... used in ChaMPlane Name Range Bx 0.3 - 8.0 keV : wavdetect band (also used as B) Sx 0.3 - 2.5 keV : used only in XPIPE Hx 2.5 - 8.0 keV : used only in XPIPE Bc 0.5 - 8.0 keV Sc 0.5 - 2.0 keV Hc 2.0 - 8.0 keV Level A "level" is assigned to each source for ...
... H S) 2.5--8.0 f Observed monochromatic, Galactic absorption--corrected, magnitude ... a counts within bandpass (0.3--2.5 keV) # and counts in hard bandpass (2.5--8.0 keV ...
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Ссылки http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/jds_paper03FINAL.ps -- 458.4 Кб -- 23.09.2003 Похожие документы
... broadband sensitivity between 0.3 and 8.0 keV enables the selection to be far less ... the soft bandpass (0.32.5 keV) and no counts in the hard bandpass (2.58.0 keV ...
... broadband sensitivity between 0.3 and 8.0 keV enables the selection to be far less ... S)/(H # S) 2.5--8.0 keV. f Observed monochromatic, Galactic absorption--corrected ...
... aperture photometry on each source to extract the basic source properties such as net count and net count rate in the conventional energy bands (SC : 0.52.0, HC : 2.08.0 and BC : 0.58.0 keV) and energy quantiles in the broad band (BX : 0.38.0 keV ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/papers/0902-draft-jaesub-xray_dist.pdf -- 750.9 Кб -- 09.03.2009 Похожие документы
... Chandra Proposers' Observatory Guide, and our own simulations with the Chandra Ray Tracer [ChaRT ]; see the Appendix), and it degrades very slowly to encircle $90% at !30 for the same energies (see Fig. 4.13 in the The Chandra Proposers' Observatory Guide ...
... in XSPEC (v11.3), where the data were restricted to 0.38.0 keV, as energies below this have calibration uncertainties, and the spectra presented here do not have significant source flux above 8.0 keV, where the data are highly contaminated by cosmic rays ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2010_N3379_LMXB_sp.pdf -- 1056.6 Кб -- 14.09.2011 Похожие документы