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http://hea-www.harvard.edu/AstroStat/etc/Schafer_AAS215_Jan2010_231.06.pdf.
http://hea-www.harvard.edu/AstroStat/etc/Schafer_AAS215_Jan2010_231.06.pdf.
1. The AstroStat Slog Blog Archive [ArXiv] Bimodal Color Distribution in GCS,
... Archives . ... ArXiv] SVM and galaxy morphological classification, Sept. 10, 2007 . ... On the Metallicity-Color Relations and Bimodal Color Distributions in Extragalactic Globular Cluster Systems by M. Cantiello and J. P. Blakeslee . Many observations on globular cluster systems (GCS) show bimodal distributions in color and metallicity space. ... Based on their simulation study, (V-H) and (V-K) are confirmed to be good colors for revealing unbiased bimodal metallicity distributions in GCS. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2007/arxiv-bimodal-gcs/index.html -- 21.4 Кб -- 01.03.2014
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2. Initial Distributions of Binary Parameters
Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node39.html -- 14.1 Кб -- 26.02.1997
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3. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0169-1-1.ps.gz
XMM-Newton CCF Release Note XMM- CCF -REL-169 EPIC MOS low energy response and Quantum Eфciency R. D. Saxton, Steve Sembay 5 August 2004 1 CCF components Name of CCF VALDATE EVALDATE Blocks changed XSCS ag EMOS1 QUANTUMEF 0016. CCF 2000-01-01 QE TOTAL NO EMOS2 QUANTUMEF 0016. CCF 2000-01-01 QE TOTAL NO EMOS1 REDIST 0035. CCF 1999-12-10 2000-07-15 CCD REDISTRIBUTION-n NO EMOS1 ... This excess was responsible for small underestimates of the Galactic absorption column. ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0169-1-1.ps.gz -- 68.4 Кб -- 10.09.2004
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4. A Simple Example With a Single Chirp Component
... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Chirplet.dir/node20.html -- 3.8 Кб -- 15.04.1998
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5. Spectral energy distribution
... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...