... deep breath before diving Finoguenov Alexis HDFS LH COSMOS COSMOS 9.5-12 keV 0.5-2 keV COSMOS Andy Read 2-4.5 keV COSMOS Andy Read OOTE Singles vs doubles Spectral compari so n After Renormalization Clean Andy Detector Outskirts: the golden Mile .. and ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/af_deep_bkg.pdf -- 2115.4 Кб -- 16.05.2014 Похожие документы
... be used · Bright optical stars create wrong detections, but positions are well know and can be vetoed · In 139 detections ~ 50 new sources · Deepest 2-10 keV all sky survey to date at 2.2x10E-12 · Only use FF, EFF, LW data 2.10 Update of the RGS Quantum ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/minutes.pdf -- 96.3 Кб -- 11.06.2014 Похожие документы
... surfaces which can image the X-ray sky with very high sensitivity and good angular ... This way, "pictures" of the sky as seen at X-ray energies are created. ... emission from the same regions on the sky can be obtained contemporaneously with the ...
... and spectrally 'for MOS' (pn is work in planning) · Blank sky files are maintained updated and used (useful comments and ... o pn new redistribution and rate dependent CTI --> deeper investigation and SAS development o MOS patch calibration currently ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/minutes.pdf -- 130.4 Кб -- 13.05.2014 Похожие документы
... operates in the energy range from 0.2-15 keV and provides spatial, energy and timing information of objects in the X-ray sky ... His major research interests are deep extragalactic multi-wavelength surveys (e.g. the XMM Large Scale Survey), as well as ...
... deepest ever Aim to issue the first slew catalogue (XMMSL1) by the end of 2005 3.5 Report from the EPIC BG w orking group (AMR) · UG recommended to EPIC to progress in BG description and treatment · Setting up of EPIC -BG working group · Define ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200510/Minutes.pdf -- 85.0 Кб -- 14.05.2014 Похожие документы
... taken for ground-based astronomy have a shot noise on sky background which will usually be significantly higher than the read ... This is most likely to happen when the photon is absorbed deep in the silicon where the electric field is small. ...
... Sky Image OM Source Lists Tracing Star Time Series Gzipped FITS Zipped FITS Zipped ... to Sky Co ordinates The task omatt converts an OM OSW source list from pixels to sky ...
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Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/documentation/xmm_abc_guide.pdf -- 1982.8 Кб -- 16.08.2005 Похожие документы