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    1. ASNPHOT (Nov98) --- nictools --- ASNPHOT (Nov98)
    ... asnphot -- plot magnitude as function of subpixel position asnphot association . association . ... parameters passed to qphot . datfile . optional ASCII output file which lists subpixel position and magnitude. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/asnphot.hlp.html -- 2.3 Кб -- 06.06.2006
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    2. No Title
    ... It was constructed from 2 minute exposures taken on 22nd May 1998 and reaches a limiting B magnitude of about 24 in 0.53 arcsec seeing. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/nicmosvlt.html -- 4.0 Кб -- 12.06.2006
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    3. The Stellar Population in the NICMOS Parallel Fields
    ... and F160 W magnitudes have been translated into the Vegamag system magnitudes by ... magnitudes brighter than 19, while it increases up to 0.5 down to the limiting ... magnitude of 23 in J and 22.5 in H. Their distribution peaks at about 20 in J and H ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node21.html -- 18.2 Кб -- 12.06.2006
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    4. ST-ECF IRAF package
    ... Examine images in an association . ASNPHOT . - . Plot magnitude as function of subpixel position . MAKEASN . - . Group images in associations . MAKEFLAT . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/index.php -- 6.5 Кб -- 09.04.2016
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    5. The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
    ... To construct the colour-magnitude diagrams we have used aperture photometry of this ... in the NICMOS image, could be affecting the magnitudes of some of the stars and ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node27.html -- 15.4 Кб -- 12.06.2006
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    6. Methods for Structuring and Searching Very Large Catalogs
    ... Create small regions of about 100 sq. arcmin sort all objects within these regions by magnitude create an histogram index of these regions, i.e., pointer to first object and number of objects within a magnitude bin. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/wiceneca.html -- 12.4 Кб -- 12.06.2006
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    7. http://www.stecf.org/documents/isr/ISR_NGST_2002-02.pdf
    ... and stars (for three Galactic latitudes) in a 12 arcmin2 FoV per unit magnitude as a function of the K magnitude (Vega system ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/ISR_NGST_2002-02.pdf -- 534.3 Кб -- 11.05.2006
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    8. NICMOS Camera 3 Parallel Imaging Observations: Number Counts, Sizes and Red
    ... magnitudes where possible and to correct these to 2 '' aperture magnitudes using an ... magnitude range of interest this transformation is well approximated by a simple ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node32.html -- 27.8 Кб -- 12.06.2006
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    9. http://www.stecf.org/conferences/adass/adassVII/reprints/wiceneca.pdf
    ... How to make the Dream Reality Create small regions of about 100 sq. arcmin sort all ob jects within these regions by magnitude create an histogram index of these regions, i.e., pointer to first ob ject and number of ob jects within a magnitude bin. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/wiceneca.pdf -- 84.0 Кб -- 12.06.2006
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    10. NICMOS Observes the Galactic Center
    ... to deredden the stellar population and place the stars on a color magnitude diagram ... be apparent - for example, O8-O9 stars should have an apparent magnitude around K ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node25.html -- 12.9 Кб -- 12.06.2006
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