Abstract We introduce the Disk Substructures at High Angular Resolution Project (DSHARP),
one of the initial Large Programs conducted with the Atacama Large Millimeter/submillimeter …

Rings are the most frequently revealed substructure in Atacama Large Millimeter/
submillimeter Array (ALMA) dust observations of protoplanetary disks, but their origin is still …

A large fraction of the protoplanetary disks observed with ALMA display multiple well-
defined and nearly perfectly circular rings in the continuum, in many cases with substantial …

Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) used ALMA
to map the 1.25 mm continuum of protoplanetary disks at a spatial resolution of∼ 5 au. We …

Abstract The Disk Substructures at High Angular Resolution Project (DSHARP) provides a
large sample of protoplanetary disks with substructures that could be induced by young …

Abstract We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …

Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous
imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a …

Since the discovery of the multiring structure of the HL Tau disk, ALMA data suggest that the
dust continuum emission of many, if not all, protoplanetary disks consists of rings and gaps …

Context. Imaged in the gap of a transition disk and found at a separation of about 195 mas (~
22 au) from its host star at a position angle of about 155°, PDS 70 b is the most robustly …

We present the highest spatial resolution Atacama Large Millimeter/submillimeter Array
(ALMA) observations to date of the Class I protostar GY 91 in the ρ Ophiuchus L1688 …