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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2014/18713
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| Title: | The Potential for Mid-Infrared Astronomy with the Next Generation Space Telescope |
| Authors: | Serabyn, E.
Barsony, M.
Beichman, C.
Koerner, D.
Orton, G.
Ressler, M.
Werner, M.
Xu, C. |
| Issue Date: | 13-Sep-1999 |
| Citation: | NGST Science & Technology Exposition
Hyannis, Massachusetts, USA |
| Abstract: | While the baseline for the Next Generation Space Telescope (NGST) is the 1 to 5 um wavelenght interval, compelling astronomical observations become possible at longer wavelenghts. |
| URI: | http://hdl.handle.net/2014/18713 |
| Appears in Collections: | JPL TRS 1992+
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