activity
20172021
most citedThe Ophiuchus DIsc Survey Employing ALMA (ODISEA)-III: the evolution of substructures in massive discs at 3-5 au resolution

129 citations · 214 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.EP202115 cited

A faint companion around CrA-9: protoplanet or obscured binary?

V. Christiaens, M. -G. Ubeira-Gabellini, H. Cánovas +16

Understanding how giant planets form requires observational input from directly imaged protoplanets. We used VLT/NACO and VLT/SPHERE to search for companions in the transition disc…

astro-ph.GA2021

Gaia Early Data Release 3: Structure and properties of the Magellanic Clouds

Gaia Collaboration, X. Luri, L. Chemin +417

We compare the Gaia DR2 and Gaia EDR3 performances in the study of the Magellanic Clouds and show the clear improvements in precision and accuracy in the new release. We also show…

astro-ph.EP2020129 cited

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

Lucas A. Cieza, Camilo González-Ruilova, Antonio S. Hales +15

We present 1.3 mm continuum ALMA long-baseline observations at 3-5 au resolution of 10 of the brightest discs from the Ophiuchus DIsc Survey Employing ALMA (ODISEA) project. We ide…

astro-ph.EP2020

A Tale of Two Transition Disks: ALMA long-baseline observations of ISO-Oph 2 reveal two closely packed non-axisymmetric rings and a 2 au cavity

Camilo González-Ruilova, Lucas A. Cieza, Antonio S. Hales +12

ISO-Oph 2 is a wide-separation (240 au) binary system where the primary star harbors a massive (M 40 M) ring-like disk with a dust cavity 50 au in r…

astro-ph.SR2019

Gaia DR2 white dwarfs in the Hercules stream

Santiago Torres, Carles Cantero, María E. Camisassa +5

We analyzed the velocity space of the thin and thick-disk Gaia white dwarf population within 100 pc looking for signatures of the Hercules stellar stream. We aimed to identify thos…

astro-ph.EP201948 cited

A census of Oph candidate members from Gaia DR2

H. Cánovas, C. Cantero, L. Cieza +6

The Ophiuchus cloud complex is one of the best laboratories to study the earlier stages of the stellar and protoplanetary disc evolution. The wealth of accurate astrometric measure…