Abstract
The ‘Far InfraRed and Submillimetre Telescope’, (FIRST), is the fourth cornerstone mission in the European Space Agency (ESA) science programme. It will perform photometry and spectroscopy in the far infrared and submillimetre part of the spectrum, covering approximately the 60–670 μm range. FIRST will carry a 3.5 metre passively cooled telescope, to be supplied by NASA, and house a science payload complement of two cameras/medium resolution spectrometers (PACS and SPIRE) and a very high resolution heterodyne spectrometer (HIFI) in a superfluid helium cryostat. FIRST will be placed in a transfer trajectory towards its operational orbit around the Earth-Sun L2 point by an Ariane 5 (shared with Planck) in early 2007. Once operational FIRST will offer a minimum of 3 years of routine observations; roughly 2/3 of the available observing time is open to the general astronomical community through a standard competitive proposal procedure.
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References
Pilbratt G.L. 1998, ‘The FIRST ESA Cornerstone Mission’ Proc. of SPIE 3356, 452–461
Schupp J., Mo\bacher B., Seidel A. 1998, ‘The FIRST PLM based on a HeII cryostat’ Proc. of 1998 Space Cryogenics Workshop, ESA WPP-157, 107–110
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Bauer O.H., Estaria P., King K.J., Pilbratt G., Robson A., Roelfsema, P.R., Schaap H. 1998, ‘FIRST Ground Segment and Science Operations Concept’ Proc. of SPIE 3349, 312–318
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© 2000 Springer-Verlag Berlin Heidelberg
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Pilbratt, G.L. (2000). The FIRST Mission. In: Lemke, D., Stickel, M., Wilke, K. (eds) ISO Surveys of a Dusty Universe. Lecture Notes in Physics, vol 548. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-45553-1_51
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DOI: https://doi.org/10.1007/3-540-45553-1_51
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