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Cited article:

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Recent progress with observations and models to characterize the magnetic fields from star-forming cores to protostellar disks

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The Ophiuchus DIsc Survey Employing ALMA (ODISEA) – III. The evolution of substructures in massive discs at 3–5 au resolution

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Dust Polarization toward Embedded Protostars in Ophiuchus with ALMA. III. Survey Overview

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The Co-evolution of Disks and Stars in Embedded Stages: The Case of the Very-low-mass Protostar IRAS 15398–3359

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Rotationally-supported disks around Class I sources in Taurus: disk formation constraints

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ALMA observations of the kinematics and chemistry of disc formation

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