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1. Tracking history files (PDF and ps)
XMM-Newton Science Analysis System . ... Meta Index / Home Page / PPS Product Files Omdrifthist produces a PDF plot file, which displays information about the satellite tracking during the exposure. This PDF file is converted into a ps file. Tracking-history PDF plot file produced by omdrifthist, eg- P0123920101OMS006TSHPLT000.PDF . Tracking-history PS plot file produced from the PDF plot file, eg- P0123920101OMS006TSHPLT000.ps . XMM-Newton SOC/SSC -- 2008-07-02 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omichain/node17.html -- 3.6 Кб -- 02.07.2008
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2. Real Time Science Displays for the Proportional Counter Array Experiment on the
... Up: Real-Time Systems . ... The Rossi X-ray Timing Explorer ( RXTE ) spacecraft contains a large Proportional Counter Array (PCA) experiment which produces high count rates for many X-ray sources. ... This allows opportunity for some serious real time interpretation and decision making by the experiment controller, duty scientist, and Guest Observer (GO), if present. ... This paper briefly describes the available Science Monitoring subsystem display options. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/gilesa.html -- 11.4 Кб -- 23.06.1998
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3. Funtools and DS9 Image Display
Describes how funtools can be integrated into the ds9 Analysis menu. SAOImage/DS9 is an astronomical imaging and data visualization application used by astronomers around the world. DS9 can display standard astronomical FITS images and binary tables, but also has support for displaying raw array files, shared memory files, and data files automatically retrieved via FTP and HTTP. ... It can be manually loaded into DS9 from the Load Analysis Commands ... option of the Analysis menu. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/RD/funtools/ds9.html -- 5.2 Кб -- 01.10.2012
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4. Chapter 3: STSDAS Basics
... 3.2 Displaying HST Images . ... 3.3 Analyzing HST Images . ... 3.4 Displaying HST Spectra . ... This chapter introduces the basics of STSDAS, showing you how to display your data, leading you through some simple data manipulations, and pointing you towards more sophisticated tasks, some of which are described in the instrument data handbooks. STSDAS is layered on top of the Image Reduction and Analysis Facility (IRAF) software developed at the National Optical Astronomy Observatory (NOAO). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_dhb/intro_ch3.html -- 9.1 Кб -- 20.02.2002
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5. PPEUC Programme - Cosmic Microwave Background Workshop
... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/ppeuc/proceedings/cmb_prog.html -- 9.9 Кб -- 24.02.1998
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6. Miscellaneous Analysis Tasks
Next: Displaying Spectral Cubes Up: Image Analysis Previous: Polarimetric Analysis Tasks . The task imdiff can be used to compare two images. ... You can use the self-explanatory task shifty for large integral pixel shifts. ... It may be that you would like the image to be written out with histogram equalisation applied, rather than it just being computed but not saved by the display task. ... Next: Displaying Spectral Cubes Up: Image Analysis Previous: Polarimetric Analysis Tasks Miriad manager . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node161.html -- 11.8 Кб -- 10.04.2016
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7. Predicting a Fine Display of Leonid Meteors
PREDICTING A FINE DISPLAY OF LEONID METEORS . Armagh Observatory, 8 November 1999: . According to calculations by Armagh Observatory astronomer Dr David Asher, the Leonid meteor shower is expected to reach a peak during the early hours of 18th November, with a rate of more than 1000 shooting stars per hour for up to an hour or two either side of 02:00 am. These meteors are produced by dust grains given off by comet Tempel-Tuttle as it orbits the Sun once every 33 years. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/Leonids-99.html -- 3.6 Кб -- 09.11.1999