activity
20052026
most citedThe Gould's Belt Distances Survey (GOBELINS) II. Distances and structure towards the Orion Molecular Clouds

235 citations · 2.3k across the 35 of their papers we have counts for

collaborators

37 papers

astro-ph.SR2026

A Multiband Catalog of Infrared-Excess Sources in the Vela-Carina Region: VVVX, DECaPS, and GLIMPSE

R. M. Torres, R. K. Saito, V. Fermiano +4

Multiwavelength surveys of the Galactic midplane enable the identification of infrared-excess sources, signatures of circumstellar material, though high extinction and crowding hin…

astro-ph.SR2026

Infrared-excess sources in VVV: candidate debris discs, SED characterization, and variability analysis

P. Esteves, R. K. Saito, C. Chavero +9

Debris disks around main-sequence stars provide important insights into planetary formation and evolution; however, identifying these systems in the Galactic plane, where high inte…

astro-ph.GA2026

Accurate proper motions of the protostellar system VLA1623-2417

Ricardo Hernández Garnica, Laurent Loinard, Carlos Carrasco-González +9

We present a detailed astrometric analysis of the quadruple protostellar system VLA1623-2417, deriving accurate absolute proper motions for components A, B, and W, as well as, for…

astro-ph.SR2026

Modeling the curved dust sublimation front in protoplanetary disks: a potential probe of midplane turbulence

Ezequiel Manzo-Martínez, Ramiro Franco-Hernández, Nuria Calvet +3

We present a new approach to calculate the geometry and emission of the dust inner wall in disks around T Tauri stars. This calculation follows a self-consistent approach given the…

astro-ph.EP2020★ 22 cited

An astrometric planetary companion candidate to the M9 Dwarf TVLM 513-46546

Salvador Curiel, Gisela N. Ortiz-León, Amy J. Mioduszewski +1

Astrometric observations of the M9 dwarf TVLM 51346546 taken with the VLBA reveal an astrometric signature consistent with a period of 221 5 days. The orbital fit implies…

astro-ph.SR2019★ 8 cited

Sub-stellar companions of the young weak-line TTauri Star DoAr21

Salvador Curiel, Gisela N. Ortiz-León, Amy J. Mioduszewski +1

The compact, non-thermal emission in DoAr21 has been studied with the VLBA to investigate the possibility that the residuals of the astrometry fitting are due to the reflex motion…