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    1. SciSim simulation of Abell 2199 X-ray spectrum
    ... is based on an input model generated in xspec, based on the results of earlier ROSAT observations, folded through the EPIC RMF ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/sciobj/a2199.html -- 3.5 Кб -- 24.09.1998
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    2. XMM Deep Survey Simulations
    ... QSO spectra in the ROSAT band are steeper than the background at harder energies ... to resolve the requirement for the ROSAT band background, and provide a harder ... extracted the luminosity function from ROSAT Deep Survey results, and extrapolated ...
    [ 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/200605/VBurwitz.pdf
    ... Compare obtained photon spectra with EUVE and ROSAT and XMM (work by Frank Haberl) Vadim Burwitz EPIC CAL/OPS, MPE May 4, 2006 Overview Vadim Burwitz EPIC CAL/OPS, MPE May 4, 2006 NLTE pure H model spectrum of HZ43 Different bound-free and free-free ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200605/VBurwitz.pdf -- 1189.5 Кб -- 14.05.2014
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    4. Description
    ... It is currently not used, however might by used for a future task that takes as input some proxies like the RA & Dec, the ROSAT broad band count rates for the target location, the corner count rates etc. and generates a best guess background file. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node678.html -- 6.8 Кб -- 20.09.2011
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    5. Description
    ... It is currently not used, however might by used for a future task that takes as input some proxies like the RA & Dec, the ROSAT broad band count rates for the target location, the corner count rates etc. and generates a best guess background file. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node681.html -- 3.4 Кб -- 20.09.2011
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    6. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0036-1-0.ps.gz
    ... This was measured with a number of fields with ROSAT / Optical IDs, including (Lockman Hole, NGC2516, M31 and NGC253) 3 Estimated Scientific Quality Based on an analysis of Lockman Hole Rev 70 data, the mean displacement of about 25 central field of view ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0036-1-0.ps.gz -- 46.8 Кб -- 03.01.2001
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    7. Future developments
    ... The task does not at present work on SDF files. In these coordinate transformations, the same method as for the ROSAT PSPC has been used. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/attcalc/node10.html -- 3.4 Кб -- 10.01.2003
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    8. References
    ... Cruddace, R., G., Hasinger, G., Schmitt, J. H., The application of a maximum likelihood analysis to detection of sources in the ROSAT database, in `Astronomy from large Databases', eds. Murtagh, F. and Heck, A., p. 177, (1988). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/emldetect/node4.html -- 3.4 Кб -- 10.01.2003
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    9. Future developments
    ... The task does not at present work on SDF files. In these coordinate transformations, the same method as for the ROSAT PSPC has been used. ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.0.0/doc/attcalc/node10.html -- 3.5 Кб -- 18.03.2004
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    10. References
    ... Cruddace, R., G., Hasinger, G., Schmitt, J. H., The application of a maximum likelihood analysis to detection of sources in the ROSAT database, in `Astronomy from large Databases', eds. Murtagh, F. and Heck, A., p. 177, (1988). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.0.0/doc/emldetect/node4.html -- 3.5 Кб -- 18.03.2004
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