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    1. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/cal_standards_collection.pdf
    ... Chair: F. Haberl · Definition of standard candles Sources with constant X-ray flux: white dwarfs isolated neutron stars supernova remnants cluster of galaxies · Scientific drivers for accurate absolute fluxes neutron star radii cosmology (e.g. total mass ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/cal_standards_collection.pdf -- 41.9 Кб -- 15.06.2006
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    2. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/FD_SC.txt
    ... During this forum the list of candidate standard candle sources compiled during the Working Session was augmented by the addition of the isolated neutron star PSR0656 and the supernova remnants PSR1509 and 0540-69. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/FD_SC.txt -- 4.0 Кб -- 20.06.2006
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    3. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0070-0-0.pdf
    ... This method is then applied to data from the Vela supernova remnant. ... example of an XMM EPIC pn observation of an area within the Vela supernova remnant ... 33 ks observation of the Vela supernova remnant, performed in December 2001 (XMM rev ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0070-0-0.pdf -- 519.1 Кб -- 03.08.2006
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    4. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/mpea_eff_ff.pdf
    ... February 2005 M. Pilar Esquej , XMM- Newton European Space Astronomy Centre Page 1 Overview · EPIC ESAC Analyze a special observation of the supernova remnant Cas-A in order to refine the energy cross-calibration of the EPIC-pn extended Full Frame mode ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/mpea_eff_ff.pdf -- 810.3 Кб -- 16.05.2014
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    5. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0012-1-0.ps.gz
    ... Celestial measurements using supernova remnants with bright emission lines have in ... in EPIC MOS ­ 1ES0102­72 supernova remnant data (crosses), thermal spectrum+power ...
    [ 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. XMM Science Objectives
    ... Stellar black holes, neutron stars, pulsars . Supernova remnants . The hot phase of the Galactic ISM . Cool gas . ... Among the most prominent Galactic X-ray sources are supernova remnants (SNRs). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/sciobj/science_top1.html -- 30.1 Кб -- 24.09.1998
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    7. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-0.pdf
    ... 1.8 Cross Calibration with other Satellites ROSAT PSPC data of the supernova remnant factor between the different instruments. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-0.pdf -- 2175.1 Кб -- 12.08.2002
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-1.pdf
    ... EPIC, RGS, ACIS-S, ASCA, and ROSAT PSPC data of the supernova remnant 1E0102.2-7219 where the only independent parameter was a ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-1.pdf -- 1574.9 Кб -- 04.04.2003
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    9. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0026-1-0.ps.gz
    ... metrology) Figure 2: EUV measurement and simulation of the vignetting function at CSL In order to verify the effective area variation over the EPIC field of view, the G21.5­0.9 supernova remnant was observed on­axis and at four off­axis positions [4, 5 ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0026-1-0.ps.gz -- 131.6 Кб -- 03.01.2001
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    10. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0172-1-1.ps.gz
    ... 3.169 NO EPN CTI 0013 2000-01-01T00:00:00 LONG TERM CTI 3.169 NO 2 Changes The EPN CTI 0013.CCF improves an under-correction of the CTI of 2-3 % for the pn Small Window mode at energies between 550 and 700 eV where O-lines are found in supernova remnants ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0172-1-1.ps.gz -- 100.2 Кб -- 20.07.2004
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