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: http://www.apo.nmsu.edu/35m_operations/35m_manual/General_Information/Spectra/Grim/Grim_Line_Comparison_Plots.html
Дата изменения: Thu Jul 22 19:46:02 2004 Дата индексирования: Sun Apr 10 10:10:03 2016 Кодировка: Поисковые слова: ion drive |
Astrophysical Research ConsortiumApache Point Observatory3.5m Telescope - GrIm II |
GrIm II | GrIm II Information |
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Filter | f/5 | f/10 | f/20 |
J | postscript | postscript | postscript |
H | postscript | postscript | postscript |
K | postscript | postscript | postscript |
K' | postscript | postscript | postscript |
Ks | postscript |
For the moment, these line identifications are tentative. The low resolution of GRIM yields broad lines that make it difficult to distinguish blends, so these are the best guesses. They are backed by dispersion solutions for line spectra with rms values of only a couple Angstroms, but in the case of blends, specific lines may not be properly identified. If you use these charts and find any errors, please contact the Observing Specialists. More properly-labeled plots will follow once the ID's are confirmed.