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Precision of Radial Velocity Surveys using Multiobject Spectrographs — Experiences with Hectochelle

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Precision Spectroscopy in Astrophysics

Part of the book series: ESO Astrophysics Symposia ((ESO))

Abstract

There are two multiobject spectrographs at the 6.5m MMT telescope (Arizona, USA), sharing the same fiber feed and fiber positioner. A robotic positioner places all 300 fibers over the 600 mm (1 degree wide field [1]) focal surface in five minutes with an accuracy of 25μm or better. The fiber diameter is 250μm, or 1.5 arcsec at the MMT f/5 plate scale. The 30m long fiber run ends in a room accommodating two bench mounted spectrographs, the moderate resolution Hectospec and the high resolution (R=34,000) Hectochelle [2]. As there is no cross disperser, the orders of Hectochelle are separated by interference filters in front of the pseudo-slit, one order being ∼ 150 Å wide. Efficiency peaks at ∼ 7%, at a wavelength ∼ 5200 Å.

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References

  1. Fabricant, D.G., et al. Proceedings of the SPIE, 5492, 767 (2004)

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  2. Szentgyorgyi, A. H., Cheimets, P., Eng, R., Fabricant, D. G., Geary, J. C., Hartmann, L., Pieri, M. R., & Roll, J. B. Proceedings of the SPIE, 3355, 242 (1998)

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© 2008 Springer-Verlag Berlin Heidelberg

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Fűrész, G., Szentgyorgyi, A.H., Meibom, S. (2008). Precision of Radial Velocity Surveys using Multiobject Spectrographs — Experiences with Hectochelle. In: Santos, N.C., Pasquini, L., Correia, A.C.M., Romaniello, M. (eds) Precision Spectroscopy in Astrophysics. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-75485-5_68

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