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    51. http://www.arcetri.astro.it/~sperello/EEPpapz2-4.pdf
    ... of the UV linear polarization in RG at high redshift should be possible in the future with the coming generation of giant optical telescopes [35­37], and would narrow the constraint on to a level smaller than what is now possible with RG and CMB ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/EEPpapz2-4.pdf -- 173.4 Кб -- 12.08.2009
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    52. http://www.arcetri.astro.it/~sperello/main.pdf
    ... radio polarization measurements of RGs and quasars, by more accurate UV polarization measurements of RGs with the coming generation of giant optical telescopes, 3,8,26 and by future CMB polarization measurements such as those from Planck 1 and BICEP3 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/main.pdf -- 177.8 Кб -- 17.02.2016
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    53. http://www.arcetri.astro.it/~sperello/JENAM2010.pdf
    ... e.g. by better targeted high resolution radio polarization measurements, by more accurate UV polarization measurements with the coming generation of giant optical telescopes [18, 21, 35], and by future CMB polarimeters such as PLANCK and POLARBEAR [34 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/JENAM2010.pdf -- 136.1 Кб -- 12.01.2012
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    54. http://www.arcetri.astro.it/~sperello/ApJ715_33.pdf
    ... linear polarization in RG at high redshift should be possible in the future with the coming generation of giant optical telescopes (Gilmozzi & Spyromilio 2008; Nelson & Sanders 2008; Johns 2008) and would narrow the constraint on to a level smaller than ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/ApJ715_33.pdf -- 504.8 Кб -- 26.04.2010
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    55. http://www.arcetri.astro.it/~masciadr/public.html
    ... 3D optical turbulence above San Pedro Martir Observatory , Astronomical Telescopes ... a 3D optical turbulence characterization in astronomy, Astronomical Telescopes and ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~masciadr/public.html -- 132.4 Кб -- 01.04.2015
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    56. http://www.arcetri.astro.it/~sperello/arXiv1603.03766.pdf
    ... high resolution radio polarization measurements of RGs and quasars, by more accurate UV polarization measurements of RGs with the coming generation of giant optical telescopes, 7,12,38 and by future CMB polarization measurements such as those from BICEP3 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/arXiv1603.03766.pdf -- 208.3 Кб -- 15.03.2016
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    57. http://www.arcetri.astro.it/~ferruzzi/SPIE_lbt_wavefrontsensor.pdf
    ... have not to conjugate the telescope pupil to the DM in the optical train of the WFS ... Binocular Telescope", Proc. SPIE, Vol. 4007, p. 461-469, (2000) Adaptive Optical ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~ferruzzi/SPIE_lbt_wavefrontsensor.pdf -- 413.4 Кб -- 22.08.2002
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    58. Youngest Brown Dwarf Yet in Multiple Stellar System (ESO Press Release 16/00)
    ... The lines emerging from the bright image are caused by optical reflection in the telescope. ... optical image was taken by ESO staff on 21 February 2000 during a technical test period ( [4] ) with the FORS-2 (FOcal Reducer ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/phot-17a-00-normal.html -- 11.9 Кб -- 29.03.2002
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    59. LonGSp: A NEAR INFRA-RED SPECTROMETER
    ... The mirros D and E are a cassegrain system (f/20) that collimates the optical beam coming from the telescope. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/publ/ucla.html -- 5.7 Кб -- 16.02.2000
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    60. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/ghostly.txt
    ... The colorful rays of light at the upper right, pointing back to the star, are an optical phenomenon produced within the telescope, and are not real. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/ghostly.txt -- 5.6 Кб -- 30.01.2001
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