Precision Radial Velocities for the Kepler Era
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| Natura: | Artículo científico |
| Lingua: | en |
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Universidad Nacional Autónoma de México
2007
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| _version_ | 1876451813521096704 |
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| author | A. H. Szentgyorgyi |
| author_facet | A. H. Szentgyorgyi |
| contents | Precision Radial Velocities for the Kepler Era A. H. Szentgyorgyi G. Fürész Física, Astronomía y Matemáticas TECHNIQUES: RADIAL VELOCITY INSTRUMENTATION: SPECTROGRAPHS STARS: PLANETARY SYSTEMS: PROTOPLANETARY DISKS The Kepler Mission will provide photometry for 100,000 dwarfs to m 14 in search of terrestrial-sized exoplanetsin a northern field 107 degrees square. This search requires massive photometric and spectroscopicreconnaissance both to identify the dwarfs from the millions of stars in the field and post facto to weed outimpostor binaries and blends that mimic transiting earth-size exoplanets. In this paper we discuss several newinstruments that the Smithsonian Astrophysical Observatory has recently commissioned or is building that arecornerstones of this spectroscopic follow-up: the Hectochelle and TRES 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102826 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.28 |
| format | Artículo científico |
| id | redalyc_57102826 |
| institution | Redalyc |
| language | en |
| publishDate | 2007 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Precision Radial Velocities for the Kepler Era A. H. Szentgyorgyi Física, Astronomía y Matemáticas TECHNIQUES: RADIAL VELOCITY INSTRUMENTATION: SPECTROGRAPHS STARS: PLANETARY SYSTEMS: PROTOPLANETARY DISKS Precision Radial Velocities for the Kepler Era A. H. Szentgyorgyi G. Fürész Física, Astronomía y Matemáticas TECHNIQUES: RADIAL VELOCITY INSTRUMENTATION: SPECTROGRAPHS STARS: PLANETARY SYSTEMS: PROTOPLANETARY DISKS The Kepler Mission will provide photometry for 100,000 dwarfs to m 14 in search of terrestrial-sized exoplanetsin a northern field 107 degrees square. This search requires massive photometric and spectroscopicreconnaissance both to identify the dwarfs from the millions of stars in the field and post facto to weed outimpostor binaries and blends that mimic transiting earth-size exoplanets. In this paper we discuss several newinstruments that the Smithsonian Astrophysical Observatory has recently commissioned or is building that arecornerstones of this spectroscopic follow-up: the Hectochelle and TRES 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102826 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.28 |
| title | Precision Radial Velocities for the Kepler Era |
| topic | Física, Astronomía y Matemáticas TECHNIQUES: RADIAL VELOCITY INSTRUMENTATION: SPECTROGRAPHS STARS: PLANETARY SYSTEMS: PROTOPLANETARY DISKS |
| url | https://www.redalyc.org/articulo.oa?id=57102826 |