Data from "Turbulence in protoplanetary disks: A systematic analysis of dust settling in 33 disks"

Continuum images, calibrated visibilities, and main imaging parameters associated with Villenave et al. “Turbulence in protoplanetary disks: A systematic analysis of dust settling in 33 disks”, A&A, arxiv

The raw data are available on the ALMA archive (https://almascience.eso.org/aq/) under projects 2013.1.00498.S, 2015.1.00888.S, 2016.1.00484.L, 2016.1.00460.S, 2016.1.00545.S, 2016.1.00771.S, 2016.1.01164.S, 2016.1.01205.S, 2016.1.01239.S, 2016.1.01370.S, 2017.A.00006.S, 2017.1.01151.S, 2017.1.01167.S, 2017.1.01460.S, 2018.1.00028.S, 2018.A.00030.S, 2018.1.00689.S, 2018.1.00958.S, 2018.1.01255.S, 2018.1.01230.S, 2018.1.01755.S, 2019.1.01051.S (see Table A.1. and Table A.2. of Villenave et al. for correspondence between source and project ID).

The models of the paper are available at https://doi.org/10.5281/zenodo.14056832

Contents

Scripts:

reduction_utils.py: Set of functions for imaging script. The main functions are 1/ Definition of the cleaning parameters for all sources, 2/ Rotate and save an image, 3/ Deproject and save an image, 4/ Get the wedge cut in an image 

script_clean_data.py: Script producing the data images of all sources. From the visibilities, generates clean image, rotate the image to have the major axis along the horizontal direction, deproject the image, and obtains the wedge cut along the major axis direction.

To be executed in CASA 5.1.1-5 in order to reproduce the images of the paper.

Calibrated measurement sets:

*_continuum.ms.zip

Reduced data images:

*_continuum.fits

For the disks included in the DSHARP survey (AS209, DoAr25, DoAr33, Elias20, Elias24, Elias27, GWLup, HD142666, HD143006, HD163296, MYLup, SR4, Sz114, WaOph6, WSB52), the data are available at https://bulk.cv.nrao.edu/almadata/lp/DSHARP/

For GM Aur, the data are available at https://zenodo.org/records/3628656

The data of RY Tau come from Ribas et al. 2024, PDS 70 from Benisty et al. 2021, DM Tau from Hashimoto et al. 2021, and DL Tau, DS Tau, GO Tau, and MWC 758 come from Long et al. 2018.