... S aturation based on 13% of flux falling within the brightest pixel for 8 µm and 13 % x (8 µm/)2 for > 8 µm. 8 µ Jy Theamera.as.arizona.edu/MIRI/ Instrument (MIRI) ht tp://irc Mid-Infrared Operated for NASA by AURA ht tp://w w w.stsci.edu/jwst ...
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Ссылки http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf -- 1576.4 Кб Похожие документы
... Example from UKIRT IRCAM: Band Sky (mag/arcsec2) Sky (ADU/sec/pix) J (1.2µm) 15.7 6 H (1.6µm) 13.6 40 K (2.2µm) 13.0 40 L' (3.5µm) 3.4 78000 M (4.7µm) 0.5 170000 Sky subtraction in thermal IR Requires even more careful treatment than for near-IR. ...
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Ссылки http://www.stsci.edu/hst/training/events/InfraredInstrumentation/IR23Mar00.pdf -- 151.4 Кб -- 23.04.2002 Похожие документы
... 13.0 ST IS E140M + 0.2x0.2 ap e r t u r e R=45,000 -1 -1 STIS/NUV 1600-3200 350 (M) 900 (L) (at 2500) - 13.5 1150-1775(M) 1150-1700 1230-2050(L) 2800 (M) 2400 (L) (at 1300) 400 (M) 1700 (L) (at 1300) log Flux (erg cm -2 sec - 14.0 C OS G13 0M R~20,000- 24 ...
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Ссылки http://www.stsci.edu/hst/cos/documents/COS_Brochure_18apr2007.pdf -- 1750.1 Кб -- 23.04.2007 Похожие документы
... the EBL measured by DIRBE at the same wavelength is (13.3±2.8) nW m-2 sr-1 [5 ... dark ages are also expected with intensities at the level of 10-5 nW m-2 sr-1 [13 ... smaller than the clustering scale of typical 1012-13M dark matter halos at z > 3 ...