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    1. First Images and Spectra from ISAAC on UT1 (ESO Press Release 19/98)
    ... of three exposures through Z (centred at 0.90 m), H (1.65 m) and Ks filters (2.16 m) and with exposure times of 160, 320 and ... system ESO202-G23 made by combining an ISAAC H (1.65 m) exposure with (blue) and R (red) exposures made with the VLT Test ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/RCW38.html -- 16.8 Кб -- 25.05.2001
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    2. LonGSp: Available Filters
    ... Hole . 3792 . EPS . LongPass Filter (1.65-2.55?m) . 4740 . H . Standard Filter H (1.48-1.82?m) . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/doc/filter.html -- 2.8 Кб -- 16.02.2000
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    3. http://www.arcetri.astro.it/~lt/preprints/g3520/g35.ps.gz
    ... We present J(1.25 Їm), H(1.65 Їm), K(2.2 Їm), H 2 (2.125 Їm) and 11.2 Їm infrared images at sub­ arcsec resolution of an area ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/g3520/g35.ps.gz -- 330.2 Кб -- 11.09.2007
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    4. http://www.arcetri.astro.it/~salinari/ELT/Detection%20of%20extrasolar%20planets_final.pdf
    ... 2001) Residual phase power spectrum After AO correction Before AO correction Not corrected by AO AO corrected PSF 20 m telescope =1.65 µm r0()=90 cm =90 cm Airy pattern, (next ennemy) Not corrected halo Aliased error Critical spatial frequency fc=1/Wc=1/2 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~salinari/ELT/Detection%20of%20extrasolar%20planets_final.pdf -- 2897.1 Кб -- 03.11.2003
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    5. http://www.arcetri.astro.it/irlab/instr/amber/docs/llsspe.pdf
    ... 2.1 Spectral coverage · · · · J Band : 0 1.25 µm 0.3 µm H Band : 0 1.65 µm 0.35 µm K Band : 0 2.2 µm 0.4 µm Total coverage 1.1 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/irlab/instr/amber/docs/llsspe.pdf -- 129.2 Кб -- 23.09.2006
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    6. http://www.arcetri.astro.it/~salinari/GSF/Wavefront%20Control.pdf
    ... 2001) Residual phase power spectrum After AO correction Before AO correction Not corrected by AO AO corrected PSF 20 m telescope =1.65 µm r0()=90 cm =90 cm Airy pattern, (next ennemy) Aliased error Not corrected halo Critical spatial frequency fc=1/Wc=1/2 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~salinari/GSF/Wavefront%20Control.pdf -- 1770.4 Кб -- 27.11.2003
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    7. http://www.arcetri.astro.it/~lt/preprints/nirsur2/nirsur2.ps.gz
    ... All the sources were observed in J, H and K (1:25 Їm, 1:65 Їm and 2:2 Їm respectively) NIR broad bands using the Las Campanas NIR camera (Persson et al. 1992) equipped with a NICMOS3 256\Theta256 HgCdTe array detector. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/nirsur2/nirsur2.ps.gz -- 602.4 Кб -- 11.09.2007
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    8. http://www.arcetri.astro.it/~lt/preprints/oribar/oribar.ps.gz
    ... H, and K broad band filters (centered at 1.25, 1.65, and 2.2 Їm, respectively) and in the Brfl narrow band filter (– = 2:166 Їm ... LONGSP Observations J (1.25Їm), H(1.65 Їm), and K (2.2Їm) band spectra of the Orion Bar were obtained using the LonGSp ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/oribar/oribar.ps.gz -- 349.5 Кб -- 11.09.2007
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    9. http://www.arcetri.astro.it/~sperello/MNRAS419_3505.pdf
    ... the 2MASS which lists J -, H - and K -band (total) magnitudes for all of our galaxies (J = 1.25 µm, H = 1.65 µm, K = 2.17 µm ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/MNRAS419_3505.pdf -- 1150.8 Кб -- 23.01.2012
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    10. http://www.arcetri.astro.it/~fmassi/papers/rcw79.pdf
    ... ESO-NTT near-IR imaging Images in the J (1.25 µm), H (1.65 µm), and KS (2.2 µm) near-infrared bands were obtained on the nights of 14 and 15 February 2003 with the SofI camera at the ESO New Technology Telescope (NTT). ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~fmassi/papers/rcw79.pdf -- 2419.8 Кб -- 13.09.2005
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