Stellar pulsation and granulation as noise sources in exoplanet transit spectroscopy in the ARIEL space mission
Subhajit Sarkar, Ioannis Argyriou, Bart Vandenbussche, Andreas, Papageorgiou, Enzo Pascale

TL;DR
This study assesses how stellar pulsations and granulation noise affect exoplanet transit spectroscopy with the ARIEL space telescope, finding minimal impact in the infrared but potential significance in the visual range, especially for certain targets.
Contribution
The paper provides a simulation-based analysis of stellar variability noise sources for ARIEL, quantifying their impact across different wavelengths and target types.
Findings
Stellar noise has negligible impact in 1.95-7.8 μm range compared to photon noise.
In the visual range, stellar noise contribution increases but remains relatively small.
Impact is more significant for planets with low atmospheric scale height and long transits around bright stars.
Abstract
Stellar variability from pulsations and granulation presents a source of correlated noise that can impact the accuracy and precision of multi-band photometric transit observations of exoplanets. This can potentially cause biased measurements in the transmission or emission spectrum or underestimation of the final error bars on the spectrum. ARIEL is a future space telescope and instrument designed to perform a transit spectroscopic survey of a large sample of exoplanets. In this paper we perform simulations to assess the impact of stellar variability arising from pulsations and granulation on ARIEL observations of GJ 1214b and HD 209458b. We take into account the correlated nature of stellar noise, quantify it, and compare it to photon noise. In the range 1.95-7.8 \textmu m, stellar pulsation and granulation noise has insignificant impact compared to photon noise for both targets. In…
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