Published August 1, 2018
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Overview of the spectrometer optical fiber feed for the habitable-zone planet finder
Abstract
The Habitable-zone Planet Finder (HPF) is a highly stabilized fiber fed precision radial velocity (RV) spec- trograph working in the Near Infrared (NIR): 810 – 1280 nm. In this paper we present an overview of the preparation of the optical fibers for HPF. The entire fiber train from the telescope focus down to the cryostat is detailed. We also discuss the fiber polishing, splicing and its integration into the instrument using a fused silica puck. HPF was designed to be able to operate in two modes, High Resolution (HR- the only mode mode currently commissioned) and High Efficiency (HE). We discuss these fiber heads and the procedure we adopted to attach the slit on to the HR fibers.
Additional Information
© 2018 Society of Photo-optical Instrumentation Engineers (SPIE). This work was partially supported by the funding from The Center for Exoplanet and Habitable Worlds. The Center for Exoplanet and Habitable Worlds is supported by The Pennsylvania State University, The Eberly College of Science, and The Pennsylvania Space Grant Consortium. We acknowledge support from NSF grants, AST1006676, AST1126413, AST1310885, and the NASA Astrobiology Institute (NNA09DA76A) in our pursuit of precision radial velocities in NIR. SK acknowledges support from the Braddock fellowship. GKS acknowledges support from the Leifur Eiriksson foundation.Attached Files
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Additional details
- Eprint ID
- 92162
- Resolver ID
- CaltechAUTHORS:20190109-101641795
- Pennsylvania State University
- Eberly College of Science
- Pennsylvania Space Grant Consortium
- AST-1006676
- NSF
- AST-1126413
- NSF
- AST-1310885
- NSF
- NNA09DA76A
- NASA
- Leifur Eiriksson Foundation
- NASA Earth and Space Science Fellowship
- Robert A. Millikan Fellowship
- NASA Sagan Fellowship
- Created
-
2019-01-09Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 10702