activity
20102023
most citedRuprecht 147 DANCe I. Members, empirical isochrone, luminosity and mass distributions

37 citations · 72 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023

Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS)

Roberta Paladini, Catherine Zucker, Robert Benjamin +67

A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is supported by a large representation of the community of Galactic astronomers. The combination of sensitiv…

astro-ph.SR2019★ 16 cited

IC 4665 DANCe I. Members, empirical isochrones, magnitude distributions, present-day system mass function, and spatial distribution

N. Miret-Roig, H. Bouy, J. Olivares +12

Context. The study of star formation is extremely challenging due to the lack of complete and clean samples of young, nearby clusters, and star forming regions. The recent Gaia DR2…

astro-ph.SR2019★ 37 cited

Ruprecht 147 DANCe I. Members, empirical isochrone, luminosity and mass distributions

J. Olivares, H. Bouy, L. M. Sarro +10

Context. Ruprecht 147 is the oldest (2.5 Gyr) open cluster in the solar vicinity (< 300 pc), making it an important target for stellar evolution studies and exoplanet searches. Aim…

astro-ph.SR2012★ 19 cited

IRAS 20050+2720: Anatomy of a young stellar cluster

H. M. Guenther, S. J. Wolk, B. Spitzbart +7

IRAS 20050+2720 is young star forming region at a distance of 700 pc without apparent high mass stars. We present results of our multiwavelength study of IRAS 20050+2720 which incl…

astro-ph.SR2010

IRAS 20050+2720: Anatomy of a young stellar cluster

H. M. Guenther, S. J. Wolk, R. A. Gutermuth +4

We present early results of our multiwavelength study of the star forming region IRAS 20050+2720. While we use X-rays and IR to classify young stellar objects, the optical data can…