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    1. Heuristic Estimates of Weighted Binomial Statistics for Use in Detecting Rare
    ... required to operate on the far tail of the distribution, where many traditional ... where converts ``sigmas'' of significance into a one-tailed p -value. ... but does not appear well suited for p -values at the far tail of the distribution ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/theilerj.html -- 14.9 Кб -- 23.06.1998
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    2. http://www.adass.org/adass/proceedings/adass96/reprints/theilerj.pdf
    ... required to op erate on the far tail of the distribution, where many traditional ... s) = 1 (1 - erfc(s/ 2)) converts "sigmas" of significance into a one2 tailed p-value ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/theilerj.pdf -- 202.8 Кб -- 14.01.1998
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    3. QPSIM: An IRAF/PROS Tool for Source Simulation
    ... 1993). In the on-axis figure, the two Gaussian functions are not easily distinguishable, and quickly decrease to the exponential tail. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/manningk.html -- 11.9 Кб -- 03.11.2000
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    4. http://www.adass.org/adass/proceedings/adass02/reprints/D10.pdf
    ... Students can use the testbed to simulate stellar dynamics: dynamics of single galaxies (relaxation, scattering and collapse); interacting galaxies (collisions and mergers); and to explore interesting structures like tidal tails. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/D10.pdf -- 67.9 Кб -- 11.03.2003
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    5. ADASS 2002 Conference Proceedings
    ... Students can use the testbed to simulate stellar dynamics: dynamics of single galaxies (relaxation, scattering and collapse); interacting galaxies (collisions and mergers); and to explore interesting structures like tidal tails. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/D10/ -- 13.2 Кб -- 12.03.2003
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    6. Porting CGS4DR to Unix
    ... The following data reduction sequence could have been generated by the DA system automatically adding observation numbers 2--3 to the ``tail'' of the queue and the observer inserting observation number 1 at the ``head'' of the queue: . ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/dalyp2.html -- 13.6 Кб -- 03.11.2000
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    7. http://www.adass.org/adass/proceedings/adass94/manningk.ps
    ... 1993). In the on­axis figure, the two Gaussian functions are not easily distinguishable, and quickly decrease to the exponential tail. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass94/manningk.ps -- 232.3 Кб -- 13.06.1995
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    8. Discrimination of Point-like Objects in Astronomical Images using Surface
    ... Figure 1 (right side) is a sketch of the ( ) diagram based on a CCD image which exhibits an extended source; the tail of comet P/Halley, a rich star field, and various defects and artifacts. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/llebariaa.html -- 15.6 Кб -- 03.11.2000
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    9. ISAS Data Archive and Transmission System (DARTS)
    ... The primary purpose of this mission is to study the structure and dynamics of the tail region of the magnetosphere. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P3-16/ -- 14.7 Кб -- 06.10.2000
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    10. Using a Data-Driven Model for Instrument Software Development
    ... With only one authoritative source of the information, programmers would not be chasing their tails trying to keep these different forms of the same data in synch; they could do more productive things with their time. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/O7-05/ -- 14.3 Кб -- 04.10.2000
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