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    1. STScI Preprint #1342
    ... Compton Heating of the Intergalactic Medium by the Hard X-Ray Background. ... the intergalactic gas by the hard X-ray background (XRB), an effect neglected in all ... background at a given epoch, where x is the hydrogen neutral fraction in units of 10 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1342/prep1342.html -- 5.7 Кб -- 26.07.2000
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    2. http://www.stsci.edu/ftp/science/goods.save/Internal/aas-posters/Alexander_aas.pdf
    ... and XMM-Newton surveys have resolved the bulk of the 0.5-10 keV X-ray background ... obscured AGNs) are dominant and contribute the vast majority of the X-ray background ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/science/goods.save/Internal/aas-posters/Alexander_aas.pdf -- 1653.6 Кб -- 17.01.2003
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    3. http://www.stsci.edu/~marel/decadal/prof/White_archives_CDH_FFP.pdf
    ... current synthesis models of the X-ray background Barger, A. J. Optical and Infrared ... Barger, A. J. The Nature of the Hard X-Ray Background Sources: Optical,.. ... Fraction of the Cosmic X-Ray Background Kastner, J. H. Evidence for Accretion: High ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/prof/White_archives_CDH_FFP.pdf -- 480.9 Кб -- 16.03.2009
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    4. Poster Abstracts
    ... 80% of the cosmic X-ray background is resolved at 2-8 keV in the deepest Chandra surveys, the peak of the cosmic X-ray background remains largely unexplained (at energies of 8-40 keV). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/jwst2007/posterAbstracts -- 92.1 Кб -- 11.04.2016
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    5. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_06_17_97
    ... 1.5 Completed Two Sets of WF/PC-2 6677 (The Origin of the X-Ray Background: What are the Faintest X-Ray Galaxies?) ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_06_17_97 -- 8.9 Кб -- 17.06.1997
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    6. Poster Abstracts
    ... 80% of the cosmic X-ray background is resolved at 2-8 keV in the deepest Chandra surveys, the peak of the cosmic X-ray background remains largely unexplained (at energies of 8-40 keV). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/jwst2007/posterAbstracts.html -- 86.8 Кб -- 11.04.2016
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    7. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_16_97
    ... 1.16 Completed WF/PC-2 6677 (The Origin of the X-Ray Background: What are the Faintest X-Ray Galaxies?) ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_16_97 -- 11.3 Кб -- 16.07.1997
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    8. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_31_97
    ... 1.7 Completed WF/PC-2 6677 (The Origin of the X-Ray Background: What are the Faintest X-Ray Galaxies?) ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_31_97 -- 7.0 Кб -- 31.07.1997
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    9. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_06_23_97
    ... 1.2 Completed WF/PC-2 6677 (The Origin of the X-Ray Background: What are the Faintest X-Ray Galaxies?) ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_06_23_97 -- 13.6 Кб -- 23.06.1997
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    10. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_03_31_97
    ... Wave 1.12 Completed WF/PC-2 6677 (The Origin of the X-Ray Background: What = are the Faintest X-Ray Galaxies?) ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_03_31_97 -- 10.1 Кб -- 31.03.1997
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