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    51. The AstroStat Slog Blog Archive SINGS
    ... consider classifying blurry galaxies by eyes: a spiral can be classified as a irregular, for example. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2009/sings/index.html -- 25.5 Кб -- 01.03.2014
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    52. http://hea-www.harvard.edu/~kim/pap/2012_YoungE_ISM_published.pdf
    ... distinctive signature in the X-ray luminosity function (XLF) of their low-mass X-ray binary (LMXB) population, which have power-law slopes in between those of typical old elliptical galaxies and of spiral and starburst galaxies with current star formation ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_YoungE_ISM_published.pdf -- 875.1 Кб -- 03.05.2012
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    53. http://hea-www.harvard.edu/AstroStat/etc/SvDKS2015_ApJ813_66_LIRA_pval.pdf
    ... In astronomy, Ripley & Sutherland (1990) used spatial stochastic processes to directly model structures in spiral galaxies, and Esch et al. (2004) obtained uncertainty estimates for reconstructed X-ray images using a Bayesian model known as EMC2 that ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/etc/SvDKS2015_ApJ813_66_LIRA_pval.pdf -- 964.8 Кб -- 30.10.2015
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    54. http://hea-www.harvard.edu/~elvis/cv.pdf
    ... 25 1984 JHKL Photometry of the Nuclei of Normal Spiral Galaxies (S.P. Willner, M. Ward, A. Longmore, A. Lawrence, G. Fabbiano, and M. Elvis) Publications of the Astronomical Society of the Pacific, volume 96, 143. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/cv.pdf -- 401.5 Кб -- 13.04.2011
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    55. http://hea-www.harvard.edu/~kim/pap/2010_YoungE_LMXB_ApJ.pdf
    ... galaxies have shown that the XLF changes from old stellar systems to young stellar systems with the XLF slope getting flatter ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2010_YoungE_LMXB_ApJ.pdf -- 555.8 Кб -- 06.12.2010
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    56. http://hea-www.harvard.edu/~kim/pap/2006_SWIRE.pdf
    ... The SEDs of the other three sources are dominated by starlight in the optical and near-IR and are best fitted with spiral galaxy templates. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2006_SWIRE.pdf -- 1812.7 Кб -- 06.12.2010
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    57. The AstroStat Slog Classification
    ... Mainly elliptical galaxy formation has been studied due to more abundance compared to spirals and the galactic bimodality in color-color or color-magnitude diagrams is the result of the gas-rich mergers by blue mergers forming the red sequence. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/classification/page/2/index.html -- 29.1 Кб -- 02.03.2014
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    58. http://hea-www.harvard.edu/~kim/pap/N1316_2003.pdf
    ... Sarazin et al. 2000), but much steeper than those in spirals and star burst galaxies (Prestwich 2001; Zezas & Fabbiano 2002 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/N1316_2003.pdf -- 1519.0 Кб -- 06.12.2010
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    59. http://hea-www.harvard.edu/~garcia/astroph.0203243.ps
    ... is t to the LF (i.e., where there is no clear break) the LFs of early type galaxies and the bulges of spirals tend to be steeper (  1:7) than those of spiral disks and galaxies with active star forming regions (  0:8, e.g, Prestwich 2001, Kilgard et al ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~garcia/astroph.0203243.ps -- 1110.1 Кб -- 08.02.2011
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    60. The AstroStat Slog VO
    ... Mainly elliptical galaxy formation has been studied due to more abundance compared to spirals and the galactic bimodality in color-color or color-magnitude diagrams is the result of the gas-rich mergers by blue mergers forming the red sequence. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/vo/index.html -- 32.3 Кб -- 01.03.2014
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