... 2} Emission line and continuum imaging of the Cone Nebula and M17 with WFC to demonstrate the improved sensitivity and angular resolution of ACS. ...
... By targeting strongly lensed galaxies behind low-redshift galaxy clusters, JWST spectra of sufficiently good quality can be obtained for M 1500 < --16.0 galaxies at z — 7 and for M 1500 < -17.5 galaxies at z — 9. ...
... 15] [16] [17] Johnston, M. 1989a: "Knowledge-Based Telescope Scheduling," in Knowledge-Based Systems in Astronomy, ed. A. Heck and F. Murtagh (Springer-Verlag: 1989) Acknowledgements: The authors are grateful to J. Sponsler, S. Vick, and R. Jackson (STScI ...
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Ссылки http://www.stsci.edu/~miller/papers-and-meetings/90-Expert-Sys-in-Gov/paper.pdf -- 106.5 Кб -- 27.02.2009 Похожие документы
... For example, the S(0) quadrupolar lines at 17.1 µm can be observed with JWST. $ There are many more issues that can be addressed by cometary spectra. ...
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Ссылки http://www.stsci.edu/jwst/doc-archive/white-papers/JWST_Solar_System.pdf -- 518.7 Кб -- 05.02.2013 Похожие документы
... The strongest aromatics are seen at 3.3, 6.2, 7.7, 8.6, 11.3, 12.7, and 17.1 µm and all the aromatics have been identified with C-H and C-C bending and stretching modes of hydrocarbons containing aromatic rings (Tielens 2005). ...
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Ссылки http://www.stsci.edu/~kgordon/papers/PS_files/spitzer_irdiag_aromatics.pdf -- 478.1 Кб -- 19.04.2006 Похожие документы
... For redshifts at z > 2, the corresponding apparent wavelengths are > 6 µm. For GRB models with high mass progenitors, WL finds the flux near maximum light to be essentially identical in this wavelength range or LAB AB6µm17.5 for z 2. ...