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18 Oct 2020: ii) Squared coherence programme which tests statistically the correlation between the oscillations in two series. ... dry conditions). Analysis was carried out with the following tests (i) Squared coherence relations: scarlet.

15 Oct 2020: 2017) as a test of its validity. The prescriptionpresented by Cataldi et al. ... For each test population, we calculate, using equations 9 11in Wyatt et al.

17 Nov 2020: Hundreds of brown dwarfs are now known. An ‘acid’ test ofthe sub-stellar nature of these objects is the presence of methane (CH4)absorption features in their near-IR spectrum. ... H-burning stars are fartoo hot to form methane in their atmospheres,

8 Jul 2020: H2. To be consistent with previous studies,we assume µ = 14. From preliminary test runs, we foundthat βt1 and β.

17 Jan 2020: of the twosources, then tests the reference PSFs (doubled using thatbinary model) to find the best-fitting empirical PSF tem-plate, repeated until the same best-fitting PSF template pro-duces ... In order to more robustly test whether the inclina-tion

8 Oct 2020: combination of these twoobservational factors renders the systemsideal tests for planet-disc alignment. ... Specifically, we consider the evolution of planetesimals inthe disc by treating them as test particles that evolve due to secu-lar perturbations

26 Nov 2020: A Kolmogorov-Smirnov test comparing the distribu-tions of singles versus multiples gives a p-value of 40% for Lupusand 51% forLupus andOphiuchus combined.

29 Jun 2020: For this ACA-only fit, and. for the later combined ACA12m fit, we test three dif-. ... Statistical. tests such as the Akaike Information Criterion (AIC). and the Bayesian Information Criterion (BIC) confirm.

30 Jan 2020: MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled using MNRAS LATEX style file v3.0. Population synthesis of exocometary gas around A stars. S. Marino1?, M. Flock1, Th. Henning1, Q. Kral2, L. Matrà3 and M. C. Wyatt41Max Planck Institute

7 Jul 2020: Future imaging ofthe faint debris disc in π Men and precise constraints on the stellar spin orientationwould provide strong tests for these formation scenarios.