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    1. Proposed Facility
    ... Mid-UV spectra of faint QSOs are the way to go, and this means a space mission. ... a successor to the HST, with good spectrographs that work in the UV is what you want ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node22.html -- 3.6 Кб -- 02.10.2012
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    2. NGC 1512 and NGC 1510
    ... Description: A pretty picture of UV (GALEX) and H-alpha emission in the interacting system NGC 1512 & NGC 1510. ... NGC 1512 and NGC 1510 A pretty picture of UV (GALEX) and H-alpha emission in the interacting system NGC 1512 & NGC 1510. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/astronomy/nonRSAA/NGC1512_NGC1510 -- 8.7 Кб -- 11.04.2016
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    3. Proposed Facility
    ... This dust will mop up all the optical and UV light produced by star-forming galaxies, and re-radiate it in the far-IR. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node28.html -- 3.6 Кб -- 02.10.2012
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    4. http://www.mso.anu.edu.au/seminars/abstracts/20141127-1100.html
    ... From their rest-frame UV emission we can estimate individual star formation rates, and study evolution of the star formation rate density with cosmic time. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141127-1100.html -- 4.4 Кб -- 10.04.2016
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    5. Images
    ... Photos of the GMRT January 2005 . GMRT UV Plane (gif animation) . Images taken by the 2002-2003 Summer Scholars on the . SSO 40-inch telescope . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/images.html -- 6.6 Кб -- 02.10.2012
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    6. Research Interests
    ... as group after group has claimed to detect new-born galaxies in the rest-frame UV ... And dust is really extremely good at blocking UV light. ... place in giant molecular clouds, and you won't get very far studying them in the UV ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node18.html -- 5.4 Кб -- 02.10.2012
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    7. http://www.mso.anu.edu.au/seminars/abstracts/20150820-1400.html
    ... Providing access to high cadence near-UV photometry. ... our balloons with small (20 - 30cm) telescopes operating in the near-UV (200 - 300nm ... We will use the balloons to perform a wide-field, high-cadence UV survey. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150820-1400.html -- 4.7 Кб -- 10.04.2016
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    8. Index of /~bessell/FTP/Shob
    ... Name Last modified Size Description . Parent Directory - giants_uv.txt 11-Dec-2002 20:25 3.8K . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Shob/ -- 1.8 Кб -- 10.04.2016
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    9. Research Interests
    ... Note that these absorption-lines occur in the UV: you can only observe this phenomenon in the early universe, where cosmological redshifts shift the relevant absorption-lines into the near-UV or optical. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node21.html -- 5.6 Кб -- 02.10.2012
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    10. Proposed Facility
    ... A space telescope capable of obtaining UV spectra would be good, for looking at QSO absorption systems at low redshifts (for example, the Ly line disappears into the UV below redshift 1.9). ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/html_dir/firstlight/node25.html -- 3.9 Кб -- 02.10.2012
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