... The Chan dra Multiwavelength Project (ChaMP) will combine radio to Xray observations of serendipitous Chandra sources, with emphasis on optical identification. ...
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Ссылки http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/HY-z-smita.ps -- 1193.2 Кб -- 19.09.2003 Похожие документы
... The BY Dra and RS CVn stars match the LDSS2 sample with 0.1% probability (see Figure 10, right-hand panels)--exceeding the luminosities of the BY Dra systems, and falling short of the RS CVn X-ray luminosities. ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/papers/0612-draft-xavier-magellan.pdf -- 603.0 Кб -- 27.02.2007 Похожие документы
... are presented with problems, such as large rotational broadening and composite spectra in the case of RS CVn and BY Dra binaries, and atmo spheric modeling difficulties in the case of active M dwarfs, the coronal regime offers an alternative route to ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/papers/cs10_drakej1/drakej1.ps -- 2037.3 Кб -- 03.11.2000 Похожие документы
... m edian 3D Parameter space probed with MCMC statistics Gamma A DA S S No v. 8 , 2 0 1 0 A n e ta S i e m i g i n o wska N H 11 Application: Calibration Uncertainties Chandra ACIS-S Effective Area Data Calibration Draw effective area Dra ke e t a l ...
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Ссылки http://hea-www.harvard.edu/AstroStat/etc/ADASS2010_skvcpr+.pdf -- 1216.1 Кб -- 08.11.2010 Похожие документы
... To take full advantage of the rich serendipitous dataset afforded by Chan dra's large FoVs (ACISI: 16 0 \Theta 16 0 ) and to maximize the science per ksec of observing time, we have organized an extragalactic serendipitous Xray survey, the ChaMP and a ...
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Ссылки http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/ChaMP_NEWFA.ps -- 969.0 Кб -- 15.11.2000 Похожие документы
... 1 (Table The sourceнnaming convention of ChaMP (CXOMP Jhhmmss.s#ddmmss) is given with a prefix CXOMP (Chanн dra Xнray Observatory Multiwavelength Project) affixed with truncated J2000.0 position Xнray source after mean field offset correction applied ...
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Ссылки http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/jds_paper03FINAL.ps -- 458.4 Кб -- 23.09.2003 Похожие документы
... At the lowest de nitively AGN luminosities (LX > 10 42 ), our Chan- dra/NOAO survey combination is highly complete to z = 0:1, where an L E/S0 host has R = 16. ...