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    • 1. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/crab_kaastra.pdf
    ... 1 and 3 partially, but except for White dwarf spectra there is nothing better Extended emission · Crab is extended: synchrotron nebula + dust scattering · RGS detectors (5' width) contain ~90 % of flux · Fraction energydependent · Determine using power ...
    [ 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/docs/documents/CAL-TN-0061-1-0.pdf
    ... a constant intensity source, since most of the emission is from the diffuse part of the nebula, which 1 mkirsch@sciops.esa.int ... The pulsar is believed to inject high-energy electrons into the nebula that radiate via synchrotron emission. ...
    [ 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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    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. 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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    5. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0012-1-0.ps.gz
    ... 1ES0102­72 65 Low energy emission line gain and and N132D 76 & 83 provide cross check with CHANDRA Crab Nebula 54 & 56 On­axis effective area in diffuse source. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0012-1-0.ps.gz -- 336.8 Кб -- 11.01.2001
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    6. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/WS_SC.txt
    ... absolute calibration of the X-ray spectrum of the Crab nebula", was recalled as an example of a dedicated calibration space ... Some discussion took place of the use of stars with emission lines as standard sources. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/WS_SC.txt -- 6.8 Кб -- 20.06.2006
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    7. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0030.pdf
    ... star RX J1856.6-3754 (black) and the Vela Pulsar Wind Nebula (red), both constant ... the area at the wavelengths of some prominent emission lines has varied since launch ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0030.pdf -- 1697.8 Кб -- 16.07.2015
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0086.pdf
    ... emission lines are thought to be present in the Fe-K band accessible to EPIC of many galactic and extragalactic X-ray spectra and claims have also been made of similar broad features in the RGS band below 2 keV, due perhaps to the equivalent Fe-L shell ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0086.pdf -- 1083.3 Кб -- 22.02.2011
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    9. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf
    ... orbit drift and consequently reduced reflected emission from Earth decreased the ... the history of X-ray astronomy the Crab nebula has served as a reference which, in ...
    [ 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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