... For the H-rich atmosphere looked at a H2O/CH4 absorption features centered at 1.4 µm, H2O at 1.8 µm and 2.7 µm, and CH4 at 4.6 µm. For the H-poor atmosphere we looked at H2O absorption features at 1.4 µm, 1.8 µm and 2.7 µm. Since we aim to calculate the ...
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Ссылки http://www.stsci.edu/jwst/doc-archive/white-papers/JWSTNirspec_BatalhaFinal.pdf -- 717.4 Кб -- 01.03.2014 Похожие документы
... F ig u r e 8 : M a p o f a ll u n s ta b le p ix e ls id e n tifie d a s p a r t o f th is b a d p ix e l s e a r c h . ... Field Observations ib9m0anoq_flt.fits, ib9m0erwq_flt.fits, ib9m0fhoq_flt.fits ib 9 m8 5 d 3 q _ f lt.f its , ib 9 m8 9 t9 q ...
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Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2012-10.pdf -- 668.2 Кб -- 13.07.2012 Похожие документы
... absolute magnitudes (relative to Vega): M V =10.9, M I =9.0, M J =8.0, M H =7.1 mag ... chosen to be randomly distributed in both galaxies and sample a range in 8.0 m flux ... All chosen targets have an 8.0 m flux greater than 2 mJy. ...
... at a distance modulus of (m \Gamma M)=16.8 given the proper reddening correction and ... for Sgr tidal debris to wrap entirely around 360 ffi , if it has a mass of 10 8M fi ...