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    1. http://hea-www.harvard.edu/AstroStat/etc/xgratings_2007_klwwenmsw.pdf
    ... ...
    [ ]   http://hea-www.harvard.edu/AstroStat/etc/xgratings_2007_klwwenmsw.pdf -- 782.9 -- 14.07.2007

    2. http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_hosung.pdf
    ... i W i U W U W W i? U ... i W e w U U U W W ... U W? U ? R U 1? ...
    [ ]   http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_hosung.pdf -- 167.3 -- 13.09.2004

    3. http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_sourlas.pdf
    ... p p f " d d ' " p u " " p u % p d 1 B ' d ... ` Q ? n ? ? ? ? 2? ...
    [ ]   http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_sourlas.pdf -- 486.2 -- 20.09.2004

    4. http://hea-www.harvard.edu/~kim/pap/ULX_N4244.pdf
    ... 4:900::36 , K ?3:38?0::82 104 0 61 ?2 70 kT 0:300?0::030 , K 3:151::42 0 027 ?1 68 ?5 92 6:880::71 , Kpow ?6:912::91 104 , ?0 087 kT 0:712 Kdiskbb 0:0160::015 1 0:22?0::46 , 2 3:85?0::20 , Eb 0:94 0:04 K ?1 ...
    [ ]   http://hea-www.harvard.edu/~kim/pap/ULX_N4244.pdf -- 195.2 -- 06.12.2010

    5. http://hea-www.harvard.edu/~kim/pap/2003_JKAS.pdf
    ... ? ...
    [ ]   http://hea-www.harvard.edu/~kim/pap/2003_JKAS.pdf -- 400.5 -- 06.12.2010

    6. http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_taeyoung_line.pdf
    ... ( 8 ( # V3 S' ? 8 7 3 % x p d m x { pw hn n x ~m ? am G ? P e cx Tx d ? u m x m n SR jP? ...
    [ ]   http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_taeyoung_line.pdf -- 155.8 -- 12.09.2004

    7. http://hea-www.harvard.edu/~kim/pap/Sombrero.pdf
    ... comes from thermal bremsstrahlung, with a flat power law ( < 1:5 in the Chandra band) or inverse Compton scattering of soft synchrotron photons by the flow electrons, with a steeper X-ray spectral shape (e.g., $ 2:2 has been used to model the nucleus ...
    [ ]   http://hea-www.harvard.edu/~kim/pap/Sombrero.pdf -- 374.3 -- 06.12.2010

    8. http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_taeyoung_HR.pdf
    ... t B F ii r i r B$? i { e x e s ...
    [ ]   http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_taeyoung_HR.pdf -- 290.8 -- 12.09.2004

    9. http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_X2.pdf
    ... A single power-law fit is not statistically acceptable, so a broken power-law model is applied as follows: dN dS ( KS bright faint KSbreak S>S S fain t The best-fit slopes for the differential log N log S are bright 2:2 0:2 at the bright end ...
    [ ]   http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_X2.pdf -- 698.7 -- 22.01.2004

    10. http://hea-www.harvard.edu/~bradw/cv/papers/BayesHR.pdf
    ... 3 where S , H , BS ,and BH are typically approximated with the Gehrels prescription (Gehrels 1986 ... 5 The observed background counts are also modeled as independent Poisson random variables, BS $ PoissonreS S ; BH ...
    [ ]   http://hea-www.harvard.edu/~bradw/cv/papers/BayesHR.pdf -- 718.5 -- 27.11.2006

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