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    • 1. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/MartinA.pdf
    ... EPIC Page 6 other pulsars (III) · PSRJ 0537-69 Rev 0357 ID Obs.Time (s) 0113020201 36000 · pulsar in the Large Magellanic Cloud · distance: ~50kPc · period: ~16ms Antonio Martin-Carrillo XMM-Newton EPIC Page 7 folded light curves Antonio Martin-Carrillo ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200610/MartinA.pdf -- 1267.7 Кб -- 14.05.2014
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    2. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0005-1-0.ps.gz
    ... Sources studied include the sources of the ''First Light Field'' to the Large Magellanic Cloud and the point sources EXO 0748­67, LMC X­3, PSR 0540­69 and PKS 0558­504. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0005-1-0.ps.gz -- 114.4 Кб -- 11.01.2001
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    3. http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf
    ... The results are outlined below. It was followed by observations of a nova detected in the Large Magellanic Cloud (Nova LMC 2000). ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/sched_tour/too_paper.pdf -- 30.7 Кб -- 07.11.2001
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    4. http://xmm.vilspa.esa.es/external/xmm_sched/sched_tour/ESA_bulletin_107.pdf
    ... The results are outlined below. It was followed by observations of a nova detected in the Large Magellanic Cloud (Nova LMC 2000). ...
    [ 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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    5. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf
    ... identified so far, although its weakness and softness compromise its use for many instruments, including the RGS which has concentrated instead on bright SNRs in the Magellanic clouds whose distance has the advantage of limiting their angular sizes ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf -- 673.9 Кб -- 10.11.2005
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    6. http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-11.ps.gz
    ... 2.1.1.2 E#ective Area, Gain/O#set Monitoring The two targets for the EPIC e#ective area and gain/o#set monitoring are the SNRs 1ES0102­72 and N132D in the Magellanic Clouds. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-11.ps.gz -- 118.2 Кб -- 09.01.2009
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    7. http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-9.ps.gz
    ... 2.1.1.2 E#ective Area, Gain/O#set Monitoring The two targets for the EPIC e#ective area and gain/o#set monitoring are the SNRs 1ES0102­72 and N132D in the Magellanic Clouds. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-9.ps.gz -- 179.2 Кб -- 31.03.2008
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    8. XMM-Newton Observation Log Summary
    ... Publications Publications Large Programmes Publication Guidelines Source Naming ... 2003-03-07 . 0402 . Sco X-1 large offset . 2002-02-18T08:05:50 . 16:21:34.20 . ... 2003-07-15 . 0423 . Magellanic Bridge . 2002-04-01T14:18:34 . 02:15:15.00 . ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_mission_plan/odf_pps/catstrip_0401_0500.shtml -- 372.1 Кб -- 11.04.2016
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    9. XMM-Newton Observation Log Summary
    ... Publications Publications Large Programmes Publication Guidelines Source Naming ... 2002-04-27 . 0105 . Magellanic Bridge . 2000-07-05T15:03:51 . 02:15:22.00 . ... 2002-09-28 . 0138 . L1551 cloud . 2000-09-09T18:15:51 . 04:31:39.00 . +18:10:00.0 . ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_mission_plan/odf_pps/catstrip_0101_0200.shtml -- 306.4 Кб -- 11.04.2016
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