A new generation multi-object high throughput Doppler instrument for a planet survey at the SDSS telescope

Jian Ge, Xiaoke Wan, Bo Zhao, Abishek Hariharan, Suvrath Mahadevan, Julian Van Eyken, Pencheng Guo, Dan McDavitt, Curtis DeWitt, Roger Cohen, Scott W. Fleming, Stephen Kane, Justin Crepp, Stuart Shaklan

Research output: Chapter in Book/Report/Conference proceedingConference contribution

3 Citations (Scopus)

Abstract

We report the design of a new generation multi-object high throughput Doppler instrument and first light results at the Sloan Digital Sky Survey (SDSS) telescope. This instrument, capable of simultaneously monitoring 60 stars for planet detection, is called the W.M. Keck Exoplanet Tracker (or Keck ET) thanks to the generous gift from the W.M. Keck Foundation. It is designed for a planet survey around hundreds of thousands of stars with V =8-13 for detecting tens of thousands of planets in 2006-2020. The Doppler precision is between 3-25 m/s depending on the star magnitude. We also report a new planet detected with a prototype single object version ET instrument at the KPNO Coude Feed/2.1 m telescopes. The extrasolar planet, ET-1 (HD 102195b), has a minimum mass of 0.49 Jupiter masses and orbits a V = 8.1 G8V star with a 4.1 day period. The planet was identified using the Coude Feed 0.9 meter telescope in spring 2005. This is the first time an extrasolar planet around a star fainter than V=8 magnitude has been discovered with an under 1 meter size astronomical telescope and Doppler instrument. This planet discovery is possible due to the extremely high throughput of the instrument, 49% measured from the fiber output end to the detector.

Original languageEnglish (US)
Title of host publicationGround-based and Airborne Instrumentation for Astronomy
Volume6269 II
DOIs
StatePublished - Oct 9 2006
EventGround-based and Airborne Instrumentation for Astronomy - Orlando, FL, United States
Duration: May 25 2006May 29 2006

Other

OtherGround-based and Airborne Instrumentation for Astronomy
CountryUnited States
CityOrlando, FL
Period5/25/065/29/06

Fingerprint

Planets
Doppler
Telescopes
High Throughput
Telescope
planets
Star
Stars
Throughput
telescopes
stars
extrasolar planets
Extrasolar Planets
Extrasolar planets
Antenna feeders
Astronomical Telescopes
planet detection
Exoplanets
Jupiter (planet)
Orbit

All Science Journal Classification (ASJC) codes

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

Ge, J., Wan, X., Zhao, B., Hariharan, A., Mahadevan, S., Van Eyken, J., ... Shaklan, S. (2006). A new generation multi-object high throughput Doppler instrument for a planet survey at the SDSS telescope. In Ground-based and Airborne Instrumentation for Astronomy (Vol. 6269 II). [62692E] https://doi.org/10.1117/12.670856
Ge, Jian ; Wan, Xiaoke ; Zhao, Bo ; Hariharan, Abishek ; Mahadevan, Suvrath ; Van Eyken, Julian ; Guo, Pencheng ; McDavitt, Dan ; DeWitt, Curtis ; Cohen, Roger ; Fleming, Scott W. ; Kane, Stephen ; Crepp, Justin ; Shaklan, Stuart. / A new generation multi-object high throughput Doppler instrument for a planet survey at the SDSS telescope. Ground-based and Airborne Instrumentation for Astronomy. Vol. 6269 II 2006.
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abstract = "We report the design of a new generation multi-object high throughput Doppler instrument and first light results at the Sloan Digital Sky Survey (SDSS) telescope. This instrument, capable of simultaneously monitoring 60 stars for planet detection, is called the W.M. Keck Exoplanet Tracker (or Keck ET) thanks to the generous gift from the W.M. Keck Foundation. It is designed for a planet survey around hundreds of thousands of stars with V =8-13 for detecting tens of thousands of planets in 2006-2020. The Doppler precision is between 3-25 m/s depending on the star magnitude. We also report a new planet detected with a prototype single object version ET instrument at the KPNO Coude Feed/2.1 m telescopes. The extrasolar planet, ET-1 (HD 102195b), has a minimum mass of 0.49 Jupiter masses and orbits a V = 8.1 G8V star with a 4.1 day period. The planet was identified using the Coude Feed 0.9 meter telescope in spring 2005. This is the first time an extrasolar planet around a star fainter than V=8 magnitude has been discovered with an under 1 meter size astronomical telescope and Doppler instrument. This planet discovery is possible due to the extremely high throughput of the instrument, 49{\%} measured from the fiber output end to the detector.",
author = "Jian Ge and Xiaoke Wan and Bo Zhao and Abishek Hariharan and Suvrath Mahadevan and {Van Eyken}, Julian and Pencheng Guo and Dan McDavitt and Curtis DeWitt and Roger Cohen and Fleming, {Scott W.} and Stephen Kane and Justin Crepp and Stuart Shaklan",
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Ge, J, Wan, X, Zhao, B, Hariharan, A, Mahadevan, S, Van Eyken, J, Guo, P, McDavitt, D, DeWitt, C, Cohen, R, Fleming, SW, Kane, S, Crepp, J & Shaklan, S 2006, A new generation multi-object high throughput Doppler instrument for a planet survey at the SDSS telescope. in Ground-based and Airborne Instrumentation for Astronomy. vol. 6269 II, 62692E, Ground-based and Airborne Instrumentation for Astronomy, Orlando, FL, United States, 5/25/06. https://doi.org/10.1117/12.670856

A new generation multi-object high throughput Doppler instrument for a planet survey at the SDSS telescope. / Ge, Jian; Wan, Xiaoke; Zhao, Bo; Hariharan, Abishek; Mahadevan, Suvrath; Van Eyken, Julian; Guo, Pencheng; McDavitt, Dan; DeWitt, Curtis; Cohen, Roger; Fleming, Scott W.; Kane, Stephen; Crepp, Justin; Shaklan, Stuart.

Ground-based and Airborne Instrumentation for Astronomy. Vol. 6269 II 2006. 62692E.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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AU - Guo, Pencheng

AU - McDavitt, Dan

AU - DeWitt, Curtis

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Ge J, Wan X, Zhao B, Hariharan A, Mahadevan S, Van Eyken J et al. A new generation multi-object high throughput Doppler instrument for a planet survey at the SDSS telescope. In Ground-based and Airborne Instrumentation for Astronomy. Vol. 6269 II. 2006. 62692E https://doi.org/10.1117/12.670856