich Instituto de AstronomМa, UNAM, MИxico CONACYT project E9507-1020P UNAM PAPIIT IN104910 Telescopes OAN OAN- SPM 2.1m telescope 1.5m telescope 0.84m telescope 2.1m telescope OAN-Tonanzintla 1m telescope Astronomical site SPM Observing statistics 1982-2002 (Tapia+ 2007 ) Photometric nights : 64.1% Spectroscopic ... Rapid - Dynamic Shack-Hartmann All modern telescopes demand installation of adaptive system. ...
... India (2011) 00, 111 Evidences of the central engine activity in the Naked-Eye Burst prompt optical emission S. Karpov1 , G. Beskin1 , S. Bondar2 , A. Guarnieri3 , C. Bartolini3 , G. Greco4 and A. Piccioni 1 2 3 4 3 Special Astropysical Observatory, Nizhnij Arkhyz, Russia, 369167 Institute for Precise Instrumentation, Nizhnij Arkhyz, Russia, 369167 Astronomy Department of Bologna University, Bologna, Italy Astronomical Observatory of Bologna, INAF, Italy Received 17th February 2012 Abstract. ...
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This module supports ISAPI Extensions within Apache for Windows. ... This module implements the Internet Server extension API. It allows Internet Server extensions ( e.g. ISAPI .dll modules) to be served by Apache for Windows, subject to the noted restrictions. ISAPI extension modules (.dll files) are written by third parties. ... Review the Additional Notes and the Programmer's Journal for additional details and clarification of the specific ISAPI support offered by mod_isapi. ...
Synthesis and Transmission of Cosmic Call 2003 . Interstellar Radio Message . Foreword: On July 6, 2003, an international science team, led by Dr. Alexander Zaitsev of the Russian Academy of Sciences and Richard Braastad of Team Encounter, LLC, broadcast scientific and personal messages in “Cosmic Call 2003” to five, sun-like stars. ... In conclusion, we would like to express our sincere gratitude to everyone who helped to create and send the Cosmic Call 2003 interstellar radio message. ...
Surveys in Geophysics (2005) 26: 95133 DOI 10.1007/s10712-005-1874-4 с Springer 2005 MAGNETOSHEATH INTERACTION WITH THE HIGH LATITUDE MAGNETOPAUSE S. SAVIN1, A. SKALSKY1, L. ZELENYI1, L. AVANOV1, N. BORODKOVA1, S. KLIMOV1, V. LUTSENKO1, E. PANOV1, S. ROMANOV1, V. SMIRNOV1, YU. YERMOLAEV1, P. SONG2, E. AMATA3, G. CONSOLINI3, T. A. FRITZ4, J. BUECHNER5, B. NIKUTOWSKI5, J. BLECKI6, C. FARRUGIA7, N. MAYNARD8, J. PICKETT9, J. A. SAUVAUD10, J. L. RAUCH11, J. G. TROTIGNON11, Y. KHOTYAINTSEV12 and K. STASIEWICZ12