Direct imaging and spectroscopy of exoplanets with the ELT/HARMONI high-contrast module

¹ Aix Marseille Univ., CNRS, CNES, LAM, Marseille, France
e-mail: mathis.houlle@lam.fr
² European Southern Observatory, Alonso de Córdova 3107, Santiago, Chile
³ Univ. Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France
⁴ Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
⁵ School of Physics and Astronomy, University of Exeter, Exeter EX4 4QL, UK
⁶ ONERA (Office National d’Etudes et de Recherches Aérospatiales), BP 72, 92322 Chatillon, France
⁷ UK Astronomy Technology Centre, Blackford Hill, Edinburgh EH9 3HJ, UK
⁸ École Normale Supérieure, Lyon, CRAL (UMR CNRS 5574), Université de Lyon, Lyon, France
⁹ Center for Space and Habitability, University of Bern, 3012 Bern, Switzerland
¹⁰ Lunar and Planetary Laboratory, University of Arizona, 1629 E. University Blvd., Tucson, AZ 85721, USA

Received: 2 February 2021
Accepted: 26 March 2021

Abstract

Combining high-contrast imaging with medium-resolution spectroscopy has been shown to significantly boost the direct detection of exoplanets. HARMONI, one of the first-light instruments to be mounted on ESO’s future extremely large telescope (ELT), will be equipped with a single-conjugated adaptive optics system to reach the diffraction limit of the ELT in the H and K bands, a high-contrast module dedicated to exoplanet imaging, and a medium-resolution (up to R = 17 000) optical and near-infrared integral field spectrograph. When combined, these systems will provide unprecedented contrast limits at separations between 50 and 400 mas. This paper is aimed at estimating the capabilities of the HARMONI high-contrast module for the direct detection of young giant exoplanets. We use an end-to-end model of the instrument to simulate high-contrast observations performed with HARMONI, based on realistic observing scenarios and conditions. We then analyze these data with the so-called “molecule mapping” technique combined with a matched-filter approach in order to disentangle companions from the host star and tellurics and to increase the signal-to-noise ratio (S/N) of the planetary signal. We detected planets above 5σ at contrasts up to 16 mag and separations down to 75 mas in several spectral configurations of the instrument. We show that molecule mapping allows for the detection of companions up to 2.5 mag fainter compared to state-of-the-art high-contrast imaging techniques based on angular differential imaging. We also demonstrate that the performance is not strongly affected by the spectral type of the host star and we show that we are able to reach close sensitivities for the best three quartiles of observing conditions at Armazones, which means that HARMONI could be used in near-critical observations during 60 to 70% of telescope time at the ELT. Finally, we simulated planets from population synthesis models to further explore the parameter space that HARMONI and its high-contrast module will open up and compare this to the current high-contrast instrumentation.