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    1. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/crab_kaastra.pdf
    ... nebula as calibration source · Good calibration sources should obey: 1) Simple continuum 2) Known continuum 3) Constant in time 4) Point source 5) No dust scattering halo Crab only obeys rule 1 and 3 partially, but except for White dwarf spectra there is ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/crab_kaastra.pdf -- 242.0 Кб -- 19.06.2006
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    2. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/INTEGRAL_SPI.pdf
    ... SPI Crab Nebula observations THE CRAB NEBULA 20-50 keV 567 ks Crab Nebula Stability in the FOV Rev 300 10° circle around the axis Crab Nebula - Calibration stability ­ revolutions 300 and 45 Crab Nebula observations Whole camera peak positions in keV and ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/INTEGRAL_SPI.pdf -- 1702.4 Кб -- 19.06.2006
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    3. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0302-1-5.pdf
    ... the results of a specific calibration experiment performed on the Crab Nebula (cf ... Two subsequent observations of the Crab Nebula were performed in September 2011 to ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0302-1-5.pdf -- 319.7 Кб -- 25.10.2013
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    4. XMM-Newton Trainee Project 2004
    ... a optimal phase and space resolved spectroscopy of the Crab pulsar and nebula ... object, the so-called Crab pulsar, and a region of nebulosity, the Crab nebula ... spatial and a high quality phase resolved spectroscopy of the Crab nebula and pulsar ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_links/trainee/2004/gabi.shtml -- 16.0 Кб -- 13.04.2016
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    5. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0238-1-0.ps.gz
    ... A final comparison with the Crab nebula allowed final adjustments for power­law slope and overall normalisation. ... the RGS fluxed spectra of the neutron star RXJ1856­3754 and the Vela Pulsar Wind Nebula, both of which are e#ectively constant ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0238-1-0.ps.gz -- 118.6 Кб -- 19.09.2007
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    6. Cross References to In-Flight Calibration Targets
    ... Pile-UP . Mode dependence . PSFPileUp,RedistPileUp . Crab Nebula . X-ray Stray light . Fast timing . XSLAreaEf,XSLDist . ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node968.html -- 40.7 Кб -- 20.09.2011
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    7. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0069-1-0.pdf
    ... We were able to distinguish four typical regions as (a) background (Cols. 1-13 and 55-64) (b) outer nebula (Cols. 14-22 and 47-54) (c) inner nebula (Cols. 23-33 and 41-46), and (d) pulsar (Cols. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0069-1-0.pdf -- 913.2 Кб -- 04.07.2006
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0061-1-0.pdf
    ... however, is independent of the Crab nebula, because this object has not been used to ... days of X-ray astronomy the Crab nebula has been used as a calibration target for ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0061-1-0.pdf -- 1023.2 Кб -- 10.11.2005
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    9. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0281-1-0.pdf
    ... Existing calibration data based on a recent (September 2011) observation of the Crab Nebula are consistent with this assumption, at least for EPIC-pn Timing Mo de. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0281-1-0.pdf -- 68.1 Кб -- 31.05.2012
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    10. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0248-1-0.ps.gz
    ... 1.051.1 Data/model ratio Energy (keV) 1000 500 2000 Cts/sec/keV Obs.0118700201 - Crab Nebula - 255.2 cts/s 1.5 2 2.5 0.90.95 1 1.051.1 Data/model ratio Energy (keV) 1000 500 2000 Cts/sec/keV Obs.0118700201 - Crab Nebula - 255.2 cts/s 1.5 2 2.5 0.90.95 1 1 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0248-1-0.ps.gz -- 334.0 Кб -- 02.02.2009
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