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  • 1. http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/n_fonseca.pdf
    ... radio galaxies, quasars, blazars... radio quiet radio quiet quasars (RQQs) Veron `06 ... Quasars and Seyfert Radio: Flux in 6cm (5GHz) and 20cm (1.4GHz) An X-ray/radio ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/alumni/n_fonseca.pdf -- 670.0 Кб -- 16.08.2006
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    2. XMM Deep Survey Simulations
    ... band are steeper than the background at harder energies, and furthermore at fluxes below 1E-14 ergs/(s cmќ) the quasar source counts flatten off and are replaced by more numerous populations of relatively low red-shift objects, apparently Narrow Emission ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/sciobj/deep_survey.html -- 6.2 Кб -- 24.02.1998
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    3. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/marshall-cal-2012.pdf
    ... BOC 2012 BLLs fit best RL Quasars BL Lacs H. Marshall -- Chandra 6 /26 EPIC BOC 2012 Combining Residuals 8 BL Lac objects Curved PL model H. Marshall -- Chandra 7 /26 EPIC BOC 2012 Combining Residuals 10 RL Quasars Double PL model H. Marshall -- Chandra 8 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/marshall-cal-2012.pdf -- 2898.0 Кб -- 13.05.2014
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    4. XMM Science Objectives
    ... Normal and starburst galaxies . Active galactic nuclei and quasars . Stellar black holes, neutron stars, pulsars,. ... contribute significantly to the detected metal content of absorption line systems on the sightlines towards distant quasars ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/sciobj/science_top1.html -- 30.1 Кб -- 24.09.1998
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    5. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0192-1-1.ps.gz
    ... As an example, in Figure 2 the residuals of a galactic absorption plus two power-law model t to the pn, MOS-1 and MOS-2 spectra of a revolution 1023 observation of the Radio-Loud Quasar 3C273 are shown. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0192-1-1.ps.gz -- 75.0 Кб -- 22.08.2005
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    6. http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf
    ... A high redshift quasar The most distant known celestial object, the quasar SDSJ1024-0125 was observed by XMM-Newton on May 28 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf -- 30.7 Кб -- 07.11.2001
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    7. http://xmm.vilspa.esa.es/external/xmm_sched/sched_tour/ESA_bulletin_107.pdf
    ... high-redshift quasar The most distant known celestial object at the time of observation, the quasar SDSJ10240125, was observed ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sched/sched_tour/ESA_bulletin_107.pdf -- 881.3 Кб -- 13.04.2004
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0064-0-0.pdf
    ... Not only galactic X-ray binaries are bright but also extragalactic objects such as quasars. ... as well as for neutron star and black hole X-ray Binaries and Quasars which also have in some cases a pronounced soft component ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0064-0-0.pdf -- 1269.1 Кб -- 13.03.2006
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    9. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/carpano-cal-2012.pdf
    ... GRO J1655-40 (6), Aql X-1 (4), PSR 0540 (3: binaries J17091-3624 (1), XTE J17520-223 (1), XTE J1817-330 (1), GRB Quasar 3C273 (1, too weak) Looking for narrow emission/absorption lines 4U 1700-37: bright emission line at 6.4 keV Cas-A: 10 emission lines ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/carpano-cal-2012.pdf -- 1723.4 Кб -- 13.05.2014
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    10. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201103/minutes-cal-2011.pdf
    ... A.Read: "The EPIC PSF" Astrometry tests of the 2-D PSF showed a systematic discrepancy between the XMM-Newton EPIC and the SDSS positions on a sample of quasars. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201103/minutes-cal-2011.pdf -- 124.4 Кб -- 13.05.2014
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