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    1. Remote Access to Mt. Kent Observatory in Queensland Australia
    ... Mt. Kent weather station . Infrared sky background . Cloud detector data . ... USQ Weather Station in Toowoomba . Australian Region Infrared Satellite Image . ... Meteorological Satellite of Japan Infrared Image . Last update: December 8, 2009 . ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/mtkent/remote/ -- 3.3 Кб -- 11.05.2010
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    2. Mount Kent Observatory Regional Weather
    ... USQ weather station in Toowoomba . Australian region infrared satellite . Meteorological Satellite of Japan . Detailed satellite view of Mt. Kent . ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/mtkent/weather/index.html -- 3.6 Кб -- 24.11.2012
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    3. http://www.astro.louisville.edu/shared_skies/archive/select/messier/m74/20111024/log.txt
    ... exposures Date of observation: 2011-10-25 at 07:03 UTC Sloan filters "g" = blue-green "r" = orange-red "i" = near infrared m74_g_coadd.fits EXPTIME = 5.000000000000E+02 / Maximum equivalent exposure time (s) m74_i_coadd.fits EXPTIME = 7.000000000000E+02 ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/shared_skies/archive/select/messier/m74/20111024/log.txt -- 1.5 Кб -- 21.11.2011
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    4. http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/BUGS
    ... November 29, 2012 ================= Support for Apogee's preflash option is being added to help remove the latent bulk image artifact that is present in images on Kodak sensors when they have been exposed to a bright infrared source. ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/BUGS -- 1.8 Кб -- 29.11.2012
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    5. http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.1/xmccd-4.2.1/BUGS
    ... April 26, 2013 ============== Support for Apogee's preflash option is being added to help remove the latent bulk image artifact that is present in images on Kodak sensors when they have been exposed to a bright infrared source. ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.1/xmccd-4.2.1/BUGS -- 1.6 Кб -- 27.04.2013
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    6. Wide Field Spectral Imager
    ... The Wide Field Spectral Imager ( WISPI ) seen here in the Roll Roof Facility provides visible and near-infrared spectra of the sky across 4 degree fields. ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/moore/wispi/index.html -- 5.5 Кб -- 17.03.2013
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    7. Shared Skies Photo Gallery
    ... Red in this image is actually near infrared through the i' filter, green is from the ... light the CCD camera can sense, from the near ultraviolet through the near infrared ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/gallery/ -- 17.7 Кб -- 08.11.2015
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    8. University of Louisville Research Telescope
    ... With efficient well-corrected optics useful from the atmospheric UV cutoff below 380 nm through the near infrared above 2 microns, the 0.18 arcsecond diffraction is achievable for visible light with very short "lucky" exposure times to minimize ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/moore/rc24/ -- 4.7 Кб -- 11.05.2010
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    9. http://www.astro.louisville.edu/shared_skies/archive/select/ic/ic348/20121109/ic348_wikipedia_20130415.pdf
    ... Based upon infrared observations using the Spitzer Space Telescope, about half of the stars in the cluster have a circumstellar disk, of which 60% are thick or primordial disks.[ ...
    [ Текст ]  Ссылки http://www.astro.louisville.edu/shared_skies/archive/select/ic/ic348/20121109/ic348_wikipedia_20130415.pdf -- 177.0 Кб -- 15.04.2013
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    10. Wispi Design Notes
    ... The Milton Roy diffraction grating is blazed for the near infrared. It may be used in the second order for shorter wavelengths. ...
    [ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/moore/wispi/wisp_const.html -- 8.6 Кб -- 10.05.2010
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