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... 77, 1995 R. A. Shaw, H. E. Payne, and J. J. E. Hayes, eds. QPSIM: An IRAF/PROS Tool for Source Simulation K. R. Manning, J. DePonte, and F. Primini Smithsonian Astrophysical Observatory, 60 Garden St., Cambridge, MA 02138 Abstract. ... Qpsim is an IRAF/PROS task which will gen erate events from sources of given intensity, shape, and position and ei ther overlay them on a flat background in a new QPOE file or inject them into an existing QPOE file. ...
... During these years, the Mercury, Apollo and Gemini programs ran concurrently while the MSC was being designed and built. ... Gemini Project Office. ... Program Analysis and Evaluation Chief Thomas W. Briggs Mercury Project Office Manager K. S. Kleinknecht Gemini Project Office Manager James A. Chamberlin Apollo Project Office Manager Charles W. Frick Systems Engineering Office Office of Manned Space Flight Asst Director Richard J. Hayes Langley Research ...
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Ссылки http://www.jsc.nasa.gov/history/suddenly_tomorrow/chapters/Chpt4.pdf -- 413.7 Кб -- 10.11.2004 Похожие документы
... 13, Moscow 119991, Russia §UK Astronomy Data Centre, Guest Investigator (Received 20 June 2007) The kinematics, structure, and stellar population properties in the centres of two brightest early-type galaxies of the Leo II group, NGC 3607 and NGC 3608, are studied by means of integral-field spectroscopy. ... Figure 1. ... Chemically decoupled cores in NGC 3607 and NGC 3608 3.1 NGC 3607 Figure 3 presents index maps for the central part of NGC 3607 constructed from the MPFS 2D spectral data. ...
Mon. Not. R. Astron. Soc. 349, 13971418 (2004) doi:10.1111/j.1365-2966.2004.07619.x The 2dF QSO Redshift Survey XII. The spectroscopic catalogue and luminosity function S. M. Croom,1 R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 L. Miller,4 P. J. Outram3 and N. S. Loaring4,5 1 2 3 4 5 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of