Search

9 Feb 2022: 2 and apply it to test cases inSec. 3 to demonstrate its behaviour and performance. ... Fig. 4 illustrates the fitting procedure applied to the three test casesfrom Sec.

30 May 2022: 1 (while such a test has, to our knowledge,not been conducted for R23).

29 Sep 2022: We will test this with simple modelsthat parameterise the surface density distribution of dust as a func-tion of the radial distance from the star. ... Albeitwith less significant fits in additional tests, i.e., poorer 𝜒2 andBICvalues, and visibly

24 May 2022: DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style in AASTeX62. The JWST Early Release Science Program for the Direct Imaging & Spectroscopyof Exoplanetary Systems. Sasha Hinkley ,1 Aarynn L. Carter ,2 Shrishmoy Ray ,1 Andrew Skemer,2

14 Feb 2022: We also test a different more physically moti-vated model for releasing the CO and assume it comes from theslow heating provided by the Sun over long timescales, whichwarms up large ... 2017, 2019) is valid for the KB (Model 1).Second, we test a more

25 Feb 2022: Posteriorprobability distributions of the model parameters are explored withtheemceepackage(Foreman-Mackeyetal.2013),animplementationof theMarkovChainMonteCarlomethod inPython.We initiate ourmodels near the solutions of previous test runs.

25 Oct 2022: DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style in AASTeX63. ALMA Observations of the HD 110058 debris diskANTONIO S. HALES,1,2 SEBASTIÁN MARINO,3,4 PATRICK D. SHEEHAN,5,2 SILVIO ULLOA,6 SEBASTIÁN PÉREZ,7,8,9 LUCA MATRÀ,10,11.

18 Apr 2022: Initial tests had shown that having thereference wavelength between 15 and 20 µm resulted in com-parable detection yields, but that shorter (e.g., 10 µm) or longer(e.g., 25