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    1. http://www.adass.org/adass/proceedings/adass02/reprints/P99-1.pdf
    ... The ESSENCE pro ject aims to constrain the equation of state of dark energy through the study of intermediate redshift (0.15 < z < 0.75) supernovae (SNe). ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/P99-1.pdf -- 66.7 Кб -- 11.03.2003
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    2. ADASS 2002 Conference Proceedings
    ... The ESSENCE project aims to constrain the equation of state of dark energy through the study of intermediate redshift ( ) supernovae (SNe). ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/P99-1/ -- 15.8 Кб -- 13.03.2003
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    3. A Test for Weak Cosmic Ray Events on CCD Exposures
    ... In Figure , where the de-glitch PDF turns over at low energy---presumably but not necessarily at an energy greater than or equal to the turnover in the dark PDF---gives some idea as to how effective the algorithm has been in removing the weaker events. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/blandhawthornj.html -- 7.9 Кб -- 03.11.2000
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    4. http://www.adass.org/adass/proceedings/adass94/blandhawthornj.ps
    ... In Figure 2, where the de­glitch PDF turns over at low energy--- presumably but not necessarily at an energy greater than or equal to the turnover in the dark PDF---gives some idea as to how effective the algorithm has been in removing the weaker events. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass94/blandhawthornj.ps -- 149.4 Кб -- 13.06.1995
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    5. http://www.adass.org/adass/proceedings/adass03/reprints/P2-2.pdf
    ... N= N N Obj Obj where N filter band wi surface, i is energy of one S = N + nbin .N Sky + nbin .RON 2 + npix .D ARK .T where RON is the contribute to the detected counts due to the Read Out Noise, DARK is the similar term due to the dark counts, nbin is the ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P2-2.pdf -- 74.8 Кб -- 27.08.2004
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    6. RoadRunner: An Automated Reduction System for Long Slit Spectroscopic Data
    ... about how and when to take biases, flats, darks, comps, skys and standards; how to ... raw data files: 40 biases, 40 flats, four darks, five skys, 83 comps, and 115 object ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/tokarzs.html -- 12.4 Кб -- 23.06.1998
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    7. Modelling Astrophysical Turbulent Convection
    ... hot fluid as bright, with downward-flowing, cold fluid as darker tones ... for the conservation of mass, momentum, and energy, along with the equation of state ... High enstrophy is bright and opaque whereas low enstrophy is dark and translucent. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/brummelln.html -- 31.6 Кб -- 03.11.2000
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    8. http://www.adass.org/adass/proceedings/adass96/reprints/wisem.pdf
    ... mirrors, the low- and high-energy transmission grating assemblies (LETG and HETG ... Sources may have arbitrary sp ectral energy distributions which are sp ecified via ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/wisem.pdf -- 511.9 Кб -- 14.01.1998
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    9. Simulated AXAF Observations with MARX
    ... mirrors, the low- and high-energy transmission grating assemblies (LETG and HETG ... Sources may have arbitrary spectral energy distributions which are specified via an ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/wisem.html -- 12.6 Кб -- 23.06.1998
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    10. Image Processing of Digitized Spectral Data
    ... One of the research fields of our group is the mechanism of energy transport and energy release in solar flares. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/boulatova.html -- 13.7 Кб -- 15.05.1998
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