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    11. Discovery and Analysis of 21 ѕ®m Feature Sources in the Magellanic Clouds
    ... Two of the four spectra without the 21 ѕ®m feature have a very strong feature near 11 ѕ®m, similar to a feature observed in some carbon-rich planetary nebulae (PNe) in the LMC. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011ApJ...735..127V.html -- 5.0 Кб -- 21.01.2016
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    12. http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf
    ... e (3) four- quadrant pha se ma sks (4QPMs) at 10.65, 11.4, & 15.5 µm (24'' x 24''), and a Lyot coronagraph at 23 µm (30'' x 30 ... MRS Continuum Sensitivit y 4QPM's! (24" x 24")! 10.65 µm! 11.4 µm! 15.5 µm! Lyot! (30" x 30")! 23 µm! Imager! (74" x 113 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf -- 1576.4 Кб
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    13. Mid Infrared Instrument
    ... 5-28.3 m. The four integral field units (IFUs) divide the spectral window as follows: (1A) 4.96-7.77 m, (1B) 7.71-11.90 m, (2A) 11.90-18.35 m, and (2B) 18.35-28.30 m. As in the figure above, the IFUs provide four simultaneous and overlapping fields of ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/jwst/instruments/miri/instrumentdesign/mrs -- 20.1 Кб -- 11.04.2016
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    14. ISRs
    ... M. Robberto 11 May 2005 . ... M. Stiavelli, M. Robberto 11 May 2003 . ... M. Giavalisco 11 Oct 2002 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs -- 92.3 Кб -- 10.04.2016
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    15. YAE Past Events
    ... At 11:45 a.m., students and parents were led to the Johns Hopkins University Physics ... At 11:30 a.m., the students returned to the auditorium for a wrap-up. ... The day?s session ended at 11:30 a.m. Photos Engineering Club Spring 2013 Session ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/youthae/events/past-events -- 75.3 Кб -- 11.04.2016
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    16. http://www.stsci.edu/~mperrin/pdfs/Poster_2006_CambridgeDisks_PDS144.pdf
    ... Gemini MICHELLE blue=7.9µm green=11.7µm red=18.5µm PAHs PAHs Silicates Keck NIRC2+AO ... emission several times continuum visible in the 3.3, 7.7, 8.6, and 11.2 µm PAH bands ...
    [ Текст ]  Ссылки http://www.stsci.edu/~mperrin/pdfs/Poster_2006_CambridgeDisks_PDS144.pdf -- 2507.1 Кб -- 06.07.2008
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    17. http://www.stsci.edu/~golim/papers/golimowski2000.pdf
    ... show a linear trend with a slope of 11.3 m s~1 yr~1, which is consistent with these ... trend with a linear slope of 11.3 ^ 0.8 m s~1 yr~1 (Cumming, Marcy, & Butler 1999 ...
    [ Текст ]  Ссылки http://www.stsci.edu/~golim/papers/golimowski2000.pdf -- 237.4 Кб -- 05.05.2004
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    18. NStars1A: Photometric searches - 2MASS and optical colours
    ... c1.7). a hodge-podge of 30 red stars: WOH S 11, listed as an ``M-type star'' (no cross-references) in SIMBAD - an OH maser ... G180-11 = 1RXS J155532.2+351207, M V =13.11, d=13+/-3.9 pc (spec. parallax), Sp=M4.5; . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/nstarsu3.html -- 14.9 Кб -- 08.06.2007
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    19. Science Results from Pan-STARRS1
    ... Registration Ends: 5/23/14 at 11:59: p.m., EST. ... Talk Abstract Submittal Ends: Friday, May 31, 2014, at 11:59:59 p.m., EST . ... Poster Submittal Ends: Friday May 31, 2014, at 11:59:59 p.m., EST . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/panstarrs1 -- 15.4 Кб -- 10.04.2016
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    20. http://www.stsci.edu/ftp/science/goods.save/Internal/Science/agn/telecons/2002-07-11.agenda
    ... 7bit X-YaleITSMailFilter: Version 1.0c (attachment(s) not renamed) A reminder that we will have a telecon Thursday at 11 a.m. EST 818 393 5392 (direct long-distance dial, from anywhere) or 800 367 5754 [pause] 575 [pause] 35392 (toll-free, within USA ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/science/goods.save/Internal/Science/agn/telecons/2002-07-11.agenda -- 4.7 Кб -- 12.02.2003
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