NuAncestor: an artificial satellite-borne star for accurate frequency calibration of ground-based EPRV spectrographs
arXiv:2507.08413 · doi:10.1117/12.3016547
Abstract
The accuracy of state-of-the-art Extreme Precision Radial Velocity (EPRV) spectrographs depends on the access to extremely precise and stable wavelength calibration sources. There are several available calibration sources (e.g., emission lamps, laser frequency combs, reference cavities) that can be used to calibrate an astronomical spectrograph. However, the calibration as it is currently performed is always 'local'. In the proposed talk we will present the NuAncestor concept that proposes an accurate (absolute) and common wavelength calibration for astronomical high-resolution, high-precision spectrographs by embarking an optical frequency comb on-board a satellite equipped with an actively pointing telescope and precision orbitography. This calibration satellite shall be available and serve EPRV spectrographs in all major observatories around the world.
Proceedings of the SPIE conference, Volume 13100, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation VI; 131005W
References in corpus (16)
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- The fundamental constants and their variation: observational status and theoretical motivations
- Spectrally resolved detection of sodium in the atmosphere of HD189733b with the HARPS spectrograph
- Nightside condensation of iron in an ultra-hot giant exoplanet
- Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
- Cosmic dynamics in the era of Extremely Large Telescopes
- Exoplanetary Atmospheres - Chemistry, Formation Conditions, and Habitability
- A giant exoplanet orbiting a very low-mass star challenges planet formation models
- A candidate short-period sub-Earth orbiting Proxima Centauri
- Instrumentation for the detection and characterization of exoplanets
- Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) I. Detection of hot neutral sodium at high altitudes on WASP-49b
- Detection of barium in the atmospheres of the ultra-hot gas giants WASP-76b and WASP-121b
- Broadband near-infrared astronomical spectrometer calibration and on-sky validation with an electro-optic laser frequency comb
- Visible blue-to-red 10 GHz frequency comb via on-chip triple-sum frequency generation
- Constraining fundamental constants of physics with quasar absorption line systems