T. M. Schmidt, A. Reiners, M. T. Murphy, G. Lo Curto, C. J. A. P. Martins, P. Huke, E. Blucher
Abstract
High-quality wavelength calibration is crucial for science cases like radial-velocity studies of exoplanets, the search for a possible variation of fundamental constants, and the redshift drift experiment. However, for state-of-the-art spectrographs, it has become difficult to verify the wavelength calibration on sky because no astrophysical source provides spectra with sufficiently stable or accurate wavelength information. We therefore propose to use iodine absorption cells to validate the wavelength calibration. Observing a bright and featureless star through the iodine cell emulates an astrophysical target with exactly known spectral features that can be analysed like any other science target, allowing to verify the wavelength calibration derived from the internal calibration sources and to identify systematics in the data processing. As demonstration, we temporarily installed an I2 absorption cell at ESPRESSO. Employing a full forward modelling approach of the I2 spectrum, including the instrumental line-spread function, we demonstrate wavelength calibration accuracy at the level of a few m s-1. We also show that wavelength measurements do depend on the geometry of the light-injection into the spectrograph fibers. This highlights the importance of probing exactly the same light path as science targets, something not possible with internal calibration sources alone. We also demonstrate excellent radial-velocity stability at the < 20 cm s-1 level in a full end-to-end fashion, from sky to data product. Our study therefore showcases the great potential of absorption cells for the verification and long-term monitoring of the wavelength calibration as well as the unique insights they can provide.
Keywords
instrumentation: spectrographs / methods: data analysis / techniques: spectroscopic / software: data analysis / cosmology: observations
Monthly Notices of the Royal Astronomical Society
Volume 539, Issue 4, Page 18
2025 June
