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    1. How to Piece Together Diffracted Grating Arms for AXAF Flight Data
    ... Once zero order source positions are found, the target source is identified by matching the sky positions with an observation ... regions need to be identified and the software must be able to decompose these regions into the component source parts ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/alexova.html -- 13.3 Кб -- 12.06.2006
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    2. The STScI NICMOS Calibration Pipeline
    ... Input Data . Combining NUMITER Images . Identifying Sources . Scalar Background Subtraction . 2-D Background Subtraction . ... pixels that are greater than 5 sigma above the median signal level in each image are identified as candidate source pixels ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node9.html -- 27.5 Кб -- 12.06.2006
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    3. http://www.stecf.org/conferences/adass/adassVII/reprints/alexova.pdf
    ... Once zero order source positions are found, the target source is identified by matching the sky positions with an observation ... regions need to be identified and the software must be able to decompose these regions into the component source parts ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/alexova.pdf -- 111.2 Кб -- 12.06.2006
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    4. http://www.stecf.org/conferences/adass/adassVII/reprints/alexova.ps.gz
    ... Once zero order source positions are found, the target source is identified by matching the sky positions with an observation ... regions need to be identified and the software must be able to decompose these regions into the component source parts ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/alexova.ps.gz -- 101.1 Кб -- 12.06.2006
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    5. NICMOS Data Calibration and Analysis
    ... Input Data . Combining NUMITER Images . Identifying Sources . Scalar Background Subtraction . 2-D Background Subtraction . Creating Mosaics . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node8.html -- 13.2 Кб -- 12.06.2006
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    6. Distributed Searching of Astronomical Databases with Pizazz
    ... Next, we must choose a model for interacting with the identified data sources in parallel. We narrow these models to two. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/gamielk.html -- 11.0 Кб -- 12.06.2006
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    7. http://www.stecf.org/conferences/adass/adassVII/reprints/gamielk.pdf
    ... Next, we must choose a model for interacting with the identified data sources in parallel. We narrow these models to two. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/gamielk.pdf -- 69.3 Кб -- 12.06.2006
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    8. http://www.stecf.org/conferences/adass/adassVII/reprints/gamielk.ps.gz
    ... Next, we must choose a model for interacting with the identified data sources in parallel. We narrow these models to two. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/gamielk.ps.gz -- 62.8 Кб -- 12.06.2006
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    9. Unusual Emission near a Compact Source in Orion
    ... and H-H 4, respectively) and some of the compact sources and proplyds identified by O'Dell and collaborators (O'Dell, Wen & Hu ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node23.html -- 19.0 Кб -- 12.06.2006
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    10. A Color Analysis of NICMOS Parallel Observations
    ... The limitation of the Camera 1 and 3 wide-band observations to the F110W and F160W filters should still allow the identification of sources of interest such as infrared luminous galaxies and young galaxies at very high redshift, which as may be seen from ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node28.html -- 19.5 Кб -- 12.06.2006
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