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    61. Martin Elvis - Brief Biography
    ... Applying the multi-wavelength approach to ROSAT spectra and ultraviolet spectra he, with his colleagues, discovered a hot wind from a number of AGN, peaking in 1995 with a UV/X-ray study of the "Seyfert galaxy" NGC 5548 . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~elvis/briefbio.html -- 7.9 Кб -- 01.10.2012
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    62. H/RCULES
    ... The Hubble/ROSAT Continuum and Ultraviolet Line Emission Study (H/RCULES) of AGN enables characterization of: . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/HRCULES.html -- 8.4 Кб -- 01.10.2012
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    63. http://hea-www.harvard.edu/AstroStat/Stat310_0708/ac_20070918.pdf
    ... 3 !2 !1 0 1 2 3 Log10(Expected Total MS Counts) EMC2 Mean Results: Null vs Interesting Null vs `Interesting' Data: Object Level Quantiles Null Soft X-Ray/Extreme Ultraviolet Sky (local "warm fuzz" around our solar system: glowing warm gas) Snowden 1995 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0708/ac_20070918.pdf -- 2871.8 Кб -- 18.09.2007
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    64. http://hea-www.harvard.edu/AstroStat/astro193/Week1-Jan28.pdf
    ... base access to optical data from the optical sky survey, images, photometry, spectra MAST Space Telescope archives tps://archive.stsci.edu/ ht data base with optical, ultraviolet and infrared data direct observational data, and pipeline processed data ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/astro193/Week1-Jan28.pdf -- 84.0 Кб -- 29.01.2015
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    65. Request for Spectral Data
    ... files (for example 3 [comprising radio, infrared, and X-ray data] or 8 [comprising radio, mmwave, far infrared, near infrared, optical, ultraviolet, X-ray, and Gamma ray data) in any units and combine and convert all to produce one file of Energy Flux (in ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~saku/DataRequest.html -- 3.0 Кб -- 01.10.2012
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    66. Hercules X-1/HZ Her
    ... Magenta arrows designate Ultraviolet observation times (FUSE, EUVE, HST). Red arrows designate Infrared (ISO) observation times. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~saku/RXTE.dir/herx1.html -- 4.1 Кб -- 01.10.2012
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    67. http://hea-www.harvard.edu/~saku/Sep2010Haiku.pdf
    ... shine singly on the milky way Are well known, but binaries still evade our full assay Complex models we have built from ultraviolet to infrared See what comes from star and disk or perhaps a wind instead O, microquasar, show thyself, are precessing jets ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~saku/Sep2010Haiku.pdf -- 2183.5 Кб -- 01.03.2011
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    68. Why Spectral Energy Distributions?
    ... of the few sources that have been examined in this way have been remarkably successful in explaining X-ray, ultraviolet (UV), and optical observations and resulted in improved physical constraints on the systems, a new understanding of the dependence of ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~saku/WhySEDs.html -- 4.0 Кб -- 01.10.2012
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    69. AstroStat Talks 2012-2013
    ... X-ray and Extreme Ultraviolet Observations of GOES C8 Solar Flare Events . ... soft X-rays (SXR) and extreme-ultraviolet (EUV) imaging and spectral observations of ... phases is observed in both soft X-ray (SXR) extreme ultraviolet (EUV) wavelengths ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1213/ -- 28.7 Кб -- 27.02.2014
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    70. PINTofALE
    ... Markov-Chain Monte Carlo Reconstruction of Emission Measure Distributions: Application to Solar Extreme-Ultraviolet Spectra , Kashyap, V. & Drake, J.J., 1998, ApJ 503, 450 . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PINTofALE/ -- 25.6 Кб -- 09.04.2016
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