Demonstration of a Near-IR Laser Comb for Precision Radial Velocity Measurements in Astronomy
arXiv:1501.02509 · doi:10.1038/ncomms10436
Abstract
We describe a successful effort to produce a laser comb around 1.55 m in the astronomical H band using a method based on a line-referenced, electro-optical-modulation frequency comb. We discuss the experimental setup, laboratory results, and proof of concept demonstrations at the NASA Infrared Telescope Facility (IRTF) and the Keck-II telescope. The laser comb has a demonstrated stability of 200 kHz, corresponding to a Doppler precision of ~0.3 m/s. This technology, when coupled with a high spectral resolution spectrograph, offers the promise of 1 m/s radial velocity precision suitable for the detection of Earth-sized planets in the habitable zones of cool M-type stars.
References in corpus (8)
- A laser frequency comb that enables radial velocity measurements with a precision of 1 cm s
- High-precision wavelength calibration of astronomical spectrographs with laser frequency combs
- Full Stabilization of a Microresonator based Optical Frequency Comb
- Instrumentation for the detection and characterization of exoplanets
- Astronomical spectrograph calibration with broad-spectrum frequency combs
- Calibrating echelle spectrographs with Fabry-Perot etalons
- Development of Fiber Fabry-Perot Interferometers as Stable Near-infrared Calibration Sources for High Resolution Spectrographs
- Self-referencing a continuous-wave laser with electro-optic modulation
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- Retrieval of Precise Radial Velocities from Near-Infrared High Resolution Spectra of Low Mass Stars
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- Astro-comb calibrator and spectrograph characterization using a turn-key laser frequency comb
- Technical description and performance of the phase II version of the Keck Planet Imager and Characterizer
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