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    1. NICMOS Camera 3 Parallel Imaging Observations: Number Counts, Sizes and Red
    ... galaxies have very sub-arcsecond angular sizes at faint apparent magnitudes (e.g ... 3 shows that this excess of counts is dominated by objects with angular sizes < 0 ... This excess is dominated by objects with small angular sizes. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node32.html -- 27.8 Кб -- 12.06.2006
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    2. http://www.stecf.org/documents/isr/ISR_NGST_2002-03.pdf
    ... The angular size of the spoiler determines the area on the sky in which spectra of target objects are contaminated. ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/ISR_NGST_2002-03.pdf -- 748.2 Кб -- 11.05.2006
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    3. http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf
    ... If the angular sizes of these sources may exceed the primary beam size of the ALMA ... some sources, the angular resolution of ALMA is needed to determine angular sizes ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008
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    4. The Astrometric Properties of the NOAO Mosaic Imager
    ... The residuals from the latter fits showed no evidence for the predicted 5th order term, most probably due to a combination of the limited angular size of the individual CCDs, and the precision of the published astrometry. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/davisl.html -- 14.5 Кб -- 12.06.2006
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    5. http://www.stecf.org/conferences/adass/adassVII/reprints/davisl.pdf
    ... residuals from the latter fits showed no evidence for the predicted 5th order term, most probably due to a combination of the limited angular size of the individual CCDs, and the precision of the published astrometry. 2.2. 0.9m Plate Solutions An accurate ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/davisl.pdf -- 84.0 Кб -- 12.06.2006
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    6. http://www.stecf.org/conferences/adass/adassVII/reprints/davisl.ps.gz
    ... the latter fits showed no evidence for the predicted 5th order term, most prob­ ably due to a combination of the limited angular size of the individual CCDs, and the precision of the published astrometry. 2.2. 0.9m Plate Solutions An accurate theoretical ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/davisl.ps.gz -- 73.3 Кб -- 12.06.2006
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    7. The STScI NICMOS Calibration Pipeline
    ... building image mosaics of large angular-size targets . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node9.html -- 27.5 Кб -- 12.06.2006
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    8. http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/strolger04.ps
    ... Alternatively, using the limiting magnitude for the survey, m lim  26 (see x 4.2), the source would have to have an angular size of  > 18 ф in order to have been lit by the Sun at its assumed distance. ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/strolger04.ps -- 1023.9 Кб -- 16.09.2004
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    9. A Posteriori Guidance for Astronomical Images
    ... The image field of view is about of diameter with an angular resolution of 12 arcsec ... drift and of small, random and faster oscillations in X-Y and in angular rotation ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/llebariaa.html -- 16.0 Кб -- 12.06.2006
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    10. http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf
    ... Herschel measurements need follow ups with higher angular resolution imaging ESA-ESO Meeting, Feb 10-11, 2005 UV Visible ... images with ALMA allow a better determination of the size of emission sources ALMA would provide high resolution images to ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf -- 2622.1 Кб -- 04.09.2008
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