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http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/PN_spectrum_thread.html.

1. How to extract MOS spectra of a point-like source and associated matrices
... This thread contains a step-by-step recipe to extract MOS spectra of a point-like source observed in Imaging mode and to create associated response matrices, starting from a calibrated, concatenated event list (either produced with emproc or available as PPS product; here it has the assumed file name MOS.fits ). ... The users should note that the SAS metatask xmmselect allows them to interactively define source and background regions (via ds9) and to run backscale on the fly. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/MOS_spectrum_thread.html -- 11.6 Кб -- 15.06.2007
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2. http://hea-www.harvard.edu/AstroStat/astro193/ChristopherMerchantz_ay193_fp_slides.pdf
Testing the Automatic Detection of Directly Imaged Exoplanets Using Wavelet Analysis Chris Merchantz Introduction · Challenges associated with direct images of planets Distinguish planets in the following way: (1) a minimum flux threshold is from speckles maxima, anddefined for the features that are identified as local (2) the "Exoplanet Recognition Using a Wavelet Analysis Technique" Fig. ... This spectrum is used as template spectrum to recognize planets in a deep image. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/astro193/ChristopherMerchantz_ay193_fp_slides.pdf -- 2905.9 Кб -- 04.05.2015
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3. Principal Components Analysis
... Among the objectives of Principal Components Analysis are the following. dimensionality reduction; љ . the determining of linear combinations of variables; љ . ... identification of groups of objects or of outliers. ... Finding a set of principal axes allows the objects to be adequately characterised on a smaller number of (artificial) variables. ... Reduction of dimensionality is practicable if the first new axes account for approximately 75 % or more of the variance. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node213.html -- 7.2 Кб -- 23.02.1996
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4. http://www.stsci.edu/hst/foc/documents/tips/tips_24feb94.ps
... There were 8 observation sets which had measur­ able targets for this analysis. ... TIPS Meeting 24 Feb 1994 W. Hack SPACETELESCOPESCIENCEINSTITUTE Summary of FOC Activities for the period 17 ­ 23 February 1994 F/48 Sensitivity and Background . ... FOC Contamination . ... TIPS Meeting 24 Feb 1994 W. Hack SPACETELESCOPESCIENCEINSTITUTE ­2 ­1 0 1 2 ­2 ­1 0 1 2 Target Offsets Since 25 Jan 1994 TIPS Meeting 24 Feb 1994 W. Hack SPACETELESCOPESCIENCEINSTITUTE TIPS Meeting 24 Feb 1994 W. Hack ...
[ Текст ]  Ссылки http://www.stsci.edu/hst/foc/documents/tips/tips_24feb94.ps -- 75.6 Кб -- 05.02.2013
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5. Space Telescope-European Coordinating Facility
... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/ -- 9.0 Кб -- 09.04.2016
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6. http://www.atnf.csiro.au/computing/software/gipsy/sub/gdscas.dc2
Function: GDSCAS Purpose: Changes the subset set selection for CLASS 1 applications. Category: USER IO File: gdsinp.c Author: K.G. Begeman Use: CALL GDSCAS( GDSOUTKEY , Input CHARACTER*(*) SELSUBSET , Input INTEGER ARRAY AXCOUNT ) Input INTEGER ARRAY GDSOUTKEY Keyword associated with a following call to GDSOUT. ... Description: Function GDSCAS changes the subset axis selection and is used by applications which are essentially CLASS 2 but leave the names of the operation axes intact. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/sub/gdscas.dc2 -- 2.0 Кб -- 21.07.2000
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